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		<id>https://www.frathwiki.com/index.php?title=Interlingua/Morphology&amp;diff=176056</id>
		<title>Interlingua/Morphology</title>
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		<summary type="html">&lt;p&gt;Aquatiki: Created page with &amp;quot;There is some systemic marking for parts of speech. But, for example, nouns do not have to end in any particular letter. Typically, however, adjectives end in &amp;#039;&amp;#039;-e&amp;#039;&amp;#039; or &amp;#039;&amp;#039;-a&amp;#039;&amp;#039;, adverbs end in &amp;#039;&amp;#039;-menti&amp;#039;&amp;#039; or &amp;#039;&amp;#039;-o&amp;#039;&amp;#039;, while nouns end in &amp;#039;&amp;#039;-a, -e, -o&amp;#039;&amp;#039; or a consonant. Finite verbs virtually always end in &amp;#039;&amp;#039;-a, -e,&amp;#039;&amp;#039; or &amp;#039;&amp;#039;-i&amp;#039;&amp;#039;, while infinitives add &amp;#039;&amp;#039;-r&amp;#039;&amp;#039;: &amp;#039;&amp;#039;scribe&amp;#039;&amp;#039;, &amp;#039;write&amp;#039;, &amp;#039;writes&amp;#039;; &amp;#039;&amp;#039;scriber&amp;#039;&amp;#039;, &amp;#039;to write&amp;#039;.   ==Articles== The definite articles are is &amp;#039;&amp;#039;le&amp;#039;&amp;#039; or &amp;#039;&amp;#039;la&amp;#039;&amp;#039; and...&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;There is some systemic marking for parts of speech. But, for example, nouns do not have to end in any particular letter. Typically, however, adjectives end in &#039;&#039;-e&#039;&#039; or &#039;&#039;-a&#039;&#039;, adverbs end in &#039;&#039;-menti&#039;&#039; or &#039;&#039;-o&#039;&#039;, while nouns end in &#039;&#039;-a, -e, -o&#039;&#039; or a consonant. Finite verbs virtually always end in &#039;&#039;-a, -e,&#039;&#039; or &#039;&#039;-i&#039;&#039;, while infinitives add &#039;&#039;-r&#039;&#039;: &#039;&#039;scribe&#039;&#039;, &#039;write&#039;, &#039;writes&#039;; &#039;&#039;scriber&#039;&#039;, &#039;to write&#039;.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Articles==&lt;br /&gt;
The definite articles are is &#039;&#039;le&#039;&#039; or &#039;&#039;la&#039;&#039; and indefinite articles are &#039;&#039;un&#039;&#039; or &#039;&#039;una&#039;&#039; (the same as the number &amp;quot;one&amp;quot;). They are invariable and are used roughly as in English. The prepositions &#039;&#039;a&#039;&#039; &#039;to&#039; and &#039;&#039;de&#039;&#039; &#039;of&#039; can optionally be fused with the definite articles into  &#039;&#039;del&#039;&#039; and &#039;&#039;al&#039;&#039;, the masculine and feminine respectively.&lt;br /&gt;
&lt;br /&gt;
==Nouns==&lt;br /&gt;
Nouns inflect for number. Plural nouns take &#039;&#039;-s&#039;&#039; after a vowel, &#039;&#039;-es&#039;&#039; after a consonant (but final &#039;&#039;-c&#039;&#039; changes to &#039;&#039;-ches&#039;&#039; to preserve the {{IPA|[k]}} sound of &#039;&#039;c&#039;&#039;).&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;catto&#039;&#039; &amp;amp;nbsp; &#039;cat&#039;&amp;amp;nbsp; →&amp;amp;nbsp; &#039;&#039;cattos&#039;&#039;&amp;amp;nbsp; &#039;cats&#039;&lt;br /&gt;
:&#039;&#039;can&#039;&#039;&amp;amp;nbsp; &#039;dog&#039;&amp;amp;nbsp; → &amp;amp;nbsp;&#039;&#039;canes&#039;&#039;&amp;amp;nbsp; &#039;dogs&#039;&lt;br /&gt;
:&#039;&#039;roc&#039;&#039; &amp;amp;nbsp; &#039;rook&#039; [chess] &amp;amp;nbsp; → &amp;amp;nbsp;&#039;&#039;roches&#039;&#039;&amp;amp;nbsp; &#039;rooks&#039;&lt;br /&gt;
&lt;br /&gt;
Interlingua has no grammatical gender, unlike all Romance languages. Animate nouns are sex-neutral, unless they refer specifically to a male or a female in the lexicon. Thus, &#039;&#039;jornalista&#039;&#039; &#039;journalist&#039; and &#039;&#039;scientista&#039;&#039; &#039;scientist&#039; are usable of both men and women, even though &#039;&#039;rege&#039;&#039; &#039;king&#039; and &#039;&#039;regina&#039;&#039; &#039;queen&#039; are sex-specific. Feminine forms can be created by substituting final &#039;&#039;-a&#039;&#039; for a final &#039;&#039;-o&#039;&#039; or &#039;&#039;-e&#039;&#039; or by adding the suffix &#039;&#039;-essa&#039;&#039;.  So it is that gender refers more to the form (i.e. ending) than to sex.&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;puero&#039;&#039; &amp;amp;nbsp; &#039;boy&#039; &amp;amp;nbsp; → &amp;amp;nbsp;&#039;&#039;puera&#039;&#039;&amp;amp;nbsp; &#039;girl&#039;&lt;br /&gt;
:&#039;&#039;tigre&#039;&#039; &amp;amp;nbsp; &#039;tiger&#039; &amp;amp;nbsp; → &amp;amp;nbsp;&#039;&#039;tigressa&#039;&#039;&amp;amp;nbsp; &#039;female tiger&#039;&lt;br /&gt;
&lt;br /&gt;
These color the regular forms as masculine when they appear in the same context.&lt;br /&gt;
&lt;br /&gt;
==Adjectives==&lt;br /&gt;
Adjectives may precede or follow the noun they modify. As a matter of style, short adjectives tend to precede, long adjectives tend to follow. Numerals always precede the noun.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;belles oculos&#039;&#039; or &#039;&#039;oculos belles&#039;&#039; &amp;amp;nbsp; &#039;beautiful eyes&#039;&lt;br /&gt;
: &#039;&#039;una bona idea, una idea ingeniosa&#039;&#039; &amp;amp;nbsp; &#039;a good idea, an ingenious idea&#039;&lt;br /&gt;
&lt;br /&gt;
Comparative degree is expressed by &#039;&#039;plus&#039;&#039; or &#039;&#039;minus&#039;&#039; preceding the adjective and superlative degree by &#039;&#039;le plus&#039;&#039; or &#039;&#039;la minus&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;un plus feroce leon&#039;&#039; &amp;amp;nbsp; &#039;a fiercer lion&#039;&lt;br /&gt;
:&#039;&#039;un traino minus rapide&#039;&#039; &amp;amp;nbsp; &#039;a less speedy train&#039;&lt;br /&gt;
:&#039;&#039;le plus alte arbore&#039;&#039; &amp;amp;nbsp; &#039;the tallest tree&#039;&lt;br /&gt;
:&#039;&#039;le solution le minus costose&#039;&#039; &amp;amp;nbsp; &#039;the least costly solution&#039;.&lt;br /&gt;
&lt;br /&gt;
The suffix &#039;&#039;-issime&#039;&#039; may be used to express the absolute superlative degree.&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;una aventura excellentissima&#039;&#039; &amp;amp;nbsp; &#039;a most excellent adventure&#039;&lt;br /&gt;
&lt;br /&gt;
The adjectives &#039;&#039;bon&#039;&#039; &#039;good&#039;, &#039;&#039;mal&#039;&#039; &#039;bad&#039;, &#039;&#039;magne&#039;&#039; &#039;great&#039;, and &#039;&#039;parve&#039;&#039; &#039;small&#039; have optional irregular forms for the comparative and superlative.&lt;br /&gt;
&lt;br /&gt;
:{|&lt;br /&gt;
|-&lt;br /&gt;
|&#039;&#039;bon → plus bon → le plus bon&#039;&#039; || &amp;amp;nbsp; || or || &amp;amp;nbsp; || &#039;&#039;bon → melior → optime&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|&#039;&#039;mal → plus mal → le plus mal&#039;&#039; || &amp;amp;nbsp; || or || &amp;amp;nbsp; || &#039;&#039;mal → pejor → pessime&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|&#039;&#039;magne → plus magne → le plus magne&#039;&#039; || &amp;amp;nbsp; || or || &amp;amp;nbsp; || &#039;&#039;magne → major → maxime&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|&#039;&#039;parve → plus parve → le plus parve&#039;&#039; || &amp;amp;nbsp; || or || &amp;amp;nbsp; || &#039;&#039;parve → minor → minime&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==Adverbs==&lt;br /&gt;
There are two types of adverbs, primary and secondary. Primary adverbs are a closed class of grammatical operators, such as &#039;&#039;quasi,&#039;&#039; &#039;almost&#039;; &#039;&#039;jam&#039;&#039;, &#039;already&#039;; and &#039;&#039;totevi,&#039;&#039; &#039;anyway&#039;. Secondary adverbs are an open class derived from corresponding adjectives by adding the suffix &#039;&#039;-menti&#039;&#039; (&#039;&#039;-amenti&#039;&#039; after final &#039;&#039;-c&#039;&#039;).&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;felice&#039;&#039; &amp;amp;nbsp; &#039;happy&#039; &amp;amp;nbsp; → &amp;amp;nbsp; &#039;&#039;felicementi&#039;&#039; &amp;amp;nbsp; &#039;happily&#039;&lt;br /&gt;
:&#039;&#039;magic&#039;&#039; &amp;amp;nbsp; &#039;magical&#039; &amp;amp;nbsp; → &amp;amp;nbsp; &#039;&#039;magicamenti&#039;&#039; &amp;amp;nbsp; &#039;magically&#039;&lt;br /&gt;
&lt;br /&gt;
A few common adverbs have optional short forms in &#039;&#039;-o&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;sol&#039;&#039; &amp;amp;nbsp; &#039;alone&#039; &amp;amp;nbsp; → &amp;amp;nbsp; &#039;&#039;solo&#039;&#039; or &#039;&#039;solmente&#039;&#039; &amp;amp;nbsp; &#039;only&#039;&lt;br /&gt;
&lt;br /&gt;
Like adjectives, adverbs use &#039;&#039;plus&#039;&#039; and &#039;&#039;minus&#039;&#039; to express the comparative and &#039;&#039;le plus&#039;&#039; and &#039;&#039;la minus&#039;&#039; to express the superlative.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Illa canta plus bellementi que illa parla.&#039;&#039; &amp;amp;nbsp; &#039;She sings more beautifully than she speaks.&#039;&lt;br /&gt;
: &#039;&#039;Le gepardo curre le plus rapide de omne animales.&#039;&#039; &amp;amp;nbsp; &#039;The cheetah runs the fastest of all animals.&#039;&lt;br /&gt;
&lt;br /&gt;
The adverbs equivalent to &#039;&#039;bon,&#039;&#039; &#039;good&#039; and &#039;&#039;mal,&#039;&#039; &#039;bad&#039; have optional irregular forms.&lt;br /&gt;
&lt;br /&gt;
:{|&lt;br /&gt;
|-&lt;br /&gt;
|&#039;&#039;bonmenti → plus bonmenti → le plus bonmenti&#039;&#039; || &amp;amp;nbsp; || or || &amp;amp;nbsp; || &#039;&#039;ben → plus ben → le plus ben&#039;&#039; || &amp;amp;nbsp; || or || &amp;amp;nbsp; || &#039;&#039;ben → melio → optimo&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|&#039;&#039;malmenti → plus malmenti→ le plus malmenti&#039;&#039; || &amp;amp;nbsp; || or || &amp;amp;nbsp; || &#039;&#039;mal → plus mal → le plus mal&#039;&#039; || &amp;amp;nbsp; || or || &amp;amp;nbsp; || &#039;&#039;mal → pejo → pessimo&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==Pronouns ==&lt;br /&gt;
&lt;br /&gt;
===Personal pronouns===&lt;br /&gt;
{{ia-pronoun}}&lt;br /&gt;
&lt;br /&gt;
Personal pronouns inflect for number, case, and (in the third person) gender.&lt;br /&gt;
&lt;br /&gt;
* The &#039;&#039;&#039;nominative case&#039;&#039;&#039; is the default form and typically serves as the subject of a verb.&lt;br /&gt;
&lt;br /&gt;
::&#039;&#039;&amp;quot;Qui es ibi?&amp;quot; &amp;quot;Io.&amp;quot;&#039;&#039; &amp;amp;nbsp; &amp;quot;Who&#039;s there?&amp;quot; &amp;quot;Me.&amp;quot;&lt;br /&gt;
::&#039;&#039;Tu arrestava le chef de policia.&#039;&#039; &amp;amp;nbsp; &#039;You have arrested the chief of police.&#039;&lt;br /&gt;
&lt;br /&gt;
* The &#039;&#039;&#039;oblique case&#039;&#039;&#039; is used for direct objects, and may also be used for indirect objects. (Alternatively, indirect objects are expressed through &#039;&#039;a,&#039;&#039; &#039;to&#039; plus a pronoun.)&lt;br /&gt;
&lt;br /&gt;
:: &#039;&#039;Le caffe es excellente: proba lo!&#039;&#039; &amp;amp;nbsp; &#039;The coffee is excellent: try it!&#039;&lt;br /&gt;
:: &#039;&#039;Dice me le conto; dice me lo&#039;&#039; (or &#039;&#039;Dice le conto a me...&#039;&#039;)  &amp;amp;nbsp; &#039;Tell me the story; tell it to me.&#039;&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;Reflexive pronouns&#039;&#039;&#039; are used when the subject of a verb is identical with the direct or indirect object. As in the Romance languages, reflexive constructions are often used where English would employ an intransitive verb or the passive voice.&lt;br /&gt;
&lt;br /&gt;
:: &#039;&#039;Deo adjuta les, qui se adjuta.&#039;&#039; &amp;amp;nbsp; &#039;God helps those who help themselves&#039;.&lt;br /&gt;
:: &#039;&#039;Io me sibila una melodia.&#039;&#039; &amp;amp;nbsp; &#039;I whistle a tune to myself.&#039;&lt;br /&gt;
:: &#039;&#039;Tu te rasava?&#039;&#039; &amp;amp;nbsp; &#039;Have you shaved?&#039;&lt;br /&gt;
:: &#039;&#039;Francese se parla in Francia.&#039;&#039; &amp;amp;nbsp; &#039;French is spoken in France.&#039;&lt;br /&gt;
&lt;br /&gt;
* The &#039;&#039;&#039;genitive case&#039;&#039;&#039; indicates possession (&#039;&#039;mi auto,&#039;&#039; &#039;my car&#039;). The longer forms &#039;&#039;mie, tue&#039;&#039; etc. are adjectives, used in constructions like &#039;&#039;le auto es le mie,&#039;&#039; &#039;the car is mine&#039;. They can also directly modify a noun.&lt;br /&gt;
&lt;br /&gt;
:: &#039;&#039;alicun amicos mie&#039;&#039; &amp;amp;nbsp; &#039;some friends of mine&#039;&lt;br /&gt;
:: &#039;&#039;Matre mia! Es una picanta bolla de carne!&#039;&#039; &amp;amp;nbsp; &#039;Mamma mia, that&#039;s a spicy meatball!&#039;&lt;br /&gt;
&lt;br /&gt;
One could also assert the existence of a separate prepositional case, since third-person pronouns use the longer forms &#039;&#039;ille, illes&#039;&#039; etc. after a preposition in place of the expected &#039;&#039;le, les&#039;&#039; etc.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Da le can a illes.&#039;&#039; &amp;amp;nbsp; &#039;Give them the dog.&#039;&lt;br /&gt;
&lt;br /&gt;
Interlingua follows the European custom of using the plural forms &#039;&#039;vos&#039;&#039; etc. rather than &#039;&#039;tu&#039;&#039; etc. in formal situations.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Esque vos passava un viage placente, Seniora Chan?&#039;&#039; &amp;amp;nbsp; &#039;Did you have a pleasant trip, Mrs. Chan?&#039;&lt;br /&gt;
: &#039;&#039;Aperi vostre valise, Senior.&#039;&#039; &amp;amp;nbsp; &#039;Open your suitcase, Sir.&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Illes&#039;&#039; can be used as a sex-neutral pronoun, like English &#039;they&#039;. &#039;&#039;Illas&#039;&#039; may be used for entirely female groups.&lt;br /&gt;
&lt;br /&gt;
===Impersonal pronouns===&lt;br /&gt;
&#039;&#039;Il&#039;&#039; is an impersonal nominative pronoun used in constructions like &#039;&#039;il pluve,&#039;&#039; &#039;it&#039;s raining&#039;. It can also serve as a placeholder when the true subject is a clause occurring later in the sentence. It may be omitted where the sense is clear.&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;Il deveni tarde.&#039;&#039; &amp;amp;nbsp; &#039;It&#039;s getting late.&#039;&lt;br /&gt;
:&#039;&#039;Il es ver que nos expende multa moneta.&#039;&#039; &amp;amp;nbsp; &#039;It&#039;s true that we&#039;re spending a lot of money.&#039;&lt;br /&gt;
:&#039;&#039;Es bon que vos veni ora.&#039;&#039; &amp;amp;nbsp; &#039;It&#039;s good that you come now.&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;On&#039;&#039; is a nominative pronoun used when the identity of the subject is vague. The English translation is often &#039;one&#039;, &#039;you&#039;, or &#039;they&#039;. It is sometimes equivalent to an English passive voice construction. The oblique form is &#039;&#039;uno&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;On non vide tal cosas actualmenti.&#039;&#039; &amp;amp;nbsp; &#039;One doesn&#039;t see such things these days.&#039;&lt;br /&gt;
:&#039;&#039;On sape nunquam lo que evenira.&#039;&#039; &amp;amp;nbsp; &#039;You never know what will happen.&#039;&lt;br /&gt;
:&#039;&#039;On construe una nova linea de metro al centro urban.&#039;&#039; &amp;amp;nbsp; &#039;They&#039;re building a new subway line to downtown.&#039;&lt;br /&gt;
:&#039;&#039;On collige le recyclabiles omne venerdi.&#039;&#039; &amp;amp;nbsp; &#039;Recyclables are picked up every Friday.&#039;&lt;br /&gt;
:&#039;&#039;Tal pensatas afflige uno in le profundo del depression.&#039;&#039; &amp;amp;nbsp; &#039;Such thoughts afflict one in the depths of depression.&#039;&lt;br /&gt;
&lt;br /&gt;
===Demonstratives===&lt;br /&gt;
{|border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;5&amp;quot; cellspacing=&amp;quot;0&amp;quot; align=&amp;quot;right&amp;quot; style=&amp;quot;border-collapse:collapse&amp;quot;&lt;br /&gt;
|- align=&amp;quot;center&amp;quot;&lt;br /&gt;
| colspan=5 style=&amp;quot;background: navy; color: white&amp;quot; | &#039;&#039;&#039;Demonstratives&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
| Role || Number || Gender || Proximate || Remote&lt;br /&gt;
|- align=&amp;quot;center&amp;quot;&lt;br /&gt;
|  align=&amp;quot;left&amp;quot; | Adjective || – || – || &#039;&#039;&#039;iste&#039;&#039;&#039; || &#039;&#039;&#039;ille&#039;&#039;&#039;&lt;br /&gt;
|- align=&amp;quot;center&amp;quot;&lt;br /&gt;
|  align=&amp;quot;left&amp;quot; rowspan=&amp;quot;6&amp;quot; | Pronoun ||  align=&amp;quot;left&amp;quot; rowspan=&amp;quot;3&amp;quot; | Sing. ||  align=&amp;quot;left&amp;quot; | masc. || &#039;&#039;&#039;iste&#039;&#039;&#039; || &#039;&#039;&#039;(ille)&#039;&#039;&#039;&lt;br /&gt;
|- align=&amp;quot;center&amp;quot;&lt;br /&gt;
|  align=&amp;quot;left&amp;quot; | fem. || &#039;&#039;&#039;ista&#039;&#039;&#039; || &#039;&#039;&#039;(illa)&#039;&#039;&#039;&lt;br /&gt;
|- align=&amp;quot;center&amp;quot;&lt;br /&gt;
|  align=&amp;quot;left&amp;quot; | neut. || &#039;&#039;&#039;isto&#039;&#039;&#039; || &#039;&#039;&#039;(illo)&#039;&#039;&#039;&lt;br /&gt;
|- align=&amp;quot;center&amp;quot;&lt;br /&gt;
|  align=&amp;quot;left&amp;quot; rowspan=&amp;quot;3&amp;quot; | Plur. ||  align=&amp;quot;left&amp;quot; | masc. || &#039;&#039;&#039;istes&#039;&#039;&#039; || &#039;&#039;&#039;(illes)&#039;&#039;&#039;&lt;br /&gt;
|- align=&amp;quot;center&amp;quot;&lt;br /&gt;
|  align=&amp;quot;left&amp;quot; | fem. || &#039;&#039;&#039;istas&#039;&#039;&#039; || &#039;&#039;&#039;(illas)&#039;&#039;&#039;&lt;br /&gt;
|- align=&amp;quot;center&amp;quot;&lt;br /&gt;
|  align=&amp;quot;left&amp;quot; | neut. || &#039;&#039;&#039;istos&#039;&#039;&#039; || &#039;&#039;&#039;(illos)&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The main demonstratives are the adjective &#039;&#039;iste,&#039;&#039; &#039;this&#039; and the corresponding pronouns &#039;&#039;iste&#039;&#039; (masculine), &#039;&#039;ista&#039;&#039; (feminine), and &#039;&#039;isto&#039;&#039; (neuter), which may be pluralized. They are used more widely than English &#039;this/these&#039;, often encroaching on the territory of English &#039;that/those&#039;. Where the subject of a sentence has two plausible antecedents, &#039;&#039;iste&#039;&#039; (or one of its derivatives) refers to the second one.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Iste vino es pessime.&#039;&#039; &amp;amp;nbsp; &#039;This wine is terrible.&#039;&lt;br /&gt;
: &#039;&#039;Isto es una bona idea.&#039;&#039; &amp;amp;nbsp; &#039;That&#039;s a good idea.&#039;&lt;br /&gt;
: &#039;&#039;Janet accompaniava su soror al galleria...&#039;&#039; &amp;amp;nbsp; &#039;Janet accompanied her sister to the gallery...&#039;&lt;br /&gt;
:: (a) &#039;&#039;Illa es una artista notabila.&#039;&#039;  &amp;amp;nbsp; &#039;She [Janet] is a well-known artist.&#039;&lt;br /&gt;
:: (b) &#039;&#039;Ista es una artista notabila.&#039;&#039;  &amp;amp;nbsp; &#039;She [Janet&#039;s sister] is a well-known artist.&#039;&lt;br /&gt;
&lt;br /&gt;
The demonstrative of remoteness is &#039;&#039;ille&#039;&#039; &#039;that&#039;.  The corresponding pronouns &#039;&#039;ille, illa, illo&#039;&#039; and their plurals are identical with the third-person personal pronouns, though they are normally accentuated in speech.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Io cognosce ille viro; ille se appella Smith.&#039;&#039; &amp;amp;nbsp; &#039;I know that man; his name is Smith.&#039;&lt;br /&gt;
: Illo &#039;&#039;es una obra magnifica.&#039;&#039; &amp;amp;nbsp; &amp;lt;nowiki&amp;gt;&#039;&amp;lt;/nowiki&amp;gt;&#039;&#039;That&#039;&#039; is a magnificent work.&#039;&lt;br /&gt;
&lt;br /&gt;
===Relative and interrogative pronouns===&lt;br /&gt;
The relative pronouns for animates are &#039;&#039;qui&#039;&#039; (nominative case and after prepositions) and &#039;&#039;que&#039;&#039; (oblique case).&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Nos vole un contabile qui sape contar.&#039;&#039; &amp;amp;nbsp; &#039;We want an accountant who knows how to count.&#039;&lt;br /&gt;
: &#039;&#039;Nos vole un contabile super qui nos pote contar.&#039;&#039;  &amp;amp;nbsp; We want an accountant who we can count on.&#039; (an accountant on whom we can count)&lt;br /&gt;
: &#039;&#039;Nos vole un contabile que la policia non perseque.&#039;&#039; &amp;amp;nbsp; &#039;We want an accountant whom the police are not pursuing.&#039;&lt;br /&gt;
&lt;br /&gt;
For inanimates, &#039;&#039;que&#039;&#039; covers both the nominative and oblique cases.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Il ha duo sortas de inventiones: illos que on discoperi e illos que discoperi uno.&#039;&#039; &amp;amp;nbsp; &#039;There are two types of inventions: those that you discover and those that discover you.&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Cuje&#039;&#039; &#039;whose&#039; is the genitive case for both animates and inanimates.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;un autor cuje libros se vende in milliones&#039;&#039; &amp;amp;nbsp; &#039;an author whose books sell in the millions&#039;&lt;br /&gt;
: &#039;&#039;una insula cuje mysterios resta irresolvite&#039;&#039; &amp;amp;nbsp; &#039;an island whose mysteries remain unsolved&#039;&lt;br /&gt;
&lt;br /&gt;
All the above may be replaced by the relative adjective forms &#039;&#039;le qual&#039;&#039; (singular) and &#039;&#039;le quales&#039;&#039; (plural).&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Mi scriptorio esseva in disordine – le qual, nota ben, es su stato normal.&#039;&#039;  &amp;amp;nbsp; &#039;My desk was in a mess – which, mind you, is its usual state.&#039;&lt;br /&gt;
: &#039;&#039;Duo cosinos remote, del quales io sape nihil, veni visitar.&#039;&#039;  &amp;amp;nbsp; &#039;Two distant cousins, of whom I know nothing, are coming to visit.&#039;&lt;br /&gt;
&lt;br /&gt;
The relative pronouns also serve as interrogative pronouns.&lt;br /&gt;
&lt;br /&gt;
==Verbs==&lt;br /&gt;
{|border=&amp;quot;1&amp;quot; cellpadding=&amp;quot;5&amp;quot; cellspacing=&amp;quot;0&amp;quot; align=&amp;quot;right&amp;quot; style=&amp;quot;border-collapse:collapse&amp;quot;&lt;br /&gt;
|- align=&amp;quot;center&amp;quot;&lt;br /&gt;
| colspan=6 style=&amp;quot;background: navy; color: white&amp;quot; | &#039;&#039;&#039;Main verb forms&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
| Tense || Ending || &#039;&#039;-ar&#039;&#039; verbs || &#039;&#039;-er&#039;&#039; verbs || &#039;&#039;-ir&#039;&#039; verbs&lt;br /&gt;
|-&lt;br /&gt;
| Infinitive || &#039;&#039;&#039;-r&#039;&#039;&#039; || &#039;&#039;parla&#039;&#039;&#039;&#039;&#039;r&#039;&#039;&#039; || &#039;&#039;vide&#039;&#039;&#039;&#039;&#039;r&#039;&#039;&#039; || &#039;&#039;audi&#039;&#039;&#039;&#039;&#039;r&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
| Present || &#039;&#039;&#039;–&#039;&#039;&#039; || &#039;&#039;parla&#039;&#039; || &#039;&#039;vide&#039;&#039; || &#039;&#039;audi&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
| Past* || &#039;&#039;&#039;-va&#039;&#039;&#039; || &#039;&#039;parla&#039;&#039;&#039;&#039;&#039;va&#039;&#039;&#039; || &#039;&#039;vide&#039;&#039;&#039;&#039;&#039;va&#039;&#039;&#039; || &#039;&#039;audi&#039;&#039;&#039;&#039;&#039;va&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
| Future* || &#039;&#039;&#039;-ra&#039;&#039;&#039; || &#039;&#039;parla&#039;&#039;&#039;&#039;&#039;ra&#039;&#039;&#039; || &#039;&#039;vide&#039;&#039;&#039;&#039;&#039;ra&#039;&#039;&#039;  || &#039;&#039;audi&#039;&#039;&#039;&#039;&#039;ra&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
| Conditional* || &#039;&#039;&#039;-rea&#039;&#039;&#039; || &#039;&#039;parla&#039;&#039;&#039;&#039;&#039;rea&#039;&#039;&#039; || &#039;&#039;vide&#039;&#039;&#039;&#039;&#039;rea&#039;&#039;&#039; || &#039;&#039;audi&#039;&#039;&#039;&#039;&#039;rea&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
| Present participle || &#039;&#039;&#039;-(e)nte&#039;&#039;&#039; || &#039;&#039;parla&#039;&#039;&#039;&#039;&#039;nte&#039;&#039;&#039; || &#039;&#039;vide&#039;&#039;&#039;&#039;&#039;nte&#039;&#039;&#039; || &#039;&#039;audi&#039;&#039;&#039;&#039;&#039;&amp;lt;u&amp;gt;e&amp;lt;/u&amp;gt;nte&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
| Past participle || &#039;&#039;&#039;-te&#039;&#039;&#039; || &#039;&#039;parla&#039;&#039;&#039;&#039;&#039;te&#039;&#039;&#039; || &#039;&#039;vid&amp;lt;u&amp;gt;i&amp;lt;/u&amp;gt;&#039;&#039;&#039;&#039;&#039;te&#039;&#039;&#039; || &#039;&#039;audi&#039;&#039;&#039;&#039;&#039;te&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
| colspan=6 | &amp;lt;small&amp;gt;*For alternative, compound forms, see Compound tenses.&amp;lt;/small&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The verb system is a simplified version of the systems found in the Romance languages. There is an imperfective aspect, as in Romance, no perfect as in English, and no continuous aspect, as in English and some Romance languages. Except for &#039;&#039;esser&#039;&#039; &#039;to be&#039;, there are no personal inflections, and the indicative also covers the subjunctive and imperative moods. Three common verbs (&#039;&#039;esse&#039;&#039;, &#039;&#039;habe&#039;&#039; and &#039;&#039;vade&#039;&#039;) usually take short forms in the present tense (&#039;&#039;es&#039;&#039;, &#039;&#039;ha&#039;&#039; and &#039;&#039;va&#039;&#039; respectively), and a few irregular verbs are available.&lt;br /&gt;
&lt;br /&gt;
For convenience&#039; sake, this section often uses the term tense to also cover mood and aspect, though this is not strict grammatical terminology.&lt;br /&gt;
&lt;br /&gt;
The table at the right shows the main verb forms, with examples for &#039;&#039;-ar, -er&#039;&#039; and &#039;&#039;-ir&#039;&#039; verbs (based on &#039;&#039;parlar&#039;&#039; &#039;to speak&#039;, &#039;&#039;vider&#039;&#039; &#039;to see&#039;, and &#039;&#039;audir&#039;&#039; &#039;to hear&#039;).&lt;br /&gt;
&lt;br /&gt;
The simple past, future, and conditional tenses correspond to semantically identical compound tenses (composed of auxiliary verbs plus infinitives or past participles). These in turn furnish patterns for building more-complex tenses such as the future perfect.&lt;br /&gt;
&lt;br /&gt;
===Infinitives===&lt;br /&gt;
Infinitive verbs always end in &#039;&#039;-ar, -er,&#039;&#039; or &#039;&#039;-ir&#039;&#039;. They cover the functions of both the infinitive and the gerund in English and can be pluralized where it makes sense.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Cognoscer nos es amar nos.&#039;&#039; &amp;amp;nbsp; &#039;To know us is to love us.&#039;&lt;br /&gt;
: &#039;&#039;Il es difficile determinar su strategia.&#039;&#039; &amp;amp;nbsp; &#039;It&#039;s hard to figure out his strategy.&#039;&lt;br /&gt;
: &#039;&#039;Illes time le venir del locustas.&#039;&#039; &amp;amp;nbsp; &#039;They fear the coming of the locusts.&#039;&lt;br /&gt;
: &#039;&#039;Le faceres de illa evocava un admiration general.&#039;&#039; &amp;amp;nbsp; &#039;Her doings evoked a widespread admiration.&#039;&lt;br /&gt;
&lt;br /&gt;
Infinitives are also used in some compound tenses (see below).&lt;br /&gt;
&lt;br /&gt;
===Simple tenses===&lt;br /&gt;
There are four simple tenses: the present, past, future, and conditional.&lt;br /&gt;
&lt;br /&gt;
* The present tense can be formed from the infinitive by removing the final &#039;&#039;-r&#039;&#039;. It covers the simple and continuous present tenses in English. The verbs &#039;&#039;esser&#039;&#039; &#039;to be&#039;, &#039;&#039;haber&#039;&#039; &#039;to have&#039;, and &#039;&#039;{{C|vader}}&#039;&#039; &#039;to go&#039; normally take the short forms &#039;&#039;es, ha,&#039;&#039; and &#039;&#039;va&#039;&#039; rather than &#039;&#039;esse, habe,&#039;&#039; and &#039;&#039;vade&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
:: &#039;&#039;Io ama mangos; io mangia un justo ora.&#039;&#039; &amp;amp;nbsp; &#039;I love mangoes; I&#039;m eating one right now.&#039;&lt;br /&gt;
:: &#039;&#039;Mi auto es vetere e ha multe defectos: naturalmenti illo va mal!&#039;&#039;  &amp;amp;nbsp; &#039;My car is old and has lots of things wrong with it: of course it runs poorly!&#039;&lt;br /&gt;
&lt;br /&gt;
* The simple past tense can be formed by adding &#039;&#039;-va&#039;&#039; to the present tense form. It covers the English simple past and past perfect, along with their continuous equivalents.&lt;br /&gt;
&lt;br /&gt;
:: &#039;&#039;Io vos diceva repetitemente: le hospites jam comenciava partir quando la casa se incendiava.&#039;&#039;   &amp;amp;nbsp; &#039;I&#039;ve told you again and again: the guests were already starting to leave when the house burst into flames.&#039;&lt;br /&gt;
&lt;br /&gt;
* The simple future can be formed by adding &#039;&#039;-ra&#039;&#039; to the present tense form. Future tense forms are stressed on the suffix (&#039;&#039;retorna&#039;&#039;&#039;ra&#039;&#039;&#039;&#039;&#039; &#039;will return&#039;). It covers the English simple and continuous future tenses.&lt;br /&gt;
&lt;br /&gt;
:: &#039;&#039;Nos volara de hic venerdi vespere, e sabbato postmeridie nos prendera le sol al plagia in Santorini.&#039;&#039;  &amp;amp;nbsp; &#039;We&#039;ll fly out Friday evening, and by Saturday afternoon we&#039;ll be sunbathing on the beach in Santorini.&#039;&lt;br /&gt;
&lt;br /&gt;
* The simple conditional consists of the present tense form plus &#039;&#039;-rea&#039;&#039;. Like the future tense, it is stressed on the suffix (&#039;&#039;prefe&#039;&#039;&#039;re&#039;&#039;&#039;a&#039;&#039; &#039;would prefer). In function it resembles the English conditional.&lt;br /&gt;
&lt;br /&gt;
:: &#039;&#039;Si ille faceva un melior reclamo, ille venderea le duple.&#039;&#039; &amp;amp;nbsp; &#039;If he did better advertising, he would sell twice as much.&#039;&lt;br /&gt;
&lt;br /&gt;
===Participles===&lt;br /&gt;
The present participle is effectively the present tense form plus &#039;&#039;-nte&#039;&#039;. Verbs in &#039;&#039;-ir&#039;&#039; take &#039;&#039;-iente&#039;&#039; rather than *&#039;&#039;-inte&#039;&#039; (&#039;&#039;nutrir&#039;&#039; &#039;to feed&#039; → &#039;&#039;nutriente&#039;&#039; &#039;feeding&#039;). It functions as an adjective or as the verb in a participial phrase.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;un corvo parlante&#039;&#039; &amp;amp;nbsp; &#039;a talking crow&#039;&lt;br /&gt;
: &#039;&#039;Approximante le station, io sentiva un apprehension terribile.&#039;&#039; &amp;amp;nbsp; &#039;Approaching the station, I felt a sense of dread.&#039;&lt;br /&gt;
&lt;br /&gt;
The past participle can be constructed by adding &#039;&#039;-te&#039;&#039; to the present tense form, except that &#039;&#039;-er&#039;&#039; verbs go to &#039;&#039;-ite&#039;&#039; rather than *&#039;&#039;-ete&#039;&#039; (&#039;&#039;eder&#039;&#039; &#039;to edit&#039;  → &#039;&#039;edite&#039;&#039; &#039;edited&#039;). It is used as an adjective and to form various compound tenses.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;un conto ben contate&#039;&#039; &amp;amp;nbsp; &#039;a well told story&#039;&lt;br /&gt;
&lt;br /&gt;
===Compound tenses===&lt;br /&gt;
Three compound tenses – the compound past, future, and conditional – are semantically identical with the corresponding simple tenses.&lt;br /&gt;
&lt;br /&gt;
* The compound past tense consists of &#039;&#039;ha&#039;&#039; (the present tense of &#039;&#039;haber&#039;&#039; &#039;to have&#039;) plus the past participle.&lt;br /&gt;
&lt;br /&gt;
:: &#039;&#039;Le imperio ha cadite.&#039;&#039; &amp;amp;nbsp; = &amp;amp;nbsp; &#039;&#039;Le imperio cadeva.&#039;&#039; &amp;amp;nbsp; &#039;The empire fell.&#039;&lt;br /&gt;
&lt;br /&gt;
* The compound future tense is constructed from &#039;&#039;va&#039;&#039; (the present tense of &#039;&#039;vader&#039;&#039; &#039;to go&#039;) plus the infinitive.&lt;br /&gt;
&lt;br /&gt;
:: &#039;&#039;Io va retornar.&#039;&#039; &amp;amp;nbsp; = &amp;amp;nbsp; &#039;&#039;Io retornara.&#039;&#039; &amp;amp;nbsp; &#039;I shall return.&#039;&lt;br /&gt;
&lt;br /&gt;
* The rarely used compound conditional tense uses the auxiliary &#039;&#039;velle&#039;&#039; plus the infinitive.&lt;br /&gt;
&lt;br /&gt;
:: &#039;&#039;Io velle preferer facer lo sol.&#039;&#039; &amp;amp;nbsp; = &amp;amp;nbsp; &#039;&#039;Io prefererea facer lo sol.&#039;&#039;  &amp;amp;nbsp; &#039;I&#039;d prefer to do it alone.&#039;&lt;br /&gt;
&lt;br /&gt;
The fourth basic compound tense is the passive, formed from &#039;&#039;es&#039;&#039; (the  present tense of &#039;&#039;esser&#039;&#039; &#039;to be&#039;) plus the past participle.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Iste salsicias es fabricate per experte salsicieros.&#039;&#039; &amp;amp;nbsp; &#039;These sausages are made by expert sausage-makers.&#039;&lt;br /&gt;
&lt;br /&gt;
A wide variety of complex tenses can be created following the above patterns, by replacing &#039;&#039;ha, va,&#039;&#039; and &#039;&#039;es&#039;&#039; with other forms of &#039;&#039;haber, vader,&#039;&#039; and &#039;&#039;esser&#039;&#039;. Examples:&lt;br /&gt;
&lt;br /&gt;
* The future perfect, using &#039;&#039;habera&#039;&#039; &#039;will have&#039; plus the past participle&lt;br /&gt;
&lt;br /&gt;
:: &#039;&#039;Ante Natal, tu habera finite tu cursos.&#039;&#039; &amp;amp;nbsp; &#039;By Christmas you will have finished your courses.&#039;&lt;br /&gt;
&lt;br /&gt;
* The past imperfect, using &#039;&#039;vadeva&#039;&#039; &#039;were going&#039; plus the infinitive&lt;br /&gt;
&lt;br /&gt;
:: &#039;&#039;Plus tarde illa vadeva scriber un romance premiate.&#039;&#039;  &amp;amp;nbsp; &#039;Later she would write a prize-winning novel.&#039;&lt;br /&gt;
&lt;br /&gt;
* The passive-voice past perfect, using &#039;&#039;habeva essite&#039;&#039; &#039;had been&#039; plus the past participle&lt;br /&gt;
&lt;br /&gt;
:: &#039;&#039;Nostre planeta habeva essite surveliate durante multe annos.&#039;&#039;  &amp;amp;nbsp; &#039;Our planet had been watched for many years.&#039;&lt;br /&gt;
&lt;br /&gt;
===Other tenses===&lt;br /&gt;
There are no distinct forms for the imperative and subjunctive moods, except in the case of &#039;&#039;esser&#039;&#039; &#039;to be&#039;. Present-tense forms normally serve both functions. For clarity&#039;s sake, a nominative pronoun may be added after the verb.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Face lo ora!&#039;&#039;  &amp;amp;nbsp; &#039;Do it now!&#039;&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Le imperatrice desira que ille attende su mandato.&#039;&#039;  &amp;amp;nbsp; &#039;The empress desires that he await her command.&#039;&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Va tu retro al campo; resta vos alteros hic.&#039;&#039;  &amp;amp;nbsp; &#039;You, go back to the camp; you others, stay here.&#039;&lt;br /&gt;
&lt;br /&gt;
The infinitive can serve as another, stylistically more impersonal, imperative form.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Cliccar hic.&#039;&#039;  &amp;amp;nbsp; &#039;Click here.&#039;&lt;br /&gt;
&lt;br /&gt;
A less urgent version of imperative, the cohortative, employs a present-tense verb within a &amp;quot;that&amp;quot; (&amp;quot;&#039;&#039;que&#039;&#039;&amp;quot;) clause and may be used with the first and third person as well as the second. The alternative &#039;&#039;vamos&#039;&#039; &#039;let&#039;s&#039; (or &#039;let&#039;s go&#039;) is available for the second-person plural.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Que tu va via!&#039;&#039; &amp;amp;nbsp; &#039;I wish you&#039;d go away!&#039;&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Que illes mangia le brioche.&#039;&#039;  &amp;amp;nbsp; &#039;Let them eat cake.&#039;&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Que nos resta hic ancora un die.&#039;&#039; &amp;amp;nbsp; or &amp;amp;nbsp; &#039;&#039;Vamos restar hic ancora un die.&#039;&#039;  &amp;amp;nbsp; &#039;Let&#039;s stay here one more day.&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Sia&#039;&#039; is the imperative and subjunctive form of &#039;&#039;esser&#039;&#039; &#039;to be&#039;. The regular form &#039;&#039;esse&#039;&#039; may also be used.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Sia caute!&#039;&#039;  &amp;amp;nbsp; &#039;Be careful!&#039;&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Sia ille vive o sia ille morte...&#039;&#039; &amp;amp;nbsp; &#039;Be he alive or be he dead...&#039;&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Que lor vita insimul sia felice!&#039;&#039;  &amp;amp;nbsp; &#039;May their life together be happy!&#039;&lt;br /&gt;
&lt;br /&gt;
===Irregular verbs===&lt;br /&gt;
The only irregular verb forms employed by most users are &#039;&#039;es, ha,&#039;&#039; and &#039;&#039;va&#039;&#039; – the shortened present-tense forms of &#039;&#039;esser&#039;&#039; &#039;to be&#039;, &#039;&#039;haber&#039;&#039; &#039;to have&#039; and &#039;&#039;vader&#039;&#039; &#039;to go&#039; – plus &#039;&#039;sia&#039;&#039;, the imperative/subjunctive of &#039;&#039;esser&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
There are certain collateral forms of &#039;&#039;esser&#039;&#039; &#039;to be&#039;: &#039;&#039;son&#039;&#039; (present plural), &#039;&#039;era&#039;&#039; (past), &#039;&#039;sera&#039;&#039; (future), and &#039;&#039;serea&#039;&#039; (conditional), instead of &#039;&#039;es,&#039;&#039; &#039;&#039;esseva,&#039;&#039; &#039;&#039;essera,&#039;&#039; and &#039;&#039;esserea&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;Nos vancouveritas son un banda pittoresc.&#039;&#039; &amp;amp;nbsp; =  &amp;amp;nbsp; &#039;&#039;Nos vancouveritas es una banda pittoresca.&#039;&#039;  &amp;amp;nbsp; &#039;We Vancouverites are a colourful lot.&#039;&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;Le timor era incognoscite.&#039;&#039;  &amp;amp;nbsp; =  &amp;amp;nbsp; &#039;&#039;Le timor esseva incognoscite.&#039;&#039;  &amp;amp;nbsp; &#039;Fear was unknown.&#039;&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;Que sera, sera.&#039;&#039;  &amp;amp;nbsp; =  &amp;amp;nbsp; &#039;&#039;Que essera, essera.&#039;&#039;  &amp;amp;nbsp; &#039;What will be, will be.&#039;&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;Il serea melior si nos non veniva.&#039;&#039; &amp;amp;nbsp; =  &amp;amp;nbsp; &#039;&#039;Il esserea melior si nos non veniva.&#039;&#039; &amp;amp;nbsp; &#039;It would be better if we hadn&#039;t come.&#039;&lt;br /&gt;
&lt;br /&gt;
The forms &#039;&#039;io so&#039;&#039; &#039;I am&#039; and &#039;&#039;nos somos&#039;&#039; &#039;we are&#039; also exist but are rarely used.&lt;br /&gt;
&lt;br /&gt;
====Double-stem verbs====&lt;br /&gt;
The Neolatin vocabulary that underlies Interlingua includes a group of verbs whose stems mutate when attached to certain suffixes. For example, &#039;&#039;agente, agentia, actrice, activista, reagente, reaction&#039;&#039; are all derivatives of &#039;&#039;ager&#039;&#039; &#039;to act&#039;, but some use the primary stem &#039;&#039;ag-&#039;&#039;, while others use the secondary stem &#039;&#039;act-&#039;&#039;. There are hundreds of such verbs, especially in international scientific vocabulary.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;sentir&#039;&#039; &#039;to feel&#039; (second stem: &#039;&#039;sens-&#039;&#039;) → &#039;&#039;sentimento, sensor&#039;&#039;&lt;br /&gt;
: &#039;&#039;repeller&#039;&#039; &#039;to push away&#039; (second stem: &#039;&#039;repuls-&#039;&#039;) → &#039;&#039;repellente, repulsive&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
This raises a logical issue. Adding &#039;&#039;-e&#039;&#039; to one of these secondary stems produces an adjective that is structurally and semantically equivalent to the past participle of the same verb. &#039;&#039;Experte&#039;&#039;, for example, is related to &#039;&#039;experir&#039;&#039; &#039;to experience&#039;, which has the past participle &#039;&#039;experite&#039;&#039;. Yet, semantically, there is little difference between &#039;&#039;un experte carpentero&#039;&#039; &#039;an expert carpenter&#039; and  &#039;&#039;un experite carpentero&#039;&#039; &#039;an experienced carpenter&#039;. Effectively, &#039;&#039;experte&#039;&#039; = &#039;&#039;experite&#039;&#039;. Furthermore, one can form a word like &#039;&#039;le experito&#039;&#039; &#039;the experienced one&#039; as a quasi-synonym of &#039;&#039;le experto&#039;&#039; &#039;the expert&#039;.&lt;br /&gt;
&lt;br /&gt;
This process can be reversed. That is, can one substitute &#039;&#039;experte&#039;&#039; for &#039;&#039;experite&#039;&#039; in compound tenses (and other second-stem adjectives for other past participles).&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Io ha experte tal cosas antea.&#039;&#039; &amp;amp;nbsp; = &amp;amp;nbsp; &#039;&#039;Io ha experite tal cosas antea.&#039;&#039; &amp;amp;nbsp; &#039;I&#039;ve experienced such things before.&#039;&lt;br /&gt;
: &#039;&#039;Illa ha scripte con una pluma.&#039;&#039; &amp;amp;nbsp; = &amp;amp;nbsp; &#039;&#039;Illa ha scribite con una pluma.&#039;&#039; &amp;amp;nbsp; &#039;She wrote with a quill.&#039;&lt;br /&gt;
&lt;br /&gt;
The original Interlingua grammar (Gode &amp;amp; Blair, 1951) permitted this usage, and illustrated it in one experimental text. A minority of Interlinguists employ the irregular roots, at least occasionally, more often with recognizable forms like &#039;&#039;scripte&#039;&#039; (for &#039;&#039;scribite&#039;&#039; &#039;written&#039;) than opaque ones like &#039;&#039;fisse&#039;&#039; (for &#039;&#039;findite&#039;&#039; &#039;split&#039;). The practice is controversial. Deprecators suggest that they may confuse beginners. Proponents argue that by using the irregular participles, students of Interlingua become more aware of the connections between words like &#039;&#039;agente&#039;&#039; and &#039;&#039;actor&#039;&#039;, &#039;&#039;consequentia&#039;&#039; and &#039;&#039;consecutive&#039;&#039;, and so on. A compromise position holds that the irregular forms may be useful in some educational contexts (e.g., when using Interlingua to teach international scientific vocabulary or as an intermediate step in the study of Romance languages), but not in general communication.&lt;br /&gt;
&lt;br /&gt;
A similar issue concerns the present participles of &#039;&#039;caper&#039;&#039; &#039;to grasp, seize&#039;, &#039;&#039;facer&#039;&#039; &#039;to do, make&#039;, &#039;&#039;saper&#039;&#039; &#039;to know&#039;, and all verbs ending in &#039;&#039;-ciper&#039;&#039;, &#039;&#039;-ficer&#039;&#039;, and &#039;&#039;-jicer&#039;&#039;. The regular forms are &#039;&#039;facente&#039;&#039;, &#039;&#039;sapente&#039;&#039;, etc., but the &amp;quot;preferred forms&amp;quot;, according to the original grammar, are &#039;&#039;faciente&#039;&#039;, sapiente,&#039;&#039; etc.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;un homine sapiente&#039;&#039; &amp;amp;nbsp; = &amp;amp;nbsp; &#039;&#039;un homine sapente&#039;&#039; &amp;amp;nbsp; &#039;a knowledgeable person&#039;&lt;br /&gt;
: &#039;&#039;Recipiente le littera, ille grimassava.&#039;&#039; &amp;amp;nbsp; = &amp;amp;nbsp; &#039;&#039;Recipente le littera, ille grimassava.&#039;&#039; &amp;amp;nbsp; &#039;Receiving the letter, he grimaced.&#039;&lt;br /&gt;
&lt;br /&gt;
Today, most users employ the regular forms in spontaneous usage. Forms like &#039;&#039;sufficiente&#039;&#039; are often used as adjectives, under the influence of similar forms in the source languages.&lt;br /&gt;
&lt;br /&gt;
==Syntax==&lt;br /&gt;
Word order is subject–verb–object, though this may be relaxed where the sense is clear.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Ille reface horologios.&#039;&#039; &amp;amp;nbsp; &#039;He fixes clocks.&#039;&lt;br /&gt;
: &#039;&#039;Amandolos ama io tanto, io comprava una amandoliera.&#039;&#039; &amp;amp;nbsp; &#039;I love almonds so much, I bought an almond orchard.&#039;&lt;br /&gt;
&lt;br /&gt;
Pronouns, however, tend to follow the Romance pattern subject–object–verb, except for infinitives and imperatives, where the object follows the verb.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Ille los reface.&#039;&#039; &amp;amp;nbsp; &#039;He fixes them.&#039;&lt;br /&gt;
: &#039;&#039;Nos vole obtener lo.&#039;&#039;  &amp;amp;nbsp; &#039;We want to get it.&#039;&lt;br /&gt;
: &#039;&#039;Jecta lo via!&#039;&#039;  &amp;amp;nbsp; &#039;Throw it away!&#039;&lt;br /&gt;
&lt;br /&gt;
When two pronouns, one a direct and one an indirect object, occur with the same verb, the indirect object comes first.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Io les lo inviava per avion.&#039;&#039; &amp;amp;nbsp; &#039;I sent it to them by air.&#039;&lt;br /&gt;
: &#039;&#039;Io la los inviava per nave.&#039;&#039; &amp;amp;nbsp; &#039;I sent them to her by ship.&#039;&lt;br /&gt;
&lt;br /&gt;
The position of adverbs and adverbial phrases is similar to English.&lt;br /&gt;
&lt;br /&gt;
===Questions===&lt;br /&gt;
Questions can be created in several ways, familiar to French speakers.&lt;br /&gt;
&lt;br /&gt;
* By reversing the position of the subject and verb.&lt;br /&gt;
&lt;br /&gt;
:: &#039;&#039;Ha ille arrivate?&#039;&#039; &amp;amp;nbsp; &#039;Has he arrived?&#039;&lt;br /&gt;
:: &#039;&#039;Cognosce tu ben Barcelona?&#039;&#039;&amp;amp;nbsp; &#039;Do you know Barcelona well?&#039;&lt;br /&gt;
:: &#039;&#039;Te place le filmes de Quentin Tarantino?&#039;&#039; &#039;Do you like the films of Quentin Tarantino?&#039;&lt;br /&gt;
&lt;br /&gt;
* By replacing the subject with an interrogative word.&lt;br /&gt;
&lt;br /&gt;
:: &#039;&#039;Qui ha dicite isto?&#039;&#039; &amp;amp;nbsp; &#039;Who said this?&#039;&lt;br /&gt;
:: &#039;&#039;&amp;quot;Que cadeva super te?&amp;quot; &amp;quot;Un incude.&amp;quot;&#039;&#039; &amp;amp;nbsp; &#039;&amp;quot;What fell on you?&amp;quot; &amp;quot;An anvil.&amp;quot;&#039;&lt;br /&gt;
&lt;br /&gt;
* For questions that can be answered with &#039;yes&#039; or &#039;no&#039;, by adding the particle &#039;&#039;esque&#039;&#039; (or rarer &#039;&#039;an&#039;&#039;) to the start of the sentence.&lt;br /&gt;
&lt;br /&gt;
:: &#039;&#039;Esque illa vermente lassava su fortuna a su catto?&#039;&#039; &amp;amp;nbsp; (or &#039;&#039;An illa...&#039;&#039;) &amp;amp;nbsp; &#039;Did she really leave her fortune to her cat?&#039;&lt;br /&gt;
&lt;br /&gt;
* By changing the intonation or adding a question mark, while keeping the normal word order.&lt;br /&gt;
&lt;br /&gt;
:: &#039;&#039;Tu jam ha finite tu labores?&#039;&#039; &amp;amp;nbsp; &#039;You finished your work yet?&#039;&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
*Gode, Alexander, and Hugh E. Blair. &#039;&#039;Interlingua: a grammar of the international language&#039;&#039;. Storm Publishers, New York, 1951.&lt;br /&gt;
&lt;br /&gt;
[[Category:Interlingua]]&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=Interlingua&amp;diff=176055</id>
		<title>Interlingua</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=Interlingua&amp;diff=176055"/>
		<updated>2025-11-14T14:29:26Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* Morphology */ subpage&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;{|border=1 align=right cellpadding=4 cellspacing=0 width=50% class=&amp;quot;bordertable&amp;quot; style=&amp;quot;margin: 0 0 1em 1em; background: #f9f9f9; font-size: 95%; float: right;&amp;quot;&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot; bgcolor=&amp;quot;#FFFFFF&amp;quot; align=&amp;quot;center&amp;quot; |&#039;&#039;&#039;Interlingua&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|valign=&amp;quot;top&amp;quot;|Spoken in:&lt;br /&gt;
||many countries of Earth&lt;br /&gt;
|-&lt;br /&gt;
|valign=&amp;quot;top&amp;quot;|Timeline/Universe:&lt;br /&gt;
||[[international auxiliary language]]&lt;br /&gt;
|-&lt;br /&gt;
|valign=&amp;quot;top&amp;quot;|Total speakers:&lt;br /&gt;
||unknown&lt;br /&gt;
|-&lt;br /&gt;
|valign=&amp;quot;top&amp;quot;|Genealogical classification:&lt;br /&gt;
||A posteriori&lt;br /&gt;
:Romance-based&lt;br /&gt;
|-&lt;br /&gt;
|valign=&amp;quot;top&amp;quot;|[[Basic word order]]:&lt;br /&gt;
||SVO&lt;br /&gt;
|-&lt;br /&gt;
|valign=&amp;quot;top&amp;quot;|[[Morphological type]]:&lt;br /&gt;
||agglutinating&lt;br /&gt;
|-&lt;br /&gt;
|valign=&amp;quot;top&amp;quot;|[[Morphosyntactic alignment]]:&lt;br /&gt;
||accusative&lt;br /&gt;
|-&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot; bgcolor=&amp;quot;#FFFFFF&amp;quot; align=&amp;quot;center&amp;quot; |&#039;&#039;&#039;Created by:&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
||IALA ||1951&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Interlingua&#039;&#039;&#039; is an [[international auxiliary language]] developed and promoted by the &#039;&#039;International Auxiliary Language Association&#039;&#039; (&#039;&#039;&#039;IALA&#039;&#039;&#039;).  The language is a [[naturalistic auxlang|naturalistic]] IAL based on common grammar and vocabulary found in [[Romance languages]] (namely [[French]], [[Italian]], [[Spanish]], and [[Portuguese]]) and Latin-influenced non-Romance languages (namely [[English]] and, to a lesser degree, [[German]] and [[Russian]]).&lt;br /&gt;
&lt;br /&gt;
== Anthropology ==&lt;br /&gt;
[[File:Flag_of_Interlingua.svg|thumb|right|Flag of Interlingua]]&lt;br /&gt;
Interlingua focuses on common vocabulary shared by Western European languages, which are often descended from or heavily influenced by the Latin language (such as the Romance languages) and Greek language. Interlingua organizers have four &amp;quot;primary control languages&amp;quot; where, by default, a word (or variant thereof) is expected to appear in at least three of them to qualify for inclusion in Interlingua. These are English; French; Italian; and a combination of Spanish and Portuguese which are treated as a single mega-language for Interlingua purposes, as both are west Iberian languages. Additionally, German and Russian have been dubbed &amp;quot;secondary control languages&amp;quot;. While the result is often akin to Neo-Latin as the most frequent source of commonality, Interlingua words can have origins in any language, as long as they have drifted into the primary control languages as loanwords. For example, the Japanese words geisha and samurai and the Finnish word sauna are used in most Western European languages, and therefore in Interlingua as well; similarly, the Guugu Yimithirr word gangurru is used in latinized form (Interlingua: kanguru, English: kangaroo).[3]&lt;br /&gt;
&lt;br /&gt;
The maintainers of Interlingua attempt to keep the grammar simple and word formation regular, and use only a small number of roots and affixes. This is intended to make the language quicker to learn.  The American heiress Alice Vanderbilt Morris (1874–1950) became interested in linguistics and the international auxiliary language movement in the early 1920s. In 1924, Morris and her husband, Dave Hennen Morris, established the non-profit International Auxiliary Language Association (IALA) in New York City. Their aim was to place the study of IALs on a more complex and scientific basis. Morris developed the research program of IALA in consultation with Edward Sapir, William Edward Collinson, and Otto Jespersen.&lt;br /&gt;
&lt;br /&gt;
Investigations of the auxiliary language problem were in progress at the International Research Council, the American Council on Education, the American Council of Learned Societies, the British, French, Italian, and American Associations for the advancement of science, and other groups of specialists. Morris created IALA as a continuation of this work.&lt;br /&gt;
&lt;br /&gt;
==Phonology==&lt;br /&gt;
&lt;br /&gt;
The phonology of Interlingua was described in 1951 by Alexander Gode and Hugh Blair in the IALA publication &#039;&#039;A Grammar of Interlingua&#039;&#039;.&amp;lt;ref&amp;gt;[http://members.optus.net/~ado_hall/interlingua/gi/spell/index.html &amp;quot;Spelling &amp;amp; Pronunciation,&amp;quot; &#039;&#039;A Grammar of Interlingua&#039;&#039;].&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Consonants===&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;text-align:center;&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
!&lt;br /&gt;
!colspan=&amp;quot;2&amp;quot;| Bilabial&lt;br /&gt;
!colspan=&amp;quot;2&amp;quot;| Labio-&amp;lt;br/&amp;gt;dental&lt;br /&gt;
!colspan=&amp;quot;2&amp;quot;| Alveolar&lt;br /&gt;
!colspan=&amp;quot;2&amp;quot;| Post-&amp;lt;br/&amp;gt;alveolar&lt;br /&gt;
!colspan=&amp;quot;2&amp;quot;| Palatal&lt;br /&gt;
!colspan=&amp;quot;2&amp;quot;| Labial-&amp;lt;br/&amp;gt;velar&lt;br /&gt;
!colspan=&amp;quot;2&amp;quot;| Velar&lt;br /&gt;
!colspan=&amp;quot;2&amp;quot;| Glottal&lt;br /&gt;
|-&lt;br /&gt;
! Plosive&lt;br /&gt;
| {{IPA|p}} || {{IPA|b}}&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
| {{IPA|t}} || {{IPA|d}}&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
| {{IPA|k}} || {{IPA|ɡ}}&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|-&lt;br /&gt;
! Nasal&lt;br /&gt;
| colspan=&amp;quot;2&amp;quot; |  {{IPA|m}}&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
| colspan=&amp;quot;2&amp;quot; | {{IPA|n}}&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|-&lt;br /&gt;
! Tap&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
| || {{IPA|ɾ}}&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|-&lt;br /&gt;
! Fricative&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
| {{IPA|f}} || {{IPA|v}}&lt;br /&gt;
| {{IPA|s}} || {{IPA|z}}&lt;br /&gt;
| {{IPA|ʃ}} || rowspan=2| {{IPA|(d)ʒ}}&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
| ({{IPA|h}}) ||&lt;br /&gt;
|-&lt;br /&gt;
! Affricates&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;1&amp;quot;|{{IPA|ts~s}}&lt;br /&gt;
|colspan=&amp;quot;1&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|-&lt;br /&gt;
! Approximant&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
| || {{IPA|j}}&lt;br /&gt;
| || {{IPA|w}}&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|-&lt;br /&gt;
! Lateral approximant&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
| || {{IPA|l}}&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|colspan=&amp;quot;2&amp;quot;|&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== Vowels ===&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
!&lt;br /&gt;
! Front&lt;br /&gt;
! Back&lt;br /&gt;
|-&lt;br /&gt;
! Close&lt;br /&gt;
| {{IPA|i}}&lt;br /&gt;
| {{IPA|u}}&lt;br /&gt;
|-&lt;br /&gt;
! Close-mid&lt;br /&gt;
| {{IPA|e}}&lt;br /&gt;
| {{IPA|o}}&lt;br /&gt;
|-&lt;br /&gt;
! Open&lt;br /&gt;
| {{IPA|a}}&lt;br /&gt;
|&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
== Morphology ==&lt;br /&gt;
{{Main|Interlingua/Morphology}}&lt;br /&gt;
There is some systemic marking for parts of speech. But, for example, nouns do not have to end in any particular letter. Typically, however, adjectives end in &#039;&#039;-e&#039;&#039; or &#039;&#039;-a&#039;&#039;, adverbs end in &#039;&#039;-menti&#039;&#039; or &#039;&#039;-o&#039;&#039;, while nouns end in &#039;&#039;-a, -e, -o&#039;&#039; or a consonant. Finite verbs virtually always end in &#039;&#039;-a, -e,&#039;&#039; or &#039;&#039;-i&#039;&#039;, while infinitives add &#039;&#039;-r&#039;&#039;: &#039;&#039;scribe&#039;&#039;, &#039;write&#039;, &#039;writes&#039;; &#039;&#039;scriber&#039;&#039;, &#039;to write&#039;.&lt;br /&gt;
&lt;br /&gt;
===Articles===&lt;br /&gt;
&amp;lt;div style=&amp;quot;float:right&amp;quot;&amp;gt;&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Interlingua 2.0&lt;br /&gt;
! Definite article&lt;br /&gt;
| le || la&lt;br /&gt;
|-&lt;br /&gt;
! Indefinite article&lt;br /&gt;
| un || una&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;/div&amp;gt;&lt;br /&gt;
The definite article is &#039;&#039;le&#039;&#039;, the indefinite article is &#039;&#039;un&#039;&#039;, and neither article shows any agreement in form with nouns. The prepositions &#039;&#039;a&#039;&#039; (&amp;quot;to&amp;quot;) and &#039;&#039;de&#039;&#039; (&amp;quot;of&amp;quot;) fuse with a following &#039;&#039;le&#039;&#039; into &#039;&#039;al&#039;&#039; and &#039;&#039;del&#039;&#039; respectively.&lt;br /&gt;
&lt;br /&gt;
The definite article is, on the whole, used as in English, with the exception that it should not be omitted with titles preceding proper names nor with abstract nouns representing an entire class, species, etc.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Nouns===&lt;br /&gt;
&amp;lt;div style=&amp;quot;float:right&amp;quot;&amp;gt;&lt;br /&gt;
&#039;&#039;&#039;Interlingua 2.0&#039;&#039;&#039; has gender, &amp;lt;br /&amp;gt;like all Romance languages&lt;br /&gt;
&amp;lt;/div&amp;gt;&lt;br /&gt;
Nouns inflect for number only. Plural nouns take &#039;&#039;-s&#039;&#039; after a vowel, &#039;&#039;-es&#039;&#039; after a consonant (but final &#039;&#039;-c, -g&#039;&#039; change in spelling to &#039;&#039;-ches, -ghes&#039;&#039; to preserve the hard {{IPA|[k] and [g]}} sound of &#039;&#039;c&#039;&#039; and &#039;&#039;g&#039;&#039;).&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;catto&#039;&#039; &amp;amp;nbsp; &#039;cat&#039;&amp;amp;nbsp; →&amp;amp;nbsp; &#039;&#039;cattos&#039;&#039;&amp;amp;nbsp; &#039;cats&#039;&lt;br /&gt;
:&#039;&#039;can&#039;&#039;&amp;amp;nbsp; &#039;dog&#039;&amp;amp;nbsp; → &amp;amp;nbsp;&#039;&#039;canes&#039;&#039;&amp;amp;nbsp; &#039;dogs&#039;&lt;br /&gt;
:&#039;&#039;roc&#039;&#039; &amp;amp;nbsp; &#039;rook&#039; [chess] &amp;amp;nbsp; → &amp;amp;nbsp;&#039;&#039;roches&#039;&#039;&amp;amp;nbsp; &#039;rooks&#039;&lt;br /&gt;
&lt;br /&gt;
Interlingua has no grammatical gender. Animate nouns are sex-neutral, unless they refer specifically to a male or a female. Thus, &#039;&#039;jornalista&#039;&#039; &#039;journalist&#039; and &#039;&#039;scientista&#039;&#039; &#039;scientist&#039; are sex-neutral, while &#039;&#039;rege&#039;&#039; &#039;king&#039; and &#039;&#039;regina&#039;&#039; &#039;queen&#039; are sex-specific. Explicit feminine forms can be created by substituting final &#039;&#039;-a&#039;&#039; for a final &#039;&#039;-o&#039;&#039; or &#039;&#039;-e&#039;&#039; or by adding the suffix &#039;&#039;-essa&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;puero&#039;&#039; &amp;amp;nbsp; &#039;boy&#039; &amp;amp;nbsp; → &amp;amp;nbsp;&#039;&#039;puera&#039;&#039;&amp;amp;nbsp; &#039;girl&#039;&lt;br /&gt;
:&#039;&#039;tigre&#039;&#039; &amp;amp;nbsp; &#039;tiger&#039; &amp;amp;nbsp; → &amp;amp;nbsp;&#039;&#039;tigressa&#039;&#039;&amp;amp;nbsp; &#039;female tiger&#039;&lt;br /&gt;
&lt;br /&gt;
These colour the regular forms as masculine when they appear in the same context.&lt;br /&gt;
&lt;br /&gt;
Unlike in English, nouns cannot take adjectival forms, such as &#039;winter weather&#039;, &#039;research laboratory&#039;, &#039;fall coat&#039;, etc. Such constructions instead require the use of a preposition or a corresponding adjective, respectively &#039;&#039;tempore hibernal&#039;&#039;, &#039;&#039;laboratoria de recerca&#039;&#039;, and &#039;&#039;mantello pro autumno&#039;&#039;. This is however excepted by proper nouns which can be used adjectivally as in English: &#039;&#039;contator Geiger&#039;&#039; &#039;Geiger counter&#039;, &#039;&#039;motor Diesel&#039;&#039; &#039;Diesel engine&#039;, &#039;&#039;radios Röntgen&#039;&#039; &#039;Roentgen rays&#039;, etc.&lt;br /&gt;
&lt;br /&gt;
Despite the above restrictions, Interlingua permits use of apposition, where the two nouns refer to the same thing.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;arbore nano&#039;&#039; &#039;dwarf tree&#039;&lt;br /&gt;
: &#039;&#039;nave domo&#039;&#039; &#039;house boat&#039;&lt;br /&gt;
&lt;br /&gt;
Male and female forms should match.&lt;br /&gt;
&lt;br /&gt;
===Adjectives===&lt;br /&gt;
&amp;lt;div style=&amp;quot;float:right&amp;quot;&amp;gt;&lt;br /&gt;
&#039;&#039;&#039;Interlingua 2.0&#039;&#039;&#039; adjective&amp;lt;br /&amp;gt;agree with their head noun &amp;lt;br/&amp;gt; in number and gender.&amp;lt;br/&amp;gt;&amp;lt;br/&amp;gt;&#039;&#039;belles oculos&#039;&#039; or &#039;&#039;oculos belles&#039;&#039;&amp;lt;br/&amp;gt;&#039;&#039;una bona idea, una idea ingeniosa&#039;&#039;&lt;br /&gt;
&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Adjectives may precede or follow the noun they modify. As a matter of style, short adjectives tend to precede, long adjectives tend to follow. Numerals always precede the noun.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;belle oculos&#039;&#039; or &#039;&#039;oculos belle&#039;&#039; &amp;amp;nbsp; &#039;beautiful eyes&#039;&lt;br /&gt;
: &#039;&#039;un bon idea, un idea ingeniose&#039;&#039; &amp;amp;nbsp; &#039;a good idea, an ingenious idea&#039;&lt;br /&gt;
&lt;br /&gt;
An adjective never has to agree with the noun it modifies, but adjectives may be pluralized when there is no explicit noun to modify.&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;le parve infantes&#039;&#039; &amp;amp;nbsp; &#039;the little children&#039;;  &amp;amp;nbsp; but  &amp;amp;nbsp; &#039;&#039;le parves&#039;&#039; &amp;amp;nbsp; &#039;the little ones&#039;&lt;br /&gt;
&lt;br /&gt;
Comparative degree is expressed by &#039;&#039;plus&#039;&#039; or &#039;&#039;minus&#039;&#039; preceding the adjective and superlative degree by &#039;&#039;le plus&#039;&#039; or &#039;&#039;le minus&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;un plus feroce leon&#039;&#039; &amp;amp;nbsp; &#039;a fiercer lion&#039;&lt;br /&gt;
:&#039;&#039;un traino minus rapide&#039;&#039; &amp;amp;nbsp; &#039;a less speedy train&#039;&lt;br /&gt;
:&#039;&#039;le plus alte arbore&#039;&#039; &amp;amp;nbsp; &#039;the tallest tree&#039;&lt;br /&gt;
:&#039;&#039;le solution le minus costose&#039;&#039; &amp;amp;nbsp; &#039;the least costly solution&#039;.&lt;br /&gt;
&lt;br /&gt;
The suffix &#039;&#039;-issime&#039;&#039; may be used to express the absolute superlative degree.&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;un aventura excellentissime&#039;&#039; &amp;amp;nbsp; &#039;a most excellent adventure&#039;&lt;br /&gt;
&lt;br /&gt;
The adjectives &#039;&#039;bon&#039;&#039; &#039;good&#039;, &#039;&#039;mal&#039;&#039; &#039;bad&#039;, &#039;&#039;magne&#039;&#039; &#039;great&#039;, and &#039;&#039;parve&#039;&#039; &#039;small&#039; have optional irregular forms for the comparative and superlative.&lt;br /&gt;
&lt;br /&gt;
:{|&lt;br /&gt;
|-&lt;br /&gt;
|&#039;&#039;bon → plus bon → le plus bon&#039;&#039; || &amp;amp;nbsp; || or || &amp;amp;nbsp; || &#039;&#039;bon → melior → optime&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|&#039;&#039;mal → plus mal → le plus mal&#039;&#039; || &amp;amp;nbsp; || or || &amp;amp;nbsp; || &#039;&#039;mal → pejor → pessime&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|&#039;&#039;magne → plus magne → le plus magne&#039;&#039; || &amp;amp;nbsp; || or || &amp;amp;nbsp; || &#039;&#039;magne → major → maxime&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|&#039;&#039;parve → plus parve → le plus parve&#039;&#039; || &amp;amp;nbsp; || or || &amp;amp;nbsp; || &#039;&#039;parve → minor → minime&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Theoretically, every adjective may serve as a pronoun referring to something expressed in a previous passage.&lt;br /&gt;
&lt;br /&gt;
=== Adverbs===&lt;br /&gt;
There are two types of adverbs, primary and secondary. Primary adverbs are a [[Closed-class word|closed class]] of grammatical operators, such as &#039;&#039;quasi,&#039;&#039; &#039;almost&#039;; &#039;&#039;jam,&#039;&#039; &#039;already&#039;; and &#039;&#039;totevia,&#039;&#039; &#039;anyway&#039;. Secondary adverbs are an [[Open class word|open class]] derived from corresponding adjectives by adding the suffix &#039;&#039;-mente&#039;&#039; (&#039;&#039;-amente&#039;&#039; after final &#039;&#039;-c&#039;&#039;).&lt;br /&gt;
&lt;br /&gt;
:&#039;&#039;felice&#039;&#039; &amp;amp;nbsp; &#039;happy&#039; &amp;amp;nbsp; → &amp;amp;nbsp; &#039;&#039;felicemente&#039;&#039; &amp;amp;nbsp; &#039;happily&#039;&lt;br /&gt;
:&#039;&#039;magic&#039;&#039; &amp;amp;nbsp; &#039;magical&#039; &amp;amp;nbsp; → &amp;amp;nbsp; &#039;&#039;magicamente&#039;&#039; &amp;amp;nbsp; &#039;magically&#039;&lt;br /&gt;
&lt;br /&gt;
A few common adverbs have optional short forms in &#039;&#039;-o&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;sol&#039;&#039; &amp;amp;nbsp; &#039;alone&#039; &amp;amp;nbsp; → &amp;amp;nbsp; &#039;&#039;solo&#039;&#039; or &#039;&#039;solmente&#039;&#039; &amp;amp;nbsp; &#039;only&#039;&lt;br /&gt;
&lt;br /&gt;
Like adjectives, adverbs use &#039;&#039;plus&#039;&#039; and &#039;&#039;minus&#039;&#039; to express the comparative and &#039;&#039;le plus&#039;&#039; and &#039;&#039;le minus&#039;&#039; to express the superlative.&lt;br /&gt;
&lt;br /&gt;
: &#039;&#039;Illa canta plus bellemente que illa parla.&#039;&#039; &amp;amp;nbsp; &#039;She sings more beautifully than she speaks.&#039;&lt;br /&gt;
: &#039;&#039;Le gepardo curre le plus rapide de omne animales.&#039;&#039; &amp;amp;nbsp; &#039;The cheetah runs the fastest of all animals.&#039;&lt;br /&gt;
&lt;br /&gt;
The adverbs equivalent to &#039;&#039;bon,&#039;&#039; &#039;good&#039; and &#039;&#039;mal,&#039;&#039; &#039;bad&#039; have optional irregular forms.&lt;br /&gt;
&lt;br /&gt;
:{|&lt;br /&gt;
|-&lt;br /&gt;
|&#039;&#039;bonmente → plus bonmente → le plus bonmente&#039;&#039; || &amp;amp;nbsp; || or || &amp;amp;nbsp; || &#039;&#039;ben → plus ben → le plus ben&#039;&#039; || &amp;amp;nbsp; || or || &amp;amp;nbsp; || &#039;&#039;ben → melio → optimo&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|&#039;&#039;malmente → plus malmente→ le plus malmente&#039;&#039; || &amp;amp;nbsp; || or || &amp;amp;nbsp; || &#039;&#039;mal → plus mal → le plus mal&#039;&#039; || &amp;amp;nbsp; || or || &amp;amp;nbsp; || &#039;&#039;mal → pejo → pessimo&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
== Notes ==&lt;br /&gt;
&amp;lt;references/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[Category:Conlangs]]&lt;br /&gt;
[[Category:Auxlangs]]&lt;br /&gt;
[[Category: A posteriori conlangs]]&lt;br /&gt;
&lt;br /&gt;
{{Universal Language}}&lt;br /&gt;
{{Auxlangs}}&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=Universal_Languages/Swadesh&amp;diff=176054</id>
		<title>Universal Languages/Swadesh</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=Universal_Languages/Swadesh&amp;diff=176054"/>
		<updated>2025-11-14T14:09:14Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: Created page with &amp;quot;{| class=&amp;quot;wikitable&amp;quot; | align=&amp;quot;center&amp;quot; style=&amp;quot;background:#f0f0f0;&amp;quot;|&amp;#039;&amp;#039;&amp;#039;No&amp;#039;&amp;#039;&amp;#039; | align=&amp;quot;center&amp;quot; style=&amp;quot;background:#f0f0f0;&amp;quot;|&amp;#039;&amp;#039;&amp;#039;English&amp;#039;&amp;#039;&amp;#039; | align=&amp;quot;center&amp;quot; style=&amp;quot;background:#f0f0f0;&amp;quot;|&amp;#039;&amp;#039;&amp;#039;Intralingua&amp;#039;&amp;#039;&amp;#039; | align=&amp;quot;center&amp;quot; style=&amp;quot;background:#f0f0f0;&amp;quot;|&amp;#039;&amp;#039;&amp;#039;Interslavic&amp;#039;&amp;#039;&amp;#039; | align=&amp;quot;center&amp;quot; style=&amp;quot;background:#f0f0f0;&amp;quot;|&amp;#039;&amp;#039;&amp;#039;Folksprak&amp;#039;&amp;#039;&amp;#039; | align=&amp;quot;center&amp;quot; style=&amp;quot;background:#f0f0f0;&amp;quot;|&amp;#039;&amp;#039;&amp;#039;Middle Semitic&amp;#039;&amp;#039;&amp;#039; | align=&amp;quot;center&amp;quot; style=&amp;quot;background:#f0f0f0;&amp;quot;|&amp;#039;&amp;#039;&amp;#039;Dan&amp;#039;a&amp;#039;yo&amp;#039;&amp;#039;&amp;#039; |- | 1 || &amp;#039;&amp;#039;&amp;#039;I&amp;#039;&amp;#039;&amp;#039; || io ||...&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
| align=&amp;quot;center&amp;quot; style=&amp;quot;background:#f0f0f0;&amp;quot;|&#039;&#039;&#039;No&#039;&#039;&#039;&lt;br /&gt;
| align=&amp;quot;center&amp;quot; style=&amp;quot;background:#f0f0f0;&amp;quot;|&#039;&#039;&#039;English&#039;&#039;&#039;&lt;br /&gt;
| align=&amp;quot;center&amp;quot; style=&amp;quot;background:#f0f0f0;&amp;quot;|&#039;&#039;&#039;Intralingua&#039;&#039;&#039;&lt;br /&gt;
| align=&amp;quot;center&amp;quot; style=&amp;quot;background:#f0f0f0;&amp;quot;|&#039;&#039;&#039;Interslavic&#039;&#039;&#039;&lt;br /&gt;
| align=&amp;quot;center&amp;quot; style=&amp;quot;background:#f0f0f0;&amp;quot;|&#039;&#039;&#039;Folksprak&#039;&#039;&#039;&lt;br /&gt;
| align=&amp;quot;center&amp;quot; style=&amp;quot;background:#f0f0f0;&amp;quot;|&#039;&#039;&#039;Middle Semitic&#039;&#039;&#039;&lt;br /&gt;
| align=&amp;quot;center&amp;quot; style=&amp;quot;background:#f0f0f0;&amp;quot;|&#039;&#039;&#039;Dan&#039;a&#039;yo&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
| 1 || &#039;&#039;&#039;I&#039;&#039;&#039; || io || я || {{Rune|ᛁᛣᛣ}} || {{Sy|ܐܢܐ}}  || {{Ruby|我|아}}&lt;br /&gt;
|-&lt;br /&gt;
| 2 || &#039;&#039;&#039;thou&#039;&#039;&#039; || tu || ты || {{Rune|ᛞᚢ}} || {{Sy|ܐܢܬܐ}} m {{Sy|ܐܢܬܝ}} || {{Ruby|君|군}}&lt;br /&gt;
|-&lt;br /&gt;
| 3 || &#039;&#039;&#039;he&#039;&#039;&#039; || ille || он || {{Rune|ᚻᛁ}} || ܗܘܐ (húwâ) || {{Ruby|其人|기닌}}&lt;br /&gt;
|-&lt;br /&gt;
| 4 || &#039;&#039;&#039;we&#039;&#039;&#039; || nos || мы || || {{Sy|ܐܢܚܢܘ}} || 我等 ( 아둥 )&lt;br /&gt;
|-&lt;br /&gt;
| 5 || &#039;&#039;&#039;you&#039;&#039;&#039; || vos || вы || || {{Sy|ܐܢܬܘܡ}} || 君等 ( 군등 )&lt;br /&gt;
|-&lt;br /&gt;
| 6||they||illes||они||||ܗܘܡ (hûm)||其人等 ( 긴닌둥 )&lt;br /&gt;
|-&lt;br /&gt;
| 7||this||iste||Той||||ܗܙܐ (hazâ)||此 ( 처 )&lt;br /&gt;
|-&lt;br /&gt;
| 8||that||illa||Той||||ܙܟܐ (zakâ)||其 ( 기 )&lt;br /&gt;
|-&lt;br /&gt;
| 9||here||hic , ci, qui||ту||||ܗܘܢ (hun)||此処 ( 처초 )&lt;br /&gt;
|-&lt;br /&gt;
| 10||there||illac, ibi , la||там‎||||ܗܘܢܟ (hunak)||其処 ( 기초 )&lt;br /&gt;
|-&lt;br /&gt;
| 11||who||qui||кто||||ܡܥܢ (mîn)||誰 ( 셰 )&lt;br /&gt;
|-&lt;br /&gt;
| 12||what||que||Что‎||ᚹᚪᛏ vat||ܡܢ (man)||何 ( 하 )&lt;br /&gt;
|-&lt;br /&gt;
| 13||where||ubi||кдє‎||ᛇᚪᚱ var||ܐܢܐ (&#039;enâ)||何処 ( 하초 )&lt;br /&gt;
|-&lt;br /&gt;
| 14||when||quando||когда‎||||ܡܬܐ (matâ)||何時 ( 하시 )&lt;br /&gt;
|-&lt;br /&gt;
| 15||how||como||як‎|||| ()||如何 ( 뇨하 )&lt;br /&gt;
|-&lt;br /&gt;
| 16||not||non , ne||нє‎||||ܠܐ (lâ)||不 ( 볻 )&lt;br /&gt;
|-&lt;br /&gt;
| 17||all||tote||||||ܟܘܠ (kol)||皆 ( 겨 )&lt;br /&gt;
|-&lt;br /&gt;
| 18||many||multe|||||| ()||多 ( 다 )&lt;br /&gt;
|-&lt;br /&gt;
| 19||some||alicun||||||ܟܡܐ (kamâ)||某 ( 못 )&lt;br /&gt;
|-&lt;br /&gt;
| 20||few||poc|||||| ()||少 ( 솟 )&lt;br /&gt;
|-&lt;br /&gt;
| 21||other||altere|||||| ()||他 ( 타 )&lt;br /&gt;
|-&lt;br /&gt;
| 22 || &#039;&#039;&#039;one&#039;&#039;&#039; || un || єдин || {{Rune|ᛖᚾ}} || {{Sy|ܘܚܕ}} || {{Ruby|一|읻}}&lt;br /&gt;
|-&lt;br /&gt;
| 23 || &#039;&#039;two&#039;&#039; || duo || два ‎|| {{Rune|ᛏᚹᛖ}} || {{Sy|ܫܢܝܡ}} || {{Ruby|二|늬}}&lt;br /&gt;
|-&lt;br /&gt;
| 24 || &#039;&#039;&#039;three&#039;&#039;&#039; || tres || три‎|| {{Rune|ᛞᚱᛁ}} || {{Sy|ܫܠܫ}}|| {{Ruby|三|삼}}&lt;br /&gt;
|-&lt;br /&gt;
| 25 || &#039;&#039;&#039;four&#039;&#039;&#039; || quatro || четыри || {{Rune|ᚠᛁᚱ}} || {{Sy|ܐܪܒܥ}} || {{Ruby|四|싀}}&lt;br /&gt;
|-&lt;br /&gt;
| 26 || &#039;&#039;&#039;five&#039;&#039;&#039;  || cinque || пет || {{Ruby|ᚠᛁᛗ}} || {{Sy|ܚܡܤܐ}} || {{Ruby|五|오}}&lt;br /&gt;
|-&lt;br /&gt;
| 27 ||big||grande||||ᚷᚱᚩᛏ grot||ܟܒܝܪ (kabir)||太 ( 대 )&lt;br /&gt;
|-&lt;br /&gt;
| 28 ||long||longe||||ᛚᚪᚾᚷ lang|| ()||長 ( 장 )&lt;br /&gt;
|-&lt;br /&gt;
| 29 ||wide||large||||ᛒᚱᛖᛞ bred||ܪܚܒ (raḥab)||広 ( 광 )&lt;br /&gt;
|-&lt;br /&gt;
| 30 ||thick||spisse|||||| ()||厚 ( 홋 )&lt;br /&gt;
|-&lt;br /&gt;
| 31||heavy||pesante|||||| ()||重 ( cong )&lt;br /&gt;
|-&lt;br /&gt;
| 32||small||parve|||||| ()||小 ( so )&lt;br /&gt;
|-&lt;br /&gt;
| 33||short||curte||||||ܩܨܪ (qaṣar)||短 ( dwan )&lt;br /&gt;
|-&lt;br /&gt;
| 34||narrow||stricte|||||| ()||狹 ( hap )&lt;br /&gt;
|-&lt;br /&gt;
| 35||thin||||||||ܪܩܝܩܐ (raqîqâ)||薄 ( bak )&lt;br /&gt;
|-&lt;br /&gt;
| 36||woman||femina|||||| ()||女人 ( nyonin )&lt;br /&gt;
|-&lt;br /&gt;
| 37 || man || viro || || || || 男人 ( namnin )&lt;br /&gt;
|-&lt;br /&gt;
| 38 || human || homine || || {{Rune|ᛗᛖᚾᚳ}} || {{Sy|ܐܢܣܢܐ}} || {{Ruby|人|닌}}&lt;br /&gt;
|-&lt;br /&gt;
| 39||child||infante||||ᛣᛁᚾᛞ||ܘܠܕܐ (waladâ)||児子 ( &#039;eiji )&lt;br /&gt;
|-&lt;br /&gt;
| 40||wife||marita , sposa||||ᚠᚱᚩᚢ||||妻 ( cei )&lt;br /&gt;
|-&lt;br /&gt;
| 41||husband||marito , sposo||||||||丈夫 ( jangbu )&lt;br /&gt;
|-&lt;br /&gt;
| 42||mother||matre||Матка||||||母親 ( moucin )&lt;br /&gt;
|-&lt;br /&gt;
| 43 || father || patre || || || || 父親 ( bucin )&lt;br /&gt;
|-&lt;br /&gt;
| 44 || animal || animal || || {{Rune|ᛞᛁᚱ}} || || {{Ruby|動物|동묻}}&lt;br /&gt;
|-&lt;br /&gt;
| 45 || fish || pisce}} || || {{Rune|ᚠᛁᛋᛣ}} || || 魚 ( &#039;yo )&lt;br /&gt;
|-&lt;br /&gt;
| 46||bird||ave||||||||鳥 ( cou )&lt;br /&gt;
|-&lt;br /&gt;
| 47||dog||can||||ᚻᚢᚾᛞ hund||||犬 ( kwen )&lt;br /&gt;
|-&lt;br /&gt;
| 48||louse||pediculo||||ᛚᚢᛋ lus||||虱 ( sit )&lt;br /&gt;
|-&lt;br /&gt;
| 49||snake||serpente||||||||蛇 ( ta )&lt;br /&gt;
|-&lt;br /&gt;
| 50||worm||verme||||||||蠕虫 ( nujung )&lt;br /&gt;
|-&lt;br /&gt;
| 51||tree||arbore||||||||木 ( mok )&lt;br /&gt;
|-&lt;br /&gt;
| 52||forest||foreste||||||||森林 ( simlim )&lt;br /&gt;
|-&lt;br /&gt;
| 53||stick||baston||||||||棍棒 ( honbang )&lt;br /&gt;
|-&lt;br /&gt;
| 54||fruit||fructo||||ᚠᚱᚢᛉᛏ fruxt||||果実 ( gwasit )&lt;br /&gt;
|-&lt;br /&gt;
| 55||seed||semine||||||||種子 ( jongji )&lt;br /&gt;
|-&lt;br /&gt;
| 56||leaf||folio||||||||葉 ( &#039;yop ) }&lt;br /&gt;
|-&lt;br /&gt;
| 57||root||radice||||||||根 ( gan )&lt;br /&gt;
|-&lt;br /&gt;
| 58||bark||cortice||||||||樹皮 ( subi )&lt;br /&gt;
|-&lt;br /&gt;
| 59||flower||flor||||ᛒᛚᚢᛗ blum||||草花 ( cauhwa )&lt;br /&gt;
|-&lt;br /&gt;
| 60||grass||herba||||ᚷᚱᚪᛋ gras||||草 ( cau )&lt;br /&gt;
|-&lt;br /&gt;
| 61||rope||corda||||||||縄 ( jing )&lt;br /&gt;
|-&lt;br /&gt;
| 62||skin||cute, pelle||||||||皮膚 ( bipu )&lt;br /&gt;
|-&lt;br /&gt;
| 63||meat||carne||||||||肉 ( nuk )&lt;br /&gt;
|-&lt;br /&gt;
| 64||blood||sanguine||||||||血 ( hwet )&lt;br /&gt;
|-&lt;br /&gt;
| 65||bone||osso||||||||骨 ( got )&lt;br /&gt;
|-&lt;br /&gt;
| 66||fat||grassia||||||||脂肪 ( jiipang )&lt;br /&gt;
|-&lt;br /&gt;
| 67||egg||ovo||||||||卵子 ( lanji )&lt;br /&gt;
|-&lt;br /&gt;
| 68||horn||corno||||ᚻᚩᚱᚾ horn||||角 ( gok )&lt;br /&gt;
|-&lt;br /&gt;
| 69||tail||cauda||||||||尾 ( mui )&lt;br /&gt;
|-&lt;br /&gt;
| 70||feather||pluma, penna||||||||羽毛 ( &#039;umau )&lt;br /&gt;
|-&lt;br /&gt;
| 71||hair||pilo, capillo||||||||頭髮 ( toupat )&lt;br /&gt;
|-&lt;br /&gt;
| 72||head||capite||||||||頭 ( tou )&lt;br /&gt;
|-&lt;br /&gt;
| 73||ear||aure||||||||耳 ( ni )&lt;br /&gt;
|-&lt;br /&gt;
| 74||eye||oculo||||||||目 ( muk )&lt;br /&gt;
|-&lt;br /&gt;
| 75||nose||naso||||||||鼻 ( bi )&lt;br /&gt;
|-&lt;br /&gt;
| 76||mouth||bucca, ore||||||||口 ( kou )&lt;br /&gt;
|-&lt;br /&gt;
| 77||tooth||dente||||||||歯 ( ci ) , 長牙 ( jang&#039;a )&lt;br /&gt;
|-&lt;br /&gt;
| 78||tongue||lingua||||||||舌 ( set )&lt;br /&gt;
|-&lt;br /&gt;
| 79||fingernail||ungula||||||||指甲 ( jiigap )&lt;br /&gt;
|-&lt;br /&gt;
| 80||foot||pede||||||||足 ( jok )&lt;br /&gt;
|-&lt;br /&gt;
| 81||leg||gamba||||||||腳 ( gyak )&lt;br /&gt;
|-&lt;br /&gt;
| 82||knee||genu||||||||膝 ( sit )&lt;br /&gt;
|-&lt;br /&gt;
| 83||hand||mano||||ᚻᚪᚾᛞ hand||||手 ( syu )&lt;br /&gt;
|-&lt;br /&gt;
| 84||wing||ala||||||||羽翼 ( &#039;u&#039;ik )&lt;br /&gt;
|-&lt;br /&gt;
| 85||belly||ventre||||||||腹 ( buk )&lt;br /&gt;
|-&lt;br /&gt;
| 86||guts||tripas||||||||腸管 ( canggwan )&lt;br /&gt;
|-&lt;br /&gt;
| 87||neck||collo||||||||頸 ( ging )&lt;br /&gt;
|-&lt;br /&gt;
| 88||back||dorso||||||||背 ( boi )&lt;br /&gt;
|-&lt;br /&gt;
| 89||breast||pectore||||||||胸部 ( hyongbou )&lt;br /&gt;
|-&lt;br /&gt;
| 90||heart||corde||||||||心臓 ( simjang )&lt;br /&gt;
|-&lt;br /&gt;
| 91||liver||ficato, hepato||||||||肝臓 ( ganjang )&lt;br /&gt;
|-&lt;br /&gt;
| 92||drink||biber||||||||飲 ( &#039;um )&lt;br /&gt;
|-&lt;br /&gt;
| 93||eat||mangiar||||||||食 ( sik )&lt;br /&gt;
|-&lt;br /&gt;
| 94||bite||morder||||||||咬 ( &#039;yau )&lt;br /&gt;
|-&lt;br /&gt;
| 95||suck||suger||||||||吸 ( hip )&lt;br /&gt;
|-&lt;br /&gt;
| 96||spit||sputar||||||||吐 ( to )&lt;br /&gt;
|-&lt;br /&gt;
| 97||vomit||vomitar||||||||吐 ( to )&lt;br /&gt;
|-&lt;br /&gt;
| 98||blow||sufflar||||||||吹 ( cui )&lt;br /&gt;
|-&lt;br /&gt;
| 99||breathe||respirar||||||||&lt;br /&gt;
|-&lt;br /&gt;
| 100||laugh||rider||||||||笑 ( syou )&lt;br /&gt;
|-&lt;br /&gt;
| 101||see||vider||||||||見 ( gyen )&lt;br /&gt;
|-&lt;br /&gt;
| 102||hear||audir||||||||聞 ( mun )&lt;br /&gt;
|-&lt;br /&gt;
| 103||know||saper||||||||知 ( jui )&lt;br /&gt;
|-&lt;br /&gt;
| 104||think||pensar||||||||思考 ( sakau )&lt;br /&gt;
|-&lt;br /&gt;
| 105||smell||olfacer||||||||嗅 ( hyu )&lt;br /&gt;
|-&lt;br /&gt;
| 106||fear||timer||||||||恐怖 ( kongpo )&lt;br /&gt;
|-&lt;br /&gt;
| 107||sleep||dormir||||||||寝 ( cim )&lt;br /&gt;
|-&lt;br /&gt;
| 108||live||viver||||||||生活 ( sanghwat )&lt;br /&gt;
|-&lt;br /&gt;
| 109||die||morir||||||||死亡 ( siimang )&lt;br /&gt;
|-&lt;br /&gt;
| 110||kill||occidar||||||||殺 ( sat )&lt;br /&gt;
|-&lt;br /&gt;
| 111||fight||luctar||||||||戦闘 ( jendou )&lt;br /&gt;
|-&lt;br /&gt;
| 110||hunt||chassar||||||||猟 ( lop )&lt;br /&gt;
|-&lt;br /&gt;
| 113||hit (beat)||colpar||||||||打撃 ( dagek )&lt;br /&gt;
|-&lt;br /&gt;
| 114||cut||secar||||||||切 ( cet )&lt;br /&gt;
|-&lt;br /&gt;
| 115||split||finder||||||||分裂 ( bunlet )&lt;br /&gt;
|-&lt;br /&gt;
| 116||stab||dagar||||||||刺 ( cik )&lt;br /&gt;
|-&lt;br /&gt;
| 117||scratch||grattar||||||||掻 ( sau )&lt;br /&gt;
|-&lt;br /&gt;
| 118||dig||foder||||||||掘 ( gut )&lt;br /&gt;
|-&lt;br /&gt;
| 119||swim||natar||||||||泳 ( &#039;wing )&lt;br /&gt;
|-&lt;br /&gt;
| 120||fly||volar||||||||飛行 ( pihang )&lt;br /&gt;
|-&lt;br /&gt;
| 121 || walk || ambular || || || || {{Ruby|散歩|산보}}&lt;br /&gt;
|-&lt;br /&gt;
| 122||come||venir||||||||来 ( lai )&lt;br /&gt;
|-&lt;br /&gt;
| 123||lie||jacer||||||||臥 ( &#039;wa )&lt;br /&gt;
|-&lt;br /&gt;
| 124||sit||seder||||||||坐 ( jwa )&lt;br /&gt;
|-&lt;br /&gt;
| 125||stand||star||||||||立 ( lip )&lt;br /&gt;
|-&lt;br /&gt;
| 126||turn||tornar||||||||回転 ( hoijwen )&lt;br /&gt;
|-&lt;br /&gt;
| 127||fall||cader||||||||落下 ( lakha )&lt;br /&gt;
|-&lt;br /&gt;
| 128||give||dar||||||||送 ( song )&lt;br /&gt;
|-&lt;br /&gt;
| 129||hold||tener||||||||持 ( di )&lt;br /&gt;
|-&lt;br /&gt;
| 130||squeeze||premer||||||||捻 ( nep )&lt;br /&gt;
|-&lt;br /&gt;
| 131||rub||fricar||||||||擦 ( cat )&lt;br /&gt;
|-&lt;br /&gt;
| 132||wash||lavar||||||||洗 ( sen )&lt;br /&gt;
|-&lt;br /&gt;
| 133||wipe||essugar||||||||擦拭 ( catsik )&lt;br /&gt;
|-&lt;br /&gt;
| 134||pull||tirar||||||||引 ( &#039;in )&lt;br /&gt;
|-&lt;br /&gt;
| 135||push||pulsar||||||||推 ( cui )&lt;br /&gt;
|-&lt;br /&gt;
| 136||throw||jectar||||||||投 ( dou )&lt;br /&gt;
|-&lt;br /&gt;
| 137||tie||ligar||||||||結 ( get )&lt;br /&gt;
|-&lt;br /&gt;
| 138||sew||suer||||||||縫製 ( bongje )&lt;br /&gt;
|-&lt;br /&gt;
| 139||count||contar||||||||計数 ( geisu )&lt;br /&gt;
|-&lt;br /&gt;
| 140||say||dicer||||||||言 ( &#039;en )&lt;br /&gt;
|-&lt;br /&gt;
| 141||sing||cantar||||||||唱歌 ( cangga )&lt;br /&gt;
|-&lt;br /&gt;
| 142||play||jocar||||||||遊戯 ( &#039;yuuhui )&lt;br /&gt;
|-&lt;br /&gt;
| 143||float||flottar||||||||浮 ( buu )&lt;br /&gt;
|-&lt;br /&gt;
| 144||flow||fluer||||||||流動 ( lyudong )&lt;br /&gt;
|-&lt;br /&gt;
| 145||freeze||gelar||||||||凍結 ( dongget )&lt;br /&gt;
|-&lt;br /&gt;
| 146||swell||tumer||||||||膨脹 ( pangcang )&lt;br /&gt;
|-&lt;br /&gt;
| 147||sun||sol||||||||太陽 ( tai&#039;yang )&lt;br /&gt;
|-&lt;br /&gt;
| 148||moon||luna||||||||月 ( &#039;wet )&lt;br /&gt;
|-&lt;br /&gt;
| 149||star||stella||||||||星 ( seng )&lt;br /&gt;
|-&lt;br /&gt;
| 150||water||aqua||||||||水 ( su )&lt;br /&gt;
|-&lt;br /&gt;
| 151||rain||pluvia||||||||雨 ( &#039;u )&lt;br /&gt;
|-&lt;br /&gt;
| 152||river||fluvio||||||||川 ( cen )&lt;br /&gt;
|-&lt;br /&gt;
| 153||lake||laco||||||||湖 ( ho )&lt;br /&gt;
|-&lt;br /&gt;
| 154||sea||mar||||||||海洋 ( hai&#039;yang )&lt;br /&gt;
|-&lt;br /&gt;
| 155||salt||sal||||||||塩 ( &#039;yem )&lt;br /&gt;
|-&lt;br /&gt;
| 156||stone||petra||||||||石頭 ( sektou )&lt;br /&gt;
|-&lt;br /&gt;
| 157 || sand ||  sablo || || || || {{Ruby|沙|사}}&lt;br /&gt;
|-&lt;br /&gt;
| 158||dust||pulvere||||||||灰塵 ( hoijin )&lt;br /&gt;
|-&lt;br /&gt;
| 159||earth||terra||||||||土 ( to )&lt;br /&gt;
|-&lt;br /&gt;
| 160||cloud||nube||||||||雲 ( &#039;un )&lt;br /&gt;
|-&lt;br /&gt;
| 161||fog||nebula||||||||霧 ( mu )&lt;br /&gt;
|-&lt;br /&gt;
| 162||sky||celo||||||||天 ( ten )&lt;br /&gt;
|-&lt;br /&gt;
| 163||wind||vento||||||||風 ( pung )&lt;br /&gt;
|-&lt;br /&gt;
| 164||snow||nive||||||||雪 ( swet )&lt;br /&gt;
|-&lt;br /&gt;
| 165||ice||glacie||||||||氷水 ( bingsu )&lt;br /&gt;
|-&lt;br /&gt;
| 166||smoke||fumo||||||||煙 ( &#039;en )&lt;br /&gt;
|-&lt;br /&gt;
| 167||fire||foco||||||||火 ( hwa )&lt;br /&gt;
|-&lt;br /&gt;
| 168||ash||cineres||||||||灰 ( hoi )&lt;br /&gt;
|-&lt;br /&gt;
| 169||burn||arder||||||||燃焼 ( nensyou )&lt;br /&gt;
|-&lt;br /&gt;
| 170||road||strata||||||||道路 ( daulo )&lt;br /&gt;
|-&lt;br /&gt;
| 171||mountain||montania||||||||山 ( san )&lt;br /&gt;
|-&lt;br /&gt;
| 172||red||rubie||||||||紅 ( hong ) 赤 ( cek )&lt;br /&gt;
|-&lt;br /&gt;
| 173||green||verde||||||||緑 ( lok )&lt;br /&gt;
|-&lt;br /&gt;
| 174||yellow||jalne||||||||黄 ( hwang )&lt;br /&gt;
|-&lt;br /&gt;
| 175||white||blanc||||||||白 ( bak )&lt;br /&gt;
|-&lt;br /&gt;
| 176||black||nigre||||||||黒 ( huk )&lt;br /&gt;
|-&lt;br /&gt;
| 177||night||nocte||||||||夜 ( &#039;ya )&lt;br /&gt;
|-&lt;br /&gt;
| 178||day||die||||||||日 ( nit )&lt;br /&gt;
|-&lt;br /&gt;
| 179||year||anno||||||||年 ( nen )&lt;br /&gt;
|-&lt;br /&gt;
| 180||warm||calide||||||||暖 ( nan )&lt;br /&gt;
|-&lt;br /&gt;
| 181||cold||frigide||||||||冷 ( lang )&lt;br /&gt;
|-&lt;br /&gt;
| 182||full||plen||||||||満 ( man )&lt;br /&gt;
|-&lt;br /&gt;
| 183||new||nove||||||||新 ( sin )&lt;br /&gt;
|-&lt;br /&gt;
| 184||old||vetere||||||||老 ( lau )&lt;br /&gt;
|-&lt;br /&gt;
| 185||good||bon||||||||好 ( hau )&lt;br /&gt;
|-&lt;br /&gt;
| 186||bad||mal||||||||悪 ( &#039;ak )&lt;br /&gt;
|-&lt;br /&gt;
| 187||rotten||corrupte||||||||腐敗 ( pubai )&lt;br /&gt;
|-&lt;br /&gt;
| 188||dirty||immunde||||||||汚 ( &#039;o )&lt;br /&gt;
|-&lt;br /&gt;
| 189||straight||recte||||||||直 ( jik )&lt;br /&gt;
|-&lt;br /&gt;
| 190||round||ronde||||||||圓 ( &#039;wen )&lt;br /&gt;
|-&lt;br /&gt;
| 191||sharp||acute||||||||鋭利 ( &#039;yelii )&lt;br /&gt;
|-&lt;br /&gt;
| 192||dull||obtuse||||||||鈍 ( don )&lt;br /&gt;
|-&lt;br /&gt;
| 193||smooth||lisie||||||||滑 ( got )&lt;br /&gt;
|-&lt;br /&gt;
| 194||wet||humide||||||||湿 ( sip )&lt;br /&gt;
|-&lt;br /&gt;
| 195||dry||sic||||||||干燥 ( gansau )&lt;br /&gt;
|-&lt;br /&gt;
| 196||correct||correcte||||||||正 ( jing )&lt;br /&gt;
|-&lt;br /&gt;
| 197||near||proxime||||||||近 ( gin )&lt;br /&gt;
|-&lt;br /&gt;
| 198||far||distante||||||||遠 ( &#039;on )&lt;br /&gt;
|-&lt;br /&gt;
| 199||right||dextre||||||||右側 ( &#039;yujik )&lt;br /&gt;
|-&lt;br /&gt;
| 200||left||sinistre||||||||左側 ( jajik )&lt;br /&gt;
|-&lt;br /&gt;
| 201 || &#039;&#039;&#039;at&#039;&#039;&#039; || a || || || || {{Ruby|於|오}}&lt;br /&gt;
|-&lt;br /&gt;
| 202 || &#039;&#039;&#039;in&#039;&#039;&#039; || in || || || || {{Ruby|於|오}}&lt;br /&gt;
|-&lt;br /&gt;
| 203 || &#039;&#039;&#039;with&#039;&#039;&#039; || con || || || || 共 ( gyong )&lt;br /&gt;
|-&lt;br /&gt;
| 204 || &#039;&#039;&#039;and&#039;&#039;&#039; || e || || || || 与 ( &#039;yo ) , 而 ( ni )&lt;br /&gt;
|-&lt;br /&gt;
| 205 || &#039;&#039;&#039;if&#039;&#039;&#039; || si || || || || {{Ruby|若|냐}}&lt;br /&gt;
|-&lt;br /&gt;
| 206 || &#039;&#039;&#039;because&#039;&#039;&#039; || proque || || || || {{Ruby|因由|인윳}}&lt;br /&gt;
|-&lt;br /&gt;
| 207 || &#039;&#039;&#039;name&#039;&#039;&#039; || nomine || {{Dict|име || {{Rune|ᚾᚪᛗ}} || || {{Ruby|名|밍}}&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
[[Category:Swadesh]]&lt;br /&gt;
[[Category:Swadesh lists]]&lt;br /&gt;
[[Category:Universal Languages]]&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=Universal_Languages&amp;diff=176053</id>
		<title>Universal Languages</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=Universal_Languages&amp;diff=176053"/>
		<updated>2025-11-14T14:01:19Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* Conclusion */ swadesh&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Many people have proposed &amp;quot;one language to unite the world&amp;quot;.  Esperanto came close.  English is slowly stomping out many native tongues around the globe.  Is the solution to back off and return to insurmountable diversity?  &lt;br /&gt;
&lt;br /&gt;
There are lessons to be learned from Esperanto.  It had several things going for it.  It was no one nation&#039;s language.  It didn&#039;t belong to anybody but Esperantists.  Its artificial nature is easy to learn, but ultimately was its downfall: it is hard to regard it as a heart-language for anyone.  Its scope was also too broad.  French and Spanish and even English are able to be united, but the little sprinkles of German, Polish, and Russian are too few and too unusual to make anyone happy.  We can do better.&lt;br /&gt;
&lt;br /&gt;
In fact, several people have already begun to do better.  Interslavic has an ISO code.  Interlingua does too.  Folksprak is developing.  Guosa is growing.  Gaspirali&#039;s old project of Jalpi could be revived.  In short, targeted Universal Languages are burgeoning.  Rather than attempting to be one-world-language, or displace any native languages, these inventions are modest in design and practical in scope&lt;br /&gt;
&lt;br /&gt;
# &#039;&#039;&#039;&#039;&#039;Unify a people.&#039;&#039;&#039;&#039;&#039;  Every Universal Language unites a group of people, either because they are phylogenically related, or because a sprachbund binds their communities together.  Even if your goal is global oneness, it makes sense to start with region oneness.&lt;br /&gt;
# &#039;&#039;&#039;&#039;&#039;Facilitate learning.&#039;&#039;&#039;&#039;&#039; &amp;quot;Basic English&amp;quot;, &amp;quot;World English&amp;quot; and other pared-down languages are attempts to invite other in with less difficulty.  An artificial language can be much, much easier to learn than a natural language.  But like learning Latin before attempting Spanish, it lays the ground work for learning a used language.&lt;br /&gt;
# &#039;&#039;&#039;&#039;&#039;Clarify identity.&#039;&#039;&#039;&#039;&#039;  If our region has a clearer identity, and our identity is clear within &#039;&#039;that&#039;&#039;, how much more we positioned are we?  For example, do you really understand German unless you know where it fits within Germanic languages/people?&lt;br /&gt;
&lt;br /&gt;
To meet these goal, 15 languages need to be designed, flushed out and then taught.  Imagine if every English-speaker was bilingual!  Throughout nearly all of human history, people who learned to read and write did so in a language not their own.  Beyond normal, this was helpful.  After a generation or two of this, a unique writing system for each Universal Language could be rolled out.  Within a region, international and outward facing businesses and signage would be in the local Universal Language.  Verbal arts would only need to be translated 14 times to reach 99% of all people.  Anyone who travelled much would be fluent in several UL&#039;s.  Regionalism would return to the world, and the very meaning of Globalism would change.  The equal ultimacy of the One and Many would be heard and understood.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;&lt;br /&gt;
[[File:Universal Language.png|1000px]]&lt;br /&gt;
&amp;lt;/center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Dan&#039;a&#039;yo ==&lt;br /&gt;
The first and biggest UL is Dan&#039;a&#039;yo (単亜語/단아요).  Uniting the largest slice of humanity, this Far East Asian language is unusual in that the peoples represented do not speak related languages.  However, China-Japan-Korea-Vietname (CJKV) all have a shared history and cultural legacy that makes communication possible.  1.5 billion people speak Mandarin, Japanese, Korean, or an older form of Vietnamese.  This piece of the Sinosphere actually has &#039;&#039;Classical Chinese&#039;&#039; in common, even though some no longer write in Chinese characters at all.  Despite being the most successful ideographic language ever, Chinese does not even unite the region, but nearly so.  To that end, Dan&#039;a&#039;yo is written in &#039;&#039;both&#039;&#039; Chinese characters and the Korean alphabet.&lt;br /&gt;
&lt;br /&gt;
Some important features that unite the region linguistically are&lt;br /&gt;
* &#039;&#039;&#039;&#039;&#039;Topic-Comment structure.&#039;&#039;&#039;&#039;&#039; This is actually more important than the SVO or SOV word-orders of the various languages.&lt;br /&gt;
* &#039;&#039;&#039;&#039;&#039;Classifiers.&#039;&#039;&#039;&#039;&#039; Like an elaborate gender system, numbers can only go on a select few words.&lt;br /&gt;
* &#039;&#039;&#039;&#039;&#039;Phonology.&#039;&#039;&#039;&#039;&#039; Nearly all the region is united in following the aspirated-vs-unaspirated distinction in stops.&lt;br /&gt;
* &#039;&#039;&#039;&#039;&#039;Texts.&#039;&#039;&#039;&#039;&#039; Confucius, Lao-Tzu, Mencius, Zhuangzi and other important texts were the backbone of all these societies until very recently.&lt;br /&gt;
&lt;br /&gt;
== Neo-Sanskrit ==&lt;br /&gt;
Through around 500 A.D. the Indo-European arrives on the Indian Subcontinent spoke Sanskrit.  Most languages in the region passed through several Prakrits (intermediate stages), before devolving into Hindusatani, Punjabi, Kashmiri, Garwali, Rajasthani, Maithili, and many more.  The native Dravidian languages had a large impact on phonology, but remained separate in most ways.  Approximately 1.4 billion people are in this language group.  It will be written in Kaithi, and it used be to the most widely used script of North India west of Bengal.&lt;br /&gt;
&lt;br /&gt;
Some important features that unite the region linguistically are:&lt;br /&gt;
* &#039;&#039;&#039;&#039;&#039;Clipped Sanskrit.&#039;&#039;&#039;&#039;&#039; Most native words are shortened versions of the word in Sanskrit.&lt;br /&gt;
* &#039;&#039;&#039;&#039;&#039;Collapsing Phonology.&#039;&#039;&#039;&#039;&#039; While previously, four kinds of stops and five places of articulation for them (and nasals) was the rule, now different language have simplified this differently.&lt;br /&gt;
* &#039;&#039;&#039;&#039;&#039;Two genders.&#039;&#039;&#039;&#039;&#039; While very difficult to agree on what is which gender, all these languages have it, and even mark it on the verb at times.&lt;br /&gt;
* &#039;&#039;&#039;&#039;&#039;Postpositions.&#039;&#039;&#039;&#039;&#039; Even more important than case markers, free postpositions still dominate all these languages.&lt;br /&gt;
* &#039;&#039;&#039;&#039;&#039;Split Ergativity.&#039;&#039;&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Interlingua ==&lt;br /&gt;
This already extant project serves the Romance languages of the world: French, Spanish, Italian, Portuguese, and others.  Approximately 800 million people are in this zone.  While we might have preferred for it to have kept two genders (as all the source languages do), it is still an excellent compromise across the region and a great Universal Language.  Eventually, it will be the sole user of the Latin alphabet, and that without diacritics.  There are four simple verb tenses, and three more compound tenses.  It is SVO.&lt;br /&gt;
&lt;br /&gt;
== Folksprak ==&lt;br /&gt;
Folksprak is also an extant project, but it is apparently crippled by the same problem which merely plagues Interlingua: English.  English&#039;s status as the de facto lingua franca of the world imposes many constraints upon a Germanic language that prevent group unity and decision making.  De-platforming English means seeing it on equal footing with German, Dutch, Afrikaans, Swedish, Danish, Norwegian, and others.  By immigration, this region includes America, Canada, Australia, New Zealand, much of South Africa, Belize, Guyana, and Suriname.  This encompasses approximately 500 million people.  After the introductory phase, Folksprak will be written in modernized runes.&lt;br /&gt;
&lt;br /&gt;
A unique feature of Germanic language is that they are V2, which is subtly different from SVO.  Other features include&lt;br /&gt;
* Front rounded vowels&lt;br /&gt;
* Short and long vowels&lt;br /&gt;
* Heavy use of discourse particles&lt;br /&gt;
&lt;br /&gt;
== Kintu ==&lt;br /&gt;
While Swahili has, in many ways, united northeastern Africa, a true pan-Bantu language is yet needed.  Approximately 450 million people would be connected by this language, called Kintu.  This includes the languages of Swahili, Shona, Zulu, Xhosa, Kinyarwanda, Kirundi, Lingala, Gikuyu, Nyanja, Tshiluba, and many more.&lt;br /&gt;
&lt;br /&gt;
* Pre-nasalized stops&lt;br /&gt;
* Eight noun classes&lt;br /&gt;
* Seven vowels&lt;br /&gt;
* Five tenses and three aspects&lt;br /&gt;
* Agglutinative morphology&lt;br /&gt;
* Heavily prefixing&lt;br /&gt;
* Two tones (hence only one marked)&lt;br /&gt;
&lt;br /&gt;
We propose a new script, Ditema tsa Dinoko, which has yet to be adopted.&lt;br /&gt;
&lt;br /&gt;
== Indo-Malay ==&lt;br /&gt;
Maritime Southeast Asia is a unique region.  380 million people.&lt;br /&gt;
&lt;br /&gt;
* Clusivity&lt;br /&gt;
* Politeness marked on pronouns&lt;br /&gt;
* Reduplication&lt;br /&gt;
&lt;br /&gt;
== Guosa ==&lt;br /&gt;
Already extant project.  Eventually using the N&#039;Ko script, 340 million people in West Africa need a neutral means of communication.&lt;br /&gt;
&lt;br /&gt;
* Analytic typology: Guosa follows an isolating, word-order-dependent structure, avoiding excessive inflections.&lt;br /&gt;
* SVO word order: This is a good choice, as it aligns with many West African languages and English (which is widely spoken in Nigeria).&lt;br /&gt;
* No extensive verb conjugation: Instead of complex tense/aspect marking, Guosa relies on auxiliary particles.&lt;br /&gt;
&lt;br /&gt;
== Interslavic ==&lt;br /&gt;
Highly successful project.  Eventually Cyrillic.  300 million, excluding South Slavic.&lt;br /&gt;
&lt;br /&gt;
== Middle Semitic ==&lt;br /&gt;
Work has begun.  Written in Syriac from the start, which is already a middle ground between Hebrew and Arabic.  290 million people.&lt;br /&gt;
&lt;br /&gt;
* Triconsonantal roots&lt;br /&gt;
* Pronominal suffixes&lt;br /&gt;
* Construct state&lt;br /&gt;
&lt;br /&gt;
== M.S.E.A.L. ==&lt;br /&gt;
Definitely a sprachbund, but fantastically diverse.  Vietnamese, Thai, Cantonese, Khmer, Hmong, Bengali, etc.  250 million people.&lt;br /&gt;
&lt;br /&gt;
== Dravindian ==&lt;br /&gt;
230 million people&lt;br /&gt;
&lt;br /&gt;
== Zens ==&lt;br /&gt;
Iranian languages.  175 million.  Written mostly in Arabic letters today, the future will see a return to the Avestan Alphabet.&lt;br /&gt;
&lt;br /&gt;
* Tripartite.  As a compromise position between the Nominative-Accusative and Split-Ergative languages.&lt;br /&gt;
&lt;br /&gt;
== Jalpi ==&lt;br /&gt;
Gaspirali invented a pan-Turkic language 200 year ago.  With minor updates, it could serve well the 170 million people in this language family.  Eventually, it will be written in the Armenian script.&lt;br /&gt;
&lt;br /&gt;
* Vowel harmony&lt;br /&gt;
* Agglutinative Structure – Jalpi preserved the fundamental agglutinative nature of Turkic languages, keeping it intuitive for Turkic speakers.&lt;br /&gt;
* Regularized Morphology – It avoided irregularities found in some Turkic languages (especially Ottoman Turkish’s Arabic/Persian borrowings).&lt;br /&gt;
* Consistent SOV Word Order – This ensured familiarity across Turkic languages.&lt;br /&gt;
&lt;br /&gt;
== S.E.D.E.S. ==&lt;br /&gt;
The Horn of Africa has long been a sprachbund.  117 million people.  Written in Ge&#039;ez for now, eventually the script invented by Bakri Sapalo will be used.&lt;br /&gt;
&lt;br /&gt;
* Ejectives: pʼ, tʼ, kʼ, sʼ&lt;br /&gt;
* Long vs Short vowels&lt;br /&gt;
* Gemination&lt;br /&gt;
* SOV&lt;br /&gt;
* head-final&lt;br /&gt;
* suffixing cases, include definiteness and focus&lt;br /&gt;
* serial verbs&lt;br /&gt;
&lt;br /&gt;
== Balkan ==&lt;br /&gt;
A small, diverse sprachbund exists in the Balkans.  60 million people.  Written in the Greek alphabet.&lt;br /&gt;
&lt;br /&gt;
* Unstressed vowel reduction&lt;br /&gt;
* fricatives!&lt;br /&gt;
* no case&lt;br /&gt;
* postposed definite article&lt;br /&gt;
* no synthetic future&lt;br /&gt;
* subordinate clause form instead of infinitive&lt;br /&gt;
* periphrastic comparatives&lt;br /&gt;
* Dative Clitic Doubling&lt;br /&gt;
&lt;br /&gt;
== Conclusion ==&lt;br /&gt;
Finno-Ugric, Mongolian, Celtic, Amerindian, Australian aborigines, the Caucasus, the Khoisan, two Baltic states, and many other regions are left out of this schema.  They can certainly choose to be part of an UL group, but the ROI on a language area of under 50 million people is simply not worth the effort.  Sorry!&lt;br /&gt;
&lt;br /&gt;
: [[Universal Languages/Swadesh]]&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable sortable&amp;quot;&lt;br /&gt;
! Latin Name !! Sample !! Population !! Big Map !! Little Map !!  Foundation !! Populous Languages&lt;br /&gt;
|-&lt;br /&gt;
| Dan&#039;a&#039;yo || 単亜語/단아요 || 1.5 billion || [[File:Far East Asia.png|200px]] || [[File:East_Asian_Cultural_Sphere.png|100px]] ||  Classical Chinese || Mandarin, Japanese, Korean, some Vietnamese&lt;br /&gt;
|-&lt;br /&gt;
| Neo-Sanskrit || 𑂍𑂨𑂟𑂲 || 1.4 billion || [[File:Indo-Aryan world.png|200px]] || [[File:Neo Sanskrit.png|120px]] || Sanskrit || Hindusatani, Punjabi, Gujarati, Bhojpuri, Marathi, etc.&lt;br /&gt;
|-&lt;br /&gt;
| Interlingua || patre nostre || 800 million || [[File:Detailed SVG map of the Romance-speaking world.png|200px]] || [[File:Romance_languages.png|120px]] ||  Proto-Romance || Spanish, French, Italian, Portuguese, Catalan, etc.&lt;br /&gt;
|-&lt;br /&gt;
| Folksprak || ᚠᚩᛚᛣᛋᛈᚱᚪᛣ || 500 million || [[File:Germanic languages.png|200px]] || [[File:Germanic_languages_with_dialects_revised.png|120px]]||  Proto-Germanic || English, German, Dutch, Afrikaans, Swedish, etc.&lt;br /&gt;
|-&lt;br /&gt;
| Kintu || [[File:Ditema_Tsa_Dinoko_Syllabary_Sample.svg|95px]] || 450 million || [[File:Big Bantu map.png|180px]] || [[File:Map_of_the_Bantu_languages.png|120px]] || Proto-Bantu || Swahili, Shona, Zulu, Xhosa, Kinyarwanda, Kirundi, etc.&lt;br /&gt;
|-&lt;br /&gt;
| Indo-Malay || ᨒᨚᨈᨑ || 380 million || [[File:IM world.png|200px]] || [[File:WGSRPD_Malesia.png|120px]]|| Proto-Malayo-Polynesian || Malay, Indonesian, Filipino, Javanese, etc.&lt;br /&gt;
|-&lt;br /&gt;
| Guosa || ߒߞߏ || 340 million || [[File:Guosa.png|200px]] || [[File:Carta_linguistica_dell&#039;Africa_Occidentale.png|120px]] || Proto-Niger-Congo || Hausa, Mande, Yoruba, Igbo, etc.&lt;br /&gt;
|-&lt;br /&gt;
| Interslavic || Меджусловјанскы || 300 million || [[File:Slavic world.png|200px]] || [[File: Slavic europe (Kosovo unshaded).png|120px]] || Proto-Slavic || Russia, Polish, Czech, Slovak, etc.&lt;br /&gt;
|-&lt;br /&gt;
| Middle Semitic || ܫܡܥ ܡܪܟܙ || 290 million || [[File:Semitic world.png|200px]] || [[File:Semitic_map.png|120px]] || Proto-Semitic || Arabic, Hebrew, Aramaic, Syriac, etc.&lt;br /&gt;
|-&lt;br /&gt;
| MSEAL || ဧသဃ || 233 million || [[File:MSEAL world.png|200px]] || [[File:Ethnolinguistic Groups of Mainland Southeast Asia.png|60px]] || Sprachbund || Vietnamese, Thai, Khmer, Bengali, etc.&lt;br /&gt;
|-&lt;br /&gt;
| Dravindian || 𑀩𑁆𑀭𑀸𑀳𑁆𑀫𑀻 || 230 million || [[File:World Dravidian.png|200px]] || [[File:Dravidian subgroups.png|120px]] || Proto-Dravidian || Telugu, Tamil, Kannada, Malayalam, etc.&lt;br /&gt;
|-&lt;br /&gt;
| Zens || 𐬰𐬈𐬥𐬯|| 200 million || [[File:Zens world.png|200px]] || [[File:The Sasanian Empire at its apex under Khosrow II.png|120px]] || Proto-Iranian || Persian, Pashto, Kurdish, Balochi, etc.&lt;br /&gt;
|-&lt;br /&gt;
| Jalpi || Ջալպի || 170 million || [[File:Map-TurkicLanguages.png|200px]] || [[File:Turkic_Languages_distribution_map.png|120px]] || Proto-Turkish || Turkish, Armenian, Turkmen, Kazakh, etc.&lt;br /&gt;
|-&lt;br /&gt;
| SEDES  || ሴዴስ || 117 million || [[File:Horn world.png|200px]] || [[File:main-qimg-f956903f62e1ab12e9c06e400c4c1f0a.png|90px]] || Horn of Africa sprachbund || Tigre, Tigrinya, Somali, etc.&lt;br /&gt;
|-&lt;br /&gt;
| Balkan || Βαλκαν || 60 million || [[File:Balkan world.png|200px]] || [[File:Languages_of_the_Balkan_Sprachbund_in_the_Balkans,_Cyprus_and_Italy.png|120px]] || Balkan sprachbund || Greek, Ottoman Turkish, Albanian, Serbian, etc.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
== WALS Chart ==&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!&lt;br /&gt;
! colspan=&amp;quot;5&amp;quot; | Europe&lt;br /&gt;
! colspan=&amp;quot;2&amp;quot; | India&lt;br /&gt;
! colspan=&amp;quot;3&amp;quot; | East Asia&lt;br /&gt;
! colspan=&amp;quot;4&amp;quot; | Africa&lt;br /&gt;
! colspan=&amp;quot;3&amp;quot; | Central Asia&lt;br /&gt;
|-&lt;br /&gt;
! !! {{Rune|[[Folksprak|ᚠᛋ]]}} !! [[Interlingua|IL]] !! [[Interslavic|слов]] !! [[Balkan|	Βαλκ]] !! [[Samboka|Sam]] !! [[Dravindian|Drav]] !! [[Neo-Sanskrit|NSS]] !! [[Dan&#039;a&#039;yo|単]] !! [[Indo-Malay|IM]] !! &amp;lt;small&amp;gt;[[MSEAL]]&amp;lt;/small&amp;gt; !! [[Guosa|Guo]] !! [[Kintu|Kintu]] !! &amp;lt;small&amp;gt;[[SEDES]]&amp;lt;/small&amp;gt; !! [[Middle Semitic|MS]] !! [[Zens]] !! [[Jalpi]] !! [[Caucas|კავ]]&lt;br /&gt;
|-&lt;br /&gt;
! Script&lt;br /&gt;
| &amp;lt;abbr title=&amp;quot;Runes&amp;quot;&amp;gt;ᚱᚢᚾᛖ&amp;lt;/abbr&amp;gt; || Latin || &amp;lt;abbr title=&amp;quot;Cyrillic&amp;quot;&amp;gt;Кирил&amp;lt;/abbr&amp;gt; || &amp;lt;abbr title=&amp;quot;Greek&amp;quot;&amp;gt;Ελλην&amp;lt;/abbr&amp;gt; || 𐲥𐳀𐳘𐳂𐳛𐳔&lt;br /&gt;
| &amp;lt;abbr title=&amp;quot;Brāhmi&amp;quot;&amp;gt;𑀩𑁆𑀭𑀸𑀳𑁆𑀫𑀻&amp;lt;/abbr&amp;gt; || &amp;lt;abbr title=&amp;quot;Kaithi&amp;quot;&amp;gt;𑂍𑂶𑂟𑂲&amp;lt;/abbr&amp;gt; || &amp;lt;abbr title=&amp;quot;Shinjitai/Hangǔl&amp;quot;&amp;gt;{{Ruby|新字体|신지테}}&amp;lt;/abbr&amp;gt; || &amp;lt;abbr title=&amp;quot;Lontara&amp;quot;&amp;gt;ᨒᨚᨈ&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| Burm || &amp;lt;abbr title=&amp;quot;N&#039;Ko&amp;quot;&amp;gt;ߒߞߏ&amp;lt;/abbr&amp;gt; || [[File:Ditema.svg|35px|Ditema]] || ግዕዝ || ܣܘܪܝܝ&lt;br /&gt;
| 𐬰𐬈𐬥𐬯 &lt;br /&gt;
| 𐰪𐰀𐰞𐰯𐰃&lt;br /&gt;
| 𐕒𐕡𐔳𐔼𐕎&lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Arm vs Hand, # of words WALS 129A&amp;quot;&amp;gt;arm&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| {{Yes|2}} || {{Yes|2}} || {{No|1}} || {{Yes|2}} ||  {{Yes|2}} || {{Yes|2}} || {{Yes|2}} || {{No|1}} || {{Yes|2}} || {{Yes|2}} || || {{No|1}} || {{Yes|2}} || {{Yes|2}} || {{No|1}} || {{Yes|2}} ||&lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Word Order (predominant) WALS 81A&amp;quot;&amp;gt;WO&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| {{Some|V2}} || {{Yes|SVO}} || {{Yes|SVO}} || {{Yes|SVO}} || || {{No|SOV}} || {{No|SOV}} || {{No|SOV}} || {{Yes|SVO}} || {{Some|VSO}} || {{Some|VSO}} || || {{Yes|SVO}} || {{Yes|SVO}} || {{No|SOV}} || {{No|SOV}} || {{No|SOV}}&lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Evidentiality (marked on verb) WALS 7&amp;quot;&amp;gt;Evid.&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| {{No}} || {{No}} || {{No}} || {{No}} || {{Yes}} || {{No}} || {{No}} || {{No}} || {{No}} || {{No}} || {{No}} || {{No}} || {{No}} || {{No}} || {{Yes}} || {{No}} || {{No}}&lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Number of grammatical cases&amp;quot;&amp;gt;Cases&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| {{Some|pro}} || {{Some|pro}} || {{Yes|6}} || {{Yes|4}} || {{Yes|16}} || {{Yes|8}} || {{Yes|4}} || {{No|0}} || {{No|0}} || {{No|0}} || {{No|0}} || {{No|0}} || {{Yes|2}} || {{No}} || {{Yes|2}} || {{Yes|7}} ||&lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Relative clause word order - post, ante, correlative&amp;quot;&amp;gt;RC&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| {{Yes|p}} || {{Yes|p}} || {{Yes|p}} || {{Yes|p}} || {{No|a}} || {{No|p}} || {{Some|c}} || {{No|a}} || {{Yes|p}} || {{Yes|p}} || {{Yes|p}} || {{Yes|p}} || {{Yes|p}} || {{Yes|p}} || {{Yes|p}} || {{No|a}} || {{No|a}} &lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Gender, number of&amp;quot;&amp;gt;Gend.&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| {{No|0}} || {{Yes|2}} || {{Yes|3}} || {{Yes|3}}  || {{No|0}} || {{Yes|3}} || {{Yes|2}} || {{No|0}} || || {{No|0}} || || {{Some|10}} || {{Yes|2}} || {{Yes|2}} || {{No|0}} || {{No|0}} || {{No|0}}&lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Tone or Pitch Accent&amp;quot;&amp;gt;TPA&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| {{No}} || {{No}} || {{No}} || {{No}} || {{No}} || {{No}} || {{No}} || {{Some|PA}} || {{No}} || {{Yes}} || {{Yes}} || {{Yes}} || {{No}} || {{No}} || {{No}} || {{No}} || &lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Definite Article WALS 37&amp;quot;&amp;gt;DA&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| {{Yes}} || {{Yes}} || {{No}} || {{No}} || {{Yes}} || {{No}} || {{No}} || {{No}} || || {{No}} || || {{Yes}} || {{Yes}} || {{Yes}} || {{No}} || {{Yes}} || &lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Indefinite Article WALS 38&amp;quot;&amp;gt;IA&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| {{Some}} || {{Some}} || {{No}} || {{Some}} || {{No}} || {{No}} || {{No}} || {{Some}} || {{Some}} || {{Some}} || || {{No}} || {{No}} || {{Some}} || {{Some}} || {{Some}} || &lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Clusivity&amp;quot;&amp;gt;Clus&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| {{No}} || {{No}} || {{No}} || {{No}} || {{No}}  || {{Yes}} || {{No}} || {{No}} || {{Yes}} || {{No}} || {{No}} || {{No}} || {{No}} || {{No}} || {{No}} || {{No}} || {{No}}&lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Typological grouping - Isolating, Fusional, Agglutinating&amp;quot;&amp;gt;Typol&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| {{No|F}} || {{No|F}} || {{No|F}} || {{No|F}} || {{Some|A}} || {{No|F}} || {{Some|A}} || {{Yes|I}} || {{Some|A}} || {{Yes|I}} || || {{Some|A}} || {{No|F}} || {{No|F}} || {{Some|A}} || {{Some|A}} || {{Some|A}}&lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Perfective/Imperfective mod is a verbal affix/conjugation&amp;quot;&amp;gt;Perf.&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| || {{Some}} || {{Yes}} || {{Yes}} || {{No}} || {{Yes}} || {{Yes}} || {{Some}} || {{No}} || {{No}} || {{No}} || {{No}} || {{No}} || {{No}} ||{{Yes}} || {{No}} || {{Some}}&lt;br /&gt;
|- &lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Reduplication (full or partial) is a productive part of the grammar WALS 27&amp;quot;&amp;gt;Redup.&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| {{No}} || {{No}} || {{No}} || {{No}} ||  {{No}} || {{Yes}} || {{Yes}} || {{Yes}} || {{Yes}} || {{Yes}} || {{Yes}} || {{Yes}} || {{Yes}} || {{No}} || {{Yes}} || {{No}} ||&lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Vowels, number of, counting nasal, length, etc.&amp;quot;&amp;gt;Vowels&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| {{Some|7}} || {{Yes|5}} || {{No|6}} || {{Yes|5}}  || {{No|6}} || {{Yes|5}} || {{Some|8}} || {{Yes|5}} || {{No|6}} || {{No|6}} || {{Some|7}} || {{Yes|5}} || {{Yes|5}} || {{Yes|5}} || {{No|6}} || {{Some|8}} || {{No|6}}&lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Gemination of consonants, beyond marginally&amp;quot;&amp;gt;Gemin.&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| {{No}} || {{No}} || {{Yes}} || {{No}} || {{Yes}} || {{Yes}} || {{No}} || {{No}} || {{No}} || {{No}} || {{No}} || {{No}} || {{Yes}} || {{Yes}} || {{No}} || {{No}} || {{Yes}}&lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Stress for the clause/utterance is defined by Left/Right edge.  No means weight-based&amp;quot;&amp;gt;Stress&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| || {{Yes|R}} || {{No}} || {{No}} || {{Some|L}} || {{Yes|R}} || {{No}} || {{Yes|R}} || {{Yes|R}} || {{No}} || {{No}} || {{No}} || {{No}} || {{Yes|R}} || {{Yes|R}} || {{No}} || {{No}}&lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Morphosyntactic Alignment&amp;quot;&amp;gt;MSA&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| {{Yes|NA}} || {{Yes|NA}} || {{Yes|NA}} || {{Yes|NA}} || {{Yes|NA}} || {{Yes|NA}} || {{Some|Spl}} || {{Yes|NA}} || {{Yes|NA}} || {{Yes|NA}} || {{Yes|NA}} || {{Yes|NA}} || {{Yes|NA}} || {{Yes|NA}} || {{Some|Tri}} || {{Yes|NA}} || {{No|Erg}}&lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Tu-Vous Distinction or more politeness&amp;quot;&amp;gt;TuVous&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| || {{Yes}} || {{Yes}} || {{Yes}} || {{Yes}} || {{Some|++}} || {{Some|++}} || {{Yes|**}} || {{Some|++}} || {{Yes|**}} || || {{No}} || {{No}} || {{Yes}} || {{Yes}} || {{Yes}} || {{Yes}}&lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Possessive Affixes attach to nouns&amp;quot;&amp;gt;Possess&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| {{No}} || {{No}} || {{No}} || {{No}} || {{Yes}} || {{No}} || {{No}} || {{No}} || {{Yes}} || {{No}} || || {{No}} || {{Yes}} || {{Yes}} || {{Yes}} || {{Yes}} || {{No}}&lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Polar Question Particle - no means verb form&amp;quot;&amp;gt;Polar&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| {{Yes}} || {{Yes}} || {{Yes}} || {{Yes}} || {{No}} || {{No}} || {{Yes}} || {{No}} || {{Yes}} || {{Yes}} || {{Yes}} || {{Yes}} || {{Yes}} || {{Yes}} || {{Yes}} || {{No}} || {{No}}&lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Future is a verbal affix&amp;quot;&amp;gt;Future&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| {{No}} || {{Yes}} || {{No}} || {{No}} || {{No}} || {{Yes}} || {{Yes}} || {{No}} || {{No}} || {{No}} || {{Yes}} || {{Yes}} || {{Yes}} || {{No}} || {{No}} || {{Some|++}} || {{Yes}}&lt;br /&gt;
|-&lt;br /&gt;
! &amp;lt;abbr title=&amp;quot;Negation Particle - VA is for verbal affix; auxiliary verb&amp;quot;&amp;gt;Negat&amp;lt;/abbr&amp;gt;&lt;br /&gt;
| {{Yes}} || {{Yes}} || {{Yes}} || {{Yes}} || {{Some|aux}} || {{No|VA}} || {{Yes}} || {{Yes}} || {{Yes}} || {{Yes}} || || {{No|VA}} || {{Yes}} || {{Yes}} || {{No|VA}} || {{No|VA}} || {{Yes}}&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== The Case for Universal Languages (ULs) ===&lt;br /&gt;
&#039;&#039;A smarter way to communicate, a fairer way to connect.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
==== What Are Universal Languages? ====&lt;br /&gt;
Universal Languages (ULs) are &#039;&#039;&#039;regional auxiliary languages&#039;&#039;&#039;designed to make communication &#039;&#039;&#039;easier, fairer, and more natural&#039;&#039;&#039; for people within the same linguistic and cultural sphere. Each UL is a carefully &#039;&#039;&#039;constructed bridge language&#039;&#039;&#039;, drawing from the &#039;&#039;&#039;shared linguistic history&#039;&#039;&#039; of a region while remaining neutral—so no single ethnic or national group dominates.&lt;br /&gt;
&lt;br /&gt;
ULs are &#039;&#039;&#039;not meant to replace&#039;&#039;&#039; indigenous languages. Instead, they act as a &#039;&#039;&#039;linguistic roundtable&#039;&#039;&#039;—a common space where people from different backgrounds can meet on &#039;&#039;&#039;equal footing&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
==== Why Do We Need Universal Languages? ====&lt;br /&gt;
; Breaks Down Barriers : ULs allow people to communicate across their region &#039;&#039;&#039;without relying on colonial or global superpowers&#039;&#039;&#039; (e.g., English, Mandarin, French).&lt;br /&gt;
; Easy to Learn, Yet Natural : Unlike overly artificial languages (Esperanto, Toki Pona), ULs feel &#039;&#039;&#039;familiar to their speakers&#039;&#039;&#039; while still being simplified for usability.&lt;br /&gt;
; Designed for Practicality : Each UL has a unique writing system, preventing confusion, and adapts to modern needs &#039;&#039;&#039;without constant reform&#039;&#039;&#039;.&lt;br /&gt;
; Fosters Regional Unity, Not Domination : ULs unite people &#039;&#039;&#039;without erasing their native tongues&#039;&#039;&#039;. No one’s culture is sidelined, and no major language unfairly takes over.&lt;br /&gt;
; A Hallway, Not a Home : ULs &#039;&#039;&#039;aren’t anyone’s native language&#039;&#039;&#039;—they’re a &#039;&#039;&#039;shared space&#039;&#039;&#039; for communication. You keep your mother tongue, but gain a doorway to understanding your neighbors.&lt;br /&gt;
&lt;br /&gt;
==== How Would They Be Implemented? ====&lt;br /&gt;
# 15 Universal Languages are assigned based on linguistic geography—not politics.&lt;br /&gt;
# Each UL is regionally intuitive, globally exotic—easy for locals, but distinct from outsiders.&lt;br /&gt;
# Gradual Adoption – Local populations can write the UL however they like at first, but within a century, each UL has its own unique script for clarity in business and diplomacy.&lt;br /&gt;
# Regulated Yet Flexible – ULs evolve over time, but slowly, ensuring stability.&lt;br /&gt;
&lt;br /&gt;
==== The End Goal ====&lt;br /&gt;
Dethrone &#039;&#039;&#039;linguistic imperialism&#039;&#039;&#039;—no more English, Mandarin, or French as default global languages. Instead, let every region have its own voice.&lt;br /&gt;
&lt;br /&gt;
Imagine a world where:&lt;br /&gt;
&lt;br /&gt;
* Bantu speakers communicate effortlessly without colonial leftovers.&lt;br /&gt;
* East Asians use a single, shared UL without relying on Mandarin.&lt;br /&gt;
* Europeans no longer default to English, but to Interlingua or Folksprak.&lt;br /&gt;
A world where understanding your neighbor’s culture is easy, and learning foreign languages is natural.&lt;br /&gt;
&lt;br /&gt;
Universal Languages aren’t just about words—they’re about fairness, identity, and human connection.&lt;br /&gt;
&lt;br /&gt;
Are you ready to build a world where no language rules over another? Then it’s time for Universal Languages.&lt;br /&gt;
&lt;br /&gt;
{{Universal Language}}&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=User:Aquatiki/Sandbox2&amp;diff=175309</id>
		<title>User:Aquatiki/Sandbox2</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=User:Aquatiki/Sandbox2&amp;diff=175309"/>
		<updated>2025-10-06T22:11:28Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* PIE (-4500) */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;__TOC__&lt;br /&gt;
&amp;lt;div style=&amp;quot;width:100%; background:#ddd;&amp;quot;&amp;gt;&lt;br /&gt;
&amp;lt;center&amp;gt;&lt;br /&gt;
==PIE (-4500)==&lt;br /&gt;
&lt;br /&gt;
Cowgill&#039;s Law&lt;br /&gt;
&lt;br /&gt;
Osthoff&#039;s Law&lt;br /&gt;
&lt;br /&gt;
Sievers&#039;s law&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/center&amp;gt;&lt;br /&gt;
&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;table&amp;gt;&lt;br /&gt;
&amp;lt;tr&amp;gt;&lt;br /&gt;
&amp;lt;td&amp;gt;&lt;br /&gt;
&amp;lt;h3&amp;gt;Proto-Germanic (-500)&amp;lt;/h3&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* Grimm&#039;s Law, Verner&#039;s Law, Primärberührung&lt;br /&gt;
&lt;br /&gt;
{|class=&amp;quot;wikitable&amp;quot; style=text-align:center&lt;br /&gt;
|- style=&amp;quot;font-size: 90%;&amp;quot;&lt;br /&gt;
|+ Proto-Germanic consonants&lt;br /&gt;
!Type&lt;br /&gt;
! colspan=&amp;quot;2&amp;quot; style=&amp;quot;width:20px;&amp;quot;| Bilabial&lt;br /&gt;
! colspan=&amp;quot;2&amp;quot; style=&amp;quot;width:20px;&amp;quot;| Dental&lt;br /&gt;
! colspan=&amp;quot;2&amp;quot; style=&amp;quot;width:20px;&amp;quot;| Alveolar&lt;br /&gt;
! colspan=&amp;quot;2&amp;quot; style=&amp;quot;width:20px;&amp;quot;| Palatal&lt;br /&gt;
! colspan=&amp;quot;2&amp;quot; style=&amp;quot;width:20px;&amp;quot;| Velar&lt;br /&gt;
! colspan=&amp;quot;2&amp;quot; style=&amp;quot;width:20px;&amp;quot;| Labial–&amp;lt;br&amp;gt;velar&lt;br /&gt;
|-&lt;br /&gt;
! Nasal&lt;br /&gt;
|  style=&amp;quot;width:20px; border-right:0;&amp;quot;| ||  style=&amp;quot;width:20px; border-left:0;&amp;quot;|{{IPA|m}}&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|  style=&amp;quot;width:20px; border-right:0;&amp;quot;| ||  style=&amp;quot;width:20px; border-left:0;&amp;quot;|{{IPA|n}}&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|  style=&amp;quot;width:20px; border-right:0;&amp;quot;| ||  style=&amp;quot;width:20px; border-left:0;&amp;quot;|({{IPA|ŋ}})&lt;br /&gt;
|  style=&amp;quot;width:20px; border-right:0;&amp;quot;| ||  style=&amp;quot;width:20px; border-left:0;&amp;quot;|({{IPA|ŋʷ}})&lt;br /&gt;
|-&lt;br /&gt;
! [[Stop consonant|Stop]]&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|p}}||style=&amp;quot;border-left: 0;&amp;quot;|{{IPA|b}}&lt;br /&gt;
|  style=&amp;quot;width:20px; border-right:0;&amp;quot;|{{IPA|t}}||  style=&amp;quot;width:20px; border-left:0;&amp;quot;|{{IPA|d}}&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|k}}||style=&amp;quot;border-left: 0;&amp;quot;|{{IPA|ɡ}}&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|kʷ}}||style=&amp;quot;border-left: 0;&amp;quot;|{{IPA|ɡʷ}}&lt;br /&gt;
|-&lt;br /&gt;
! [[Fricative consonant|Fricative]]&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|ɸ}}||style=&amp;quot;border-left: 0;&amp;quot;|({{IPA|β}})&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|θ}}||style=&amp;quot;border-left: 0;&amp;quot;|({{IPA|ð}})&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|s}}||style=&amp;quot;border-left: 0;&amp;quot;|{{IPA|z}}&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|x}}||style=&amp;quot;border-left: 0;&amp;quot;|({{IPA|ɣ}})&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|xʷ}}||style=&amp;quot;border-left: 0;&amp;quot;|&lt;br /&gt;
|-&lt;br /&gt;
! [[Approximant consonant|Approximant]]&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|colspan=2| {{{IPA|l}}}&lt;br /&gt;
|  style=&amp;quot;width:20px; border-right:0;&amp;quot;| ||  style=&amp;quot;width:20px; border-left:0;&amp;quot;|{{IPA|j}}&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;| ||style=&amp;quot;border-left: 0;&amp;quot;|{{IPA|w}}&lt;br /&gt;
|-&lt;br /&gt;
! [[Trill consonant|Trill]]&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;| ||style=&amp;quot;border-left: 0;&amp;quot;|{{IPA|r}}&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Vowels&lt;br /&gt;
* i iː ĩ ĩː&lt;br /&gt;
* e eː&lt;br /&gt;
* ɛː ɛːː&lt;br /&gt;
* ɑ ɑː ɑ̃ ɑ̃ː&lt;br /&gt;
* ɔː ɔːː ɔ̃ː ɔ̃ːː&lt;br /&gt;
* u uː ũ ũː&lt;br /&gt;
Diphthongs&lt;br /&gt;
* Short: /ɑu/, /ɑi/, /eu/, /iu/ (from i-umlaut of /eu/) before /i/ or /j/&lt;br /&gt;
* Long: /ɔːu/, /ɔːi/, (possibly /ɛːu/, /ɛːi/)&lt;br /&gt;
:  ô (aka ɔːː) became -a in ON and OE, but -oin OHG&lt;br /&gt;
: -ǭ became -a in OHG but -e in OE&lt;br /&gt;
: -ōn became -ōn in OHG but -an in OE&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;td&amp;gt;&lt;br /&gt;
&amp;lt;h3&amp;gt;Proto-Celtic (-800)&amp;lt;/h3&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Proto-Celtic consonants&lt;br /&gt;
|-&lt;br /&gt;
! Type&lt;br /&gt;
! colspan=2|&amp;amp;nbsp;[[Bilabial consonant|Bilabial]]&amp;amp;nbsp;&lt;br /&gt;
! colspan=2|&amp;amp;nbsp;[[Alveolar consonant|Alveolar]]&amp;amp;nbsp;&lt;br /&gt;
! colspan=2|&amp;amp;nbsp;[[Palatal consonant|Palatal]]&amp;amp;nbsp;&lt;br /&gt;
! colspan=2|&amp;amp;nbsp;[[Velar consonant|Velar]]&amp;amp;nbsp;&lt;br /&gt;
! colspan=2| Labial–&amp;lt;br&amp;gt;velar&lt;br /&gt;
|- style=&amp;quot;text-align:center;&amp;quot;&lt;br /&gt;
! [[Nasal stop|Nasal]]&lt;br /&gt;
| colspan=2|{{IPA|m}}&lt;br /&gt;
| colspan=2|{{IPA|n}}&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2|({{IPA|ŋ}})&lt;br /&gt;
| colspan=2|({{IPA|ŋʷ}})&lt;br /&gt;
|- style=&amp;quot;text-align:center;&amp;quot;&lt;br /&gt;
! [[Plosive consonant|Plosive]]&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|b}}&lt;br /&gt;
| {{IPA|t}}&lt;br /&gt;
| {{IPA|d}}&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| {{IPA|k}}&lt;br /&gt;
| {{IPA|ɡ}}&lt;br /&gt;
| {{IPA|kʷ}}&lt;br /&gt;
| {{IPA|ɡʷ}}&lt;br /&gt;
|- style=&amp;quot;text-align:center;&amp;quot;&lt;br /&gt;
! [[Fricative consonant|Fricative]]&lt;br /&gt;
| {{IPA|ɸ}}&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|s}}&lt;br /&gt;
|&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2| x&lt;br /&gt;
| colspan=2|&lt;br /&gt;
|- style=&amp;quot;text-align:center;&amp;quot;&lt;br /&gt;
! [[Approximant consonant|Approximant]]&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2| {{IPA|l}}&lt;br /&gt;
| colspan=2|{{IPA|j}}&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2| {{IPA|w}}&lt;br /&gt;
|- style=&amp;quot;text-align:center;&amp;quot;&lt;br /&gt;
! [[Trill consonant|Trill]]&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2| {{IPA|r}}&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2|&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* then kʷ/p/_   (P-Celtic)&lt;br /&gt;
&lt;br /&gt;
Vowels&lt;br /&gt;
* i iː&lt;br /&gt;
* e&lt;br /&gt;
* a aː&lt;br /&gt;
* o oː&lt;br /&gt;
* u uː&lt;br /&gt;
and au, ai, ou, oi&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;/tr&amp;gt;&lt;br /&gt;
&amp;lt;/table&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;table style=&amp;quot;width:100%; background:#ddd;&amp;quot;&amp;gt;&lt;br /&gt;
&amp;lt;tr&amp;gt;&lt;br /&gt;
&amp;lt;td colspan=2&amp;gt;&lt;br /&gt;
&amp;lt;center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Through Roman Times ==&lt;br /&gt;
&amp;lt;/center&amp;gt;&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;/tr&amp;gt;&lt;br /&gt;
&amp;lt;tr&amp;gt;&lt;br /&gt;
&amp;lt;td&amp;gt;&lt;br /&gt;
=== Western Germanic ===&lt;br /&gt;
Ingvaeonic and Irminonic&lt;br /&gt;
&lt;br /&gt;
* /ɛː/, also written ǣ,  to ā&lt;br /&gt;
* umlaut&lt;br /&gt;
* z/r/V_V&lt;br /&gt;
* demonstrative &#039;&#039;this&#039;&#039;&lt;br /&gt;
* C/C²/_j   West Germanic gemination&lt;br /&gt;
&lt;br /&gt;
Decision Time!&lt;br /&gt;
* V/Ã/_NF   Ingvaeonic nasal spirant law (vowel + nasal + voiceless fricative = nasal-vowel + fric.)&lt;br /&gt;
* k/ts/_[ie]     palatalization of k&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;td&amp;gt;&lt;br /&gt;
=== Insular Celtic ===&lt;br /&gt;
a.k.a Brittonic&lt;br /&gt;
&lt;br /&gt;
* keep am and an&lt;br /&gt;
* u/gw/#_&lt;br /&gt;
* s/h/#_V&lt;br /&gt;
* s//#_[lmn]&lt;br /&gt;
* sp/f/#_&lt;br /&gt;
* sr/fr/#_&lt;br /&gt;
* sw/xw/#_&lt;br /&gt;
* P/B/V_V  Voiceless stops become voiced stops in intervocalic position&lt;br /&gt;
* B/Z/V_V  Voiced plosives and /m/ became soft spirants in an intervocalic position&lt;br /&gt;
* B/Z/_L    Voiced plosives and /m/ became soft spirants before liquids&lt;br /&gt;
* P/F/_[LV]   Geminated voiceless plosives transformed into spirants before a vowel or liquid&lt;br /&gt;
* P/F/L_    Voiceless stops become spirants after liquids&lt;br /&gt;
* B//N_    Voiced stops were assimilated to a preceding nasal&lt;br /&gt;
&lt;br /&gt;
later ɣ/j/_&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;/tr&amp;gt;&lt;br /&gt;
&amp;lt;/table&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;&lt;br /&gt;
== Pre-1066 ==&lt;br /&gt;
&amp;lt;/center&amp;gt;&lt;br /&gt;
&amp;lt;table&amp;gt;&lt;br /&gt;
&amp;lt;tr&amp;gt;&lt;br /&gt;
&amp;lt;td&amp;gt;&lt;br /&gt;
=== To Old English ===&lt;br /&gt;
* Backing and nasalization of West Germanic a and ā before a nasal consonant&lt;br /&gt;
* Loss of n before a spirant, resulting in lengthening and nasalization of preceding vowel&lt;br /&gt;
* The present and preterite plurals reduced to a single form&lt;br /&gt;
* A-fronting: WGmc a, ā → æ, ǣ, even in the diphthongs ai and au (see Anglo-Frisian brightening)&lt;br /&gt;
* palatalization of Proto-Germanic *k and *g before front vowels (but not phonemicization of palatals)&lt;br /&gt;
* A-restoration: æ, ǣ → a, ā under the influence of neighboring consonants&lt;br /&gt;
* Second fronting: OE dialects (except West Saxon) and Frisian ǣ → ē&lt;br /&gt;
* A-restoration: a restored before a back vowel in the following syllable (later in the Southumbrian dialects); Frisian æu → au → Old Frisian ā/a&lt;br /&gt;
* OE breaking; in West Saxon palatal diphthongization follows&lt;br /&gt;
* i-mutation followed by syncope; Old Frisian breaking follows&lt;br /&gt;
* Phonemicization of palatals and assibilation, followed by second fronting in parts of West Mercia&lt;br /&gt;
* Smoothing and back mutation&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* loss of high vowels in syllable after stress&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=text-align:center&lt;br /&gt;
!&lt;br /&gt;
! Labial&lt;br /&gt;
! [[Dental consonant|Dental]]&lt;br /&gt;
! [[Alveolar consonant|Alveolar]]&lt;br /&gt;
! [[Postalveolar consonant|Post-&amp;lt;br /&amp;gt;alveolar]]&lt;br /&gt;
! [[Palatal consonant|Palatal]]&lt;br /&gt;
! [[Velar consonant|Velar]]&lt;br /&gt;
! [[Glottal consonant|Glottal]]&lt;br /&gt;
|-&lt;br /&gt;
! [[Nasal consonant|Nasal]]&lt;br /&gt;
| {{IPA|m}}&lt;br /&gt;
|&lt;br /&gt;
| ({{IPA|n̥}}) {{IPA|n}}&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| ({{IPA|ŋ}})&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
! [[Stop consonant|Stop]]&lt;br /&gt;
| {{IPA|p}} {{IPA|b}}&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|t}} {{IPA|d}}&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|k}} {{IPA|ɡ}}&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
! [[Affricate consonant|Affricate]]&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|tʃ}} ({{IPA|dʒ}})&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
! [[Fricative consonant|Fricative]]&lt;br /&gt;
| {{IPA|f}} ({{IPA|v}})&lt;br /&gt;
| {{IPA|θ}} ({{IPA|ð}})&lt;br /&gt;
| {{IPA|s}} ({{IPA|z}})&lt;br /&gt;
| {{IPA|ʃ}}&lt;br /&gt;
| ({{IPA|ç}})&lt;br /&gt;
| ({{IPA|x}} {{IPA|ɣ}})&lt;br /&gt;
| {{IPA|h}}&lt;br /&gt;
|-&lt;br /&gt;
! [[Approximant consonant|Approximant]]&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| ({{IPA|l̥}}) {{IPA|l}}&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|j}}&lt;br /&gt;
| ({{IPA|ʍ}}) {{IPA|w}}&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
! [[Trill consonant|Trill]]&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|colspan=2| ({{IPA|r̥}}) {{IPA|r}}&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;td&amp;gt;&lt;br /&gt;
=== To Middle Welsh ===&lt;br /&gt;
* Vː → V / _#&lt;br /&gt;
* ei → eː&lt;br /&gt;
* st → sː (with some exceptions)&lt;br /&gt;
** initial str → צ , middle/end str → sr&lt;br /&gt;
* ai → ɛ&lt;br /&gt;
* s → ∅ / V_V&lt;br /&gt;
* V → ə / _(C)#, also in proclitics&lt;br /&gt;
* s → ∅ / x_&lt;br /&gt;
* {au,eu,ou} → ∅&lt;br /&gt;
* uː {oi,ɔː} → yː uː&lt;br /&gt;
* j → ð / V_&lt;br /&gt;
* i u → e o / _Ca&lt;br /&gt;
* yː → ɨ&lt;br /&gt;
* p t k {b,m} d ɡ → b d ɡ v ð ɣ / _V&lt;br /&gt;
* aː → ɔː&lt;br /&gt;
* a o → ei {ɨ,ei} / _(C…)j(C…)#&lt;br /&gt;
* a → {ɨ,ei} / _(C…)j(C…)#&lt;br /&gt;
* V → ɨ / _(C…)j(C…)#&lt;br /&gt;
* {a,o} → e / _(C…)i(ː)&lt;br /&gt;
* {a,e,o} → ei / _(C…)j&lt;br /&gt;
* V → ∅ / _#&lt;br /&gt;
* mb nd ŋɡ → mː nː ŋː&lt;br /&gt;
* e → i / _N&lt;br /&gt;
* $ → h / V_ (what $ is is unclear)&lt;br /&gt;
* V → ∅ / _[+intertonic]&lt;br /&gt;
* pː tː kː → f θ x&lt;br /&gt;
* p t k → f θ x / {r,l}_&lt;br /&gt;
* ɣ → i / _C&lt;br /&gt;
* xt → iθ&lt;br /&gt;
* ɣ → i / C_V&lt;br /&gt;
* ɛː → ui&lt;br /&gt;
* ɔː → au / when stressed&lt;br /&gt;
* l → ɬ / _t&lt;br /&gt;
* w → gw / #[aeou] - w to gw before vowels-not-i&lt;br /&gt;
* mp nt ŋk → m̥ n̥ ŋ̊&lt;br /&gt;
* ɔ → ə / #_sC&lt;br /&gt;
* l r → ɬ r̥ / #_&lt;br /&gt;
* ɣ → ə / _#&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;text-align: center;&amp;quot;&lt;br /&gt;
|&lt;br /&gt;
! Labial&lt;br /&gt;
! Dental&lt;br /&gt;
! Alveolar&lt;br /&gt;
! Post-&amp;lt;br/&amp;gt;alveolar&lt;br /&gt;
! Palatal&lt;br /&gt;
! Velar&lt;br /&gt;
! Glottal&lt;br /&gt;
|-&lt;br /&gt;
!  Nasal&lt;br /&gt;
| {{IPA|m̥}} {{IPA|m}}&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|n̥}} {{IPA|n}}&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|ŋ̊}} {{IPA|ŋ}}&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
!  Stop&lt;br /&gt;
| {{IPA|p b}}&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|t d}}&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|k g}}&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
!  Fricative&lt;br /&gt;
| {{IPA|f v}}&lt;br /&gt;
| {{IPA|θ ð}}&lt;br /&gt;
| {{IPA|s z}}&lt;br /&gt;
| {{IPA|ɬ}} ({{IPA|ʃ}})&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|x}}&lt;br /&gt;
| {{IPA|h}}&lt;br /&gt;
|-&lt;br /&gt;
! Approximant&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|l}}&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|j}}&lt;br /&gt;
| {{IPA|w}}&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
! Trill&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|r̥ r}}&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;/tr&amp;gt;&lt;br /&gt;
&amp;lt;/table&amp;gt;&lt;br /&gt;
{{Aquatiki}}&lt;br /&gt;
[[Category:Weddish]]&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=User:Aquatiki/Sandbox2&amp;diff=175308</id>
		<title>User:Aquatiki/Sandbox2</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=User:Aquatiki/Sandbox2&amp;diff=175308"/>
		<updated>2025-10-06T22:10:05Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* PIE (-4500) */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;__TOC__&lt;br /&gt;
&amp;lt;div style=&amp;quot;width:100%; background:#ddd;&amp;quot;&amp;gt;&lt;br /&gt;
&amp;lt;center&amp;gt;&lt;br /&gt;
==PIE (-4500)==&lt;br /&gt;
&lt;br /&gt;
Cowgill&#039;s Law&lt;br /&gt;
&lt;br /&gt;
Osthoff&#039;s Law&lt;br /&gt;
&lt;br /&gt;
Sievers&#039;s law&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/center&amp;gt;&lt;br /&gt;
&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;table&amp;gt;&lt;br /&gt;
&amp;lt;tr&amp;gt;&lt;br /&gt;
&amp;lt;td&amp;gt;&lt;br /&gt;
&amp;lt;h3&amp;gt;Proto-Germanic (-500)&amp;lt;/h3&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* Grimm&#039;s Law, Verner&#039;s Law, Primärberührung&lt;br /&gt;
&lt;br /&gt;
{|class=&amp;quot;wikitable&amp;quot; style=text-align:center&lt;br /&gt;
|- style=&amp;quot;font-size: 90%;&amp;quot;&lt;br /&gt;
|+ Proto-Germanic consonants&lt;br /&gt;
!Type&lt;br /&gt;
! colspan=&amp;quot;2&amp;quot; style=&amp;quot;width:20px;&amp;quot;| Bilabial&lt;br /&gt;
! colspan=&amp;quot;2&amp;quot; style=&amp;quot;width:20px;&amp;quot;| Dental&lt;br /&gt;
! colspan=&amp;quot;2&amp;quot; style=&amp;quot;width:20px;&amp;quot;| Alveolar&lt;br /&gt;
! colspan=&amp;quot;2&amp;quot; style=&amp;quot;width:20px;&amp;quot;| Palatal&lt;br /&gt;
! colspan=&amp;quot;2&amp;quot; style=&amp;quot;width:20px;&amp;quot;| Velar&lt;br /&gt;
! colspan=&amp;quot;2&amp;quot; style=&amp;quot;width:20px;&amp;quot;| Labial–&amp;lt;br&amp;gt;velar&lt;br /&gt;
|-&lt;br /&gt;
! Nasal&lt;br /&gt;
|  style=&amp;quot;width:20px; border-right:0;&amp;quot;| ||  style=&amp;quot;width:20px; border-left:0;&amp;quot;|{{IPA|m}}&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|  style=&amp;quot;width:20px; border-right:0;&amp;quot;| ||  style=&amp;quot;width:20px; border-left:0;&amp;quot;|{{IPA|n}}&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|  style=&amp;quot;width:20px; border-right:0;&amp;quot;| ||  style=&amp;quot;width:20px; border-left:0;&amp;quot;|({{IPA|ŋ}})&lt;br /&gt;
|  style=&amp;quot;width:20px; border-right:0;&amp;quot;| ||  style=&amp;quot;width:20px; border-left:0;&amp;quot;|({{IPA|ŋʷ}})&lt;br /&gt;
|-&lt;br /&gt;
! [[Stop consonant|Stop]]&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|p}}||style=&amp;quot;border-left: 0;&amp;quot;|{{IPA|b}}&lt;br /&gt;
|  style=&amp;quot;width:20px; border-right:0;&amp;quot;|{{IPA|t}}||  style=&amp;quot;width:20px; border-left:0;&amp;quot;|{{IPA|d}}&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|k}}||style=&amp;quot;border-left: 0;&amp;quot;|{{IPA|ɡ}}&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|kʷ}}||style=&amp;quot;border-left: 0;&amp;quot;|{{IPA|ɡʷ}}&lt;br /&gt;
|-&lt;br /&gt;
! [[Fricative consonant|Fricative]]&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|ɸ}}||style=&amp;quot;border-left: 0;&amp;quot;|({{IPA|β}})&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|θ}}||style=&amp;quot;border-left: 0;&amp;quot;|({{IPA|ð}})&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|s}}||style=&amp;quot;border-left: 0;&amp;quot;|{{IPA|z}}&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|x}}||style=&amp;quot;border-left: 0;&amp;quot;|({{IPA|ɣ}})&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|xʷ}}||style=&amp;quot;border-left: 0;&amp;quot;|&lt;br /&gt;
|-&lt;br /&gt;
! [[Approximant consonant|Approximant]]&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|colspan=2| {{{IPA|l}}}&lt;br /&gt;
|  style=&amp;quot;width:20px; border-right:0;&amp;quot;| ||  style=&amp;quot;width:20px; border-left:0;&amp;quot;|{{IPA|j}}&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;| ||style=&amp;quot;border-left: 0;&amp;quot;|{{IPA|w}}&lt;br /&gt;
|-&lt;br /&gt;
! [[Trill consonant|Trill]]&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;| ||style=&amp;quot;border-left: 0;&amp;quot;|{{IPA|r}}&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Vowels&lt;br /&gt;
* i iː ĩ ĩː&lt;br /&gt;
* e eː&lt;br /&gt;
* ɛː ɛːː&lt;br /&gt;
* ɑ ɑː ɑ̃ ɑ̃ː&lt;br /&gt;
* ɔː ɔːː ɔ̃ː ɔ̃ːː&lt;br /&gt;
* u uː ũ ũː&lt;br /&gt;
&lt;br /&gt;
:  ô (aka ɔːː) became -a in ON and OE, but -oin OHG&lt;br /&gt;
: -ǭ became -a in OHG but -e in OE&lt;br /&gt;
: -ōn became -ōn in OHG but -an in OE&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;td&amp;gt;&lt;br /&gt;
&amp;lt;h3&amp;gt;Proto-Celtic (-800)&amp;lt;/h3&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Proto-Celtic consonants&lt;br /&gt;
|-&lt;br /&gt;
! Type&lt;br /&gt;
! colspan=2|&amp;amp;nbsp;[[Bilabial consonant|Bilabial]]&amp;amp;nbsp;&lt;br /&gt;
! colspan=2|&amp;amp;nbsp;[[Alveolar consonant|Alveolar]]&amp;amp;nbsp;&lt;br /&gt;
! colspan=2|&amp;amp;nbsp;[[Palatal consonant|Palatal]]&amp;amp;nbsp;&lt;br /&gt;
! colspan=2|&amp;amp;nbsp;[[Velar consonant|Velar]]&amp;amp;nbsp;&lt;br /&gt;
! colspan=2| Labial–&amp;lt;br&amp;gt;velar&lt;br /&gt;
|- style=&amp;quot;text-align:center;&amp;quot;&lt;br /&gt;
! [[Nasal stop|Nasal]]&lt;br /&gt;
| colspan=2|{{IPA|m}}&lt;br /&gt;
| colspan=2|{{IPA|n}}&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2|({{IPA|ŋ}})&lt;br /&gt;
| colspan=2|({{IPA|ŋʷ}})&lt;br /&gt;
|- style=&amp;quot;text-align:center;&amp;quot;&lt;br /&gt;
! [[Plosive consonant|Plosive]]&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|b}}&lt;br /&gt;
| {{IPA|t}}&lt;br /&gt;
| {{IPA|d}}&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| {{IPA|k}}&lt;br /&gt;
| {{IPA|ɡ}}&lt;br /&gt;
| {{IPA|kʷ}}&lt;br /&gt;
| {{IPA|ɡʷ}}&lt;br /&gt;
|- style=&amp;quot;text-align:center;&amp;quot;&lt;br /&gt;
! [[Fricative consonant|Fricative]]&lt;br /&gt;
| {{IPA|ɸ}}&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|s}}&lt;br /&gt;
|&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2| x&lt;br /&gt;
| colspan=2|&lt;br /&gt;
|- style=&amp;quot;text-align:center;&amp;quot;&lt;br /&gt;
! [[Approximant consonant|Approximant]]&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2| {{IPA|l}}&lt;br /&gt;
| colspan=2|{{IPA|j}}&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2| {{IPA|w}}&lt;br /&gt;
|- style=&amp;quot;text-align:center;&amp;quot;&lt;br /&gt;
! [[Trill consonant|Trill]]&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2| {{IPA|r}}&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2|&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* then kʷ/p/_   (P-Celtic)&lt;br /&gt;
&lt;br /&gt;
Vowels&lt;br /&gt;
* i iː&lt;br /&gt;
* e&lt;br /&gt;
* a aː&lt;br /&gt;
* o oː&lt;br /&gt;
* u uː&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;/tr&amp;gt;&lt;br /&gt;
&amp;lt;/table&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;table style=&amp;quot;width:100%; background:#ddd;&amp;quot;&amp;gt;&lt;br /&gt;
&amp;lt;tr&amp;gt;&lt;br /&gt;
&amp;lt;td colspan=2&amp;gt;&lt;br /&gt;
&amp;lt;center&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Through Roman Times ==&lt;br /&gt;
&amp;lt;/center&amp;gt;&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;/tr&amp;gt;&lt;br /&gt;
&amp;lt;tr&amp;gt;&lt;br /&gt;
&amp;lt;td&amp;gt;&lt;br /&gt;
=== Western Germanic ===&lt;br /&gt;
Ingvaeonic and Irminonic&lt;br /&gt;
&lt;br /&gt;
* /ɛː/, also written ǣ,  to ā&lt;br /&gt;
* umlaut&lt;br /&gt;
* z/r/V_V&lt;br /&gt;
* demonstrative &#039;&#039;this&#039;&#039;&lt;br /&gt;
* C/C²/_j   West Germanic gemination&lt;br /&gt;
&lt;br /&gt;
Decision Time!&lt;br /&gt;
* V/Ã/_NF   Ingvaeonic nasal spirant law (vowel + nasal + voiceless fricative = nasal-vowel + fric.)&lt;br /&gt;
* k/ts/_[ie]     palatalization of k&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;td&amp;gt;&lt;br /&gt;
=== Insular Celtic ===&lt;br /&gt;
a.k.a Brittonic&lt;br /&gt;
&lt;br /&gt;
* keep am and an&lt;br /&gt;
* u/gw/#_&lt;br /&gt;
* s/h/#_V&lt;br /&gt;
* s//#_[lmn]&lt;br /&gt;
* sp/f/#_&lt;br /&gt;
* sr/fr/#_&lt;br /&gt;
* sw/xw/#_&lt;br /&gt;
* P/B/V_V  Voiceless stops become voiced stops in intervocalic position&lt;br /&gt;
* B/Z/V_V  Voiced plosives and /m/ became soft spirants in an intervocalic position&lt;br /&gt;
* B/Z/_L    Voiced plosives and /m/ became soft spirants before liquids&lt;br /&gt;
* P/F/_[LV]   Geminated voiceless plosives transformed into spirants before a vowel or liquid&lt;br /&gt;
* P/F/L_    Voiceless stops become spirants after liquids&lt;br /&gt;
* B//N_    Voiced stops were assimilated to a preceding nasal&lt;br /&gt;
&lt;br /&gt;
later ɣ/j/_&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;/tr&amp;gt;&lt;br /&gt;
&amp;lt;/table&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;&lt;br /&gt;
== Pre-1066 ==&lt;br /&gt;
&amp;lt;/center&amp;gt;&lt;br /&gt;
&amp;lt;table&amp;gt;&lt;br /&gt;
&amp;lt;tr&amp;gt;&lt;br /&gt;
&amp;lt;td&amp;gt;&lt;br /&gt;
=== To Old English ===&lt;br /&gt;
* Backing and nasalization of West Germanic a and ā before a nasal consonant&lt;br /&gt;
* Loss of n before a spirant, resulting in lengthening and nasalization of preceding vowel&lt;br /&gt;
* The present and preterite plurals reduced to a single form&lt;br /&gt;
* A-fronting: WGmc a, ā → æ, ǣ, even in the diphthongs ai and au (see Anglo-Frisian brightening)&lt;br /&gt;
* palatalization of Proto-Germanic *k and *g before front vowels (but not phonemicization of palatals)&lt;br /&gt;
* A-restoration: æ, ǣ → a, ā under the influence of neighboring consonants&lt;br /&gt;
* Second fronting: OE dialects (except West Saxon) and Frisian ǣ → ē&lt;br /&gt;
* A-restoration: a restored before a back vowel in the following syllable (later in the Southumbrian dialects); Frisian æu → au → Old Frisian ā/a&lt;br /&gt;
* OE breaking; in West Saxon palatal diphthongization follows&lt;br /&gt;
* i-mutation followed by syncope; Old Frisian breaking follows&lt;br /&gt;
* Phonemicization of palatals and assibilation, followed by second fronting in parts of West Mercia&lt;br /&gt;
* Smoothing and back mutation&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* loss of high vowels in syllable after stress&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=text-align:center&lt;br /&gt;
!&lt;br /&gt;
! Labial&lt;br /&gt;
! [[Dental consonant|Dental]]&lt;br /&gt;
! [[Alveolar consonant|Alveolar]]&lt;br /&gt;
! [[Postalveolar consonant|Post-&amp;lt;br /&amp;gt;alveolar]]&lt;br /&gt;
! [[Palatal consonant|Palatal]]&lt;br /&gt;
! [[Velar consonant|Velar]]&lt;br /&gt;
! [[Glottal consonant|Glottal]]&lt;br /&gt;
|-&lt;br /&gt;
! [[Nasal consonant|Nasal]]&lt;br /&gt;
| {{IPA|m}}&lt;br /&gt;
|&lt;br /&gt;
| ({{IPA|n̥}}) {{IPA|n}}&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| ({{IPA|ŋ}})&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
! [[Stop consonant|Stop]]&lt;br /&gt;
| {{IPA|p}} {{IPA|b}}&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|t}} {{IPA|d}}&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|k}} {{IPA|ɡ}}&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
! [[Affricate consonant|Affricate]]&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|tʃ}} ({{IPA|dʒ}})&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
! [[Fricative consonant|Fricative]]&lt;br /&gt;
| {{IPA|f}} ({{IPA|v}})&lt;br /&gt;
| {{IPA|θ}} ({{IPA|ð}})&lt;br /&gt;
| {{IPA|s}} ({{IPA|z}})&lt;br /&gt;
| {{IPA|ʃ}}&lt;br /&gt;
| ({{IPA|ç}})&lt;br /&gt;
| ({{IPA|x}} {{IPA|ɣ}})&lt;br /&gt;
| {{IPA|h}}&lt;br /&gt;
|-&lt;br /&gt;
! [[Approximant consonant|Approximant]]&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| ({{IPA|l̥}}) {{IPA|l}}&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|j}}&lt;br /&gt;
| ({{IPA|ʍ}}) {{IPA|w}}&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
! [[Trill consonant|Trill]]&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|colspan=2| ({{IPA|r̥}}) {{IPA|r}}&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;td&amp;gt;&lt;br /&gt;
=== To Middle Welsh ===&lt;br /&gt;
* Vː → V / _#&lt;br /&gt;
* ei → eː&lt;br /&gt;
* st → sː (with some exceptions)&lt;br /&gt;
** initial str → צ , middle/end str → sr&lt;br /&gt;
* ai → ɛ&lt;br /&gt;
* s → ∅ / V_V&lt;br /&gt;
* V → ə / _(C)#, also in proclitics&lt;br /&gt;
* s → ∅ / x_&lt;br /&gt;
* {au,eu,ou} → ∅&lt;br /&gt;
* uː {oi,ɔː} → yː uː&lt;br /&gt;
* j → ð / V_&lt;br /&gt;
* i u → e o / _Ca&lt;br /&gt;
* yː → ɨ&lt;br /&gt;
* p t k {b,m} d ɡ → b d ɡ v ð ɣ / _V&lt;br /&gt;
* aː → ɔː&lt;br /&gt;
* a o → ei {ɨ,ei} / _(C…)j(C…)#&lt;br /&gt;
* a → {ɨ,ei} / _(C…)j(C…)#&lt;br /&gt;
* V → ɨ / _(C…)j(C…)#&lt;br /&gt;
* {a,o} → e / _(C…)i(ː)&lt;br /&gt;
* {a,e,o} → ei / _(C…)j&lt;br /&gt;
* V → ∅ / _#&lt;br /&gt;
* mb nd ŋɡ → mː nː ŋː&lt;br /&gt;
* e → i / _N&lt;br /&gt;
* $ → h / V_ (what $ is is unclear)&lt;br /&gt;
* V → ∅ / _[+intertonic]&lt;br /&gt;
* pː tː kː → f θ x&lt;br /&gt;
* p t k → f θ x / {r,l}_&lt;br /&gt;
* ɣ → i / _C&lt;br /&gt;
* xt → iθ&lt;br /&gt;
* ɣ → i / C_V&lt;br /&gt;
* ɛː → ui&lt;br /&gt;
* ɔː → au / when stressed&lt;br /&gt;
* l → ɬ / _t&lt;br /&gt;
* w → gw / #[aeou] - w to gw before vowels-not-i&lt;br /&gt;
* mp nt ŋk → m̥ n̥ ŋ̊&lt;br /&gt;
* ɔ → ə / #_sC&lt;br /&gt;
* l r → ɬ r̥ / #_&lt;br /&gt;
* ɣ → ə / _#&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;text-align: center;&amp;quot;&lt;br /&gt;
|&lt;br /&gt;
! Labial&lt;br /&gt;
! Dental&lt;br /&gt;
! Alveolar&lt;br /&gt;
! Post-&amp;lt;br/&amp;gt;alveolar&lt;br /&gt;
! Palatal&lt;br /&gt;
! Velar&lt;br /&gt;
! Glottal&lt;br /&gt;
|-&lt;br /&gt;
!  Nasal&lt;br /&gt;
| {{IPA|m̥}} {{IPA|m}}&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|n̥}} {{IPA|n}}&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|ŋ̊}} {{IPA|ŋ}}&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
!  Stop&lt;br /&gt;
| {{IPA|p b}}&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|t d}}&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|k g}}&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
!  Fricative&lt;br /&gt;
| {{IPA|f v}}&lt;br /&gt;
| {{IPA|θ ð}}&lt;br /&gt;
| {{IPA|s z}}&lt;br /&gt;
| {{IPA|ɬ}} ({{IPA|ʃ}})&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|x}}&lt;br /&gt;
| {{IPA|h}}&lt;br /&gt;
|-&lt;br /&gt;
! Approximant&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|l}}&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|j}}&lt;br /&gt;
| {{IPA|w}}&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
! Trill&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|r̥ r}}&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;/tr&amp;gt;&lt;br /&gt;
&amp;lt;/table&amp;gt;&lt;br /&gt;
{{Aquatiki}}&lt;br /&gt;
[[Category:Weddish]]&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=User:Aquatiki/Sandbox2&amp;diff=175307</id>
		<title>User:Aquatiki/Sandbox2</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=User:Aquatiki/Sandbox2&amp;diff=175307"/>
		<updated>2025-10-06T22:03:29Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: temp&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;__TOC__&lt;br /&gt;
&amp;lt;div style=&amp;quot;width:100%; background:#ddd;&amp;quot;&amp;gt;&lt;br /&gt;
&amp;lt;center&amp;gt;&lt;br /&gt;
==PIE (-4500)==&lt;br /&gt;
&lt;br /&gt;
Cowgill&#039;s Law&lt;br /&gt;
&lt;br /&gt;
Osthoff&#039;s Law&lt;br /&gt;
&lt;br /&gt;
Sievers&#039;s law&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/center&amp;gt;&lt;br /&gt;
&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;table&amp;gt;&lt;br /&gt;
&amp;lt;tr&amp;gt;&lt;br /&gt;
&amp;lt;td&amp;gt;&lt;br /&gt;
&amp;lt;h3&amp;gt;Proto-Germanic (-500)&amp;lt;/h3&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* Grimm&#039;s Law, Verner&#039;s Law, Primärberührung&lt;br /&gt;
&lt;br /&gt;
{|class=&amp;quot;wikitable&amp;quot; style=text-align:center&lt;br /&gt;
|- style=&amp;quot;font-size: 90%;&amp;quot;&lt;br /&gt;
|+ Proto-Germanic consonants&lt;br /&gt;
!Type&lt;br /&gt;
! colspan=&amp;quot;2&amp;quot; style=&amp;quot;width:20px;&amp;quot;| Bilabial&lt;br /&gt;
! colspan=&amp;quot;2&amp;quot; style=&amp;quot;width:20px;&amp;quot;| Dental&lt;br /&gt;
! colspan=&amp;quot;2&amp;quot; style=&amp;quot;width:20px;&amp;quot;| Alveolar&lt;br /&gt;
! colspan=&amp;quot;2&amp;quot; style=&amp;quot;width:20px;&amp;quot;| Palatal&lt;br /&gt;
! colspan=&amp;quot;2&amp;quot; style=&amp;quot;width:20px;&amp;quot;| Velar&lt;br /&gt;
! colspan=&amp;quot;2&amp;quot; style=&amp;quot;width:20px;&amp;quot;| Labial–&amp;lt;br&amp;gt;velar&lt;br /&gt;
|-&lt;br /&gt;
! Nasal&lt;br /&gt;
|  style=&amp;quot;width:20px; border-right:0;&amp;quot;| ||  style=&amp;quot;width:20px; border-left:0;&amp;quot;|{{IPA|m}}&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|  style=&amp;quot;width:20px; border-right:0;&amp;quot;| ||  style=&amp;quot;width:20px; border-left:0;&amp;quot;|{{IPA|n}}&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|  style=&amp;quot;width:20px; border-right:0;&amp;quot;| ||  style=&amp;quot;width:20px; border-left:0;&amp;quot;|({{IPA|ŋ}})&lt;br /&gt;
|  style=&amp;quot;width:20px; border-right:0;&amp;quot;| ||  style=&amp;quot;width:20px; border-left:0;&amp;quot;|({{IPA|ŋʷ}})&lt;br /&gt;
|-&lt;br /&gt;
! [[Stop consonant|Stop]]&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|p}}||style=&amp;quot;border-left: 0;&amp;quot;|{{IPA|b}}&lt;br /&gt;
|  style=&amp;quot;width:20px; border-right:0;&amp;quot;|{{IPA|t}}||  style=&amp;quot;width:20px; border-left:0;&amp;quot;|{{IPA|d}}&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|k}}||style=&amp;quot;border-left: 0;&amp;quot;|{{IPA|ɡ}}&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|kʷ}}||style=&amp;quot;border-left: 0;&amp;quot;|{{IPA|ɡʷ}}&lt;br /&gt;
|-&lt;br /&gt;
! [[Fricative consonant|Fricative]]&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|ɸ}}||style=&amp;quot;border-left: 0;&amp;quot;|({{IPA|β}})&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|θ}}||style=&amp;quot;border-left: 0;&amp;quot;|({{IPA|ð}})&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|s}}||style=&amp;quot;border-left: 0;&amp;quot;|{{IPA|z}}&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|x}}||style=&amp;quot;border-left: 0;&amp;quot;|({{IPA|ɣ}})&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;|{{IPA|xʷ}}||style=&amp;quot;border-left: 0;&amp;quot;|&lt;br /&gt;
|-&lt;br /&gt;
! [[Approximant consonant|Approximant]]&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|colspan=2| {{{IPA|l}}}&lt;br /&gt;
|  style=&amp;quot;width:20px; border-right:0;&amp;quot;| ||  style=&amp;quot;width:20px; border-left:0;&amp;quot;|{{IPA|j}}&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;| ||style=&amp;quot;border-left: 0;&amp;quot;|{{IPA|w}}&lt;br /&gt;
|-&lt;br /&gt;
! [[Trill consonant|Trill]]&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|style=&amp;quot;border-right: 0;&amp;quot;| ||style=&amp;quot;border-left: 0;&amp;quot;|{{IPA|r}}&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|colspan=2|&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Vowels&lt;br /&gt;
* i iː ĩ ĩː&lt;br /&gt;
* e eː&lt;br /&gt;
* ɛː ɛːː&lt;br /&gt;
* ɑ ɑː ɑ̃ ɑ̃ː&lt;br /&gt;
* ɔː ɔːː ɔ̃ː ɔ̃ːː&lt;br /&gt;
* u uː ũ ũː&lt;br /&gt;
&lt;br /&gt;
:  ô (aka ɔːː) became -a in ON and OE, but -oin OHG&lt;br /&gt;
: -ǭ became -a in OHG but -e in OE&lt;br /&gt;
: -ōn became -ōn in OHG but -an in OE&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;td&amp;gt;&lt;br /&gt;
&amp;lt;h3&amp;gt;Proto-Celtic (-800)&amp;lt;/h3&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Proto-Celtic consonants&lt;br /&gt;
|-&lt;br /&gt;
! Type&lt;br /&gt;
! colspan=2|&amp;amp;nbsp;[[Bilabial consonant|Bilabial]]&amp;amp;nbsp;&lt;br /&gt;
! colspan=2|&amp;amp;nbsp;[[Alveolar consonant|Alveolar]]&amp;amp;nbsp;&lt;br /&gt;
! colspan=2|&amp;amp;nbsp;[[Palatal consonant|Palatal]]&amp;amp;nbsp;&lt;br /&gt;
! colspan=2|&amp;amp;nbsp;[[Velar consonant|Velar]]&amp;amp;nbsp;&lt;br /&gt;
! colspan=2| Labial–&amp;lt;br&amp;gt;velar&lt;br /&gt;
|- style=&amp;quot;text-align:center;&amp;quot;&lt;br /&gt;
! [[Nasal stop|Nasal]]&lt;br /&gt;
| colspan=2|{{IPA|m}}&lt;br /&gt;
| colspan=2|{{IPA|n}}&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2|({{IPA|ŋ}})&lt;br /&gt;
| colspan=2|({{IPA|ŋʷ}})&lt;br /&gt;
|- style=&amp;quot;text-align:center;&amp;quot;&lt;br /&gt;
! [[Plosive consonant|Plosive]]&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|b}}&lt;br /&gt;
| {{IPA|t}}&lt;br /&gt;
| {{IPA|d}}&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| {{IPA|k}}&lt;br /&gt;
| {{IPA|ɡ}}&lt;br /&gt;
| {{IPA|kʷ}}&lt;br /&gt;
| {{IPA|ɡʷ}}&lt;br /&gt;
|- style=&amp;quot;text-align:center;&amp;quot;&lt;br /&gt;
! [[Fricative consonant|Fricative]]&lt;br /&gt;
| {{IPA|ɸ}}&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|s}}&lt;br /&gt;
|&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2|&lt;br /&gt;
|- style=&amp;quot;text-align:center;&amp;quot;&lt;br /&gt;
! [[Approximant consonant|Approximant]]&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2| {{IPA|l}}&lt;br /&gt;
| colspan=2|{{IPA|j}}&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2| {{IPA|w}}&lt;br /&gt;
|- style=&amp;quot;text-align:center;&amp;quot;&lt;br /&gt;
! [[Trill consonant|Trill]]&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2| {{IPA|r}}&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2|&lt;br /&gt;
| colspan=2|&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* then kʷ/p/_   (P-Celtic)&lt;br /&gt;
&lt;br /&gt;
Vowels&lt;br /&gt;
* i iː&lt;br /&gt;
* e&lt;br /&gt;
* a aː&lt;br /&gt;
* o oː&lt;br /&gt;
* u uː&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;/tr&amp;gt;&lt;br /&gt;
&amp;lt;/table&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;table style=&amp;quot;width:100%; background:#ddd;&amp;quot;&amp;gt;&lt;br /&gt;
&amp;lt;tr&amp;gt;&lt;br /&gt;
&amp;lt;td colspan=2&amp;gt;&lt;br /&gt;
&amp;lt;center&amp;gt;&lt;br /&gt;
== Through Roman Times ==&lt;br /&gt;
&amp;lt;/center&amp;gt;&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;/tr&amp;gt;&lt;br /&gt;
&amp;lt;tr&amp;gt;&lt;br /&gt;
&amp;lt;td&amp;gt;&lt;br /&gt;
=== Western Germanic ===&lt;br /&gt;
Ingvaeonic and Irminonic&lt;br /&gt;
&lt;br /&gt;
* /ɛː/, also written ǣ,  to ā&lt;br /&gt;
* umlaut&lt;br /&gt;
* z/r/V_V&lt;br /&gt;
* demonstrative &#039;&#039;this&#039;&#039;&lt;br /&gt;
* C/C²/_j   West Germanic gemination&lt;br /&gt;
&lt;br /&gt;
Decision Time!&lt;br /&gt;
* V/Ã/_NF   Ingvaeonic nasal spirant law (vowel + nasal + voiceless fricative = nasal-vowel + fric.)&lt;br /&gt;
* k/ts/_[ie]     palatalization of k&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;td&amp;gt;&lt;br /&gt;
=== Insular Celtic ===&lt;br /&gt;
a.k.a Brittonic&lt;br /&gt;
&lt;br /&gt;
* keep am and an&lt;br /&gt;
* u/gw/#_&lt;br /&gt;
* s/h/#_V&lt;br /&gt;
* s//#_[lmn]&lt;br /&gt;
* sp/f/#_&lt;br /&gt;
* sr/fr/#_&lt;br /&gt;
* sw/xw/#_&lt;br /&gt;
* P/B/V_V  Voiceless stops become voiced stops in intervocalic position&lt;br /&gt;
* B/Z/V_V  Voiced plosives and /m/ became soft spirants in an intervocalic position&lt;br /&gt;
* B/Z/_L    Voiced plosives and /m/ became soft spirants before liquids&lt;br /&gt;
* P/F/_[LV]   Geminated voiceless plosives transformed into spirants before a vowel or liquid&lt;br /&gt;
* P/F/L_    Voiceless stops become spirants after liquids&lt;br /&gt;
* B//N_    Voiced stops were assimilated to a preceding nasal&lt;br /&gt;
&lt;br /&gt;
later ɣ/j/_&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;/tr&amp;gt;&lt;br /&gt;
&amp;lt;/table&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;center&amp;gt;&lt;br /&gt;
== Pre-1066 ==&lt;br /&gt;
&amp;lt;/center&amp;gt;&lt;br /&gt;
&amp;lt;table&amp;gt;&lt;br /&gt;
&amp;lt;tr&amp;gt;&lt;br /&gt;
&amp;lt;td&amp;gt;&lt;br /&gt;
=== To Old English ===&lt;br /&gt;
* Backing and nasalization of West Germanic a and ā before a nasal consonant&lt;br /&gt;
* Loss of n before a spirant, resulting in lengthening and nasalization of preceding vowel&lt;br /&gt;
* The present and preterite plurals reduced to a single form&lt;br /&gt;
* A-fronting: WGmc a, ā → æ, ǣ, even in the diphthongs ai and au (see Anglo-Frisian brightening)&lt;br /&gt;
* palatalization of Proto-Germanic *k and *g before front vowels (but not phonemicization of palatals)&lt;br /&gt;
* A-restoration: æ, ǣ → a, ā under the influence of neighboring consonants&lt;br /&gt;
* Second fronting: OE dialects (except West Saxon) and Frisian ǣ → ē&lt;br /&gt;
* A-restoration: a restored before a back vowel in the following syllable (later in the Southumbrian dialects); Frisian æu → au → Old Frisian ā/a&lt;br /&gt;
* OE breaking; in West Saxon palatal diphthongization follows&lt;br /&gt;
* i-mutation followed by syncope; Old Frisian breaking follows&lt;br /&gt;
* Phonemicization of palatals and assibilation, followed by second fronting in parts of West Mercia&lt;br /&gt;
* Smoothing and back mutation&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
* loss of high vowels in syllable after stress&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=text-align:center&lt;br /&gt;
!&lt;br /&gt;
! Labial&lt;br /&gt;
! [[Dental consonant|Dental]]&lt;br /&gt;
! [[Alveolar consonant|Alveolar]]&lt;br /&gt;
! [[Postalveolar consonant|Post-&amp;lt;br /&amp;gt;alveolar]]&lt;br /&gt;
! [[Palatal consonant|Palatal]]&lt;br /&gt;
! [[Velar consonant|Velar]]&lt;br /&gt;
! [[Glottal consonant|Glottal]]&lt;br /&gt;
|-&lt;br /&gt;
! [[Nasal consonant|Nasal]]&lt;br /&gt;
| {{IPA|m}}&lt;br /&gt;
|&lt;br /&gt;
| ({{IPA|n̥}}) {{IPA|n}}&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| ({{IPA|ŋ}})&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
! [[Stop consonant|Stop]]&lt;br /&gt;
| {{IPA|p}} {{IPA|b}}&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|t}} {{IPA|d}}&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|k}} {{IPA|ɡ}}&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
! [[Affricate consonant|Affricate]]&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|tʃ}} ({{IPA|dʒ}})&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
! [[Fricative consonant|Fricative]]&lt;br /&gt;
| {{IPA|f}} ({{IPA|v}})&lt;br /&gt;
| {{IPA|θ}} ({{IPA|ð}})&lt;br /&gt;
| {{IPA|s}} ({{IPA|z}})&lt;br /&gt;
| {{IPA|ʃ}}&lt;br /&gt;
| ({{IPA|ç}})&lt;br /&gt;
| ({{IPA|x}} {{IPA|ɣ}})&lt;br /&gt;
| {{IPA|h}}&lt;br /&gt;
|-&lt;br /&gt;
! [[Approximant consonant|Approximant]]&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| ({{IPA|l̥}}) {{IPA|l}}&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|j}}&lt;br /&gt;
| ({{IPA|ʍ}}) {{IPA|w}}&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
! [[Trill consonant|Trill]]&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|colspan=2| ({{IPA|r̥}}) {{IPA|r}}&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;td&amp;gt;&lt;br /&gt;
=== To Middle Welsh ===&lt;br /&gt;
* Vː → V / _#&lt;br /&gt;
* ei → eː&lt;br /&gt;
* st → sː (with some exceptions)&lt;br /&gt;
** initial str → צ , middle/end str → sr&lt;br /&gt;
* ai → ɛ&lt;br /&gt;
* s → ∅ / V_V&lt;br /&gt;
* V → ə / _(C)#, also in proclitics&lt;br /&gt;
* s → ∅ / x_&lt;br /&gt;
* {au,eu,ou} → ∅&lt;br /&gt;
* uː {oi,ɔː} → yː uː&lt;br /&gt;
* j → ð / V_&lt;br /&gt;
* i u → e o / _Ca&lt;br /&gt;
* yː → ɨ&lt;br /&gt;
* p t k {b,m} d ɡ → b d ɡ v ð ɣ / _V&lt;br /&gt;
* aː → ɔː&lt;br /&gt;
* a o → ei {ɨ,ei} / _(C…)j(C…)#&lt;br /&gt;
* a → {ɨ,ei} / _(C…)j(C…)#&lt;br /&gt;
* V → ɨ / _(C…)j(C…)#&lt;br /&gt;
* {a,o} → e / _(C…)i(ː)&lt;br /&gt;
* {a,e,o} → ei / _(C…)j&lt;br /&gt;
* V → ∅ / _#&lt;br /&gt;
* mb nd ŋɡ → mː nː ŋː&lt;br /&gt;
* e → i / _N&lt;br /&gt;
* $ → h / V_ (what $ is is unclear)&lt;br /&gt;
* V → ∅ / _[+intertonic]&lt;br /&gt;
* pː tː kː → f θ x&lt;br /&gt;
* p t k → f θ x / {r,l}_&lt;br /&gt;
* ɣ → i / _C&lt;br /&gt;
* xt → iθ&lt;br /&gt;
* ɣ → i / C_V&lt;br /&gt;
* ɛː → ui&lt;br /&gt;
* ɔː → au / when stressed&lt;br /&gt;
* l → ɬ / _t&lt;br /&gt;
* w → gw / #[aeou] - w to gw before vowels-not-i&lt;br /&gt;
* mp nt ŋk → m̥ n̥ ŋ̊&lt;br /&gt;
* ɔ → ə / #_sC&lt;br /&gt;
* l r → ɬ r̥ / #_&lt;br /&gt;
* ɣ → ə / _#&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;text-align: center;&amp;quot;&lt;br /&gt;
|&lt;br /&gt;
! Labial&lt;br /&gt;
! Dental&lt;br /&gt;
! Alveolar&lt;br /&gt;
! Post-&amp;lt;br/&amp;gt;alveolar&lt;br /&gt;
! Palatal&lt;br /&gt;
! Velar&lt;br /&gt;
! Glottal&lt;br /&gt;
|-&lt;br /&gt;
!  Nasal&lt;br /&gt;
| {{IPA|m̥}} {{IPA|m}}&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|n̥}} {{IPA|n}}&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|ŋ̊}} {{IPA|ŋ}}&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
!  Stop&lt;br /&gt;
| {{IPA|p b}}&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|t d}}&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|k g}}&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
!  Fricative&lt;br /&gt;
| {{IPA|f v}}&lt;br /&gt;
| {{IPA|θ ð}}&lt;br /&gt;
| {{IPA|s z}}&lt;br /&gt;
| {{IPA|ɬ}} ({{IPA|ʃ}})&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|x}}&lt;br /&gt;
| {{IPA|h}}&lt;br /&gt;
|-&lt;br /&gt;
! Approximant&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|l}}&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|j}}&lt;br /&gt;
| {{IPA|w}}&lt;br /&gt;
|&lt;br /&gt;
|-&lt;br /&gt;
! Trill&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
| {{IPA|r̥ r}}&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/td&amp;gt;&lt;br /&gt;
&amp;lt;/tr&amp;gt;&lt;br /&gt;
&amp;lt;/table&amp;gt;&lt;br /&gt;
{{Aquatiki}}&lt;br /&gt;
[[Category:Weddish]]&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=Dan%27a%27yo/Psalm2&amp;diff=174925</id>
		<title>Dan&#039;a&#039;yo/Psalm2</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=Dan%27a%27yo/Psalm2&amp;diff=174925"/>
		<updated>2025-09-17T00:24:58Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: Created page with &amp;quot;何故萬邦喧？ 萬民誦虛？  列王起立， 群侯同謀； 逆偕者、逆天子： 「斷其縛！棄其繩！」  天上坐哂。 天皇譏之。 怒而言， 忿而驚： 「我立我王， 於郇聖山。」  我述其詔： 偕者謂我曰： 「爾為我子， 今日我生爾。 求我， 萬國爾業， 地極爾產。 鐵杖牧之， 陶器碎之。」  王其智！ 士其訓！ 畏而事偕者， 懼而喜。  惜囝！ 免其怒； 免亡於途。 頃...&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;何故萬邦喧？&lt;br /&gt;
萬民誦虛？&lt;br /&gt;
&lt;br /&gt;
列王起立，&lt;br /&gt;
群侯同謀；&lt;br /&gt;
逆偕者、逆天子：&lt;br /&gt;
「斷其縛！棄其繩！」&lt;br /&gt;
&lt;br /&gt;
天上坐哂。&lt;br /&gt;
天皇譏之。&lt;br /&gt;
怒而言，&lt;br /&gt;
忿而驚：&lt;br /&gt;
「我立我王，&lt;br /&gt;
於郇聖山。」&lt;br /&gt;
&lt;br /&gt;
我述其詔：&lt;br /&gt;
偕者謂我曰：&lt;br /&gt;
「爾為我子，&lt;br /&gt;
今日我生爾。&lt;br /&gt;
求我，&lt;br /&gt;
萬國爾業，&lt;br /&gt;
地極爾產。&lt;br /&gt;
鐵杖牧之，&lt;br /&gt;
陶器碎之。」&lt;br /&gt;
&lt;br /&gt;
王其智！&lt;br /&gt;
士其訓！&lt;br /&gt;
畏而事偕者，&lt;br /&gt;
懼而喜。&lt;br /&gt;
&lt;br /&gt;
惜囝！&lt;br /&gt;
免其怒；&lt;br /&gt;
免亡於途。&lt;br /&gt;
頃刻忿燃。&lt;br /&gt;
&lt;br /&gt;
凡投靠彼者，&lt;br /&gt;
皆有福。&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=Dan%27a%27yo/Psalm1&amp;diff=174924</id>
		<title>Dan&#039;a&#039;yo/Psalm1</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=Dan%27a%27yo/Psalm1&amp;diff=174924"/>
		<updated>2025-09-16T23:43:25Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: format&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&amp;lt;pre&amp;gt;&lt;br /&gt;
有福之人：&lt;br /&gt;
不行惡謀，&lt;br /&gt;
不立罪途，&lt;br /&gt;
不坐譏席。&lt;br /&gt;
惟喜偕法，&lt;br /&gt;
晝夜誦思。&lt;br /&gt;
若樹臨溪，&lt;br /&gt;
根飲清泉；&lt;br /&gt;
時結嘉實，&lt;br /&gt;
葉不凋零。&lt;br /&gt;
凡所為者，&lt;br /&gt;
皆遂其成。&lt;br /&gt;
&lt;br /&gt;
惡人不然！&lt;br /&gt;
乃若糠粃，&lt;br /&gt;
風吹散逸。&lt;br /&gt;
是故審判，&lt;br /&gt;
惡者不立；&lt;br /&gt;
義眾之中，&lt;br /&gt;
罪人不居。&lt;br /&gt;
義人之途，&lt;br /&gt;
偕者所識；&lt;br /&gt;
惡人之路，&lt;br /&gt;
終必敗亡。&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
偕者=YHWH&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=Dan%27a%27yo/Psalm1&amp;diff=174923</id>
		<title>Dan&#039;a&#039;yo/Psalm1</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=Dan%27a%27yo/Psalm1&amp;diff=174923"/>
		<updated>2025-09-16T23:41:32Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: Created page with &amp;quot;&amp;lt;pre&amp;gt; 有福之人： 不行惡謀， 不立罪途， 不坐譏席。惟喜偕法， 晝夜誦思。若樹臨溪， 根飲清泉； 時結嘉實， 葉不凋零。 凡所為者， 皆遂其成。惡人不然！ 乃若糠粃， 風吹散逸。是故審判， 惡者不立； 義眾之中， 罪人不居。義人之途， 偕者所識； 惡人之路， 終必敗亡。  &amp;lt;/pre&amp;gt;&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&amp;lt;pre&amp;gt;&lt;br /&gt;
有福之人：&lt;br /&gt;
不行惡謀，&lt;br /&gt;
不立罪途，&lt;br /&gt;
不坐譏席。惟喜偕法，&lt;br /&gt;
晝夜誦思。若樹臨溪，&lt;br /&gt;
根飲清泉；&lt;br /&gt;
時結嘉實，&lt;br /&gt;
葉不凋零。&lt;br /&gt;
凡所為者，&lt;br /&gt;
皆遂其成。惡人不然！&lt;br /&gt;
乃若糠粃，&lt;br /&gt;
風吹散逸。是故審判，&lt;br /&gt;
惡者不立；&lt;br /&gt;
義眾之中，&lt;br /&gt;
罪人不居。義人之途，&lt;br /&gt;
偕者所識；&lt;br /&gt;
惡人之路，&lt;br /&gt;
終必敗亡。&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=Ko%C7%A7an/218&amp;diff=171032</id>
		<title>Koǧan/218</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=Ko%C7%A7an/218&amp;diff=171032"/>
		<updated>2025-05-28T02:22:17Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: revisions&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;# Al sol brillazh.&lt;br /&gt;
# Al sol estázh brillant.&lt;br /&gt;
# Al sol brillázh.&lt;br /&gt;
# Al sol brillarázh.&lt;br /&gt;
# Al sol azh estat brillant.&lt;br /&gt;
# Al sol estázh brillant xuv.&lt;br /&gt;
# Al sol brillarázh kras.&lt;br /&gt;
# Al sol brillazh kòn fwèrca.&lt;br /&gt;
# Al sol luxònte brillazh.&lt;br /&gt;
# Al sol estázh naxint alán.&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=Ko%C7%A7an/218&amp;diff=171020</id>
		<title>Koǧan/218</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=Ko%C7%A7an/218&amp;diff=171020"/>
		<updated>2025-05-27T22:17:06Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: spelling&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;# Al sol brillazh.&lt;br /&gt;
# Al sol estázh brillant.&lt;br /&gt;
# Al sol brillázh.&lt;br /&gt;
# Al sol brillarázh.&lt;br /&gt;
# Al sol azh estat brillant.&lt;br /&gt;
# Al sol èzh brillant xuv.&lt;br /&gt;
# Al sol brillarázh kras.&lt;br /&gt;
# Al sol brillazh kòn fwèrca.&lt;br /&gt;
# Al sol luzhònte brillazh.&lt;br /&gt;
# Al sol esta naxint lan.&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=Ko%C7%A7an&amp;diff=170989</id>
		<title>Koǧan</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=Ko%C7%A7an&amp;diff=170989"/>
		<updated>2025-05-26T04:10:36Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: spelling update&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Aspect !! Details&lt;br /&gt;
|-&lt;br /&gt;
! Name&lt;br /&gt;
| *Caudia*, from Latin *cauda* &amp;quot;tail&amp;quot; — a metaphor for “tail-end” of Latinity          &lt;br /&gt;
|-&lt;br /&gt;
! Location&lt;br /&gt;
| Southeast of the Balearics, equidistant from Ibiza, Algiers, and Cagliari&lt;br /&gt;
|-&lt;br /&gt;
! Size &lt;br /&gt;
| Roughly 120 km long, mountainous interior, coastal plains &lt;br /&gt;
|-&lt;br /&gt;
! Geological Origin&lt;br /&gt;
|  Volcanic + limestone; freshwater aquifers, arable valleys&lt;br /&gt;
|-&lt;br /&gt;
! Climate&lt;br /&gt;
| Mediterranean; olive, fig, almond, and cereal agriculture&lt;br /&gt;
|-&lt;br /&gt;
!  Historical Timeline&lt;br /&gt;
| Phoenician colony, Muslim conquest, Cordoban/Andalusian territory, later than Reconquista, &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Koǧa was part of the Caliphate of Córdoba from early on and developed as an exceptionally tolerant multicultural haven, offering the greatest protection and coexistence for Jews and Christians anywhere in the empire.  Extended exposure to Classical Arabic, not merely rural dialects. Jewish linguistic influence (e.g., Hebrew calques, Semitic syntax transfers, or Judeo-Romance variants). Christian Latin continuity via protected ecclesiastical communities and monastic scribes. An intellectual center for translation, scientific synthesis, and lexical borrowing in philosophy, agriculture, medicine, and jurisprudence.&lt;br /&gt;
&lt;br /&gt;
== Historical Background of Caudia ==&lt;br /&gt;
&lt;br /&gt;
The island of Caudia (endonym: Koǧa) occupies a unique position in the Romance-speaking world. Located in the western Mediterranean, equidistant from Ibiza, Algiers, and Cagliari, Caudia developed in partial isolation yet maintained sustained maritime contact with several major cultural centers. Its linguistic history reflects a sequence of layered influences, beginning with Roman colonization and extending through a complex legacy of religious, political, and intellectual exchange. The result is a Romance language of singular character, deeply shaped by Semitic and Hellenistic overlays, yet structurally descended from Vulgar Latin.&lt;br /&gt;
&lt;br /&gt;
=== I. Late Roman and Early Post-Roman Period ===&lt;br /&gt;
&lt;br /&gt;
During the late Roman Empire, Caudia was settled by a community of Latin-speaking provincials with strong ties to the eastern Mediterranean. Archaeological and textual evidence suggest that the early Caudian population may have included a substantial Jewish demographic, either as voluntary migrants or as resettled populations following the destruction of the Second Temple and later Roman crackdowns. These settlers brought with them not only Latin but also a background in Koine Greek, Hebrew, and the legalistic registers of Classical education.&lt;br /&gt;
&lt;br /&gt;
The variety of Latin spoken on Caudia diverged early from continental Vulgar Latin. While it maintained the phonological shifts typical of spoken Latin (e.g., syncope, monophthongization), the syntactic and lexical profile of early Caudian Latin bore traces of its learned origins:&lt;br /&gt;
&lt;br /&gt;
* Lexical borrowings from Greek and Hebrew entered at an early stage.&lt;br /&gt;
* Certain Classical Latin archaisms, particularly in legal and rhetorical constructions, were preserved in fossilized forms.&lt;br /&gt;
* Syntax exhibited conservatism in verbal periphrases and pronoun usage, possibly influenced by scriptural Hebrew and ecclesiastical Latin.&lt;br /&gt;
&lt;br /&gt;
This substratum, referred to by linguists as Proto-Koǧan, laid the foundation for later development. It is best viewed as a peripheral but not isolated offshoot of Proto-Romance, exhibiting both conservatism and early hybridization.&lt;br /&gt;
&lt;br /&gt;
=== II. Islamic Period: Integration into al-Andalus ===&lt;br /&gt;
&lt;br /&gt;
In the early 8th century CE, Caudia was absorbed into the expanding Umayyad Caliphate, and subsequently became an overseas dependency of the Emirate, later Caliphate, of Córdoba. Owing to its small size and strategic position, Caudia functioned less as a military outpost and more as an intellectual and mercantile enclave. Its ports hosted traders, translators, and jurists; its inland monasteries and zawiyas (زوايا) became centers of scholarship and religious dialogue.&lt;br /&gt;
&lt;br /&gt;
During this period, Caudia acquired a reputation for exceptional religious tolerance. Jewish, Christian, and Muslim communities coexisted under the relatively lenient dhimmi system, with Jewish communities in particular enjoying a degree of autonomy and prestige rarely matched elsewhere in the Islamic world. Koǧan oral traditions record this period as a &amp;quot;golden age&amp;quot; of letters.&lt;br /&gt;
&lt;br /&gt;
The impact on the language was profound:&lt;br /&gt;
* Arabic loanwords entered in significant numbers, particularly in domains such as philosophy, jurisprudence, medicine, agriculture, architecture, and administration.&lt;br /&gt;
* Unlike Iberian Romance languages, Arabic borrowings were typically adopted without the definite article al-, a sign of the Caudians’ familiarity with Arabic morphology and semantics. Thus, mufada (pillow) rather than almufada, or zawija (monastery) rather than alzawija.&lt;br /&gt;
* Arabic borrowings were often morphologically integrated into native derivational patterns, and show consistent phonological adaptation to Koǧan phonotactics.&lt;br /&gt;
* The variety of Arabic spoken on the island was closer to Classical Arabic (fuṣḥā) than to Maghrebi vernaculars, further differentiating Caudian Arabic from that of the Iberian Peninsula.&lt;br /&gt;
&lt;br /&gt;
This period also witnessed the rise of Caudia as a translation center, where Hebrew exegetes, Latin scribes, and Arabic philosophers worked in tandem to produce multilingual treatises. This tri-scriptural culture left a permanent imprint on Koǧan lexicon and discourse style.&lt;br /&gt;
&lt;br /&gt;
=== III. Post-Andalusian Period: Semi-Autonomous Continuity ===&lt;br /&gt;
&lt;br /&gt;
The island&#039;s relationship to the Christian Reconquista was anomalous. While Caudia formally came under the suzerainty of various Christian polities (at various times Pisa, Aragon, or Genoa), it was rarely subjected to direct ecclesiastical or military control. As such, Caudia remained culturally hybrid, and retained both Arabic and Hebrew institutions long after their suppression on the mainland.&lt;br /&gt;
&lt;br /&gt;
During this period, Latin liturgical practices reasserted themselves, particularly in coastal cathedrals and episcopal centers. However, these coexisted with enduring Muslim and Jewish communities. The vernacular Koǧan language became the principal vehicle of interfaith communication, absorbing and transmitting the philosophical, legal, and agricultural terminologies of the three traditions.&lt;br /&gt;
&lt;br /&gt;
The linguistic consequences included:&lt;br /&gt;
* Continued but more selective lexical borrowing from Latin and emerging Ibero-Romance varieties.&lt;br /&gt;
* Increased semantic specialization in loanwords — e.g., Arabic terms retained specific technical senses.&lt;br /&gt;
* Preservation of older grammatical constructions due to textual conservatism in religious and legal documents.&lt;br /&gt;
* Emergence of a prestige dialect among urban literati, with phonological hypercorrections and borrowings from ecclesiastical Latin.&lt;br /&gt;
&lt;br /&gt;
=== IV. Linguistic Summary ===&lt;br /&gt;
&lt;br /&gt;
The Koǧan language as it exists today is thus the product of a deeply stratified linguistic ecology, in which:&lt;br /&gt;
* Proto-Romance provides the grammatical skeleton.&lt;br /&gt;
* Classical Latin and Koine Greek supply archaisms and syntactic conservatism.&lt;br /&gt;
* Hebrew contributes both lexical items and subtle syntactic calques, particularly in parallelism and discourse structure.&lt;br /&gt;
* Arabic offers a rich stratum of vocabulary and intellectual idioms, stripped of folk transmission markers such as definite articles.&lt;br /&gt;
* Ecclesiastical Latin in the post-Reconquista era reaffirms certain nominal and participial structures in formal contexts.&lt;br /&gt;
&lt;br /&gt;
The resulting language is Romance at its core, but notably non-European in its evolution — a Romance language that grew up not under the shadow of Charlemagne or Castile, but under the dome of Córdoba and the scrolls of Tiberias.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Phonology ==&lt;br /&gt;
Forms that differ from IPA are shown in bold.  Most allophony occurs intervocalically.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;text-align: center&amp;quot;&lt;br /&gt;
|+ Koǧan Consonant Phonemes&lt;br /&gt;
! Manner \ Place || Labial || Alveolar || Palatal || Velar &lt;br /&gt;
|-&lt;br /&gt;
! Nasal&lt;br /&gt;
| /m/ || /n || /ɲ/ &#039;&#039;&#039;ñ&#039;&#039;&#039; || &lt;br /&gt;
|-&lt;br /&gt;
! Stop (voiceless)&lt;br /&gt;
| /p/ || /t~θ/ &#039;&#039;&#039;t&#039;&#039;&#039; || || /k/ &lt;br /&gt;
|-&lt;br /&gt;
! Stop (voiced)&lt;br /&gt;
| /b/ || /d~ð/ &#039;&#039;&#039;d&#039;&#039;&#039; || || /g~ɣ̞/ &lt;br /&gt;
|-&lt;br /&gt;
! Fricative (voiceless)&lt;br /&gt;
| /f/ || /s/ || /ʃ/ &#039;&#039;&#039;x&#039;&#039;&#039; || /x~h~ɦ/ &#039;&#039;&#039;h&#039;&#039;&#039; &lt;br /&gt;
|-&lt;br /&gt;
! Fricative (voiced)&lt;br /&gt;
| /v/ || /z/ || /ʒ/ &#039;&#039;&#039;zh&#039;&#039;&#039; || &lt;br /&gt;
|-&lt;br /&gt;
! Affricate &lt;br /&gt;
| || || /tʃ/ &#039;&#039;&#039;c&#039;&#039;&#039;  || &lt;br /&gt;
|-&lt;br /&gt;
! Affricate&lt;br /&gt;
| || || /dʒ/ &#039;&#039;&#039;ǧ&#039;&#039;&#039; ||&lt;br /&gt;
|-&lt;br /&gt;
! Lateral approximant&lt;br /&gt;
| || /l/ || /ʎ/ &#039;&#039;&#039;ll&#039;&#039;&#039; || &lt;br /&gt;
|-&lt;br /&gt;
! Approximant &lt;br /&gt;
| || /ɾ/ &#039;&#039;&#039;r&#039;&#039;&#039; || /ʝ/ &#039;&#039;&#039;j&#039;&#039;&#039; || &lt;br /&gt;
|-&lt;br /&gt;
! Trill&lt;br /&gt;
| || /r/ &#039;&#039;&#039;rr&#039;&#039;&#039; || || &lt;br /&gt;
|}&lt;br /&gt;
Voicing spreads in consonant cluster, and is usually written.  &#039;&#039;&#039;h&#039;&#039;&#039; voices intervocalically.  Men tend to velarize it as /x/, while /h/ is typically viewed as more feminine.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;text-align: center&amp;quot;&lt;br /&gt;
|+ Koǧan Vowel Phonemes&lt;br /&gt;
! Height \ Backness || Front || Central || Back&lt;br /&gt;
|-&lt;br /&gt;
! High&lt;br /&gt;
| /i/ || || /u/&lt;br /&gt;
|-&lt;br /&gt;
! Mid-high (close-mid)&lt;br /&gt;
| /e/ || (/ǝ/) || /o/&lt;br /&gt;
|-&lt;br /&gt;
! Mid-low (open-mid)&lt;br /&gt;
| /ɛ/ &#039;&#039;&#039;è&#039;&#039;&#039; || || /ɔ/ &#039;&#039;&#039;ò&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Low&lt;br /&gt;
| colspan=&amp;quot;3&amp;quot; | /a/&lt;br /&gt;
|}&lt;br /&gt;
Schwa is found in rushed speech and apocopated syllables.&lt;br /&gt;
&lt;br /&gt;
=== Traits ===&lt;br /&gt;
Aragonese has many historical traits in common with Catalan and Aragonese. Some are conservative features that are also shared with the Asturleonese languages and Galician–Portuguese, where Spanish innovated in ways that did not spread to nearby languages.  It also has many conservative vocabulary items in common with Sardinian.&lt;br /&gt;
&lt;br /&gt;
* Romance initial &#039;&#039;f-&#039;&#039; is preserved, e.g. &#039;&#039;fīlium&#039;&#039; &amp;gt; &#039;&#039;fillo&#039;&#039; (&#039;son&#039;, Sp. &#039;&#039;hijo&#039;&#039;, Cat. &#039;&#039;fill&#039;&#039;, Pt. &#039;&#039;filho&#039;&#039;).&lt;br /&gt;
* &#039;&#039;cl-&#039;&#039;, &#039;&#039;fl-&#039;&#039;, &#039;&#039;pl-&#039;&#039; are never preserved, becoming &#039;&#039;zh-&#039;&#039;, &#039;&#039;x-&#039;&#039;, &#039;&#039;br-&#039;&#039;.&lt;br /&gt;
* Romance palatal approximant (&#039;&#039;ge-&#039;&#039;, &#039;&#039;gi-&#039;&#039;, &#039;&#039;i-&#039;&#039;) consistently became medieval [ʒ], unlike medieval Catalan and Portuguese.&lt;br /&gt;
* Romance groups &#039;&#039;-lt-&#039;&#039;, &#039;&#039;-ct-&#039;&#039; result in [jt], e.g. &#039;&#039;factum&#039;&#039; &amp;gt; &#039;&#039;fèjto&#039;&#039; (&#039;done&#039;, Sp. &#039;&#039;hecho&#039;&#039;, Cat. &#039;&#039;fet&#039;&#039;, Gal./Port. &#039;&#039;feito&#039;&#039;), &#039;&#039;multum&#039;&#039; &amp;gt; &#039;&#039;mwito&#039;&#039; (&#039;many, much&#039;, Sp. &#039;&#039;mucho&#039;&#039;, Cat. &#039;&#039;molt&#039;&#039;, Gal. &#039;&#039;moito&#039;&#039;, Port. &#039;&#039;muito&#039;&#039;).&lt;br /&gt;
* Romance groups &#039;&#039;-x-&#039;&#039;, &#039;&#039;-ps-&#039;&#039;, &#039;&#039;scj-&#039;&#039; result in voiceless palatal fricative &#039;&#039;&#039;sj&#039;&#039; [ʃ], e.g. &#039;&#039;coxu&#039;&#039; &amp;gt; &#039;&#039;koxo&#039;&#039; (&#039;crippled&#039;, Sp. cojo, Cat. coix), &#039;&#039;ipse&#039;&#039; &amp;gt; &#039;&#039;èxe&#039;&#039;, &#039;&#039;scientia&#039;&#039; &amp;gt; &#039;&#039;exènca&#039;&#039;.&lt;br /&gt;
* Romance groups &#039;&#039;-lj-&#039;&#039;, &#039;&#039;-c&#039;l-&#039;&#039;, &#039;&#039;-t&#039;l-&#039;&#039; result in palatal lateral &#039;&#039;lj&#039;&#039; [ʎ], e.g. &#039;&#039;muliere&#039;&#039; &amp;gt; &#039;&#039;muller&#039;&#039; (&#039;woman&#039;, Sp. &#039;&#039;mujer&#039;&#039;, Cat. &#039;&#039;muller&#039;&#039;), &#039;&#039;acuc&#039;la&#039;&#039; &amp;gt; &#039;&#039;agulla&#039;&#039; (&#039;needle&#039;, Sp. &#039;&#039;aguja&#039;&#039;, Cat. &#039;&#039;agulla&#039;&#039;).&lt;br /&gt;
* Open &#039;&#039;o&#039;&#039;, &#039;&#039;e&#039;&#039; from Romance result systematically in diphthongs [we], [je], e.g. &#039;&#039;vet&#039;la&#039;&#039; &amp;gt; &#039;&#039;vièlla&#039;&#039; (&#039;old woman&#039;, Sp. &#039;&#039;vieja&#039;&#039;, Cat. &#039;&#039;vella&#039;&#039;, Pt. &#039;&#039;velha&#039;&#039;). This includes before a palatal approximant, e.g. &#039;&#039;octō&#039;&#039; &amp;gt; &#039;&#039;wèjto&#039;&#039; (&#039;eight&#039;, Sp. &#039;&#039;ocho&#039;&#039;, Cat. &#039;&#039;vuit&#039;&#039;, Pt. &#039;&#039;oito&#039;&#039;). Spanish diphthongizes except before yod, whereas Catalan only diphthongizes before yod.  Koǧan is unique in the uniformity of these changes.&lt;br /&gt;
* Voiced stops /b, d, ɡ/ lenite to approximants [β, ð, ɣ] intervocalically.&lt;br /&gt;
* Loss of neither final unstressed &#039;&#039;-e&#039;&#039; nor &#039;&#039;-o&#039;&#039;, e.g. &#039;&#039;grande&#039;&#039; &amp;gt; &#039;&#039;grande&#039;&#039; (&#039;big&#039;), &#039;&#039;factum&#039;&#039; &amp;gt; &#039;&#039;fèjto&#039;&#039; (&#039;done&#039;). Catalan loses both &#039;&#039;-e&#039;&#039; and &#039;&#039;-o&#039;&#039; (Cat. &#039;&#039;gran&#039;&#039;, &#039;&#039;fet&#039;&#039;); Spanish preserves &#039;&#039;-o&#039;&#039; and sometimes &#039;&#039;-e&#039;&#039; (Sp. &#039;&#039;hecho&#039;&#039;, &#039;&#039;gran ~ grande&#039;&#039;).  Aragonese loses &#039;&#039;-e&#039;&#039; but not &#039;&#039;-o&#039;&#039;.&lt;br /&gt;
* Unlike Spanish and Aragonese, voiced sibilants do not become voiceless.&lt;br /&gt;
* The palatal /j/ is often realized as a fricative [ʝ].&lt;br /&gt;
* Latin &#039;&#039;-b-&#039;&#039; became &#039;&#039;-v-&#039;&#039; in past imperfect endings of verbs of the second and third conjugations: &#039;&#039;teneva&#039;&#039;, &#039;&#039;teniva&#039;&#039; (&#039;he had&#039;, Sp. &#039;&#039;tenía&#039;&#039;, Cat. &#039;&#039;tenia&#039;&#039;), &#039;&#039;dormiva&#039;&#039; (&#039;he was sleeping&#039;, Sp. &#039;&#039;dormía&#039;&#039;, Cat. &#039;&#039;dormia&#039;&#039;).&lt;br /&gt;
* Voicing of many intervocalic stop consonants, e.g. &#039;&#039;cletam&#039;&#039; &amp;gt; &#039;&#039;zheda&#039;&#039; (&#039;sheep hurdle&#039;, Cat. &#039;&#039;cleda&#039;&#039;, Fr. &#039;&#039;claie&#039;&#039;), &#039;&#039;cuculliatam&#039;&#039; &amp;gt; &#039;&#039;koguljada&#039;&#039; (&#039;crested lark&#039;, Sp. &#039;&#039;cogujada&#039;&#039;, Cat. &#039;&#039;cogullada&#039;&#039;).&lt;br /&gt;
* Latin geminate &#039;&#039;-ll-&#039;&#039; became [ʎ].&lt;br /&gt;
* Initial [r] is trilled.  Latin geminate [rr] is also preserved.&lt;br /&gt;
* Latin [nn] and [ni] became ñ.&lt;br /&gt;
* Like English and unlike Spanish, word-final vowels followed by word-initial vowels get a glottal stop inserted.&lt;br /&gt;
&lt;br /&gt;
Stress is assumed to be penultimate.  Other locations are marked with an acute.&lt;br /&gt;
&lt;br /&gt;
== Nouns ==&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Gender !! Markers !! Examples !! Notes&lt;br /&gt;
|-&lt;br /&gt;
| Masculine      || -ò, -e    || librò, kwò   || Default for most Latin-derived nouns      &lt;br /&gt;
|-&lt;br /&gt;
| Feminine       || -a, -è       || taza, mira || Inherited from Latin -a and Arabic -ah&lt;br /&gt;
|-&lt;br /&gt;
| Ambiguous/loan || -consonant || saxan, xiber, kativ   || Gender marked only via articles/clitics   &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
== Plural Formation ==&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Singular Ending !! Plural Ending !! Example (Sing.) !! Example (Pl.) !! Notes&lt;br /&gt;
|-&lt;br /&gt;
| Vowel (a, e, ò, è, o, u) || -s || taza || tazas || Add -s directly to vowel-final nouns&lt;br /&gt;
|-&lt;br /&gt;
| Consonant || -es || saxan || saxanes || Insert epenthetic -e- for ease of pronunciation&lt;br /&gt;
|-&lt;br /&gt;
| Irregular || Varies || midraxa || midraxot || Certain inherited or borrowed nouns are irregular&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Articles ===&lt;br /&gt;
&lt;br /&gt;
==== Definite Articles ====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Gender !! Singular !! Plural !! Etymology/Notes&lt;br /&gt;
|-&lt;br /&gt;
| Masculine || al || als || Arabic &#039;&#039;al-&#039;&#039; + Romance plural &#039;&#039;-s&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
| Feminine || la || las || from Latin &#039;&#039;illa&#039;&#039;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==== Indefinite Articles ====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Gender !! Singular !! Plural !! Etymology/Notes&lt;br /&gt;
|-&lt;br /&gt;
| Masculine || un || uns || Latin &#039;&#039;unus&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
| Feminine || una || unas || Latin &#039;&#039;una&#039;&#039;&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;&#039;als&#039;&#039;&#039; and &#039;&#039;&#039;uns&#039;&#039;&#039; tend to assimilate the voicing of the following head now, i.e. /alz/ or /unz/ vs /al̥s/ or /un̥s/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Pronouns ===&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Number !! Person !! Politeness !! Nom. !! Acc. !! Dat. !! Obl. !! Poss. !! Clitic Acc. !! Clitic Dat.&lt;br /&gt;
|-&lt;br /&gt;
! rowspan=&amp;quot;4&amp;quot; | Singular !! 1 !! -&lt;br /&gt;
| zhè || colspan=&amp;quot;2&amp;quot; | me || mi || mi/ma/mes/mas || -me || -mi&lt;br /&gt;
|-&lt;br /&gt;
! 2 !! Informal&lt;br /&gt;
| tu || colspan=&amp;quot;2&amp;quot; | te || ti || ti/ta/tes/tas || -te || -ti &lt;br /&gt;
|-&lt;br /&gt;
! 3m !! -&lt;br /&gt;
| èl || colspan=&amp;quot;2&amp;quot; | so || si || se/sa/ses/sas || -se || -si&lt;br /&gt;
|-&lt;br /&gt;
! 3f !! -&lt;br /&gt;
| èlla || colspan=&amp;quot;2&amp;quot; | lo || li || le/lua/les/luas || -le || li&lt;br /&gt;
|-&lt;br /&gt;
! rowspan=&amp;quot;3&amp;quot; | Plural !! 1 !! -&lt;br /&gt;
| colspan=&amp;quot;2&amp;quot; | nos || colspan=&amp;quot;2&amp;quot; | nov || nòsce/nòca/nòsces/nòscas || -nos || -ni&lt;br /&gt;
|-&lt;br /&gt;
! 2 !! Informal&lt;br /&gt;
| colspan=&amp;quot;2&amp;quot; | vos || colspan=&amp;quot;2&amp;quot; | vov || vèsce/vèsca/vèsces/vèscas || -vos || -vi&lt;br /&gt;
|-&lt;br /&gt;
! 3 !! -&lt;br /&gt;
| èls || colspan=&amp;quot;2&amp;quot; | los || lis || lor/lar/lors/lars || -las || lis&lt;br /&gt;
|-&lt;br /&gt;
! Both !! 2 !! Formal&lt;br /&gt;
| antu || - || lèkum || kum || &#039;&#039;paraph&#039;&#039; || -kum || -ki&lt;br /&gt;
|}&lt;br /&gt;
Two clitics both attaching to a verb is possible.  If there are two, dative always precedes accusative, e.g. &#039;&#039;da-mi-le&#039;&#039; &amp;quot;give me her&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
Another important pronoun is &#039;&#039;&#039;es&#039;&#039;&#039;.  It reflexive without person or number, clitic or independent, dative or accusative.&lt;br /&gt;
&lt;br /&gt;
== Verbs ==&lt;br /&gt;
* -ar class -&amp;gt; active, from -āre, e.g. kantar &#039;to sing&#039;&lt;br /&gt;
* -èr class -&amp;gt; active, from -ēre, e.g. temer &#039;to fear&#039;&lt;br /&gt;
* -ir class -&amp;gt; inchoative, from -īre, e.g. dormir &#039;to sleep&#039;&lt;br /&gt;
* -òr class -&amp;gt; mediopassive, from -or, e.g. moròr &#039;to die&#039;, lavòr &#039;to bathe (oneself)&#039;.  Amazingly, new verbs enter this category, such as &#039;&#039;umidékor&#039;&#039; &amp;quot;to get wet&amp;quot;&lt;br /&gt;
&lt;br /&gt;
For -ar, present indicative active: -o, -as, -a, -am, -ac, -an. &lt;br /&gt;
-èr is -o, -ès, -è, -èm, -èc, -èm.&lt;br /&gt;
-ir is -o, -is, -i, -im, -ic, -im.&lt;br /&gt;
-òr is -o, -us, -u, -um, -uc, -um.  -ò- appears in other stems.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Person !! Present !! Imperfect !! Preterite !! Synthetic Future !! Periphrastic Future&lt;br /&gt;
|-&lt;br /&gt;
| 1sg || kanto || kantèva || kantè || kantarè || avjo kantar&lt;br /&gt;
|-&lt;br /&gt;
| 2sg || kantas || kantèvas || kantàs || kantaràs || avjas kantar&lt;br /&gt;
|-&lt;br /&gt;
| 3sg || kanta || kantèva || kantà || kantarà || avja kantar&lt;br /&gt;
|-&lt;br /&gt;
| 1pl || kantam || kantèvam || kantam || kantarèm || avjam kantar&lt;br /&gt;
|-&lt;br /&gt;
| 2pl || kantac || kantèvac || kantac || kantarèc || avjac kantar&lt;br /&gt;
|-&lt;br /&gt;
| 3pl || kantan || kantèvan || kantàron || kantaràn || avjan kantar&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Person !! Present Subjunctive !! Preterite Subjunctive !! Conditional&lt;br /&gt;
|-&lt;br /&gt;
| 1sg || kantje || kantèse || volria kantar&lt;br /&gt;
|-&lt;br /&gt;
| 2sg || kantjes || kantèses || volrias kantar&lt;br /&gt;
|-&lt;br /&gt;
| 3sg || kantje || kantèse || volria kantar&lt;br /&gt;
|-&lt;br /&gt;
| 1pl || kantjem || kantèsem || volriam kantar&lt;br /&gt;
|-&lt;br /&gt;
| 2pl || kantjec || kantèsec || volriac kantar&lt;br /&gt;
|-&lt;br /&gt;
| 3pl || kantjen || kantèsen || volrian kantar&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
* 2sg: kanta!&lt;br /&gt;
* 2pl: kantac!&lt;br /&gt;
* 3sg: kantje!&lt;br /&gt;
* 3pl: kantan! (or kantjen!&lt;br /&gt;
* Negative forms use subjunctive:&lt;br /&gt;
** non kantjes&lt;br /&gt;
** non kantjec&lt;br /&gt;
** non kantje&lt;br /&gt;
** non kantjen&lt;br /&gt;
&lt;br /&gt;
* Infinitive: kantar&lt;br /&gt;
* Past participle: kantat&lt;br /&gt;
* Gerund: kantant&lt;br /&gt;
* Present participle: kantanto (used adjectivally)&lt;br /&gt;
* Perfect participle: kantat&lt;br /&gt;
&lt;br /&gt;
== Grammar ==&lt;br /&gt;
SVO, except in formal register VSO&lt;br /&gt;
&lt;br /&gt;
== Sound Changes ==&lt;br /&gt;
Stress followed Latin rules: penultimate if heavy, otherwise antepenultimate.  Write latin c as k.  Write latin qu as kw.&lt;br /&gt;
&lt;br /&gt;
Vowels&lt;br /&gt;
* a,ā -&amp;gt; a&lt;br /&gt;
* e -&amp;gt; è&lt;br /&gt;
* ē -&amp;gt; e&lt;br /&gt;
* o -&amp;gt; ò&lt;br /&gt;
* ō -&amp;gt; o&lt;br /&gt;
* ī, i -&amp;gt; i&lt;br /&gt;
* ū, u -&amp;gt; u&lt;br /&gt;
* &#039;è -&amp;gt; jè (stressed)&lt;br /&gt;
* &#039;ò -&amp;gt; wè (stressed)&lt;br /&gt;
&lt;br /&gt;
Palatalization&lt;br /&gt;
* li,ll -&amp;gt; ll&lt;br /&gt;
* di, de -&amp;gt; ǧ&lt;br /&gt;
* tiV, teV -&amp;gt; cV&lt;br /&gt;
* trV -&amp;gt; cV&lt;br /&gt;
* drV -&amp;gt; ǧV&lt;br /&gt;
* lt -&amp;gt; jt&lt;br /&gt;
* gn -&amp;gt; ñ&lt;br /&gt;
* cl -&amp;gt; zh&lt;br /&gt;
* ViV -&amp;gt; VzhV&lt;br /&gt;
* fl -&amp;gt; x&lt;br /&gt;
* gl -&amp;gt; ll&lt;br /&gt;
&lt;br /&gt;
Lenition&lt;br /&gt;
* V[bdg]V -&amp;gt; V[vðh]V (not written for ð)&lt;br /&gt;
* V[ptk]V -&amp;gt; V[bdg]V &lt;br /&gt;
* medial kw -&amp;gt; xw&lt;br /&gt;
* initial and medial ß -&amp;gt; gw&lt;br /&gt;
&lt;br /&gt;
Cluster&lt;br /&gt;
* pl -&amp;gt; br&lt;br /&gt;
* kr stays&lt;br /&gt;
* de-geminate all except rr, ll&lt;br /&gt;
* skr -&amp;gt; ehw&lt;br /&gt;
* sp -&amp;gt; esp&lt;br /&gt;
* str -&amp;gt; ec&lt;br /&gt;
* st -&amp;gt; est&lt;br /&gt;
&lt;br /&gt;
rhotic&lt;br /&gt;
* initial r -&amp;gt; rr&lt;br /&gt;
* [lns]r -&amp;gt; [lns]rr (and old geminates)&lt;br /&gt;
&lt;br /&gt;
Late&lt;br /&gt;
* snobs say ʁ instead of r&lt;br /&gt;
* Arabic ð written dh&lt;br /&gt;
* Arabic ṯ written th&lt;br /&gt;
&lt;br /&gt;
== Passages ==&lt;br /&gt;
=== North Wind ===&lt;br /&gt;
* La Tramutaña j&#039;al Sol kontendègwan kwo de èls era mazhòr.&lt;br /&gt;
&lt;br /&gt;
=== Rerum Novarum ===&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Language !! Text&lt;br /&gt;
|-&lt;br /&gt;
| Latin || Salutem et Apostolicam Benedictionem.  Rerum novarum semel excitata cupiditate, quae diu societatem commovit, illud fere consequens erat, ut hominum mentes ad res novas cogitationes appellerentur: unde factum est ut ex una parte homines, qui opibus praestarent, eas veluti ius suum esse contenderent, nulla in re aut divino aut humano iuri obnoxias; ex altera vero parte ut opifices, inopia et duriore condicione pressati, id unum quaererent, ut se ab eiusmodi servitute omnino expediant. Quae res eos, vel invita, in easdem sententias et consilia impulerunt, quae socialismi nomine vulgo appellantur; siquidem facilius est animis eorum persuadere, eas opes, quae iniquitate et iniuria coacervatae sint, ita in commune deduci posse, ut iis, qui nulla re praediti sint, pro sua parte prosint.  Verum haec omnia, quae hucusque a socialistis proposita sunt, tametsi in speciem alliciant, nihil aliud ostendunt, nisi falsas rationes et inefficaces ad id, quod spectant; immo vero talia remedia longe peiora sunt morbis, quae sanare velle videntur.&lt;br /&gt;
|-&lt;br /&gt;
| Spanish || Salud y Bendición Apostólica.  Una vez despertado el deseo de cosas nuevas, que desde hace tiempo agita a la sociedad, era casi inevitable que los ánimos de los hombres se inclinaran hacia nuevas ideas: de aquí resultó que, por una parte, los que poseían riquezas las defendieran como si fueran un derecho suyo, no sujeto en nada a la ley divina ni humana; y por otra, que los obreros, oprimidos por la miseria y una condición más dura, solo buscaran librarse completamente de tal servidumbre. Esto los llevó, incluso contra su voluntad, a abrazar aquellas opiniones y proyectos que comúnmente se llaman socialismo; pues es más fácil persuadir a sus almas que esas riquezas, acumuladas por la iniquidad y la injusticia, podrían distribuirse en común para beneficiar, según su parte, a aquellos que nada poseen.  Pero todas estas propuestas de los socialistas, aunque parezcan atractivas a primera vista, no muestran más que razones falsas e ineficaces para lograr su propósito; antes bien, tales remedios son mucho peores que los males que pretenden curar.&lt;br /&gt;
|-&lt;br /&gt;
| &#039;&#039;Catalan&#039;&#039; || Salut i Benedicció Apostòlica.  Una vegada despertada la set de coses noves, que fa temps que agita la societat, era gairebé inevitable que els ànims dels homes es decantessin cap a noves idees: d’aquí va resultar que, d’una banda, els qui posseïen riqueses les defensessin com si fossin un dret seu, no sotmès a cap llei divina ni humana; i de l’altra, que els treballadors, oprimits per la misèria i una condició més dura, només cerquessin alliberar-se completament d’aquesta servitud. Això els va portar, fins i tot contra la seva voluntat, a abraçar aquelles opinions i projectes que s’anomenen comunament socialisme; perquè és més fàcil convèncer els seus esperits que aquestes riqueses, acumulades amb iniquitat i injustícia, podrien repartir-se en comú per beneficiar, segons la seva part, els qui no tenen res.&lt;br /&gt;
|-&lt;br /&gt;
| Italian || Salute e Benedizione Apostolica.  Una volta suscitata la brama di cose nuove, che da tempo turba la società, era quasi inevitabile che gli animi degli uomini si volgessero a nuove idee: ne è derivato che, da una parte, coloro che possedevano ricchezze le rivendicassero come un loro diritto, non soggetto in nulla alla legge divina o umana; dall’altra, che i lavoratori, oppressi dalla miseria e da una condizione più dura, cercassero unicamente di liberarsi completamente da tale servitù. Ciò li ha spinti, anche contro la loro volontà, ad abbracciare quelle opinioni e quei progetti che vengono comunemente chiamati socialismo; poiché è più facile persuadere le loro menti che tali ricchezze, accumulate con iniquità e ingiustizia, possano essere distribuite in comune, così da giovare, secondo la loro parte, a coloro che nulla possiedono.  Ma tutte queste proposte dei socialisti, benché a prima vista sembrino allettanti, non dimostrano altro che ragionamenti falsi e inefficaci per il fine che si propongono; anzi, tali rimedi sono di gran lunga peggiori dei mali che pretendono di sanare.&lt;br /&gt;
|-&lt;br /&gt;
| Kodzjan || Salut i Benedikzhon Apostòlika.  Una gwegada despertat al xok de kosas nwèvas, kwe fa tèm agita la soxedat, èra kwazi inegwitabile kwe las animas dals òmes se gwolvòsen verz unas idèzhas nwevas:&lt;br /&gt;
&lt;br /&gt;
|}&lt;br /&gt;
# [[Koǧan/Swadesh]]&lt;br /&gt;
{{Aquatiki}}&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=Ko%C7%A7an/218&amp;diff=170969</id>
		<title>Koǧan/218</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=Ko%C7%A7an/218&amp;diff=170969"/>
		<updated>2025-05-25T14:16:38Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: Created page with &amp;quot;# Al sol brillazh. # Al sol èzh brillant. # Al sol brillázh. # Al sol brillarázh. # Al sol azh estat brillant. # Al sol èzh brillant xuv. # Al sol brillarázh kras. # Al sol brillazh kòn fwèrca. # Al sol luzhònte brillazh. # Al sol esta naxint lan.&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;# Al sol brillazh.&lt;br /&gt;
# Al sol èzh brillant.&lt;br /&gt;
# Al sol brillázh.&lt;br /&gt;
# Al sol brillarázh.&lt;br /&gt;
# Al sol azh estat brillant.&lt;br /&gt;
# Al sol èzh brillant xuv.&lt;br /&gt;
# Al sol brillarázh kras.&lt;br /&gt;
# Al sol brillazh kòn fwèrca.&lt;br /&gt;
# Al sol luzhònte brillazh.&lt;br /&gt;
# Al sol esta naxint lan.&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=Ko%C7%A7an&amp;diff=170923</id>
		<title>Koǧan</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=Ko%C7%A7an&amp;diff=170923"/>
		<updated>2025-05-24T17:14:03Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: Created page with &amp;quot;{| class=&amp;quot;wikitable&amp;quot; ! Aspect !! Details |- ! Name | *Caudia*, from Latin *cauda* &amp;quot;tail&amp;quot; — a metaphor for “tail-end” of Latinity           |- ! Location | Southeast of the Balearics, equidistant from Ibiza, Algiers, and Cagliari |- ! Size  | Roughly 120 km long, mountainous interior, coastal plains  |- ! Geological Origin |  Volcanic + limestone; freshwater aquifers, arable valleys |- ! Climate | Mediterranean; olive, fig, almond, and cereal agriculture |- !  Histo...&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Aspect !! Details&lt;br /&gt;
|-&lt;br /&gt;
! Name&lt;br /&gt;
| *Caudia*, from Latin *cauda* &amp;quot;tail&amp;quot; — a metaphor for “tail-end” of Latinity          &lt;br /&gt;
|-&lt;br /&gt;
! Location&lt;br /&gt;
| Southeast of the Balearics, equidistant from Ibiza, Algiers, and Cagliari&lt;br /&gt;
|-&lt;br /&gt;
! Size &lt;br /&gt;
| Roughly 120 km long, mountainous interior, coastal plains &lt;br /&gt;
|-&lt;br /&gt;
! Geological Origin&lt;br /&gt;
|  Volcanic + limestone; freshwater aquifers, arable valleys&lt;br /&gt;
|-&lt;br /&gt;
! Climate&lt;br /&gt;
| Mediterranean; olive, fig, almond, and cereal agriculture&lt;br /&gt;
|-&lt;br /&gt;
!  Historical Timeline&lt;br /&gt;
| Phoenician colony, Muslim conquest, Cordoban/Andalusian territory, later than Reconquista, &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Koǧa was part of the Caliphate of Córdoba from early on and developed as an exceptionally tolerant multicultural haven, offering the greatest protection and coexistence for Jews and Christians anywhere in the empire.  Extended exposure to Classical Arabic, not merely rural dialects. Jewish linguistic influence (e.g., Hebrew calques, Semitic syntax transfers, or Judeo-Romance variants). Christian Latin continuity via protected ecclesiastical communities and monastic scribes. An intellectual center for translation, scientific synthesis, and lexical borrowing in philosophy, agriculture, medicine, and jurisprudence.&lt;br /&gt;
&lt;br /&gt;
== Historical Background of Caudia ==&lt;br /&gt;
&lt;br /&gt;
The island of Caudia (endonym: Koǧa) occupies a unique position in the Romance-speaking world. Located in the western Mediterranean, equidistant from Ibiza, Algiers, and Cagliari, Caudia developed in partial isolation yet maintained sustained maritime contact with several major cultural centers. Its linguistic history reflects a sequence of layered influences, beginning with Roman colonization and extending through a complex legacy of religious, political, and intellectual exchange. The result is a Romance language of singular character, deeply shaped by Semitic and Hellenistic overlays, yet structurally descended from Vulgar Latin.&lt;br /&gt;
&lt;br /&gt;
=== I. Late Roman and Early Post-Roman Period ===&lt;br /&gt;
&lt;br /&gt;
During the late Roman Empire, Caudia was settled by a community of Latin-speaking provincials with strong ties to the eastern Mediterranean. Archaeological and textual evidence suggest that the early Caudian population may have included a substantial Jewish demographic, either as voluntary migrants or as resettled populations following the destruction of the Second Temple and later Roman crackdowns. These settlers brought with them not only Latin but also a background in Koine Greek, Hebrew, and the legalistic registers of Classical education.&lt;br /&gt;
&lt;br /&gt;
The variety of Latin spoken on Caudia diverged early from continental Vulgar Latin. While it maintained the phonological shifts typical of spoken Latin (e.g., syncope, monophthongization), the syntactic and lexical profile of early Caudian Latin bore traces of its learned origins:&lt;br /&gt;
&lt;br /&gt;
* Lexical borrowings from Greek and Hebrew entered at an early stage.&lt;br /&gt;
* Certain Classical Latin archaisms, particularly in legal and rhetorical constructions, were preserved in fossilized forms.&lt;br /&gt;
* Syntax exhibited conservatism in verbal periphrases and pronoun usage, possibly influenced by scriptural Hebrew and ecclesiastical Latin.&lt;br /&gt;
&lt;br /&gt;
This substratum, referred to by linguists as Proto-Koǧan, laid the foundation for later development. It is best viewed as a peripheral but not isolated offshoot of Proto-Romance, exhibiting both conservatism and early hybridization.&lt;br /&gt;
&lt;br /&gt;
=== II. Islamic Period: Integration into al-Andalus ===&lt;br /&gt;
&lt;br /&gt;
In the early 8th century CE, Caudia was absorbed into the expanding Umayyad Caliphate, and subsequently became an overseas dependency of the Emirate, later Caliphate, of Córdoba. Owing to its small size and strategic position, Caudia functioned less as a military outpost and more as an intellectual and mercantile enclave. Its ports hosted traders, translators, and jurists; its inland monasteries and zawiyas (زوايا) became centers of scholarship and religious dialogue.&lt;br /&gt;
&lt;br /&gt;
During this period, Caudia acquired a reputation for exceptional religious tolerance. Jewish, Christian, and Muslim communities coexisted under the relatively lenient dhimmi system, with Jewish communities in particular enjoying a degree of autonomy and prestige rarely matched elsewhere in the Islamic world. Koǧan oral traditions record this period as a &amp;quot;golden age&amp;quot; of letters.&lt;br /&gt;
&lt;br /&gt;
The impact on the language was profound:&lt;br /&gt;
* Arabic loanwords entered in significant numbers, particularly in domains such as philosophy, jurisprudence, medicine, agriculture, architecture, and administration.&lt;br /&gt;
* Unlike Iberian Romance languages, Arabic borrowings were typically adopted without the definite article al-, a sign of the Caudians’ familiarity with Arabic morphology and semantics. Thus, mufada (pillow) rather than almufada, or zawija (monastery) rather than alzawija.&lt;br /&gt;
* Arabic borrowings were often morphologically integrated into native derivational patterns, and show consistent phonological adaptation to Koǧan phonotactics.&lt;br /&gt;
* The variety of Arabic spoken on the island was closer to Classical Arabic (fuṣḥā) than to Maghrebi vernaculars, further differentiating Caudian Arabic from that of the Iberian Peninsula.&lt;br /&gt;
&lt;br /&gt;
This period also witnessed the rise of Caudia as a translation center, where Hebrew exegetes, Latin scribes, and Arabic philosophers worked in tandem to produce multilingual treatises. This tri-scriptural culture left a permanent imprint on Koǧan lexicon and discourse style.&lt;br /&gt;
&lt;br /&gt;
=== III. Post-Andalusian Period: Semi-Autonomous Continuity ===&lt;br /&gt;
&lt;br /&gt;
The island&#039;s relationship to the Christian Reconquista was anomalous. While Caudia formally came under the suzerainty of various Christian polities (at various times Pisa, Aragon, or Genoa), it was rarely subjected to direct ecclesiastical or military control. As such, Caudia remained culturally hybrid, and retained both Arabic and Hebrew institutions long after their suppression on the mainland.&lt;br /&gt;
&lt;br /&gt;
During this period, Latin liturgical practices reasserted themselves, particularly in coastal cathedrals and episcopal centers. However, these coexisted with enduring Muslim and Jewish communities. The vernacular Koǧan language became the principal vehicle of interfaith communication, absorbing and transmitting the philosophical, legal, and agricultural terminologies of the three traditions.&lt;br /&gt;
&lt;br /&gt;
The linguistic consequences included:&lt;br /&gt;
* Continued but more selective lexical borrowing from Latin and emerging Ibero-Romance varieties.&lt;br /&gt;
* Increased semantic specialization in loanwords — e.g., Arabic terms retained specific technical senses.&lt;br /&gt;
* Preservation of older grammatical constructions due to textual conservatism in religious and legal documents.&lt;br /&gt;
* Emergence of a prestige dialect among urban literati, with phonological hypercorrections and borrowings from ecclesiastical Latin.&lt;br /&gt;
&lt;br /&gt;
=== IV. Linguistic Summary ===&lt;br /&gt;
&lt;br /&gt;
The Koǧan language as it exists today is thus the product of a deeply stratified linguistic ecology, in which:&lt;br /&gt;
* Proto-Romance provides the grammatical skeleton.&lt;br /&gt;
* Classical Latin and Koine Greek supply archaisms and syntactic conservatism.&lt;br /&gt;
* Hebrew contributes both lexical items and subtle syntactic calques, particularly in parallelism and discourse structure.&lt;br /&gt;
* Arabic offers a rich stratum of vocabulary and intellectual idioms, stripped of folk transmission markers such as definite articles.&lt;br /&gt;
* Ecclesiastical Latin in the post-Reconquista era reaffirms certain nominal and participial structures in formal contexts.&lt;br /&gt;
&lt;br /&gt;
The resulting language is Romance at its core, but notably non-European in its evolution — a Romance language that grew up not under the shadow of Charlemagne or Castile, but under the dome of Córdoba and the scrolls of Tiberias.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Phonology ==&lt;br /&gt;
Forms that differ from IPA are shown in bold.  Most allophony occurs intervocalically.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;text-align: center&amp;quot;&lt;br /&gt;
|+ Koǧan Consonant Phonemes&lt;br /&gt;
! Manner \ Place || Labial || Alveolar || Palatal || Velar &lt;br /&gt;
|-&lt;br /&gt;
! Nasal&lt;br /&gt;
| /m/ || /n || /ɲ/ &#039;&#039;&#039;ñ&#039;&#039;&#039; || &lt;br /&gt;
|-&lt;br /&gt;
! Stop (voiceless)&lt;br /&gt;
| /p/ || /t~θ/ &#039;&#039;&#039;t&#039;&#039;&#039; || || /k/ &lt;br /&gt;
|-&lt;br /&gt;
! Stop (voiced)&lt;br /&gt;
| /b/ || /d~ð/ &#039;&#039;&#039;d&#039;&#039;&#039; || || /g~ɣ̞/ &lt;br /&gt;
|-&lt;br /&gt;
! Fricative (voiceless)&lt;br /&gt;
| /f/ || /s/ || /ʃ/ &#039;&#039;&#039;x&#039;&#039;&#039; || /x~h/ &#039;&#039;&#039;h&#039;&#039;&#039; &lt;br /&gt;
|-&lt;br /&gt;
! Fricative (voiced)&lt;br /&gt;
| /v/ || /z/ || /ʒ/ &#039;&#039;&#039;zh&#039;&#039;&#039; || &lt;br /&gt;
|-&lt;br /&gt;
! Affricate &lt;br /&gt;
| || || /tʃ/ &#039;&#039;&#039;c&#039;&#039;&#039;  || &lt;br /&gt;
|-&lt;br /&gt;
! Affricate&lt;br /&gt;
| || || /dʒ/ &#039;&#039;&#039;ǧ&#039;&#039;&#039; ||&lt;br /&gt;
|-&lt;br /&gt;
! Lateral approximant&lt;br /&gt;
| || /l/ || /ʎ/ &#039;&#039;&#039;ll&#039;&#039;&#039; || &lt;br /&gt;
|-&lt;br /&gt;
! Approximant &lt;br /&gt;
| || /ɾ/ &#039;&#039;&#039;r&#039;&#039;&#039; || /ʝ/ &#039;&#039;&#039;j&#039;&#039;&#039; || &lt;br /&gt;
|-&lt;br /&gt;
! Trill&lt;br /&gt;
| || /r/ &#039;&#039;&#039;rr&#039;&#039;&#039; || || &lt;br /&gt;
|}&lt;br /&gt;
Voicing spreads in consonant cluster, and is usually written.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;text-align: center&amp;quot;&lt;br /&gt;
|+ Koǧan Vowel Phonemes&lt;br /&gt;
! Height \ Backness || Front || Central || Back&lt;br /&gt;
|-&lt;br /&gt;
! High&lt;br /&gt;
| /i/ || || /u/&lt;br /&gt;
|-&lt;br /&gt;
! Mid-high (close-mid)&lt;br /&gt;
| /e/ || (/ǝ/) || /o/&lt;br /&gt;
|-&lt;br /&gt;
! Mid-low (open-mid)&lt;br /&gt;
| /ɛ/ &#039;&#039;&#039;è&#039;&#039;&#039; || || /ɔ/ &#039;&#039;&#039;ò&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Low&lt;br /&gt;
| colspan=&amp;quot;3&amp;quot; | /a/&lt;br /&gt;
|}&lt;br /&gt;
Schwa is found in rushed speech and apocopated syllables.&lt;br /&gt;
&lt;br /&gt;
=== Traits ===&lt;br /&gt;
Aragonese has many historical traits in common with Catalan and Aragonese. Some are conservative features that are also shared with the Asturleonese languages and Galician–Portuguese, where Spanish innovated in ways that did not spread to nearby languages.  It also has many conservative vocabulary items in common with Sardinian.&lt;br /&gt;
&lt;br /&gt;
* Romance initial &#039;&#039;f-&#039;&#039; is preserved, e.g. &#039;&#039;fīlium&#039;&#039; &amp;amp;gt; &#039;&#039;fillo (&#039;son&#039;, Sp. &#039;&#039;hijo&#039;&#039;, Cat. &#039;&#039;fill&#039;&#039;, Pt. &#039;&#039;filho&#039;&#039;).&lt;br /&gt;
* &#039;&#039;cl-&#039;&#039;, &#039;&#039;fl-&#039;&#039;, &#039;&#039;pl-&#039;&#039; are never preserved, becoming &#039;&#039;zh-&#039;&#039;, &#039;&#039;x-&#039;&#039;, &#039;&#039;br-&#039;&#039;.&lt;br /&gt;
* Romance palatal approximant (&#039;&#039;ge-&#039;&#039;, &#039;&#039;gi-&#039;&#039;, &#039;&#039;i-&#039;&#039;) consistently became medieval [ʒ], unlikely medieval Catalan and Portuguese.&lt;br /&gt;
* Romance groups &#039;&#039;-lt-&#039;&#039;, &#039;&#039;-ct-&#039;&#039; result in [jt], e.g. &#039;&#039;factum&#039;&#039; &amp;amp;gt; &#039;&#039;fèjto&#039;&#039; (&#039;done&#039;, Sp. &#039;&#039;hecho&#039;&#039;, Cat. &#039;&#039;fet&#039;&#039;, Gal./Port. &#039;&#039;feito&#039;&#039;), &#039;&#039;multum&#039;&#039; &amp;amp;gt; &#039;&#039;mwito&#039;&#039; (&#039;many, much&#039;, Sp. &#039;&#039;mucho&#039;&#039;, Cat. &#039;&#039;molt&#039;&#039;, Gal. &#039;&#039;moito&#039;&#039;, Port. &#039;&#039;muito&#039;&#039;).&lt;br /&gt;
* Romance groups &#039;&#039;-x-&#039;&#039;, &#039;&#039;-ps-&#039;&#039;, &#039;&#039;scj-&#039;&#039; result in voiceless palatal fricative &#039;&#039;&#039;sj&#039;&#039; [ʃ], e.g. &#039;&#039;coxu&#039;&#039; &amp;amp;gt; &#039;&#039;coxo&#039;&#039; (&#039;crippled&#039;, Sp. cojo, Cat. coix), &#039;&#039;ipse&#039;&#039; &amp;amp;gt; &#039;&#039;èxe&#039;&#039;, &#039;&#039;scientia&#039;&#039; &amp;amp;gt; &#039;&#039;exènca&#039;&#039;.&lt;br /&gt;
* Romance groups &#039;&#039;-lj-&#039;&#039;, &#039;&#039;-c&#039;l-&#039;&#039;, &#039;&#039;-t&#039;l-&#039;&#039; result in palatal lateral &#039;&#039;lj&#039;&#039; [ʎ], e.g. &#039;&#039;muliere&#039;&#039; &amp;amp;gt; &#039;&#039;muller&#039;&#039; (&#039;woman&#039;, Sp. &#039;&#039;mujer&#039;&#039;, Cat. &#039;&#039;muller&#039;&#039;), &#039;&#039;acuc&#039;la&#039;&#039; &amp;amp;gt; &#039;&#039;agulla&#039;&#039; (&#039;needle&#039;, Sp. &#039;&#039;aguja&#039;&#039;, Cat. &#039;&#039;agulla&#039;&#039;).&lt;br /&gt;
* Open &#039;&#039;o&#039;&#039;, &#039;&#039;e&#039;&#039; from Romance result systematically in diphthongs [we], [je], e.g. &#039;&#039;vet&#039;la&#039;&#039; &amp;amp;gt; &#039;&#039;vièlla&#039;&#039; (&#039;old woman&#039;, Sp. &#039;&#039;vieja&#039;&#039;, Cat. &#039;&#039;vella&#039;&#039;, Pt. &#039;&#039;velha&#039;&#039;). This includes before a palatal approximant, e.g. &#039;&#039;octō&#039;&#039; &amp;amp;gt; &#039;&#039;wèjto&#039;&#039; (&#039;eight&#039;, Sp. &#039;&#039;ocho&#039;&#039;, Cat. &#039;&#039;vuit&#039;&#039;, Pt. &#039;&#039;oito&#039;&#039;). Spanish diphthongizes except before yod, whereas Catalan only diphthongizes before yod.&lt;br /&gt;
* Voiced stops /b, d, ɡ/ lenited to approximants [β, ð, ɣ].  This continues through the present, so it is sometimes written, sometimes not.&lt;br /&gt;
* Loss of neither final unstressed &#039;&#039;-e&#039;&#039; nor &#039;&#039;-o&#039;&#039;, e.g. &#039;&#039;grande&#039;&#039; &amp;amp;gt; &#039;&#039;grande&#039;&#039; (&#039;big&#039;), &#039;&#039;factum&#039;&#039; &amp;amp;gt; &#039;&#039;fèjto&#039;&#039; (&#039;done&#039;). Catalan loses both &#039;&#039;-e&#039;&#039; and &#039;&#039;-o&#039;&#039; (Cat. &#039;&#039;gran&#039;&#039;, &#039;&#039;fet&#039;&#039;); Spanish preserves &#039;&#039;-o&#039;&#039; and sometimes &#039;&#039;-e&#039;&#039; (Sp. &#039;&#039;hecho&#039;&#039;, &#039;&#039;gran ~ grande&#039;&#039;).  Aragonese loses &#039;&#039;-e&#039;&#039; but not &#039;&#039;-o&#039;&#039;.&lt;br /&gt;
* Unlike Spanish and Aragonese, voiced sibilants do not become voiceless.&lt;br /&gt;
* The palatal /j/ is often realized as a fricative [ʝ].&lt;br /&gt;
* Latin &#039;&#039;-b-&#039;&#039; became &#039;&#039;-v-&#039;&#039; in past imperfect endings of verbs of the second and third conjugations: &#039;&#039;teneva&#039;&#039;, &#039;&#039;teniva&#039;&#039; (&#039;he had&#039;, Sp. &#039;&#039;tenía&#039;&#039;, Cat. &#039;&#039;tenia&#039;&#039;), &#039;&#039;dormiva&#039;&#039; (&#039;he was sleeping&#039;, Sp. &#039;&#039;dormía&#039;&#039;, Cat. &#039;&#039;dormia&#039;&#039;).&lt;br /&gt;
* Voicing of many intervocalic stop consonants, e.g. &#039;&#039;cletam&#039;&#039; &amp;amp;gt; &#039;&#039;zjeda&#039;&#039; (&#039;sheep hurdle&#039;, Cat. &#039;&#039;cleda&#039;&#039;, Fr. &#039;&#039;claie&#039;&#039;), &#039;&#039;cuculliatam&#039;&#039; &amp;amp;gt; &#039;&#039;coguljada&#039;&#039; (&#039;crested lark&#039;, Sp. &#039;&#039;cogujada&#039;&#039;, Cat. &#039;&#039;cogullada&#039;&#039;).&lt;br /&gt;
* Latin geminate &#039;&#039;-ll-&#039;&#039; became [ʎ].&lt;br /&gt;
* Initial [r] is trilled.&lt;br /&gt;
&lt;br /&gt;
== Nouns ==&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Gender !! Markers !! Examples !! Notes&lt;br /&gt;
|-&lt;br /&gt;
| Masculine      || -ò, -e    || librò, kwò   || Default for most Latin-derived nouns      &lt;br /&gt;
|-&lt;br /&gt;
| Feminine       || -a, -è       || taza, mira || Inherited from Latin -a and Arabic -ah&lt;br /&gt;
|-&lt;br /&gt;
| Ambiguous/loan || -consonant || saxan, xiber, kativ   || Gender marked only via articles/clitics   &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
== Plural Formation ==&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Singular Ending !! Plural Ending !! Example (Sing.) !! Example (Pl.) !! Notes&lt;br /&gt;
|-&lt;br /&gt;
| Vowel (a, e, ò, è, o, u) || -s || taza || tazas || Add -s directly to vowel-final nouns&lt;br /&gt;
|-&lt;br /&gt;
| Consonant || -es || saxan || saxanes || Insert epenthetic -e- for ease of pronunciation&lt;br /&gt;
|-&lt;br /&gt;
| Irregular || Varies || midraxa || midraxot || Certain inherited or borrowed nouns are irregular&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Articles ===&lt;br /&gt;
&lt;br /&gt;
==== Definite Articles ====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Gender !! Singular !! Plural !! Etymology/Notes&lt;br /&gt;
|-&lt;br /&gt;
| Masculine || al || als || Arabic &#039;&#039;al-&#039;&#039; + Romance plural &#039;&#039;-s&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
| Feminine || la || las || from Latin &#039;&#039;illa&#039;&#039;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==== Indefinite Articles ====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Gender !! Singular !! Plural !! Etymology/Notes&lt;br /&gt;
|-&lt;br /&gt;
| Masculine || un || uns || Latin &#039;&#039;unus&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
| Feminine || una || unas || Latin &#039;&#039;una&#039;&#039;&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;&#039;als&#039;&#039;&#039; and &#039;&#039;&#039;uns&#039;&#039;&#039; tend to assimilate the voicing of the following head now, i.e. /alz/ or /unz/ vs /al̥s/ or /un̥s/&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Pronouns ===&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Number !! Person !! Politeness !! Nom. !! Acc. !! Dat. !! Obl. !! Poss. !! Clitic Acc. !! Clitic Dat.&lt;br /&gt;
|-&lt;br /&gt;
! rowspan=&amp;quot;4&amp;quot; | Singular !! 1 !! -&lt;br /&gt;
| zhè || colspan=&amp;quot;2&amp;quot; | me || mi || mi/ma/mes/mas || -me || -mi&lt;br /&gt;
|-&lt;br /&gt;
! 2 !! Informal&lt;br /&gt;
| tu || colspan=&amp;quot;2&amp;quot; | te || ti || ti/ta/tes/tas || -te || -ti &lt;br /&gt;
|-&lt;br /&gt;
! 3m !! -&lt;br /&gt;
| èl || colspan=&amp;quot;2&amp;quot; | so || si || se/sa/ses/sas || -se || -si&lt;br /&gt;
|-&lt;br /&gt;
! 3f !! -&lt;br /&gt;
| èlla || colspan=&amp;quot;2&amp;quot; | lo || li || le/lua/les/luas || -le || li&lt;br /&gt;
|-&lt;br /&gt;
! rowspan=&amp;quot;3&amp;quot; | Plural !! 1 !! -&lt;br /&gt;
| colspan=&amp;quot;2&amp;quot; | nos || colspan=&amp;quot;2&amp;quot; | nov || nòsce/nòca/nòsces/nòscas || -nos || -ni&lt;br /&gt;
|-&lt;br /&gt;
! 2 !! Informal&lt;br /&gt;
| colspan=&amp;quot;2&amp;quot; | vos || colspan=&amp;quot;2&amp;quot; | vov || vèsce/vèsca/vèsces/vèscas || -vos || -vi&lt;br /&gt;
|-&lt;br /&gt;
! 3 !! -&lt;br /&gt;
| èls || colspan=&amp;quot;2&amp;quot; | los || lis || lor/lar/lors/lars || -las || lis&lt;br /&gt;
|-&lt;br /&gt;
! Both !! 2 !! Formal&lt;br /&gt;
| antu || - || lèkum || kum || &#039;&#039;paraph&#039;&#039; || -kum || -ki&lt;br /&gt;
|}&lt;br /&gt;
Two clitics both attaching to a verb is possible.  If there are two, dative always precedes accusative, e.g. &#039;&#039;da-mi-le&#039;&#039; &amp;quot;give me her&amp;quot;.&lt;br /&gt;
&lt;br /&gt;
Another important pronoun is &#039;&#039;&#039;es&#039;&#039;&#039;.  It reflexive without person or number, clitic or independent, dative or accusative.&lt;br /&gt;
&lt;br /&gt;
== Verbs ==&lt;br /&gt;
* -ar class -&amp;amp;gt; active, from -āre, e.g. kantar &#039;to sing&#039;&lt;br /&gt;
* -èr class -&amp;amp;gt; active, from -ēre, e.g. temer &#039;to fear&#039;&lt;br /&gt;
* -ir class -&amp;amp;gt; inchoative, from -īre, e.g. dormir &#039;to sleep&#039;&lt;br /&gt;
* -òr class -&amp;amp;gt; mediopassive, from -or, e.g. moròr &#039;to die&#039;, lavòr &#039;to bathe (oneself)&#039;.  Amazingly, new verbs enter this category, such as &#039;&#039;umidékor&#039;&#039; &amp;quot;to get wet&amp;quot;&lt;br /&gt;
&lt;br /&gt;
For -ar, present indicative active: -o, -as, -a, -am, -ac, -an. &lt;br /&gt;
-èr is -o, -ès, -è, -èm, -èc, -èm.&lt;br /&gt;
-ir is -o, -is, -i, -im, -ic, -im.&lt;br /&gt;
-òr is -o, -us, -u, -um, -uc, -um.  -ò- appears in other stems.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Person !! Present !! Imperfect !! Preterite !! Synthetic Future !! Periphrastic Future&lt;br /&gt;
|-&lt;br /&gt;
| 1sg || kanto || kantèva || kantè || kantarè || avjo kantar&lt;br /&gt;
|-&lt;br /&gt;
| 2sg || kantas || kantèvas || kantàs || kantaràs || avjas kantar&lt;br /&gt;
|-&lt;br /&gt;
| 3sg || kanta || kantèva || kantà || kantarà || avja kantar&lt;br /&gt;
|-&lt;br /&gt;
| 1pl || kantam || kantèvam || kantam || kantarèm || avjam kantar&lt;br /&gt;
|-&lt;br /&gt;
| 2pl || kantac || kantèvac || kantac || kantarèc || avjac kantar&lt;br /&gt;
|-&lt;br /&gt;
| 3pl || kantan || kantèvan || kantàron || kantaràn || avjan kantar&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Person !! Present Subjunctive !! Preterite Subjunctive !! Conditional&lt;br /&gt;
|-&lt;br /&gt;
| 1sg || kantje || kantèse || volria kantar&lt;br /&gt;
|-&lt;br /&gt;
| 2sg || kantjes || kantèses || volrias kantar&lt;br /&gt;
|-&lt;br /&gt;
| 3sg || kantje || kantèse || volria kantar&lt;br /&gt;
|-&lt;br /&gt;
| 1pl || kantjem || kantèsem || volriam kantar&lt;br /&gt;
|-&lt;br /&gt;
| 2pl || kantjec || kantèsec || volriac kantar&lt;br /&gt;
|-&lt;br /&gt;
| 3pl || kantjen || kantèsen || volrian kantar&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
* 2sg: kanta!&lt;br /&gt;
* 2pl: kantac!&lt;br /&gt;
* 3sg: kantje!&lt;br /&gt;
* 3pl: kantan! (or kantjen!&lt;br /&gt;
* Negative forms use subjunctive:&lt;br /&gt;
** non kantjes&lt;br /&gt;
** non kantjec&lt;br /&gt;
** non kantje&lt;br /&gt;
** non kantjen&lt;br /&gt;
&lt;br /&gt;
* Infinitive: kantar&lt;br /&gt;
* Past participle: kantat&lt;br /&gt;
* Gerund: kantant&lt;br /&gt;
* Present participle: kantanto (used adjectivally)&lt;br /&gt;
* Perfect participle: kantat&lt;br /&gt;
&lt;br /&gt;
== Vocab ==&lt;br /&gt;
* mèǧ - middle&lt;br /&gt;
* ǧurn - daily&lt;br /&gt;
* oǧo - I hear&lt;br /&gt;
* zhamar - to cry out&lt;br /&gt;
* rezhina - queen&lt;br /&gt;
* lloria - glory&lt;br /&gt;
* lezher - to read&lt;br /&gt;
* ehwiver - to write&lt;br /&gt;
* espèǧar - to watch&lt;br /&gt;
* mazhòr - bigger&lt;br /&gt;
* eca - road&lt;br /&gt;
* paxènxa - patience&lt;br /&gt;
* soc - companion&lt;br /&gt;
* raxò - reason&lt;br /&gt;
* nojta - night&lt;br /&gt;
* año - lamb&lt;br /&gt;
* ahwa - water&lt;br /&gt;
* bruvia - rain&lt;br /&gt;
* lihwor - liquid&lt;br /&gt;
* xor - flower&lt;br /&gt;
* kwo - which&lt;br /&gt;
* xama - flame&lt;br /&gt;
* i/j&#039; - and&lt;br /&gt;
&lt;br /&gt;
=== More Arabic ===&lt;br /&gt;
; kadi : major, from القاضي&lt;br /&gt;
; xadrez : chess, from الشطرنج&lt;br /&gt;
; mufada : pillow, from المخدة&lt;br /&gt;
; zhafran : saffron, from الزعفران&lt;br /&gt;
; zejtona : olive, from الزيتون&lt;br /&gt;
; ohalá : hopefully, from ¿إن شاء الله?&lt;br /&gt;
; mihrab : sanctum, from محراب&lt;br /&gt;
; zawija : monastery, from زاوية&lt;br /&gt;
; azhur : blue, from لازورد&lt;br /&gt;
; taza : cup, from طاسة&lt;br /&gt;
; sekwa : irrigation ditch, from سَاقِيَة&lt;br /&gt;
; kazar : castle, from اَلْقَصْر&lt;br /&gt;
; safanòria : carrot, from *سَفُنَّارْيَة&lt;br /&gt;
; midraxa : seminary, from مدرسة (Heb)&lt;br /&gt;
; sahan : plate, courtyard, from صحن&lt;br /&gt;
; kativ : scribe, from كاتب (Heb)&lt;br /&gt;
; xiber : ink, from حبر&lt;br /&gt;
; baharat : seasoning, from بهارات&lt;br /&gt;
; mira : mirror, from مرآة&lt;br /&gt;
; diwan : court, from ديوان&lt;br /&gt;
; gwaf : endowment, from وقف&lt;br /&gt;
; zit : oil, olive oil, from زيت&lt;br /&gt;
&lt;br /&gt;
== Sound Changes ==&lt;br /&gt;
Stress followed Latin rules: penultimate if heavy, otherwise antepenultimate.  Write latin c as k.  Write latin qu as kw.&lt;br /&gt;
&lt;br /&gt;
Vowels&lt;br /&gt;
* a,ā -&amp;amp;gt; a&lt;br /&gt;
* e -&amp;amp;gt; è&lt;br /&gt;
* ē -&amp;amp;gt; e&lt;br /&gt;
* o -&amp;amp;gt; ò&lt;br /&gt;
* ō -&amp;amp;gt; o&lt;br /&gt;
* ī, i -&amp;amp;gt; i&lt;br /&gt;
* ū, u -&amp;amp;gt; u&lt;br /&gt;
* &#039;è -&amp;amp;gt; jè (stressed)&lt;br /&gt;
* &#039;ò -&amp;amp;gt; wè (stressed)&lt;br /&gt;
&lt;br /&gt;
Palatalization&lt;br /&gt;
* li,ll -&amp;amp;gt; ll&lt;br /&gt;
* di, de -&amp;amp;gt; ǧ&lt;br /&gt;
* tiV, teV -&amp;amp;gt; cV&lt;br /&gt;
* trV -&amp;amp;gt; cV&lt;br /&gt;
* drV -&amp;amp;gt; ǧV&lt;br /&gt;
* lt -&amp;amp;gt; jt&lt;br /&gt;
* gn -&amp;amp;gt; ñ&lt;br /&gt;
* cl -&amp;amp;gt; zh&lt;br /&gt;
* ViV -&amp;amp;gt; VzhV&lt;br /&gt;
* fl -&amp;amp;gt; x&lt;br /&gt;
* gl -&amp;amp;gt; ll&lt;br /&gt;
&lt;br /&gt;
Lenition&lt;br /&gt;
* V[bdg]V -&amp;amp;gt; V[vðh]V (not written for ð)&lt;br /&gt;
* V[ptk]V -&amp;amp;gt; V[bdg]V &lt;br /&gt;
* medial kw -&amp;amp;gt; xw&lt;br /&gt;
* initial and medial ß -&amp;amp;gt; gw&lt;br /&gt;
&lt;br /&gt;
Cluster&lt;br /&gt;
* pl -&amp;amp;gt; br&lt;br /&gt;
* kr stays&lt;br /&gt;
* de-geminate all except rr, ll&lt;br /&gt;
* skr -&amp;amp;gt; ehw&lt;br /&gt;
* sp -&amp;amp;gt; esp&lt;br /&gt;
* str -&amp;amp;gt; ec&lt;br /&gt;
* st -&amp;amp;gt; est&lt;br /&gt;
&lt;br /&gt;
rhotic&lt;br /&gt;
* initial r -&amp;amp;gt; rr&lt;br /&gt;
* [lns]r -&amp;amp;gt; [lns]rr (and old geminates)&lt;br /&gt;
&lt;br /&gt;
Late&lt;br /&gt;
* snobs say ʁ instead of r&lt;br /&gt;
* Arabic ð written dh&lt;br /&gt;
* Arabic ṯ written th&lt;br /&gt;
&lt;br /&gt;
== Passages ==&lt;br /&gt;
=== North Wind ===&lt;br /&gt;
* La Tramutaña j&#039;al Sol kontendègwan kwo de èls era mazhòr.&lt;br /&gt;
&lt;br /&gt;
=== Rerum Novarum ===&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Language !! Text&lt;br /&gt;
|-&lt;br /&gt;
| Latin || Salutem et Apostolicam Benedictionem.  Rerum novarum semel excitata cupiditate, quae diu societatem commovit, illud fere consequens erat, ut hominum mentes ad res novas cogitationes appellerentur: unde factum est ut ex una parte homines, qui opibus praestarent, eas veluti ius suum esse contenderent, nulla in re aut divino aut humano iuri obnoxias; ex altera vero parte ut opifices, inopia et duriore condicione pressati, id unum quaererent, ut se ab eiusmodi servitute omnino expediant. Quae res eos, vel invita, in easdem sententias et consilia impulerunt, quae socialismi nomine vulgo appellantur; siquidem facilius est animis eorum persuadere, eas opes, quae iniquitate et iniuria coacervatae sint, ita in commune deduci posse, ut iis, qui nulla re praediti sint, pro sua parte prosint.  Verum haec omnia, quae hucusque a socialistis proposita sunt, tametsi in speciem alliciant, nihil aliud ostendunt, nisi falsas rationes et inefficaces ad id, quod spectant; immo vero talia remedia longe peiora sunt morbis, quae sanare velle videntur.&lt;br /&gt;
|-&lt;br /&gt;
| Spanish || Salud y Bendición Apostólica.  Una vez despertado el deseo de cosas nuevas, que desde hace tiempo agita a la sociedad, era casi inevitable que los ánimos de los hombres se inclinaran hacia nuevas ideas: de aquí resultó que, por una parte, los que poseían riquezas las defendieran como si fueran un derecho suyo, no sujeto en nada a la ley divina ni humana; y por otra, que los obreros, oprimidos por la miseria y una condición más dura, solo buscaran librarse completamente de tal servidumbre. Esto los llevó, incluso contra su voluntad, a abrazar aquellas opiniones y proyectos que comúnmente se llaman socialismo; pues es más fácil persuadir a sus almas que esas riquezas, acumuladas por la iniquidad y la injusticia, podrían distribuirse en común para beneficiar, según su parte, a aquellos que nada poseen.  Pero todas estas propuestas de los socialistas, aunque parezcan atractivas a primera vista, no muestran más que razones falsas e ineficaces para lograr su propósito; antes bien, tales remedios son mucho peores que los males que pretenden curar.&lt;br /&gt;
|-&lt;br /&gt;
| &#039;&#039;Catalan&#039;&#039; || Salut i Benedicció Apostòlica.  Una vegada despertada la set de coses noves, que fa temps que agita la societat, era gairebé inevitable que els ànims dels homes es decantessin cap a noves idees: d’aquí va resultar que, d’una banda, els qui posseïen riqueses les defensessin com si fossin un dret seu, no sotmès a cap llei divina ni humana; i de l’altra, que els treballadors, oprimits per la misèria i una condició més dura, només cerquessin alliberar-se completament d’aquesta servitud. Això els va portar, fins i tot contra la seva voluntat, a abraçar aquelles opinions i projectes que s’anomenen comunament socialisme; perquè és més fàcil convèncer els seus esperits que aquestes riqueses, acumulades amb iniquitat i injustícia, podrien repartir-se en comú per beneficiar, segons la seva part, els qui no tenen res.&lt;br /&gt;
|-&lt;br /&gt;
| Italian || Salute e Benedizione Apostolica.  Una volta suscitata la brama di cose nuove, che da tempo turba la società, era quasi inevitabile che gli animi degli uomini si volgessero a nuove idee: ne è derivato che, da una parte, coloro che possedevano ricchezze le rivendicassero come un loro diritto, non soggetto in nulla alla legge divina o umana; dall’altra, che i lavoratori, oppressi dalla miseria e da una condizione più dura, cercassero unicamente di liberarsi completamente da tale servitù. Ciò li ha spinti, anche contro la loro volontà, ad abbracciare quelle opinioni e quei progetti che vengono comunemente chiamati socialismo; poiché è più facile persuadere le loro menti che tali ricchezze, accumulate con iniquità e ingiustizia, possano essere distribuite in comune, così da giovare, secondo la loro parte, a coloro che nulla possiedono.  Ma tutte queste proposte dei socialisti, benché a prima vista sembrino allettanti, non dimostrano altro che ragionamenti falsi e inefficaci per il fine che si propongono; anzi, tali rimedi sono di gran lunga peggiori dei mali che pretendono di sanare.&lt;br /&gt;
|-&lt;br /&gt;
| Koǧan || Salut i Benedikzho Apostòlik.  Una gwedata despertat al xok de kosas nwèvas, kwe fa tèm agita la soxedat, èra kwazi inegwitabile kwe las animas dals òmes se gwolvòsen verz unas idèzhas nwevas:&lt;br /&gt;
&lt;br /&gt;
|}&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=User:Aquatiki&amp;diff=170922</id>
		<title>User:Aquatiki</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=User:Aquatiki&amp;diff=170922"/>
		<updated>2025-05-24T17:11:29Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;{{Userpage&lt;br /&gt;
|name=Robert Marshall Murphy&lt;br /&gt;
|conlangs=[[Weddish]], [[Stilio|Parseltongue]], [[Proto-Polynesian Hebrew]], [[Syrenian]], [[Semitic Korean]]&lt;br /&gt;
|natlangs=[[English]], [[Wikipedia:Korean language|Korean]], [[Wikipedia:Ancient Greek|Ancient Greek]], [[Wikipedia:Hebrew language|Hebrew]], [[Wikipedia:Aramaic language|Aramaic]], [[Wikipedia:Syriac language|Syriac]], [[Wikipedia:Akkadian language|Akkadian]], [[Wikipedia:Ugaritic language|Ugaritic]], [[Yiddish]]&lt;br /&gt;
|otherlangs=[[Na&#039;vi]], [[Koǧan]], [[Syrunian]], [[Klingon]]&lt;br /&gt;
|interests=Philosophy, theology, math&lt;br /&gt;
|birth=Planet Earth&lt;br /&gt;
|profession=Upper school (high school) math teacher&lt;br /&gt;
|more=Feel free to contact me about anything&lt;br /&gt;
}}&lt;br /&gt;
I&#039;d love to chat any time, so feel free to email me anything you like, any time.&lt;br /&gt;
&lt;br /&gt;
I mainly like IAL (International Auxiliary Languages), which part of [[Universal Languages]] project.  These 15 languages are (not all by me):&lt;br /&gt;
# [[Dan&#039;a&#039;yo]] - 1.5 billion people in China, Japan, the Koreas, and part of Vietnam (combination of sprachbunds)&lt;br /&gt;
# [[Neo-Sanskrit]] - 1.4 billion people on the Indian subcontinent (Indo-Aryan)&lt;br /&gt;
# [[Interlingua]] - 800 million people in the Romance-speaking world (Romance of Indo-European)&lt;br /&gt;
# [[Folksprak]] - 500 million people in the Germanic world (Germanic of Indo-European)&lt;br /&gt;
# [[Kintu]] - 450 million people in the Bantusphere (Bantu of Niger-Congo)&lt;br /&gt;
# [[Indo-Malay]] - 380 million people in Maritime Southeast Asia&lt;br /&gt;
# [[Guosa]] - 340 million people in West Africa (combination of sprachbunds)&lt;br /&gt;
# [[Interslavic]] - 300 million in the Slavisphere (Slavic of Indo-European)&lt;br /&gt;
# [[Middle Semitic]] - 290 million speak the Arabics and Israeli (and Syriac) (Semitic of Afro-asiatic)&lt;br /&gt;
# [[MSEAL]] - 233 million (combination of sprachbunds)&lt;br /&gt;
# [[Dravindian]] - 230 million (Dravidian)&lt;br /&gt;
# [[Zens]] - 200 million (Iranian of Indo-European)&lt;br /&gt;
# [[Jalpi Turkic]] - 170 million (Turkic)&lt;br /&gt;
# [[SEDES]] - 117 million from the Horn of Africa sprachbund&lt;br /&gt;
# [[Balkan]] - 60 million people in the sprachbund&lt;br /&gt;
I have a naturalistic auxlang with a rich history for my personalang, called [[Weddish]].  Like a lot of my personal projects, it is a Jewish language.  I also imagined some fictive histories.  A big project is [[Oceanic Hebrew]], which has [[Austronesian Hebrew]], [[Polynesian Hebrew]], and a minilang called [[Neo-Oceanic Hebrew]].&lt;br /&gt;
&lt;br /&gt;
[[File:Caucasus Flag.svg|thumb|Perhaps I will make an IAL for the Caucasus.  A polypersonal IAL would be cool.]]&lt;br /&gt;
&lt;br /&gt;
{{Universal Language}}&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=170312</id>
		<title>Ɬiʔa/Conworlding</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=170312"/>
		<updated>2025-05-07T21:29:15Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: clearing&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=170311</id>
		<title>Ɬiʔa/Conworlding</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=170311"/>
		<updated>2025-05-07T20:56:32Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: cleaning&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== System ==&lt;br /&gt;
&lt;br /&gt;
== Planet C ==&lt;br /&gt;
[[File:Planet C and its tethered moon.png|right|700px]]&lt;br /&gt;
* With an albedo of 0.2, the global average temp is 263ºK.  Because of modest greenhouse effects, surface temperatures are higher, on the sun-side.&lt;br /&gt;
# Mass: 1.5M⊕&lt;br /&gt;
# Gravity: 1g⊕&lt;br /&gt;
# Radius = 1.225⊕, or 7805km&lt;br /&gt;
Terminator Zone&lt;br /&gt;
# +/-30º: 1.28 E8 km&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; (slightly less than all the land of the Earth)&lt;br /&gt;
# Escape velocity is 12.4km/s, 11% higher than Earth&lt;br /&gt;
# Orbital velocity is 8.79km/s&lt;br /&gt;
=== Atmosphere ===&lt;br /&gt;
Water content is low because&lt;br /&gt;
* Water vapor is a potent greenhouse gas; vast surface water can trap too much heat, especially near the substellar point.&lt;br /&gt;
* Water leads to climate homogenization&lt;br /&gt;
* Lack of exposed silicate rock: Necessary for carbon-silicate weathering feedback, which stabilizes climate on geological timescales.&lt;br /&gt;
Earth has ~1.4 billion km³ of water.  In our habitable zone, we have no more than 10% of that, or 100 million km³, though there is much more on the night side, both liquid and ice.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Factor !! Ɬiʔa atm !! Ɬiʔa % !! Earth atm !! Earth % !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! Total Pressure &lt;br /&gt;
| 1.6 atm || || 1.0 atm || || Enhanced convective heat transfer, increased IR trapping&lt;br /&gt;
|-&lt;br /&gt;
! Nitrogen (N₂) &lt;br /&gt;
| 1.00 || 62.50% || 0.7808 || 78.08% || Reduced; still inert, still dominant&lt;br /&gt;
|-&lt;br /&gt;
! Oxygen (O₂) &lt;br /&gt;
| 0.21 || 13.13% || 0.2095 || 20.95% || Earth-normal partial pressure &lt;br /&gt;
|-&lt;br /&gt;
! Argon (Ar)&lt;br /&gt;
| 0.40 || 25.00% || 0.0093 || 0.93% || Major heat distribution enhancement, inert&lt;br /&gt;
|-&lt;br /&gt;
! Krypton + Xenon&lt;br /&gt;
| 0.005 || 0.31% || trace || trace || High molecular mass → improved heat retention, still safe&lt;br /&gt;
|-&lt;br /&gt;
! CO₂&lt;br /&gt;
| 0.005 || 0.31% || 0.004 || 0.04% || slightly elevated; sub-greenhouse threshold&lt;br /&gt;
|-&lt;br /&gt;
! H₂O vapor &lt;br /&gt;
| 0.015 || ~1% || || 0-4% || Maintains greenhouse without excess moisture&lt;br /&gt;
|}&lt;br /&gt;
==== Atmospheric Effects on Clouds ====&lt;br /&gt;
# Increased Pressure (1.6 atm) compresses gases, raising the dew point at which water vapor condenses. Clouds form closer to the surface, and are denser than similar altitudes compared to Earth.&lt;br /&gt;
# Low Water Inventory (~20% of Earth&#039;s): less frequent and less massive cloud systems than on Earth, but still present—especially over &amp;quot;hotspots&amp;quot; on the day side.&lt;br /&gt;
# Tidally Locked Climate: Cloud formation concentrate along the substellar point, where warm, moist air rises and cools.&lt;br /&gt;
#* A permanent “eyewall” storm system has formed at the subsolar point, like a giant hurricane.&lt;br /&gt;
#* As air rises and is advected to the night side, thin cloud bands or ice hazes form as it descends and cools.&lt;br /&gt;
&lt;br /&gt;
Appearance:&lt;br /&gt;
* The presence of noble gases (Ar, Kr, Xe) and higher pressure enhance Mie scattering, making clouds appear whiter and more silvered, especially at sunrise/sunset boundaries.&lt;br /&gt;
* Night side clouds are thin, high-altitude icy sheets, glowing faintly in aurorae or thermal emissions.&lt;br /&gt;
&lt;br /&gt;
==== Sky Color ====&lt;br /&gt;
[[File:Life near the terminator.png|thumb|right|Life near the terminator]]&lt;br /&gt;
The color of the sky is shaped by Rayleigh scattering, which depends on:&lt;br /&gt;
# Molecular composition: Heavier gases like Ar, Kr, and Xe scatter light less efficiently than N₂.&lt;br /&gt;
# Spectral output of the star: the red dwarf emits predominantly infrared and red light, with very little blue or violet.&lt;br /&gt;
&lt;br /&gt;
Consequence:&lt;br /&gt;
* Even with atmospheric scattering, there is insufficient blue light in the stellar spectrum to produce a blue sky.&lt;br /&gt;
* Day sky would likely appear:&lt;br /&gt;
** Dark peach, dusky rose, or reddish beige near zenith,&lt;br /&gt;
** Grading to deep salmon or mauve near the horizon,&lt;br /&gt;
** A slight metallic sheen due to noble gas content and high pressure.&lt;br /&gt;
&lt;br /&gt;
Twilight &amp;amp; Limb Scattering:&lt;br /&gt;
* The terminator (twilight zone) sees a diffuse, ruddy light, scattering through haze and clouds into luminous reds, purples, and copper tones.&lt;br /&gt;
* Aurorae are spectacular on the night side, especially since stellar flares are frequent.&lt;br /&gt;
&lt;br /&gt;
==== Sound Propagation ====&lt;br /&gt;
: &#039;&#039;Sound is profoundly affected by atmospheric pressure and composition.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Compared to Earth:&lt;br /&gt;
* Higher pressure → greater air density → faster transmission of sound and less attenuation.&lt;br /&gt;
* Argon and Xenon are heavy gases, which:&lt;br /&gt;
** Lower the speed of sound relative to air at the same pressure (despite the pressure increase).&lt;br /&gt;
** Shift resonance frequencies downward, resulting in deeper, rounder sounds.&lt;br /&gt;
&lt;br /&gt;
Consequences:&lt;br /&gt;
* Voices sound subtly lower-pitched and richer, especially for consonants and low vowels.&lt;br /&gt;
* Ambient sounds (wind, water, animals) would carry farther and sound more muffled or sonorous.&lt;br /&gt;
* Music or speech would resonate more warmly, especially indoors or in enclosed spaces.&lt;br /&gt;
&lt;br /&gt;
In short: it sounds like it’s wrapped in velvet.&lt;br /&gt;
&lt;br /&gt;
==== Heat Transport to the Night Side ====&lt;br /&gt;
Mechanisms:&lt;br /&gt;
# Thick Atmosphere (1.6 atm) increases:&lt;br /&gt;
#* Advection efficiency: Warm air masses can move more heat horizontally.&lt;br /&gt;
#* Radiative time constant: The atmosphere holds heat longer before releasing it.&lt;br /&gt;
# Noble Gases (especially Kr/Xe):&lt;br /&gt;
#* High molecular mass → more IR opacity → trapping and radiating heat more evenly.&lt;br /&gt;
# Slow Rotation / Tidal Locking:&lt;br /&gt;
#* Global Hadley-like cells dominate circulation, carrying warm air from the day side to the night side and descending it there.&lt;br /&gt;
&lt;br /&gt;
Result:&lt;br /&gt;
* The night side is not so freezing.  Temperatures differ by tens of degrees, not hundreds.&lt;br /&gt;
* There are still ice caps and a cold deserts at the anti-stellar point, but not a glaciated wasteland.&lt;br /&gt;
&lt;br /&gt;
=== Magnetosphere ===&lt;br /&gt;
* Larger mass --&amp;gt; larger iron core, generating more internal heat&lt;br /&gt;
* Larger radius --&amp;gt; Vigorous convection in the core&lt;br /&gt;
* Tidal Flexing --&amp;gt; still drives magnetic activity&lt;br /&gt;
&lt;br /&gt;
# Aurorae at lower latitudes&lt;br /&gt;
## higher magnetic rigidity, wider magnetotail, and greater reconnection energy.&lt;br /&gt;
## Combined with a higher flux of stellar particles, this means:&lt;br /&gt;
### Auroral ovals expand, reaching mid-latitudes sometimes equator.&lt;br /&gt;
### The skies are alive with rippling green, violet, and crimson aurorae, especially on the night side.&lt;br /&gt;
### Daily auroral activity occur during stellar flare cycles.&lt;br /&gt;
# Compasses&lt;br /&gt;
## compasses respond more sharply, with:&lt;br /&gt;
### Faster alignment.&lt;br /&gt;
### Greater resistance to local perturbations.&lt;br /&gt;
## However, frequent magnetic storms from stellar activity cause sudden declinations, reversals, or local anomalies.  In short, lots of aurorae equals dead compasses at the same time.&lt;br /&gt;
# Magnetic Field Strength &amp;gt; 100 μT &lt;br /&gt;
# Electromagnetism is more basic than chemistry or almost any other natural philosophy&lt;br /&gt;
&lt;br /&gt;
=== Substellar Point ===&lt;br /&gt;
The maximum incoming flux is very nearly the same as Earth&#039;s solar constant (≈1361 W/m²), but concentrated over one point rather than averaged over a rotating sphere.  Temperatures should be above 500ºK most of the time.  &lt;br /&gt;
&lt;br /&gt;
The magnetic north is also here. The thick atmosphere prevents too much loss here, but &lt;br /&gt;
* Charged particle influx&lt;br /&gt;
** Maximized at the substellar point—intense auroral and energetic particle precipitation&lt;br /&gt;
* Atmospheric ionization&lt;br /&gt;
** Constant production of high-energy ions and NOx compounds—UV fluorescence in upper sky&lt;br /&gt;
* Localized heating&lt;br /&gt;
** Augments already extreme temperatures—600–700 K surface&lt;br /&gt;
&lt;br /&gt;
== Artificially Tethered Moon ==&lt;br /&gt;
* 670,000 km up&lt;br /&gt;
* 7805 km in radius = same as the planet&lt;br /&gt;
* 1.33º of the sky, same as the sun&lt;br /&gt;
&lt;br /&gt;
A network of tethers/tension lines from the moon to multiple anchor points on the planet’s surface (a tripod or hexapod structure), woven like hair&lt;br /&gt;
* Uses active tension management and orbital station-keeping to stabilize the moon&lt;br /&gt;
* Counterweights and inward-pointing mass drivers on the moon to oppose drift&lt;br /&gt;
&lt;br /&gt;
The tethers are not bearing the full weight, but merely damping drift, providing restoring force, and enabling long-term stability through active compensation.  The moon&lt;br /&gt;
* Blocks the worst of the heat&lt;br /&gt;
* Blocks the worst of the solar radiation&lt;br /&gt;
The moon has &lt;br /&gt;
* low mass&lt;br /&gt;
* high albedo - enormous reflectivity&lt;br /&gt;
* scatters charges particles, UV, X-rays, auroral flux tubes&lt;br /&gt;
* sunward - crazy hot, high emissivity&lt;br /&gt;
* earthward - crazy cool, low emissivity&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=170310</id>
		<title>Ɬiʔa/Conworlding</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=170310"/>
		<updated>2025-05-07T20:54:59Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* Star */ cleaning&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== System ==&lt;br /&gt;
&lt;br /&gt;
==== d: the wet eye with depths ====&lt;br /&gt;
[[File:wet eye planet.png|thumb|right|An reasonable approximation of d&#039;s appearance]]&lt;br /&gt;
From the outside, d is a &amp;quot;wet eye&amp;quot; just outside the habitable zone.  It is a water world, twice the mass of Earth, 1.4 times the radius, tidally locked.  The substellar point is the only place without surface ice.  However, it is better to think of the planet top-to-bottom.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;atmosphere&#039;&#039;&#039; is tenuous, less than 0.2 bars.  It is thin, N₂-rich with traces of H₂O, NH₃ vapor, and transient geyser outputs.  It is highly UV-irradiated, and Mars-like in its inability to retain volatiles.&lt;br /&gt;
&lt;br /&gt;
Next, there is a &#039;&#039;&#039;surface ice shell&#039;&#039;&#039;, ~20 km of thick Ice I.  Swirling currents beneath have cracked continent-sized ice plates, similar to Europa&#039;s crust.  It is permanently frozen except at the substellar furnace.  It accumulates chemical stains, mineral deposits, and cryovolcanic eruption plumes.  Accumulations of complex hydrates—like methanol clathrates—precipitate out and form false reefs, rising like coral from beneath. Transient thermal vents push hot plumes into the thin air, freezing instantly and snowing down crystals that form mineral spires.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;subglacial ocean&#039;&#039;&#039; is hundreds of kilometers thick.  It is super-pressurized liquid H₂O mixed with NH₃, CH₃OH, H₂O₂, and trace salts.  The movement is slow, planetary-scale currents originating from the Furnace and Coriolis force.  Strong layers exist: the surface is oxidized; the abyssal layer is reducing.&lt;br /&gt;
&lt;br /&gt;
A new &amp;quot;surface&amp;quot; is next.  The &#039;&#039;&#039;Ice Mantle&#039;&#039;&#039; is solid Ice VI and VII.  There are massive, slowly shifting &amp;quot;sub-oceanic continents&amp;quot;. It is periodically fractured and resurfaced by cryoquakes and brine-driven eruptions.  Some regions have developed elevated domes or ridges, continental “shelves” under the ocean.&lt;br /&gt;
&lt;br /&gt;
Finally, underneath is the &#039;&#039;&#039;core&#039;&#039;&#039;. Temperatures exceed 2000–3000 K locally.  Pressures range from 100 to 300 GPa.  The core is rich in heavy elements.  This makes radiogenic hotspots, localized magnetic eddies.  Heat gradients + ion flows = thermoelectric currents.  These make magnetic storms within the ocean itself, not the sky.  When uranium-rich corium pods shift or explode upward through the mantle, their heat and conductivity disturb the local magnetic field, generating geomagnetic quakes.  These pulse through the ocean, creating short-lived magnetic lenses.  These interact with atmospheric charged particles above the Furnace, giving rise to transient magnetic halos visible from orbit—false auroras without a sunstorm.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Planet C ==&lt;br /&gt;
[[File:Planet C and its tethered moon.png|right|700px]]&lt;br /&gt;
* With an albedo of 0.2, the global average temp is 263ºK.  Because of modest greenhouse effects, surface temperatures are higher, on the sun-side.&lt;br /&gt;
# Mass: 1.5M⊕&lt;br /&gt;
# Gravity: 1g⊕&lt;br /&gt;
# Radius = 1.225⊕, or 7805km&lt;br /&gt;
Terminator Zone&lt;br /&gt;
# +/-30º: 1.28 E8 km&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; (slightly less than all the land of the Earth)&lt;br /&gt;
# Escape velocity is 12.4km/s, 11% higher than Earth&lt;br /&gt;
# Orbital velocity is 8.79km/s&lt;br /&gt;
=== Atmosphere ===&lt;br /&gt;
Water content is low because&lt;br /&gt;
* Water vapor is a potent greenhouse gas; vast surface water can trap too much heat, especially near the substellar point.&lt;br /&gt;
* Water leads to climate homogenization&lt;br /&gt;
* Lack of exposed silicate rock: Necessary for carbon-silicate weathering feedback, which stabilizes climate on geological timescales.&lt;br /&gt;
Earth has ~1.4 billion km³ of water.  In our habitable zone, we have no more than 10% of that, or 100 million km³, though there is much more on the night side, both liquid and ice.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Factor !! Ɬiʔa atm !! Ɬiʔa % !! Earth atm !! Earth % !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! Total Pressure &lt;br /&gt;
| 1.6 atm || || 1.0 atm || || Enhanced convective heat transfer, increased IR trapping&lt;br /&gt;
|-&lt;br /&gt;
! Nitrogen (N₂) &lt;br /&gt;
| 1.00 || 62.50% || 0.7808 || 78.08% || Reduced; still inert, still dominant&lt;br /&gt;
|-&lt;br /&gt;
! Oxygen (O₂) &lt;br /&gt;
| 0.21 || 13.13% || 0.2095 || 20.95% || Earth-normal partial pressure &lt;br /&gt;
|-&lt;br /&gt;
! Argon (Ar)&lt;br /&gt;
| 0.40 || 25.00% || 0.0093 || 0.93% || Major heat distribution enhancement, inert&lt;br /&gt;
|-&lt;br /&gt;
! Krypton + Xenon&lt;br /&gt;
| 0.005 || 0.31% || trace || trace || High molecular mass → improved heat retention, still safe&lt;br /&gt;
|-&lt;br /&gt;
! CO₂&lt;br /&gt;
| 0.005 || 0.31% || 0.004 || 0.04% || slightly elevated; sub-greenhouse threshold&lt;br /&gt;
|-&lt;br /&gt;
! H₂O vapor &lt;br /&gt;
| 0.015 || ~1% || || 0-4% || Maintains greenhouse without excess moisture&lt;br /&gt;
|}&lt;br /&gt;
==== Atmospheric Effects on Clouds ====&lt;br /&gt;
# Increased Pressure (1.6 atm) compresses gases, raising the dew point at which water vapor condenses. Clouds form closer to the surface, and are denser than similar altitudes compared to Earth.&lt;br /&gt;
# Low Water Inventory (~20% of Earth&#039;s): less frequent and less massive cloud systems than on Earth, but still present—especially over &amp;quot;hotspots&amp;quot; on the day side.&lt;br /&gt;
# Tidally Locked Climate: Cloud formation concentrate along the substellar point, where warm, moist air rises and cools.&lt;br /&gt;
#* A permanent “eyewall” storm system has formed at the subsolar point, like a giant hurricane.&lt;br /&gt;
#* As air rises and is advected to the night side, thin cloud bands or ice hazes form as it descends and cools.&lt;br /&gt;
&lt;br /&gt;
Appearance:&lt;br /&gt;
* The presence of noble gases (Ar, Kr, Xe) and higher pressure enhance Mie scattering, making clouds appear whiter and more silvered, especially at sunrise/sunset boundaries.&lt;br /&gt;
* Night side clouds are thin, high-altitude icy sheets, glowing faintly in aurorae or thermal emissions.&lt;br /&gt;
&lt;br /&gt;
==== Sky Color ====&lt;br /&gt;
[[File:Life near the terminator.png|thumb|right|Life near the terminator]]&lt;br /&gt;
The color of the sky is shaped by Rayleigh scattering, which depends on:&lt;br /&gt;
# Molecular composition: Heavier gases like Ar, Kr, and Xe scatter light less efficiently than N₂.&lt;br /&gt;
# Spectral output of the star: the red dwarf emits predominantly infrared and red light, with very little blue or violet.&lt;br /&gt;
&lt;br /&gt;
Consequence:&lt;br /&gt;
* Even with atmospheric scattering, there is insufficient blue light in the stellar spectrum to produce a blue sky.&lt;br /&gt;
* Day sky would likely appear:&lt;br /&gt;
** Dark peach, dusky rose, or reddish beige near zenith,&lt;br /&gt;
** Grading to deep salmon or mauve near the horizon,&lt;br /&gt;
** A slight metallic sheen due to noble gas content and high pressure.&lt;br /&gt;
&lt;br /&gt;
Twilight &amp;amp; Limb Scattering:&lt;br /&gt;
* The terminator (twilight zone) sees a diffuse, ruddy light, scattering through haze and clouds into luminous reds, purples, and copper tones.&lt;br /&gt;
* Aurorae are spectacular on the night side, especially since stellar flares are frequent.&lt;br /&gt;
&lt;br /&gt;
==== Sound Propagation ====&lt;br /&gt;
: &#039;&#039;Sound is profoundly affected by atmospheric pressure and composition.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Compared to Earth:&lt;br /&gt;
* Higher pressure → greater air density → faster transmission of sound and less attenuation.&lt;br /&gt;
* Argon and Xenon are heavy gases, which:&lt;br /&gt;
** Lower the speed of sound relative to air at the same pressure (despite the pressure increase).&lt;br /&gt;
** Shift resonance frequencies downward, resulting in deeper, rounder sounds.&lt;br /&gt;
&lt;br /&gt;
Consequences:&lt;br /&gt;
* Voices sound subtly lower-pitched and richer, especially for consonants and low vowels.&lt;br /&gt;
* Ambient sounds (wind, water, animals) would carry farther and sound more muffled or sonorous.&lt;br /&gt;
* Music or speech would resonate more warmly, especially indoors or in enclosed spaces.&lt;br /&gt;
&lt;br /&gt;
In short: it sounds like it’s wrapped in velvet.&lt;br /&gt;
&lt;br /&gt;
==== Heat Transport to the Night Side ====&lt;br /&gt;
Mechanisms:&lt;br /&gt;
# Thick Atmosphere (1.6 atm) increases:&lt;br /&gt;
#* Advection efficiency: Warm air masses can move more heat horizontally.&lt;br /&gt;
#* Radiative time constant: The atmosphere holds heat longer before releasing it.&lt;br /&gt;
# Noble Gases (especially Kr/Xe):&lt;br /&gt;
#* High molecular mass → more IR opacity → trapping and radiating heat more evenly.&lt;br /&gt;
# Slow Rotation / Tidal Locking:&lt;br /&gt;
#* Global Hadley-like cells dominate circulation, carrying warm air from the day side to the night side and descending it there.&lt;br /&gt;
&lt;br /&gt;
Result:&lt;br /&gt;
* The night side is not so freezing.  Temperatures differ by tens of degrees, not hundreds.&lt;br /&gt;
* There are still ice caps and a cold deserts at the anti-stellar point, but not a glaciated wasteland.&lt;br /&gt;
&lt;br /&gt;
=== Magnetosphere ===&lt;br /&gt;
* Larger mass --&amp;gt; larger iron core, generating more internal heat&lt;br /&gt;
* Larger radius --&amp;gt; Vigorous convection in the core&lt;br /&gt;
* Tidal Flexing --&amp;gt; still drives magnetic activity&lt;br /&gt;
&lt;br /&gt;
# Aurorae at lower latitudes&lt;br /&gt;
## higher magnetic rigidity, wider magnetotail, and greater reconnection energy.&lt;br /&gt;
## Combined with a higher flux of stellar particles, this means:&lt;br /&gt;
### Auroral ovals expand, reaching mid-latitudes sometimes equator.&lt;br /&gt;
### The skies are alive with rippling green, violet, and crimson aurorae, especially on the night side.&lt;br /&gt;
### Daily auroral activity occur during stellar flare cycles.&lt;br /&gt;
# Compasses&lt;br /&gt;
## compasses respond more sharply, with:&lt;br /&gt;
### Faster alignment.&lt;br /&gt;
### Greater resistance to local perturbations.&lt;br /&gt;
## However, frequent magnetic storms from stellar activity cause sudden declinations, reversals, or local anomalies.  In short, lots of aurorae equals dead compasses at the same time.&lt;br /&gt;
# Magnetic Field Strength &amp;gt; 100 μT &lt;br /&gt;
# Electromagnetism is more basic than chemistry or almost any other natural philosophy&lt;br /&gt;
&lt;br /&gt;
=== Substellar Point ===&lt;br /&gt;
The maximum incoming flux is very nearly the same as Earth&#039;s solar constant (≈1361 W/m²), but concentrated over one point rather than averaged over a rotating sphere.  Temperatures should be above 500ºK most of the time.  &lt;br /&gt;
&lt;br /&gt;
The magnetic north is also here. The thick atmosphere prevents too much loss here, but &lt;br /&gt;
* Charged particle influx&lt;br /&gt;
** Maximized at the substellar point—intense auroral and energetic particle precipitation&lt;br /&gt;
* Atmospheric ionization&lt;br /&gt;
** Constant production of high-energy ions and NOx compounds—UV fluorescence in upper sky&lt;br /&gt;
* Localized heating&lt;br /&gt;
** Augments already extreme temperatures—600–700 K surface&lt;br /&gt;
&lt;br /&gt;
== Artificially Tethered Moon ==&lt;br /&gt;
* 670,000 km up&lt;br /&gt;
* 7805 km in radius = same as the planet&lt;br /&gt;
* 1.33º of the sky, same as the sun&lt;br /&gt;
&lt;br /&gt;
A network of tethers/tension lines from the moon to multiple anchor points on the planet’s surface (a tripod or hexapod structure), woven like hair&lt;br /&gt;
* Uses active tension management and orbital station-keeping to stabilize the moon&lt;br /&gt;
* Counterweights and inward-pointing mass drivers on the moon to oppose drift&lt;br /&gt;
&lt;br /&gt;
The tethers are not bearing the full weight, but merely damping drift, providing restoring force, and enabling long-term stability through active compensation.  The moon&lt;br /&gt;
* Blocks the worst of the heat&lt;br /&gt;
* Blocks the worst of the solar radiation&lt;br /&gt;
The moon has &lt;br /&gt;
* low mass&lt;br /&gt;
* high albedo - enormous reflectivity&lt;br /&gt;
* scatters charges particles, UV, X-rays, auroral flux tubes&lt;br /&gt;
* sunward - crazy hot, high emissivity&lt;br /&gt;
* earthward - crazy cool, low emissivity&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=170260</id>
		<title>Ɬiʔa/Conworlding</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=170260"/>
		<updated>2025-05-07T01:12:12Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* h */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Star ==&lt;br /&gt;
The star is a red-dwarf (M5V) named Gliese 710b minoris, or informally &#039;&#039;Mirar&#039;s Veil&#039;&#039;.  It is 7.9 light-years (≈2.42 parsecs) from Sol, toward the galactic plane, in Scorpius–Ophiuchus.  It lies just &amp;quot;behind&amp;quot; a brighter, well-known K-dwarf, and was not observed until after humanity&#039;s trip to Proxima Centauri: in situ gravitational navigation by the first robotic probe en route to Proxima Centauri. The probe’s optical gyros noticed an unmodeled gravitational perturbation.&lt;br /&gt;
&lt;br /&gt;
* Stellar luminosity (L*) ≈ 0.01 𝐿⊙ (1/100th Sol&#039;s brightness)&lt;br /&gt;
* Stellar mass (M*) ≈ 0.2 𝑀⊙ (1/5 the mass of Sol)&lt;br /&gt;
* Stellar radius (R*) ≈ 0.25 𝑅⊙ (1/4 as wide as Sol)&lt;br /&gt;
* Effective temperature (T*) ≈ 3500 K&lt;br /&gt;
* Average surface field is ~1.5 kG, with frequent bursts of &amp;gt; 3kG&lt;br /&gt;
** Frequent, energetic flares, multiple per day, with for extreme variability over time, often above 10&amp;lt;sup&amp;gt;35&amp;lt;/sup&amp;gt; erg&lt;br /&gt;
* The frostline is at 0.27 AU&lt;br /&gt;
&lt;br /&gt;
​The habitable zone (a) is about square root of L* over L⊙, so ~0.1 AU.&lt;br /&gt;
&lt;br /&gt;
=== Solar System ===&lt;br /&gt;
There are seven planets in the system&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Planet !!	Mass (M🜨)!!	Radius (R🜨)!! Moons/Rings	!!Resonance !!	&amp;lt;small&amp;gt;Semi-Major&amp;lt;/small&amp;gt; !!	Rings !! Moons !! Period !! Size !! Type !! Sidereal !! A. Mag.&lt;br /&gt;
|-&lt;br /&gt;
| b ||	2.17 ||	1.1 ||	No ||	2:3 with c	|| 0.0763 ||	No || No || 17.2 || 13.6&#039; to 1.5&#039; || Super-Mercury || 51.6 || -10.98&lt;br /&gt;
|-&lt;br /&gt;
| c ||	1.5	 ||1.225 ||	1* ||	—	        || 0.100  || No    || No || 25.8 || - || Super-Earth || - || - &lt;br /&gt;
|-&lt;br /&gt;
| d ||	2.0	 ||1.4 ||No ||	2:3 with c	 ||0.131 ||	No || No || 38.7 || 13.1&#039; to 1.8&#039; || Super Waterworld || 77.4 || -11.85&lt;br /&gt;
|-&lt;br /&gt;
| e ||	0.9 ||	1.0 || No	 ||	2:3 with d	 ||0.172 ||	No || No || 58 || 4.1&#039; to 1.1&#039; || Cracked Earth || 46.44 || -8.86&lt;br /&gt;
|- &lt;br /&gt;
| f ||	3.5 ||	2.0 ||	Yes! ||	2:3 with e	 ||0.227 || Yes || Junk || 87 || 4.6&#039; to 1.8&#039; || Mini-Neptune || 36.66 || -9.78&lt;br /&gt;
|-&lt;br /&gt;
| AB || 0.004 || - || 1-300km || 3:2 with f || ~0.3 || - || - || ~60 || - || Fe, Ni, Ar || - || -&lt;br /&gt;
|-&lt;br /&gt;
| g ||	2.6 ||	1.7 ||	2 ||	-	 ||0.40 ||	Yes || Junk || 206 || 1.6&#039; to 1.0&#039; || Stripped Neptune || 29.5 || -7.16&lt;br /&gt;
|-&lt;br /&gt;
| h ||	5.0x2 ||2.3x2 || yes	 || -	 ||1.5 ||	Yes || No || 1500 || 0.5&#039; 16.4&#039; apart (at max) || Double Neptune || 26.25 || -5.43&lt;br /&gt;
|-&lt;br /&gt;
| CDD || 0.1 || - || 1-100km || - || 3-10 || - || - || 2000-11500 || - || H₂O, CO₂, CH₄, Ar || - || 75ºK&lt;br /&gt;
|}&lt;br /&gt;
==== b: super Mercury with a ring of fire  ====&lt;br /&gt;
[[File:planet b by GPT.png|thumb|right|An artistic rendering of planet b]]&lt;br /&gt;
b is a super-Mercury, tidally locked, and incredibly dense.  ~700ºK on the day side, ~50ºK on the night.  2.1 Earth Masses, 1.1 Earth radii (~7000km) in size.  Orbital period 17.2 days.  Density 9.0 g/cm&amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt;.  Gravity is ~1.8g.  &lt;br /&gt;
&lt;br /&gt;
The iron core is huge, being 75% of the mass.  A thin silicate mantle, with metallic plains and exhumed ultramafic crust, with frequent iron meteorite craters, lacking typical “stone” breccias.&lt;br /&gt;
&lt;br /&gt;
The night side is intense, as simple hydrocarbons (methane, ethane, propane) condense and freeze into layered deposits.  Complex organics (tholins, polycyclic aromatics) accumulate on the sea floor, under miles of nitrogen ice.  Massive slush layers slosh around above cryovolcanic brines of ammonia.&lt;br /&gt;
&lt;br /&gt;
There is a crucial layer of Superionic Ice XI above the core, which acts as an electromagnetic insulator, and ionic heat bridge.  The crust is ultramafic silicates (olivine, pyroxene, perovskite) riddled with with sulfide veins, iron alloys, and graphite networks.  The poles of the magnetosphere are sideways, like Uranus, with poles at the equator in the Terminator Zone.  Persistent surface charges develop, because the whole planet is basically a ginormous Leyden jar!&lt;br /&gt;
&lt;br /&gt;
A planetary flux rope forms and un-forms with the star and planet b.  This induces electric jets at the terminator.  This is where temps are Earth-like.  Hydrocarbons sublimate and eject into the atmosphere, even while aurorae come right down to the ground.  A small, low pressure atmosphere prevents photodissociation, even while electrothermal instabilities lift molecules, forming an anomalous haze, a standing, glowing ring.  Coronal events cause localized lightning geysers with magnetic arcing.&lt;br /&gt;
&lt;br /&gt;
In short, b is visible with a blinding bright sun side (glowing orange bronze), a utterly black night side, and a burning, glowing, erupting, arcing ring at the terminator (all colors).  At biggest, it&#039;s half the size of Earth&#039;s moon in the sky, shrinking down to a star at it&#039;s furthest away.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== d: the wet eye with depths ====&lt;br /&gt;
[[File:wet eye planet.png|thumb|right|An reasonable approximation of d&#039;s appearance]]&lt;br /&gt;
From the outside, d is a &amp;quot;wet eye&amp;quot; just outside the habitable zone.  It is a water world, twice the mass of Earth, 1.4 times the radius, tidally locked.  The substellar point is the only place without surface ice.  However, it is better to think of the planet top-to-bottom.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;atmosphere&#039;&#039;&#039; is tenuous, less than 0.2 bars.  It is thin, N₂-rich with traces of H₂O, NH₃ vapor, and transient geyser outputs.  It is highly UV-irradiated, and Mars-like in its inability to retain volatiles.&lt;br /&gt;
&lt;br /&gt;
Next, there is a &#039;&#039;&#039;surface ice shell&#039;&#039;&#039;, ~20 km of thick Ice I.  Swirling currents beneath have cracked continent-sized ice plates, similar to Europa&#039;s crust.  It is permanently frozen except at the substellar furnace.  It accumulates chemical stains, mineral deposits, and cryovolcanic eruption plumes.  Accumulations of complex hydrates—like methanol clathrates—precipitate out and form false reefs, rising like coral from beneath. Transient thermal vents push hot plumes into the thin air, freezing instantly and snowing down crystals that form mineral spires.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;subglacial ocean&#039;&#039;&#039; is hundreds of kilometers thick.  It is super-pressurized liquid H₂O mixed with NH₃, CH₃OH, H₂O₂, and trace salts.  The movement is slow, planetary-scale currents originating from the Furnace and Coriolis force.  Strong layers exist: the surface is oxidized; the abyssal layer is reducing.&lt;br /&gt;
&lt;br /&gt;
A new &amp;quot;surface&amp;quot; is next.  The &#039;&#039;&#039;Ice Mantle&#039;&#039;&#039; is solid Ice VI and VII.  There are massive, slowly shifting &amp;quot;sub-oceanic continents&amp;quot;. It is periodically fractured and resurfaced by cryoquakes and brine-driven eruptions.  Some regions have developed elevated domes or ridges, continental “shelves” under the ocean.&lt;br /&gt;
&lt;br /&gt;
Finally, underneath is the &#039;&#039;&#039;core&#039;&#039;&#039;. Temperatures exceed 2000–3000 K locally.  Pressures range from 100 to 300 GPa.  The core is rich in heavy elements.  This makes radiogenic hotspots, localized magnetic eddies.  Heat gradients + ion flows = thermoelectric currents.  These make magnetic storms within the ocean itself, not the sky.  When uranium-rich corium pods shift or explode upward through the mantle, their heat and conductivity disturb the local magnetic field, generating geomagnetic quakes.  These pulse through the ocean, creating short-lived magnetic lenses.  These interact with atmospheric charged particles above the Furnace, giving rise to transient magnetic halos visible from orbit—false auroras without a sunstorm.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== e: The Tortured Near-Sphere ====&lt;br /&gt;
[[File:Blasting and shattered.png|thumb|right|An axial recoil event in progress]]&lt;br /&gt;
Orbital and Physical Characteristics&lt;br /&gt;
* Mass: 0.9 Earth masses&lt;br /&gt;
* Radius: 1.0 Earth radii&lt;br /&gt;
* Orbital Period: 58 Earth days&lt;br /&gt;
* Surface Gravity: ~0.9 g&lt;br /&gt;
* Semimajor Axis: ~0.17 AU &lt;br /&gt;
* Spin State: In the &#039;&#039;process&#039;&#039; of becoming tidally locked&lt;br /&gt;
* Obliquity: Extreme, experiencing chaotic realignment events&lt;br /&gt;
&lt;br /&gt;
Internal Structure and Composition&lt;br /&gt;
* &#039;&#039;&#039;Crust:&#039;&#039;&#039; A thick, rigid outer shell of water ice I mixed with clathrates (CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; and CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; hydrates), underlain by layers of ammonia-water ice eutectics. Inclusions of carbon under extreme pressure form diamond strata in the lower crust, lending rigidity and brittle behavior.&lt;br /&gt;
* &#039;&#039;&#039;Mantle:&#039;&#039;&#039; Comprised of Ice VI and Ice VII, with ammonia- and methane-rich brines forming localized conduits and pockets of unstable volatiles.&lt;br /&gt;
* &#039;&#039;&#039;Core:&#039;&#039;&#039; Differentiated and semi-molten. Inner core of iron-nickel alloy spins at a different rate. Outer core is a highly viscous slurry of silicate, iron, carbon, sulfur, and dissolved volatiles. Chemical veins (e.g., uranium silicates, perovskites) act as mechanical shear zones. Tidal torque leads to periodic frictional heating.&lt;br /&gt;
&lt;br /&gt;
Tectonic and Cryovolcanic Behavior&lt;br /&gt;
* The planet resists tidal locking due to core-crust decoupling and uneven angular momentum transfer.&lt;br /&gt;
* High obliquity experiences &#039;&#039;&#039;&#039;&#039;Axial Recoil Events&#039;&#039;&#039;&#039;&#039;, where the entire planet jerks between metastable orientations (e.g., from 110° to 70°) in sudden spasms.&lt;br /&gt;
* These events generate:&lt;br /&gt;
** Global-scale crustal cracking&lt;br /&gt;
** Venting of pressurized subsurface gases (H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;O, CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt;)&lt;br /&gt;
** Surface deformation and glacial faulting&lt;br /&gt;
* Volatiles erupt ballistically into space (200+lm) from exposed fissures and calderas, driven by phase-change explosions.&lt;br /&gt;
&lt;br /&gt;
Surface Conditions&lt;br /&gt;
* Global temperature well below freezing; warmest zones around cryovolcanic hotspots&lt;br /&gt;
* Crustal coloration varies by volatile deposition:&lt;br /&gt;
** Pale blue-white from water ice&lt;br /&gt;
** Red-brown from CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; frostfields&lt;br /&gt;
** Green-black CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; stains from plume fallout&lt;br /&gt;
* Surface features include:&lt;br /&gt;
** Cryovolcanic calderas&lt;br /&gt;
** Diamond-studded impact-like basins&lt;br /&gt;
** Faulted plains crossed by salt-streaked rift zones&lt;br /&gt;
&lt;br /&gt;
Atmosphere and Ejected Material&lt;br /&gt;
* Thin transient exosphere formed from eruptive events&lt;br /&gt;
* Gases often escape to space or freeze back out in polar regions&lt;br /&gt;
* Fallback material creates uneven surface mass distributions, altering moment of inertia and prolonging instability&lt;br /&gt;
&lt;br /&gt;
Appearance from Planet c&lt;br /&gt;
&lt;br /&gt;
* Angular Size: ~4-1 arcminutes&lt;br /&gt;
* Coloration: Overall dusky grey-white, with changing colored bands due to volatile fallout; craterless but mottled&lt;br /&gt;
&lt;br /&gt;
Transient visible phenomena:&lt;br /&gt;
&lt;br /&gt;
* Cryovolcanic plumes visible as fan-like arcs at the limb during outburst events&lt;br /&gt;
* Infrared brightening during Axial Recoil Events&lt;br /&gt;
* Occasional light-scattering halos from plume particles&lt;br /&gt;
&lt;br /&gt;
Event Cycle Summary&lt;br /&gt;
&lt;br /&gt;
# Tidal torque builds due to obliquity misalignment&lt;br /&gt;
# Core resists, crust locks tension&lt;br /&gt;
# Critical stress threshold breached&lt;br /&gt;
# Obliquity lurches to new orientation&lt;br /&gt;
# Crust fractures globally, vents open&lt;br /&gt;
# Supersonic cryovolcanism hurls volatiles into space&lt;br /&gt;
# Fallback modifies crustal mass distribution&lt;br /&gt;
# Obliquity rebuilds instability over decades&lt;br /&gt;
# Repeat.&lt;br /&gt;
&lt;br /&gt;
Planet e is a tortured world caught in an unending cycle of self-correcting failure—its body unable to align, its gases unable to stay contained, its appearance in the sky a visible signature of internal catastrophe.&lt;br /&gt;
&lt;br /&gt;
==== f: Ringed Mini-Neptune ====&lt;br /&gt;
[[File:Ringed Neptune with four moons.png|thumb|right|Aperspectival view of f, its rings, and four moons]]&lt;br /&gt;
This planet is a substantial mini-Neptune, with a mass of approximately 3.5 Earth masses and a radius of 2.0 Earth radii, orbiting at 0.227 AU. Its low mean density (~0.44 ρ⊕) signals the presence of a deep, volatile-rich envelope overlying a denser core. The bulk of its volume is composed of hydrogen and helium, accreted from the protoplanetary disk, with trace amounts of methane (CH₄) and ammonia (NH₃)—gases that dominate its photochemical and radiative behavior. Beneath this envelope, the planet hosts a water–rock–metal core layered in complex phases, with high-pressure ices and possibly superionic water enveloping a metallic center.  Lower atmosphere reaches 300–500 K (27–227°C) near the bottom of the troposphere, depending on opacity and convection.&lt;br /&gt;
&lt;br /&gt;
Visually, the planet exhibits a blue-to-cyan atmospheric hue, governed by Rayleigh scattering and methane absorption in the red and near-infrared spectrum. While not as banded or storm-laced as Jupiter, it features broad zonal flows, high-altitude methane ice clouds, and long-lived anticyclonic storms akin to Neptune’s Great Dark Spot. Due to its tidal locking to the host star, the planet presents hemispheric climatic asymmetry: a sunlit dayside prone to atmospheric upwelling and cloud formation, and a cooler, darker nightside. While colder, the backside is not freezing— in the 150–250 K range, depending on circulation efficiency. Atmospheric circulation is dominated by slow, large-scale overturning cells, moderated by planetary-scale waves and a subdued Coriolis force. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Rings =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Ring!!	Range (Rₚ)!!	Approx.! Range (km)!!	Description&lt;br /&gt;
|-&lt;br /&gt;
! C&lt;br /&gt;
| 	1.5–1.65 Rₚ	||19,100–21,000	||Faint, dusty interior ring&lt;br /&gt;
|-&lt;br /&gt;
! B&lt;br /&gt;
| 	1.65–1.96 Rₚ	||21,000–25,000||	Bright, dense primary ring&lt;br /&gt;
|-&lt;br /&gt;
! Division&lt;br /&gt;
|	1.96–2.04 Rₚ ||25,000–26,000 || a low-density gap&lt;br /&gt;
|-&lt;br /&gt;
!  A&lt;br /&gt;
|	2.04–2.3 Rₚ||26,000–29,300||	Sharp-edged outer ring&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Moon !!	Orbit (km) !!	Orbit (Rₚ) !!	Diameter (km) !!	Type	!! Period !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! I&lt;br /&gt;
|	60,000	||4.7 Rₚ	||~400	||Rocky	|| 0.9 ||Cratered&lt;br /&gt;
|-&lt;br /&gt;
! II&lt;br /&gt;
| 	110,000	|| 8.6 Rₚ	|| ~800	|| Mixed rock/ice	|| 2.25|| Cracked surface, frozen ocean&lt;br /&gt;
|-&lt;br /&gt;
! III &lt;br /&gt;
| 190,000	|| 14.9 Rₚ ||	~1200 ||	Icy major moon ||	5.1|| Cryovolcanism, smooth plains&lt;br /&gt;
|-&lt;br /&gt;
! IV &lt;br /&gt;
|340,000	||26.7 Rₚ	||~200	||Irregular/prograde	|| 12.21 || Dark red/carbon, inclined (20º, eccentric orbit (0.1)&lt;br /&gt;
|-&lt;br /&gt;
! V &lt;br /&gt;
| 710,000 ||	55.7 Rₚ	||~350	|| Captured/retrograde	|| 36.83 || Highly inclined (130º), Split terrain—half rugged highlands, half smooth resurfaced plain&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==== g: Stripped Sub-Neptune Remnant ====&lt;br /&gt;
[[File:Stripped Planet with Two Cool Moons.png|700px|right]]&lt;br /&gt;
Basic Parameters&lt;br /&gt;
* Mass: 2.6 Earth masses (M⊕)&lt;br /&gt;
* Radius: 1.7 Earth radii (R⊕)&lt;br /&gt;
* Mean Density: ~2.92 g/cm³&lt;br /&gt;
* Orbital Distance: 0.4 AU &lt;br /&gt;
* Albedo: ~0.5 (moderately high)&lt;br /&gt;
* Rotation: Tidally locked &lt;br /&gt;
&lt;br /&gt;
Origin and Evolution&lt;br /&gt;
* Formed beyond the snow line (~0.8–1.2 AU) from a mix of rock, iron, and ices&lt;br /&gt;
* Migrated inward early during protoplanetary disk phase&lt;br /&gt;
* Accreted a modest hydrogen-helium envelope (&amp;gt;1% by mass)&lt;br /&gt;
* Exposed to intense stellar X-ray and UV radiation during the M dwarf&#039;s pre-main-sequence phase&lt;br /&gt;
* Lacked a magnetic dynamo (metal-poor and early core freezing)&lt;br /&gt;
* Entire atmosphere lost over ~100 Myr via photoevaporation, core-powered mass loss, and sputtering&lt;br /&gt;
&lt;br /&gt;
Current State&lt;br /&gt;
* Atmosphere: None (trace mineral vapors possible in hot regions)&lt;br /&gt;
* Surface: Stark contrast between hemispheres due to tidal locking&lt;br /&gt;
** Dayside: ~700–1000 K; high-silica lava fields, salt flats, exposed alumino-silicates&lt;br /&gt;
** Nightside: ~100–150 K; gypsum and calcite in cold traps, frozen regolith&lt;br /&gt;
* Magnetosphere: Absent&lt;br /&gt;
* Volcanism:episodic; high-silica flows, volcanic glass, sodium-rich crusts&lt;br /&gt;
* Geological Activity: Tectonically inactive; thermally fractured plains, impact craters&lt;br /&gt;
&lt;br /&gt;
Surface Composition&lt;br /&gt;
* Titanium dioxide (rutile): bright, high-albedo mineral condensate&lt;br /&gt;
* Calcite (CaCO₃): carbonate deposits in cold traps&lt;br /&gt;
* Gypsum (CaSO₄·2H₂O): hydration mineral, stable only on the nightside&lt;br /&gt;
* Sodium chloride: salt flats, especially in evaporated basins&lt;br /&gt;
* High-silica volcanic deposits: glassy, oxidized, and light-colored&lt;br /&gt;
&lt;br /&gt;
Visual and Observational Notes&lt;br /&gt;
&lt;br /&gt;
* High visual contrast between molten and frozen hemispheres&lt;br /&gt;
* Surface appears mottled: obsidian-black lava, gleaming salt flats, white calcium deposits&lt;br /&gt;
* No clouds, auroras, or magnetic activity&lt;br /&gt;
* Extreme day/night temperature gradient&lt;br /&gt;
* Reflective phase curve possible in photometric observations&lt;br /&gt;
* Surface pressure: effectively 0 bar&lt;br /&gt;
&lt;br /&gt;
Planet g is the airless skeleton of a once-sub-Neptune world. Born icy and distant, it migrated into the young star&#039;s wrath, where its fragile envelope boiled away under a sky of flares. Bereft of a magnetic shield, it was slowly stripped to bare rock. Today, one hemisphere bakes in molten silence while the other freezes in shadow. No air, no oceans, only salt, stone, and the echo of a lost atmosphere.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property !!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~75,000 km (~0.26 R&amp;lt;sub&amp;gt;hill&amp;lt;/sub&amp;gt;)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~1,400 km (~0.22 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass	&lt;br /&gt;
| ~0.01 M⊕ (~1.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~3.0 g/cm³ (rock–ice mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temp&lt;br /&gt;
|	~150–180 K&lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
| 0.20g&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere&lt;br /&gt;
|	Trace O₂, from radiolysis and outgassing&lt;br /&gt;
|-&lt;br /&gt;
! Subsurface Ocean&lt;br /&gt;
|	heated by tidal flexing&lt;br /&gt;
|-&lt;br /&gt;
! Surface Features	&lt;br /&gt;
|Fractured ice crust, chaos terrain, cryogeysers, lenticulae&lt;br /&gt;
|}&lt;br /&gt;
gI is a cracked glass orb, rimed with frost and laced with luminous fissures. Below its crust, tides flex a hidden ocean in rhythmic silence. Its faint oxygen exosphere is ghostly but present.  It is frosted quartz with cobwebbed streaks and mineral discoloration.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property!!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~150,000 km (~0.5 Rₕill)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~2,100 km (~0.33 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass&lt;br /&gt;
|	~0.035 M⊕ (~4.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~2.1 g/cm³ (icy-rocky mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes &lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
|	~0.35 g&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temperature&lt;br /&gt;
|	~115–130 K (pressure and greenhouse effects)&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere	&lt;br /&gt;
| ~0.18 bar N₂ + ~0.1 bar Ar + ~0.02 bar CH₄, minor CO, trace haze &lt;br /&gt;
|}&lt;br /&gt;
gII is a muted blue-green crescent veiled in gold. Its sky glows with the weight of argon and the shimmer of methane haze, and its surface smolders with the memory of internal warmth. Liquid hydrocarbons shine like ink in the basins, while glaciers ebb across the uplands. To the star it shows only one face, but beneath that still gaze lies the soft breath of a world more welcoming than its master.&lt;br /&gt;
&lt;br /&gt;
== Planet C ==&lt;br /&gt;
[[File:Planet C and its tethered moon.png|right|700px]]&lt;br /&gt;
* With an albedo of 0.2, the global average temp is 263ºK.  Because of modest greenhouse effects, surface temperatures are higher, on the sun-side.&lt;br /&gt;
# Mass: 1.5M⊕&lt;br /&gt;
# Gravity: 1g⊕&lt;br /&gt;
# Radius = 1.225⊕, or 7805km&lt;br /&gt;
Terminator Zone&lt;br /&gt;
# +/-30º: 1.28 E8 km&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; (slightly less than all the land of the Earth)&lt;br /&gt;
# Escape velocity is 12.4km/s, 11% higher than Earth&lt;br /&gt;
# Orbital velocity is 8.79km/s&lt;br /&gt;
=== Atmosphere ===&lt;br /&gt;
Water content is low because&lt;br /&gt;
* Water vapor is a potent greenhouse gas; vast surface water can trap too much heat, especially near the substellar point.&lt;br /&gt;
* Water leads to climate homogenization&lt;br /&gt;
* Lack of exposed silicate rock: Necessary for carbon-silicate weathering feedback, which stabilizes climate on geological timescales.&lt;br /&gt;
Earth has ~1.4 billion km³ of water.  In our habitable zone, we have no more than 10% of that, or 100 million km³, though there is much more on the night side, both liquid and ice.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Factor !! Ɬiʔa atm !! Ɬiʔa % !! Earth atm !! Earth % !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! Total Pressure &lt;br /&gt;
| 1.6 atm || || 1.0 atm || || Enhanced convective heat transfer, increased IR trapping&lt;br /&gt;
|-&lt;br /&gt;
! Nitrogen (N₂) &lt;br /&gt;
| 1.00 || 62.50% || 0.7808 || 78.08% || Reduced; still inert, still dominant&lt;br /&gt;
|-&lt;br /&gt;
! Oxygen (O₂) &lt;br /&gt;
| 0.21 || 13.13% || 0.2095 || 20.95% || Earth-normal partial pressure &lt;br /&gt;
|-&lt;br /&gt;
! Argon (Ar)&lt;br /&gt;
| 0.40 || 25.00% || 0.0093 || 0.93% || Major heat distribution enhancement, inert&lt;br /&gt;
|-&lt;br /&gt;
! Krypton + Xenon&lt;br /&gt;
| 0.005 || 0.31% || trace || trace || High molecular mass → improved heat retention, still safe&lt;br /&gt;
|-&lt;br /&gt;
! CO₂&lt;br /&gt;
| 0.005 || 0.31% || 0.004 || 0.04% || slightly elevated; sub-greenhouse threshold&lt;br /&gt;
|-&lt;br /&gt;
! H₂O vapor &lt;br /&gt;
| 0.015 || ~1% || || 0-4% || Maintains greenhouse without excess moisture&lt;br /&gt;
|}&lt;br /&gt;
==== Atmospheric Effects on Clouds ====&lt;br /&gt;
# Increased Pressure (1.6 atm) compresses gases, raising the dew point at which water vapor condenses. Clouds form closer to the surface, and are denser than similar altitudes compared to Earth.&lt;br /&gt;
# Low Water Inventory (~20% of Earth&#039;s): less frequent and less massive cloud systems than on Earth, but still present—especially over &amp;quot;hotspots&amp;quot; on the day side.&lt;br /&gt;
# Tidally Locked Climate: Cloud formation concentrate along the substellar point, where warm, moist air rises and cools.&lt;br /&gt;
#* A permanent “eyewall” storm system has formed at the subsolar point, like a giant hurricane.&lt;br /&gt;
#* As air rises and is advected to the night side, thin cloud bands or ice hazes form as it descends and cools.&lt;br /&gt;
&lt;br /&gt;
Appearance:&lt;br /&gt;
* The presence of noble gases (Ar, Kr, Xe) and higher pressure enhance Mie scattering, making clouds appear whiter and more silvered, especially at sunrise/sunset boundaries.&lt;br /&gt;
* Night side clouds are thin, high-altitude icy sheets, glowing faintly in aurorae or thermal emissions.&lt;br /&gt;
&lt;br /&gt;
==== Sky Color ====&lt;br /&gt;
[[File:Life near the terminator.png|thumb|right|Life near the terminator]]&lt;br /&gt;
The color of the sky is shaped by Rayleigh scattering, which depends on:&lt;br /&gt;
# Molecular composition: Heavier gases like Ar, Kr, and Xe scatter light less efficiently than N₂.&lt;br /&gt;
# Spectral output of the star: the red dwarf emits predominantly infrared and red light, with very little blue or violet.&lt;br /&gt;
&lt;br /&gt;
Consequence:&lt;br /&gt;
* Even with atmospheric scattering, there is insufficient blue light in the stellar spectrum to produce a blue sky.&lt;br /&gt;
* Day sky would likely appear:&lt;br /&gt;
** Dark peach, dusky rose, or reddish beige near zenith,&lt;br /&gt;
** Grading to deep salmon or mauve near the horizon,&lt;br /&gt;
** A slight metallic sheen due to noble gas content and high pressure.&lt;br /&gt;
&lt;br /&gt;
Twilight &amp;amp; Limb Scattering:&lt;br /&gt;
* The terminator (twilight zone) sees a diffuse, ruddy light, scattering through haze and clouds into luminous reds, purples, and copper tones.&lt;br /&gt;
* Aurorae are spectacular on the night side, especially since stellar flares are frequent.&lt;br /&gt;
&lt;br /&gt;
==== Sound Propagation ====&lt;br /&gt;
: &#039;&#039;Sound is profoundly affected by atmospheric pressure and composition.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Compared to Earth:&lt;br /&gt;
* Higher pressure → greater air density → faster transmission of sound and less attenuation.&lt;br /&gt;
* Argon and Xenon are heavy gases, which:&lt;br /&gt;
** Lower the speed of sound relative to air at the same pressure (despite the pressure increase).&lt;br /&gt;
** Shift resonance frequencies downward, resulting in deeper, rounder sounds.&lt;br /&gt;
&lt;br /&gt;
Consequences:&lt;br /&gt;
* Voices sound subtly lower-pitched and richer, especially for consonants and low vowels.&lt;br /&gt;
* Ambient sounds (wind, water, animals) would carry farther and sound more muffled or sonorous.&lt;br /&gt;
* Music or speech would resonate more warmly, especially indoors or in enclosed spaces.&lt;br /&gt;
&lt;br /&gt;
In short: it sounds like it’s wrapped in velvet.&lt;br /&gt;
&lt;br /&gt;
==== Heat Transport to the Night Side ====&lt;br /&gt;
Mechanisms:&lt;br /&gt;
# Thick Atmosphere (1.6 atm) increases:&lt;br /&gt;
#* Advection efficiency: Warm air masses can move more heat horizontally.&lt;br /&gt;
#* Radiative time constant: The atmosphere holds heat longer before releasing it.&lt;br /&gt;
# Noble Gases (especially Kr/Xe):&lt;br /&gt;
#* High molecular mass → more IR opacity → trapping and radiating heat more evenly.&lt;br /&gt;
# Slow Rotation / Tidal Locking:&lt;br /&gt;
#* Global Hadley-like cells dominate circulation, carrying warm air from the day side to the night side and descending it there.&lt;br /&gt;
&lt;br /&gt;
Result:&lt;br /&gt;
* The night side is not so freezing.  Temperatures differ by tens of degrees, not hundreds.&lt;br /&gt;
* There are still ice caps and a cold deserts at the anti-stellar point, but not a glaciated wasteland.&lt;br /&gt;
&lt;br /&gt;
=== Magnetosphere ===&lt;br /&gt;
* Larger mass --&amp;gt; larger iron core, generating more internal heat&lt;br /&gt;
* Larger radius --&amp;gt; Vigorous convection in the core&lt;br /&gt;
* Tidal Flexing --&amp;gt; still drives magnetic activity&lt;br /&gt;
&lt;br /&gt;
# Aurorae at lower latitudes&lt;br /&gt;
## higher magnetic rigidity, wider magnetotail, and greater reconnection energy.&lt;br /&gt;
## Combined with a higher flux of stellar particles, this means:&lt;br /&gt;
### Auroral ovals expand, reaching mid-latitudes sometimes equator.&lt;br /&gt;
### The skies are alive with rippling green, violet, and crimson aurorae, especially on the night side.&lt;br /&gt;
### Daily auroral activity occur during stellar flare cycles.&lt;br /&gt;
# Compasses&lt;br /&gt;
## compasses respond more sharply, with:&lt;br /&gt;
### Faster alignment.&lt;br /&gt;
### Greater resistance to local perturbations.&lt;br /&gt;
## However, frequent magnetic storms from stellar activity cause sudden declinations, reversals, or local anomalies.  In short, lots of aurorae equals dead compasses at the same time.&lt;br /&gt;
# Magnetic Field Strength &amp;gt; 100 μT &lt;br /&gt;
# Electromagnetism is more basic than chemistry or almost any other natural philosophy&lt;br /&gt;
&lt;br /&gt;
=== Substellar Point ===&lt;br /&gt;
The maximum incoming flux is very nearly the same as Earth&#039;s solar constant (≈1361 W/m²), but concentrated over one point rather than averaged over a rotating sphere.  Temperatures should be above 500ºK most of the time.  &lt;br /&gt;
&lt;br /&gt;
The magnetic north is also here. The thick atmosphere prevents too much loss here, but &lt;br /&gt;
* Charged particle influx&lt;br /&gt;
** Maximized at the substellar point—intense auroral and energetic particle precipitation&lt;br /&gt;
* Atmospheric ionization&lt;br /&gt;
** Constant production of high-energy ions and NOx compounds—UV fluorescence in upper sky&lt;br /&gt;
* Localized heating&lt;br /&gt;
** Augments already extreme temperatures—600–700 K surface&lt;br /&gt;
&lt;br /&gt;
== Artificially Tethered Moon ==&lt;br /&gt;
* 670,000 km up&lt;br /&gt;
* 7805 km in radius = same as the planet&lt;br /&gt;
* 1.33º of the sky, same as the sun&lt;br /&gt;
&lt;br /&gt;
A network of tethers/tension lines from the moon to multiple anchor points on the planet’s surface (a tripod or hexapod structure), woven like hair&lt;br /&gt;
* Uses active tension management and orbital station-keeping to stabilize the moon&lt;br /&gt;
* Counterweights and inward-pointing mass drivers on the moon to oppose drift&lt;br /&gt;
&lt;br /&gt;
The tethers are not bearing the full weight, but merely damping drift, providing restoring force, and enabling long-term stability through active compensation.  The moon&lt;br /&gt;
* Blocks the worst of the heat&lt;br /&gt;
* Blocks the worst of the solar radiation&lt;br /&gt;
The moon has &lt;br /&gt;
* low mass&lt;br /&gt;
* high albedo - enormous reflectivity&lt;br /&gt;
* scatters charges particles, UV, X-rays, auroral flux tubes&lt;br /&gt;
* sunward - crazy hot, high emissivity&lt;br /&gt;
* earthward - crazy cool, low emissivity&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168773</id>
		<title>Ɬiʔa/Conworlding</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168773"/>
		<updated>2025-04-06T23:29:18Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* Solar System */ asteroid fields&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Star ==&lt;br /&gt;
The star is a red-dwarf (M5V) named Gliese 710b minoris, or informally &#039;&#039;Mirar&#039;s Veil&#039;&#039;.  It is 7.9 light-years (≈2.42 parsecs) from Sol, toward the galactic plane, in Scorpius–Ophiuchus.  It lies just &amp;quot;behind&amp;quot; a brighter, well-known K-dwarf, and was not observed until after humanity&#039;s trip to Proxima Centauri: in situ gravitational navigation by the first robotic probe en route to Proxima Centauri. The probe’s optical gyros noticed an unmodeled gravitational perturbation.&lt;br /&gt;
&lt;br /&gt;
* Stellar luminosity (L*) ≈ 0.01 𝐿⊙ (1/100th Sol&#039;s brightness)&lt;br /&gt;
* Stellar mass (M*) ≈ 0.2 𝑀⊙ (1/5 the mass of Sol)&lt;br /&gt;
* Stellar radius (R*) ≈ 0.25 𝑅⊙ (1/4 as wide as Sol)&lt;br /&gt;
* Effective temperature (T*) ≈ 3500 K&lt;br /&gt;
* Average surface field is ~1.5 kG, with frequent bursts of &amp;gt; 3kG&lt;br /&gt;
** Frequent, energetic flares, multiple per day, with for extreme variability over time, often above 10&amp;lt;sup&amp;gt;35&amp;lt;/sup&amp;gt; erg&lt;br /&gt;
* The frostline is at 0.27 AU&lt;br /&gt;
&lt;br /&gt;
​The habitable zone (a) is about square root of L* over L⊙, so ~0.1 AU.&lt;br /&gt;
&lt;br /&gt;
=== Solar System ===&lt;br /&gt;
There are seven planets in the system&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Planet !!	Mass (M🜨)!!	Radius (R🜨)!! Moons/Rings	!!Resonance !!	&amp;lt;small&amp;gt;Semi-Major&amp;lt;/small&amp;gt; !!	Rings !! Moons !! Period !! Size !! Type !! Sidereal !! A. Mag.&lt;br /&gt;
|-&lt;br /&gt;
| b ||	2.17 ||	1.1 ||	No ||	2:3 with c	|| 0.0763 ||	No || No || 17.2 || 13.6&#039; to 1.5&#039; || Super-Mercury || 51.6 || -10.98&lt;br /&gt;
|-&lt;br /&gt;
| c ||	1.5	 ||1.225 ||	1* ||	—	        || 0.100  || No    || No || 25.8 || - || Super-Earth || - || - &lt;br /&gt;
|-&lt;br /&gt;
| d ||	2.0	 ||1.4 ||No ||	2:3 with c	 ||0.131 ||	No || No || 38.7 || 13.1&#039; to 1.8&#039; || Super Waterworld || 77.4 || -11.85&lt;br /&gt;
|-&lt;br /&gt;
| e ||	0.9 ||	1.0 || No	 ||	2:3 with d	 ||0.172 ||	No || No || 58 || 4.1&#039; to 1.1&#039; || Cracked Earth || 46.44 || -8.86&lt;br /&gt;
|- &lt;br /&gt;
| f ||	3.5 ||	2.0 ||	Yes! ||	2:3 with e	 ||0.227 || Yes || Junk || 87 || 4.6&#039; to 1.8&#039; || Mini-Neptune || 36.66 || -9.78&lt;br /&gt;
|-&lt;br /&gt;
| AB || 0.004 || - || 1-300km || 3:2 with f || ~0.3 || - || - || ~60 || - || Fe, Ni, Ar || - || -&lt;br /&gt;
|-&lt;br /&gt;
| g ||	2.6 ||	1.7 ||	2 ||	-	 ||0.40 ||	Yes || Junk || 206 || 1.6&#039; to 1.0&#039; || Stripped Neptune || 29.5 || -7.16&lt;br /&gt;
|-&lt;br /&gt;
| h ||	5.0x2 ||2.3x2 || yes	 || -	 ||1.5 ||	Yes || No || 1500 || 0.5&#039; 16.4&#039; apart (at max) || Double Neptune || 26.25 || -5.43&lt;br /&gt;
|-&lt;br /&gt;
| CDD || 0.1 || - || 1-100km || - || 3-10 || - || - || 2000-11500 || - || H₂O, CO₂, CH₄, Ar || - || 75ºK&lt;br /&gt;
|}&lt;br /&gt;
==== b: super Mercury with a ring of fire  ====&lt;br /&gt;
[[File:planet b by GPT.png|thumb|right|An artistic rendering of planet b]]&lt;br /&gt;
b is a super-Mercury, tidally locked, and incredibly dense.  ~700ºK on the day side, ~50ºK on the night.  2.1 Earth Masses, 1.1 Earth radii (~7000km) in size.  Orbital period 17.2 days.  Density 9.0 g/cm&amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt;.  Gravity is ~1.8g.  &lt;br /&gt;
&lt;br /&gt;
The iron core is huge, being 75% of the mass.  A thin silicate mantle, with metallic plains and exhumed ultramafic crust, with frequent iron meteorite craters, lacking typical “stone” breccias.&lt;br /&gt;
&lt;br /&gt;
The night side is intense, as simple hydrocarbons (methane, ethane, propane) condense and freeze into layered deposits.  Complex organics (tholins, polycyclic aromatics) accumulate on the sea floor, under miles of nitrogen ice.  Massive slush layers slosh around above cryovolcanic brines of ammonia.&lt;br /&gt;
&lt;br /&gt;
There is a crucial layer of Superionic Ice XI above the core, which acts as an electromagnetic insulator, and ionic heat bridge.  The crust is ultramafic silicates (olivine, pyroxene, perovskite) riddled with with sulfide veins, iron alloys, and graphite networks.  The poles of the magnetosphere are sideways, like Uranus, with poles at the equator in the Terminator Zone.  Persistent surface charges develop, because the whole planet is basically a ginormous Leyden jar!&lt;br /&gt;
&lt;br /&gt;
A planetary flux rope forms and un-forms with the star and planet b.  This induces electric jets at the terminator.  This is where temps are Earth-like.  Hydrocarbons sublimate and eject into the atmosphere, even while aurorae come right down to the ground.  A small, low pressure atmosphere prevents photodissociation, even while electrothermal instabilities lift molecules, forming an anomalous haze, a standing, glowing ring.  Coronal events cause localized lightning geysers with magnetic arcing.&lt;br /&gt;
&lt;br /&gt;
In short, b is visible with a blinding bright sun side (glowing orange bronze), a utterly black night side, and a burning, glowing, erupting, arcing ring at the terminator (all colors).  At biggest, it&#039;s half the size of Earth&#039;s moon in the sky, shrinking down to a star at it&#039;s furthest away.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== d: the wet eye with depths ====&lt;br /&gt;
[[File:wet eye planet.png|thumb|right|An reasonable approximation of d&#039;s appearance]]&lt;br /&gt;
From the outside, d is a &amp;quot;wet eye&amp;quot; just outside the habitable zone.  It is a water world, twice the mass of Earth, 1.4 times the radius, tidally locked.  The substellar point is the only place without surface ice.  However, it is better to think of the planet top-to-bottom.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;atmosphere&#039;&#039;&#039; is tenuous, less than 0.2 bars.  It is thin, N₂-rich with traces of H₂O, NH₃ vapor, and transient geyser outputs.  It is highly UV-irradiated, and Mars-like in its inability to retain volatiles.&lt;br /&gt;
&lt;br /&gt;
Next, there is a &#039;&#039;&#039;surface ice shell&#039;&#039;&#039;, ~20 km of thick Ice I.  Swirling currents beneath have cracked continent-sized ice plates, similar to Europa&#039;s crust.  It is permanently frozen except at the substellar furnace.  It accumulates chemical stains, mineral deposits, and cryovolcanic eruption plumes.  Accumulations of complex hydrates—like methanol clathrates—precipitate out and form false reefs, rising like coral from beneath. Transient thermal vents push hot plumes into the thin air, freezing instantly and snowing down crystals that form mineral spires.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;subglacial ocean&#039;&#039;&#039; is hundreds of kilometers thick.  It is super-pressurized liquid H₂O mixed with NH₃, CH₃OH, H₂O₂, and trace salts.  The movement is slow, planetary-scale currents originating from the Furnace and Coriolis force.  Strong layers exist: the surface is oxidized; the abyssal layer is reducing.&lt;br /&gt;
&lt;br /&gt;
A new &amp;quot;surface&amp;quot; is next.  The &#039;&#039;&#039;Ice Mantle&#039;&#039;&#039; is solid Ice VI and VII.  There are massive, slowly shifting &amp;quot;sub-oceanic continents&amp;quot;. It is periodically fractured and resurfaced by cryoquakes and brine-driven eruptions.  Some regions have developed elevated domes or ridges, continental “shelves” under the ocean.&lt;br /&gt;
&lt;br /&gt;
Finally, underneath is the &#039;&#039;&#039;core&#039;&#039;&#039;. Temperatures exceed 2000–3000 K locally.  Pressures range from 100 to 300 GPa.  The core is rich in heavy elements.  This makes radiogenic hotspots, localized magnetic eddies.  Heat gradients + ion flows = thermoelectric currents.  These make magnetic storms within the ocean itself, not the sky.  When uranium-rich corium pods shift or explode upward through the mantle, their heat and conductivity disturb the local magnetic field, generating geomagnetic quakes.  These pulse through the ocean, creating short-lived magnetic lenses.  These interact with atmospheric charged particles above the Furnace, giving rise to transient magnetic halos visible from orbit—false auroras without a sunstorm.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== e: The Tortured Near-Sphere ====&lt;br /&gt;
[[File:Blasting and shattered.png|thumb|right|An axial recoil event in progress]]&lt;br /&gt;
Orbital and Physical Characteristics&lt;br /&gt;
* Mass: 0.9 Earth masses&lt;br /&gt;
* Radius: 1.0 Earth radii&lt;br /&gt;
* Orbital Period: 58 Earth days&lt;br /&gt;
* Surface Gravity: ~0.9 g&lt;br /&gt;
* Semimajor Axis: ~0.17 AU &lt;br /&gt;
* Spin State: In the &#039;&#039;process&#039;&#039; of becoming tidally locked&lt;br /&gt;
* Obliquity: Extreme, experiencing chaotic realignment events&lt;br /&gt;
&lt;br /&gt;
Internal Structure and Composition&lt;br /&gt;
* &#039;&#039;&#039;Crust:&#039;&#039;&#039; A thick, rigid outer shell of water ice I mixed with clathrates (CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; and CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; hydrates), underlain by layers of ammonia-water ice eutectics. Inclusions of carbon under extreme pressure form diamond strata in the lower crust, lending rigidity and brittle behavior.&lt;br /&gt;
* &#039;&#039;&#039;Mantle:&#039;&#039;&#039; Comprised of Ice VI and Ice VII, with ammonia- and methane-rich brines forming localized conduits and pockets of unstable volatiles.&lt;br /&gt;
* &#039;&#039;&#039;Core:&#039;&#039;&#039; Differentiated and semi-molten. Inner core of iron-nickel alloy spins at a different rate. Outer core is a highly viscous slurry of silicate, iron, carbon, sulfur, and dissolved volatiles. Chemical veins (e.g., uranium silicates, perovskites) act as mechanical shear zones. Tidal torque leads to periodic frictional heating.&lt;br /&gt;
&lt;br /&gt;
Tectonic and Cryovolcanic Behavior&lt;br /&gt;
* The planet resists tidal locking due to core-crust decoupling and uneven angular momentum transfer.&lt;br /&gt;
* High obliquity experiences &#039;&#039;&#039;&#039;&#039;Axial Recoil Events&#039;&#039;&#039;&#039;&#039;, where the entire planet jerks between metastable orientations (e.g., from 110° to 70°) in sudden spasms.&lt;br /&gt;
* These events generate:&lt;br /&gt;
** Global-scale crustal cracking&lt;br /&gt;
** Venting of pressurized subsurface gases (H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;O, CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt;)&lt;br /&gt;
** Surface deformation and glacial faulting&lt;br /&gt;
* Volatiles erupt ballistically into space (200+lm) from exposed fissures and calderas, driven by phase-change explosions.&lt;br /&gt;
&lt;br /&gt;
Surface Conditions&lt;br /&gt;
* Global temperature well below freezing; warmest zones around cryovolcanic hotspots&lt;br /&gt;
* Crustal coloration varies by volatile deposition:&lt;br /&gt;
** Pale blue-white from water ice&lt;br /&gt;
** Red-brown from CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; frostfields&lt;br /&gt;
** Green-black CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; stains from plume fallout&lt;br /&gt;
* Surface features include:&lt;br /&gt;
** Cryovolcanic calderas&lt;br /&gt;
** Diamond-studded impact-like basins&lt;br /&gt;
** Faulted plains crossed by salt-streaked rift zones&lt;br /&gt;
&lt;br /&gt;
Atmosphere and Ejected Material&lt;br /&gt;
* Thin transient exosphere formed from eruptive events&lt;br /&gt;
* Gases often escape to space or freeze back out in polar regions&lt;br /&gt;
* Fallback material creates uneven surface mass distributions, altering moment of inertia and prolonging instability&lt;br /&gt;
&lt;br /&gt;
Appearance from Planet c&lt;br /&gt;
&lt;br /&gt;
* Angular Size: ~4-1 arcminutes&lt;br /&gt;
* Coloration: Overall dusky grey-white, with changing colored bands due to volatile fallout; craterless but mottled&lt;br /&gt;
&lt;br /&gt;
Transient visible phenomena:&lt;br /&gt;
&lt;br /&gt;
* Cryovolcanic plumes visible as fan-like arcs at the limb during outburst events&lt;br /&gt;
* Infrared brightening during Axial Recoil Events&lt;br /&gt;
* Occasional light-scattering halos from plume particles&lt;br /&gt;
&lt;br /&gt;
Event Cycle Summary&lt;br /&gt;
&lt;br /&gt;
# Tidal torque builds due to obliquity misalignment&lt;br /&gt;
# Core resists, crust locks tension&lt;br /&gt;
# Critical stress threshold breached&lt;br /&gt;
# Obliquity lurches to new orientation&lt;br /&gt;
# Crust fractures globally, vents open&lt;br /&gt;
# Supersonic cryovolcanism hurls volatiles into space&lt;br /&gt;
# Fallback modifies crustal mass distribution&lt;br /&gt;
# Obliquity rebuilds instability over decades&lt;br /&gt;
# Repeat.&lt;br /&gt;
&lt;br /&gt;
Planet e is a tortured world caught in an unending cycle of self-correcting failure—its body unable to align, its gases unable to stay contained, its appearance in the sky a visible signature of internal catastrophe.&lt;br /&gt;
&lt;br /&gt;
==== f: Ringed Mini-Neptune ====&lt;br /&gt;
[[File:Ringed Neptune with four moons.png|thumb|right|Aperspectival view of f, its rings, and four moons]]&lt;br /&gt;
This planet is a substantial mini-Neptune, with a mass of approximately 3.5 Earth masses and a radius of 2.0 Earth radii, orbiting at 0.227 AU. Its low mean density (~0.44 ρ⊕) signals the presence of a deep, volatile-rich envelope overlying a denser core. The bulk of its volume is composed of hydrogen and helium, accreted from the protoplanetary disk, with trace amounts of methane (CH₄) and ammonia (NH₃)—gases that dominate its photochemical and radiative behavior. Beneath this envelope, the planet hosts a water–rock–metal core layered in complex phases, with high-pressure ices and possibly superionic water enveloping a metallic center.  Lower atmosphere reaches 300–500 K (27–227°C) near the bottom of the troposphere, depending on opacity and convection.&lt;br /&gt;
&lt;br /&gt;
Visually, the planet exhibits a blue-to-cyan atmospheric hue, governed by Rayleigh scattering and methane absorption in the red and near-infrared spectrum. While not as banded or storm-laced as Jupiter, it features broad zonal flows, high-altitude methane ice clouds, and long-lived anticyclonic storms akin to Neptune’s Great Dark Spot. Due to its tidal locking to the host star, the planet presents hemispheric climatic asymmetry: a sunlit dayside prone to atmospheric upwelling and cloud formation, and a cooler, darker nightside. While colder, the backside is not freezing— in the 150–250 K range, depending on circulation efficiency. Atmospheric circulation is dominated by slow, large-scale overturning cells, moderated by planetary-scale waves and a subdued Coriolis force. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Rings =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Ring!!	Range (Rₚ)!!	Approx.! Range (km)!!	Description&lt;br /&gt;
|-&lt;br /&gt;
! C&lt;br /&gt;
| 	1.5–1.65 Rₚ	||19,100–21,000	||Faint, dusty interior ring&lt;br /&gt;
|-&lt;br /&gt;
! B&lt;br /&gt;
| 	1.65–1.96 Rₚ	||21,000–25,000||	Bright, dense primary ring&lt;br /&gt;
|-&lt;br /&gt;
! Division&lt;br /&gt;
|	1.96–2.04 Rₚ ||25,000–26,000 || a low-density gap&lt;br /&gt;
|-&lt;br /&gt;
!  A&lt;br /&gt;
|	2.04–2.3 Rₚ||26,000–29,300||	Sharp-edged outer ring&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Moon !!	Orbit (km) !!	Orbit (Rₚ) !!	Diameter (km) !!	Type	!! Period !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! I&lt;br /&gt;
|	60,000	||4.7 Rₚ	||~400	||Rocky	|| 0.9 ||Cratered&lt;br /&gt;
|-&lt;br /&gt;
! II&lt;br /&gt;
| 	110,000	|| 8.6 Rₚ	|| ~800	|| Mixed rock/ice	|| 2.25|| Cracked surface, frozen ocean&lt;br /&gt;
|-&lt;br /&gt;
! III &lt;br /&gt;
| 190,000	|| 14.9 Rₚ ||	~1200 ||	Icy major moon ||	5.1|| Cryovolcanism, smooth plains&lt;br /&gt;
|-&lt;br /&gt;
! IV &lt;br /&gt;
|340,000	||26.7 Rₚ	||~200	||Irregular/prograde	|| 12.21 || Dark red/carbon, inclined (20º, eccentric orbit (0.1)&lt;br /&gt;
|-&lt;br /&gt;
! V &lt;br /&gt;
| 710,000 ||	55.7 Rₚ	||~350	|| Captured/retrograde	|| 36.83 || Highly inclined (130º), Split terrain—half rugged highlands, half smooth resurfaced plain&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==== g: Stripped Sub-Neptune Remnant ====&lt;br /&gt;
[[File:Stripped Planet with Two Cool Moons.png|700px|right]]&lt;br /&gt;
Basic Parameters&lt;br /&gt;
* Mass: 2.6 Earth masses (M⊕)&lt;br /&gt;
* Radius: 1.7 Earth radii (R⊕)&lt;br /&gt;
* Mean Density: ~2.92 g/cm³&lt;br /&gt;
* Orbital Distance: 0.4 AU &lt;br /&gt;
* Albedo: ~0.5 (moderately high)&lt;br /&gt;
* Rotation: Tidally locked &lt;br /&gt;
&lt;br /&gt;
Origin and Evolution&lt;br /&gt;
* Formed beyond the snow line (~0.8–1.2 AU) from a mix of rock, iron, and ices&lt;br /&gt;
* Migrated inward early during protoplanetary disk phase&lt;br /&gt;
* Accreted a modest hydrogen-helium envelope (&amp;gt;1% by mass)&lt;br /&gt;
* Exposed to intense stellar X-ray and UV radiation during the M dwarf&#039;s pre-main-sequence phase&lt;br /&gt;
* Lacked a magnetic dynamo (metal-poor and early core freezing)&lt;br /&gt;
* Entire atmosphere lost over ~100 Myr via photoevaporation, core-powered mass loss, and sputtering&lt;br /&gt;
&lt;br /&gt;
Current State&lt;br /&gt;
* Atmosphere: None (trace mineral vapors possible in hot regions)&lt;br /&gt;
* Surface: Stark contrast between hemispheres due to tidal locking&lt;br /&gt;
** Dayside: ~700–1000 K; high-silica lava fields, salt flats, exposed alumino-silicates&lt;br /&gt;
** Nightside: ~100–150 K; gypsum and calcite in cold traps, frozen regolith&lt;br /&gt;
* Magnetosphere: Absent&lt;br /&gt;
* Volcanism:episodic; high-silica flows, volcanic glass, sodium-rich crusts&lt;br /&gt;
* Geological Activity: Tectonically inactive; thermally fractured plains, impact craters&lt;br /&gt;
&lt;br /&gt;
Surface Composition&lt;br /&gt;
* Titanium dioxide (rutile): bright, high-albedo mineral condensate&lt;br /&gt;
* Calcite (CaCO₃): carbonate deposits in cold traps&lt;br /&gt;
* Gypsum (CaSO₄·2H₂O): hydration mineral, stable only on the nightside&lt;br /&gt;
* Sodium chloride: salt flats, especially in evaporated basins&lt;br /&gt;
* High-silica volcanic deposits: glassy, oxidized, and light-colored&lt;br /&gt;
&lt;br /&gt;
Visual and Observational Notes&lt;br /&gt;
&lt;br /&gt;
* High visual contrast between molten and frozen hemispheres&lt;br /&gt;
* Surface appears mottled: obsidian-black lava, gleaming salt flats, white calcium deposits&lt;br /&gt;
* No clouds, auroras, or magnetic activity&lt;br /&gt;
* Extreme day/night temperature gradient&lt;br /&gt;
* Reflective phase curve possible in photometric observations&lt;br /&gt;
* Surface pressure: effectively 0 bar&lt;br /&gt;
&lt;br /&gt;
Planet g is the airless skeleton of a once-sub-Neptune world. Born icy and distant, it migrated into the young star&#039;s wrath, where its fragile envelope boiled away under a sky of flares. Bereft of a magnetic shield, it was slowly stripped to bare rock. Today, one hemisphere bakes in molten silence while the other freezes in shadow. No air, no oceans, only salt, stone, and the echo of a lost atmosphere.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property !!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~75,000 km (~0.26 R&amp;lt;sub&amp;gt;hill&amp;lt;/sub&amp;gt;)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~1,400 km (~0.22 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass	&lt;br /&gt;
| ~0.01 M⊕ (~1.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~3.0 g/cm³ (rock–ice mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temp&lt;br /&gt;
|	~150–180 K&lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
| 0.20g&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere&lt;br /&gt;
|	Trace O₂, from radiolysis and outgassing&lt;br /&gt;
|-&lt;br /&gt;
! Subsurface Ocean&lt;br /&gt;
|	heated by tidal flexing&lt;br /&gt;
|-&lt;br /&gt;
! Surface Features	&lt;br /&gt;
|Fractured ice crust, chaos terrain, cryogeysers, lenticulae&lt;br /&gt;
|}&lt;br /&gt;
gI is a cracked glass orb, rimed with frost and laced with luminous fissures. Below its crust, tides flex a hidden ocean in rhythmic silence. Its faint oxygen exosphere is ghostly but present.  It is frosted quartz with cobwebbed streaks and mineral discoloration.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property!!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~150,000 km (~0.5 Rₕill)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~2,100 km (~0.33 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass&lt;br /&gt;
|	~0.035 M⊕ (~4.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~2.1 g/cm³ (icy-rocky mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes &lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
|	~0.35 g&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temperature&lt;br /&gt;
|	~115–130 K (pressure and greenhouse effects)&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere	&lt;br /&gt;
| ~0.18 bar N₂ + ~0.1 bar Ar + ~0.02 bar CH₄, minor CO, trace haze &lt;br /&gt;
|}&lt;br /&gt;
gII is a muted blue-green crescent veiled in gold. Its sky glows with the weight of argon and the shimmer of methane haze, and its surface smolders with the memory of internal warmth. Liquid hydrocarbons shine like ink in the basins, while glaciers ebb across the uplands. To the star it shows only one face, but beneath that still gaze lies the soft breath of a world more welcoming than its master.&lt;br /&gt;
&lt;br /&gt;
==== h ====&lt;br /&gt;
[[File:Twin Planet, red and blue.png|right|600px]]&lt;br /&gt;
h is a twin-planet system, 1.5 AU from the star, with a period of 4.1 years&lt;br /&gt;
&lt;br /&gt;
Mutual Orbital Configuration&lt;br /&gt;
* Type: True binary planet pair, gravitationally bound, equal mass&lt;br /&gt;
* Masses: 5.0 M⊕ each&lt;br /&gt;
* Radii: 2.3 R⊕ each&lt;br /&gt;
* Mutual Orbit: Essentially circular, ~1 million km separation (~8–10 planetary radii)&lt;br /&gt;
* Period (mutual orbit): ~4.5 days&lt;br /&gt;
* Orbital Plane: Perpendicular to system ecliptic &lt;br /&gt;
* Tidal State: Tidally locked to each other (mutual synchronous rotation)&lt;br /&gt;
&lt;br /&gt;
Planet A — &amp;quot;Sapphire&amp;quot;&lt;br /&gt;
* Coloration: Deep sapphire blue with white high-altitude methane ice hazes&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: H₂, He&lt;br /&gt;
** Methane (CH₄): high&lt;br /&gt;
** Ammonia: trace&lt;br /&gt;
** Argon: moderate&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: slightly enriched&lt;br /&gt;
* Magnetosphere: Strong, symmetric; supports brilliant blue-violet aurorae&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Superionic water mantle&lt;br /&gt;
** Stratified silicate-ice alloy core&lt;br /&gt;
** Radiogenic heating and layered convection&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar hexagonal jet (stronger than Saturn&#039;s)&lt;br /&gt;
** Methane plasma flares at terminator&lt;br /&gt;
** Iridescent methane cirrus clouds&lt;br /&gt;
** Massive auroral crowns aligned with spin-magnetic axis misalignment&lt;br /&gt;
&lt;br /&gt;
Planet B — &amp;quot;Rust&amp;quot;&lt;br /&gt;
* Coloration: Dark crimson to rust-red, streaked with black and violet haze bands&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: N₂, CO&lt;br /&gt;
** CH₄: trace&lt;br /&gt;
** Tholins: abundant&lt;br /&gt;
** Argon: high&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: moderate&lt;br /&gt;
** Magnetosphere: Weak, multipolar and intermittent&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Dense iron-rich core with impact inclusions (e.g., iridium, ruthenium)&lt;br /&gt;
** Volcanically active mantle with carbon-rich inclusions&lt;br /&gt;
** Higher internal heat flow than Sapphire&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar cyclonic basins with geyser-like haze columns&lt;br /&gt;
** Frequent UV lightning within organic clouds&lt;br /&gt;
** Faint auroral echoes from Sapphire’s magnetospheric tail&lt;br /&gt;
** Surface glow from argon emissions during conjunction&lt;br /&gt;
&lt;br /&gt;
Mutual Phenomena &amp;amp; Sky Effects&lt;br /&gt;
* Eclipse Cycles: Frequent, due to short mutual period and perpendicular orbit; cause wave-like haze patterns and shadow bands&lt;br /&gt;
* Filamentary Atmosphere Bridges: Transient stratospheric strands near L1, illuminated during eclipses&lt;br /&gt;
* Auroral Flux Tubes: Occasionally connect the two with violet-green flickering arcs&lt;br /&gt;
* Gravitational Stability: Mutual orbit stable within Hill sphere; resistant to long-term disruption&lt;br /&gt;
&lt;br /&gt;
* Legacy of the Comet Shield&lt;br /&gt;
* Each planet’s core contains embedded relics of the system’s ancient bombardment:&lt;br /&gt;
** Sapphire: interstellar dust, primordial isotopes, deep xenon pockets&lt;br /&gt;
** Rust: impact-derived siderophiles, compressed organics, rare isotopic anomalies&lt;br /&gt;
* Capture Events: Both planets have intercepted and redirected hundreds of large icy bodies over system history&lt;br /&gt;
&lt;br /&gt;
They each have 2 small irregular moons, &amp;lt;100 km diameter, retrograde, on distant orbits.  Negligible.&lt;br /&gt;
&lt;br /&gt;
== Planet C ==&lt;br /&gt;
[[File:Planet C and its tethered moon.png|right|700px]]&lt;br /&gt;
* With an albedo of 0.2, the global average temp is 263ºK.  Because of modest greenhouse effects, surface temperatures are higher, on the sun-side.&lt;br /&gt;
# Mass: 1.5M⊕&lt;br /&gt;
# Gravity: 1g⊕&lt;br /&gt;
# Radius = 1.225⊕, or 7805km&lt;br /&gt;
Terminator Zone&lt;br /&gt;
# +/-30º: 1.28 E8 km&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; (slightly less than all the land of the Earth)&lt;br /&gt;
# Escape velocity is 12.4km/s, 11% higher than Earth&lt;br /&gt;
# Orbital velocity is 8.79km/s&lt;br /&gt;
=== Atmosphere ===&lt;br /&gt;
Water content is low because&lt;br /&gt;
* Water vapor is a potent greenhouse gas; vast surface water can trap too much heat, especially near the substellar point.&lt;br /&gt;
* Water leads to climate homogenization&lt;br /&gt;
* Lack of exposed silicate rock: Necessary for carbon-silicate weathering feedback, which stabilizes climate on geological timescales.&lt;br /&gt;
Earth has ~1.4 billion km³ of water.  In our habitable zone, we have no more than 10% of that, or 100 million km³, though there is much more on the night side, both liquid and ice.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Factor !! Ɬiʔa atm !! Ɬiʔa % !! Earth atm !! Earth % !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! Total Pressure &lt;br /&gt;
| 1.6 atm || || 1.0 atm || || Enhanced convective heat transfer, increased IR trapping&lt;br /&gt;
|-&lt;br /&gt;
! Nitrogen (N₂) &lt;br /&gt;
| 1.00 || 62.50% || 0.7808 || 78.08% || Reduced; still inert, still dominant&lt;br /&gt;
|-&lt;br /&gt;
! Oxygen (O₂) &lt;br /&gt;
| 0.21 || 13.13% || 0.2095 || 20.95% || Earth-normal partial pressure &lt;br /&gt;
|-&lt;br /&gt;
! Argon (Ar)&lt;br /&gt;
| 0.40 || 25.00% || 0.0093 || 0.93% || Major heat distribution enhancement, inert&lt;br /&gt;
|-&lt;br /&gt;
! Krypton + Xenon&lt;br /&gt;
| 0.005 || 0.31% || trace || trace || High molecular mass → improved heat retention, still safe&lt;br /&gt;
|-&lt;br /&gt;
! CO₂&lt;br /&gt;
| 0.005 || 0.31% || 0.004 || 0.04% || slightly elevated; sub-greenhouse threshold&lt;br /&gt;
|-&lt;br /&gt;
! H₂O vapor &lt;br /&gt;
| 0.015 || ~1% || || 0-4% || Maintains greenhouse without excess moisture&lt;br /&gt;
|}&lt;br /&gt;
==== Atmospheric Effects on Clouds ====&lt;br /&gt;
# Increased Pressure (1.6 atm) compresses gases, raising the dew point at which water vapor condenses. Clouds form closer to the surface, and are denser than similar altitudes compared to Earth.&lt;br /&gt;
# Low Water Inventory (~20% of Earth&#039;s): less frequent and less massive cloud systems than on Earth, but still present—especially over &amp;quot;hotspots&amp;quot; on the day side.&lt;br /&gt;
# Tidally Locked Climate: Cloud formation concentrate along the substellar point, where warm, moist air rises and cools.&lt;br /&gt;
#* A permanent “eyewall” storm system has formed at the subsolar point, like a giant hurricane.&lt;br /&gt;
#* As air rises and is advected to the night side, thin cloud bands or ice hazes form as it descends and cools.&lt;br /&gt;
&lt;br /&gt;
Appearance:&lt;br /&gt;
* The presence of noble gases (Ar, Kr, Xe) and higher pressure enhance Mie scattering, making clouds appear whiter and more silvered, especially at sunrise/sunset boundaries.&lt;br /&gt;
* Night side clouds are thin, high-altitude icy sheets, glowing faintly in aurorae or thermal emissions.&lt;br /&gt;
&lt;br /&gt;
==== Sky Color ====&lt;br /&gt;
[[File:Life near the terminator.png|thumb|right|Life near the terminator]]&lt;br /&gt;
The color of the sky is shaped by Rayleigh scattering, which depends on:&lt;br /&gt;
# Molecular composition: Heavier gases like Ar, Kr, and Xe scatter light less efficiently than N₂.&lt;br /&gt;
# Spectral output of the star: the red dwarf emits predominantly infrared and red light, with very little blue or violet.&lt;br /&gt;
&lt;br /&gt;
Consequence:&lt;br /&gt;
* Even with atmospheric scattering, there is insufficient blue light in the stellar spectrum to produce a blue sky.&lt;br /&gt;
* Day sky would likely appear:&lt;br /&gt;
** Dark peach, dusky rose, or reddish beige near zenith,&lt;br /&gt;
** Grading to deep salmon or mauve near the horizon,&lt;br /&gt;
** A slight metallic sheen due to noble gas content and high pressure.&lt;br /&gt;
&lt;br /&gt;
Twilight &amp;amp; Limb Scattering:&lt;br /&gt;
* The terminator (twilight zone) sees a diffuse, ruddy light, scattering through haze and clouds into luminous reds, purples, and copper tones.&lt;br /&gt;
* Aurorae are spectacular on the night side, especially since stellar flares are frequent.&lt;br /&gt;
&lt;br /&gt;
==== Sound Propagation ====&lt;br /&gt;
: &#039;&#039;Sound is profoundly affected by atmospheric pressure and composition.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Compared to Earth:&lt;br /&gt;
* Higher pressure → greater air density → faster transmission of sound and less attenuation.&lt;br /&gt;
* Argon and Xenon are heavy gases, which:&lt;br /&gt;
** Lower the speed of sound relative to air at the same pressure (despite the pressure increase).&lt;br /&gt;
** Shift resonance frequencies downward, resulting in deeper, rounder sounds.&lt;br /&gt;
&lt;br /&gt;
Consequences:&lt;br /&gt;
* Voices sound subtly lower-pitched and richer, especially for consonants and low vowels.&lt;br /&gt;
* Ambient sounds (wind, water, animals) would carry farther and sound more muffled or sonorous.&lt;br /&gt;
* Music or speech would resonate more warmly, especially indoors or in enclosed spaces.&lt;br /&gt;
&lt;br /&gt;
In short: it sounds like it’s wrapped in velvet.&lt;br /&gt;
&lt;br /&gt;
==== Heat Transport to the Night Side ====&lt;br /&gt;
Mechanisms:&lt;br /&gt;
# Thick Atmosphere (1.6 atm) increases:&lt;br /&gt;
#* Advection efficiency: Warm air masses can move more heat horizontally.&lt;br /&gt;
#* Radiative time constant: The atmosphere holds heat longer before releasing it.&lt;br /&gt;
# Noble Gases (especially Kr/Xe):&lt;br /&gt;
#* High molecular mass → more IR opacity → trapping and radiating heat more evenly.&lt;br /&gt;
# Slow Rotation / Tidal Locking:&lt;br /&gt;
#* Global Hadley-like cells dominate circulation, carrying warm air from the day side to the night side and descending it there.&lt;br /&gt;
&lt;br /&gt;
Result:&lt;br /&gt;
* The night side is not so freezing.  Temperatures differ by tens of degrees, not hundreds.&lt;br /&gt;
* There are still ice caps and a cold deserts at the anti-stellar point, but not a glaciated wasteland.&lt;br /&gt;
&lt;br /&gt;
=== Magnetosphere ===&lt;br /&gt;
* Larger mass --&amp;gt; larger iron core, generating more internal heat&lt;br /&gt;
* Larger radius --&amp;gt; Vigorous convection in the core&lt;br /&gt;
* Tidal Flexing --&amp;gt; still drives magnetic activity&lt;br /&gt;
&lt;br /&gt;
# Aurorae at lower latitudes&lt;br /&gt;
## higher magnetic rigidity, wider magnetotail, and greater reconnection energy.&lt;br /&gt;
## Combined with a higher flux of stellar particles, this means:&lt;br /&gt;
### Auroral ovals expand, reaching mid-latitudes sometimes equator.&lt;br /&gt;
### The skies are alive with rippling green, violet, and crimson aurorae, especially on the night side.&lt;br /&gt;
### Daily auroral activity occur during stellar flare cycles.&lt;br /&gt;
# Compasses&lt;br /&gt;
## compasses respond more sharply, with:&lt;br /&gt;
### Faster alignment.&lt;br /&gt;
### Greater resistance to local perturbations.&lt;br /&gt;
## However, frequent magnetic storms from stellar activity cause sudden declinations, reversals, or local anomalies.  In short, lots of aurorae equals dead compasses at the same time.&lt;br /&gt;
# Magnetic Field Strength &amp;gt; 100 μT &lt;br /&gt;
# Electromagnetism is more basic than chemistry or almost any other natural philosophy&lt;br /&gt;
&lt;br /&gt;
=== Substellar Point ===&lt;br /&gt;
The maximum incoming flux is very nearly the same as Earth&#039;s solar constant (≈1361 W/m²), but concentrated over one point rather than averaged over a rotating sphere.  Temperatures should be above 500ºK most of the time.  &lt;br /&gt;
&lt;br /&gt;
The magnetic north is also here. The thick atmosphere prevents too much loss here, but &lt;br /&gt;
* Charged particle influx&lt;br /&gt;
** Maximized at the substellar point—intense auroral and energetic particle precipitation&lt;br /&gt;
* Atmospheric ionization&lt;br /&gt;
** Constant production of high-energy ions and NOx compounds—UV fluorescence in upper sky&lt;br /&gt;
* Localized heating&lt;br /&gt;
** Augments already extreme temperatures—600–700 K surface&lt;br /&gt;
&lt;br /&gt;
== Artificially Tethered Moon ==&lt;br /&gt;
* 670,000 km up&lt;br /&gt;
* 7805 km in radius = same as the planet&lt;br /&gt;
* 1.33º of the sky, same as the sun&lt;br /&gt;
&lt;br /&gt;
A network of tethers/tension lines from the moon to multiple anchor points on the planet’s surface (a tripod or hexapod structure), woven like hair&lt;br /&gt;
* Uses active tension management and orbital station-keeping to stabilize the moon&lt;br /&gt;
* Counterweights and inward-pointing mass drivers on the moon to oppose drift&lt;br /&gt;
&lt;br /&gt;
The tethers are not bearing the full weight, but merely damping drift, providing restoring force, and enabling long-term stability through active compensation.  The moon&lt;br /&gt;
* Blocks the worst of the heat&lt;br /&gt;
* Blocks the worst of the solar radiation&lt;br /&gt;
The moon has &lt;br /&gt;
* low mass&lt;br /&gt;
* high albedo - enormous reflectivity&lt;br /&gt;
* scatters charges particles, UV, X-rays, auroral flux tubes&lt;br /&gt;
* sunward - crazy hot, high emissivity&lt;br /&gt;
* earthward - crazy cool, low emissivity&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168738</id>
		<title>Ɬiʔa/Conworlding</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168738"/>
		<updated>2025-04-05T20:07:25Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* Solar System */ more data&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Star ==&lt;br /&gt;
The star is a red-dwarf (M5V) named Gliese 710b minoris, or informally &#039;&#039;Mirar&#039;s Veil&#039;&#039;.  It is 7.9 light-years (≈2.42 parsecs) from Sol, toward the galactic plane, in Scorpius–Ophiuchus.  It lies just &amp;quot;behind&amp;quot; a brighter, well-known K-dwarf, and was not observed until after humanity&#039;s trip to Proxima Centauri: in situ gravitational navigation by the first robotic probe en route to Proxima Centauri. The probe’s optical gyros noticed an unmodeled gravitational perturbation.&lt;br /&gt;
&lt;br /&gt;
* Stellar luminosity (L*) ≈ 0.01 𝐿⊙ (1/100th Sol&#039;s brightness)&lt;br /&gt;
* Stellar mass (M*) ≈ 0.2 𝑀⊙ (1/5 the mass of Sol)&lt;br /&gt;
* Stellar radius (R*) ≈ 0.25 𝑅⊙ (1/4 as wide as Sol)&lt;br /&gt;
* Effective temperature (T*) ≈ 3500 K&lt;br /&gt;
* Average surface field is ~1.5 kG, with frequent bursts of &amp;gt; 3kG&lt;br /&gt;
** Frequent, energetic flares, multiple per day, with for extreme variability over time, often above 10&amp;lt;sup&amp;gt;35&amp;lt;/sup&amp;gt; erg&lt;br /&gt;
* The frostline is at 0.27 AU&lt;br /&gt;
&lt;br /&gt;
​The habitable zone (a) is about square root of L* over L⊙, so ~0.1 AU.&lt;br /&gt;
&lt;br /&gt;
=== Solar System ===&lt;br /&gt;
There are seven planets in the system&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Planet !!	Mass (M🜨)!!	Radius (R🜨)!! Moons/Rings	!!Resonance !!	&amp;lt;small&amp;gt;Semi-Major&amp;lt;/small&amp;gt; !!	Rings !! Moons !! Period !! Size !! Type !! Sidereal !! A. Mag.&lt;br /&gt;
|-&lt;br /&gt;
| b ||	2.17 ||	1.1 ||	No ||	2:3 with c	|| 0.0763 ||	No || No || 17.2 || 13.6&#039; to 1.5&#039; || Super-Mercury || 51.6 || -10.98&lt;br /&gt;
|-&lt;br /&gt;
| c ||	1.5	 ||1.225 ||	1* ||	—	        || 0.100 || No || No || 25.8 || - || Super-Earth || - || - &lt;br /&gt;
|-&lt;br /&gt;
| d ||	2.0	 ||1.4 ||No ||	2:3 with c	 ||0.131 ||	No || No || 38.7 || 13.1&#039; to 1.8&#039; || Super Waterworld || 77.4 || -11.85&lt;br /&gt;
|-&lt;br /&gt;
| e ||	0.9 ||	1.0 || No	 ||	2:3 with d	 ||0.172 ||	No || No || 58 || 4.1&#039; to 1.1&#039; || Earth || 46.5 || -8.86&lt;br /&gt;
|- &lt;br /&gt;
| f ||	3.5 ||	2.0 ||	Yes! ||	2:3 with e	 ||0.227 || Yes || Junk || 87 || 4.6&#039; to 1.8&#039; || Mini-Neptune || 36.7 || -9.78&lt;br /&gt;
|-&lt;br /&gt;
| g ||	2.6 ||	1.7 ||	2 ||	-	 ||0.40 ||	Yes || Junk || 206 || 1.6&#039; to 1.0&#039; || Stripped Neptune || 29.5 || -7.16&lt;br /&gt;
|-&lt;br /&gt;
| h ||	5.0x2 ||2.3x2 || yes	 || -	 ||1.5 ||	Yes || No || 1500 || 0.5&#039; 16.4&#039; apart (at max) || Double Neptune || 26.25 || -5.43&lt;br /&gt;
|}&lt;br /&gt;
==== b: super Mercury with a ring of fire  ====&lt;br /&gt;
[[File:planet b by GPT.png|thumb|right|An artistic rendering of planet b]]&lt;br /&gt;
b is a super-Mercury, tidally locked, and incredibly dense.  ~700ºK on the day side, ~50ºK on the night.  2.1 Earth Masses, 1.1 Earth radii (~7000km) in size.  Orbital period 17.2 days.  Density 9.0 g/cm&amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt;.  Gravity is ~1.8g.  &lt;br /&gt;
&lt;br /&gt;
The iron core is huge, being 75% of the mass.  A thin silicate mantle, with metallic plains and exhumed ultramafic crust, with frequent iron meteorite craters, lacking typical “stone” breccias.&lt;br /&gt;
&lt;br /&gt;
The night side is intense, as simple hydrocarbons (methane, ethane, propane) condense and freeze into layered deposits.  Complex organics (tholins, polycyclic aromatics) accumulate on the sea floor, under miles of nitrogen ice.  Massive slush layers slosh around above cryovolcanic brines of ammonia.&lt;br /&gt;
&lt;br /&gt;
There is a crucial layer of Superionic Ice XI above the core, which acts as an electromagnetic insulator, and ionic heat bridge.  The crust is ultramafic silicates (olivine, pyroxene, perovskite) riddled with with sulfide veins, iron alloys, and graphite networks.  The poles of the magnetosphere are sideways, like Uranus, with poles at the equator in the Terminator Zone.  Persistent surface charges develop, because the whole planet is basically a ginormous Leyden jar!&lt;br /&gt;
&lt;br /&gt;
A planetary flux rope forms and un-forms with the star and planet b.  This induces electric jets at the terminator.  This is where temps are Earth-like.  Hydrocarbons sublimate and eject into the atmosphere, even while aurorae come right down to the ground.  A small, low pressure atmosphere prevents photodissociation, even while electrothermal instabilities lift molecules, forming an anomalous haze, a standing, glowing ring.  Coronal events cause localized lightning geysers with magnetic arcing.&lt;br /&gt;
&lt;br /&gt;
In short, b is visible with a blinding bright sun side (glowing orange bronze), a utterly black night side, and a burning, glowing, erupting, arcing ring at the terminator (all colors).  At biggest, it&#039;s half the size of Earth&#039;s moon in the sky, shrinking down to a star at it&#039;s furthest away.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== d: the wet eye with depths ====&lt;br /&gt;
[[File:wet eye planet.png|thumb|right|An reasonable approximation of d&#039;s appearance]]&lt;br /&gt;
From the outside, d is a &amp;quot;wet eye&amp;quot; just outside the habitable zone.  It is a water world, twice the mass of Earth, 1.4 times the radius, tidally locked.  The substellar point is the only place without surface ice.  However, it is better to think of the planet top-to-bottom.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;atmosphere&#039;&#039;&#039; is tenuous, less than 0.2 bars.  It is thin, N₂-rich with traces of H₂O, NH₃ vapor, and transient geyser outputs.  It is highly UV-irradiated, and Mars-like in its inability to retain volatiles.&lt;br /&gt;
&lt;br /&gt;
Next, there is a &#039;&#039;&#039;surface ice shell&#039;&#039;&#039;, ~20 km of thick Ice I.  Swirling currents beneath have cracked continent-sized ice plates, similar to Europa&#039;s crust.  It is permanently frozen except at the substellar furnace.  It accumulates chemical stains, mineral deposits, and cryovolcanic eruption plumes.  Accumulations of complex hydrates—like methanol clathrates—precipitate out and form false reefs, rising like coral from beneath. Transient thermal vents push hot plumes into the thin air, freezing instantly and snowing down crystals that form mineral spires.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;subglacial ocean&#039;&#039;&#039; is hundreds of kilometers thick.  It is super-pressurized liquid H₂O mixed with NH₃, CH₃OH, H₂O₂, and trace salts.  The movement is slow, planetary-scale currents originating from the Furnace and Coriolis force.  Strong layers exist: the surface is oxidized; the abyssal layer is reducing.&lt;br /&gt;
&lt;br /&gt;
A new &amp;quot;surface&amp;quot; is next.  The &#039;&#039;&#039;Ice Mantle&#039;&#039;&#039; is solid Ice VI and VII.  There are massive, slowly shifting &amp;quot;sub-oceanic continents&amp;quot;. It is periodically fractured and resurfaced by cryoquakes and brine-driven eruptions.  Some regions have developed elevated domes or ridges, continental “shelves” under the ocean.&lt;br /&gt;
&lt;br /&gt;
Finally, underneath is the &#039;&#039;&#039;core&#039;&#039;&#039;. Temperatures exceed 2000–3000 K locally.  Pressures range from 100 to 300 GPa.  The core is rich in heavy elements.  This makes radiogenic hotspots, localized magnetic eddies.  Heat gradients + ion flows = thermoelectric currents.  These make magnetic storms within the ocean itself, not the sky.  When uranium-rich corium pods shift or explode upward through the mantle, their heat and conductivity disturb the local magnetic field, generating geomagnetic quakes.  These pulse through the ocean, creating short-lived magnetic lenses.  These interact with atmospheric charged particles above the Furnace, giving rise to transient magnetic halos visible from orbit—false auroras without a sunstorm.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== e: The Tortured Near-Sphere ====&lt;br /&gt;
[[File:Blasting and shattered.png|thumb|right|An axial recoil event in progress]]&lt;br /&gt;
Orbital and Physical Characteristics&lt;br /&gt;
* Mass: 0.9 Earth masses&lt;br /&gt;
* Radius: 1.0 Earth radii&lt;br /&gt;
* Orbital Period: 58 Earth days&lt;br /&gt;
* Surface Gravity: ~0.9 g&lt;br /&gt;
* Semimajor Axis: ~0.17 AU &lt;br /&gt;
* Spin State: In the &#039;&#039;process&#039;&#039; of becoming tidally locked&lt;br /&gt;
* Obliquity: Extreme, experiencing chaotic realignment events&lt;br /&gt;
&lt;br /&gt;
Internal Structure and Composition&lt;br /&gt;
* &#039;&#039;&#039;Crust:&#039;&#039;&#039; A thick, rigid outer shell of water ice I mixed with clathrates (CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; and CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; hydrates), underlain by layers of ammonia-water ice eutectics. Inclusions of carbon under extreme pressure form diamond strata in the lower crust, lending rigidity and brittle behavior.&lt;br /&gt;
* &#039;&#039;&#039;Mantle:&#039;&#039;&#039; Comprised of Ice VI and Ice VII, with ammonia- and methane-rich brines forming localized conduits and pockets of unstable volatiles.&lt;br /&gt;
* &#039;&#039;&#039;Core:&#039;&#039;&#039; Differentiated and semi-molten. Inner core of iron-nickel alloy spins at a different rate. Outer core is a highly viscous slurry of silicate, iron, carbon, sulfur, and dissolved volatiles. Chemical veins (e.g., uranium silicates, perovskites) act as mechanical shear zones. Tidal torque leads to periodic frictional heating.&lt;br /&gt;
&lt;br /&gt;
Tectonic and Cryovolcanic Behavior&lt;br /&gt;
* The planet resists tidal locking due to core-crust decoupling and uneven angular momentum transfer.&lt;br /&gt;
* High obliquity experiences &#039;&#039;&#039;&#039;&#039;Axial Recoil Events&#039;&#039;&#039;&#039;&#039;, where the entire planet jerks between metastable orientations (e.g., from 110° to 70°) in sudden spasms.&lt;br /&gt;
* These events generate:&lt;br /&gt;
** Global-scale crustal cracking&lt;br /&gt;
** Venting of pressurized subsurface gases (H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;O, CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt;)&lt;br /&gt;
** Surface deformation and glacial faulting&lt;br /&gt;
* Volatiles erupt ballistically into space (200+lm) from exposed fissures and calderas, driven by phase-change explosions.&lt;br /&gt;
&lt;br /&gt;
Surface Conditions&lt;br /&gt;
* Global temperature well below freezing; warmest zones around cryovolcanic hotspots&lt;br /&gt;
* Crustal coloration varies by volatile deposition:&lt;br /&gt;
** Pale blue-white from water ice&lt;br /&gt;
** Red-brown from CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; frostfields&lt;br /&gt;
** Green-black CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; stains from plume fallout&lt;br /&gt;
* Surface features include:&lt;br /&gt;
** Cryovolcanic calderas&lt;br /&gt;
** Diamond-studded impact-like basins&lt;br /&gt;
** Faulted plains crossed by salt-streaked rift zones&lt;br /&gt;
&lt;br /&gt;
Atmosphere and Ejected Material&lt;br /&gt;
* Thin transient exosphere formed from eruptive events&lt;br /&gt;
* Gases often escape to space or freeze back out in polar regions&lt;br /&gt;
* Fallback material creates uneven surface mass distributions, altering moment of inertia and prolonging instability&lt;br /&gt;
&lt;br /&gt;
Appearance from Planet c&lt;br /&gt;
&lt;br /&gt;
* Angular Size: ~4-1 arcminutes&lt;br /&gt;
* Coloration: Overall dusky grey-white, with changing colored bands due to volatile fallout; craterless but mottled&lt;br /&gt;
&lt;br /&gt;
Transient visible phenomena:&lt;br /&gt;
&lt;br /&gt;
* Cryovolcanic plumes visible as fan-like arcs at the limb during outburst events&lt;br /&gt;
* Infrared brightening during Axial Recoil Events&lt;br /&gt;
* Occasional light-scattering halos from plume particles&lt;br /&gt;
&lt;br /&gt;
Event Cycle Summary&lt;br /&gt;
&lt;br /&gt;
# Tidal torque builds due to obliquity misalignment&lt;br /&gt;
# Core resists, crust locks tension&lt;br /&gt;
# Critical stress threshold breached&lt;br /&gt;
# Obliquity lurches to new orientation&lt;br /&gt;
# Crust fractures globally, vents open&lt;br /&gt;
# Supersonic cryovolcanism hurls volatiles into space&lt;br /&gt;
# Fallback modifies crustal mass distribution&lt;br /&gt;
# Obliquity rebuilds instability over decades&lt;br /&gt;
# Repeat.&lt;br /&gt;
&lt;br /&gt;
Planet e is a tortured world caught in an unending cycle of self-correcting failure—its body unable to align, its gases unable to stay contained, its appearance in the sky a visible signature of internal catastrophe.&lt;br /&gt;
&lt;br /&gt;
==== f: Ringed Mini-Neptune ====&lt;br /&gt;
[[File:Ringed Neptune with four moons.png|thumb|right|Aperspectival view of f, its rings, and four moons]]&lt;br /&gt;
This planet is a substantial mini-Neptune, with a mass of approximately 3.5 Earth masses and a radius of 2.0 Earth radii, orbiting at 0.227 AU. Its low mean density (~0.44 ρ⊕) signals the presence of a deep, volatile-rich envelope overlying a denser core. The bulk of its volume is composed of hydrogen and helium, accreted from the protoplanetary disk, with trace amounts of methane (CH₄) and ammonia (NH₃)—gases that dominate its photochemical and radiative behavior. Beneath this envelope, the planet hosts a water–rock–metal core layered in complex phases, with high-pressure ices and possibly superionic water enveloping a metallic center.  Lower atmosphere reaches 300–500 K (27–227°C) near the bottom of the troposphere, depending on opacity and convection.&lt;br /&gt;
&lt;br /&gt;
Visually, the planet exhibits a blue-to-cyan atmospheric hue, governed by Rayleigh scattering and methane absorption in the red and near-infrared spectrum. While not as banded or storm-laced as Jupiter, it features broad zonal flows, high-altitude methane ice clouds, and long-lived anticyclonic storms akin to Neptune’s Great Dark Spot. Due to its tidal locking to the host star, the planet presents hemispheric climatic asymmetry: a sunlit dayside prone to atmospheric upwelling and cloud formation, and a cooler, darker nightside. While colder, the backside is not freezing— in the 150–250 K range, depending on circulation efficiency. Atmospheric circulation is dominated by slow, large-scale overturning cells, moderated by planetary-scale waves and a subdued Coriolis force. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Rings =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Ring!!	Range (Rₚ)!!	Approx.! Range (km)!!	Description&lt;br /&gt;
|-&lt;br /&gt;
! C&lt;br /&gt;
| 	1.5–1.65 Rₚ	||19,100–21,000	||Faint, dusty interior ring&lt;br /&gt;
|-&lt;br /&gt;
! B&lt;br /&gt;
| 	1.65–1.96 Rₚ	||21,000–25,000||	Bright, dense primary ring&lt;br /&gt;
|-&lt;br /&gt;
! Division&lt;br /&gt;
|	1.96–2.04 Rₚ ||25,000–26,000 || a low-density gap&lt;br /&gt;
|-&lt;br /&gt;
!  A&lt;br /&gt;
|	2.04–2.3 Rₚ||26,000–29,300||	Sharp-edged outer ring&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Moon !!	Orbit (km) !!	Orbit (Rₚ) !!	Diameter (km) !!	Type	!! Period !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! I&lt;br /&gt;
|	60,000	||4.7 Rₚ	||~400	||Rocky	|| 0.9 ||Cratered&lt;br /&gt;
|-&lt;br /&gt;
! II&lt;br /&gt;
| 	110,000	|| 8.6 Rₚ	|| ~800	|| Mixed rock/ice	|| 2.25|| Cracked surface, frozen ocean&lt;br /&gt;
|-&lt;br /&gt;
! III &lt;br /&gt;
| 190,000	|| 14.9 Rₚ ||	~1200 ||	Icy major moon ||	5.1|| Cryovolcanism, smooth plains&lt;br /&gt;
|-&lt;br /&gt;
! IV &lt;br /&gt;
|340,000	||26.7 Rₚ	||~200	||Irregular/prograde	|| 12.21 || Dark red/carbon, inclined (20º, eccentric orbit (0.1)&lt;br /&gt;
|-&lt;br /&gt;
! V &lt;br /&gt;
| 710,000 ||	55.7 Rₚ	||~350	|| Captured/retrograde	|| 36.83 || Highly inclined (130º), Split terrain—half rugged highlands, half smooth resurfaced plain&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==== g: Stripped Sub-Neptune Remnant ====&lt;br /&gt;
[[File:Stripped Planet with Two Cool Moons.png|700px|right]]&lt;br /&gt;
Basic Parameters&lt;br /&gt;
* Mass: 2.6 Earth masses (M⊕)&lt;br /&gt;
* Radius: 1.7 Earth radii (R⊕)&lt;br /&gt;
* Mean Density: ~2.92 g/cm³&lt;br /&gt;
* Orbital Distance: 0.4 AU &lt;br /&gt;
* Albedo: ~0.5 (moderately high)&lt;br /&gt;
* Rotation: Tidally locked &lt;br /&gt;
&lt;br /&gt;
Origin and Evolution&lt;br /&gt;
* Formed beyond the snow line (~0.8–1.2 AU) from a mix of rock, iron, and ices&lt;br /&gt;
* Migrated inward early during protoplanetary disk phase&lt;br /&gt;
* Accreted a modest hydrogen-helium envelope (&amp;gt;1% by mass)&lt;br /&gt;
* Exposed to intense stellar X-ray and UV radiation during the M dwarf&#039;s pre-main-sequence phase&lt;br /&gt;
* Lacked a magnetic dynamo (metal-poor and early core freezing)&lt;br /&gt;
* Entire atmosphere lost over ~100 Myr via photoevaporation, core-powered mass loss, and sputtering&lt;br /&gt;
&lt;br /&gt;
Current State&lt;br /&gt;
* Atmosphere: None (trace mineral vapors possible in hot regions)&lt;br /&gt;
* Surface: Stark contrast between hemispheres due to tidal locking&lt;br /&gt;
** Dayside: ~700–1000 K; high-silica lava fields, salt flats, exposed alumino-silicates&lt;br /&gt;
** Nightside: ~100–150 K; gypsum and calcite in cold traps, frozen regolith&lt;br /&gt;
* Magnetosphere: Absent&lt;br /&gt;
* Volcanism:episodic; high-silica flows, volcanic glass, sodium-rich crusts&lt;br /&gt;
* Geological Activity: Tectonically inactive; thermally fractured plains, impact craters&lt;br /&gt;
&lt;br /&gt;
Surface Composition&lt;br /&gt;
* Titanium dioxide (rutile): bright, high-albedo mineral condensate&lt;br /&gt;
* Calcite (CaCO₃): carbonate deposits in cold traps&lt;br /&gt;
* Gypsum (CaSO₄·2H₂O): hydration mineral, stable only on the nightside&lt;br /&gt;
* Sodium chloride: salt flats, especially in evaporated basins&lt;br /&gt;
* High-silica volcanic deposits: glassy, oxidized, and light-colored&lt;br /&gt;
&lt;br /&gt;
Visual and Observational Notes&lt;br /&gt;
&lt;br /&gt;
* High visual contrast between molten and frozen hemispheres&lt;br /&gt;
* Surface appears mottled: obsidian-black lava, gleaming salt flats, white calcium deposits&lt;br /&gt;
* No clouds, auroras, or magnetic activity&lt;br /&gt;
* Extreme day/night temperature gradient&lt;br /&gt;
* Reflective phase curve possible in photometric observations&lt;br /&gt;
* Surface pressure: effectively 0 bar&lt;br /&gt;
&lt;br /&gt;
Planet g is the airless skeleton of a once-sub-Neptune world. Born icy and distant, it migrated into the young star&#039;s wrath, where its fragile envelope boiled away under a sky of flares. Bereft of a magnetic shield, it was slowly stripped to bare rock. Today, one hemisphere bakes in molten silence while the other freezes in shadow. No air, no oceans, only salt, stone, and the echo of a lost atmosphere.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property !!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~75,000 km (~0.26 R&amp;lt;sub&amp;gt;hill&amp;lt;/sub&amp;gt;)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~1,400 km (~0.22 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass	&lt;br /&gt;
| ~0.01 M⊕ (~1.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~3.0 g/cm³ (rock–ice mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temp&lt;br /&gt;
|	~150–180 K&lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
| 0.20g&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere&lt;br /&gt;
|	Trace O₂, from radiolysis and outgassing&lt;br /&gt;
|-&lt;br /&gt;
! Subsurface Ocean&lt;br /&gt;
|	heated by tidal flexing&lt;br /&gt;
|-&lt;br /&gt;
! Surface Features	&lt;br /&gt;
|Fractured ice crust, chaos terrain, cryogeysers, lenticulae&lt;br /&gt;
|}&lt;br /&gt;
gI is a cracked glass orb, rimed with frost and laced with luminous fissures. Below its crust, tides flex a hidden ocean in rhythmic silence. Its faint oxygen exosphere is ghostly but present.  It is frosted quartz with cobwebbed streaks and mineral discoloration.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property!!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~150,000 km (~0.5 Rₕill)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~2,100 km (~0.33 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass&lt;br /&gt;
|	~0.035 M⊕ (~4.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~2.1 g/cm³ (icy-rocky mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes &lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
|	~0.35 g&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temperature&lt;br /&gt;
|	~115–130 K (pressure and greenhouse effects)&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere	&lt;br /&gt;
| ~0.18 bar N₂ + ~0.1 bar Ar + ~0.02 bar CH₄, minor CO, trace haze &lt;br /&gt;
|}&lt;br /&gt;
gII is a muted blue-green crescent veiled in gold. Its sky glows with the weight of argon and the shimmer of methane haze, and its surface smolders with the memory of internal warmth. Liquid hydrocarbons shine like ink in the basins, while glaciers ebb across the uplands. To the star it shows only one face, but beneath that still gaze lies the soft breath of a world more welcoming than its master.&lt;br /&gt;
&lt;br /&gt;
==== h ====&lt;br /&gt;
[[File:Twin Planet, red and blue.png|right|600px]]&lt;br /&gt;
h is a twin-planet system, 1.5 AU from the star, with a period of 4.1 years&lt;br /&gt;
&lt;br /&gt;
Mutual Orbital Configuration&lt;br /&gt;
* Type: True binary planet pair, gravitationally bound, equal mass&lt;br /&gt;
* Masses: 5.0 M⊕ each&lt;br /&gt;
* Radii: 2.3 R⊕ each&lt;br /&gt;
* Mutual Orbit: Essentially circular, ~1 million km separation (~8–10 planetary radii)&lt;br /&gt;
* Period (mutual orbit): ~4.5 days&lt;br /&gt;
* Orbital Plane: Perpendicular to system ecliptic &lt;br /&gt;
* Tidal State: Tidally locked to each other (mutual synchronous rotation)&lt;br /&gt;
&lt;br /&gt;
Planet A — &amp;quot;Sapphire&amp;quot;&lt;br /&gt;
* Coloration: Deep sapphire blue with white high-altitude methane ice hazes&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: H₂, He&lt;br /&gt;
** Methane (CH₄): high&lt;br /&gt;
** Ammonia: trace&lt;br /&gt;
** Argon: moderate&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: slightly enriched&lt;br /&gt;
* Magnetosphere: Strong, symmetric; supports brilliant blue-violet aurorae&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Superionic water mantle&lt;br /&gt;
** Stratified silicate-ice alloy core&lt;br /&gt;
** Radiogenic heating and layered convection&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar hexagonal jet (stronger than Saturn&#039;s)&lt;br /&gt;
** Methane plasma flares at terminator&lt;br /&gt;
** Iridescent methane cirrus clouds&lt;br /&gt;
** Massive auroral crowns aligned with spin-magnetic axis misalignment&lt;br /&gt;
&lt;br /&gt;
Planet B — &amp;quot;Rust&amp;quot;&lt;br /&gt;
* Coloration: Dark crimson to rust-red, streaked with black and violet haze bands&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: N₂, CO&lt;br /&gt;
** CH₄: trace&lt;br /&gt;
** Tholins: abundant&lt;br /&gt;
** Argon: high&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: moderate&lt;br /&gt;
** Magnetosphere: Weak, multipolar and intermittent&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Dense iron-rich core with impact inclusions (e.g., iridium, ruthenium)&lt;br /&gt;
** Volcanically active mantle with carbon-rich inclusions&lt;br /&gt;
** Higher internal heat flow than Sapphire&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar cyclonic basins with geyser-like haze columns&lt;br /&gt;
** Frequent UV lightning within organic clouds&lt;br /&gt;
** Faint auroral echoes from Sapphire’s magnetospheric tail&lt;br /&gt;
** Surface glow from argon emissions during conjunction&lt;br /&gt;
&lt;br /&gt;
Mutual Phenomena &amp;amp; Sky Effects&lt;br /&gt;
* Eclipse Cycles: Frequent, due to short mutual period and perpendicular orbit; cause wave-like haze patterns and shadow bands&lt;br /&gt;
* Filamentary Atmosphere Bridges: Transient stratospheric strands near L1, illuminated during eclipses&lt;br /&gt;
* Auroral Flux Tubes: Occasionally connect the two with violet-green flickering arcs&lt;br /&gt;
* Gravitational Stability: Mutual orbit stable within Hill sphere; resistant to long-term disruption&lt;br /&gt;
&lt;br /&gt;
* Legacy of the Comet Shield&lt;br /&gt;
* Each planet’s core contains embedded relics of the system’s ancient bombardment:&lt;br /&gt;
** Sapphire: interstellar dust, primordial isotopes, deep xenon pockets&lt;br /&gt;
** Rust: impact-derived siderophiles, compressed organics, rare isotopic anomalies&lt;br /&gt;
* Capture Events: Both planets have intercepted and redirected hundreds of large icy bodies over system history&lt;br /&gt;
&lt;br /&gt;
They each have 2 small irregular moons, &amp;lt;100 km diameter, retrograde, on distant orbits.  Negligible.&lt;br /&gt;
&lt;br /&gt;
== Planet C ==&lt;br /&gt;
[[File:Planet C and its tethered moon.png|right|700px]]&lt;br /&gt;
* With an albedo of 0.2, the global average temp is 263ºK.  Because of modest greenhouse effects, surface temperatures are higher, on the sun-side.&lt;br /&gt;
# Mass: 1.5M⊕&lt;br /&gt;
# Gravity: 1g⊕&lt;br /&gt;
# Radius = 1.225⊕, or 7805km&lt;br /&gt;
Terminator Zone&lt;br /&gt;
# +/-30º: 1.28 E8 km&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; (slightly less than all the land of the Earth)&lt;br /&gt;
# Escape velocity is 12.4km/s, 11% higher than Earth&lt;br /&gt;
# Orbital velocity is 8.79km/s&lt;br /&gt;
=== Atmosphere ===&lt;br /&gt;
Water content is low because&lt;br /&gt;
* Water vapor is a potent greenhouse gas; vast surface water can trap too much heat, especially near the substellar point.&lt;br /&gt;
* Water leads to climate homogenization&lt;br /&gt;
* Lack of exposed silicate rock: Necessary for carbon-silicate weathering feedback, which stabilizes climate on geological timescales.&lt;br /&gt;
Earth has ~1.4 billion km³ of water.  In our habitable zone, we have no more than 10% of that, or 100 million km³, though there is much more on the night side, both liquid and ice.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Factor !! Ɬiʔa atm !! Ɬiʔa % !! Earth atm !! Earth % !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! Total Pressure &lt;br /&gt;
| 1.6 atm || || 1.0 atm || || Enhanced convective heat transfer, increased IR trapping&lt;br /&gt;
|-&lt;br /&gt;
! Nitrogen (N₂) &lt;br /&gt;
| 1.00 || 62.50% || 0.7808 || 78.08% || Reduced; still inert, still dominant&lt;br /&gt;
|-&lt;br /&gt;
! Oxygen (O₂) &lt;br /&gt;
| 0.21 || 13.13% || 0.2095 || 20.95% || Earth-normal partial pressure &lt;br /&gt;
|-&lt;br /&gt;
! Argon (Ar)&lt;br /&gt;
| 0.40 || 25.00% || 0.0093 || 0.93% || Major heat distribution enhancement, inert&lt;br /&gt;
|-&lt;br /&gt;
! Krypton + Xenon&lt;br /&gt;
| 0.005 || 0.31% || trace || trace || High molecular mass → improved heat retention, still safe&lt;br /&gt;
|-&lt;br /&gt;
! CO₂&lt;br /&gt;
| 0.005 || 0.31% || 0.004 || 0.04% || slightly elevated; sub-greenhouse threshold&lt;br /&gt;
|-&lt;br /&gt;
! H₂O vapor &lt;br /&gt;
| 0.015 || ~1% || || 0-4% || Maintains greenhouse without excess moisture&lt;br /&gt;
|}&lt;br /&gt;
==== Atmospheric Effects on Clouds ====&lt;br /&gt;
# Increased Pressure (1.6 atm) compresses gases, raising the dew point at which water vapor condenses. Clouds form closer to the surface, and are denser than similar altitudes compared to Earth.&lt;br /&gt;
# Low Water Inventory (~20% of Earth&#039;s): less frequent and less massive cloud systems than on Earth, but still present—especially over &amp;quot;hotspots&amp;quot; on the day side.&lt;br /&gt;
# Tidally Locked Climate: Cloud formation concentrate along the substellar point, where warm, moist air rises and cools.&lt;br /&gt;
#* A permanent “eyewall” storm system has formed at the subsolar point, like a giant hurricane.&lt;br /&gt;
#* As air rises and is advected to the night side, thin cloud bands or ice hazes form as it descends and cools.&lt;br /&gt;
&lt;br /&gt;
Appearance:&lt;br /&gt;
* The presence of noble gases (Ar, Kr, Xe) and higher pressure enhance Mie scattering, making clouds appear whiter and more silvered, especially at sunrise/sunset boundaries.&lt;br /&gt;
* Night side clouds are thin, high-altitude icy sheets, glowing faintly in aurorae or thermal emissions.&lt;br /&gt;
&lt;br /&gt;
==== Sky Color ====&lt;br /&gt;
[[File:Life near the terminator.png|thumb|right|Life near the terminator]]&lt;br /&gt;
The color of the sky is shaped by Rayleigh scattering, which depends on:&lt;br /&gt;
# Molecular composition: Heavier gases like Ar, Kr, and Xe scatter light less efficiently than N₂.&lt;br /&gt;
# Spectral output of the star: the red dwarf emits predominantly infrared and red light, with very little blue or violet.&lt;br /&gt;
&lt;br /&gt;
Consequence:&lt;br /&gt;
* Even with atmospheric scattering, there is insufficient blue light in the stellar spectrum to produce a blue sky.&lt;br /&gt;
* Day sky would likely appear:&lt;br /&gt;
** Dark peach, dusky rose, or reddish beige near zenith,&lt;br /&gt;
** Grading to deep salmon or mauve near the horizon,&lt;br /&gt;
** A slight metallic sheen due to noble gas content and high pressure.&lt;br /&gt;
&lt;br /&gt;
Twilight &amp;amp; Limb Scattering:&lt;br /&gt;
* The terminator (twilight zone) sees a diffuse, ruddy light, scattering through haze and clouds into luminous reds, purples, and copper tones.&lt;br /&gt;
* Aurorae are spectacular on the night side, especially since stellar flares are frequent.&lt;br /&gt;
&lt;br /&gt;
==== Sound Propagation ====&lt;br /&gt;
: &#039;&#039;Sound is profoundly affected by atmospheric pressure and composition.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Compared to Earth:&lt;br /&gt;
* Higher pressure → greater air density → faster transmission of sound and less attenuation.&lt;br /&gt;
* Argon and Xenon are heavy gases, which:&lt;br /&gt;
** Lower the speed of sound relative to air at the same pressure (despite the pressure increase).&lt;br /&gt;
** Shift resonance frequencies downward, resulting in deeper, rounder sounds.&lt;br /&gt;
&lt;br /&gt;
Consequences:&lt;br /&gt;
* Voices sound subtly lower-pitched and richer, especially for consonants and low vowels.&lt;br /&gt;
* Ambient sounds (wind, water, animals) would carry farther and sound more muffled or sonorous.&lt;br /&gt;
* Music or speech would resonate more warmly, especially indoors or in enclosed spaces.&lt;br /&gt;
&lt;br /&gt;
In short: it sounds like it’s wrapped in velvet.&lt;br /&gt;
&lt;br /&gt;
==== Heat Transport to the Night Side ====&lt;br /&gt;
Mechanisms:&lt;br /&gt;
# Thick Atmosphere (1.6 atm) increases:&lt;br /&gt;
#* Advection efficiency: Warm air masses can move more heat horizontally.&lt;br /&gt;
#* Radiative time constant: The atmosphere holds heat longer before releasing it.&lt;br /&gt;
# Noble Gases (especially Kr/Xe):&lt;br /&gt;
#* High molecular mass → more IR opacity → trapping and radiating heat more evenly.&lt;br /&gt;
# Slow Rotation / Tidal Locking:&lt;br /&gt;
#* Global Hadley-like cells dominate circulation, carrying warm air from the day side to the night side and descending it there.&lt;br /&gt;
&lt;br /&gt;
Result:&lt;br /&gt;
* The night side is not so freezing.  Temperatures differ by tens of degrees, not hundreds.&lt;br /&gt;
* There are still ice caps and a cold deserts at the anti-stellar point, but not a glaciated wasteland.&lt;br /&gt;
&lt;br /&gt;
=== Magnetosphere ===&lt;br /&gt;
* Larger mass --&amp;gt; larger iron core, generating more internal heat&lt;br /&gt;
* Larger radius --&amp;gt; Vigorous convection in the core&lt;br /&gt;
* Tidal Flexing --&amp;gt; still drives magnetic activity&lt;br /&gt;
&lt;br /&gt;
# Aurorae at lower latitudes&lt;br /&gt;
## higher magnetic rigidity, wider magnetotail, and greater reconnection energy.&lt;br /&gt;
## Combined with a higher flux of stellar particles, this means:&lt;br /&gt;
### Auroral ovals expand, reaching mid-latitudes sometimes equator.&lt;br /&gt;
### The skies are alive with rippling green, violet, and crimson aurorae, especially on the night side.&lt;br /&gt;
### Daily auroral activity occur during stellar flare cycles.&lt;br /&gt;
# Compasses&lt;br /&gt;
## compasses respond more sharply, with:&lt;br /&gt;
### Faster alignment.&lt;br /&gt;
### Greater resistance to local perturbations.&lt;br /&gt;
## However, frequent magnetic storms from stellar activity cause sudden declinations, reversals, or local anomalies.  In short, lots of aurorae equals dead compasses at the same time.&lt;br /&gt;
# Magnetic Field Strength &amp;gt; 100 μT &lt;br /&gt;
# Electromagnetism is more basic than chemistry or almost any other natural philosophy&lt;br /&gt;
&lt;br /&gt;
=== Substellar Point ===&lt;br /&gt;
The maximum incoming flux is very nearly the same as Earth&#039;s solar constant (≈1361 W/m²), but concentrated over one point rather than averaged over a rotating sphere.  Temperatures should be above 500ºK most of the time.  &lt;br /&gt;
&lt;br /&gt;
The magnetic north is also here. The thick atmosphere prevents too much loss here, but &lt;br /&gt;
* Charged particle influx&lt;br /&gt;
** Maximized at the substellar point—intense auroral and energetic particle precipitation&lt;br /&gt;
* Atmospheric ionization&lt;br /&gt;
** Constant production of high-energy ions and NOx compounds—UV fluorescence in upper sky&lt;br /&gt;
* Localized heating&lt;br /&gt;
** Augments already extreme temperatures—600–700 K surface&lt;br /&gt;
&lt;br /&gt;
== Artificially Tethered Moon ==&lt;br /&gt;
* 670,000 km up&lt;br /&gt;
* 7805 km in radius = same as the planet&lt;br /&gt;
* 1.33º of the sky, same as the sun&lt;br /&gt;
&lt;br /&gt;
A network of tethers/tension lines from the moon to multiple anchor points on the planet’s surface (a tripod or hexapod structure), woven like hair&lt;br /&gt;
* Uses active tension management and orbital station-keeping to stabilize the moon&lt;br /&gt;
* Counterweights and inward-pointing mass drivers on the moon to oppose drift&lt;br /&gt;
&lt;br /&gt;
The tethers are not bearing the full weight, but merely damping drift, providing restoring force, and enabling long-term stability through active compensation.  The moon&lt;br /&gt;
* Blocks the worst of the heat&lt;br /&gt;
* Blocks the worst of the solar radiation&lt;br /&gt;
The moon has &lt;br /&gt;
* low mass&lt;br /&gt;
* high albedo - enormous reflectivity&lt;br /&gt;
* scatters charges particles, UV, X-rays, auroral flux tubes&lt;br /&gt;
* sunward - crazy hot, high emissivity&lt;br /&gt;
* earthward - crazy cool, low emissivity&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a&amp;diff=168550</id>
		<title>Ɬiʔa</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a&amp;diff=168550"/>
		<updated>2025-04-02T00:31:20Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* Morphology */ inclusive and 2nd don&amp;#039;t mix&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Goals ==&lt;br /&gt;
# Endgoal - A truly verbless language I can use&lt;br /&gt;
# Vague phrases&lt;br /&gt;
## Glacial pace&lt;br /&gt;
## Navajo-of-nouns&lt;br /&gt;
## lazy but clever&lt;br /&gt;
## carved in stone&lt;br /&gt;
## complicated rituals&lt;br /&gt;
# Naturalism - 6/10&lt;br /&gt;
#* I want some naturalistic elements&lt;br /&gt;
#* Different setting (parallel Earth)&lt;br /&gt;
#* Different nature (immortal humans)&lt;br /&gt;
#* Irregularities but not many&lt;br /&gt;
#* Idioms within reason&lt;br /&gt;
# Complexity - insane.  Navajo but with only nouns&lt;br /&gt;
# Derivation - clear.  Agglutinative, basically&lt;br /&gt;
# Features&lt;br /&gt;
## Phonology &lt;br /&gt;
### Vowel harmony&lt;br /&gt;
### A couple of clicks, and ejectives (un-earth-like)&lt;br /&gt;
### CV, and CVC &lt;br /&gt;
## Grammar&lt;br /&gt;
### No verbs at all&lt;br /&gt;
### assumed copular between topic and subject&lt;br /&gt;
### 6 nouns classes (genders), like animacy &lt;br /&gt;
### Many cases (12?)&lt;br /&gt;
### Case-stacking&lt;br /&gt;
### word glue, like German&lt;br /&gt;
### mostly agglutinative, touch of fusional&lt;br /&gt;
## Culture&lt;br /&gt;
### things happen, not because someone does them, but because the world unfolds in prescribed patterns&lt;br /&gt;
### discourse is formulaic, ceremonial, or sacred: more on set relational expressions and fixed semantic roles, rather than on active description of novel events&lt;br /&gt;
### agency is less linguistically salient, so predicates assigning blame, initiative, or creativity are avoided&lt;br /&gt;
### Tidally Locked Planet&lt;br /&gt;
#### The sun never moves in the sky.&lt;br /&gt;
#### The world is divided into zones of permanent day, eternal night, and a narrow habitable twilight ring.&lt;br /&gt;
#### People live in a stable band where temperature and light are forever the same.&lt;br /&gt;
### Mountain life&lt;br /&gt;
#### Isolated communities → heavy internal consistency, less external pressure to simplify&lt;br /&gt;
#### Thin air → favoring sharp, closed articulation: ejectives, glottalization, voiceless stops&lt;br /&gt;
#### Cultural inwardness → deep philosophies of stasis and permanence&lt;br /&gt;
### Time is measured in generations, epochs, weathering of stone, growth cycles of ultra-slow plants&lt;br /&gt;
&lt;br /&gt;
{{See also|Ɬiʔa/Conworlding}}&lt;br /&gt;
&lt;br /&gt;
== Morphology ==&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Case !! Function !! Gloss !! Ending&lt;br /&gt;
|+ Existential cases&lt;br /&gt;
|-&lt;br /&gt;
! Topical&lt;br /&gt;
| Frames the referent of the utterance ||	“As for…”&lt;br /&gt;
! -mxa&lt;br /&gt;
|-&lt;br /&gt;
! Identity&lt;br /&gt;
| Category, essence, nominal predicate ||	“is a…” / “equals…”&lt;br /&gt;
! -&lt;br /&gt;
|-&lt;br /&gt;
! Possessive&lt;br /&gt;
| ownership, authorship, kinship, part-whole || “X’s Y”&lt;br /&gt;
! -rkI&lt;br /&gt;
|-&lt;br /&gt;
! Partitive &lt;br /&gt;
| part-to-whole, uncertainty, scalarity || &amp;quot;some of, partially&amp;quot;&lt;br /&gt;
! -g(Ö)&lt;br /&gt;
|-&lt;br /&gt;
! Genitive	&lt;br /&gt;
| association, content, theme, objective, attribution || “Y of X”&lt;br /&gt;
! -ł(Ö)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Where/When Cases&lt;br /&gt;
! Case !!	Function !!	Typical gloss !! Ending&lt;br /&gt;
|-&lt;br /&gt;
! Locative&lt;br /&gt;
| Place, state, context of being, time-within ||	“in,” “at,” “on”, &amp;quot;during&amp;quot;&lt;br /&gt;
! -z&lt;br /&gt;
|-&lt;br /&gt;
! Dative&lt;br /&gt;
| Target, direction ||	“to,” “for,” “until&amp;quot;, &amp;quot;as far as&amp;quot;&lt;br /&gt;
! -n!O&lt;br /&gt;
|-&lt;br /&gt;
! Ablative&lt;br /&gt;
| Source, cause, origin || “from,” “because of,” “due to”&lt;br /&gt;
! -bdI&lt;br /&gt;
|-&lt;br /&gt;
! Benefactive&lt;br /&gt;
| Advantage, interest, concern || “for the benefit of…”, &amp;quot;at the behest of&amp;quot;&lt;br /&gt;
! -aI&lt;br /&gt;
|-&lt;br /&gt;
! Abessive&lt;br /&gt;
| Absence, privation, “lacking”	|| “without,” “lacking,” “free from”, &amp;quot;exclude&amp;quot;&lt;br /&gt;
! -st&#039;Ö&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ How Cases&lt;br /&gt;
! Case !! Function 	!! Typical gloss !! Ending&lt;br /&gt;
|-&lt;br /&gt;
! Instrumental &lt;br /&gt;
| Means, medium, material || “by (means of)”, “through,” “with”, &amp;quot;using&amp;quot;&lt;br /&gt;
! -fla&lt;br /&gt;
|-&lt;br /&gt;
! Adverbial&lt;br /&gt;
| Role/state modifier, part of speech shift	|| “as (a) X,” “in a X way”, &amp;quot;like&amp;quot;&lt;br /&gt;
! -Oad&lt;br /&gt;
|-&lt;br /&gt;
! Translative&lt;br /&gt;
| Change of state, transform/manifestation ||	“becoming,” “into,” “turning into”&lt;br /&gt;
! -k&#039;(I)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Noun Classes&lt;br /&gt;
! !! Not &amp;quot;Container&amp;quot; (mass: paucal, whole) !! &amp;quot;Container&amp;quot; (count: number)&lt;br /&gt;
|-&lt;br /&gt;
! Idea + Matter	&lt;br /&gt;
| Animals (also temperaments) || 	Persons / Gods&lt;br /&gt;
|-&lt;br /&gt;
! Matter only	&lt;br /&gt;
| (Diffuse) Substances: air, fire || 	Tools , &amp;quot;rocks&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
! Idea only	&lt;br /&gt;
| Actions	|| Abstracts, Categories, Sets&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Number: Containers are unmarked for number, as in Chinese/Japanese/Korean.  Non-containers default to a collective/mass-noun number, but can take a paucal (which can mean as few as one).&lt;br /&gt;
&lt;br /&gt;
Polypersonal pronouns:&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! !! 1x !! 1n !! 2 !! 3P !! 3T !! 3R !! 3D !! 3S !! 3A !! 4&lt;br /&gt;
|-&lt;br /&gt;
! 1x !! ø !! ø&lt;br /&gt;
|       tifq ||  tis ||  tił ||  tiwi || tiþ || tið || tiv || tir&lt;br /&gt;
|-&lt;br /&gt;
! 1in !! ø !! ø !! ø&lt;br /&gt;
|        tqis ||  tqił ||  tqiwi || tqiþ || tqið || tqiv || tqir        &lt;br /&gt;
|-&lt;br /&gt;
! 2&lt;br /&gt;
| fqwöt &lt;br /&gt;
! ø&lt;br /&gt;
! ø&lt;br /&gt;
|                  fqwös || fqwöł || fqwöu || fqwöþ || fqwöð || fqwöv || fqwör &lt;br /&gt;
|-&lt;br /&gt;
! 3P&lt;br /&gt;
| sjet || sjetq || sjefq &lt;br /&gt;
! ø&lt;br /&gt;
|                   sjeł || sjewi || sjeþ || sjeð || sjev || sjer&lt;br /&gt;
|-&lt;br /&gt;
! 3T&lt;br /&gt;
| łot || łotq || łofq || łos&lt;br /&gt;
! ø&lt;br /&gt;
|                        łou || łoþ || łoð || łov || łor&lt;br /&gt;
|-&lt;br /&gt;
! 3R&lt;br /&gt;
| ut || utq || ufq || us || uł&lt;br /&gt;
! ø&lt;br /&gt;
|                           uþ || uð || uv || ur&lt;br /&gt;
|-&lt;br /&gt;
! 3D&lt;br /&gt;
| þwöt || þwötq || þwöfq || þwös || þwöł || þwöu&lt;br /&gt;
! ø&lt;br /&gt;
|                                þwöð || þwöv || þwör&lt;br /&gt;
|-&lt;br /&gt;
! 3S&lt;br /&gt;
| ðet || ðetq || ðefq || ðes || ðeł || ðewi || ðeþ&lt;br /&gt;
! ø&lt;br /&gt;
|                                       ðev || ðer&lt;br /&gt;
|-&lt;br /&gt;
! 3S&lt;br /&gt;
| vöt || vötq || vöfq || vös || vöł || vöu || vöþ || vöð&lt;br /&gt;
! ø&lt;br /&gt;
| vör&lt;br /&gt;
|-&lt;br /&gt;
! 4&lt;br /&gt;
| rut || rutq || rufq || rus || ruł || ruwu || ruþ || ruð || ruv&lt;br /&gt;
! ø&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
== Phonology/Orthography ==&lt;br /&gt;
{| class=&amp;quot;bluetable&amp;quot; style=&amp;quot;text-align:center; float:left&amp;quot;&lt;br /&gt;
! !!	Labial !!	Labiolingual !!	Alveolar !!	Palatal !! Velar !!	Glottal&lt;br /&gt;
|-&lt;br /&gt;
! Nasal	&lt;br /&gt;
| colspan=&amp;quot;3&amp;quot; | /m~n/ &#039;&#039;&#039;M&#039;&#039;&#039; || (/ɲ/ &#039;&#039;&#039;nj&#039;&#039;&#039;) || /ŋ/ &#039;&#039;&#039;M&#039;&#039;&#039;			||&lt;br /&gt;
|-&lt;br /&gt;
! Click&lt;br /&gt;
| colspan=&amp;quot;2&amp;quot; | (/ᵐʘ/ &#039;&#039;&#039;mx&#039;&#039;&#039;) || colspan=&amp;quot;3&amp;quot; | (/ŋǃ/ &#039;&#039;&#039;y&#039;&#039;&#039;) || &lt;br /&gt;
|-&lt;br /&gt;
! Voiced Stop&lt;br /&gt;
| &#039;&#039;&#039;b&#039;&#039;&#039; || 	||	&#039;&#039;&#039;d&#039;&#039;&#039; ||	(/dʑ/ &#039;&#039;&#039;dj&#039;&#039;&#039;) || &#039;&#039;&#039;g&#039;&#039;&#039;	||&lt;br /&gt;
|-&lt;br /&gt;
! Eject. Stop&lt;br /&gt;
| /pʼ/ &#039;&#039;&#039;pq&#039;&#039;&#039; ||	|| /t’/ &#039;&#039;&#039;tq&#039;&#039;&#039;	|| /c&#039;/ &#039;&#039;&#039;cq&#039;&#039;&#039; || /k’/ &#039;&#039;&#039;kq&#039;&#039;&#039; ||	/ʔ/ &#039;&#039;&#039; &#039; &#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Unvoiced Stop&lt;br /&gt;
| &#039;&#039;&#039;p&#039;&#039;&#039; ||	||	&#039;&#039;&#039;t&#039;&#039;&#039; || (/tɕ/ &#039;&#039;&#039;tj&#039;&#039;&#039;) || /k~x/ &#039;&#039;&#039;k&#039;&#039;&#039;	||&lt;br /&gt;
|-&lt;br /&gt;
! Voiced Fricative&lt;br /&gt;
| /β~v/ &#039;&#039;&#039;v&#039;&#039;&#039; || /ð̼/ &#039;&#039;&#039;ð&#039;&#039;&#039; || &#039;&#039;&#039;z&#039;&#039;&#039; || (/ʒ/ &#039;&#039;&#039;zj&#039;&#039;&#039;) || ||&lt;br /&gt;
|-&lt;br /&gt;
! Unvoiced Fricative&lt;br /&gt;
| /ɸ~f/ &#039;&#039;&#039;f&#039;&#039;&#039; ||	/θ̼/ &#039;&#039;&#039;þ&#039;&#039;&#039;	|| &#039;&#039;&#039;s&#039;&#039;&#039; || (/ʃ/ &#039;&#039;&#039;sj&#039;&#039;&#039;) || ||&lt;br /&gt;
|-&lt;br /&gt;
! Eject. Fricative&lt;br /&gt;
| /fʼ/ &#039;&#039;&#039;fq&#039;&#039;&#039; ||	/θ̼ʼ/ &#039;&#039;&#039;þq&#039;&#039;&#039; || /s’~ts’/ &#039;&#039;&#039;sq&#039;&#039;&#039;		|| || ||&lt;br /&gt;
|-&lt;br /&gt;
! Approx./Trill	&lt;br /&gt;
| &#039;&#039;&#039;w&#039;&#039;&#039;	|| || &#039;&#039;&#039;r&#039;&#039;&#039; || &#039;&#039;&#039;j&#039;&#039;&#039; ||	|| /h~ɦ/ &#039;&#039;&#039;h&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Laterals&lt;br /&gt;
| || /l̼/ &#039;&#039;&#039;l&#039;&#039;&#039; ||	/ɬ/ &#039;&#039;&#039;ł&#039;&#039;&#039;		|| (/ʎ/ &#039;&#039;&#039;lj&#039;&#039;&#039;) || ||&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;bluetable&amp;quot; style=&amp;quot;float:right; text-align:center;&amp;quot;&lt;br /&gt;
! !! Front !! Back !! Underspecified&lt;br /&gt;
|-&lt;br /&gt;
! High&lt;br /&gt;
| &#039;&#039;&#039;i&#039;&#039;&#039; || &#039;&#039;&#039;u&#039;&#039;&#039; || I&lt;br /&gt;
|-&lt;br /&gt;
! High-Mid&lt;br /&gt;
| &#039;&#039;&#039;e&#039;&#039;&#039; || &#039;&#039;&#039;o&#039;&#039;&#039; || O&lt;br /&gt;
|-&lt;br /&gt;
! Low-Mid&lt;br /&gt;
| /ɛ/ &#039;&#039;&#039;ë&#039;&#039;&#039; || /ɔ/ &#039;&#039;&#039;ö&#039;&#039;&#039; || Ö&lt;br /&gt;
|-&lt;br /&gt;
! Low&lt;br /&gt;
| colspan=&amp;quot;2&amp;quot; | /ä/ &#039;&#039;&#039;a&#039;&#039;&#039;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Allophony:&lt;br /&gt;
* nasal + labial ejective -&amp;gt; [m͡ʘ]&lt;br /&gt;
* nasal + non-labial ejective -&amp;gt; [ŋ͡ǃ]&lt;br /&gt;
&lt;br /&gt;
Phonotactics are (C)(G)V(C&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;):&lt;br /&gt;
* any consonant or none can a syllable&lt;br /&gt;
* Glides (/j/ or /w/) after anything, if after nothing, insert glottal stop&lt;br /&gt;
* hiatus allowed, diphthongs not&lt;br /&gt;
* any coda, except glides&lt;br /&gt;
&lt;br /&gt;
=== Sentences ===&lt;br /&gt;
# The storm scared the people.&lt;br /&gt;
#* vökqöthumxa &#039;usëk venargofq&lt;br /&gt;
#* As for the storm, (there is) fear in the people.&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a&amp;diff=168458</id>
		<title>Ɬiʔa</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a&amp;diff=168458"/>
		<updated>2025-04-01T01:18:42Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* Morphology */ typo&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Goals ==&lt;br /&gt;
# Endgoal - A truly verbless language I can use&lt;br /&gt;
# Vague phrases&lt;br /&gt;
## Glacial pace&lt;br /&gt;
## Navajo-of-nouns&lt;br /&gt;
## lazy but clever&lt;br /&gt;
## carved in stone&lt;br /&gt;
## complicated rituals&lt;br /&gt;
# Naturalism - 6/10&lt;br /&gt;
#* I want some naturalistic elements&lt;br /&gt;
#* Different setting (parallel Earth)&lt;br /&gt;
#* Different nature (immortal humans)&lt;br /&gt;
#* Irregularities but not many&lt;br /&gt;
#* Idioms within reason&lt;br /&gt;
# Complexity - insane.  Navajo but with only nouns&lt;br /&gt;
# Derivation - clear.  Agglutinative, basically&lt;br /&gt;
# Features&lt;br /&gt;
## Phonology &lt;br /&gt;
### Vowel harmony&lt;br /&gt;
### A couple of clicks, and ejectives (un-earth-like)&lt;br /&gt;
### CV, and CVC &lt;br /&gt;
## Grammar&lt;br /&gt;
### No verbs at all&lt;br /&gt;
### assumed copular between topic and subject&lt;br /&gt;
### 6 nouns classes (genders), like animacy &lt;br /&gt;
### Many cases (12?)&lt;br /&gt;
### Case-stacking&lt;br /&gt;
### word glue, like German&lt;br /&gt;
### mostly agglutinative, touch of fusional&lt;br /&gt;
## Culture&lt;br /&gt;
### things happen, not because someone does them, but because the world unfolds in prescribed patterns&lt;br /&gt;
### discourse is formulaic, ceremonial, or sacred: more on set relational expressions and fixed semantic roles, rather than on active description of novel events&lt;br /&gt;
### agency is less linguistically salient, so predicates assigning blame, initiative, or creativity are avoided&lt;br /&gt;
### Tidally Locked Planet&lt;br /&gt;
#### The sun never moves in the sky.&lt;br /&gt;
#### The world is divided into zones of permanent day, eternal night, and a narrow habitable twilight ring.&lt;br /&gt;
#### People live in a stable band where temperature and light are forever the same.&lt;br /&gt;
### Mountain life&lt;br /&gt;
#### Isolated communities → heavy internal consistency, less external pressure to simplify&lt;br /&gt;
#### Thin air → favoring sharp, closed articulation: ejectives, glottalization, voiceless stops&lt;br /&gt;
#### Cultural inwardness → deep philosophies of stasis and permanence&lt;br /&gt;
### Time is measured in generations, epochs, weathering of stone, growth cycles of ultra-slow plants&lt;br /&gt;
&lt;br /&gt;
{{See also|Ɬiʔa/Conworlding}}&lt;br /&gt;
&lt;br /&gt;
== Morphology ==&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Case !! Function !! Gloss !! Ending&lt;br /&gt;
|+ Existential cases&lt;br /&gt;
|-&lt;br /&gt;
! Topical&lt;br /&gt;
| Frames the referent of the utterance ||	“As for…”&lt;br /&gt;
! -mxa&lt;br /&gt;
|-&lt;br /&gt;
! Identity&lt;br /&gt;
| Category, essence, nominal predicate ||	“is a…” / “equals…”&lt;br /&gt;
! -&lt;br /&gt;
|-&lt;br /&gt;
! Possessive&lt;br /&gt;
| ownership, authorship, kinship, part-whole || “X’s Y”&lt;br /&gt;
! -rkI&lt;br /&gt;
|-&lt;br /&gt;
! Partitive &lt;br /&gt;
| part-to-whole, uncertainty, scalarity || &amp;quot;some of, partially&amp;quot;&lt;br /&gt;
! -g(Ö)&lt;br /&gt;
|-&lt;br /&gt;
! Genitive	&lt;br /&gt;
| association, content, theme, objective, attribution || “Y of X”&lt;br /&gt;
! -ł(Ö)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Where/When Cases&lt;br /&gt;
! Case !!	Function !!	Typical gloss !! Ending&lt;br /&gt;
|-&lt;br /&gt;
! Locative&lt;br /&gt;
| Place, state, context of being, time-within ||	“in,” “at,” “on”, &amp;quot;during&amp;quot;&lt;br /&gt;
! -z&lt;br /&gt;
|-&lt;br /&gt;
! Dative&lt;br /&gt;
| Target, direction ||	“to,” “for,” “until&amp;quot;, &amp;quot;as far as&amp;quot;&lt;br /&gt;
! -n!O&lt;br /&gt;
|-&lt;br /&gt;
! Ablative&lt;br /&gt;
| Source, cause, origin || “from,” “because of,” “due to”&lt;br /&gt;
! -bdI&lt;br /&gt;
|-&lt;br /&gt;
! Benefactive&lt;br /&gt;
| Advantage, interest, concern || “for the benefit of…”, &amp;quot;at the behest of&amp;quot;&lt;br /&gt;
! -aI&lt;br /&gt;
|-&lt;br /&gt;
! Abessive&lt;br /&gt;
| Absence, privation, “lacking”	|| “without,” “lacking,” “free from”, &amp;quot;exclude&amp;quot;&lt;br /&gt;
! -st&#039;Ö&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ How Cases&lt;br /&gt;
! Case !! Function 	!! Typical gloss !! Ending&lt;br /&gt;
|-&lt;br /&gt;
! Instrumental &lt;br /&gt;
| Means, medium, material || “by (means of)”, “through,” “with”, &amp;quot;using&amp;quot;&lt;br /&gt;
! -fla&lt;br /&gt;
|-&lt;br /&gt;
! Adverbial&lt;br /&gt;
| Role/state modifier, part of speech shift	|| “as (a) X,” “in a X way”, &amp;quot;like&amp;quot;&lt;br /&gt;
! -Oad&lt;br /&gt;
|-&lt;br /&gt;
! Translative&lt;br /&gt;
| Change of state, transform/manifestation ||	“becoming,” “into,” “turning into”&lt;br /&gt;
! -k&#039;(I)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Noun Classes&lt;br /&gt;
! !! Not &amp;quot;Container&amp;quot; (mass: paucal, whole) !! &amp;quot;Container&amp;quot; (count: number)&lt;br /&gt;
|-&lt;br /&gt;
! Idea + Matter	&lt;br /&gt;
| Animals (also temperaments) || 	Persons / Gods&lt;br /&gt;
|-&lt;br /&gt;
! Matter only	&lt;br /&gt;
| (Diffuse) Substances: air, fire || 	Tools , &amp;quot;rocks&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
! Idea only	&lt;br /&gt;
| Actions	|| Abstracts, Categories, Sets&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Number: Containers are unmarked for number, as in Chinese/Japanese/Korean.  Non-containers default to a collective/mass-noun number, but can take a paucal (which can mean as few as one).&lt;br /&gt;
&lt;br /&gt;
Polypersonal pronouns:&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! !! 1x !! 1n !! 2 !! 3P !! 3T !! 3R !! 3D !! 3S !! 3A !! 4&lt;br /&gt;
|-&lt;br /&gt;
! 1x !! ø !! ø&lt;br /&gt;
|       tifq ||  tis ||  tił ||  tiwi || tiþ || tið || tiv || tir&lt;br /&gt;
|-&lt;br /&gt;
! 1in !! ø !! ø&lt;br /&gt;
|       tqifq ||  tqis ||  tqił ||  tqiwi || tqiþ || tqið || tqiv || tqir        &lt;br /&gt;
|-&lt;br /&gt;
! 2&lt;br /&gt;
| fqwöt || fqwötq&lt;br /&gt;
! ø&lt;br /&gt;
|                  fqwös || fqwöł || fqwöu || fqwöþ || fqwöð || fqwöv || fqwör &lt;br /&gt;
|-&lt;br /&gt;
! 3P&lt;br /&gt;
| sjet || sjetq || sjefq &lt;br /&gt;
! ø&lt;br /&gt;
|                   sjeł || sjewi || sjeþ || sjeð || sjev || sjer&lt;br /&gt;
|-&lt;br /&gt;
! 3T&lt;br /&gt;
| łot || łotq || łofq || łos&lt;br /&gt;
! ø&lt;br /&gt;
|                        łou || łoþ || łoð || łov || łor&lt;br /&gt;
|-&lt;br /&gt;
! 3R&lt;br /&gt;
| ut || utq || ufq || us || uł&lt;br /&gt;
! ø&lt;br /&gt;
|                           uþ || uð || uv || ur&lt;br /&gt;
|-&lt;br /&gt;
! 3D&lt;br /&gt;
| þwöt || þwötq || þwöfq || þwös || þwöł || þwöu&lt;br /&gt;
! ø&lt;br /&gt;
|                                þwöð || þwöv || þwör&lt;br /&gt;
|-&lt;br /&gt;
! 3S&lt;br /&gt;
| ðet || ðetq || ðefq || ðes || ðeł || ðewi || ðeþ&lt;br /&gt;
! ø&lt;br /&gt;
|                                       ðev || ðer&lt;br /&gt;
|-&lt;br /&gt;
! 3S&lt;br /&gt;
| vöt || vötq || vöfq || vös || vöł || vöu || vöþ || vöð&lt;br /&gt;
! ø&lt;br /&gt;
| vör&lt;br /&gt;
|-&lt;br /&gt;
! 4&lt;br /&gt;
| rut || rutq || rufq || rus || ruł || ruwu || ruþ || ruð || ruv&lt;br /&gt;
! ø&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
== Phonology/Orthography ==&lt;br /&gt;
{| class=&amp;quot;bluetable&amp;quot; style=&amp;quot;text-align:center; float:left&amp;quot;&lt;br /&gt;
! !!	Labial !!	Labiolingual !!	Alveolar !!	Palatal !! Velar !!	Glottal&lt;br /&gt;
|-&lt;br /&gt;
! Nasal	&lt;br /&gt;
| colspan=&amp;quot;3&amp;quot; | /m~n/ &#039;&#039;&#039;M&#039;&#039;&#039; || (/ɲ/ &#039;&#039;&#039;nj&#039;&#039;&#039;) || /ŋ/ &#039;&#039;&#039;M&#039;&#039;&#039;			||&lt;br /&gt;
|-&lt;br /&gt;
! Click&lt;br /&gt;
| colspan=&amp;quot;2&amp;quot; | (/ᵐʘ/ &#039;&#039;&#039;mx&#039;&#039;&#039;) || colspan=&amp;quot;3&amp;quot; | (/ŋǃ/ &#039;&#039;&#039;y&#039;&#039;&#039;) || &lt;br /&gt;
|-&lt;br /&gt;
! Voiced Stop&lt;br /&gt;
| &#039;&#039;&#039;b&#039;&#039;&#039; || 	||	&#039;&#039;&#039;d&#039;&#039;&#039; ||	(/dʑ/ &#039;&#039;&#039;dj&#039;&#039;&#039;) || &#039;&#039;&#039;g&#039;&#039;&#039;	||&lt;br /&gt;
|-&lt;br /&gt;
! Eject. Stop&lt;br /&gt;
| /pʼ/ &#039;&#039;&#039;pq&#039;&#039;&#039; ||	|| /t’/ &#039;&#039;&#039;tq&#039;&#039;&#039;	|| /c&#039;/ &#039;&#039;&#039;cq&#039;&#039;&#039; || /k’/ &#039;&#039;&#039;kq&#039;&#039;&#039; ||	/ʔ/ &#039;&#039;&#039; &#039; &#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Unvoiced Stop&lt;br /&gt;
| &#039;&#039;&#039;p&#039;&#039;&#039; ||	||	&#039;&#039;&#039;t&#039;&#039;&#039; || (/tɕ/ &#039;&#039;&#039;tj&#039;&#039;&#039;) || /k~x/ &#039;&#039;&#039;k&#039;&#039;&#039;	||&lt;br /&gt;
|-&lt;br /&gt;
! Voiced Fricative&lt;br /&gt;
| /β~v/ &#039;&#039;&#039;v&#039;&#039;&#039; || /ð̼/ &#039;&#039;&#039;ð&#039;&#039;&#039; || &#039;&#039;&#039;z&#039;&#039;&#039; || (/ʒ/ &#039;&#039;&#039;zj&#039;&#039;&#039;) || ||&lt;br /&gt;
|-&lt;br /&gt;
! Unvoiced Fricative&lt;br /&gt;
| /ɸ~f/ &#039;&#039;&#039;f&#039;&#039;&#039; ||	/θ̼/ &#039;&#039;&#039;þ&#039;&#039;&#039;	|| &#039;&#039;&#039;s&#039;&#039;&#039; || (/ʃ/ &#039;&#039;&#039;sj&#039;&#039;&#039;) || ||&lt;br /&gt;
|-&lt;br /&gt;
! Eject. Fricative&lt;br /&gt;
| /fʼ/ &#039;&#039;&#039;fq&#039;&#039;&#039; ||	/θ̼ʼ/ &#039;&#039;&#039;þq&#039;&#039;&#039; || /s’~ts’/ &#039;&#039;&#039;sq&#039;&#039;&#039;		|| || ||&lt;br /&gt;
|-&lt;br /&gt;
! Approx./Trill	&lt;br /&gt;
| &#039;&#039;&#039;w&#039;&#039;&#039;	|| || &#039;&#039;&#039;r&#039;&#039;&#039; || &#039;&#039;&#039;j&#039;&#039;&#039; ||	|| /h~ɦ/ &#039;&#039;&#039;h&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Laterals&lt;br /&gt;
| || /l̼/ &#039;&#039;&#039;l&#039;&#039;&#039; ||	/ɬ/ &#039;&#039;&#039;ł&#039;&#039;&#039;		|| (/ʎ/ &#039;&#039;&#039;lj&#039;&#039;&#039;) || ||&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;bluetable&amp;quot; style=&amp;quot;float:right; text-align:center;&amp;quot;&lt;br /&gt;
! !! Front !! Back !! Underspecified&lt;br /&gt;
|-&lt;br /&gt;
! High&lt;br /&gt;
| &#039;&#039;&#039;i&#039;&#039;&#039; || &#039;&#039;&#039;u&#039;&#039;&#039; || I&lt;br /&gt;
|-&lt;br /&gt;
! High-Mid&lt;br /&gt;
| &#039;&#039;&#039;e&#039;&#039;&#039; || &#039;&#039;&#039;o&#039;&#039;&#039; || O&lt;br /&gt;
|-&lt;br /&gt;
! Low-Mid&lt;br /&gt;
| /ɛ/ &#039;&#039;&#039;ë&#039;&#039;&#039; || /ɔ/ &#039;&#039;&#039;ö&#039;&#039;&#039; || Ö&lt;br /&gt;
|-&lt;br /&gt;
! Low&lt;br /&gt;
| colspan=&amp;quot;2&amp;quot; | /ä/ &#039;&#039;&#039;a&#039;&#039;&#039;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Allophony:&lt;br /&gt;
* nasal + labial ejective -&amp;gt; [m͡ʘ]&lt;br /&gt;
* nasal + non-labial ejective -&amp;gt; [ŋ͡ǃ]&lt;br /&gt;
&lt;br /&gt;
Phonotactics are (C)(G)V(C&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;):&lt;br /&gt;
* any consonant or none can a syllable&lt;br /&gt;
* Glides (/j/ or /w/) after anything, if after nothing, insert glottal stop&lt;br /&gt;
* hiatus allowed, diphthongs not&lt;br /&gt;
* any coda, except glides&lt;br /&gt;
&lt;br /&gt;
=== Sentences ===&lt;br /&gt;
# The storm scared the people.&lt;br /&gt;
#* vökqöthumxa &#039;usëk venargofq&lt;br /&gt;
#* As for the storm, (there is) fear in the people.&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=User_talk:Masako&amp;diff=168432</id>
		<title>User talk:Masako</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=User_talk:Masako&amp;diff=168432"/>
		<updated>2025-03-31T18:39:58Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* 완 */ new section&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;==Category tags==&lt;br /&gt;
The categories that you marked &amp;quot;for deletion&amp;quot;- do you want all the included images removed?  I&#039;m hesitant to just empty them out without making absolutely sure.  - [[User:Bornfor|bornfor]] 11:27 (EDT) 15 Nov 2012&lt;br /&gt;
&lt;br /&gt;
: [[User:Bornfor|bornfor]], thank you for clarifying/verifying, and the answer is a resounding &#039;&#039;&#039;yes&#039;&#039;&#039;. I do &#039;&#039;&#039;NOT&#039;&#039;&#039; want/need the images for any current/future projects. [[User:Masako|masako]]&lt;br /&gt;
&lt;br /&gt;
== Vingdagese ==&lt;br /&gt;
I finally noticed your comment over [[Talk:Vingdagese#Kudos|there]], and responded to it. Thought I would leave a line here as it isn&#039;t likely that you&#039;d see it otherwise. :) — [[File:Pill-37.png|24px|link=User:Thirty7]]&amp;amp;nbsp;{{small|[[User talk:Thirty7|Talk]] {{dot}} [[Special:Contributions/Thirty7|Cont]]}}&amp;amp;nbsp; 01:24, 11 January 2020 (PST)&lt;br /&gt;
&lt;br /&gt;
== Some questions on Kala lexicon ==&lt;br /&gt;
&lt;br /&gt;
Yata! A few questions on your Kala lexicon.&lt;br /&gt;
&lt;br /&gt;
#Is &#039;&#039;&#039;hasi&#039;&#039;&#039; derived from the Japanese &amp;quot;hashi&amp;quot;?&lt;br /&gt;
## Yes. [[User:Masako|masako]] ([[User talk:Masako|talk]])&lt;br /&gt;
### Yay! Got it right! [[User:Khemehekis|Khemehekis]] ([[User talk:Khemehekis|talk]])&lt;br /&gt;
#Am I correct in guessing that &#039;&#039;&#039;apakipyo&#039;&#039;&#039; comes from a Kalanization of the name &amp;quot;Asperger&amp;quot;, plus the word &#039;&#039;&#039;pyo&#039;&#039;&#039; meaning disease?&lt;br /&gt;
## No. &#039;&#039;&#039;apa&#039;&#039;&#039; means &amp;quot;closed, shut&amp;quot;; &#039;&#039;&#039;ki&#039;&#039;&#039; means &amp;quot;self, reflexive&amp;quot;; and &#039;&#039;&#039;-pyo&#039;&#039;&#039; is from &amp;quot;disease; illness&amp;quot; [[User:Masako|masako]] ([[User talk:Masako|talk]])&lt;br /&gt;
### So I was way off! (Well, except for the &#039;&#039;&#039;-pyo&#039;&#039;&#039; part.) Interesting that it&#039;s just a coincidence that apaki- looks like &amp;quot;Asperger&amp;quot;. Perhaps &amp;quot;Asperger&amp;quot; would become &#039;&#039;&#039;apaka&#039;&#039;&#039; or &#039;&#039;&#039;apeka&#039;&#039;&#039; in Kala? [[User:Khemehekis|Khemehekis]] ([[User talk:Khemehekis|talk]])&lt;br /&gt;
#Your words for girl (&#039;&#039;&#039;nahi&#039;&#039;&#039;) and boy (&#039;&#039;&#039;tahi&#039;&#039;&#039;) directly tie into &#039;&#039;&#039;ntahi&#039;&#039;&#039; (child). What word would you use for, say, a 16-year-old girl, or a 22-year-old boy?&lt;br /&gt;
## &#039;&#039;&#039;tsonta&#039;&#039;&#039; is used for &amp;quot;teen/ager&amp;quot;, and &#039;&#039;&#039;tlaka&#039;&#039;&#039; or &#039;&#039;&#039;tahi&#039;&#039;&#039; would be used for a 22 year old. [[User:Masako|masako]] ([[User talk:Masako|talk]])&lt;br /&gt;
### I see. So you don&#039;t have to be a &#039;&#039;&#039;ntahi&#039;&#039;&#039; to be a &#039;&#039;&#039;tahi&#039;&#039;&#039; or &#039;&#039;&#039;nahi&#039;&#039;&#039;. [[User:Khemehekis|Khemehekis]] ([[User talk:Khemehekis|talk]])&lt;br /&gt;
###Question: If you wanted to say &amp;quot;teen-age girl&amp;quot;, specifying both the girl&#039;s age group and her gender, would you say &#039;&#039;&#039;tsonta nahi&#039;&#039;&#039;, or &#039;&#039;&#039;nahi tsonta&#039;&#039;&#039;, or would one or both of the words be inflected? [[User:Khemehekis|Khemehekis]] ([[User talk:Khemehekis|talk]]) 08:11, 6 October 2020 (PDT)&lt;br /&gt;
#### &amp;quot;teen-age girl&amp;quot; would be &#039;&#039;&#039;tsontana&#039;&#039;&#039; [[User:Masako|masako]] ([[User talk:Masako|talk]])&lt;br /&gt;
#####Thank you! [[User:Khemehekis|Khemehekis]] ([[User talk:Khemehekis|talk]]) 08:43, 6 October 2020 (PDT)&lt;br /&gt;
Thanks for your answers. [[User:Khemehekis|Khemehekis]] ([[User talk:Khemehekis|talk]]) 18:05, 12 January 2020 (PST)&lt;br /&gt;
&lt;br /&gt;
== Reply to &amp;quot;Sentence Enders/Separators ==&lt;br /&gt;
&amp;quot;The image you link to belongs to Bbbourq. masako&amp;quot;&lt;br /&gt;
&lt;br /&gt;
oh, thanks for informing me, although I am surprised you decided to inform me here rather than on the forum. [[User:Ahzoh|Ahzoh]] ([[User talk:Ahzoh|talk]]) 21:52, 2 May 2021 (PDT)&lt;br /&gt;
:Ahzoh, Masako has left the CBB for good. His sig on that board now reads &amp;quot;gone&amp;quot;. [[User:Khemehekis|Khemehekis]] ([[User talk:Khemehekis|talk]]) 13:26, 3 May 2021 (PDT)&lt;br /&gt;
&lt;br /&gt;
== Crediting you on Klingon site ==&lt;br /&gt;
&lt;br /&gt;
Hey, Masako! The page https://klingon.wiki/En/OnlineDictionaries at the Klingon wiki mentions the Klingon lexicon page that you started (and I regularly update) here. But they don&#039;t know who created it, so I&#039;m going to mention that you started the page and I now maintain it. How would you like to be known on that webpage? By Masako? By your real name? By a Klingon name? [[User:Khemehekis|Khemehekis]] ([[User talk:Khemehekis|talk]]) 21:32, 9 March 2024 (PST)&lt;br /&gt;
:: My real name will be fine &amp;quot;Carl Buck&amp;quot;. [[User:Masako|masako]] ([[User talk:Masako|talk]])&lt;br /&gt;
::: OK, thanks! [[User:Khemehekis|Khemehekis]] ([[User talk:Khemehekis|talk]]) 16:06, 10 March 2024 (PDT)&lt;br /&gt;
&lt;br /&gt;
== 완 ==&lt;br /&gt;
&lt;br /&gt;
Why is 완 a pic in your Miyu writing?  I have to know! :-) --11:39, 31 March 2025 (PDT)&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a&amp;diff=168428</id>
		<title>Ɬiʔa</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a&amp;diff=168428"/>
		<updated>2025-03-31T18:35:49Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* Morphology */ big table&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Goals ==&lt;br /&gt;
# Endgoal - A truly verbless language I can use&lt;br /&gt;
# Vague phrases&lt;br /&gt;
## Glacial pace&lt;br /&gt;
## Navajo-of-nouns&lt;br /&gt;
## lazy but clever&lt;br /&gt;
## carved in stone&lt;br /&gt;
## complicated rituals&lt;br /&gt;
# Naturalism - 6/10&lt;br /&gt;
#* I want some naturalistic elements&lt;br /&gt;
#* Different setting (parallel Earth)&lt;br /&gt;
#* Different nature (immortal humans)&lt;br /&gt;
#* Irregularities but not many&lt;br /&gt;
#* Idioms within reason&lt;br /&gt;
# Complexity - insane.  Navajo but with only nouns&lt;br /&gt;
# Derivation - clear.  Agglutinative, basically&lt;br /&gt;
# Features&lt;br /&gt;
## Phonology &lt;br /&gt;
### Vowel harmony&lt;br /&gt;
### A couple of clicks, and ejectives (un-earth-like)&lt;br /&gt;
### CV, and CVC &lt;br /&gt;
## Grammar&lt;br /&gt;
### No verbs at all&lt;br /&gt;
### assumed copular between topic and subject&lt;br /&gt;
### 6 nouns classes (genders), like animacy &lt;br /&gt;
### Many cases (12?)&lt;br /&gt;
### Case-stacking&lt;br /&gt;
### word glue, like German&lt;br /&gt;
### mostly agglutinative, touch of fusional&lt;br /&gt;
## Culture&lt;br /&gt;
### things happen, not because someone does them, but because the world unfolds in prescribed patterns&lt;br /&gt;
### discourse is formulaic, ceremonial, or sacred: more on set relational expressions and fixed semantic roles, rather than on active description of novel events&lt;br /&gt;
### agency is less linguistically salient, so predicates assigning blame, initiative, or creativity are avoided&lt;br /&gt;
### Tidally Locked Planet&lt;br /&gt;
#### The sun never moves in the sky.&lt;br /&gt;
#### The world is divided into zones of permanent day, eternal night, and a narrow habitable twilight ring.&lt;br /&gt;
#### People live in a stable band where temperature and light are forever the same.&lt;br /&gt;
### Mountain life&lt;br /&gt;
#### Isolated communities → heavy internal consistency, less external pressure to simplify&lt;br /&gt;
#### Thin air → favoring sharp, closed articulation: ejectives, glottalization, voiceless stops&lt;br /&gt;
#### Cultural inwardness → deep philosophies of stasis and permanence&lt;br /&gt;
### Time is measured in generations, epochs, weathering of stone, growth cycles of ultra-slow plants&lt;br /&gt;
&lt;br /&gt;
{{See also|Ɬiʔa/Conworlding}}&lt;br /&gt;
&lt;br /&gt;
== Morphology ==&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Case !! Function !! Gloss !! Ending&lt;br /&gt;
|+ Existential cases&lt;br /&gt;
|-&lt;br /&gt;
! Topical&lt;br /&gt;
| Frames the referent of the utterance ||	“As for…”&lt;br /&gt;
! -mxa&lt;br /&gt;
|-&lt;br /&gt;
! Identity&lt;br /&gt;
| Category, essence, nominal predicate ||	“is a…” / “equals…”&lt;br /&gt;
! -&lt;br /&gt;
|-&lt;br /&gt;
! Possessive&lt;br /&gt;
| ownership, authorship, kinship, part-whole || “X’s Y”&lt;br /&gt;
! -rkI&lt;br /&gt;
|-&lt;br /&gt;
! Partitive &lt;br /&gt;
| part-to-whole, uncertainty, scalarity || &amp;quot;some of, partially&amp;quot;&lt;br /&gt;
! -g(Ö)&lt;br /&gt;
|-&lt;br /&gt;
! Genitive	&lt;br /&gt;
| association, content, theme, objective, attribution || “Y of X”&lt;br /&gt;
! -ł(Ö)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Where/When Cases&lt;br /&gt;
! Case !!	Function !!	Typical gloss !! Ending&lt;br /&gt;
|-&lt;br /&gt;
! Locative&lt;br /&gt;
| Place, state, context of being, time-within ||	“in,” “at,” “on”, &amp;quot;during&amp;quot;&lt;br /&gt;
! -f&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Dative&lt;br /&gt;
| Target, direction ||	“to,” “for,” “until&amp;quot;, &amp;quot;as far as&amp;quot;&lt;br /&gt;
! -n!O&lt;br /&gt;
|-&lt;br /&gt;
! Ablative&lt;br /&gt;
| Source, cause, origin || “from,” “because of,” “due to”&lt;br /&gt;
! -bdI&lt;br /&gt;
|-&lt;br /&gt;
! Benefactive&lt;br /&gt;
| Advantage, interest, concern || “for the benefit of…”, &amp;quot;at the behest of&amp;quot;&lt;br /&gt;
! -aI&lt;br /&gt;
|-&lt;br /&gt;
! Abessive&lt;br /&gt;
| Absence, privation, “lacking”	|| “without,” “lacking,” “free from”, &amp;quot;exclude&amp;quot;&lt;br /&gt;
! -st&#039;Ö&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ How Cases&lt;br /&gt;
! Case !! Function 	!! Typical gloss !! Ending&lt;br /&gt;
|-&lt;br /&gt;
! Instrumental &lt;br /&gt;
| Means, medium, material || “by (means of)”, “through,” “with”, &amp;quot;using&amp;quot;&lt;br /&gt;
! -fla&lt;br /&gt;
|-&lt;br /&gt;
! Adverbial&lt;br /&gt;
| Role/state modifier, part of speech shift	|| “as (a) X,” “in a X way”, &amp;quot;like&amp;quot;&lt;br /&gt;
! -Oad&lt;br /&gt;
|-&lt;br /&gt;
! Translative&lt;br /&gt;
| Change of state, transform/manifestation ||	“becoming,” “into,” “turning into”&lt;br /&gt;
! -k&#039;(I)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Noun Classes&lt;br /&gt;
! !! Not &amp;quot;Container&amp;quot; (mass: paucal, whole) !! &amp;quot;Container&amp;quot; (count: number)&lt;br /&gt;
|-&lt;br /&gt;
! Idea + Matter	&lt;br /&gt;
| Animals (also temperaments) || 	Persons / Gods&lt;br /&gt;
|-&lt;br /&gt;
! Matter only	&lt;br /&gt;
| (Diffuse) Substances: air, fire || 	Tools , &amp;quot;rocks&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
! Idea only	&lt;br /&gt;
| Actions	|| Abstracts, Categories, Sets&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Number: Containers are unmarked for number, as in Chinese/Japanese/Korean.  Non-containers default to a collective/mass-noun number, but can take a paucal (which can mean as few as one).&lt;br /&gt;
&lt;br /&gt;
Polypersonal pronouns:&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! !! 1x !! 1n !! 2 !! 3P !! 3T !! 3R !! 3D !! 3S !! 3A !! 4&lt;br /&gt;
|-&lt;br /&gt;
! 1x !! ø !! ø&lt;br /&gt;
|       tifq ||  tis ||  tił ||  tiwi || tiþ || tið || tiv || tir&lt;br /&gt;
|-&lt;br /&gt;
! 1in !! ø !! ø&lt;br /&gt;
|       tqifq ||  tqis ||  tqił ||  tqiwi || tqiþ || tqið || tqiv || tqir        &lt;br /&gt;
|-&lt;br /&gt;
! 2&lt;br /&gt;
| fqwöt || fqwötq&lt;br /&gt;
! ø&lt;br /&gt;
|                  fqwös || fqwöł || fqwöu || fqwöþ || fqwöð || fqwöv || fqwör &lt;br /&gt;
|-&lt;br /&gt;
! 3P&lt;br /&gt;
| sjet || sjetq || sjefq &lt;br /&gt;
! ø&lt;br /&gt;
|                   sjeł || sjewi || sjeþ || sjeð || sjev || sjer&lt;br /&gt;
|-&lt;br /&gt;
! 3T&lt;br /&gt;
| łot || łotq || łofq || łos&lt;br /&gt;
! ø&lt;br /&gt;
|                        łou || łoþ || łoð || łov || łor&lt;br /&gt;
|-&lt;br /&gt;
! 3R&lt;br /&gt;
| ut || utq || ufq || us || uł&lt;br /&gt;
! ø&lt;br /&gt;
|                           uþ || uð || uv || ur&lt;br /&gt;
|-&lt;br /&gt;
! 3D&lt;br /&gt;
| þwöt || þwötq || þwöfq || þwös || þwöł || þwöu&lt;br /&gt;
! ø&lt;br /&gt;
|                                þwöð || þwöv || þwör&lt;br /&gt;
|-&lt;br /&gt;
! 3S&lt;br /&gt;
| ðet || ðetq || ðefq || ðes || ðeł || ðewi || ðeþ&lt;br /&gt;
! ø&lt;br /&gt;
|                                       ðev || ðer&lt;br /&gt;
|-&lt;br /&gt;
! 3S&lt;br /&gt;
| vöt || vötq || vöfq || vös || vöł || vöu || vöþ || vöð&lt;br /&gt;
! ø&lt;br /&gt;
| vör&lt;br /&gt;
|-&lt;br /&gt;
! 4&lt;br /&gt;
| rut || rutq || rufq || rus || ruł || ruwu || ruþ || ruð || ruv&lt;br /&gt;
! ø&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
== Phonology/Orthography ==&lt;br /&gt;
{| class=&amp;quot;bluetable&amp;quot; style=&amp;quot;text-align:center; float:left&amp;quot;&lt;br /&gt;
! !!	Labial !!	Labiolingual !!	Alveolar !!	Palatal !! Velar !!	Glottal&lt;br /&gt;
|-&lt;br /&gt;
! Nasal	&lt;br /&gt;
| colspan=&amp;quot;3&amp;quot; | /m~n/ &#039;&#039;&#039;M&#039;&#039;&#039; || (/ɲ/ &#039;&#039;&#039;nj&#039;&#039;&#039;) || /ŋ/ &#039;&#039;&#039;M&#039;&#039;&#039;			||&lt;br /&gt;
|-&lt;br /&gt;
! Click&lt;br /&gt;
| colspan=&amp;quot;2&amp;quot; | (/ᵐʘ/ &#039;&#039;&#039;mx&#039;&#039;&#039;) || colspan=&amp;quot;3&amp;quot; | (/ŋǃ/ &#039;&#039;&#039;y&#039;&#039;&#039;) || &lt;br /&gt;
|-&lt;br /&gt;
! Voiced Stop&lt;br /&gt;
| &#039;&#039;&#039;b&#039;&#039;&#039; || 	||	&#039;&#039;&#039;d&#039;&#039;&#039; ||	(/dʑ/ &#039;&#039;&#039;dj&#039;&#039;&#039;) || &#039;&#039;&#039;g&#039;&#039;&#039;	||&lt;br /&gt;
|-&lt;br /&gt;
! Eject. Stop&lt;br /&gt;
| /pʼ/ &#039;&#039;&#039;pq&#039;&#039;&#039; ||	|| /t’/ &#039;&#039;&#039;tq&#039;&#039;&#039;	|| /c&#039;/ &#039;&#039;&#039;cq&#039;&#039;&#039; || /k’/ &#039;&#039;&#039;kq&#039;&#039;&#039; ||	/ʔ/ &#039;&#039;&#039; &#039; &#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Unvoiced Stop&lt;br /&gt;
| &#039;&#039;&#039;p&#039;&#039;&#039; ||	||	&#039;&#039;&#039;t&#039;&#039;&#039; || (/tɕ/ &#039;&#039;&#039;tj&#039;&#039;&#039;) || /k~x/ &#039;&#039;&#039;k&#039;&#039;&#039;	||&lt;br /&gt;
|-&lt;br /&gt;
! Voiced Fricative&lt;br /&gt;
| /β~v/ &#039;&#039;&#039;v&#039;&#039;&#039; || /ð̼/ &#039;&#039;&#039;ð&#039;&#039;&#039; || &#039;&#039;&#039;z&#039;&#039;&#039; || (/ʒ/ &#039;&#039;&#039;zj&#039;&#039;&#039;) || ||&lt;br /&gt;
|-&lt;br /&gt;
! Unvoiced Fricative&lt;br /&gt;
| /ɸ~f/ &#039;&#039;&#039;f&#039;&#039;&#039; ||	/θ̼/ &#039;&#039;&#039;þ&#039;&#039;&#039;	|| &#039;&#039;&#039;s&#039;&#039;&#039; || (/ʃ/ &#039;&#039;&#039;sj&#039;&#039;&#039;) || ||&lt;br /&gt;
|-&lt;br /&gt;
! Eject. Fricative&lt;br /&gt;
| /fʼ/ &#039;&#039;&#039;fq&#039;&#039;&#039; ||	/θ̼ʼ/ &#039;&#039;&#039;þq&#039;&#039;&#039; || /s’~ts’/ &#039;&#039;&#039;sq&#039;&#039;&#039;		|| || ||&lt;br /&gt;
|-&lt;br /&gt;
! Approx./Trill	&lt;br /&gt;
| &#039;&#039;&#039;w&#039;&#039;&#039;	|| || &#039;&#039;&#039;r&#039;&#039;&#039; || &#039;&#039;&#039;j&#039;&#039;&#039; ||	|| /h~ɦ/ &#039;&#039;&#039;h&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Laterals&lt;br /&gt;
| || /l̼/ &#039;&#039;&#039;l&#039;&#039;&#039; ||	/ɬ/ &#039;&#039;&#039;ł&#039;&#039;&#039;		|| (/ʎ/ &#039;&#039;&#039;lj&#039;&#039;&#039;) || ||&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;bluetable&amp;quot; style=&amp;quot;float:right; text-align:center;&amp;quot;&lt;br /&gt;
! !! Front !! Back !! Underspecified&lt;br /&gt;
|-&lt;br /&gt;
! High&lt;br /&gt;
| &#039;&#039;&#039;i&#039;&#039;&#039; || &#039;&#039;&#039;u&#039;&#039;&#039; || I&lt;br /&gt;
|-&lt;br /&gt;
! High-Mid&lt;br /&gt;
| &#039;&#039;&#039;e&#039;&#039;&#039; || &#039;&#039;&#039;o&#039;&#039;&#039; || O&lt;br /&gt;
|-&lt;br /&gt;
! Low-Mid&lt;br /&gt;
| /ɛ/ &#039;&#039;&#039;ë&#039;&#039;&#039; || /ɔ/ &#039;&#039;&#039;ö&#039;&#039;&#039; || Ö&lt;br /&gt;
|-&lt;br /&gt;
! Low&lt;br /&gt;
| colspan=&amp;quot;2&amp;quot; | /ä/ &#039;&#039;&#039;a&#039;&#039;&#039;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Allophony:&lt;br /&gt;
* nasal + labial ejective -&amp;gt; [m͡ʘ]&lt;br /&gt;
* nasal + non-labial ejective -&amp;gt; [ŋ͡ǃ]&lt;br /&gt;
&lt;br /&gt;
Phonotactics are (C)(G)V(C&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;):&lt;br /&gt;
* any consonant or none can a syllable&lt;br /&gt;
* Glides (/j/ or /w/) after anything, if after nothing, insert glottal stop&lt;br /&gt;
* hiatus allowed, diphthongs not&lt;br /&gt;
* any coda, except glides&lt;br /&gt;
&lt;br /&gt;
=== Sentences ===&lt;br /&gt;
# The storm scared the people.&lt;br /&gt;
#* vökqöthumxa &#039;usëk venargofq&lt;br /&gt;
#* As for the storm, (there is) fear in the people.&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a&amp;diff=168304</id>
		<title>Ɬiʔa</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a&amp;diff=168304"/>
		<updated>2025-03-29T23:44:54Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* Phonology/Orthography */ moar consonants!&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Goals ==&lt;br /&gt;
# Endgoal - A truly verbless language I can use&lt;br /&gt;
# Vague phrases&lt;br /&gt;
## Glacial pace&lt;br /&gt;
## Navajo-of-nouns&lt;br /&gt;
## lazy but clever&lt;br /&gt;
## carved in stone&lt;br /&gt;
## complicated rituals&lt;br /&gt;
# Naturalism - 6/10&lt;br /&gt;
#* I want some naturalistic elements&lt;br /&gt;
#* Different setting (parallel Earth)&lt;br /&gt;
#* Different nature (immortal humans)&lt;br /&gt;
#* Irregularities but not many&lt;br /&gt;
#* Idioms within reason&lt;br /&gt;
# Complexity - insane.  Navajo but with only nouns&lt;br /&gt;
# Derivation - clear.  Agglutinative, basically&lt;br /&gt;
# Features&lt;br /&gt;
## Phonology &lt;br /&gt;
### Vowel harmony&lt;br /&gt;
### A couple of clicks, and ejectives (un-earth-like)&lt;br /&gt;
### CV, and CVC &lt;br /&gt;
## Grammar&lt;br /&gt;
### No verbs at all&lt;br /&gt;
### assumed copular between topic and subject&lt;br /&gt;
### 6 nouns classes (genders), like animacy &lt;br /&gt;
### Many cases (12?)&lt;br /&gt;
### Case-stacking&lt;br /&gt;
### word glue, like German&lt;br /&gt;
### mostly agglutinative, touch of fusional&lt;br /&gt;
## Culture&lt;br /&gt;
### things happen, not because someone does them, but because the world unfolds in prescribed patterns&lt;br /&gt;
### discourse is formulaic, ceremonial, or sacred: more on set relational expressions and fixed semantic roles, rather than on active description of novel events&lt;br /&gt;
### agency is less linguistically salient, so predicates assigning blame, initiative, or creativity are avoided&lt;br /&gt;
### Tidally Locked Planet&lt;br /&gt;
#### The sun never moves in the sky.&lt;br /&gt;
#### The world is divided into zones of permanent day, eternal night, and a narrow habitable twilight ring.&lt;br /&gt;
#### People live in a stable band where temperature and light are forever the same.&lt;br /&gt;
### Mountain life&lt;br /&gt;
#### Isolated communities → heavy internal consistency, less external pressure to simplify&lt;br /&gt;
#### Thin air → favoring sharp, closed articulation: ejectives, glottalization, voiceless stops&lt;br /&gt;
#### Cultural inwardness → deep philosophies of stasis and permanence&lt;br /&gt;
### Time is measured in generations, epochs, weathering of stone, growth cycles of ultra-slow plants&lt;br /&gt;
&lt;br /&gt;
{{See also|Ɬiʔa/Conworlding}}&lt;br /&gt;
&lt;br /&gt;
== Morphology ==&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Case !! Function !! Gloss !! Ending&lt;br /&gt;
|+ Existential cases&lt;br /&gt;
|-&lt;br /&gt;
! Topical&lt;br /&gt;
| Frames the referent of the utterance ||	“As for…”&lt;br /&gt;
! -Mp&#039;a&lt;br /&gt;
|-&lt;br /&gt;
! Identity&lt;br /&gt;
| Category, essence, nominal predicate ||	“is a…” / “equals…”&lt;br /&gt;
! -&lt;br /&gt;
|-&lt;br /&gt;
! Possessive&lt;br /&gt;
| ownership, authorship, kinship, part-whole || “X’s Y”&lt;br /&gt;
! -rkI&lt;br /&gt;
|-&lt;br /&gt;
! Partitive &lt;br /&gt;
| part-to-whole, uncertainty, scalarity || &amp;quot;some of, partially&amp;quot;&lt;br /&gt;
! -g(Ö)&lt;br /&gt;
|-&lt;br /&gt;
! Genitive	&lt;br /&gt;
| association, content, theme, objective, attribution || “Y of X”&lt;br /&gt;
! -ł(Ö)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Where/When Cases&lt;br /&gt;
! Case !!	Function !!	Typical gloss !! Ending&lt;br /&gt;
|-&lt;br /&gt;
! Locative&lt;br /&gt;
| Place, state, context of being, time-within ||	“in,” “at,” “on”, &amp;quot;during&amp;quot;&lt;br /&gt;
! -f&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Dative&lt;br /&gt;
| Target, direction ||	“to,” “for,” “until&amp;quot;, &amp;quot;as far as&amp;quot;&lt;br /&gt;
! -Mk&#039;O&lt;br /&gt;
|-&lt;br /&gt;
! Ablative&lt;br /&gt;
| Source, cause, origin || “from,” “because of,” “due to”&lt;br /&gt;
! -bdI&lt;br /&gt;
|-&lt;br /&gt;
! Benefactive&lt;br /&gt;
| Advantage, interest, concern || “for the benefit of…”, &amp;quot;at the behest of&amp;quot;&lt;br /&gt;
! -aI&lt;br /&gt;
|-&lt;br /&gt;
! Abessive&lt;br /&gt;
| Absence, privation, “lacking”	|| “without,” “lacking,” “free from”, &amp;quot;exclude&amp;quot;&lt;br /&gt;
! -st&#039;Ö&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ How Cases&lt;br /&gt;
! Case !! Function 	!! Typical gloss !! Ending&lt;br /&gt;
|-&lt;br /&gt;
! Instrumental &lt;br /&gt;
| Means, medium, material || “by (means of)”, “through,” “with”, &amp;quot;using&amp;quot;&lt;br /&gt;
! -fla&lt;br /&gt;
|-&lt;br /&gt;
! Adverbial&lt;br /&gt;
| Role/state modifier, part of speech shift	|| “as (a) X,” “in a X way”, &amp;quot;like&amp;quot;&lt;br /&gt;
! -Oad&lt;br /&gt;
|-&lt;br /&gt;
! Translative&lt;br /&gt;
| Change of state, transform/manifestation ||	“becoming,” “into,” “turning into”&lt;br /&gt;
! -k&#039;(I)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Noun Classes&lt;br /&gt;
! !! Not &amp;quot;Container&amp;quot; (mass: paucal, whole) !! &amp;quot;Container&amp;quot; (count: number)&lt;br /&gt;
|-&lt;br /&gt;
! Idea + Matter	&lt;br /&gt;
| Animals (also temperaments) || 	Persons / Gods&lt;br /&gt;
|-&lt;br /&gt;
! Matter only	&lt;br /&gt;
| (Diffuse) Substances: air, fire || 	Tools , &amp;quot;rocks&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
! Idea only	&lt;br /&gt;
| Actions	|| Abstracts, Categories, Sets&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Number: Containers are unmarked for number, as in Chinese/Japanese/Korean.  Non-containers default to a collective/mass-noun number, but can take a paucal (which can mean as few as one).&lt;br /&gt;
&lt;br /&gt;
Polypersonal pronouns:&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! !! 1x !! 1n !! 2 !! 3P !! 3T !! 3R !! 3D !! 3S !! 3A !! 4&lt;br /&gt;
|-&lt;br /&gt;
! 1x !! ø&lt;br /&gt;
|-&lt;br /&gt;
! 1in&lt;br /&gt;
|&lt;br /&gt;
! ø&lt;br /&gt;
|-&lt;br /&gt;
! 2&lt;br /&gt;
| ||&lt;br /&gt;
! ø&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
== Phonology/Orthography ==&lt;br /&gt;
{| class=&amp;quot;bluetable&amp;quot; style=&amp;quot;text-align:center; float:left&amp;quot;&lt;br /&gt;
! !!	Labial !!	Labiolingual !!	Alveolar !!	Palatal !! Velar !!	Glottal&lt;br /&gt;
|-&lt;br /&gt;
! Nasal	&lt;br /&gt;
| colspan=&amp;quot;3&amp;quot; | /m~n/ &#039;&#039;&#039;M&#039;&#039;&#039; || (/ɲ/ &#039;&#039;&#039;nj&#039;&#039;&#039;) || /ŋ/ &#039;&#039;&#039;M&#039;&#039;&#039;			||&lt;br /&gt;
|-&lt;br /&gt;
! Click&lt;br /&gt;
| colspan=&amp;quot;2&amp;quot; | (/ᵐʘ/ &#039;&#039;&#039;mx&#039;&#039;&#039;) || colspan=&amp;quot;3&amp;quot; | (/ŋǃ/ &#039;&#039;&#039;y&#039;&#039;&#039;) || &lt;br /&gt;
|-&lt;br /&gt;
! Voiced Stop&lt;br /&gt;
| &#039;&#039;&#039;b&#039;&#039;&#039; || 	||	&#039;&#039;&#039;d&#039;&#039;&#039; ||	(/dʑ/ &#039;&#039;&#039;dj&#039;&#039;&#039;) || &#039;&#039;&#039;g&#039;&#039;&#039;	||&lt;br /&gt;
|-&lt;br /&gt;
! Eject. Stop&lt;br /&gt;
| /pʼ/ &#039;&#039;&#039;pq&#039;&#039;&#039; ||	|| /t’/ &#039;&#039;&#039;tq&#039;&#039;&#039;	|| /c&#039;/ &#039;&#039;&#039;cq&#039;&#039;&#039; || /k’/ &#039;&#039;&#039;kq&#039;&#039;&#039; ||	/ʔ/ &#039;&#039;&#039; &#039; &#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Unvoiced Stop&lt;br /&gt;
| &#039;&#039;&#039;p&#039;&#039;&#039; ||	||	&#039;&#039;&#039;t&#039;&#039;&#039; || (/tɕ/ &#039;&#039;&#039;tj&#039;&#039;&#039;) || /k~x/ &#039;&#039;&#039;k&#039;&#039;&#039;	||&lt;br /&gt;
|-&lt;br /&gt;
! Voiced Fricative&lt;br /&gt;
| /β~v/ &#039;&#039;&#039;v&#039;&#039;&#039; || /ð̼/ &#039;&#039;&#039;ð&#039;&#039;&#039; || &#039;&#039;&#039;z&#039;&#039;&#039; || (/ʒ/ &#039;&#039;&#039;zj&#039;&#039;&#039;) || ||&lt;br /&gt;
|-&lt;br /&gt;
! Unvoiced Fricative&lt;br /&gt;
| /ɸ~f/ &#039;&#039;&#039;f&#039;&#039;&#039; ||	/θ̼/ &#039;&#039;&#039;þ&#039;&#039;&#039;	|| &#039;&#039;&#039;s&#039;&#039;&#039; || (/ʃ/ &#039;&#039;&#039;sj&#039;&#039;&#039;) || ||&lt;br /&gt;
|-&lt;br /&gt;
! Eject. Fricative&lt;br /&gt;
| /fʼ/ &#039;&#039;&#039;fq&#039;&#039;&#039; ||	/θ̼ʼ/ &#039;&#039;&#039;þq&#039;&#039;&#039; || /s’~ts’/ &#039;&#039;&#039;sq&#039;&#039;&#039;		|| || ||&lt;br /&gt;
|-&lt;br /&gt;
! Approx./Trill	&lt;br /&gt;
| &#039;&#039;&#039;w&#039;&#039;&#039;	|| || &#039;&#039;&#039;r&#039;&#039;&#039; || &#039;&#039;&#039;j&#039;&#039;&#039; ||	|| /h~ɦ/ &#039;&#039;&#039;h&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Laterals&lt;br /&gt;
| || /l̼/ &#039;&#039;&#039;l&#039;&#039;&#039; ||	/ɬ/ &#039;&#039;&#039;ł&#039;&#039;&#039;		|| (/ʎ/ &#039;&#039;&#039;lj&#039;&#039;&#039;) || ||&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;bluetable&amp;quot; style=&amp;quot;float:right; text-align:center;&amp;quot;&lt;br /&gt;
! !! Front !! Back !! Underspecified&lt;br /&gt;
|-&lt;br /&gt;
! High&lt;br /&gt;
| &#039;&#039;&#039;i&#039;&#039;&#039; || &#039;&#039;&#039;u&#039;&#039;&#039; || I&lt;br /&gt;
|-&lt;br /&gt;
! High-Mid&lt;br /&gt;
| &#039;&#039;&#039;e&#039;&#039;&#039; || &#039;&#039;&#039;o&#039;&#039;&#039; || O&lt;br /&gt;
|-&lt;br /&gt;
! Low-Mid&lt;br /&gt;
| /ɛ/ &#039;&#039;&#039;ë&#039;&#039;&#039; || /ɔ/ &#039;&#039;&#039;ö&#039;&#039;&#039; || Ö&lt;br /&gt;
|-&lt;br /&gt;
! Low&lt;br /&gt;
| colspan=&amp;quot;2&amp;quot; | /ä/ &#039;&#039;&#039;a&#039;&#039;&#039;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Allophony:&lt;br /&gt;
* nasal + labial ejective -&amp;gt; [m͡ʘ]&lt;br /&gt;
* nasal + non-labial ejective -&amp;gt; [ŋ͡ǃ]&lt;br /&gt;
&lt;br /&gt;
Phonotactics are (C)(G)V(C&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;):&lt;br /&gt;
* any consonant or none can a syllable&lt;br /&gt;
* Glides (/j/ or /w/) after anything, if after nothing, insert glottal stop&lt;br /&gt;
* hiatus allowed, diphthongs not&lt;br /&gt;
* any coda, except glides&lt;br /&gt;
&lt;br /&gt;
=== Sentences ===&lt;br /&gt;
# The storm scared the people.&lt;br /&gt;
#* vökqöthumxa &#039;usëk venargofq&lt;br /&gt;
#* As for the storm, (there is) fear in the people.&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a&amp;diff=168286</id>
		<title>Ɬiʔa</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a&amp;diff=168286"/>
		<updated>2025-03-29T19:42:11Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* Morphology */ adding another case&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Goals ==&lt;br /&gt;
# Endgoal - A truly verbless language I can use&lt;br /&gt;
# Vague phrases&lt;br /&gt;
## Glacial pace&lt;br /&gt;
## Navajo-of-nouns&lt;br /&gt;
## lazy but clever&lt;br /&gt;
## carved in stone&lt;br /&gt;
## complicated rituals&lt;br /&gt;
# Naturalism - 6/10&lt;br /&gt;
#* I want some naturalistic elements&lt;br /&gt;
#* Different setting (parallel Earth)&lt;br /&gt;
#* Different nature (immortal humans)&lt;br /&gt;
#* Irregularities but not many&lt;br /&gt;
#* Idioms within reason&lt;br /&gt;
# Complexity - insane.  Navajo but with only nouns&lt;br /&gt;
# Derivation - clear.  Agglutinative, basically&lt;br /&gt;
# Features&lt;br /&gt;
## Phonology &lt;br /&gt;
### Vowel harmony&lt;br /&gt;
### A couple of clicks, and ejectives (un-earth-like)&lt;br /&gt;
### CV, and CVC &lt;br /&gt;
## Grammar&lt;br /&gt;
### No verbs at all&lt;br /&gt;
### assumed copular between topic and subject&lt;br /&gt;
### 6 nouns classes (genders), like animacy &lt;br /&gt;
### Many cases (12?)&lt;br /&gt;
### Case-stacking&lt;br /&gt;
### word glue, like German&lt;br /&gt;
### mostly agglutinative, touch of fusional&lt;br /&gt;
## Culture&lt;br /&gt;
### things happen, not because someone does them, but because the world unfolds in prescribed patterns&lt;br /&gt;
### discourse is formulaic, ceremonial, or sacred: more on set relational expressions and fixed semantic roles, rather than on active description of novel events&lt;br /&gt;
### agency is less linguistically salient, so predicates assigning blame, initiative, or creativity are avoided&lt;br /&gt;
### Tidally Locked Planet&lt;br /&gt;
#### The sun never moves in the sky.&lt;br /&gt;
#### The world is divided into zones of permanent day, eternal night, and a narrow habitable twilight ring.&lt;br /&gt;
#### People live in a stable band where temperature and light are forever the same.&lt;br /&gt;
### Mountain life&lt;br /&gt;
#### Isolated communities → heavy internal consistency, less external pressure to simplify&lt;br /&gt;
#### Thin air → favoring sharp, closed articulation: ejectives, glottalization, voiceless stops&lt;br /&gt;
#### Cultural inwardness → deep philosophies of stasis and permanence&lt;br /&gt;
### Time is measured in generations, epochs, weathering of stone, growth cycles of ultra-slow plants&lt;br /&gt;
&lt;br /&gt;
{{See also|Ɬiʔa/Conworlding}}&lt;br /&gt;
&lt;br /&gt;
== Morphology ==&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Case !! Function !! Gloss !! Ending&lt;br /&gt;
|+ Existential cases&lt;br /&gt;
|-&lt;br /&gt;
! Topical&lt;br /&gt;
| Frames the referent of the utterance ||	“As for…”&lt;br /&gt;
! -Mp&#039;a&lt;br /&gt;
|-&lt;br /&gt;
! Identity&lt;br /&gt;
| Category, essence, nominal predicate ||	“is a…” / “equals…”&lt;br /&gt;
! -&lt;br /&gt;
|-&lt;br /&gt;
! Possessive&lt;br /&gt;
| ownership, authorship, kinship, part-whole || “X’s Y”&lt;br /&gt;
! -rkI&lt;br /&gt;
|-&lt;br /&gt;
! Partitive &lt;br /&gt;
| part-to-whole, uncertainty, scalarity || &amp;quot;some of, partially&amp;quot;&lt;br /&gt;
! -g(Ö)&lt;br /&gt;
|-&lt;br /&gt;
! Genitive	&lt;br /&gt;
| association, content, theme, objective, attribution || “Y of X”&lt;br /&gt;
! -ł(Ö)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Where/When Cases&lt;br /&gt;
! Case !!	Function !!	Typical gloss !! Ending&lt;br /&gt;
|-&lt;br /&gt;
! Locative&lt;br /&gt;
| Place, state, context of being, time-within ||	“in,” “at,” “on”, &amp;quot;during&amp;quot;&lt;br /&gt;
! -f&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Dative&lt;br /&gt;
| Target, direction ||	“to,” “for,” “until&amp;quot;, &amp;quot;as far as&amp;quot;&lt;br /&gt;
! -Mk&#039;O&lt;br /&gt;
|-&lt;br /&gt;
! Ablative&lt;br /&gt;
| Source, cause, origin || “from,” “because of,” “due to”&lt;br /&gt;
! -bdI&lt;br /&gt;
|-&lt;br /&gt;
! Benefactive&lt;br /&gt;
| Advantage, interest, concern || “for the benefit of…”, &amp;quot;at the behest of&amp;quot;&lt;br /&gt;
! -aI&lt;br /&gt;
|-&lt;br /&gt;
! Abessive&lt;br /&gt;
| Absence, privation, “lacking”	|| “without,” “lacking,” “free from”, &amp;quot;exclude&amp;quot;&lt;br /&gt;
! -st&#039;Ö&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ How Cases&lt;br /&gt;
! Case !! Function 	!! Typical gloss !! Ending&lt;br /&gt;
|-&lt;br /&gt;
! Instrumental &lt;br /&gt;
| Means, medium, material || “by (means of)”, “through,” “with”, &amp;quot;using&amp;quot;&lt;br /&gt;
! -fla&lt;br /&gt;
|-&lt;br /&gt;
! Adverbial&lt;br /&gt;
| Role/state modifier, part of speech shift	|| “as (a) X,” “in a X way”, &amp;quot;like&amp;quot;&lt;br /&gt;
! -Oad&lt;br /&gt;
|-&lt;br /&gt;
! Translative&lt;br /&gt;
| Change of state, transform/manifestation ||	“becoming,” “into,” “turning into”&lt;br /&gt;
! -k&#039;(I)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Noun Classes&lt;br /&gt;
! !! Not &amp;quot;Container&amp;quot; (mass: paucal, whole) !! &amp;quot;Container&amp;quot; (count: number)&lt;br /&gt;
|-&lt;br /&gt;
! Idea + Matter	&lt;br /&gt;
| Animals (also temperaments) || 	Persons / Gods&lt;br /&gt;
|-&lt;br /&gt;
! Matter only	&lt;br /&gt;
| (Diffuse) Substances: air, fire || 	Tools , &amp;quot;rocks&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
! Idea only	&lt;br /&gt;
| Actions	|| Abstracts, Categories, Sets&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Number: Containers are unmarked for number, as in Chinese/Japanese/Korean.  Non-containers default to a collective/mass-noun number, but can take a paucal (which can mean as few as one).&lt;br /&gt;
&lt;br /&gt;
Polypersonal pronouns:&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! !! 1x !! 1n !! 2 !! 3P !! 3T !! 3R !! 3D !! 3S !! 3A !! 4&lt;br /&gt;
|-&lt;br /&gt;
! 1x !! ø&lt;br /&gt;
|-&lt;br /&gt;
! 1in&lt;br /&gt;
|&lt;br /&gt;
! ø&lt;br /&gt;
|-&lt;br /&gt;
! 2&lt;br /&gt;
| ||&lt;br /&gt;
! ø&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
== Phonology/Orthography ==&lt;br /&gt;
{| class=&amp;quot;bluetable&amp;quot; style=&amp;quot;text-align:center; float:left&amp;quot;&lt;br /&gt;
! !!	Labial !!	Labiolingual !!	Alveolar !!	Palatal !! Velar !!	Glottal&lt;br /&gt;
|-&lt;br /&gt;
! Nasal	&lt;br /&gt;
| /m/	&#039;&#039;&#039;m&#039;&#039;&#039; || /n̼/ &#039;&#039;&#039;n&#039;&#039;&#039; || /n/ &#039;&#039;&#039;n&#039;&#039;&#039; || /ŋ/ &#039;&#039;&#039;ŋ&#039;&#039;&#039;			||&lt;br /&gt;
|-&lt;br /&gt;
! Click&lt;br /&gt;
| (/ᵐʘ/ &#039;&#039;&#039;mx&#039;&#039;&#039;) || || (/ŋǃ/ &#039;&#039;&#039;nc&#039;&#039;&#039;) || ||&lt;br /&gt;
|-&lt;br /&gt;
! Voiced Stop&lt;br /&gt;
| &#039;&#039;&#039;b&#039;&#039;&#039; || 	||	&#039;&#039;&#039;d&#039;&#039;&#039; ||	&#039;&#039;&#039;g&#039;&#039;&#039;	||&lt;br /&gt;
|-&lt;br /&gt;
! Eject. Stop&lt;br /&gt;
| /pʼ/ &#039;&#039;&#039;pq&#039;&#039;&#039; ||	|| /t’/ &#039;&#039;&#039;tq&#039;&#039;&#039;	|| /k’/ &#039;&#039;&#039;kq&#039;&#039;&#039; ||	/ʔ/ &#039;&#039;&#039; &#039; &#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Unvoiced Stop&lt;br /&gt;
| &#039;&#039;&#039;p&#039;&#039;&#039; ||	||	&#039;&#039;&#039;t&#039;&#039;&#039; || /k~x/ &#039;&#039;&#039;k&#039;&#039;&#039;	||&lt;br /&gt;
|-&lt;br /&gt;
! Plain Fricative&lt;br /&gt;
| /ɸ~β/ &#039;&#039;&#039;f&#039;&#039;&#039; ||	/θ̼~ð̼/ &#039;&#039;&#039;þ&#039;&#039;&#039;	|| /s~z/ &#039;&#039;&#039;s&#039;&#039;&#039; || (/ʒ/ &#039;&#039;&#039;ž&#039;&#039;&#039;) || ||&lt;br /&gt;
|-&lt;br /&gt;
! Eject. Fricative&lt;br /&gt;
| /fʼ/ &#039;&#039;&#039;fq&#039;&#039;&#039; ||	/θ̼ʼ/ &#039;&#039;&#039;þq&#039;&#039;&#039; || /s’~ts’/ &#039;&#039;&#039;sq&#039;&#039;&#039;		|| ||&lt;br /&gt;
|-&lt;br /&gt;
! Approx./Trill	&lt;br /&gt;
| &#039;&#039;&#039;w&#039;&#039;&#039;	|| || &#039;&#039;&#039;r&#039;&#039;&#039; || &#039;&#039;&#039;j&#039;&#039;&#039; ||	/h~ɦ/ &#039;&#039;&#039;h&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Laterals&lt;br /&gt;
| || /l̼/ &#039;&#039;&#039;l&#039;&#039;&#039; ||	/ɬ/ &#039;&#039;&#039;ł&#039;&#039;&#039;		|| ||&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;bluetable&amp;quot; style=&amp;quot;float:right; text-align:center;&amp;quot;&lt;br /&gt;
! !! Front !! Back !! Underspecified&lt;br /&gt;
|-&lt;br /&gt;
! High&lt;br /&gt;
| &#039;&#039;&#039;i&#039;&#039;&#039; || &#039;&#039;&#039;u&#039;&#039;&#039; || I&lt;br /&gt;
|-&lt;br /&gt;
! High-Mid&lt;br /&gt;
| &#039;&#039;&#039;e&#039;&#039;&#039; || &#039;&#039;&#039;o&#039;&#039;&#039; || O&lt;br /&gt;
|-&lt;br /&gt;
! Low-Mid&lt;br /&gt;
| /ɛ/ &#039;&#039;&#039;ë&#039;&#039;&#039; || /ɔ/ &#039;&#039;&#039;ö&#039;&#039;&#039; || Ö&lt;br /&gt;
|-&lt;br /&gt;
! Low&lt;br /&gt;
| colspan=&amp;quot;2&amp;quot; | /ä/ &#039;&#039;&#039;a&#039;&#039;&#039;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Allophony:&lt;br /&gt;
* nasal + labial ejective -&amp;gt; [m͡ʘ]&lt;br /&gt;
* nasal + non-labial ejective -&amp;gt; [ŋ͡ǃ]&lt;br /&gt;
&lt;br /&gt;
Phonotactics are (C)(G)V(C&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;):&lt;br /&gt;
* any consonant or none can a syllable&lt;br /&gt;
* Glides (/j/ or /w/) after anything&lt;br /&gt;
* hiatus allowed, diphthongs not&lt;br /&gt;
* any coda, except glides&lt;br /&gt;
&lt;br /&gt;
=== Sentences ===&lt;br /&gt;
# The storm scared people&lt;br /&gt;
#* k’ɛthu-Mp’a ʔusɛk närgo-f’&lt;br /&gt;
#* kqëthumxa ’usëk närgofq&lt;br /&gt;
#* As for the storm, (there is) fear in people.&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168214</id>
		<title>Ɬiʔa/Conworlding</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168214"/>
		<updated>2025-03-28T19:04:59Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* Star */ more facts&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Star ==&lt;br /&gt;
The star is a red-dwarf (M5V) named Gliese 710b minoris, or informally &#039;&#039;Mirar&#039;s Veil&#039;&#039;.  It is 7.9 light-years (≈2.42 parsecs) from Sol, toward the galactic plane, in Scorpius–Ophiuchus.  It lies just &amp;quot;behind&amp;quot; a brighter, well-known K-dwarf, and was not observed until after humanity&#039;s trip to Proxima Centauri: in situ gravitational navigation by the first robotic probe en route to Proxima Centauri. The probe’s optical gyros noticed an unmodeled gravitational perturbation.&lt;br /&gt;
&lt;br /&gt;
* Stellar luminosity (L*) ≈ 0.01 𝐿⊙ (1/100th Sol&#039;s brightness)&lt;br /&gt;
* Stellar mass (M*) ≈ 0.2 𝑀⊙ (1/5 the mass of Sol)&lt;br /&gt;
* Stellar radius (R*) ≈ 0.25 𝑅⊙ (1/4 as wide as Sol)&lt;br /&gt;
* Effective temperature (T*) ≈ 3500 K&lt;br /&gt;
* Average surface field is ~1.5 kG, with frequent bursts of &amp;gt; 3kG&lt;br /&gt;
** Frequent, energetic flares, multiple per day, with for extreme variability over time, often above 10&amp;lt;sup&amp;gt;35&amp;lt;/sup&amp;gt; erg&lt;br /&gt;
* The frostline is at 0.27 AU&lt;br /&gt;
&lt;br /&gt;
​The habitable zone (a) is about square root of L* over L⊙, so ~0.1 AU.&lt;br /&gt;
&lt;br /&gt;
=== Solar System ===&lt;br /&gt;
There are seven planets in the system&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Planet !!	Mass (M🜨)!!	Radius (R🜨)!! Moons/Rings	!!Resonance !!	&amp;lt;small&amp;gt;Semi-Major&amp;lt;/small&amp;gt; !!	Rings !! Moons !! Period !! Size !! Type&lt;br /&gt;
|-&lt;br /&gt;
| b ||	2.17 ||	1.1 ||	No ||	2:3 with c	|| 0.0763 ||	No || No || 17.2 || 13.6&#039; to 1.5&#039; || Super-Mercury&lt;br /&gt;
|-&lt;br /&gt;
| c ||	1.5	 ||1.225 ||	1* ||	—	        || 0.100 || No || No || 25.8 || - || Super-Earth&lt;br /&gt;
|-&lt;br /&gt;
| d ||	2.0	 ||1.4 ||No ||	2:3 with c	 ||0.131 ||	No || No || 38.7 || 13.1&#039; to 1.8&#039; || Super Waterworld&lt;br /&gt;
|-&lt;br /&gt;
| e ||	0.9 ||	1.0 || No	 ||	2:3 with d	 ||0.172 ||	No || No || 58 || 4.1&#039; to 1.1&#039; || Earth&lt;br /&gt;
|- &lt;br /&gt;
| f ||	3.5 ||	2.0 ||	Yes! ||	2:3 with e	 ||0.227 || Yes || Junk || 87 || 4.6&#039; to 1.8&#039; || Mini-Neptune&lt;br /&gt;
|-&lt;br /&gt;
| g ||	2.6 ||	1.7 ||	2 ||	-	 ||0.40 ||	Yes || Junk || 206 || 1.6&#039; to 1.0&#039; || Stripped Neptune &lt;br /&gt;
|-&lt;br /&gt;
| h ||	5.0x2 ||2.3x2 || yes	 || -	 ||1.5 ||	Yes || No || 1500 || 0.5&#039; 16.4&#039; apart (at max) || Double Neptune&lt;br /&gt;
|}&lt;br /&gt;
==== b: super Mercury with a ring of fire  ====&lt;br /&gt;
[[File:planet b by GPT.png|thumb|right|An artistic rendering of planet b]]&lt;br /&gt;
b is a super-Mercury, tidally locked, and incredibly dense.  ~700ºK on the day side, ~50ºK on the night.  2.1 Earth Masses, 1.1 Earth radii (~7000km) in size.  Orbital period 17.2 days.  Density 9.0 g/cm&amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt;.  Gravity is ~1.8g.  &lt;br /&gt;
&lt;br /&gt;
The iron core is huge, being 75% of the mass.  A thin silicate mantle, with metallic plains and exhumed ultramafic crust, with frequent iron meteorite craters, lacking typical “stone” breccias.&lt;br /&gt;
&lt;br /&gt;
The night side is intense, as simple hydrocarbons (methane, ethane, propane) condense and freeze into layered deposits.  Complex organics (tholins, polycyclic aromatics) accumulate on the sea floor, under miles of nitrogen ice.  Massive slush layers slosh around above cryovolcanic brines of ammonia.&lt;br /&gt;
&lt;br /&gt;
There is a crucial layer of Superionic Ice XI above the core, which acts as an electromagnetic insulator, and ionic heat bridge.  The crust is ultramafic silicates (olivine, pyroxene, perovskite) riddled with with sulfide veins, iron alloys, and graphite networks.  The poles of the magnetosphere are sideways, like Uranus, with poles at the equator in the Terminator Zone.  Persistent surface charges develop, because the whole planet is basically a ginormous Leyden jar!&lt;br /&gt;
&lt;br /&gt;
A planetary flux rope forms and un-forms with the star and planet b.  This induces electric jets at the terminator.  This is where temps are Earth-like.  Hydrocarbons sublimate and eject into the atmosphere, even while aurorae come right down to the ground.  A small, low pressure atmosphere prevents photodissociation, even while electrothermal instabilities lift molecules, forming an anomalous haze, a standing, glowing ring.  Coronal events cause localized lightning geysers with magnetic arcing.&lt;br /&gt;
&lt;br /&gt;
In short, b is visible with a blinding bright sun side (glowing orange bronze), a utterly black night side, and a burning, glowing, erupting, arcing ring at the terminator (all colors).  At biggest, it&#039;s half the size of Earth&#039;s moon in the sky, shrinking down to a star at it&#039;s furthest away.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== d: the wet eye with depths ====&lt;br /&gt;
[[File:wet eye planet.png|thumb|right|An reasonable approximation of d&#039;s appearance]]&lt;br /&gt;
From the outside, d is a &amp;quot;wet eye&amp;quot; just outside the habitable zone.  It is a water world, twice the mass of Earth, 1.4 times the radius, tidally locked.  The substellar point is the only place without surface ice.  However, it is better to think of the planet top-to-bottom.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;atmosphere&#039;&#039;&#039; is tenuous, less than 0.2 bars.  It is thin, N₂-rich with traces of H₂O, NH₃ vapor, and transient geyser outputs.  It is highly UV-irradiated, and Mars-like in its inability to retain volatiles.&lt;br /&gt;
&lt;br /&gt;
Next, there is a &#039;&#039;&#039;surface ice shell&#039;&#039;&#039;, ~20 km of thick Ice I.  Swirling currents beneath have cracked continent-sized ice plates, similar to Europa&#039;s crust.  It is permanently frozen except at the substellar furnace.  It accumulates chemical stains, mineral deposits, and cryovolcanic eruption plumes.  Accumulations of complex hydrates—like methanol clathrates—precipitate out and form false reefs, rising like coral from beneath. Transient thermal vents push hot plumes into the thin air, freezing instantly and snowing down crystals that form mineral spires.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;subglacial ocean&#039;&#039;&#039; is hundreds of kilometers thick.  It is super-pressurized liquid H₂O mixed with NH₃, CH₃OH, H₂O₂, and trace salts.  The movement is slow, planetary-scale currents originating from the Furnace and Coriolis force.  Strong layers exist: the surface is oxidized; the abyssal layer is reducing.&lt;br /&gt;
&lt;br /&gt;
A new &amp;quot;surface&amp;quot; is next.  The &#039;&#039;&#039;Ice Mantle&#039;&#039;&#039; is solid Ice VI and VII.  There are massive, slowly shifting &amp;quot;sub-oceanic continents&amp;quot;. It is periodically fractured and resurfaced by cryoquakes and brine-driven eruptions.  Some regions have developed elevated domes or ridges, continental “shelves” under the ocean.&lt;br /&gt;
&lt;br /&gt;
Finally, underneath is the &#039;&#039;&#039;core&#039;&#039;&#039;. Temperatures exceed 2000–3000 K locally.  Pressures range from 100 to 300 GPa.  The core is rich in heavy elements.  This makes radiogenic hotspots, localized magnetic eddies.  Heat gradients + ion flows = thermoelectric currents.  These make magnetic storms within the ocean itself, not the sky.  When uranium-rich corium pods shift or explode upward through the mantle, their heat and conductivity disturb the local magnetic field, generating geomagnetic quakes.  These pulse through the ocean, creating short-lived magnetic lenses.  These interact with atmospheric charged particles above the Furnace, giving rise to transient magnetic halos visible from orbit—false auroras without a sunstorm.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== e: The Tortured Near-Sphere ====&lt;br /&gt;
[[File:Blasting and shattered.png|thumb|right|An axial recoil event in progress]]&lt;br /&gt;
Orbital and Physical Characteristics&lt;br /&gt;
* Mass: 0.9 Earth masses&lt;br /&gt;
* Radius: 1.0 Earth radii&lt;br /&gt;
* Orbital Period: 58 Earth days&lt;br /&gt;
* Surface Gravity: ~0.9 g&lt;br /&gt;
* Semimajor Axis: ~0.17 AU &lt;br /&gt;
* Spin State: In the &#039;&#039;process&#039;&#039; of becoming tidally locked&lt;br /&gt;
* Obliquity: Extreme, experiencing chaotic realignment events&lt;br /&gt;
&lt;br /&gt;
Internal Structure and Composition&lt;br /&gt;
* &#039;&#039;&#039;Crust:&#039;&#039;&#039; A thick, rigid outer shell of water ice I mixed with clathrates (CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; and CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; hydrates), underlain by layers of ammonia-water ice eutectics. Inclusions of carbon under extreme pressure form diamond strata in the lower crust, lending rigidity and brittle behavior.&lt;br /&gt;
* &#039;&#039;&#039;Mantle:&#039;&#039;&#039; Comprised of Ice VI and Ice VII, with ammonia- and methane-rich brines forming localized conduits and pockets of unstable volatiles.&lt;br /&gt;
* &#039;&#039;&#039;Core:&#039;&#039;&#039; Differentiated and semi-molten. Inner core of iron-nickel alloy spins at a different rate. Outer core is a highly viscous slurry of silicate, iron, carbon, sulfur, and dissolved volatiles. Chemical veins (e.g., uranium silicates, perovskites) act as mechanical shear zones. Tidal torque leads to periodic frictional heating.&lt;br /&gt;
&lt;br /&gt;
Tectonic and Cryovolcanic Behavior&lt;br /&gt;
* The planet resists tidal locking due to core-crust decoupling and uneven angular momentum transfer.&lt;br /&gt;
* High obliquity experiences &#039;&#039;&#039;&#039;&#039;Axial Recoil Events&#039;&#039;&#039;&#039;&#039;, where the entire planet jerks between metastable orientations (e.g., from 110° to 70°) in sudden spasms.&lt;br /&gt;
* These events generate:&lt;br /&gt;
** Global-scale crustal cracking&lt;br /&gt;
** Venting of pressurized subsurface gases (H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;O, CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt;)&lt;br /&gt;
** Surface deformation and glacial faulting&lt;br /&gt;
* Volatiles erupt ballistically into space (200+lm) from exposed fissures and calderas, driven by phase-change explosions.&lt;br /&gt;
&lt;br /&gt;
Surface Conditions&lt;br /&gt;
* Global temperature well below freezing; warmest zones around cryovolcanic hotspots&lt;br /&gt;
* Crustal coloration varies by volatile deposition:&lt;br /&gt;
** Pale blue-white from water ice&lt;br /&gt;
** Red-brown from CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; frostfields&lt;br /&gt;
** Green-black CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; stains from plume fallout&lt;br /&gt;
* Surface features include:&lt;br /&gt;
** Cryovolcanic calderas&lt;br /&gt;
** Diamond-studded impact-like basins&lt;br /&gt;
** Faulted plains crossed by salt-streaked rift zones&lt;br /&gt;
&lt;br /&gt;
Atmosphere and Ejected Material&lt;br /&gt;
* Thin transient exosphere formed from eruptive events&lt;br /&gt;
* Gases often escape to space or freeze back out in polar regions&lt;br /&gt;
* Fallback material creates uneven surface mass distributions, altering moment of inertia and prolonging instability&lt;br /&gt;
&lt;br /&gt;
Appearance from Planet c&lt;br /&gt;
&lt;br /&gt;
* Angular Size: ~4-1 arcminutes&lt;br /&gt;
* Coloration: Overall dusky grey-white, with changing colored bands due to volatile fallout; craterless but mottled&lt;br /&gt;
&lt;br /&gt;
Transient visible phenomena:&lt;br /&gt;
&lt;br /&gt;
* Cryovolcanic plumes visible as fan-like arcs at the limb during outburst events&lt;br /&gt;
* Infrared brightening during Axial Recoil Events&lt;br /&gt;
* Occasional light-scattering halos from plume particles&lt;br /&gt;
&lt;br /&gt;
Event Cycle Summary&lt;br /&gt;
&lt;br /&gt;
# Tidal torque builds due to obliquity misalignment&lt;br /&gt;
# Core resists, crust locks tension&lt;br /&gt;
# Critical stress threshold breached&lt;br /&gt;
# Obliquity lurches to new orientation&lt;br /&gt;
# Crust fractures globally, vents open&lt;br /&gt;
# Supersonic cryovolcanism hurls volatiles into space&lt;br /&gt;
# Fallback modifies crustal mass distribution&lt;br /&gt;
# Obliquity rebuilds instability over decades&lt;br /&gt;
# Repeat.&lt;br /&gt;
&lt;br /&gt;
Planet e is a tortured world caught in an unending cycle of self-correcting failure—its body unable to align, its gases unable to stay contained, its appearance in the sky a visible signature of internal catastrophe.&lt;br /&gt;
&lt;br /&gt;
==== f: Ringed Mini-Neptune ====&lt;br /&gt;
[[File:Ringed Neptune with four moons.png|thumb|right|Aperspectival view of f, its rings, and four moons]]&lt;br /&gt;
This planet is a substantial mini-Neptune, with a mass of approximately 3.5 Earth masses and a radius of 2.0 Earth radii, orbiting at 0.227 AU. Its low mean density (~0.44 ρ⊕) signals the presence of a deep, volatile-rich envelope overlying a denser core. The bulk of its volume is composed of hydrogen and helium, accreted from the protoplanetary disk, with trace amounts of methane (CH₄) and ammonia (NH₃)—gases that dominate its photochemical and radiative behavior. Beneath this envelope, the planet hosts a water–rock–metal core layered in complex phases, with high-pressure ices and possibly superionic water enveloping a metallic center.  Lower atmosphere reaches 300–500 K (27–227°C) near the bottom of the troposphere, depending on opacity and convection.&lt;br /&gt;
&lt;br /&gt;
Visually, the planet exhibits a blue-to-cyan atmospheric hue, governed by Rayleigh scattering and methane absorption in the red and near-infrared spectrum. While not as banded or storm-laced as Jupiter, it features broad zonal flows, high-altitude methane ice clouds, and long-lived anticyclonic storms akin to Neptune’s Great Dark Spot. Due to its tidal locking to the host star, the planet presents hemispheric climatic asymmetry: a sunlit dayside prone to atmospheric upwelling and cloud formation, and a cooler, darker nightside. While colder, the backside is not freezing— in the 150–250 K range, depending on circulation efficiency. Atmospheric circulation is dominated by slow, large-scale overturning cells, moderated by planetary-scale waves and a subdued Coriolis force. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Rings =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Ring!!	Range (Rₚ)!!	Approx.! Range (km)!!	Description&lt;br /&gt;
|-&lt;br /&gt;
! C&lt;br /&gt;
| 	1.5–1.65 Rₚ	||19,100–21,000	||Faint, dusty interior ring&lt;br /&gt;
|-&lt;br /&gt;
! B&lt;br /&gt;
| 	1.65–1.96 Rₚ	||21,000–25,000||	Bright, dense primary ring&lt;br /&gt;
|-&lt;br /&gt;
! Division&lt;br /&gt;
|	1.96–2.04 Rₚ ||25,000–26,000 || a low-density gap&lt;br /&gt;
|-&lt;br /&gt;
!  A&lt;br /&gt;
|	2.04–2.3 Rₚ||26,000–29,300||	Sharp-edged outer ring&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Moon !!	Orbit (km) !!	Orbit (Rₚ) !!	Diameter (km) !!	Type	!! Period !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! I&lt;br /&gt;
|	60,000	||4.7 Rₚ	||~400	||Rocky	|| 0.9 ||Cratered&lt;br /&gt;
|-&lt;br /&gt;
! II&lt;br /&gt;
| 	110,000	|| 8.6 Rₚ	|| ~800	|| Mixed rock/ice	|| 2.25|| Cracked surface, frozen ocean&lt;br /&gt;
|-&lt;br /&gt;
! III &lt;br /&gt;
| 190,000	|| 14.9 Rₚ ||	~1200 ||	Icy major moon ||	5.1|| Cryovolcanism, smooth plains&lt;br /&gt;
|-&lt;br /&gt;
! IV &lt;br /&gt;
|340,000	||26.7 Rₚ	||~200	||Irregular/prograde	|| 12.21 || Dark red/carbon, inclined (20º, eccentric orbit (0.1)&lt;br /&gt;
|-&lt;br /&gt;
! V &lt;br /&gt;
| 710,000 ||	55.7 Rₚ	||~350	|| Captured/retrograde	|| 36.83 || Highly inclined (130º), Split terrain—half rugged highlands, half smooth resurfaced plain&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==== g: Stripped Sub-Neptune Remnant ====&lt;br /&gt;
[[File:Stripped Planet with Two Cool Moons.png|700px|right]]&lt;br /&gt;
Basic Parameters&lt;br /&gt;
* Mass: 2.6 Earth masses (M⊕)&lt;br /&gt;
* Radius: 1.7 Earth radii (R⊕)&lt;br /&gt;
* Mean Density: ~2.92 g/cm³&lt;br /&gt;
* Orbital Distance: 0.4 AU &lt;br /&gt;
* Albedo: ~0.5 (moderately high)&lt;br /&gt;
* Rotation: Tidally locked &lt;br /&gt;
&lt;br /&gt;
Origin and Evolution&lt;br /&gt;
* Formed beyond the snow line (~0.8–1.2 AU) from a mix of rock, iron, and ices&lt;br /&gt;
* Migrated inward early during protoplanetary disk phase&lt;br /&gt;
* Accreted a modest hydrogen-helium envelope (&amp;gt;1% by mass)&lt;br /&gt;
* Exposed to intense stellar X-ray and UV radiation during the M dwarf&#039;s pre-main-sequence phase&lt;br /&gt;
* Lacked a magnetic dynamo (metal-poor and early core freezing)&lt;br /&gt;
* Entire atmosphere lost over ~100 Myr via photoevaporation, core-powered mass loss, and sputtering&lt;br /&gt;
&lt;br /&gt;
Current State&lt;br /&gt;
* Atmosphere: None (trace mineral vapors possible in hot regions)&lt;br /&gt;
* Surface: Stark contrast between hemispheres due to tidal locking&lt;br /&gt;
** Dayside: ~700–1000 K; high-silica lava fields, salt flats, exposed alumino-silicates&lt;br /&gt;
** Nightside: ~100–150 K; gypsum and calcite in cold traps, frozen regolith&lt;br /&gt;
* Magnetosphere: Absent&lt;br /&gt;
* Volcanism:episodic; high-silica flows, volcanic glass, sodium-rich crusts&lt;br /&gt;
* Geological Activity: Tectonically inactive; thermally fractured plains, impact craters&lt;br /&gt;
&lt;br /&gt;
Surface Composition&lt;br /&gt;
* Titanium dioxide (rutile): bright, high-albedo mineral condensate&lt;br /&gt;
* Calcite (CaCO₃): carbonate deposits in cold traps&lt;br /&gt;
* Gypsum (CaSO₄·2H₂O): hydration mineral, stable only on the nightside&lt;br /&gt;
* Sodium chloride: salt flats, especially in evaporated basins&lt;br /&gt;
* High-silica volcanic deposits: glassy, oxidized, and light-colored&lt;br /&gt;
&lt;br /&gt;
Visual and Observational Notes&lt;br /&gt;
&lt;br /&gt;
* High visual contrast between molten and frozen hemispheres&lt;br /&gt;
* Surface appears mottled: obsidian-black lava, gleaming salt flats, white calcium deposits&lt;br /&gt;
* No clouds, auroras, or magnetic activity&lt;br /&gt;
* Extreme day/night temperature gradient&lt;br /&gt;
* Reflective phase curve possible in photometric observations&lt;br /&gt;
* Surface pressure: effectively 0 bar&lt;br /&gt;
&lt;br /&gt;
Planet g is the airless skeleton of a once-sub-Neptune world. Born icy and distant, it migrated into the young star&#039;s wrath, where its fragile envelope boiled away under a sky of flares. Bereft of a magnetic shield, it was slowly stripped to bare rock. Today, one hemisphere bakes in molten silence while the other freezes in shadow. No air, no oceans, only salt, stone, and the echo of a lost atmosphere.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property !!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~75,000 km (~0.26 R&amp;lt;sub&amp;gt;hill&amp;lt;/sub&amp;gt;)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~1,400 km (~0.22 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass	&lt;br /&gt;
| ~0.01 M⊕ (~1.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~3.0 g/cm³ (rock–ice mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temp&lt;br /&gt;
|	~150–180 K&lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
| 0.20g&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere&lt;br /&gt;
|	Trace O₂, from radiolysis and outgassing&lt;br /&gt;
|-&lt;br /&gt;
! Subsurface Ocean&lt;br /&gt;
|	heated by tidal flexing&lt;br /&gt;
|-&lt;br /&gt;
! Surface Features	&lt;br /&gt;
|Fractured ice crust, chaos terrain, cryogeysers, lenticulae&lt;br /&gt;
|}&lt;br /&gt;
gI is a cracked glass orb, rimed with frost and laced with luminous fissures. Below its crust, tides flex a hidden ocean in rhythmic silence. Its faint oxygen exosphere is ghostly but present.  It is frosted quartz with cobwebbed streaks and mineral discoloration.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property!!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~150,000 km (~0.5 Rₕill)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~2,100 km (~0.33 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass&lt;br /&gt;
|	~0.035 M⊕ (~4.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~2.1 g/cm³ (icy-rocky mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes &lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
|	~0.35 g&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temperature&lt;br /&gt;
|	~115–130 K (pressure and greenhouse effects)&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere	&lt;br /&gt;
| ~0.18 bar N₂ + ~0.1 bar Ar + ~0.02 bar CH₄, minor CO, trace haze &lt;br /&gt;
|}&lt;br /&gt;
gII is a muted blue-green crescent veiled in gold. Its sky glows with the weight of argon and the shimmer of methane haze, and its surface smolders with the memory of internal warmth. Liquid hydrocarbons shine like ink in the basins, while glaciers ebb across the uplands. To the star it shows only one face, but beneath that still gaze lies the soft breath of a world more welcoming than its master.&lt;br /&gt;
&lt;br /&gt;
==== h ====&lt;br /&gt;
[[File:Twin Planet, red and blue.png|right|600px]]&lt;br /&gt;
h is a twin-planet system, 1.5 AU from the star, with a period of 4.1 years&lt;br /&gt;
&lt;br /&gt;
Mutual Orbital Configuration&lt;br /&gt;
* Type: True binary planet pair, gravitationally bound, equal mass&lt;br /&gt;
* Masses: 5.0 M⊕ each&lt;br /&gt;
* Radii: 2.3 R⊕ each&lt;br /&gt;
* Mutual Orbit: Essentially circular, ~1 million km separation (~8–10 planetary radii)&lt;br /&gt;
* Period (mutual orbit): ~4.5 days&lt;br /&gt;
* Orbital Plane: Perpendicular to system ecliptic &lt;br /&gt;
* Tidal State: Tidally locked to each other (mutual synchronous rotation)&lt;br /&gt;
&lt;br /&gt;
Planet A — &amp;quot;Sapphire&amp;quot;&lt;br /&gt;
* Coloration: Deep sapphire blue with white high-altitude methane ice hazes&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: H₂, He&lt;br /&gt;
** Methane (CH₄): high&lt;br /&gt;
** Ammonia: trace&lt;br /&gt;
** Argon: moderate&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: slightly enriched&lt;br /&gt;
* Magnetosphere: Strong, symmetric; supports brilliant blue-violet aurorae&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Superionic water mantle&lt;br /&gt;
** Stratified silicate-ice alloy core&lt;br /&gt;
** Radiogenic heating and layered convection&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar hexagonal jet (stronger than Saturn&#039;s)&lt;br /&gt;
** Methane plasma flares at terminator&lt;br /&gt;
** Iridescent methane cirrus clouds&lt;br /&gt;
** Massive auroral crowns aligned with spin-magnetic axis misalignment&lt;br /&gt;
&lt;br /&gt;
Planet B — &amp;quot;Rust&amp;quot;&lt;br /&gt;
* Coloration: Dark crimson to rust-red, streaked with black and violet haze bands&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: N₂, CO&lt;br /&gt;
** CH₄: trace&lt;br /&gt;
** Tholins: abundant&lt;br /&gt;
** Argon: high&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: moderate&lt;br /&gt;
** Magnetosphere: Weak, multipolar and intermittent&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Dense iron-rich core with impact inclusions (e.g., iridium, ruthenium)&lt;br /&gt;
** Volcanically active mantle with carbon-rich inclusions&lt;br /&gt;
** Higher internal heat flow than Sapphire&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar cyclonic basins with geyser-like haze columns&lt;br /&gt;
** Frequent UV lightning within organic clouds&lt;br /&gt;
** Faint auroral echoes from Sapphire’s magnetospheric tail&lt;br /&gt;
** Surface glow from argon emissions during conjunction&lt;br /&gt;
&lt;br /&gt;
Mutual Phenomena &amp;amp; Sky Effects&lt;br /&gt;
* Eclipse Cycles: Frequent, due to short mutual period and perpendicular orbit; cause wave-like haze patterns and shadow bands&lt;br /&gt;
* Filamentary Atmosphere Bridges: Transient stratospheric strands near L1, illuminated during eclipses&lt;br /&gt;
* Auroral Flux Tubes: Occasionally connect the two with violet-green flickering arcs&lt;br /&gt;
* Gravitational Stability: Mutual orbit stable within Hill sphere; resistant to long-term disruption&lt;br /&gt;
&lt;br /&gt;
* Legacy of the Comet Shield&lt;br /&gt;
* Each planet’s core contains embedded relics of the system’s ancient bombardment:&lt;br /&gt;
** Sapphire: interstellar dust, primordial isotopes, deep xenon pockets&lt;br /&gt;
** Rust: impact-derived siderophiles, compressed organics, rare isotopic anomalies&lt;br /&gt;
* Capture Events: Both planets have intercepted and redirected hundreds of large icy bodies over system history&lt;br /&gt;
&lt;br /&gt;
They each have 2 small irregular moons, &amp;lt;100 km diameter, retrograde, on distant orbits.  Negligible.&lt;br /&gt;
&lt;br /&gt;
== Planet C ==&lt;br /&gt;
[[File:Planet C and its tethered moon.png|right|700px]]&lt;br /&gt;
* With an albedo of 0.2, the global average temp is 263ºK.  Because of modest greenhouse effects, surface temperatures are higher, on the sun-side.&lt;br /&gt;
# Mass: 1.5M⊕&lt;br /&gt;
# Gravity: 1g⊕&lt;br /&gt;
# Radius = 1.225⊕, or 7805km&lt;br /&gt;
Terminator Zone&lt;br /&gt;
# +/-30º: 1.28 E8 km&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; (slightly less than all the land of the Earth)&lt;br /&gt;
# Escape velocity is 12.4km/s, 11% higher than Earth&lt;br /&gt;
# Orbital velocity is 8.79km/s&lt;br /&gt;
=== Atmosphere ===&lt;br /&gt;
Water content is low because&lt;br /&gt;
* Water vapor is a potent greenhouse gas; vast surface water can trap too much heat, especially near the substellar point.&lt;br /&gt;
* Water leads to climate homogenization&lt;br /&gt;
* Lack of exposed silicate rock: Necessary for carbon-silicate weathering feedback, which stabilizes climate on geological timescales.&lt;br /&gt;
Earth has ~1.4 billion km³ of water.  In our habitable zone, we have no more than 10% of that, or 100 million km³, though there is much more on the night side, both liquid and ice.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Factor !! Ɬiʔa atm !! Ɬiʔa % !! Earth atm !! Earth % !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! Total Pressure &lt;br /&gt;
| 1.6 atm || || 1.0 atm || || Enhanced convective heat transfer, increased IR trapping&lt;br /&gt;
|-&lt;br /&gt;
! Nitrogen (N₂) &lt;br /&gt;
| 1.00 || 62.50% || 0.7808 || 78.08% || Reduced; still inert, still dominant&lt;br /&gt;
|-&lt;br /&gt;
! Oxygen (O₂) &lt;br /&gt;
| 0.21 || 13.13% || 0.2095 || 20.95% || Earth-normal partial pressure &lt;br /&gt;
|-&lt;br /&gt;
! Argon (Ar)&lt;br /&gt;
| 0.40 || 25.00% || 0.0093 || 0.93% || Major heat distribution enhancement, inert&lt;br /&gt;
|-&lt;br /&gt;
! Krypton + Xenon&lt;br /&gt;
| 0.005 || 0.31% || trace || trace || High molecular mass → improved heat retention, still safe&lt;br /&gt;
|-&lt;br /&gt;
! CO₂&lt;br /&gt;
| 0.005 || 0.31% || 0.004 || 0.04% || slightly elevated; sub-greenhouse threshold&lt;br /&gt;
|-&lt;br /&gt;
! H₂O vapor &lt;br /&gt;
| 0.015 || ~1% || || 0-4% || Maintains greenhouse without excess moisture&lt;br /&gt;
|}&lt;br /&gt;
==== Atmospheric Effects on Clouds ====&lt;br /&gt;
# Increased Pressure (1.6 atm) compresses gases, raising the dew point at which water vapor condenses. Clouds form closer to the surface, and are denser than similar altitudes compared to Earth.&lt;br /&gt;
# Low Water Inventory (~20% of Earth&#039;s): less frequent and less massive cloud systems than on Earth, but still present—especially over &amp;quot;hotspots&amp;quot; on the day side.&lt;br /&gt;
# Tidally Locked Climate: Cloud formation concentrate along the substellar point, where warm, moist air rises and cools.&lt;br /&gt;
#* A permanent “eyewall” storm system has formed at the subsolar point, like a giant hurricane.&lt;br /&gt;
#* As air rises and is advected to the night side, thin cloud bands or ice hazes form as it descends and cools.&lt;br /&gt;
&lt;br /&gt;
Appearance:&lt;br /&gt;
* The presence of noble gases (Ar, Kr, Xe) and higher pressure enhance Mie scattering, making clouds appear whiter and more silvered, especially at sunrise/sunset boundaries.&lt;br /&gt;
* Night side clouds are thin, high-altitude icy sheets, glowing faintly in aurorae or thermal emissions.&lt;br /&gt;
&lt;br /&gt;
==== Sky Color ====&lt;br /&gt;
[[File:Life near the terminator.png|thumb|right|Life near the terminator]]&lt;br /&gt;
The color of the sky is shaped by Rayleigh scattering, which depends on:&lt;br /&gt;
# Molecular composition: Heavier gases like Ar, Kr, and Xe scatter light less efficiently than N₂.&lt;br /&gt;
# Spectral output of the star: the red dwarf emits predominantly infrared and red light, with very little blue or violet.&lt;br /&gt;
&lt;br /&gt;
Consequence:&lt;br /&gt;
* Even with atmospheric scattering, there is insufficient blue light in the stellar spectrum to produce a blue sky.&lt;br /&gt;
* Day sky would likely appear:&lt;br /&gt;
** Dark peach, dusky rose, or reddish beige near zenith,&lt;br /&gt;
** Grading to deep salmon or mauve near the horizon,&lt;br /&gt;
** A slight metallic sheen due to noble gas content and high pressure.&lt;br /&gt;
&lt;br /&gt;
Twilight &amp;amp; Limb Scattering:&lt;br /&gt;
* The terminator (twilight zone) sees a diffuse, ruddy light, scattering through haze and clouds into luminous reds, purples, and copper tones.&lt;br /&gt;
* Aurorae are spectacular on the night side, especially since stellar flares are frequent.&lt;br /&gt;
&lt;br /&gt;
==== Sound Propagation ====&lt;br /&gt;
: &#039;&#039;Sound is profoundly affected by atmospheric pressure and composition.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Compared to Earth:&lt;br /&gt;
* Higher pressure → greater air density → faster transmission of sound and less attenuation.&lt;br /&gt;
* Argon and Xenon are heavy gases, which:&lt;br /&gt;
** Lower the speed of sound relative to air at the same pressure (despite the pressure increase).&lt;br /&gt;
** Shift resonance frequencies downward, resulting in deeper, rounder sounds.&lt;br /&gt;
&lt;br /&gt;
Consequences:&lt;br /&gt;
* Voices sound subtly lower-pitched and richer, especially for consonants and low vowels.&lt;br /&gt;
* Ambient sounds (wind, water, animals) would carry farther and sound more muffled or sonorous.&lt;br /&gt;
* Music or speech would resonate more warmly, especially indoors or in enclosed spaces.&lt;br /&gt;
&lt;br /&gt;
In short: it sounds like it’s wrapped in velvet.&lt;br /&gt;
&lt;br /&gt;
==== Heat Transport to the Night Side ====&lt;br /&gt;
Mechanisms:&lt;br /&gt;
# Thick Atmosphere (1.6 atm) increases:&lt;br /&gt;
#* Advection efficiency: Warm air masses can move more heat horizontally.&lt;br /&gt;
#* Radiative time constant: The atmosphere holds heat longer before releasing it.&lt;br /&gt;
# Noble Gases (especially Kr/Xe):&lt;br /&gt;
#* High molecular mass → more IR opacity → trapping and radiating heat more evenly.&lt;br /&gt;
# Slow Rotation / Tidal Locking:&lt;br /&gt;
#* Global Hadley-like cells dominate circulation, carrying warm air from the day side to the night side and descending it there.&lt;br /&gt;
&lt;br /&gt;
Result:&lt;br /&gt;
* The night side is not so freezing.  Temperatures differ by tens of degrees, not hundreds.&lt;br /&gt;
* There are still ice caps and a cold deserts at the anti-stellar point, but not a glaciated wasteland.&lt;br /&gt;
&lt;br /&gt;
=== Magnetosphere ===&lt;br /&gt;
* Larger mass --&amp;gt; larger iron core, generating more internal heat&lt;br /&gt;
* Larger radius --&amp;gt; Vigorous convection in the core&lt;br /&gt;
* Tidal Flexing --&amp;gt; still drives magnetic activity&lt;br /&gt;
&lt;br /&gt;
# Aurorae at lower latitudes&lt;br /&gt;
## higher magnetic rigidity, wider magnetotail, and greater reconnection energy.&lt;br /&gt;
## Combined with a higher flux of stellar particles, this means:&lt;br /&gt;
### Auroral ovals expand, reaching mid-latitudes sometimes equator.&lt;br /&gt;
### The skies are alive with rippling green, violet, and crimson aurorae, especially on the night side.&lt;br /&gt;
### Daily auroral activity occur during stellar flare cycles.&lt;br /&gt;
# Compasses&lt;br /&gt;
## compasses respond more sharply, with:&lt;br /&gt;
### Faster alignment.&lt;br /&gt;
### Greater resistance to local perturbations.&lt;br /&gt;
## However, frequent magnetic storms from stellar activity cause sudden declinations, reversals, or local anomalies.  In short, lots of aurorae equals dead compasses at the same time.&lt;br /&gt;
# Magnetic Field Strength &amp;gt; 100 μT &lt;br /&gt;
# Electromagnetism is more basic than chemistry or almost any other natural philosophy&lt;br /&gt;
&lt;br /&gt;
=== Substellar Point ===&lt;br /&gt;
The maximum incoming flux is very nearly the same as Earth&#039;s solar constant (≈1361 W/m²), but concentrated over one point rather than averaged over a rotating sphere.  Temperatures should be above 500ºK most of the time.  &lt;br /&gt;
&lt;br /&gt;
The magnetic north is also here. The thick atmosphere prevents too much loss here, but &lt;br /&gt;
* Charged particle influx&lt;br /&gt;
** Maximized at the substellar point—intense auroral and energetic particle precipitation&lt;br /&gt;
* Atmospheric ionization&lt;br /&gt;
** Constant production of high-energy ions and NOx compounds—UV fluorescence in upper sky&lt;br /&gt;
* Localized heating&lt;br /&gt;
** Augments already extreme temperatures—600–700 K surface&lt;br /&gt;
&lt;br /&gt;
== Artificially Tethered Moon ==&lt;br /&gt;
* 670,000 km up&lt;br /&gt;
* 7805 km in radius = same as the planet&lt;br /&gt;
* 1.33º of the sky, same as the sun&lt;br /&gt;
&lt;br /&gt;
A network of tethers/tension lines from the moon to multiple anchor points on the planet’s surface (a tripod or hexapod structure), woven like hair&lt;br /&gt;
* Uses active tension management and orbital station-keeping to stabilize the moon&lt;br /&gt;
* Counterweights and inward-pointing mass drivers on the moon to oppose drift&lt;br /&gt;
&lt;br /&gt;
The tethers are not bearing the full weight, but merely damping drift, providing restoring force, and enabling long-term stability through active compensation.  The moon&lt;br /&gt;
* Blocks the worst of the heat&lt;br /&gt;
* Blocks the worst of the solar radiation&lt;br /&gt;
The moon has &lt;br /&gt;
* low mass&lt;br /&gt;
* high albedo - enormous reflectivity&lt;br /&gt;
* scatters charges particles, UV, X-rays, auroral flux tubes&lt;br /&gt;
* sunward - crazy hot, high emissivity&lt;br /&gt;
* earthward - crazy cool, low emissivity&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168171</id>
		<title>Ɬiʔa/Conworlding</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168171"/>
		<updated>2025-03-28T01:54:13Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* Sky Color */ pic&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Star ==&lt;br /&gt;
Our star is a red-dwarf.&lt;br /&gt;
# Type: M5V&lt;br /&gt;
## M: This indicates it&#039;s a cool, red star with a surface temperature less than 3,500ºK&lt;br /&gt;
## 5: Within the M class, stars are further divided into subclasses 0-9, with 0 being the hottest and 9 the coolest. An M5 star is in the middle of this range.&lt;br /&gt;
## V: Denotes that it&#039;s a main sequence star, also known as a dwarf star&lt;br /&gt;
# Stellar luminosity (L*) ≈ 0.01 𝐿⊙ (1/100th Sol&#039;s brightness)&lt;br /&gt;
# Stellar mass (M*) ≈ 0.2 𝑀⊙ (1/5 the mass of Sol)&lt;br /&gt;
# Stellar radius (R*) ≈ 0.25 𝑅⊙ (1/4 as wide as Sol)&lt;br /&gt;
# Effective temperature (T*) ≈ 3500 K&lt;br /&gt;
​The habitable zone (a) is about square root of L* over L⊙, so ~0.1 AU.&lt;br /&gt;
&lt;br /&gt;
=== Solar System ===&lt;br /&gt;
There are seven planets in the system&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Planet !!	Mass (M🜨)!!	Radius (R🜨)!! Moons/Rings	!!Resonance !!	Semi-Major Axis (AU)!!	Rings !! Moons !! Period !! Size&lt;br /&gt;
|-&lt;br /&gt;
| b ||	2.17 ||	1.1 ||	No ||	2:3 with c	|| 0.0763 ||	No || No || 17.2 || 13.6&#039; to 1.5&#039;&lt;br /&gt;
|-&lt;br /&gt;
| c ||	1.5	 ||1.225 ||	1* ||	—	        || 0.100 || No || No || 25.8 || -&lt;br /&gt;
|-&lt;br /&gt;
| d ||	2.0	 ||1.4 ||No ||	2:3 with c	 ||0.131 ||	No || No || 38.7 || 13.1&#039; to 1.8&#039;&lt;br /&gt;
|-&lt;br /&gt;
| e ||	0.9 ||	1.0 || No	 ||	2:3 with d	 ||0.172 ||	No || No || 58 || 4.1&#039; to 1.1&#039;&lt;br /&gt;
|-&lt;br /&gt;
| f ||	3.5 ||	2.0 ||	Yes! ||	2:3 with e	 ||0.227 || Yes || Junk || 87 || 4.6&#039; to 1.8&#039;&lt;br /&gt;
|-&lt;br /&gt;
| g ||	2.6 ||	1.7 ||	2 ||	-	 ||0.40 ||	Yes || Junk || 206 || 1.6&#039; to 1.0&#039;&lt;br /&gt;
|-&lt;br /&gt;
| h ||	5.0x2 ||2.3x2 || yes	 || -	 ||1.5 ||	Yes || No || 1500 || 0.5&#039; 16.4&#039; apart (at max)&lt;br /&gt;
|}&lt;br /&gt;
==== b: super Mercury with a ring of fire  ====&lt;br /&gt;
[[File:planet b by GPT.png|thumb|right|An artistic rendering of planet b]]&lt;br /&gt;
b is a super-Mercury, tidally locked, and incredibly dense.  ~700ºK on the day side, ~50ºK on the night.  2.1 Earth Masses, 1.1 Earth radii (~7000km) in size.  Orbital period 17.2 days.  Density 9.0 g/cm&amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt;.  Gravity is ~1.8g.  &lt;br /&gt;
&lt;br /&gt;
The iron core is huge, being 75% of the mass.  A thin silicate mantle, with metallic plains and exhumed ultramafic crust, with frequent iron meteorite craters, lacking typical “stone” breccias.&lt;br /&gt;
&lt;br /&gt;
The night side is intense, as simple hydrocarbons (methane, ethane, propane) condense and freeze into layered deposits.  Complex organics (tholins, polycyclic aromatics) accumulate on the sea floor, under miles of nitrogen ice.  Massive slush layers slosh around above cryovolcanic brines of ammonia.&lt;br /&gt;
&lt;br /&gt;
There is a crucial layer of Superionic Ice XI above the core, which acts as an electromagnetic insulator, and ionic heat bridge.  The crust is ultramafic silicates (olivine, pyroxene, perovskite) riddled with with sulfide veins, iron alloys, and graphite networks.  The poles of the magnetosphere are sideways, like Uranus, with poles at the equator in the Terminator Zone.  Persistent surface charges develop, because the whole planet is basically a ginormous Leyden jar!&lt;br /&gt;
&lt;br /&gt;
A planetary flux rope forms and un-forms with the star and planet b.  This induces electric jets at the terminator.  This is where temps are Earth-like.  Hydrocarbons sublimate and eject into the atmosphere, even while aurorae come right down to the ground.  A small, low pressure atmosphere prevents photodissociation, even while electrothermal instabilities lift molecules, forming an anomalous haze, a standing, glowing ring.  Coronal events cause localized lightning geysers with magnetic arcing.&lt;br /&gt;
&lt;br /&gt;
In short, b is visible with a blinding bright sun side (glowing orange bronze), a utterly black night side, and a burning, glowing, erupting, arcing ring at the terminator (all colors).  At biggest, it&#039;s half the size of Earth&#039;s moon in the sky, shrinking down to a star at it&#039;s furthest away.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== d: the wet eye with depths ====&lt;br /&gt;
[[File:wet eye planet.png|thumb|right|An reasonable approximation of d&#039;s appearance]]&lt;br /&gt;
From the outside, d is a &amp;quot;wet eye&amp;quot; just outside the habitable zone.  It is a water world, twice the mass of Earth, 1.4 times the radius, tidally locked.  The substellar point is the only place without surface ice.  However, it is better to think of the planet top-to-bottom.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;atmosphere&#039;&#039;&#039; is tenuous, less than 0.2 bars.  It is thin, N₂-rich with traces of H₂O, NH₃ vapor, and transient geyser outputs.  It is highly UV-irradiated, and Mars-like in its inability to retain volatiles.&lt;br /&gt;
&lt;br /&gt;
Next, there is a &#039;&#039;&#039;surface ice shell&#039;&#039;&#039;, ~20 km of thick Ice I.  Swirling currents beneath have cracked continent-sized ice plates, similar to Europa&#039;s crust.  It is permanently frozen except at the substellar furnace.  It accumulates chemical stains, mineral deposits, and cryovolcanic eruption plumes.  Accumulations of complex hydrates—like methanol clathrates—precipitate out and form false reefs, rising like coral from beneath. Transient thermal vents push hot plumes into the thin air, freezing instantly and snowing down crystals that form mineral spires.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;subglacial ocean&#039;&#039;&#039; is hundreds of kilometers thick.  It is super-pressurized liquid H₂O mixed with NH₃, CH₃OH, H₂O₂, and trace salts.  The movement is slow, planetary-scale currents originating from the Furnace and Coriolis force.  Strong layers exist: the surface is oxidized; the abyssal layer is reducing.&lt;br /&gt;
&lt;br /&gt;
A new &amp;quot;surface&amp;quot; is next.  The &#039;&#039;&#039;Ice Mantle&#039;&#039;&#039; is solid Ice VI and VII.  There are massive, slowly shifting &amp;quot;sub-oceanic continents&amp;quot;. It is periodically fractured and resurfaced by cryoquakes and brine-driven eruptions.  Some regions have developed elevated domes or ridges, continental “shelves” under the ocean.&lt;br /&gt;
&lt;br /&gt;
Finally, underneath is the &#039;&#039;&#039;core&#039;&#039;&#039;. Temperatures exceed 2000–3000 K locally.  Pressures range from 100 to 300 GPa.  The core is rich in heavy elements.  This makes radiogenic hotspots, localized magnetic eddies.  Heat gradients + ion flows = thermoelectric currents.  These make magnetic storms within the ocean itself, not the sky.  When uranium-rich corium pods shift or explode upward through the mantle, their heat and conductivity disturb the local magnetic field, generating geomagnetic quakes.  These pulse through the ocean, creating short-lived magnetic lenses.  These interact with atmospheric charged particles above the Furnace, giving rise to transient magnetic halos visible from orbit—false auroras without a sunstorm.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== e: The Tortured Near-Sphere ====&lt;br /&gt;
[[File:Blasting and shattered.png|thumb|right|An axial recoil event in progress]]&lt;br /&gt;
Orbital and Physical Characteristics&lt;br /&gt;
* Mass: 0.9 Earth masses&lt;br /&gt;
* Radius: 1.0 Earth radii&lt;br /&gt;
* Orbital Period: 58 Earth days&lt;br /&gt;
* Surface Gravity: ~0.9 g&lt;br /&gt;
* Semimajor Axis: ~0.17 AU &lt;br /&gt;
* Spin State: In the &#039;&#039;process&#039;&#039; of becoming tidally locked&lt;br /&gt;
* Obliquity: Extreme, experiencing chaotic realignment events&lt;br /&gt;
&lt;br /&gt;
Internal Structure and Composition&lt;br /&gt;
* &#039;&#039;&#039;Crust:&#039;&#039;&#039; A thick, rigid outer shell of water ice I mixed with clathrates (CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; and CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; hydrates), underlain by layers of ammonia-water ice eutectics. Inclusions of carbon under extreme pressure form diamond strata in the lower crust, lending rigidity and brittle behavior.&lt;br /&gt;
* &#039;&#039;&#039;Mantle:&#039;&#039;&#039; Comprised of Ice VI and Ice VII, with ammonia- and methane-rich brines forming localized conduits and pockets of unstable volatiles.&lt;br /&gt;
* &#039;&#039;&#039;Core:&#039;&#039;&#039; Differentiated and semi-molten. Inner core of iron-nickel alloy spins at a different rate. Outer core is a highly viscous slurry of silicate, iron, carbon, sulfur, and dissolved volatiles. Chemical veins (e.g., uranium silicates, perovskites) act as mechanical shear zones. Tidal torque leads to periodic frictional heating.&lt;br /&gt;
&lt;br /&gt;
Tectonic and Cryovolcanic Behavior&lt;br /&gt;
* The planet resists tidal locking due to core-crust decoupling and uneven angular momentum transfer.&lt;br /&gt;
* High obliquity experiences &#039;&#039;&#039;&#039;&#039;Axial Recoil Events&#039;&#039;&#039;&#039;&#039;, where the entire planet jerks between metastable orientations (e.g., from 110° to 70°) in sudden spasms.&lt;br /&gt;
* These events generate:&lt;br /&gt;
** Global-scale crustal cracking&lt;br /&gt;
** Venting of pressurized subsurface gases (H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;O, CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt;)&lt;br /&gt;
** Surface deformation and glacial faulting&lt;br /&gt;
* Volatiles erupt ballistically into space (200+lm) from exposed fissures and calderas, driven by phase-change explosions.&lt;br /&gt;
&lt;br /&gt;
Surface Conditions&lt;br /&gt;
* Global temperature well below freezing; warmest zones around cryovolcanic hotspots&lt;br /&gt;
* Crustal coloration varies by volatile deposition:&lt;br /&gt;
** Pale blue-white from water ice&lt;br /&gt;
** Red-brown from CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; frostfields&lt;br /&gt;
** Green-black CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; stains from plume fallout&lt;br /&gt;
* Surface features include:&lt;br /&gt;
** Cryovolcanic calderas&lt;br /&gt;
** Diamond-studded impact-like basins&lt;br /&gt;
** Faulted plains crossed by salt-streaked rift zones&lt;br /&gt;
&lt;br /&gt;
Atmosphere and Ejected Material&lt;br /&gt;
* Thin transient exosphere formed from eruptive events&lt;br /&gt;
* Gases often escape to space or freeze back out in polar regions&lt;br /&gt;
* Fallback material creates uneven surface mass distributions, altering moment of inertia and prolonging instability&lt;br /&gt;
&lt;br /&gt;
Appearance from Planet c&lt;br /&gt;
&lt;br /&gt;
* Angular Size: ~4-1 arcminutes&lt;br /&gt;
* Coloration: Overall dusky grey-white, with changing colored bands due to volatile fallout; craterless but mottled&lt;br /&gt;
&lt;br /&gt;
Transient visible phenomena:&lt;br /&gt;
&lt;br /&gt;
* Cryovolcanic plumes visible as fan-like arcs at the limb during outburst events&lt;br /&gt;
* Infrared brightening during Axial Recoil Events&lt;br /&gt;
* Occasional light-scattering halos from plume particles&lt;br /&gt;
&lt;br /&gt;
Event Cycle Summary&lt;br /&gt;
&lt;br /&gt;
# Tidal torque builds due to obliquity misalignment&lt;br /&gt;
# Core resists, crust locks tension&lt;br /&gt;
# Critical stress threshold breached&lt;br /&gt;
# Obliquity lurches to new orientation&lt;br /&gt;
# Crust fractures globally, vents open&lt;br /&gt;
# Supersonic cryovolcanism hurls volatiles into space&lt;br /&gt;
# Fallback modifies crustal mass distribution&lt;br /&gt;
# Obliquity rebuilds instability over decades&lt;br /&gt;
# Repeat.&lt;br /&gt;
&lt;br /&gt;
Planet e is a tortured world caught in an unending cycle of self-correcting failure—its body unable to align, its gases unable to stay contained, its appearance in the sky a visible signature of internal catastrophe.&lt;br /&gt;
&lt;br /&gt;
==== f: Ringed Mini-Neptune ====&lt;br /&gt;
[[File:Ringed Neptune with four moons.png|thumb|right|Aperspectival view of f, its rings, and four moons]]&lt;br /&gt;
This planet is a substantial mini-Neptune, with a mass of approximately 3.5 Earth masses and a radius of 2.0 Earth radii, orbiting at 0.227 AU. Its low mean density (~0.44 ρ⊕) signals the presence of a deep, volatile-rich envelope overlying a denser core. The bulk of its volume is composed of hydrogen and helium, accreted from the protoplanetary disk, with trace amounts of methane (CH₄) and ammonia (NH₃)—gases that dominate its photochemical and radiative behavior. Beneath this envelope, the planet hosts a water–rock–metal core layered in complex phases, with high-pressure ices and possibly superionic water enveloping a metallic center.  Lower atmosphere reaches 300–500 K (27–227°C) near the bottom of the troposphere, depending on opacity and convection.&lt;br /&gt;
&lt;br /&gt;
Visually, the planet exhibits a blue-to-cyan atmospheric hue, governed by Rayleigh scattering and methane absorption in the red and near-infrared spectrum. While not as banded or storm-laced as Jupiter, it features broad zonal flows, high-altitude methane ice clouds, and long-lived anticyclonic storms akin to Neptune’s Great Dark Spot. Due to its tidal locking to the host star, the planet presents hemispheric climatic asymmetry: a sunlit dayside prone to atmospheric upwelling and cloud formation, and a cooler, darker nightside. While colder, the backside is not freezing— in the 150–250 K range, depending on circulation efficiency. Atmospheric circulation is dominated by slow, large-scale overturning cells, moderated by planetary-scale waves and a subdued Coriolis force. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Rings =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Ring!!	Range (Rₚ)!!	Approx.! Range (km)!!	Description&lt;br /&gt;
|-&lt;br /&gt;
! C&lt;br /&gt;
| 	1.5–1.65 Rₚ	||19,100–21,000	||Faint, dusty interior ring&lt;br /&gt;
|-&lt;br /&gt;
! B&lt;br /&gt;
| 	1.65–1.96 Rₚ	||21,000–25,000||	Bright, dense primary ring&lt;br /&gt;
|-&lt;br /&gt;
! Division&lt;br /&gt;
|	1.96–2.04 Rₚ ||25,000–26,000 || a low-density gap&lt;br /&gt;
|-&lt;br /&gt;
!  A&lt;br /&gt;
|	2.04–2.3 Rₚ||26,000–29,300||	Sharp-edged outer ring&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Moon !!	Orbit (km) !!	Orbit (Rₚ) !!	Diameter (km) !!	Type	!! Period !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! I&lt;br /&gt;
|	60,000	||4.7 Rₚ	||~400	||Rocky	|| 0.9 ||Cratered&lt;br /&gt;
|-&lt;br /&gt;
! II&lt;br /&gt;
| 	110,000	|| 8.6 Rₚ	|| ~800	|| Mixed rock/ice	|| 2.25|| Cracked surface, frozen ocean&lt;br /&gt;
|-&lt;br /&gt;
! III &lt;br /&gt;
| 190,000	|| 14.9 Rₚ ||	~1200 ||	Icy major moon ||	5.1|| Cryovolcanism, smooth plains&lt;br /&gt;
|-&lt;br /&gt;
! IV &lt;br /&gt;
|340,000	||26.7 Rₚ	||~200	||Irregular/prograde	|| 12.21 || Dark red/carbon, inclined (20º, eccentric orbit (0.1)&lt;br /&gt;
|-&lt;br /&gt;
! V &lt;br /&gt;
| 710,000 ||	55.7 Rₚ	||~350	|| Captured/retrograde	|| 36.83 || Highly inclined (130º), Split terrain—half rugged highlands, half smooth resurfaced plain&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==== g: Stripped Sub-Neptune Remnant ====&lt;br /&gt;
[[File:Stripped Planet with Two Cool Moons.png|700px|right]]&lt;br /&gt;
Basic Parameters&lt;br /&gt;
* Mass: 2.6 Earth masses (M⊕)&lt;br /&gt;
* Radius: 1.7 Earth radii (R⊕)&lt;br /&gt;
* Mean Density: ~2.92 g/cm³&lt;br /&gt;
* Orbital Distance: 0.4 AU &lt;br /&gt;
* Albedo: ~0.5 (moderately high)&lt;br /&gt;
* Rotation: Tidally locked &lt;br /&gt;
&lt;br /&gt;
Origin and Evolution&lt;br /&gt;
* Formed beyond the snow line (~0.8–1.2 AU) from a mix of rock, iron, and ices&lt;br /&gt;
* Migrated inward early during protoplanetary disk phase&lt;br /&gt;
* Accreted a modest hydrogen-helium envelope (&amp;gt;1% by mass)&lt;br /&gt;
* Exposed to intense stellar X-ray and UV radiation during the M dwarf&#039;s pre-main-sequence phase&lt;br /&gt;
* Lacked a magnetic dynamo (metal-poor and early core freezing)&lt;br /&gt;
* Entire atmosphere lost over ~100 Myr via photoevaporation, core-powered mass loss, and sputtering&lt;br /&gt;
&lt;br /&gt;
Current State&lt;br /&gt;
* Atmosphere: None (trace mineral vapors possible in hot regions)&lt;br /&gt;
* Surface: Stark contrast between hemispheres due to tidal locking&lt;br /&gt;
** Dayside: ~700–1000 K; high-silica lava fields, salt flats, exposed alumino-silicates&lt;br /&gt;
** Nightside: ~100–150 K; gypsum and calcite in cold traps, frozen regolith&lt;br /&gt;
* Magnetosphere: Absent&lt;br /&gt;
* Volcanism:episodic; high-silica flows, volcanic glass, sodium-rich crusts&lt;br /&gt;
* Geological Activity: Tectonically inactive; thermally fractured plains, impact craters&lt;br /&gt;
&lt;br /&gt;
Surface Composition&lt;br /&gt;
* Titanium dioxide (rutile): bright, high-albedo mineral condensate&lt;br /&gt;
* Calcite (CaCO₃): carbonate deposits in cold traps&lt;br /&gt;
* Gypsum (CaSO₄·2H₂O): hydration mineral, stable only on the nightside&lt;br /&gt;
* Sodium chloride: salt flats, especially in evaporated basins&lt;br /&gt;
* High-silica volcanic deposits: glassy, oxidized, and light-colored&lt;br /&gt;
&lt;br /&gt;
Visual and Observational Notes&lt;br /&gt;
&lt;br /&gt;
* High visual contrast between molten and frozen hemispheres&lt;br /&gt;
* Surface appears mottled: obsidian-black lava, gleaming salt flats, white calcium deposits&lt;br /&gt;
* No clouds, auroras, or magnetic activity&lt;br /&gt;
* Extreme day/night temperature gradient&lt;br /&gt;
* Reflective phase curve possible in photometric observations&lt;br /&gt;
* Surface pressure: effectively 0 bar&lt;br /&gt;
&lt;br /&gt;
Planet g is the airless skeleton of a once-sub-Neptune world. Born icy and distant, it migrated into the young star&#039;s wrath, where its fragile envelope boiled away under a sky of flares. Bereft of a magnetic shield, it was slowly stripped to bare rock. Today, one hemisphere bakes in molten silence while the other freezes in shadow. No air, no oceans, only salt, stone, and the echo of a lost atmosphere.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property !!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~75,000 km (~0.26 R&amp;lt;sub&amp;gt;hill&amp;lt;/sub&amp;gt;)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~1,400 km (~0.22 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass	&lt;br /&gt;
| ~0.01 M⊕ (~1.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~3.0 g/cm³ (rock–ice mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temp&lt;br /&gt;
|	~150–180 K&lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
| 0.20g&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere&lt;br /&gt;
|	Trace O₂, from radiolysis and outgassing&lt;br /&gt;
|-&lt;br /&gt;
! Subsurface Ocean&lt;br /&gt;
|	heated by tidal flexing&lt;br /&gt;
|-&lt;br /&gt;
! Surface Features	&lt;br /&gt;
|Fractured ice crust, chaos terrain, cryogeysers, lenticulae&lt;br /&gt;
|}&lt;br /&gt;
gI is a cracked glass orb, rimed with frost and laced with luminous fissures. Below its crust, tides flex a hidden ocean in rhythmic silence. Its faint oxygen exosphere is ghostly but present.  It is frosted quartz with cobwebbed streaks and mineral discoloration.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property!!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~150,000 km (~0.5 Rₕill)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~2,100 km (~0.33 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass&lt;br /&gt;
|	~0.035 M⊕ (~4.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~2.1 g/cm³ (icy-rocky mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes &lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
|	~0.35 g&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temperature&lt;br /&gt;
|	~115–130 K (pressure and greenhouse effects)&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere	&lt;br /&gt;
| ~0.18 bar N₂ + ~0.1 bar Ar + ~0.02 bar CH₄, minor CO, trace haze &lt;br /&gt;
|}&lt;br /&gt;
gII is a muted blue-green crescent veiled in gold. Its sky glows with the weight of argon and the shimmer of methane haze, and its surface smolders with the memory of internal warmth. Liquid hydrocarbons shine like ink in the basins, while glaciers ebb across the uplands. To the star it shows only one face, but beneath that still gaze lies the soft breath of a world more welcoming than its master.&lt;br /&gt;
&lt;br /&gt;
==== h ====&lt;br /&gt;
[[File:Twin Planet, red and blue.png|right|600px]]&lt;br /&gt;
h is a twin-planet system, 1.5 AU from the star, with a period of 4.1 years&lt;br /&gt;
&lt;br /&gt;
Mutual Orbital Configuration&lt;br /&gt;
* Type: True binary planet pair, gravitationally bound, equal mass&lt;br /&gt;
* Masses: 5.0 M⊕ each&lt;br /&gt;
* Radii: 2.3 R⊕ each&lt;br /&gt;
* Mutual Orbit: Essentially circular, ~1 million km separation (~8–10 planetary radii)&lt;br /&gt;
* Period (mutual orbit): ~4.5 days&lt;br /&gt;
* Orbital Plane: Perpendicular to system ecliptic &lt;br /&gt;
* Tidal State: Tidally locked to each other (mutual synchronous rotation)&lt;br /&gt;
&lt;br /&gt;
Planet A — &amp;quot;Sapphire&amp;quot;&lt;br /&gt;
* Coloration: Deep sapphire blue with white high-altitude methane ice hazes&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: H₂, He&lt;br /&gt;
** Methane (CH₄): high&lt;br /&gt;
** Ammonia: trace&lt;br /&gt;
** Argon: moderate&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: slightly enriched&lt;br /&gt;
* Magnetosphere: Strong, symmetric; supports brilliant blue-violet aurorae&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Superionic water mantle&lt;br /&gt;
** Stratified silicate-ice alloy core&lt;br /&gt;
** Radiogenic heating and layered convection&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar hexagonal jet (stronger than Saturn&#039;s)&lt;br /&gt;
** Methane plasma flares at terminator&lt;br /&gt;
** Iridescent methane cirrus clouds&lt;br /&gt;
** Massive auroral crowns aligned with spin-magnetic axis misalignment&lt;br /&gt;
&lt;br /&gt;
Planet B — &amp;quot;Rust&amp;quot;&lt;br /&gt;
* Coloration: Dark crimson to rust-red, streaked with black and violet haze bands&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: N₂, CO&lt;br /&gt;
** CH₄: trace&lt;br /&gt;
** Tholins: abundant&lt;br /&gt;
** Argon: high&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: moderate&lt;br /&gt;
** Magnetosphere: Weak, multipolar and intermittent&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Dense iron-rich core with impact inclusions (e.g., iridium, ruthenium)&lt;br /&gt;
** Volcanically active mantle with carbon-rich inclusions&lt;br /&gt;
** Higher internal heat flow than Sapphire&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar cyclonic basins with geyser-like haze columns&lt;br /&gt;
** Frequent UV lightning within organic clouds&lt;br /&gt;
** Faint auroral echoes from Sapphire’s magnetospheric tail&lt;br /&gt;
** Surface glow from argon emissions during conjunction&lt;br /&gt;
&lt;br /&gt;
Mutual Phenomena &amp;amp; Sky Effects&lt;br /&gt;
* Eclipse Cycles: Frequent, due to short mutual period and perpendicular orbit; cause wave-like haze patterns and shadow bands&lt;br /&gt;
* Filamentary Atmosphere Bridges: Transient stratospheric strands near L1, illuminated during eclipses&lt;br /&gt;
* Auroral Flux Tubes: Occasionally connect the two with violet-green flickering arcs&lt;br /&gt;
* Gravitational Stability: Mutual orbit stable within Hill sphere; resistant to long-term disruption&lt;br /&gt;
&lt;br /&gt;
* Legacy of the Comet Shield&lt;br /&gt;
* Each planet’s core contains embedded relics of the system’s ancient bombardment:&lt;br /&gt;
** Sapphire: interstellar dust, primordial isotopes, deep xenon pockets&lt;br /&gt;
** Rust: impact-derived siderophiles, compressed organics, rare isotopic anomalies&lt;br /&gt;
* Capture Events: Both planets have intercepted and redirected hundreds of large icy bodies over system history&lt;br /&gt;
&lt;br /&gt;
They each have 2 small irregular moons, &amp;lt;100 km diameter, retrograde, on distant orbits.  Negligible.&lt;br /&gt;
&lt;br /&gt;
== Planet C ==&lt;br /&gt;
[[File:Planet C and its tethered moon.png|right|700px]]&lt;br /&gt;
* With an albedo of 0.2, the global average temp is 263ºK.  Because of modest greenhouse effects, surface temperatures are higher, on the sun-side.&lt;br /&gt;
# Mass: 1.5M⊕&lt;br /&gt;
# Gravity: 1g⊕&lt;br /&gt;
# Radius = 1.225⊕, or 7805km&lt;br /&gt;
Terminator Zone&lt;br /&gt;
# +/-30º: 1.28 E8 km&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; (slightly less than all the land of the Earth)&lt;br /&gt;
# Escape velocity is 12.4km/s, 11% higher than Earth&lt;br /&gt;
# Orbital velocity is 8.79km/s&lt;br /&gt;
=== Atmosphere ===&lt;br /&gt;
Water content is low because&lt;br /&gt;
* Water vapor is a potent greenhouse gas; vast surface water can trap too much heat, especially near the substellar point.&lt;br /&gt;
* Water leads to climate homogenization&lt;br /&gt;
* Lack of exposed silicate rock: Necessary for carbon-silicate weathering feedback, which stabilizes climate on geological timescales.&lt;br /&gt;
Earth has ~1.4 billion km³ of water.  In our habitable zone, we have no more than 10% of that, or 100 million km³, though there is much more on the night side, both liquid and ice.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Factor !! Ɬiʔa atm !! Ɬiʔa % !! Earth atm !! Earth % !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! Total Pressure &lt;br /&gt;
| 1.6 atm || || 1.0 atm || || Enhanced convective heat transfer, increased IR trapping&lt;br /&gt;
|-&lt;br /&gt;
! Nitrogen (N₂) &lt;br /&gt;
| 1.00 || 62.50% || 0.7808 || 78.08% || Reduced; still inert, still dominant&lt;br /&gt;
|-&lt;br /&gt;
! Oxygen (O₂) &lt;br /&gt;
| 0.21 || 13.13% || 0.2095 || 20.95% || Earth-normal partial pressure &lt;br /&gt;
|-&lt;br /&gt;
! Argon (Ar)&lt;br /&gt;
| 0.40 || 25.00% || 0.0093 || 0.93% || Major heat distribution enhancement, inert&lt;br /&gt;
|-&lt;br /&gt;
! Krypton + Xenon&lt;br /&gt;
| 0.005 || 0.31% || trace || trace || High molecular mass → improved heat retention, still safe&lt;br /&gt;
|-&lt;br /&gt;
! CO₂&lt;br /&gt;
| 0.005 || 0.31% || 0.004 || 0.04% || slightly elevated; sub-greenhouse threshold&lt;br /&gt;
|-&lt;br /&gt;
! H₂O vapor &lt;br /&gt;
| 0.015 || ~1% || || 0-4% || Maintains greenhouse without excess moisture&lt;br /&gt;
|}&lt;br /&gt;
==== Atmospheric Effects on Clouds ====&lt;br /&gt;
# Increased Pressure (1.6 atm) compresses gases, raising the dew point at which water vapor condenses. Clouds form closer to the surface, and are denser than similar altitudes compared to Earth.&lt;br /&gt;
# Low Water Inventory (~20% of Earth&#039;s): less frequent and less massive cloud systems than on Earth, but still present—especially over &amp;quot;hotspots&amp;quot; on the day side.&lt;br /&gt;
# Tidally Locked Climate: Cloud formation concentrate along the substellar point, where warm, moist air rises and cools.&lt;br /&gt;
#* A permanent “eyewall” storm system has formed at the subsolar point, like a giant hurricane.&lt;br /&gt;
#* As air rises and is advected to the night side, thin cloud bands or ice hazes form as it descends and cools.&lt;br /&gt;
&lt;br /&gt;
Appearance:&lt;br /&gt;
* The presence of noble gases (Ar, Kr, Xe) and higher pressure enhance Mie scattering, making clouds appear whiter and more silvered, especially at sunrise/sunset boundaries.&lt;br /&gt;
* Night side clouds are thin, high-altitude icy sheets, glowing faintly in aurorae or thermal emissions.&lt;br /&gt;
&lt;br /&gt;
==== Sky Color ====&lt;br /&gt;
[[File:Life near the terminator.png|thumb|right|Life near the terminator]]&lt;br /&gt;
The color of the sky is shaped by Rayleigh scattering, which depends on:&lt;br /&gt;
# Molecular composition: Heavier gases like Ar, Kr, and Xe scatter light less efficiently than N₂.&lt;br /&gt;
# Spectral output of the star: the red dwarf emits predominantly infrared and red light, with very little blue or violet.&lt;br /&gt;
&lt;br /&gt;
Consequence:&lt;br /&gt;
* Even with atmospheric scattering, there is insufficient blue light in the stellar spectrum to produce a blue sky.&lt;br /&gt;
* Day sky would likely appear:&lt;br /&gt;
** Dark peach, dusky rose, or reddish beige near zenith,&lt;br /&gt;
** Grading to deep salmon or mauve near the horizon,&lt;br /&gt;
** A slight metallic sheen due to noble gas content and high pressure.&lt;br /&gt;
&lt;br /&gt;
Twilight &amp;amp; Limb Scattering:&lt;br /&gt;
* The terminator (twilight zone) sees a diffuse, ruddy light, scattering through haze and clouds into luminous reds, purples, and copper tones.&lt;br /&gt;
* Aurorae are spectacular on the night side, especially since stellar flares are frequent.&lt;br /&gt;
&lt;br /&gt;
==== Sound Propagation ====&lt;br /&gt;
: &#039;&#039;Sound is profoundly affected by atmospheric pressure and composition.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Compared to Earth:&lt;br /&gt;
* Higher pressure → greater air density → faster transmission of sound and less attenuation.&lt;br /&gt;
* Argon and Xenon are heavy gases, which:&lt;br /&gt;
** Lower the speed of sound relative to air at the same pressure (despite the pressure increase).&lt;br /&gt;
** Shift resonance frequencies downward, resulting in deeper, rounder sounds.&lt;br /&gt;
&lt;br /&gt;
Consequences:&lt;br /&gt;
* Voices sound subtly lower-pitched and richer, especially for consonants and low vowels.&lt;br /&gt;
* Ambient sounds (wind, water, animals) would carry farther and sound more muffled or sonorous.&lt;br /&gt;
* Music or speech would resonate more warmly, especially indoors or in enclosed spaces.&lt;br /&gt;
&lt;br /&gt;
In short: it sounds like it’s wrapped in velvet.&lt;br /&gt;
&lt;br /&gt;
==== Heat Transport to the Night Side ====&lt;br /&gt;
Mechanisms:&lt;br /&gt;
# Thick Atmosphere (1.6 atm) increases:&lt;br /&gt;
#* Advection efficiency: Warm air masses can move more heat horizontally.&lt;br /&gt;
#* Radiative time constant: The atmosphere holds heat longer before releasing it.&lt;br /&gt;
# Noble Gases (especially Kr/Xe):&lt;br /&gt;
#* High molecular mass → more IR opacity → trapping and radiating heat more evenly.&lt;br /&gt;
# Slow Rotation / Tidal Locking:&lt;br /&gt;
#* Global Hadley-like cells dominate circulation, carrying warm air from the day side to the night side and descending it there.&lt;br /&gt;
&lt;br /&gt;
Result:&lt;br /&gt;
* The night side is not so freezing.  Temperatures differ by tens of degrees, not hundreds.&lt;br /&gt;
* There are still ice caps and a cold deserts at the anti-stellar point, but not a glaciated wasteland.&lt;br /&gt;
&lt;br /&gt;
=== Magnetosphere ===&lt;br /&gt;
* Larger mass --&amp;gt; larger iron core, generating more internal heat&lt;br /&gt;
* Larger radius --&amp;gt; Vigorous convection in the core&lt;br /&gt;
* Tidal Flexing --&amp;gt; still drives magnetic activity&lt;br /&gt;
&lt;br /&gt;
# Aurorae at lower latitudes&lt;br /&gt;
## higher magnetic rigidity, wider magnetotail, and greater reconnection energy.&lt;br /&gt;
## Combined with a higher flux of stellar particles, this means:&lt;br /&gt;
### Auroral ovals expand, reaching mid-latitudes sometimes equator.&lt;br /&gt;
### The skies are alive with rippling green, violet, and crimson aurorae, especially on the night side.&lt;br /&gt;
### Daily auroral activity occur during stellar flare cycles.&lt;br /&gt;
# Compasses&lt;br /&gt;
## compasses respond more sharply, with:&lt;br /&gt;
### Faster alignment.&lt;br /&gt;
### Greater resistance to local perturbations.&lt;br /&gt;
## However, frequent magnetic storms from stellar activity cause sudden declinations, reversals, or local anomalies.  In short, lots of aurorae equals dead compasses at the same time.&lt;br /&gt;
# Magnetic Field Strength &amp;gt; 100 μT &lt;br /&gt;
# Electromagnetism is more basic than chemistry or almost any other natural philosophy&lt;br /&gt;
&lt;br /&gt;
=== Substellar Point ===&lt;br /&gt;
The maximum incoming flux is very nearly the same as Earth&#039;s solar constant (≈1361 W/m²), but concentrated over one point rather than averaged over a rotating sphere.  Temperatures should be above 500ºK most of the time.  &lt;br /&gt;
&lt;br /&gt;
The magnetic north is also here. The thick atmosphere prevents too much loss here, but &lt;br /&gt;
* Charged particle influx&lt;br /&gt;
** Maximized at the substellar point—intense auroral and energetic particle precipitation&lt;br /&gt;
* Atmospheric ionization&lt;br /&gt;
** Constant production of high-energy ions and NOx compounds—UV fluorescence in upper sky&lt;br /&gt;
* Localized heating&lt;br /&gt;
** Augments already extreme temperatures—600–700 K surface&lt;br /&gt;
&lt;br /&gt;
== Artificially Tethered Moon ==&lt;br /&gt;
* 670,000 km up&lt;br /&gt;
* 7805 km in radius = same as the planet&lt;br /&gt;
* 1.33º of the sky, same as the sun&lt;br /&gt;
&lt;br /&gt;
A network of tethers/tension lines from the moon to multiple anchor points on the planet’s surface (a tripod or hexapod structure), woven like hair&lt;br /&gt;
* Uses active tension management and orbital station-keeping to stabilize the moon&lt;br /&gt;
* Counterweights and inward-pointing mass drivers on the moon to oppose drift&lt;br /&gt;
&lt;br /&gt;
The tethers are not bearing the full weight, but merely damping drift, providing restoring force, and enabling long-term stability through active compensation.  The moon&lt;br /&gt;
* Blocks the worst of the heat&lt;br /&gt;
* Blocks the worst of the solar radiation&lt;br /&gt;
The moon has &lt;br /&gt;
* low mass&lt;br /&gt;
* high albedo - enormous reflectivity&lt;br /&gt;
* scatters charges particles, UV, X-rays, auroral flux tubes&lt;br /&gt;
* sunward - crazy hot, high emissivity&lt;br /&gt;
* earthward - crazy cool, low emissivity&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=File:Life_near_the_terminator.png&amp;diff=168170</id>
		<title>File:Life near the terminator.png</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=File:Life_near_the_terminator.png&amp;diff=168170"/>
		<updated>2025-03-28T01:53:47Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: peachy planet&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Summary ==&lt;br /&gt;
peachy planet&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168169</id>
		<title>Ɬiʔa/Conworlding</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168169"/>
		<updated>2025-03-28T01:43:43Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* Planet C */ pic&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Star ==&lt;br /&gt;
Our star is a red-dwarf.&lt;br /&gt;
# Type: M5V&lt;br /&gt;
## M: This indicates it&#039;s a cool, red star with a surface temperature less than 3,500ºK&lt;br /&gt;
## 5: Within the M class, stars are further divided into subclasses 0-9, with 0 being the hottest and 9 the coolest. An M5 star is in the middle of this range.&lt;br /&gt;
## V: Denotes that it&#039;s a main sequence star, also known as a dwarf star&lt;br /&gt;
# Stellar luminosity (L*) ≈ 0.01 𝐿⊙ (1/100th Sol&#039;s brightness)&lt;br /&gt;
# Stellar mass (M*) ≈ 0.2 𝑀⊙ (1/5 the mass of Sol)&lt;br /&gt;
# Stellar radius (R*) ≈ 0.25 𝑅⊙ (1/4 as wide as Sol)&lt;br /&gt;
# Effective temperature (T*) ≈ 3500 K&lt;br /&gt;
​The habitable zone (a) is about square root of L* over L⊙, so ~0.1 AU.&lt;br /&gt;
&lt;br /&gt;
=== Solar System ===&lt;br /&gt;
There are seven planets in the system&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Planet !!	Mass (M🜨)!!	Radius (R🜨)!! Moons/Rings	!!Resonance !!	Semi-Major Axis (AU)!!	Rings !! Moons !! Period !! Size&lt;br /&gt;
|-&lt;br /&gt;
| b ||	2.17 ||	1.1 ||	No ||	2:3 with c	|| 0.0763 ||	No || No || 17.2 || 13.6&#039; to 1.5&#039;&lt;br /&gt;
|-&lt;br /&gt;
| c ||	1.5	 ||1.225 ||	1* ||	—	        || 0.100 || No || No || 25.8 || -&lt;br /&gt;
|-&lt;br /&gt;
| d ||	2.0	 ||1.4 ||No ||	2:3 with c	 ||0.131 ||	No || No || 38.7 || 13.1&#039; to 1.8&#039;&lt;br /&gt;
|-&lt;br /&gt;
| e ||	0.9 ||	1.0 || No	 ||	2:3 with d	 ||0.172 ||	No || No || 58 || 4.1&#039; to 1.1&#039;&lt;br /&gt;
|-&lt;br /&gt;
| f ||	3.5 ||	2.0 ||	Yes! ||	2:3 with e	 ||0.227 || Yes || Junk || 87 || 4.6&#039; to 1.8&#039;&lt;br /&gt;
|-&lt;br /&gt;
| g ||	2.6 ||	1.7 ||	2 ||	-	 ||0.40 ||	Yes || Junk || 206 || 1.6&#039; to 1.0&#039;&lt;br /&gt;
|-&lt;br /&gt;
| h ||	5.0x2 ||2.3x2 || yes	 || -	 ||1.5 ||	Yes || No || 1500 || 0.5&#039; 16.4&#039; apart (at max)&lt;br /&gt;
|}&lt;br /&gt;
==== b: super Mercury with a ring of fire  ====&lt;br /&gt;
[[File:planet b by GPT.png|thumb|right|An artistic rendering of planet b]]&lt;br /&gt;
b is a super-Mercury, tidally locked, and incredibly dense.  ~700ºK on the day side, ~50ºK on the night.  2.1 Earth Masses, 1.1 Earth radii (~7000km) in size.  Orbital period 17.2 days.  Density 9.0 g/cm&amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt;.  Gravity is ~1.8g.  &lt;br /&gt;
&lt;br /&gt;
The iron core is huge, being 75% of the mass.  A thin silicate mantle, with metallic plains and exhumed ultramafic crust, with frequent iron meteorite craters, lacking typical “stone” breccias.&lt;br /&gt;
&lt;br /&gt;
The night side is intense, as simple hydrocarbons (methane, ethane, propane) condense and freeze into layered deposits.  Complex organics (tholins, polycyclic aromatics) accumulate on the sea floor, under miles of nitrogen ice.  Massive slush layers slosh around above cryovolcanic brines of ammonia.&lt;br /&gt;
&lt;br /&gt;
There is a crucial layer of Superionic Ice XI above the core, which acts as an electromagnetic insulator, and ionic heat bridge.  The crust is ultramafic silicates (olivine, pyroxene, perovskite) riddled with with sulfide veins, iron alloys, and graphite networks.  The poles of the magnetosphere are sideways, like Uranus, with poles at the equator in the Terminator Zone.  Persistent surface charges develop, because the whole planet is basically a ginormous Leyden jar!&lt;br /&gt;
&lt;br /&gt;
A planetary flux rope forms and un-forms with the star and planet b.  This induces electric jets at the terminator.  This is where temps are Earth-like.  Hydrocarbons sublimate and eject into the atmosphere, even while aurorae come right down to the ground.  A small, low pressure atmosphere prevents photodissociation, even while electrothermal instabilities lift molecules, forming an anomalous haze, a standing, glowing ring.  Coronal events cause localized lightning geysers with magnetic arcing.&lt;br /&gt;
&lt;br /&gt;
In short, b is visible with a blinding bright sun side (glowing orange bronze), a utterly black night side, and a burning, glowing, erupting, arcing ring at the terminator (all colors).  At biggest, it&#039;s half the size of Earth&#039;s moon in the sky, shrinking down to a star at it&#039;s furthest away.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== d: the wet eye with depths ====&lt;br /&gt;
[[File:wet eye planet.png|thumb|right|An reasonable approximation of d&#039;s appearance]]&lt;br /&gt;
From the outside, d is a &amp;quot;wet eye&amp;quot; just outside the habitable zone.  It is a water world, twice the mass of Earth, 1.4 times the radius, tidally locked.  The substellar point is the only place without surface ice.  However, it is better to think of the planet top-to-bottom.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;atmosphere&#039;&#039;&#039; is tenuous, less than 0.2 bars.  It is thin, N₂-rich with traces of H₂O, NH₃ vapor, and transient geyser outputs.  It is highly UV-irradiated, and Mars-like in its inability to retain volatiles.&lt;br /&gt;
&lt;br /&gt;
Next, there is a &#039;&#039;&#039;surface ice shell&#039;&#039;&#039;, ~20 km of thick Ice I.  Swirling currents beneath have cracked continent-sized ice plates, similar to Europa&#039;s crust.  It is permanently frozen except at the substellar furnace.  It accumulates chemical stains, mineral deposits, and cryovolcanic eruption plumes.  Accumulations of complex hydrates—like methanol clathrates—precipitate out and form false reefs, rising like coral from beneath. Transient thermal vents push hot plumes into the thin air, freezing instantly and snowing down crystals that form mineral spires.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;subglacial ocean&#039;&#039;&#039; is hundreds of kilometers thick.  It is super-pressurized liquid H₂O mixed with NH₃, CH₃OH, H₂O₂, and trace salts.  The movement is slow, planetary-scale currents originating from the Furnace and Coriolis force.  Strong layers exist: the surface is oxidized; the abyssal layer is reducing.&lt;br /&gt;
&lt;br /&gt;
A new &amp;quot;surface&amp;quot; is next.  The &#039;&#039;&#039;Ice Mantle&#039;&#039;&#039; is solid Ice VI and VII.  There are massive, slowly shifting &amp;quot;sub-oceanic continents&amp;quot;. It is periodically fractured and resurfaced by cryoquakes and brine-driven eruptions.  Some regions have developed elevated domes or ridges, continental “shelves” under the ocean.&lt;br /&gt;
&lt;br /&gt;
Finally, underneath is the &#039;&#039;&#039;core&#039;&#039;&#039;. Temperatures exceed 2000–3000 K locally.  Pressures range from 100 to 300 GPa.  The core is rich in heavy elements.  This makes radiogenic hotspots, localized magnetic eddies.  Heat gradients + ion flows = thermoelectric currents.  These make magnetic storms within the ocean itself, not the sky.  When uranium-rich corium pods shift or explode upward through the mantle, their heat and conductivity disturb the local magnetic field, generating geomagnetic quakes.  These pulse through the ocean, creating short-lived magnetic lenses.  These interact with atmospheric charged particles above the Furnace, giving rise to transient magnetic halos visible from orbit—false auroras without a sunstorm.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== e: The Tortured Near-Sphere ====&lt;br /&gt;
[[File:Blasting and shattered.png|thumb|right|An axial recoil event in progress]]&lt;br /&gt;
Orbital and Physical Characteristics&lt;br /&gt;
* Mass: 0.9 Earth masses&lt;br /&gt;
* Radius: 1.0 Earth radii&lt;br /&gt;
* Orbital Period: 58 Earth days&lt;br /&gt;
* Surface Gravity: ~0.9 g&lt;br /&gt;
* Semimajor Axis: ~0.17 AU &lt;br /&gt;
* Spin State: In the &#039;&#039;process&#039;&#039; of becoming tidally locked&lt;br /&gt;
* Obliquity: Extreme, experiencing chaotic realignment events&lt;br /&gt;
&lt;br /&gt;
Internal Structure and Composition&lt;br /&gt;
* &#039;&#039;&#039;Crust:&#039;&#039;&#039; A thick, rigid outer shell of water ice I mixed with clathrates (CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; and CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; hydrates), underlain by layers of ammonia-water ice eutectics. Inclusions of carbon under extreme pressure form diamond strata in the lower crust, lending rigidity and brittle behavior.&lt;br /&gt;
* &#039;&#039;&#039;Mantle:&#039;&#039;&#039; Comprised of Ice VI and Ice VII, with ammonia- and methane-rich brines forming localized conduits and pockets of unstable volatiles.&lt;br /&gt;
* &#039;&#039;&#039;Core:&#039;&#039;&#039; Differentiated and semi-molten. Inner core of iron-nickel alloy spins at a different rate. Outer core is a highly viscous slurry of silicate, iron, carbon, sulfur, and dissolved volatiles. Chemical veins (e.g., uranium silicates, perovskites) act as mechanical shear zones. Tidal torque leads to periodic frictional heating.&lt;br /&gt;
&lt;br /&gt;
Tectonic and Cryovolcanic Behavior&lt;br /&gt;
* The planet resists tidal locking due to core-crust decoupling and uneven angular momentum transfer.&lt;br /&gt;
* High obliquity experiences &#039;&#039;&#039;&#039;&#039;Axial Recoil Events&#039;&#039;&#039;&#039;&#039;, where the entire planet jerks between metastable orientations (e.g., from 110° to 70°) in sudden spasms.&lt;br /&gt;
* These events generate:&lt;br /&gt;
** Global-scale crustal cracking&lt;br /&gt;
** Venting of pressurized subsurface gases (H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;O, CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt;)&lt;br /&gt;
** Surface deformation and glacial faulting&lt;br /&gt;
* Volatiles erupt ballistically into space (200+lm) from exposed fissures and calderas, driven by phase-change explosions.&lt;br /&gt;
&lt;br /&gt;
Surface Conditions&lt;br /&gt;
* Global temperature well below freezing; warmest zones around cryovolcanic hotspots&lt;br /&gt;
* Crustal coloration varies by volatile deposition:&lt;br /&gt;
** Pale blue-white from water ice&lt;br /&gt;
** Red-brown from CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; frostfields&lt;br /&gt;
** Green-black CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; stains from plume fallout&lt;br /&gt;
* Surface features include:&lt;br /&gt;
** Cryovolcanic calderas&lt;br /&gt;
** Diamond-studded impact-like basins&lt;br /&gt;
** Faulted plains crossed by salt-streaked rift zones&lt;br /&gt;
&lt;br /&gt;
Atmosphere and Ejected Material&lt;br /&gt;
* Thin transient exosphere formed from eruptive events&lt;br /&gt;
* Gases often escape to space or freeze back out in polar regions&lt;br /&gt;
* Fallback material creates uneven surface mass distributions, altering moment of inertia and prolonging instability&lt;br /&gt;
&lt;br /&gt;
Appearance from Planet c&lt;br /&gt;
&lt;br /&gt;
* Angular Size: ~4-1 arcminutes&lt;br /&gt;
* Coloration: Overall dusky grey-white, with changing colored bands due to volatile fallout; craterless but mottled&lt;br /&gt;
&lt;br /&gt;
Transient visible phenomena:&lt;br /&gt;
&lt;br /&gt;
* Cryovolcanic plumes visible as fan-like arcs at the limb during outburst events&lt;br /&gt;
* Infrared brightening during Axial Recoil Events&lt;br /&gt;
* Occasional light-scattering halos from plume particles&lt;br /&gt;
&lt;br /&gt;
Event Cycle Summary&lt;br /&gt;
&lt;br /&gt;
# Tidal torque builds due to obliquity misalignment&lt;br /&gt;
# Core resists, crust locks tension&lt;br /&gt;
# Critical stress threshold breached&lt;br /&gt;
# Obliquity lurches to new orientation&lt;br /&gt;
# Crust fractures globally, vents open&lt;br /&gt;
# Supersonic cryovolcanism hurls volatiles into space&lt;br /&gt;
# Fallback modifies crustal mass distribution&lt;br /&gt;
# Obliquity rebuilds instability over decades&lt;br /&gt;
# Repeat.&lt;br /&gt;
&lt;br /&gt;
Planet e is a tortured world caught in an unending cycle of self-correcting failure—its body unable to align, its gases unable to stay contained, its appearance in the sky a visible signature of internal catastrophe.&lt;br /&gt;
&lt;br /&gt;
==== f: Ringed Mini-Neptune ====&lt;br /&gt;
[[File:Ringed Neptune with four moons.png|thumb|right|Aperspectival view of f, its rings, and four moons]]&lt;br /&gt;
This planet is a substantial mini-Neptune, with a mass of approximately 3.5 Earth masses and a radius of 2.0 Earth radii, orbiting at 0.227 AU. Its low mean density (~0.44 ρ⊕) signals the presence of a deep, volatile-rich envelope overlying a denser core. The bulk of its volume is composed of hydrogen and helium, accreted from the protoplanetary disk, with trace amounts of methane (CH₄) and ammonia (NH₃)—gases that dominate its photochemical and radiative behavior. Beneath this envelope, the planet hosts a water–rock–metal core layered in complex phases, with high-pressure ices and possibly superionic water enveloping a metallic center.  Lower atmosphere reaches 300–500 K (27–227°C) near the bottom of the troposphere, depending on opacity and convection.&lt;br /&gt;
&lt;br /&gt;
Visually, the planet exhibits a blue-to-cyan atmospheric hue, governed by Rayleigh scattering and methane absorption in the red and near-infrared spectrum. While not as banded or storm-laced as Jupiter, it features broad zonal flows, high-altitude methane ice clouds, and long-lived anticyclonic storms akin to Neptune’s Great Dark Spot. Due to its tidal locking to the host star, the planet presents hemispheric climatic asymmetry: a sunlit dayside prone to atmospheric upwelling and cloud formation, and a cooler, darker nightside. While colder, the backside is not freezing— in the 150–250 K range, depending on circulation efficiency. Atmospheric circulation is dominated by slow, large-scale overturning cells, moderated by planetary-scale waves and a subdued Coriolis force. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Rings =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Ring!!	Range (Rₚ)!!	Approx.! Range (km)!!	Description&lt;br /&gt;
|-&lt;br /&gt;
! C&lt;br /&gt;
| 	1.5–1.65 Rₚ	||19,100–21,000	||Faint, dusty interior ring&lt;br /&gt;
|-&lt;br /&gt;
! B&lt;br /&gt;
| 	1.65–1.96 Rₚ	||21,000–25,000||	Bright, dense primary ring&lt;br /&gt;
|-&lt;br /&gt;
! Division&lt;br /&gt;
|	1.96–2.04 Rₚ ||25,000–26,000 || a low-density gap&lt;br /&gt;
|-&lt;br /&gt;
!  A&lt;br /&gt;
|	2.04–2.3 Rₚ||26,000–29,300||	Sharp-edged outer ring&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Moon !!	Orbit (km) !!	Orbit (Rₚ) !!	Diameter (km) !!	Type	!! Period !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! I&lt;br /&gt;
|	60,000	||4.7 Rₚ	||~400	||Rocky	|| 0.9 ||Cratered&lt;br /&gt;
|-&lt;br /&gt;
! II&lt;br /&gt;
| 	110,000	|| 8.6 Rₚ	|| ~800	|| Mixed rock/ice	|| 2.25|| Cracked surface, frozen ocean&lt;br /&gt;
|-&lt;br /&gt;
! III &lt;br /&gt;
| 190,000	|| 14.9 Rₚ ||	~1200 ||	Icy major moon ||	5.1|| Cryovolcanism, smooth plains&lt;br /&gt;
|-&lt;br /&gt;
! IV &lt;br /&gt;
|340,000	||26.7 Rₚ	||~200	||Irregular/prograde	|| 12.21 || Dark red/carbon, inclined (20º, eccentric orbit (0.1)&lt;br /&gt;
|-&lt;br /&gt;
! V &lt;br /&gt;
| 710,000 ||	55.7 Rₚ	||~350	|| Captured/retrograde	|| 36.83 || Highly inclined (130º), Split terrain—half rugged highlands, half smooth resurfaced plain&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==== g: Stripped Sub-Neptune Remnant ====&lt;br /&gt;
[[File:Stripped Planet with Two Cool Moons.png|700px|right]]&lt;br /&gt;
Basic Parameters&lt;br /&gt;
* Mass: 2.6 Earth masses (M⊕)&lt;br /&gt;
* Radius: 1.7 Earth radii (R⊕)&lt;br /&gt;
* Mean Density: ~2.92 g/cm³&lt;br /&gt;
* Orbital Distance: 0.4 AU &lt;br /&gt;
* Albedo: ~0.5 (moderately high)&lt;br /&gt;
* Rotation: Tidally locked &lt;br /&gt;
&lt;br /&gt;
Origin and Evolution&lt;br /&gt;
* Formed beyond the snow line (~0.8–1.2 AU) from a mix of rock, iron, and ices&lt;br /&gt;
* Migrated inward early during protoplanetary disk phase&lt;br /&gt;
* Accreted a modest hydrogen-helium envelope (&amp;gt;1% by mass)&lt;br /&gt;
* Exposed to intense stellar X-ray and UV radiation during the M dwarf&#039;s pre-main-sequence phase&lt;br /&gt;
* Lacked a magnetic dynamo (metal-poor and early core freezing)&lt;br /&gt;
* Entire atmosphere lost over ~100 Myr via photoevaporation, core-powered mass loss, and sputtering&lt;br /&gt;
&lt;br /&gt;
Current State&lt;br /&gt;
* Atmosphere: None (trace mineral vapors possible in hot regions)&lt;br /&gt;
* Surface: Stark contrast between hemispheres due to tidal locking&lt;br /&gt;
** Dayside: ~700–1000 K; high-silica lava fields, salt flats, exposed alumino-silicates&lt;br /&gt;
** Nightside: ~100–150 K; gypsum and calcite in cold traps, frozen regolith&lt;br /&gt;
* Magnetosphere: Absent&lt;br /&gt;
* Volcanism:episodic; high-silica flows, volcanic glass, sodium-rich crusts&lt;br /&gt;
* Geological Activity: Tectonically inactive; thermally fractured plains, impact craters&lt;br /&gt;
&lt;br /&gt;
Surface Composition&lt;br /&gt;
* Titanium dioxide (rutile): bright, high-albedo mineral condensate&lt;br /&gt;
* Calcite (CaCO₃): carbonate deposits in cold traps&lt;br /&gt;
* Gypsum (CaSO₄·2H₂O): hydration mineral, stable only on the nightside&lt;br /&gt;
* Sodium chloride: salt flats, especially in evaporated basins&lt;br /&gt;
* High-silica volcanic deposits: glassy, oxidized, and light-colored&lt;br /&gt;
&lt;br /&gt;
Visual and Observational Notes&lt;br /&gt;
&lt;br /&gt;
* High visual contrast between molten and frozen hemispheres&lt;br /&gt;
* Surface appears mottled: obsidian-black lava, gleaming salt flats, white calcium deposits&lt;br /&gt;
* No clouds, auroras, or magnetic activity&lt;br /&gt;
* Extreme day/night temperature gradient&lt;br /&gt;
* Reflective phase curve possible in photometric observations&lt;br /&gt;
* Surface pressure: effectively 0 bar&lt;br /&gt;
&lt;br /&gt;
Planet g is the airless skeleton of a once-sub-Neptune world. Born icy and distant, it migrated into the young star&#039;s wrath, where its fragile envelope boiled away under a sky of flares. Bereft of a magnetic shield, it was slowly stripped to bare rock. Today, one hemisphere bakes in molten silence while the other freezes in shadow. No air, no oceans, only salt, stone, and the echo of a lost atmosphere.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property !!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~75,000 km (~0.26 R&amp;lt;sub&amp;gt;hill&amp;lt;/sub&amp;gt;)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~1,400 km (~0.22 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass	&lt;br /&gt;
| ~0.01 M⊕ (~1.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~3.0 g/cm³ (rock–ice mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temp&lt;br /&gt;
|	~150–180 K&lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
| 0.20g&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere&lt;br /&gt;
|	Trace O₂, from radiolysis and outgassing&lt;br /&gt;
|-&lt;br /&gt;
! Subsurface Ocean&lt;br /&gt;
|	heated by tidal flexing&lt;br /&gt;
|-&lt;br /&gt;
! Surface Features	&lt;br /&gt;
|Fractured ice crust, chaos terrain, cryogeysers, lenticulae&lt;br /&gt;
|}&lt;br /&gt;
gI is a cracked glass orb, rimed with frost and laced with luminous fissures. Below its crust, tides flex a hidden ocean in rhythmic silence. Its faint oxygen exosphere is ghostly but present.  It is frosted quartz with cobwebbed streaks and mineral discoloration.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property!!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~150,000 km (~0.5 Rₕill)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~2,100 km (~0.33 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass&lt;br /&gt;
|	~0.035 M⊕ (~4.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~2.1 g/cm³ (icy-rocky mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes &lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
|	~0.35 g&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temperature&lt;br /&gt;
|	~115–130 K (pressure and greenhouse effects)&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere	&lt;br /&gt;
| ~0.18 bar N₂ + ~0.1 bar Ar + ~0.02 bar CH₄, minor CO, trace haze &lt;br /&gt;
|}&lt;br /&gt;
gII is a muted blue-green crescent veiled in gold. Its sky glows with the weight of argon and the shimmer of methane haze, and its surface smolders with the memory of internal warmth. Liquid hydrocarbons shine like ink in the basins, while glaciers ebb across the uplands. To the star it shows only one face, but beneath that still gaze lies the soft breath of a world more welcoming than its master.&lt;br /&gt;
&lt;br /&gt;
==== h ====&lt;br /&gt;
[[File:Twin Planet, red and blue.png|right|600px]]&lt;br /&gt;
h is a twin-planet system, 1.5 AU from the star, with a period of 4.1 years&lt;br /&gt;
&lt;br /&gt;
Mutual Orbital Configuration&lt;br /&gt;
* Type: True binary planet pair, gravitationally bound, equal mass&lt;br /&gt;
* Masses: 5.0 M⊕ each&lt;br /&gt;
* Radii: 2.3 R⊕ each&lt;br /&gt;
* Mutual Orbit: Essentially circular, ~1 million km separation (~8–10 planetary radii)&lt;br /&gt;
* Period (mutual orbit): ~4.5 days&lt;br /&gt;
* Orbital Plane: Perpendicular to system ecliptic &lt;br /&gt;
* Tidal State: Tidally locked to each other (mutual synchronous rotation)&lt;br /&gt;
&lt;br /&gt;
Planet A — &amp;quot;Sapphire&amp;quot;&lt;br /&gt;
* Coloration: Deep sapphire blue with white high-altitude methane ice hazes&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: H₂, He&lt;br /&gt;
** Methane (CH₄): high&lt;br /&gt;
** Ammonia: trace&lt;br /&gt;
** Argon: moderate&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: slightly enriched&lt;br /&gt;
* Magnetosphere: Strong, symmetric; supports brilliant blue-violet aurorae&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Superionic water mantle&lt;br /&gt;
** Stratified silicate-ice alloy core&lt;br /&gt;
** Radiogenic heating and layered convection&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar hexagonal jet (stronger than Saturn&#039;s)&lt;br /&gt;
** Methane plasma flares at terminator&lt;br /&gt;
** Iridescent methane cirrus clouds&lt;br /&gt;
** Massive auroral crowns aligned with spin-magnetic axis misalignment&lt;br /&gt;
&lt;br /&gt;
Planet B — &amp;quot;Rust&amp;quot;&lt;br /&gt;
* Coloration: Dark crimson to rust-red, streaked with black and violet haze bands&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: N₂, CO&lt;br /&gt;
** CH₄: trace&lt;br /&gt;
** Tholins: abundant&lt;br /&gt;
** Argon: high&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: moderate&lt;br /&gt;
** Magnetosphere: Weak, multipolar and intermittent&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Dense iron-rich core with impact inclusions (e.g., iridium, ruthenium)&lt;br /&gt;
** Volcanically active mantle with carbon-rich inclusions&lt;br /&gt;
** Higher internal heat flow than Sapphire&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar cyclonic basins with geyser-like haze columns&lt;br /&gt;
** Frequent UV lightning within organic clouds&lt;br /&gt;
** Faint auroral echoes from Sapphire’s magnetospheric tail&lt;br /&gt;
** Surface glow from argon emissions during conjunction&lt;br /&gt;
&lt;br /&gt;
Mutual Phenomena &amp;amp; Sky Effects&lt;br /&gt;
* Eclipse Cycles: Frequent, due to short mutual period and perpendicular orbit; cause wave-like haze patterns and shadow bands&lt;br /&gt;
* Filamentary Atmosphere Bridges: Transient stratospheric strands near L1, illuminated during eclipses&lt;br /&gt;
* Auroral Flux Tubes: Occasionally connect the two with violet-green flickering arcs&lt;br /&gt;
* Gravitational Stability: Mutual orbit stable within Hill sphere; resistant to long-term disruption&lt;br /&gt;
&lt;br /&gt;
* Legacy of the Comet Shield&lt;br /&gt;
* Each planet’s core contains embedded relics of the system’s ancient bombardment:&lt;br /&gt;
** Sapphire: interstellar dust, primordial isotopes, deep xenon pockets&lt;br /&gt;
** Rust: impact-derived siderophiles, compressed organics, rare isotopic anomalies&lt;br /&gt;
* Capture Events: Both planets have intercepted and redirected hundreds of large icy bodies over system history&lt;br /&gt;
&lt;br /&gt;
They each have 2 small irregular moons, &amp;lt;100 km diameter, retrograde, on distant orbits.  Negligible.&lt;br /&gt;
&lt;br /&gt;
== Planet C ==&lt;br /&gt;
[[File:Planet C and its tethered moon.png|right|700px]]&lt;br /&gt;
* With an albedo of 0.2, the global average temp is 263ºK.  Because of modest greenhouse effects, surface temperatures are higher, on the sun-side.&lt;br /&gt;
# Mass: 1.5M⊕&lt;br /&gt;
# Gravity: 1g⊕&lt;br /&gt;
# Radius = 1.225⊕, or 7805km&lt;br /&gt;
Terminator Zone&lt;br /&gt;
# +/-30º: 1.28 E8 km&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; (slightly less than all the land of the Earth)&lt;br /&gt;
# Escape velocity is 12.4km/s, 11% higher than Earth&lt;br /&gt;
# Orbital velocity is 8.79km/s&lt;br /&gt;
=== Atmosphere ===&lt;br /&gt;
Water content is low because&lt;br /&gt;
* Water vapor is a potent greenhouse gas; vast surface water can trap too much heat, especially near the substellar point.&lt;br /&gt;
* Water leads to climate homogenization&lt;br /&gt;
* Lack of exposed silicate rock: Necessary for carbon-silicate weathering feedback, which stabilizes climate on geological timescales.&lt;br /&gt;
Earth has ~1.4 billion km³ of water.  In our habitable zone, we have no more than 10% of that, or 100 million km³, though there is much more on the night side, both liquid and ice.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Factor !! Ɬiʔa atm !! Ɬiʔa % !! Earth atm !! Earth % !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! Total Pressure &lt;br /&gt;
| 1.6 atm || || 1.0 atm || || Enhanced convective heat transfer, increased IR trapping&lt;br /&gt;
|-&lt;br /&gt;
! Nitrogen (N₂) &lt;br /&gt;
| 1.00 || 62.50% || 0.7808 || 78.08% || Reduced; still inert, still dominant&lt;br /&gt;
|-&lt;br /&gt;
! Oxygen (O₂) &lt;br /&gt;
| 0.21 || 13.13% || 0.2095 || 20.95% || Earth-normal partial pressure &lt;br /&gt;
|-&lt;br /&gt;
! Argon (Ar)&lt;br /&gt;
| 0.40 || 25.00% || 0.0093 || 0.93% || Major heat distribution enhancement, inert&lt;br /&gt;
|-&lt;br /&gt;
! Krypton + Xenon&lt;br /&gt;
| 0.005 || 0.31% || trace || trace || High molecular mass → improved heat retention, still safe&lt;br /&gt;
|-&lt;br /&gt;
! CO₂&lt;br /&gt;
| 0.005 || 0.31% || 0.004 || 0.04% || slightly elevated; sub-greenhouse threshold&lt;br /&gt;
|-&lt;br /&gt;
! H₂O vapor &lt;br /&gt;
| 0.015 || ~1% || || 0-4% || Maintains greenhouse without excess moisture&lt;br /&gt;
|}&lt;br /&gt;
==== Atmospheric Effects on Clouds ====&lt;br /&gt;
# Increased Pressure (1.6 atm) compresses gases, raising the dew point at which water vapor condenses. Clouds form closer to the surface, and are denser than similar altitudes compared to Earth.&lt;br /&gt;
# Low Water Inventory (~20% of Earth&#039;s): less frequent and less massive cloud systems than on Earth, but still present—especially over &amp;quot;hotspots&amp;quot; on the day side.&lt;br /&gt;
# Tidally Locked Climate: Cloud formation concentrate along the substellar point, where warm, moist air rises and cools.&lt;br /&gt;
#* A permanent “eyewall” storm system has formed at the subsolar point, like a giant hurricane.&lt;br /&gt;
#* As air rises and is advected to the night side, thin cloud bands or ice hazes form as it descends and cools.&lt;br /&gt;
&lt;br /&gt;
Appearance:&lt;br /&gt;
* The presence of noble gases (Ar, Kr, Xe) and higher pressure enhance Mie scattering, making clouds appear whiter and more silvered, especially at sunrise/sunset boundaries.&lt;br /&gt;
* Night side clouds are thin, high-altitude icy sheets, glowing faintly in aurorae or thermal emissions.&lt;br /&gt;
&lt;br /&gt;
==== Sky Color ====&lt;br /&gt;
The color of the sky is shaped by Rayleigh scattering, which depends on:&lt;br /&gt;
# Molecular composition: Heavier gases like Ar, Kr, and Xe scatter light less efficiently than N₂.&lt;br /&gt;
# Spectral output of the star: the red dwarf emits predominantly infrared and red light, with very little blue or violet.&lt;br /&gt;
&lt;br /&gt;
Consequence:&lt;br /&gt;
* Even with atmospheric scattering, there is insufficient blue light in the stellar spectrum to produce a blue sky.&lt;br /&gt;
* Day sky would likely appear:&lt;br /&gt;
** Dark peach, dusky rose, or reddish beige near zenith,&lt;br /&gt;
** Grading to deep salmon or mauve near the horizon,&lt;br /&gt;
** A slight metallic sheen due to noble gas content and high pressure.&lt;br /&gt;
&lt;br /&gt;
Twilight &amp;amp; Limb Scattering:&lt;br /&gt;
* The terminator (twilight zone) sees a diffuse, ruddy light, scattering through haze and clouds into luminous reds, purples, and copper tones.&lt;br /&gt;
* Aurorae are spectacular on the night side, especially since stellar flares are frequent.&lt;br /&gt;
&lt;br /&gt;
==== Sound Propagation ====&lt;br /&gt;
: &#039;&#039;Sound is profoundly affected by atmospheric pressure and composition.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Compared to Earth:&lt;br /&gt;
* Higher pressure → greater air density → faster transmission of sound and less attenuation.&lt;br /&gt;
* Argon and Xenon are heavy gases, which:&lt;br /&gt;
** Lower the speed of sound relative to air at the same pressure (despite the pressure increase).&lt;br /&gt;
** Shift resonance frequencies downward, resulting in deeper, rounder sounds.&lt;br /&gt;
&lt;br /&gt;
Consequences:&lt;br /&gt;
* Voices sound subtly lower-pitched and richer, especially for consonants and low vowels.&lt;br /&gt;
* Ambient sounds (wind, water, animals) would carry farther and sound more muffled or sonorous.&lt;br /&gt;
* Music or speech would resonate more warmly, especially indoors or in enclosed spaces.&lt;br /&gt;
&lt;br /&gt;
In short: it sounds like it’s wrapped in velvet.&lt;br /&gt;
&lt;br /&gt;
==== Heat Transport to the Night Side ====&lt;br /&gt;
Mechanisms:&lt;br /&gt;
# Thick Atmosphere (1.6 atm) increases:&lt;br /&gt;
#* Advection efficiency: Warm air masses can move more heat horizontally.&lt;br /&gt;
#* Radiative time constant: The atmosphere holds heat longer before releasing it.&lt;br /&gt;
# Noble Gases (especially Kr/Xe):&lt;br /&gt;
#* High molecular mass → more IR opacity → trapping and radiating heat more evenly.&lt;br /&gt;
# Slow Rotation / Tidal Locking:&lt;br /&gt;
#* Global Hadley-like cells dominate circulation, carrying warm air from the day side to the night side and descending it there.&lt;br /&gt;
&lt;br /&gt;
Result:&lt;br /&gt;
* The night side is not so freezing.  Temperatures differ by tens of degrees, not hundreds.&lt;br /&gt;
* There are still ice caps and a cold deserts at the anti-stellar point, but not a glaciated wasteland.&lt;br /&gt;
&lt;br /&gt;
=== Magnetosphere ===&lt;br /&gt;
* Larger mass --&amp;gt; larger iron core, generating more internal heat&lt;br /&gt;
* Larger radius --&amp;gt; Vigorous convection in the core&lt;br /&gt;
* Tidal Flexing --&amp;gt; still drives magnetic activity&lt;br /&gt;
&lt;br /&gt;
# Aurorae at lower latitudes&lt;br /&gt;
## higher magnetic rigidity, wider magnetotail, and greater reconnection energy.&lt;br /&gt;
## Combined with a higher flux of stellar particles, this means:&lt;br /&gt;
### Auroral ovals expand, reaching mid-latitudes sometimes equator.&lt;br /&gt;
### The skies are alive with rippling green, violet, and crimson aurorae, especially on the night side.&lt;br /&gt;
### Daily auroral activity occur during stellar flare cycles.&lt;br /&gt;
# Compasses&lt;br /&gt;
## compasses respond more sharply, with:&lt;br /&gt;
### Faster alignment.&lt;br /&gt;
### Greater resistance to local perturbations.&lt;br /&gt;
## However, frequent magnetic storms from stellar activity cause sudden declinations, reversals, or local anomalies.  In short, lots of aurorae equals dead compasses at the same time.&lt;br /&gt;
# Magnetic Field Strength &amp;gt; 100 μT &lt;br /&gt;
# Electromagnetism is more basic than chemistry or almost any other natural philosophy&lt;br /&gt;
&lt;br /&gt;
=== Substellar Point ===&lt;br /&gt;
The maximum incoming flux is very nearly the same as Earth&#039;s solar constant (≈1361 W/m²), but concentrated over one point rather than averaged over a rotating sphere.  Temperatures should be above 500ºK most of the time.  &lt;br /&gt;
&lt;br /&gt;
The magnetic north is also here. The thick atmosphere prevents too much loss here, but &lt;br /&gt;
* Charged particle influx&lt;br /&gt;
** Maximized at the substellar point—intense auroral and energetic particle precipitation&lt;br /&gt;
* Atmospheric ionization&lt;br /&gt;
** Constant production of high-energy ions and NOx compounds—UV fluorescence in upper sky&lt;br /&gt;
* Localized heating&lt;br /&gt;
** Augments already extreme temperatures—600–700 K surface&lt;br /&gt;
&lt;br /&gt;
== Artificially Tethered Moon ==&lt;br /&gt;
* 670,000 km up&lt;br /&gt;
* 7805 km in radius = same as the planet&lt;br /&gt;
* 1.33º of the sky, same as the sun&lt;br /&gt;
&lt;br /&gt;
A network of tethers/tension lines from the moon to multiple anchor points on the planet’s surface (a tripod or hexapod structure), woven like hair&lt;br /&gt;
* Uses active tension management and orbital station-keeping to stabilize the moon&lt;br /&gt;
* Counterweights and inward-pointing mass drivers on the moon to oppose drift&lt;br /&gt;
&lt;br /&gt;
The tethers are not bearing the full weight, but merely damping drift, providing restoring force, and enabling long-term stability through active compensation.  The moon&lt;br /&gt;
* Blocks the worst of the heat&lt;br /&gt;
* Blocks the worst of the solar radiation&lt;br /&gt;
The moon has &lt;br /&gt;
* low mass&lt;br /&gt;
* high albedo - enormous reflectivity&lt;br /&gt;
* scatters charges particles, UV, X-rays, auroral flux tubes&lt;br /&gt;
* sunward - crazy hot, high emissivity&lt;br /&gt;
* earthward - crazy cool, low emissivity&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=File:Planet_C_and_its_tethered_moon.png&amp;diff=168168</id>
		<title>File:Planet C and its tethered moon.png</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=File:Planet_C_and_its_tethered_moon.png&amp;diff=168168"/>
		<updated>2025-03-28T01:41:58Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: AI is a powerful thing&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Summary ==&lt;br /&gt;
AI is a powerful thing&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168167</id>
		<title>Ɬiʔa/Conworlding</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168167"/>
		<updated>2025-03-28T01:03:30Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* h */ pic&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Star ==&lt;br /&gt;
Our star is a red-dwarf.&lt;br /&gt;
# Type: M5V&lt;br /&gt;
## M: This indicates it&#039;s a cool, red star with a surface temperature less than 3,500ºK&lt;br /&gt;
## 5: Within the M class, stars are further divided into subclasses 0-9, with 0 being the hottest and 9 the coolest. An M5 star is in the middle of this range.&lt;br /&gt;
## V: Denotes that it&#039;s a main sequence star, also known as a dwarf star&lt;br /&gt;
# Stellar luminosity (L*) ≈ 0.01 𝐿⊙ (1/100th Sol&#039;s brightness)&lt;br /&gt;
# Stellar mass (M*) ≈ 0.2 𝑀⊙ (1/5 the mass of Sol)&lt;br /&gt;
# Stellar radius (R*) ≈ 0.25 𝑅⊙ (1/4 as wide as Sol)&lt;br /&gt;
# Effective temperature (T*) ≈ 3500 K&lt;br /&gt;
​The habitable zone (a) is about square root of L* over L⊙, so ~0.1 AU.&lt;br /&gt;
&lt;br /&gt;
=== Solar System ===&lt;br /&gt;
There are seven planets in the system&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Planet !!	Mass (M🜨)!!	Radius (R🜨)!! Moons/Rings	!!Resonance !!	Semi-Major Axis (AU)!!	Rings !! Moons !! Period !! Size&lt;br /&gt;
|-&lt;br /&gt;
| b ||	2.17 ||	1.1 ||	No ||	2:3 with c	|| 0.0763 ||	No || No || 17.2 || 13.6&#039; to 1.5&#039;&lt;br /&gt;
|-&lt;br /&gt;
| c ||	1.5	 ||1.225 ||	1* ||	—	        || 0.100 || No || No || 25.8 || -&lt;br /&gt;
|-&lt;br /&gt;
| d ||	2.0	 ||1.4 ||No ||	2:3 with c	 ||0.131 ||	No || No || 38.7 || 13.1&#039; to 1.8&#039;&lt;br /&gt;
|-&lt;br /&gt;
| e ||	0.9 ||	1.0 || No	 ||	2:3 with d	 ||0.172 ||	No || No || 58 || 4.1&#039; to 1.1&#039;&lt;br /&gt;
|-&lt;br /&gt;
| f ||	3.5 ||	2.0 ||	Yes! ||	2:3 with e	 ||0.227 || Yes || Junk || 87 || 4.6&#039; to 1.8&#039;&lt;br /&gt;
|-&lt;br /&gt;
| g ||	2.6 ||	1.7 ||	2 ||	-	 ||0.40 ||	Yes || Junk || 206 || 1.6&#039; to 1.0&#039;&lt;br /&gt;
|-&lt;br /&gt;
| h ||	5.0x2 ||2.3x2 || yes	 || -	 ||1.5 ||	Yes || No || 1500 || 0.5&#039; 16.4&#039; apart (at max)&lt;br /&gt;
|}&lt;br /&gt;
==== b: super Mercury with a ring of fire  ====&lt;br /&gt;
[[File:planet b by GPT.png|thumb|right|An artistic rendering of planet b]]&lt;br /&gt;
b is a super-Mercury, tidally locked, and incredibly dense.  ~700ºK on the day side, ~50ºK on the night.  2.1 Earth Masses, 1.1 Earth radii (~7000km) in size.  Orbital period 17.2 days.  Density 9.0 g/cm&amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt;.  Gravity is ~1.8g.  &lt;br /&gt;
&lt;br /&gt;
The iron core is huge, being 75% of the mass.  A thin silicate mantle, with metallic plains and exhumed ultramafic crust, with frequent iron meteorite craters, lacking typical “stone” breccias.&lt;br /&gt;
&lt;br /&gt;
The night side is intense, as simple hydrocarbons (methane, ethane, propane) condense and freeze into layered deposits.  Complex organics (tholins, polycyclic aromatics) accumulate on the sea floor, under miles of nitrogen ice.  Massive slush layers slosh around above cryovolcanic brines of ammonia.&lt;br /&gt;
&lt;br /&gt;
There is a crucial layer of Superionic Ice XI above the core, which acts as an electromagnetic insulator, and ionic heat bridge.  The crust is ultramafic silicates (olivine, pyroxene, perovskite) riddled with with sulfide veins, iron alloys, and graphite networks.  The poles of the magnetosphere are sideways, like Uranus, with poles at the equator in the Terminator Zone.  Persistent surface charges develop, because the whole planet is basically a ginormous Leyden jar!&lt;br /&gt;
&lt;br /&gt;
A planetary flux rope forms and un-forms with the star and planet b.  This induces electric jets at the terminator.  This is where temps are Earth-like.  Hydrocarbons sublimate and eject into the atmosphere, even while aurorae come right down to the ground.  A small, low pressure atmosphere prevents photodissociation, even while electrothermal instabilities lift molecules, forming an anomalous haze, a standing, glowing ring.  Coronal events cause localized lightning geysers with magnetic arcing.&lt;br /&gt;
&lt;br /&gt;
In short, b is visible with a blinding bright sun side (glowing orange bronze), a utterly black night side, and a burning, glowing, erupting, arcing ring at the terminator (all colors).  At biggest, it&#039;s half the size of Earth&#039;s moon in the sky, shrinking down to a star at it&#039;s furthest away.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== d: the wet eye with depths ====&lt;br /&gt;
[[File:wet eye planet.png|thumb|right|An reasonable approximation of d&#039;s appearance]]&lt;br /&gt;
From the outside, d is a &amp;quot;wet eye&amp;quot; just outside the habitable zone.  It is a water world, twice the mass of Earth, 1.4 times the radius, tidally locked.  The substellar point is the only place without surface ice.  However, it is better to think of the planet top-to-bottom.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;atmosphere&#039;&#039;&#039; is tenuous, less than 0.2 bars.  It is thin, N₂-rich with traces of H₂O, NH₃ vapor, and transient geyser outputs.  It is highly UV-irradiated, and Mars-like in its inability to retain volatiles.&lt;br /&gt;
&lt;br /&gt;
Next, there is a &#039;&#039;&#039;surface ice shell&#039;&#039;&#039;, ~20 km of thick Ice I.  Swirling currents beneath have cracked continent-sized ice plates, similar to Europa&#039;s crust.  It is permanently frozen except at the substellar furnace.  It accumulates chemical stains, mineral deposits, and cryovolcanic eruption plumes.  Accumulations of complex hydrates—like methanol clathrates—precipitate out and form false reefs, rising like coral from beneath. Transient thermal vents push hot plumes into the thin air, freezing instantly and snowing down crystals that form mineral spires.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;subglacial ocean&#039;&#039;&#039; is hundreds of kilometers thick.  It is super-pressurized liquid H₂O mixed with NH₃, CH₃OH, H₂O₂, and trace salts.  The movement is slow, planetary-scale currents originating from the Furnace and Coriolis force.  Strong layers exist: the surface is oxidized; the abyssal layer is reducing.&lt;br /&gt;
&lt;br /&gt;
A new &amp;quot;surface&amp;quot; is next.  The &#039;&#039;&#039;Ice Mantle&#039;&#039;&#039; is solid Ice VI and VII.  There are massive, slowly shifting &amp;quot;sub-oceanic continents&amp;quot;. It is periodically fractured and resurfaced by cryoquakes and brine-driven eruptions.  Some regions have developed elevated domes or ridges, continental “shelves” under the ocean.&lt;br /&gt;
&lt;br /&gt;
Finally, underneath is the &#039;&#039;&#039;core&#039;&#039;&#039;. Temperatures exceed 2000–3000 K locally.  Pressures range from 100 to 300 GPa.  The core is rich in heavy elements.  This makes radiogenic hotspots, localized magnetic eddies.  Heat gradients + ion flows = thermoelectric currents.  These make magnetic storms within the ocean itself, not the sky.  When uranium-rich corium pods shift or explode upward through the mantle, their heat and conductivity disturb the local magnetic field, generating geomagnetic quakes.  These pulse through the ocean, creating short-lived magnetic lenses.  These interact with atmospheric charged particles above the Furnace, giving rise to transient magnetic halos visible from orbit—false auroras without a sunstorm.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== e: The Tortured Near-Sphere ====&lt;br /&gt;
[[File:Blasting and shattered.png|thumb|right|An axial recoil event in progress]]&lt;br /&gt;
Orbital and Physical Characteristics&lt;br /&gt;
* Mass: 0.9 Earth masses&lt;br /&gt;
* Radius: 1.0 Earth radii&lt;br /&gt;
* Orbital Period: 58 Earth days&lt;br /&gt;
* Surface Gravity: ~0.9 g&lt;br /&gt;
* Semimajor Axis: ~0.17 AU &lt;br /&gt;
* Spin State: In the &#039;&#039;process&#039;&#039; of becoming tidally locked&lt;br /&gt;
* Obliquity: Extreme, experiencing chaotic realignment events&lt;br /&gt;
&lt;br /&gt;
Internal Structure and Composition&lt;br /&gt;
* &#039;&#039;&#039;Crust:&#039;&#039;&#039; A thick, rigid outer shell of water ice I mixed with clathrates (CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; and CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; hydrates), underlain by layers of ammonia-water ice eutectics. Inclusions of carbon under extreme pressure form diamond strata in the lower crust, lending rigidity and brittle behavior.&lt;br /&gt;
* &#039;&#039;&#039;Mantle:&#039;&#039;&#039; Comprised of Ice VI and Ice VII, with ammonia- and methane-rich brines forming localized conduits and pockets of unstable volatiles.&lt;br /&gt;
* &#039;&#039;&#039;Core:&#039;&#039;&#039; Differentiated and semi-molten. Inner core of iron-nickel alloy spins at a different rate. Outer core is a highly viscous slurry of silicate, iron, carbon, sulfur, and dissolved volatiles. Chemical veins (e.g., uranium silicates, perovskites) act as mechanical shear zones. Tidal torque leads to periodic frictional heating.&lt;br /&gt;
&lt;br /&gt;
Tectonic and Cryovolcanic Behavior&lt;br /&gt;
* The planet resists tidal locking due to core-crust decoupling and uneven angular momentum transfer.&lt;br /&gt;
* High obliquity experiences &#039;&#039;&#039;&#039;&#039;Axial Recoil Events&#039;&#039;&#039;&#039;&#039;, where the entire planet jerks between metastable orientations (e.g., from 110° to 70°) in sudden spasms.&lt;br /&gt;
* These events generate:&lt;br /&gt;
** Global-scale crustal cracking&lt;br /&gt;
** Venting of pressurized subsurface gases (H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;O, CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt;)&lt;br /&gt;
** Surface deformation and glacial faulting&lt;br /&gt;
* Volatiles erupt ballistically into space (200+lm) from exposed fissures and calderas, driven by phase-change explosions.&lt;br /&gt;
&lt;br /&gt;
Surface Conditions&lt;br /&gt;
* Global temperature well below freezing; warmest zones around cryovolcanic hotspots&lt;br /&gt;
* Crustal coloration varies by volatile deposition:&lt;br /&gt;
** Pale blue-white from water ice&lt;br /&gt;
** Red-brown from CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; frostfields&lt;br /&gt;
** Green-black CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; stains from plume fallout&lt;br /&gt;
* Surface features include:&lt;br /&gt;
** Cryovolcanic calderas&lt;br /&gt;
** Diamond-studded impact-like basins&lt;br /&gt;
** Faulted plains crossed by salt-streaked rift zones&lt;br /&gt;
&lt;br /&gt;
Atmosphere and Ejected Material&lt;br /&gt;
* Thin transient exosphere formed from eruptive events&lt;br /&gt;
* Gases often escape to space or freeze back out in polar regions&lt;br /&gt;
* Fallback material creates uneven surface mass distributions, altering moment of inertia and prolonging instability&lt;br /&gt;
&lt;br /&gt;
Appearance from Planet c&lt;br /&gt;
&lt;br /&gt;
* Angular Size: ~4-1 arcminutes&lt;br /&gt;
* Coloration: Overall dusky grey-white, with changing colored bands due to volatile fallout; craterless but mottled&lt;br /&gt;
&lt;br /&gt;
Transient visible phenomena:&lt;br /&gt;
&lt;br /&gt;
* Cryovolcanic plumes visible as fan-like arcs at the limb during outburst events&lt;br /&gt;
* Infrared brightening during Axial Recoil Events&lt;br /&gt;
* Occasional light-scattering halos from plume particles&lt;br /&gt;
&lt;br /&gt;
Event Cycle Summary&lt;br /&gt;
&lt;br /&gt;
# Tidal torque builds due to obliquity misalignment&lt;br /&gt;
# Core resists, crust locks tension&lt;br /&gt;
# Critical stress threshold breached&lt;br /&gt;
# Obliquity lurches to new orientation&lt;br /&gt;
# Crust fractures globally, vents open&lt;br /&gt;
# Supersonic cryovolcanism hurls volatiles into space&lt;br /&gt;
# Fallback modifies crustal mass distribution&lt;br /&gt;
# Obliquity rebuilds instability over decades&lt;br /&gt;
# Repeat.&lt;br /&gt;
&lt;br /&gt;
Planet e is a tortured world caught in an unending cycle of self-correcting failure—its body unable to align, its gases unable to stay contained, its appearance in the sky a visible signature of internal catastrophe.&lt;br /&gt;
&lt;br /&gt;
==== f: Ringed Mini-Neptune ====&lt;br /&gt;
[[File:Ringed Neptune with four moons.png|thumb|right|Aperspectival view of f, its rings, and four moons]]&lt;br /&gt;
This planet is a substantial mini-Neptune, with a mass of approximately 3.5 Earth masses and a radius of 2.0 Earth radii, orbiting at 0.227 AU. Its low mean density (~0.44 ρ⊕) signals the presence of a deep, volatile-rich envelope overlying a denser core. The bulk of its volume is composed of hydrogen and helium, accreted from the protoplanetary disk, with trace amounts of methane (CH₄) and ammonia (NH₃)—gases that dominate its photochemical and radiative behavior. Beneath this envelope, the planet hosts a water–rock–metal core layered in complex phases, with high-pressure ices and possibly superionic water enveloping a metallic center.  Lower atmosphere reaches 300–500 K (27–227°C) near the bottom of the troposphere, depending on opacity and convection.&lt;br /&gt;
&lt;br /&gt;
Visually, the planet exhibits a blue-to-cyan atmospheric hue, governed by Rayleigh scattering and methane absorption in the red and near-infrared spectrum. While not as banded or storm-laced as Jupiter, it features broad zonal flows, high-altitude methane ice clouds, and long-lived anticyclonic storms akin to Neptune’s Great Dark Spot. Due to its tidal locking to the host star, the planet presents hemispheric climatic asymmetry: a sunlit dayside prone to atmospheric upwelling and cloud formation, and a cooler, darker nightside. While colder, the backside is not freezing— in the 150–250 K range, depending on circulation efficiency. Atmospheric circulation is dominated by slow, large-scale overturning cells, moderated by planetary-scale waves and a subdued Coriolis force. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Rings =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Ring!!	Range (Rₚ)!!	Approx.! Range (km)!!	Description&lt;br /&gt;
|-&lt;br /&gt;
! C&lt;br /&gt;
| 	1.5–1.65 Rₚ	||19,100–21,000	||Faint, dusty interior ring&lt;br /&gt;
|-&lt;br /&gt;
! B&lt;br /&gt;
| 	1.65–1.96 Rₚ	||21,000–25,000||	Bright, dense primary ring&lt;br /&gt;
|-&lt;br /&gt;
! Division&lt;br /&gt;
|	1.96–2.04 Rₚ ||25,000–26,000 || a low-density gap&lt;br /&gt;
|-&lt;br /&gt;
!  A&lt;br /&gt;
|	2.04–2.3 Rₚ||26,000–29,300||	Sharp-edged outer ring&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Moon !!	Orbit (km) !!	Orbit (Rₚ) !!	Diameter (km) !!	Type	!! Period !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! I&lt;br /&gt;
|	60,000	||4.7 Rₚ	||~400	||Rocky	|| 0.9 ||Cratered&lt;br /&gt;
|-&lt;br /&gt;
! II&lt;br /&gt;
| 	110,000	|| 8.6 Rₚ	|| ~800	|| Mixed rock/ice	|| 2.25|| Cracked surface, frozen ocean&lt;br /&gt;
|-&lt;br /&gt;
! III &lt;br /&gt;
| 190,000	|| 14.9 Rₚ ||	~1200 ||	Icy major moon ||	5.1|| Cryovolcanism, smooth plains&lt;br /&gt;
|-&lt;br /&gt;
! IV &lt;br /&gt;
|340,000	||26.7 Rₚ	||~200	||Irregular/prograde	|| 12.21 || Dark red/carbon, inclined (20º, eccentric orbit (0.1)&lt;br /&gt;
|-&lt;br /&gt;
! V &lt;br /&gt;
| 710,000 ||	55.7 Rₚ	||~350	|| Captured/retrograde	|| 36.83 || Highly inclined (130º), Split terrain—half rugged highlands, half smooth resurfaced plain&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==== g: Stripped Sub-Neptune Remnant ====&lt;br /&gt;
[[File:Stripped Planet with Two Cool Moons.png|700px|right]]&lt;br /&gt;
Basic Parameters&lt;br /&gt;
* Mass: 2.6 Earth masses (M⊕)&lt;br /&gt;
* Radius: 1.7 Earth radii (R⊕)&lt;br /&gt;
* Mean Density: ~2.92 g/cm³&lt;br /&gt;
* Orbital Distance: 0.4 AU &lt;br /&gt;
* Albedo: ~0.5 (moderately high)&lt;br /&gt;
* Rotation: Tidally locked &lt;br /&gt;
&lt;br /&gt;
Origin and Evolution&lt;br /&gt;
* Formed beyond the snow line (~0.8–1.2 AU) from a mix of rock, iron, and ices&lt;br /&gt;
* Migrated inward early during protoplanetary disk phase&lt;br /&gt;
* Accreted a modest hydrogen-helium envelope (&amp;gt;1% by mass)&lt;br /&gt;
* Exposed to intense stellar X-ray and UV radiation during the M dwarf&#039;s pre-main-sequence phase&lt;br /&gt;
* Lacked a magnetic dynamo (metal-poor and early core freezing)&lt;br /&gt;
* Entire atmosphere lost over ~100 Myr via photoevaporation, core-powered mass loss, and sputtering&lt;br /&gt;
&lt;br /&gt;
Current State&lt;br /&gt;
* Atmosphere: None (trace mineral vapors possible in hot regions)&lt;br /&gt;
* Surface: Stark contrast between hemispheres due to tidal locking&lt;br /&gt;
** Dayside: ~700–1000 K; high-silica lava fields, salt flats, exposed alumino-silicates&lt;br /&gt;
** Nightside: ~100–150 K; gypsum and calcite in cold traps, frozen regolith&lt;br /&gt;
* Magnetosphere: Absent&lt;br /&gt;
* Volcanism:episodic; high-silica flows, volcanic glass, sodium-rich crusts&lt;br /&gt;
* Geological Activity: Tectonically inactive; thermally fractured plains, impact craters&lt;br /&gt;
&lt;br /&gt;
Surface Composition&lt;br /&gt;
* Titanium dioxide (rutile): bright, high-albedo mineral condensate&lt;br /&gt;
* Calcite (CaCO₃): carbonate deposits in cold traps&lt;br /&gt;
* Gypsum (CaSO₄·2H₂O): hydration mineral, stable only on the nightside&lt;br /&gt;
* Sodium chloride: salt flats, especially in evaporated basins&lt;br /&gt;
* High-silica volcanic deposits: glassy, oxidized, and light-colored&lt;br /&gt;
&lt;br /&gt;
Visual and Observational Notes&lt;br /&gt;
&lt;br /&gt;
* High visual contrast between molten and frozen hemispheres&lt;br /&gt;
* Surface appears mottled: obsidian-black lava, gleaming salt flats, white calcium deposits&lt;br /&gt;
* No clouds, auroras, or magnetic activity&lt;br /&gt;
* Extreme day/night temperature gradient&lt;br /&gt;
* Reflective phase curve possible in photometric observations&lt;br /&gt;
* Surface pressure: effectively 0 bar&lt;br /&gt;
&lt;br /&gt;
Planet g is the airless skeleton of a once-sub-Neptune world. Born icy and distant, it migrated into the young star&#039;s wrath, where its fragile envelope boiled away under a sky of flares. Bereft of a magnetic shield, it was slowly stripped to bare rock. Today, one hemisphere bakes in molten silence while the other freezes in shadow. No air, no oceans, only salt, stone, and the echo of a lost atmosphere.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property !!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~75,000 km (~0.26 R&amp;lt;sub&amp;gt;hill&amp;lt;/sub&amp;gt;)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~1,400 km (~0.22 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass	&lt;br /&gt;
| ~0.01 M⊕ (~1.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~3.0 g/cm³ (rock–ice mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temp&lt;br /&gt;
|	~150–180 K&lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
| 0.20g&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere&lt;br /&gt;
|	Trace O₂, from radiolysis and outgassing&lt;br /&gt;
|-&lt;br /&gt;
! Subsurface Ocean&lt;br /&gt;
|	heated by tidal flexing&lt;br /&gt;
|-&lt;br /&gt;
! Surface Features	&lt;br /&gt;
|Fractured ice crust, chaos terrain, cryogeysers, lenticulae&lt;br /&gt;
|}&lt;br /&gt;
gI is a cracked glass orb, rimed with frost and laced with luminous fissures. Below its crust, tides flex a hidden ocean in rhythmic silence. Its faint oxygen exosphere is ghostly but present.  It is frosted quartz with cobwebbed streaks and mineral discoloration.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property!!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~150,000 km (~0.5 Rₕill)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~2,100 km (~0.33 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass&lt;br /&gt;
|	~0.035 M⊕ (~4.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~2.1 g/cm³ (icy-rocky mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes &lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
|	~0.35 g&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temperature&lt;br /&gt;
|	~115–130 K (pressure and greenhouse effects)&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere	&lt;br /&gt;
| ~0.18 bar N₂ + ~0.1 bar Ar + ~0.02 bar CH₄, minor CO, trace haze &lt;br /&gt;
|}&lt;br /&gt;
gII is a muted blue-green crescent veiled in gold. Its sky glows with the weight of argon and the shimmer of methane haze, and its surface smolders with the memory of internal warmth. Liquid hydrocarbons shine like ink in the basins, while glaciers ebb across the uplands. To the star it shows only one face, but beneath that still gaze lies the soft breath of a world more welcoming than its master.&lt;br /&gt;
&lt;br /&gt;
==== h ====&lt;br /&gt;
[[File:Twin Planet, red and blue.png|right|600px]]&lt;br /&gt;
h is a twin-planet system, 1.5 AU from the star, with a period of 4.1 years&lt;br /&gt;
&lt;br /&gt;
Mutual Orbital Configuration&lt;br /&gt;
* Type: True binary planet pair, gravitationally bound, equal mass&lt;br /&gt;
* Masses: 5.0 M⊕ each&lt;br /&gt;
* Radii: 2.3 R⊕ each&lt;br /&gt;
* Mutual Orbit: Essentially circular, ~1 million km separation (~8–10 planetary radii)&lt;br /&gt;
* Period (mutual orbit): ~4.5 days&lt;br /&gt;
* Orbital Plane: Perpendicular to system ecliptic &lt;br /&gt;
* Tidal State: Tidally locked to each other (mutual synchronous rotation)&lt;br /&gt;
&lt;br /&gt;
Planet A — &amp;quot;Sapphire&amp;quot;&lt;br /&gt;
* Coloration: Deep sapphire blue with white high-altitude methane ice hazes&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: H₂, He&lt;br /&gt;
** Methane (CH₄): high&lt;br /&gt;
** Ammonia: trace&lt;br /&gt;
** Argon: moderate&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: slightly enriched&lt;br /&gt;
* Magnetosphere: Strong, symmetric; supports brilliant blue-violet aurorae&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Superionic water mantle&lt;br /&gt;
** Stratified silicate-ice alloy core&lt;br /&gt;
** Radiogenic heating and layered convection&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar hexagonal jet (stronger than Saturn&#039;s)&lt;br /&gt;
** Methane plasma flares at terminator&lt;br /&gt;
** Iridescent methane cirrus clouds&lt;br /&gt;
** Massive auroral crowns aligned with spin-magnetic axis misalignment&lt;br /&gt;
&lt;br /&gt;
Planet B — &amp;quot;Rust&amp;quot;&lt;br /&gt;
* Coloration: Dark crimson to rust-red, streaked with black and violet haze bands&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: N₂, CO&lt;br /&gt;
** CH₄: trace&lt;br /&gt;
** Tholins: abundant&lt;br /&gt;
** Argon: high&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: moderate&lt;br /&gt;
** Magnetosphere: Weak, multipolar and intermittent&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Dense iron-rich core with impact inclusions (e.g., iridium, ruthenium)&lt;br /&gt;
** Volcanically active mantle with carbon-rich inclusions&lt;br /&gt;
** Higher internal heat flow than Sapphire&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar cyclonic basins with geyser-like haze columns&lt;br /&gt;
** Frequent UV lightning within organic clouds&lt;br /&gt;
** Faint auroral echoes from Sapphire’s magnetospheric tail&lt;br /&gt;
** Surface glow from argon emissions during conjunction&lt;br /&gt;
&lt;br /&gt;
Mutual Phenomena &amp;amp; Sky Effects&lt;br /&gt;
* Eclipse Cycles: Frequent, due to short mutual period and perpendicular orbit; cause wave-like haze patterns and shadow bands&lt;br /&gt;
* Filamentary Atmosphere Bridges: Transient stratospheric strands near L1, illuminated during eclipses&lt;br /&gt;
* Auroral Flux Tubes: Occasionally connect the two with violet-green flickering arcs&lt;br /&gt;
* Gravitational Stability: Mutual orbit stable within Hill sphere; resistant to long-term disruption&lt;br /&gt;
&lt;br /&gt;
* Legacy of the Comet Shield&lt;br /&gt;
* Each planet’s core contains embedded relics of the system’s ancient bombardment:&lt;br /&gt;
** Sapphire: interstellar dust, primordial isotopes, deep xenon pockets&lt;br /&gt;
** Rust: impact-derived siderophiles, compressed organics, rare isotopic anomalies&lt;br /&gt;
* Capture Events: Both planets have intercepted and redirected hundreds of large icy bodies over system history&lt;br /&gt;
&lt;br /&gt;
They each have 2 small irregular moons, &amp;lt;100 km diameter, retrograde, on distant orbits.  Negligible.&lt;br /&gt;
&lt;br /&gt;
== Planet C ==&lt;br /&gt;
&lt;br /&gt;
* With an albedo of 0.2, the global average temp is 263ºK.  Because of modest greenhouse effects, surface temperatures are higher, on the sun-side.&lt;br /&gt;
# Mass: 1.5M⊕&lt;br /&gt;
# Gravity: 1g⊕&lt;br /&gt;
# Radius = 1.225⊕, or 7805km&lt;br /&gt;
Terminator Zone&lt;br /&gt;
# +/-30º: 1.28 E8 km&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; (slightly less than all the land of the Earth)&lt;br /&gt;
# Escape velocity is 12.4km/s, 11% higher than Earth&lt;br /&gt;
# Orbital velocity is 8.79km/s&lt;br /&gt;
=== Atmosphere ===&lt;br /&gt;
Water content is low because&lt;br /&gt;
* Water vapor is a potent greenhouse gas; vast surface water can trap too much heat, especially near the substellar point.&lt;br /&gt;
* Water leads to climate homogenization&lt;br /&gt;
* Lack of exposed silicate rock: Necessary for carbon-silicate weathering feedback, which stabilizes climate on geological timescales.&lt;br /&gt;
Earth has ~1.4 billion km³ of water.  In our habitable zone, we have no more than 10% of that, or 100 million km³, though there is much more on the night side, both liquid and ice.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Factor !! Ɬiʔa atm !! Ɬiʔa % !! Earth atm !! Earth % !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! Total Pressure &lt;br /&gt;
| 1.6 atm || || 1.0 atm || || Enhanced convective heat transfer, increased IR trapping&lt;br /&gt;
|-&lt;br /&gt;
! Nitrogen (N₂) &lt;br /&gt;
| 1.00 || 62.50% || 0.7808 || 78.08% || Reduced; still inert, still dominant&lt;br /&gt;
|-&lt;br /&gt;
! Oxygen (O₂) &lt;br /&gt;
| 0.21 || 13.13% || 0.2095 || 20.95% || Earth-normal partial pressure &lt;br /&gt;
|-&lt;br /&gt;
! Argon (Ar)&lt;br /&gt;
| 0.40 || 25.00% || 0.0093 || 0.93% || Major heat distribution enhancement, inert&lt;br /&gt;
|-&lt;br /&gt;
! Krypton + Xenon&lt;br /&gt;
| 0.005 || 0.31% || trace || trace || High molecular mass → improved heat retention, still safe&lt;br /&gt;
|-&lt;br /&gt;
! CO₂&lt;br /&gt;
| 0.005 || 0.31% || 0.004 || 0.04% || slightly elevated; sub-greenhouse threshold&lt;br /&gt;
|-&lt;br /&gt;
! H₂O vapor &lt;br /&gt;
| 0.015 || ~1% || || 0-4% || Maintains greenhouse without excess moisture&lt;br /&gt;
|}&lt;br /&gt;
==== Atmospheric Effects on Clouds ====&lt;br /&gt;
# Increased Pressure (1.6 atm) compresses gases, raising the dew point at which water vapor condenses. Clouds form closer to the surface, and are denser than similar altitudes compared to Earth.&lt;br /&gt;
# Low Water Inventory (~20% of Earth&#039;s): less frequent and less massive cloud systems than on Earth, but still present—especially over &amp;quot;hotspots&amp;quot; on the day side.&lt;br /&gt;
# Tidally Locked Climate: Cloud formation concentrate along the substellar point, where warm, moist air rises and cools.&lt;br /&gt;
#* A permanent “eyewall” storm system has formed at the subsolar point, like a giant hurricane.&lt;br /&gt;
#* As air rises and is advected to the night side, thin cloud bands or ice hazes form as it descends and cools.&lt;br /&gt;
&lt;br /&gt;
Appearance:&lt;br /&gt;
* The presence of noble gases (Ar, Kr, Xe) and higher pressure enhance Mie scattering, making clouds appear whiter and more silvered, especially at sunrise/sunset boundaries.&lt;br /&gt;
* Night side clouds are thin, high-altitude icy sheets, glowing faintly in aurorae or thermal emissions.&lt;br /&gt;
&lt;br /&gt;
==== Sky Color ====&lt;br /&gt;
The color of the sky is shaped by Rayleigh scattering, which depends on:&lt;br /&gt;
# Molecular composition: Heavier gases like Ar, Kr, and Xe scatter light less efficiently than N₂.&lt;br /&gt;
# Spectral output of the star: the red dwarf emits predominantly infrared and red light, with very little blue or violet.&lt;br /&gt;
&lt;br /&gt;
Consequence:&lt;br /&gt;
* Even with atmospheric scattering, there is insufficient blue light in the stellar spectrum to produce a blue sky.&lt;br /&gt;
* Day sky would likely appear:&lt;br /&gt;
** Dark peach, dusky rose, or reddish beige near zenith,&lt;br /&gt;
** Grading to deep salmon or mauve near the horizon,&lt;br /&gt;
** A slight metallic sheen due to noble gas content and high pressure.&lt;br /&gt;
&lt;br /&gt;
Twilight &amp;amp; Limb Scattering:&lt;br /&gt;
* The terminator (twilight zone) sees a diffuse, ruddy light, scattering through haze and clouds into luminous reds, purples, and copper tones.&lt;br /&gt;
* Aurorae are spectacular on the night side, especially since stellar flares are frequent.&lt;br /&gt;
&lt;br /&gt;
==== Sound Propagation ====&lt;br /&gt;
: &#039;&#039;Sound is profoundly affected by atmospheric pressure and composition.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Compared to Earth:&lt;br /&gt;
* Higher pressure → greater air density → faster transmission of sound and less attenuation.&lt;br /&gt;
* Argon and Xenon are heavy gases, which:&lt;br /&gt;
** Lower the speed of sound relative to air at the same pressure (despite the pressure increase).&lt;br /&gt;
** Shift resonance frequencies downward, resulting in deeper, rounder sounds.&lt;br /&gt;
&lt;br /&gt;
Consequences:&lt;br /&gt;
* Voices sound subtly lower-pitched and richer, especially for consonants and low vowels.&lt;br /&gt;
* Ambient sounds (wind, water, animals) would carry farther and sound more muffled or sonorous.&lt;br /&gt;
* Music or speech would resonate more warmly, especially indoors or in enclosed spaces.&lt;br /&gt;
&lt;br /&gt;
In short: it sounds like it’s wrapped in velvet.&lt;br /&gt;
&lt;br /&gt;
==== Heat Transport to the Night Side ====&lt;br /&gt;
Mechanisms:&lt;br /&gt;
# Thick Atmosphere (1.6 atm) increases:&lt;br /&gt;
#* Advection efficiency: Warm air masses can move more heat horizontally.&lt;br /&gt;
#* Radiative time constant: The atmosphere holds heat longer before releasing it.&lt;br /&gt;
# Noble Gases (especially Kr/Xe):&lt;br /&gt;
#* High molecular mass → more IR opacity → trapping and radiating heat more evenly.&lt;br /&gt;
# Slow Rotation / Tidal Locking:&lt;br /&gt;
#* Global Hadley-like cells dominate circulation, carrying warm air from the day side to the night side and descending it there.&lt;br /&gt;
&lt;br /&gt;
Result:&lt;br /&gt;
* The night side is not so freezing.  Temperatures differ by tens of degrees, not hundreds.&lt;br /&gt;
* There are still ice caps and a cold deserts at the anti-stellar point, but not a glaciated wasteland.&lt;br /&gt;
&lt;br /&gt;
=== Magnetosphere ===&lt;br /&gt;
* Larger mass --&amp;gt; larger iron core, generating more internal heat&lt;br /&gt;
* Larger radius --&amp;gt; Vigorous convection in the core&lt;br /&gt;
* Tidal Flexing --&amp;gt; still drives magnetic activity&lt;br /&gt;
&lt;br /&gt;
# Aurorae at lower latitudes&lt;br /&gt;
## higher magnetic rigidity, wider magnetotail, and greater reconnection energy.&lt;br /&gt;
## Combined with a higher flux of stellar particles, this means:&lt;br /&gt;
### Auroral ovals expand, reaching mid-latitudes sometimes equator.&lt;br /&gt;
### The skies are alive with rippling green, violet, and crimson aurorae, especially on the night side.&lt;br /&gt;
### Daily auroral activity occur during stellar flare cycles.&lt;br /&gt;
# Compasses&lt;br /&gt;
## compasses respond more sharply, with:&lt;br /&gt;
### Faster alignment.&lt;br /&gt;
### Greater resistance to local perturbations.&lt;br /&gt;
## However, frequent magnetic storms from stellar activity cause sudden declinations, reversals, or local anomalies.  In short, lots of aurorae equals dead compasses at the same time.&lt;br /&gt;
# Magnetic Field Strength &amp;gt; 100 μT &lt;br /&gt;
# Electromagnetism is more basic than chemistry or almost any other natural philosophy&lt;br /&gt;
&lt;br /&gt;
=== Substellar Point ===&lt;br /&gt;
The maximum incoming flux is very nearly the same as Earth&#039;s solar constant (≈1361 W/m²), but concentrated over one point rather than averaged over a rotating sphere.  Temperatures should be above 500ºK most of the time.  &lt;br /&gt;
&lt;br /&gt;
The magnetic north is also here. The thick atmosphere prevents too much loss here, but &lt;br /&gt;
* Charged particle influx&lt;br /&gt;
** Maximized at the substellar point—intense auroral and energetic particle precipitation&lt;br /&gt;
* Atmospheric ionization&lt;br /&gt;
** Constant production of high-energy ions and NOx compounds—UV fluorescence in upper sky&lt;br /&gt;
* Localized heating&lt;br /&gt;
** Augments already extreme temperatures—600–700 K surface&lt;br /&gt;
&lt;br /&gt;
== Artificially Tethered Moon ==&lt;br /&gt;
* 670,000 km up&lt;br /&gt;
* 7805 km in radius = same as the planet&lt;br /&gt;
* 1.33º of the sky, same as the sun&lt;br /&gt;
&lt;br /&gt;
A network of tethers/tension lines from the moon to multiple anchor points on the planet’s surface (a tripod or hexapod structure), woven like hair&lt;br /&gt;
* Uses active tension management and orbital station-keeping to stabilize the moon&lt;br /&gt;
* Counterweights and inward-pointing mass drivers on the moon to oppose drift&lt;br /&gt;
&lt;br /&gt;
The tethers are not bearing the full weight, but merely damping drift, providing restoring force, and enabling long-term stability through active compensation.  The moon&lt;br /&gt;
* Blocks the worst of the heat&lt;br /&gt;
* Blocks the worst of the solar radiation&lt;br /&gt;
The moon has &lt;br /&gt;
* low mass&lt;br /&gt;
* high albedo - enormous reflectivity&lt;br /&gt;
* scatters charges particles, UV, X-rays, auroral flux tubes&lt;br /&gt;
* sunward - crazy hot, high emissivity&lt;br /&gt;
* earthward - crazy cool, low emissivity&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=File:Twin_Planet,_red_and_blue.png&amp;diff=168166</id>
		<title>File:Twin Planet, red and blue.png</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=File:Twin_Planet,_red_and_blue.png&amp;diff=168166"/>
		<updated>2025-03-28T01:02:58Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: Twin exoplanets, orbiting a common barycenter&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Summary ==&lt;br /&gt;
Twin exoplanets, orbiting a common barycenter&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168165</id>
		<title>Ɬiʔa/Conworlding</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168165"/>
		<updated>2025-03-27T23:55:43Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* g: Stripped Sub-Neptune Remnant */ pic&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Star ==&lt;br /&gt;
Our star is a red-dwarf.&lt;br /&gt;
# Type: M5V&lt;br /&gt;
## M: This indicates it&#039;s a cool, red star with a surface temperature less than 3,500ºK&lt;br /&gt;
## 5: Within the M class, stars are further divided into subclasses 0-9, with 0 being the hottest and 9 the coolest. An M5 star is in the middle of this range.&lt;br /&gt;
## V: Denotes that it&#039;s a main sequence star, also known as a dwarf star&lt;br /&gt;
# Stellar luminosity (L*) ≈ 0.01 𝐿⊙ (1/100th Sol&#039;s brightness)&lt;br /&gt;
# Stellar mass (M*) ≈ 0.2 𝑀⊙ (1/5 the mass of Sol)&lt;br /&gt;
# Stellar radius (R*) ≈ 0.25 𝑅⊙ (1/4 as wide as Sol)&lt;br /&gt;
# Effective temperature (T*) ≈ 3500 K&lt;br /&gt;
​The habitable zone (a) is about square root of L* over L⊙, so ~0.1 AU.&lt;br /&gt;
&lt;br /&gt;
=== Solar System ===&lt;br /&gt;
There are seven planets in the system&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Planet !!	Mass (M🜨)!!	Radius (R🜨)!! Moons/Rings	!!Resonance !!	Semi-Major Axis (AU)!!	Rings !! Moons !! Period !! Size&lt;br /&gt;
|-&lt;br /&gt;
| b ||	2.17 ||	1.1 ||	No ||	2:3 with c	|| 0.0763 ||	No || No || 17.2 || 13.6&#039; to 1.5&#039;&lt;br /&gt;
|-&lt;br /&gt;
| c ||	1.5	 ||1.225 ||	1* ||	—	        || 0.100 || No || No || 25.8 || -&lt;br /&gt;
|-&lt;br /&gt;
| d ||	2.0	 ||1.4 ||No ||	2:3 with c	 ||0.131 ||	No || No || 38.7 || 13.1&#039; to 1.8&#039;&lt;br /&gt;
|-&lt;br /&gt;
| e ||	0.9 ||	1.0 || No	 ||	2:3 with d	 ||0.172 ||	No || No || 58 || 4.1&#039; to 1.1&#039;&lt;br /&gt;
|-&lt;br /&gt;
| f ||	3.5 ||	2.0 ||	Yes! ||	2:3 with e	 ||0.227 || Yes || Junk || 87 || 4.6&#039; to 1.8&#039;&lt;br /&gt;
|-&lt;br /&gt;
| g ||	2.6 ||	1.7 ||	2 ||	-	 ||0.40 ||	Yes || Junk || 206 || 1.6&#039; to 1.0&#039;&lt;br /&gt;
|-&lt;br /&gt;
| h ||	5.0x2 ||2.3x2 || yes	 || -	 ||1.5 ||	Yes || No || 1500 || 0.5&#039; 16.4&#039; apart (at max)&lt;br /&gt;
|}&lt;br /&gt;
==== b: super Mercury with a ring of fire  ====&lt;br /&gt;
[[File:planet b by GPT.png|thumb|right|An artistic rendering of planet b]]&lt;br /&gt;
b is a super-Mercury, tidally locked, and incredibly dense.  ~700ºK on the day side, ~50ºK on the night.  2.1 Earth Masses, 1.1 Earth radii (~7000km) in size.  Orbital period 17.2 days.  Density 9.0 g/cm&amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt;.  Gravity is ~1.8g.  &lt;br /&gt;
&lt;br /&gt;
The iron core is huge, being 75% of the mass.  A thin silicate mantle, with metallic plains and exhumed ultramafic crust, with frequent iron meteorite craters, lacking typical “stone” breccias.&lt;br /&gt;
&lt;br /&gt;
The night side is intense, as simple hydrocarbons (methane, ethane, propane) condense and freeze into layered deposits.  Complex organics (tholins, polycyclic aromatics) accumulate on the sea floor, under miles of nitrogen ice.  Massive slush layers slosh around above cryovolcanic brines of ammonia.&lt;br /&gt;
&lt;br /&gt;
There is a crucial layer of Superionic Ice XI above the core, which acts as an electromagnetic insulator, and ionic heat bridge.  The crust is ultramafic silicates (olivine, pyroxene, perovskite) riddled with with sulfide veins, iron alloys, and graphite networks.  The poles of the magnetosphere are sideways, like Uranus, with poles at the equator in the Terminator Zone.  Persistent surface charges develop, because the whole planet is basically a ginormous Leyden jar!&lt;br /&gt;
&lt;br /&gt;
A planetary flux rope forms and un-forms with the star and planet b.  This induces electric jets at the terminator.  This is where temps are Earth-like.  Hydrocarbons sublimate and eject into the atmosphere, even while aurorae come right down to the ground.  A small, low pressure atmosphere prevents photodissociation, even while electrothermal instabilities lift molecules, forming an anomalous haze, a standing, glowing ring.  Coronal events cause localized lightning geysers with magnetic arcing.&lt;br /&gt;
&lt;br /&gt;
In short, b is visible with a blinding bright sun side (glowing orange bronze), a utterly black night side, and a burning, glowing, erupting, arcing ring at the terminator (all colors).  At biggest, it&#039;s half the size of Earth&#039;s moon in the sky, shrinking down to a star at it&#039;s furthest away.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== d: the wet eye with depths ====&lt;br /&gt;
[[File:wet eye planet.png|thumb|right|An reasonable approximation of d&#039;s appearance]]&lt;br /&gt;
From the outside, d is a &amp;quot;wet eye&amp;quot; just outside the habitable zone.  It is a water world, twice the mass of Earth, 1.4 times the radius, tidally locked.  The substellar point is the only place without surface ice.  However, it is better to think of the planet top-to-bottom.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;atmosphere&#039;&#039;&#039; is tenuous, less than 0.2 bars.  It is thin, N₂-rich with traces of H₂O, NH₃ vapor, and transient geyser outputs.  It is highly UV-irradiated, and Mars-like in its inability to retain volatiles.&lt;br /&gt;
&lt;br /&gt;
Next, there is a &#039;&#039;&#039;surface ice shell&#039;&#039;&#039;, ~20 km of thick Ice I.  Swirling currents beneath have cracked continent-sized ice plates, similar to Europa&#039;s crust.  It is permanently frozen except at the substellar furnace.  It accumulates chemical stains, mineral deposits, and cryovolcanic eruption plumes.  Accumulations of complex hydrates—like methanol clathrates—precipitate out and form false reefs, rising like coral from beneath. Transient thermal vents push hot plumes into the thin air, freezing instantly and snowing down crystals that form mineral spires.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;subglacial ocean&#039;&#039;&#039; is hundreds of kilometers thick.  It is super-pressurized liquid H₂O mixed with NH₃, CH₃OH, H₂O₂, and trace salts.  The movement is slow, planetary-scale currents originating from the Furnace and Coriolis force.  Strong layers exist: the surface is oxidized; the abyssal layer is reducing.&lt;br /&gt;
&lt;br /&gt;
A new &amp;quot;surface&amp;quot; is next.  The &#039;&#039;&#039;Ice Mantle&#039;&#039;&#039; is solid Ice VI and VII.  There are massive, slowly shifting &amp;quot;sub-oceanic continents&amp;quot;. It is periodically fractured and resurfaced by cryoquakes and brine-driven eruptions.  Some regions have developed elevated domes or ridges, continental “shelves” under the ocean.&lt;br /&gt;
&lt;br /&gt;
Finally, underneath is the &#039;&#039;&#039;core&#039;&#039;&#039;. Temperatures exceed 2000–3000 K locally.  Pressures range from 100 to 300 GPa.  The core is rich in heavy elements.  This makes radiogenic hotspots, localized magnetic eddies.  Heat gradients + ion flows = thermoelectric currents.  These make magnetic storms within the ocean itself, not the sky.  When uranium-rich corium pods shift or explode upward through the mantle, their heat and conductivity disturb the local magnetic field, generating geomagnetic quakes.  These pulse through the ocean, creating short-lived magnetic lenses.  These interact with atmospheric charged particles above the Furnace, giving rise to transient magnetic halos visible from orbit—false auroras without a sunstorm.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== e: The Tortured Near-Sphere ====&lt;br /&gt;
[[File:Blasting and shattered.png|thumb|right|An axial recoil event in progress]]&lt;br /&gt;
Orbital and Physical Characteristics&lt;br /&gt;
* Mass: 0.9 Earth masses&lt;br /&gt;
* Radius: 1.0 Earth radii&lt;br /&gt;
* Orbital Period: 58 Earth days&lt;br /&gt;
* Surface Gravity: ~0.9 g&lt;br /&gt;
* Semimajor Axis: ~0.17 AU &lt;br /&gt;
* Spin State: In the &#039;&#039;process&#039;&#039; of becoming tidally locked&lt;br /&gt;
* Obliquity: Extreme, experiencing chaotic realignment events&lt;br /&gt;
&lt;br /&gt;
Internal Structure and Composition&lt;br /&gt;
* &#039;&#039;&#039;Crust:&#039;&#039;&#039; A thick, rigid outer shell of water ice I mixed with clathrates (CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; and CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; hydrates), underlain by layers of ammonia-water ice eutectics. Inclusions of carbon under extreme pressure form diamond strata in the lower crust, lending rigidity and brittle behavior.&lt;br /&gt;
* &#039;&#039;&#039;Mantle:&#039;&#039;&#039; Comprised of Ice VI and Ice VII, with ammonia- and methane-rich brines forming localized conduits and pockets of unstable volatiles.&lt;br /&gt;
* &#039;&#039;&#039;Core:&#039;&#039;&#039; Differentiated and semi-molten. Inner core of iron-nickel alloy spins at a different rate. Outer core is a highly viscous slurry of silicate, iron, carbon, sulfur, and dissolved volatiles. Chemical veins (e.g., uranium silicates, perovskites) act as mechanical shear zones. Tidal torque leads to periodic frictional heating.&lt;br /&gt;
&lt;br /&gt;
Tectonic and Cryovolcanic Behavior&lt;br /&gt;
* The planet resists tidal locking due to core-crust decoupling and uneven angular momentum transfer.&lt;br /&gt;
* High obliquity experiences &#039;&#039;&#039;&#039;&#039;Axial Recoil Events&#039;&#039;&#039;&#039;&#039;, where the entire planet jerks between metastable orientations (e.g., from 110° to 70°) in sudden spasms.&lt;br /&gt;
* These events generate:&lt;br /&gt;
** Global-scale crustal cracking&lt;br /&gt;
** Venting of pressurized subsurface gases (H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;O, CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt;)&lt;br /&gt;
** Surface deformation and glacial faulting&lt;br /&gt;
* Volatiles erupt ballistically into space (200+lm) from exposed fissures and calderas, driven by phase-change explosions.&lt;br /&gt;
&lt;br /&gt;
Surface Conditions&lt;br /&gt;
* Global temperature well below freezing; warmest zones around cryovolcanic hotspots&lt;br /&gt;
* Crustal coloration varies by volatile deposition:&lt;br /&gt;
** Pale blue-white from water ice&lt;br /&gt;
** Red-brown from CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; frostfields&lt;br /&gt;
** Green-black CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; stains from plume fallout&lt;br /&gt;
* Surface features include:&lt;br /&gt;
** Cryovolcanic calderas&lt;br /&gt;
** Diamond-studded impact-like basins&lt;br /&gt;
** Faulted plains crossed by salt-streaked rift zones&lt;br /&gt;
&lt;br /&gt;
Atmosphere and Ejected Material&lt;br /&gt;
* Thin transient exosphere formed from eruptive events&lt;br /&gt;
* Gases often escape to space or freeze back out in polar regions&lt;br /&gt;
* Fallback material creates uneven surface mass distributions, altering moment of inertia and prolonging instability&lt;br /&gt;
&lt;br /&gt;
Appearance from Planet c&lt;br /&gt;
&lt;br /&gt;
* Angular Size: ~4-1 arcminutes&lt;br /&gt;
* Coloration: Overall dusky grey-white, with changing colored bands due to volatile fallout; craterless but mottled&lt;br /&gt;
&lt;br /&gt;
Transient visible phenomena:&lt;br /&gt;
&lt;br /&gt;
* Cryovolcanic plumes visible as fan-like arcs at the limb during outburst events&lt;br /&gt;
* Infrared brightening during Axial Recoil Events&lt;br /&gt;
* Occasional light-scattering halos from plume particles&lt;br /&gt;
&lt;br /&gt;
Event Cycle Summary&lt;br /&gt;
&lt;br /&gt;
# Tidal torque builds due to obliquity misalignment&lt;br /&gt;
# Core resists, crust locks tension&lt;br /&gt;
# Critical stress threshold breached&lt;br /&gt;
# Obliquity lurches to new orientation&lt;br /&gt;
# Crust fractures globally, vents open&lt;br /&gt;
# Supersonic cryovolcanism hurls volatiles into space&lt;br /&gt;
# Fallback modifies crustal mass distribution&lt;br /&gt;
# Obliquity rebuilds instability over decades&lt;br /&gt;
# Repeat.&lt;br /&gt;
&lt;br /&gt;
Planet e is a tortured world caught in an unending cycle of self-correcting failure—its body unable to align, its gases unable to stay contained, its appearance in the sky a visible signature of internal catastrophe.&lt;br /&gt;
&lt;br /&gt;
==== f: Ringed Mini-Neptune ====&lt;br /&gt;
[[File:Ringed Neptune with four moons.png|thumb|right|Aperspectival view of f, its rings, and four moons]]&lt;br /&gt;
This planet is a substantial mini-Neptune, with a mass of approximately 3.5 Earth masses and a radius of 2.0 Earth radii, orbiting at 0.227 AU. Its low mean density (~0.44 ρ⊕) signals the presence of a deep, volatile-rich envelope overlying a denser core. The bulk of its volume is composed of hydrogen and helium, accreted from the protoplanetary disk, with trace amounts of methane (CH₄) and ammonia (NH₃)—gases that dominate its photochemical and radiative behavior. Beneath this envelope, the planet hosts a water–rock–metal core layered in complex phases, with high-pressure ices and possibly superionic water enveloping a metallic center.  Lower atmosphere reaches 300–500 K (27–227°C) near the bottom of the troposphere, depending on opacity and convection.&lt;br /&gt;
&lt;br /&gt;
Visually, the planet exhibits a blue-to-cyan atmospheric hue, governed by Rayleigh scattering and methane absorption in the red and near-infrared spectrum. While not as banded or storm-laced as Jupiter, it features broad zonal flows, high-altitude methane ice clouds, and long-lived anticyclonic storms akin to Neptune’s Great Dark Spot. Due to its tidal locking to the host star, the planet presents hemispheric climatic asymmetry: a sunlit dayside prone to atmospheric upwelling and cloud formation, and a cooler, darker nightside. While colder, the backside is not freezing— in the 150–250 K range, depending on circulation efficiency. Atmospheric circulation is dominated by slow, large-scale overturning cells, moderated by planetary-scale waves and a subdued Coriolis force. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Rings =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Ring!!	Range (Rₚ)!!	Approx.! Range (km)!!	Description&lt;br /&gt;
|-&lt;br /&gt;
! C&lt;br /&gt;
| 	1.5–1.65 Rₚ	||19,100–21,000	||Faint, dusty interior ring&lt;br /&gt;
|-&lt;br /&gt;
! B&lt;br /&gt;
| 	1.65–1.96 Rₚ	||21,000–25,000||	Bright, dense primary ring&lt;br /&gt;
|-&lt;br /&gt;
! Division&lt;br /&gt;
|	1.96–2.04 Rₚ ||25,000–26,000 || a low-density gap&lt;br /&gt;
|-&lt;br /&gt;
!  A&lt;br /&gt;
|	2.04–2.3 Rₚ||26,000–29,300||	Sharp-edged outer ring&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Moon !!	Orbit (km) !!	Orbit (Rₚ) !!	Diameter (km) !!	Type	!! Period !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! I&lt;br /&gt;
|	60,000	||4.7 Rₚ	||~400	||Rocky	|| 0.9 ||Cratered&lt;br /&gt;
|-&lt;br /&gt;
! II&lt;br /&gt;
| 	110,000	|| 8.6 Rₚ	|| ~800	|| Mixed rock/ice	|| 2.25|| Cracked surface, frozen ocean&lt;br /&gt;
|-&lt;br /&gt;
! III &lt;br /&gt;
| 190,000	|| 14.9 Rₚ ||	~1200 ||	Icy major moon ||	5.1|| Cryovolcanism, smooth plains&lt;br /&gt;
|-&lt;br /&gt;
! IV &lt;br /&gt;
|340,000	||26.7 Rₚ	||~200	||Irregular/prograde	|| 12.21 || Dark red/carbon, inclined (20º, eccentric orbit (0.1)&lt;br /&gt;
|-&lt;br /&gt;
! V &lt;br /&gt;
| 710,000 ||	55.7 Rₚ	||~350	|| Captured/retrograde	|| 36.83 || Highly inclined (130º), Split terrain—half rugged highlands, half smooth resurfaced plain&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==== g: Stripped Sub-Neptune Remnant ====&lt;br /&gt;
[[File:Stripped Planet with Two Cool Moons.png|700px|right]]&lt;br /&gt;
Basic Parameters&lt;br /&gt;
* Mass: 2.6 Earth masses (M⊕)&lt;br /&gt;
* Radius: 1.7 Earth radii (R⊕)&lt;br /&gt;
* Mean Density: ~2.92 g/cm³&lt;br /&gt;
* Orbital Distance: 0.4 AU &lt;br /&gt;
* Albedo: ~0.5 (moderately high)&lt;br /&gt;
* Rotation: Tidally locked &lt;br /&gt;
&lt;br /&gt;
Origin and Evolution&lt;br /&gt;
* Formed beyond the snow line (~0.8–1.2 AU) from a mix of rock, iron, and ices&lt;br /&gt;
* Migrated inward early during protoplanetary disk phase&lt;br /&gt;
* Accreted a modest hydrogen-helium envelope (&amp;gt;1% by mass)&lt;br /&gt;
* Exposed to intense stellar X-ray and UV radiation during the M dwarf&#039;s pre-main-sequence phase&lt;br /&gt;
* Lacked a magnetic dynamo (metal-poor and early core freezing)&lt;br /&gt;
* Entire atmosphere lost over ~100 Myr via photoevaporation, core-powered mass loss, and sputtering&lt;br /&gt;
&lt;br /&gt;
Current State&lt;br /&gt;
* Atmosphere: None (trace mineral vapors possible in hot regions)&lt;br /&gt;
* Surface: Stark contrast between hemispheres due to tidal locking&lt;br /&gt;
** Dayside: ~700–1000 K; high-silica lava fields, salt flats, exposed alumino-silicates&lt;br /&gt;
** Nightside: ~100–150 K; gypsum and calcite in cold traps, frozen regolith&lt;br /&gt;
* Magnetosphere: Absent&lt;br /&gt;
* Volcanism:episodic; high-silica flows, volcanic glass, sodium-rich crusts&lt;br /&gt;
* Geological Activity: Tectonically inactive; thermally fractured plains, impact craters&lt;br /&gt;
&lt;br /&gt;
Surface Composition&lt;br /&gt;
* Titanium dioxide (rutile): bright, high-albedo mineral condensate&lt;br /&gt;
* Calcite (CaCO₃): carbonate deposits in cold traps&lt;br /&gt;
* Gypsum (CaSO₄·2H₂O): hydration mineral, stable only on the nightside&lt;br /&gt;
* Sodium chloride: salt flats, especially in evaporated basins&lt;br /&gt;
* High-silica volcanic deposits: glassy, oxidized, and light-colored&lt;br /&gt;
&lt;br /&gt;
Visual and Observational Notes&lt;br /&gt;
&lt;br /&gt;
* High visual contrast between molten and frozen hemispheres&lt;br /&gt;
* Surface appears mottled: obsidian-black lava, gleaming salt flats, white calcium deposits&lt;br /&gt;
* No clouds, auroras, or magnetic activity&lt;br /&gt;
* Extreme day/night temperature gradient&lt;br /&gt;
* Reflective phase curve possible in photometric observations&lt;br /&gt;
* Surface pressure: effectively 0 bar&lt;br /&gt;
&lt;br /&gt;
Planet g is the airless skeleton of a once-sub-Neptune world. Born icy and distant, it migrated into the young star&#039;s wrath, where its fragile envelope boiled away under a sky of flares. Bereft of a magnetic shield, it was slowly stripped to bare rock. Today, one hemisphere bakes in molten silence while the other freezes in shadow. No air, no oceans, only salt, stone, and the echo of a lost atmosphere.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property !!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~75,000 km (~0.26 R&amp;lt;sub&amp;gt;hill&amp;lt;/sub&amp;gt;)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~1,400 km (~0.22 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass	&lt;br /&gt;
| ~0.01 M⊕ (~1.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~3.0 g/cm³ (rock–ice mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temp&lt;br /&gt;
|	~150–180 K&lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
| 0.20g&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere&lt;br /&gt;
|	Trace O₂, from radiolysis and outgassing&lt;br /&gt;
|-&lt;br /&gt;
! Subsurface Ocean&lt;br /&gt;
|	heated by tidal flexing&lt;br /&gt;
|-&lt;br /&gt;
! Surface Features	&lt;br /&gt;
|Fractured ice crust, chaos terrain, cryogeysers, lenticulae&lt;br /&gt;
|}&lt;br /&gt;
gI is a cracked glass orb, rimed with frost and laced with luminous fissures. Below its crust, tides flex a hidden ocean in rhythmic silence. Its faint oxygen exosphere is ghostly but present.  It is frosted quartz with cobwebbed streaks and mineral discoloration.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property!!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~150,000 km (~0.5 Rₕill)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~2,100 km (~0.33 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass&lt;br /&gt;
|	~0.035 M⊕ (~4.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~2.1 g/cm³ (icy-rocky mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes &lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
|	~0.35 g&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temperature&lt;br /&gt;
|	~115–130 K (pressure and greenhouse effects)&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere	&lt;br /&gt;
| ~0.18 bar N₂ + ~0.1 bar Ar + ~0.02 bar CH₄, minor CO, trace haze &lt;br /&gt;
|}&lt;br /&gt;
gII is a muted blue-green crescent veiled in gold. Its sky glows with the weight of argon and the shimmer of methane haze, and its surface smolders with the memory of internal warmth. Liquid hydrocarbons shine like ink in the basins, while glaciers ebb across the uplands. To the star it shows only one face, but beneath that still gaze lies the soft breath of a world more welcoming than its master.&lt;br /&gt;
&lt;br /&gt;
==== h ====&lt;br /&gt;
h is a twin-planet system, 1.5 AU from the star, with a period of 4.1 years&lt;br /&gt;
&lt;br /&gt;
Mutual Orbital Configuration&lt;br /&gt;
* Type: True binary planet pair, gravitationally bound, equal mass&lt;br /&gt;
* Masses: 5.0 M⊕ each&lt;br /&gt;
* Radii: 2.3 R⊕ each&lt;br /&gt;
* Mutual Orbit: Essentially circular, ~1 million km separation (~8–10 planetary radii)&lt;br /&gt;
* Period (mutual orbit): ~4.5 days&lt;br /&gt;
* Orbital Plane: Perpendicular to system ecliptic &lt;br /&gt;
* Tidal State: Tidally locked to each other (mutual synchronous rotation)&lt;br /&gt;
&lt;br /&gt;
Planet A — &amp;quot;Sapphire&amp;quot;&lt;br /&gt;
* Coloration: Deep sapphire blue with white high-altitude methane ice hazes&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: H₂, He&lt;br /&gt;
** Methane (CH₄): high&lt;br /&gt;
** Ammonia: trace&lt;br /&gt;
** Argon: moderate&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: slightly enriched&lt;br /&gt;
* Magnetosphere: Strong, symmetric; supports brilliant blue-violet aurorae&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Superionic water mantle&lt;br /&gt;
** Stratified silicate-ice alloy core&lt;br /&gt;
** Radiogenic heating and layered convection&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar hexagonal jet (stronger than Saturn&#039;s)&lt;br /&gt;
** Methane plasma flares at terminator&lt;br /&gt;
** Iridescent methane cirrus clouds&lt;br /&gt;
** Massive auroral crowns aligned with spin-magnetic axis misalignment&lt;br /&gt;
&lt;br /&gt;
Planet B — &amp;quot;Rust&amp;quot;&lt;br /&gt;
* Coloration: Dark crimson to rust-red, streaked with black and violet haze bands&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: N₂, CO&lt;br /&gt;
** CH₄: trace&lt;br /&gt;
** Tholins: abundant&lt;br /&gt;
** Argon: high&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: moderate&lt;br /&gt;
** Magnetosphere: Weak, multipolar and intermittent&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Dense iron-rich core with impact inclusions (e.g., iridium, ruthenium)&lt;br /&gt;
** Volcanically active mantle with carbon-rich inclusions&lt;br /&gt;
** Higher internal heat flow than Sapphire&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar cyclonic basins with geyser-like haze columns&lt;br /&gt;
** Frequent UV lightning within organic clouds&lt;br /&gt;
** Faint auroral echoes from Sapphire’s magnetospheric tail&lt;br /&gt;
** Surface glow from argon emissions during conjunction&lt;br /&gt;
&lt;br /&gt;
Mutual Phenomena &amp;amp; Sky Effects&lt;br /&gt;
* Eclipse Cycles: Frequent, due to short mutual period and perpendicular orbit; cause wave-like haze patterns and shadow bands&lt;br /&gt;
* Filamentary Atmosphere Bridges: Transient stratospheric strands near L1, illuminated during eclipses&lt;br /&gt;
* Auroral Flux Tubes: Occasionally connect the two with violet-green flickering arcs&lt;br /&gt;
* Gravitational Stability: Mutual orbit stable within Hill sphere; resistant to long-term disruption&lt;br /&gt;
&lt;br /&gt;
* Legacy of the Comet Shield&lt;br /&gt;
* Each planet’s core contains embedded relics of the system’s ancient bombardment:&lt;br /&gt;
** Sapphire: interstellar dust, primordial isotopes, deep xenon pockets&lt;br /&gt;
** Rust: impact-derived siderophiles, compressed organics, rare isotopic anomalies&lt;br /&gt;
* Capture Events: Both planets have intercepted and redirected hundreds of large icy bodies over system history&lt;br /&gt;
&lt;br /&gt;
They each have 2 small irregular moons, &amp;lt;100 km diameter, retrograde, on distant orbits.  Negligible.&lt;br /&gt;
== Planet C ==&lt;br /&gt;
&lt;br /&gt;
* With an albedo of 0.2, the global average temp is 263ºK.  Because of modest greenhouse effects, surface temperatures are higher, on the sun-side.&lt;br /&gt;
# Mass: 1.5M⊕&lt;br /&gt;
# Gravity: 1g⊕&lt;br /&gt;
# Radius = 1.225⊕, or 7805km&lt;br /&gt;
Terminator Zone&lt;br /&gt;
# +/-30º: 1.28 E8 km&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; (slightly less than all the land of the Earth)&lt;br /&gt;
# Escape velocity is 12.4km/s, 11% higher than Earth&lt;br /&gt;
# Orbital velocity is 8.79km/s&lt;br /&gt;
=== Atmosphere ===&lt;br /&gt;
Water content is low because&lt;br /&gt;
* Water vapor is a potent greenhouse gas; vast surface water can trap too much heat, especially near the substellar point.&lt;br /&gt;
* Water leads to climate homogenization&lt;br /&gt;
* Lack of exposed silicate rock: Necessary for carbon-silicate weathering feedback, which stabilizes climate on geological timescales.&lt;br /&gt;
Earth has ~1.4 billion km³ of water.  In our habitable zone, we have no more than 10% of that, or 100 million km³, though there is much more on the night side, both liquid and ice.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Factor !! Ɬiʔa atm !! Ɬiʔa % !! Earth atm !! Earth % !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! Total Pressure &lt;br /&gt;
| 1.6 atm || || 1.0 atm || || Enhanced convective heat transfer, increased IR trapping&lt;br /&gt;
|-&lt;br /&gt;
! Nitrogen (N₂) &lt;br /&gt;
| 1.00 || 62.50% || 0.7808 || 78.08% || Reduced; still inert, still dominant&lt;br /&gt;
|-&lt;br /&gt;
! Oxygen (O₂) &lt;br /&gt;
| 0.21 || 13.13% || 0.2095 || 20.95% || Earth-normal partial pressure &lt;br /&gt;
|-&lt;br /&gt;
! Argon (Ar)&lt;br /&gt;
| 0.40 || 25.00% || 0.0093 || 0.93% || Major heat distribution enhancement, inert&lt;br /&gt;
|-&lt;br /&gt;
! Krypton + Xenon&lt;br /&gt;
| 0.005 || 0.31% || trace || trace || High molecular mass → improved heat retention, still safe&lt;br /&gt;
|-&lt;br /&gt;
! CO₂&lt;br /&gt;
| 0.005 || 0.31% || 0.004 || 0.04% || slightly elevated; sub-greenhouse threshold&lt;br /&gt;
|-&lt;br /&gt;
! H₂O vapor &lt;br /&gt;
| 0.015 || ~1% || || 0-4% || Maintains greenhouse without excess moisture&lt;br /&gt;
|}&lt;br /&gt;
==== Atmospheric Effects on Clouds ====&lt;br /&gt;
# Increased Pressure (1.6 atm) compresses gases, raising the dew point at which water vapor condenses. Clouds form closer to the surface, and are denser than similar altitudes compared to Earth.&lt;br /&gt;
# Low Water Inventory (~20% of Earth&#039;s): less frequent and less massive cloud systems than on Earth, but still present—especially over &amp;quot;hotspots&amp;quot; on the day side.&lt;br /&gt;
# Tidally Locked Climate: Cloud formation concentrate along the substellar point, where warm, moist air rises and cools.&lt;br /&gt;
#* A permanent “eyewall” storm system has formed at the subsolar point, like a giant hurricane.&lt;br /&gt;
#* As air rises and is advected to the night side, thin cloud bands or ice hazes form as it descends and cools.&lt;br /&gt;
&lt;br /&gt;
Appearance:&lt;br /&gt;
* The presence of noble gases (Ar, Kr, Xe) and higher pressure enhance Mie scattering, making clouds appear whiter and more silvered, especially at sunrise/sunset boundaries.&lt;br /&gt;
* Night side clouds are thin, high-altitude icy sheets, glowing faintly in aurorae or thermal emissions.&lt;br /&gt;
&lt;br /&gt;
==== Sky Color ====&lt;br /&gt;
The color of the sky is shaped by Rayleigh scattering, which depends on:&lt;br /&gt;
# Molecular composition: Heavier gases like Ar, Kr, and Xe scatter light less efficiently than N₂.&lt;br /&gt;
# Spectral output of the star: the red dwarf emits predominantly infrared and red light, with very little blue or violet.&lt;br /&gt;
&lt;br /&gt;
Consequence:&lt;br /&gt;
* Even with atmospheric scattering, there is insufficient blue light in the stellar spectrum to produce a blue sky.&lt;br /&gt;
* Day sky would likely appear:&lt;br /&gt;
** Dark peach, dusky rose, or reddish beige near zenith,&lt;br /&gt;
** Grading to deep salmon or mauve near the horizon,&lt;br /&gt;
** A slight metallic sheen due to noble gas content and high pressure.&lt;br /&gt;
&lt;br /&gt;
Twilight &amp;amp; Limb Scattering:&lt;br /&gt;
* The terminator (twilight zone) sees a diffuse, ruddy light, scattering through haze and clouds into luminous reds, purples, and copper tones.&lt;br /&gt;
* Aurorae are spectacular on the night side, especially since stellar flares are frequent.&lt;br /&gt;
&lt;br /&gt;
==== Sound Propagation ====&lt;br /&gt;
: &#039;&#039;Sound is profoundly affected by atmospheric pressure and composition.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Compared to Earth:&lt;br /&gt;
* Higher pressure → greater air density → faster transmission of sound and less attenuation.&lt;br /&gt;
* Argon and Xenon are heavy gases, which:&lt;br /&gt;
** Lower the speed of sound relative to air at the same pressure (despite the pressure increase).&lt;br /&gt;
** Shift resonance frequencies downward, resulting in deeper, rounder sounds.&lt;br /&gt;
&lt;br /&gt;
Consequences:&lt;br /&gt;
* Voices sound subtly lower-pitched and richer, especially for consonants and low vowels.&lt;br /&gt;
* Ambient sounds (wind, water, animals) would carry farther and sound more muffled or sonorous.&lt;br /&gt;
* Music or speech would resonate more warmly, especially indoors or in enclosed spaces.&lt;br /&gt;
&lt;br /&gt;
In short: it sounds like it’s wrapped in velvet.&lt;br /&gt;
&lt;br /&gt;
==== Heat Transport to the Night Side ====&lt;br /&gt;
Mechanisms:&lt;br /&gt;
# Thick Atmosphere (1.6 atm) increases:&lt;br /&gt;
#* Advection efficiency: Warm air masses can move more heat horizontally.&lt;br /&gt;
#* Radiative time constant: The atmosphere holds heat longer before releasing it.&lt;br /&gt;
# Noble Gases (especially Kr/Xe):&lt;br /&gt;
#* High molecular mass → more IR opacity → trapping and radiating heat more evenly.&lt;br /&gt;
# Slow Rotation / Tidal Locking:&lt;br /&gt;
#* Global Hadley-like cells dominate circulation, carrying warm air from the day side to the night side and descending it there.&lt;br /&gt;
&lt;br /&gt;
Result:&lt;br /&gt;
* The night side is not so freezing.  Temperatures differ by tens of degrees, not hundreds.&lt;br /&gt;
* There are still ice caps and a cold deserts at the anti-stellar point, but not a glaciated wasteland.&lt;br /&gt;
&lt;br /&gt;
=== Magnetosphere ===&lt;br /&gt;
* Larger mass --&amp;gt; larger iron core, generating more internal heat&lt;br /&gt;
* Larger radius --&amp;gt; Vigorous convection in the core&lt;br /&gt;
* Tidal Flexing --&amp;gt; still drives magnetic activity&lt;br /&gt;
&lt;br /&gt;
# Aurorae at lower latitudes&lt;br /&gt;
## higher magnetic rigidity, wider magnetotail, and greater reconnection energy.&lt;br /&gt;
## Combined with a higher flux of stellar particles, this means:&lt;br /&gt;
### Auroral ovals expand, reaching mid-latitudes sometimes equator.&lt;br /&gt;
### The skies are alive with rippling green, violet, and crimson aurorae, especially on the night side.&lt;br /&gt;
### Daily auroral activity occur during stellar flare cycles.&lt;br /&gt;
# Compasses&lt;br /&gt;
## compasses respond more sharply, with:&lt;br /&gt;
### Faster alignment.&lt;br /&gt;
### Greater resistance to local perturbations.&lt;br /&gt;
## However, frequent magnetic storms from stellar activity cause sudden declinations, reversals, or local anomalies.  In short, lots of aurorae equals dead compasses at the same time.&lt;br /&gt;
# Magnetic Field Strength &amp;gt; 100 μT &lt;br /&gt;
# Electromagnetism is more basic than chemistry or almost any other natural philosophy&lt;br /&gt;
&lt;br /&gt;
=== Substellar Point ===&lt;br /&gt;
The maximum incoming flux is very nearly the same as Earth&#039;s solar constant (≈1361 W/m²), but concentrated over one point rather than averaged over a rotating sphere.  Temperatures should be above 500ºK most of the time.  &lt;br /&gt;
&lt;br /&gt;
The magnetic north is also here. The thick atmosphere prevents too much loss here, but &lt;br /&gt;
* Charged particle influx&lt;br /&gt;
** Maximized at the substellar point—intense auroral and energetic particle precipitation&lt;br /&gt;
* Atmospheric ionization&lt;br /&gt;
** Constant production of high-energy ions and NOx compounds—UV fluorescence in upper sky&lt;br /&gt;
* Localized heating&lt;br /&gt;
** Augments already extreme temperatures—600–700 K surface&lt;br /&gt;
&lt;br /&gt;
== Artificially Tethered Moon ==&lt;br /&gt;
* 670,000 km up&lt;br /&gt;
* 7805 km in radius = same as the planet&lt;br /&gt;
* 1.33º of the sky, same as the sun&lt;br /&gt;
&lt;br /&gt;
A network of tethers/tension lines from the moon to multiple anchor points on the planet’s surface (a tripod or hexapod structure), woven like hair&lt;br /&gt;
* Uses active tension management and orbital station-keeping to stabilize the moon&lt;br /&gt;
* Counterweights and inward-pointing mass drivers on the moon to oppose drift&lt;br /&gt;
&lt;br /&gt;
The tethers are not bearing the full weight, but merely damping drift, providing restoring force, and enabling long-term stability through active compensation.  The moon&lt;br /&gt;
* Blocks the worst of the heat&lt;br /&gt;
* Blocks the worst of the solar radiation&lt;br /&gt;
The moon has &lt;br /&gt;
* low mass&lt;br /&gt;
* high albedo - enormous reflectivity&lt;br /&gt;
* scatters charges particles, UV, X-rays, auroral flux tubes&lt;br /&gt;
* sunward - crazy hot, high emissivity&lt;br /&gt;
* earthward - crazy cool, low emissivity&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=File:Stripped_Planet_with_Two_Cool_Moons.png&amp;diff=168164</id>
		<title>File:Stripped Planet with Two Cool Moons.png</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=File:Stripped_Planet_with_Two_Cool_Moons.png&amp;diff=168164"/>
		<updated>2025-03-27T23:53:16Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: Two moons and a planet&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Summary ==&lt;br /&gt;
Two moons and a planet&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168163</id>
		<title>Ɬiʔa/Conworlding</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168163"/>
		<updated>2025-03-27T23:36:30Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* f: Ringed Mini-Neptune */ pic&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Star ==&lt;br /&gt;
Our star is a red-dwarf.&lt;br /&gt;
# Type: M5V&lt;br /&gt;
## M: This indicates it&#039;s a cool, red star with a surface temperature less than 3,500ºK&lt;br /&gt;
## 5: Within the M class, stars are further divided into subclasses 0-9, with 0 being the hottest and 9 the coolest. An M5 star is in the middle of this range.&lt;br /&gt;
## V: Denotes that it&#039;s a main sequence star, also known as a dwarf star&lt;br /&gt;
# Stellar luminosity (L*) ≈ 0.01 𝐿⊙ (1/100th Sol&#039;s brightness)&lt;br /&gt;
# Stellar mass (M*) ≈ 0.2 𝑀⊙ (1/5 the mass of Sol)&lt;br /&gt;
# Stellar radius (R*) ≈ 0.25 𝑅⊙ (1/4 as wide as Sol)&lt;br /&gt;
# Effective temperature (T*) ≈ 3500 K&lt;br /&gt;
​The habitable zone (a) is about square root of L* over L⊙, so ~0.1 AU.&lt;br /&gt;
&lt;br /&gt;
=== Solar System ===&lt;br /&gt;
There are seven planets in the system&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Planet !!	Mass (M🜨)!!	Radius (R🜨)!! Moons/Rings	!!Resonance !!	Semi-Major Axis (AU)!!	Rings !! Moons !! Period !! Size&lt;br /&gt;
|-&lt;br /&gt;
| b ||	2.17 ||	1.1 ||	No ||	2:3 with c	|| 0.0763 ||	No || No || 17.2 || 13.6&#039; to 1.5&#039;&lt;br /&gt;
|-&lt;br /&gt;
| c ||	1.5	 ||1.225 ||	1* ||	—	        || 0.100 || No || No || 25.8 || -&lt;br /&gt;
|-&lt;br /&gt;
| d ||	2.0	 ||1.4 ||No ||	2:3 with c	 ||0.131 ||	No || No || 38.7 || 13.1&#039; to 1.8&#039;&lt;br /&gt;
|-&lt;br /&gt;
| e ||	0.9 ||	1.0 || No	 ||	2:3 with d	 ||0.172 ||	No || No || 58 || 4.1&#039; to 1.1&#039;&lt;br /&gt;
|-&lt;br /&gt;
| f ||	3.5 ||	2.0 ||	Yes! ||	2:3 with e	 ||0.227 || Yes || Junk || 87 || 4.6&#039; to 1.8&#039;&lt;br /&gt;
|-&lt;br /&gt;
| g ||	2.6 ||	1.7 ||	2 ||	-	 ||0.40 ||	Yes || Junk || 206 || 1.6&#039; to 1.0&#039;&lt;br /&gt;
|-&lt;br /&gt;
| h ||	5.0x2 ||2.3x2 || yes	 || -	 ||1.5 ||	Yes || No || 1500 || 0.5&#039; 16.4&#039; apart (at max)&lt;br /&gt;
|}&lt;br /&gt;
==== b: super Mercury with a ring of fire  ====&lt;br /&gt;
[[File:planet b by GPT.png|thumb|right|An artistic rendering of planet b]]&lt;br /&gt;
b is a super-Mercury, tidally locked, and incredibly dense.  ~700ºK on the day side, ~50ºK on the night.  2.1 Earth Masses, 1.1 Earth radii (~7000km) in size.  Orbital period 17.2 days.  Density 9.0 g/cm&amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt;.  Gravity is ~1.8g.  &lt;br /&gt;
&lt;br /&gt;
The iron core is huge, being 75% of the mass.  A thin silicate mantle, with metallic plains and exhumed ultramafic crust, with frequent iron meteorite craters, lacking typical “stone” breccias.&lt;br /&gt;
&lt;br /&gt;
The night side is intense, as simple hydrocarbons (methane, ethane, propane) condense and freeze into layered deposits.  Complex organics (tholins, polycyclic aromatics) accumulate on the sea floor, under miles of nitrogen ice.  Massive slush layers slosh around above cryovolcanic brines of ammonia.&lt;br /&gt;
&lt;br /&gt;
There is a crucial layer of Superionic Ice XI above the core, which acts as an electromagnetic insulator, and ionic heat bridge.  The crust is ultramafic silicates (olivine, pyroxene, perovskite) riddled with with sulfide veins, iron alloys, and graphite networks.  The poles of the magnetosphere are sideways, like Uranus, with poles at the equator in the Terminator Zone.  Persistent surface charges develop, because the whole planet is basically a ginormous Leyden jar!&lt;br /&gt;
&lt;br /&gt;
A planetary flux rope forms and un-forms with the star and planet b.  This induces electric jets at the terminator.  This is where temps are Earth-like.  Hydrocarbons sublimate and eject into the atmosphere, even while aurorae come right down to the ground.  A small, low pressure atmosphere prevents photodissociation, even while electrothermal instabilities lift molecules, forming an anomalous haze, a standing, glowing ring.  Coronal events cause localized lightning geysers with magnetic arcing.&lt;br /&gt;
&lt;br /&gt;
In short, b is visible with a blinding bright sun side (glowing orange bronze), a utterly black night side, and a burning, glowing, erupting, arcing ring at the terminator (all colors).  At biggest, it&#039;s half the size of Earth&#039;s moon in the sky, shrinking down to a star at it&#039;s furthest away.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== d: the wet eye with depths ====&lt;br /&gt;
[[File:wet eye planet.png|thumb|right|An reasonable approximation of d&#039;s appearance]]&lt;br /&gt;
From the outside, d is a &amp;quot;wet eye&amp;quot; just outside the habitable zone.  It is a water world, twice the mass of Earth, 1.4 times the radius, tidally locked.  The substellar point is the only place without surface ice.  However, it is better to think of the planet top-to-bottom.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;atmosphere&#039;&#039;&#039; is tenuous, less than 0.2 bars.  It is thin, N₂-rich with traces of H₂O, NH₃ vapor, and transient geyser outputs.  It is highly UV-irradiated, and Mars-like in its inability to retain volatiles.&lt;br /&gt;
&lt;br /&gt;
Next, there is a &#039;&#039;&#039;surface ice shell&#039;&#039;&#039;, ~20 km of thick Ice I.  Swirling currents beneath have cracked continent-sized ice plates, similar to Europa&#039;s crust.  It is permanently frozen except at the substellar furnace.  It accumulates chemical stains, mineral deposits, and cryovolcanic eruption plumes.  Accumulations of complex hydrates—like methanol clathrates—precipitate out and form false reefs, rising like coral from beneath. Transient thermal vents push hot plumes into the thin air, freezing instantly and snowing down crystals that form mineral spires.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;subglacial ocean&#039;&#039;&#039; is hundreds of kilometers thick.  It is super-pressurized liquid H₂O mixed with NH₃, CH₃OH, H₂O₂, and trace salts.  The movement is slow, planetary-scale currents originating from the Furnace and Coriolis force.  Strong layers exist: the surface is oxidized; the abyssal layer is reducing.&lt;br /&gt;
&lt;br /&gt;
A new &amp;quot;surface&amp;quot; is next.  The &#039;&#039;&#039;Ice Mantle&#039;&#039;&#039; is solid Ice VI and VII.  There are massive, slowly shifting &amp;quot;sub-oceanic continents&amp;quot;. It is periodically fractured and resurfaced by cryoquakes and brine-driven eruptions.  Some regions have developed elevated domes or ridges, continental “shelves” under the ocean.&lt;br /&gt;
&lt;br /&gt;
Finally, underneath is the &#039;&#039;&#039;core&#039;&#039;&#039;. Temperatures exceed 2000–3000 K locally.  Pressures range from 100 to 300 GPa.  The core is rich in heavy elements.  This makes radiogenic hotspots, localized magnetic eddies.  Heat gradients + ion flows = thermoelectric currents.  These make magnetic storms within the ocean itself, not the sky.  When uranium-rich corium pods shift or explode upward through the mantle, their heat and conductivity disturb the local magnetic field, generating geomagnetic quakes.  These pulse through the ocean, creating short-lived magnetic lenses.  These interact with atmospheric charged particles above the Furnace, giving rise to transient magnetic halos visible from orbit—false auroras without a sunstorm.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== e: The Tortured Near-Sphere ====&lt;br /&gt;
[[File:Blasting and shattered.png|thumb|right|An axial recoil event in progress]]&lt;br /&gt;
Orbital and Physical Characteristics&lt;br /&gt;
* Mass: 0.9 Earth masses&lt;br /&gt;
* Radius: 1.0 Earth radii&lt;br /&gt;
* Orbital Period: 58 Earth days&lt;br /&gt;
* Surface Gravity: ~0.9 g&lt;br /&gt;
* Semimajor Axis: ~0.17 AU &lt;br /&gt;
* Spin State: In the &#039;&#039;process&#039;&#039; of becoming tidally locked&lt;br /&gt;
* Obliquity: Extreme, experiencing chaotic realignment events&lt;br /&gt;
&lt;br /&gt;
Internal Structure and Composition&lt;br /&gt;
* &#039;&#039;&#039;Crust:&#039;&#039;&#039; A thick, rigid outer shell of water ice I mixed with clathrates (CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; and CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; hydrates), underlain by layers of ammonia-water ice eutectics. Inclusions of carbon under extreme pressure form diamond strata in the lower crust, lending rigidity and brittle behavior.&lt;br /&gt;
* &#039;&#039;&#039;Mantle:&#039;&#039;&#039; Comprised of Ice VI and Ice VII, with ammonia- and methane-rich brines forming localized conduits and pockets of unstable volatiles.&lt;br /&gt;
* &#039;&#039;&#039;Core:&#039;&#039;&#039; Differentiated and semi-molten. Inner core of iron-nickel alloy spins at a different rate. Outer core is a highly viscous slurry of silicate, iron, carbon, sulfur, and dissolved volatiles. Chemical veins (e.g., uranium silicates, perovskites) act as mechanical shear zones. Tidal torque leads to periodic frictional heating.&lt;br /&gt;
&lt;br /&gt;
Tectonic and Cryovolcanic Behavior&lt;br /&gt;
* The planet resists tidal locking due to core-crust decoupling and uneven angular momentum transfer.&lt;br /&gt;
* High obliquity experiences &#039;&#039;&#039;&#039;&#039;Axial Recoil Events&#039;&#039;&#039;&#039;&#039;, where the entire planet jerks between metastable orientations (e.g., from 110° to 70°) in sudden spasms.&lt;br /&gt;
* These events generate:&lt;br /&gt;
** Global-scale crustal cracking&lt;br /&gt;
** Venting of pressurized subsurface gases (H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;O, CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt;)&lt;br /&gt;
** Surface deformation and glacial faulting&lt;br /&gt;
* Volatiles erupt ballistically into space (200+lm) from exposed fissures and calderas, driven by phase-change explosions.&lt;br /&gt;
&lt;br /&gt;
Surface Conditions&lt;br /&gt;
* Global temperature well below freezing; warmest zones around cryovolcanic hotspots&lt;br /&gt;
* Crustal coloration varies by volatile deposition:&lt;br /&gt;
** Pale blue-white from water ice&lt;br /&gt;
** Red-brown from CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; frostfields&lt;br /&gt;
** Green-black CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; stains from plume fallout&lt;br /&gt;
* Surface features include:&lt;br /&gt;
** Cryovolcanic calderas&lt;br /&gt;
** Diamond-studded impact-like basins&lt;br /&gt;
** Faulted plains crossed by salt-streaked rift zones&lt;br /&gt;
&lt;br /&gt;
Atmosphere and Ejected Material&lt;br /&gt;
* Thin transient exosphere formed from eruptive events&lt;br /&gt;
* Gases often escape to space or freeze back out in polar regions&lt;br /&gt;
* Fallback material creates uneven surface mass distributions, altering moment of inertia and prolonging instability&lt;br /&gt;
&lt;br /&gt;
Appearance from Planet c&lt;br /&gt;
&lt;br /&gt;
* Angular Size: ~4-1 arcminutes&lt;br /&gt;
* Coloration: Overall dusky grey-white, with changing colored bands due to volatile fallout; craterless but mottled&lt;br /&gt;
&lt;br /&gt;
Transient visible phenomena:&lt;br /&gt;
&lt;br /&gt;
* Cryovolcanic plumes visible as fan-like arcs at the limb during outburst events&lt;br /&gt;
* Infrared brightening during Axial Recoil Events&lt;br /&gt;
* Occasional light-scattering halos from plume particles&lt;br /&gt;
&lt;br /&gt;
Event Cycle Summary&lt;br /&gt;
&lt;br /&gt;
# Tidal torque builds due to obliquity misalignment&lt;br /&gt;
# Core resists, crust locks tension&lt;br /&gt;
# Critical stress threshold breached&lt;br /&gt;
# Obliquity lurches to new orientation&lt;br /&gt;
# Crust fractures globally, vents open&lt;br /&gt;
# Supersonic cryovolcanism hurls volatiles into space&lt;br /&gt;
# Fallback modifies crustal mass distribution&lt;br /&gt;
# Obliquity rebuilds instability over decades&lt;br /&gt;
# Repeat.&lt;br /&gt;
&lt;br /&gt;
Planet e is a tortured world caught in an unending cycle of self-correcting failure—its body unable to align, its gases unable to stay contained, its appearance in the sky a visible signature of internal catastrophe.&lt;br /&gt;
&lt;br /&gt;
==== f: Ringed Mini-Neptune ====&lt;br /&gt;
[[File:Ringed Neptune with four moons.png|thumb|right|Aperspectival view of f, its rings, and four moons]]&lt;br /&gt;
This planet is a substantial mini-Neptune, with a mass of approximately 3.5 Earth masses and a radius of 2.0 Earth radii, orbiting at 0.227 AU. Its low mean density (~0.44 ρ⊕) signals the presence of a deep, volatile-rich envelope overlying a denser core. The bulk of its volume is composed of hydrogen and helium, accreted from the protoplanetary disk, with trace amounts of methane (CH₄) and ammonia (NH₃)—gases that dominate its photochemical and radiative behavior. Beneath this envelope, the planet hosts a water–rock–metal core layered in complex phases, with high-pressure ices and possibly superionic water enveloping a metallic center.  Lower atmosphere reaches 300–500 K (27–227°C) near the bottom of the troposphere, depending on opacity and convection.&lt;br /&gt;
&lt;br /&gt;
Visually, the planet exhibits a blue-to-cyan atmospheric hue, governed by Rayleigh scattering and methane absorption in the red and near-infrared spectrum. While not as banded or storm-laced as Jupiter, it features broad zonal flows, high-altitude methane ice clouds, and long-lived anticyclonic storms akin to Neptune’s Great Dark Spot. Due to its tidal locking to the host star, the planet presents hemispheric climatic asymmetry: a sunlit dayside prone to atmospheric upwelling and cloud formation, and a cooler, darker nightside. While colder, the backside is not freezing— in the 150–250 K range, depending on circulation efficiency. Atmospheric circulation is dominated by slow, large-scale overturning cells, moderated by planetary-scale waves and a subdued Coriolis force. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Rings =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Ring!!	Range (Rₚ)!!	Approx.! Range (km)!!	Description&lt;br /&gt;
|-&lt;br /&gt;
! C&lt;br /&gt;
| 	1.5–1.65 Rₚ	||19,100–21,000	||Faint, dusty interior ring&lt;br /&gt;
|-&lt;br /&gt;
! B&lt;br /&gt;
| 	1.65–1.96 Rₚ	||21,000–25,000||	Bright, dense primary ring&lt;br /&gt;
|-&lt;br /&gt;
! Division&lt;br /&gt;
|	1.96–2.04 Rₚ ||25,000–26,000 || a low-density gap&lt;br /&gt;
|-&lt;br /&gt;
!  A&lt;br /&gt;
|	2.04–2.3 Rₚ||26,000–29,300||	Sharp-edged outer ring&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Moon !!	Orbit (km) !!	Orbit (Rₚ) !!	Diameter (km) !!	Type	!! Period !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! I&lt;br /&gt;
|	60,000	||4.7 Rₚ	||~400	||Rocky	|| 0.9 ||Cratered&lt;br /&gt;
|-&lt;br /&gt;
! II&lt;br /&gt;
| 	110,000	|| 8.6 Rₚ	|| ~800	|| Mixed rock/ice	|| 2.25|| Cracked surface, frozen ocean&lt;br /&gt;
|-&lt;br /&gt;
! III &lt;br /&gt;
| 190,000	|| 14.9 Rₚ ||	~1200 ||	Icy major moon ||	5.1|| Cryovolcanism, smooth plains&lt;br /&gt;
|-&lt;br /&gt;
! IV &lt;br /&gt;
|340,000	||26.7 Rₚ	||~200	||Irregular/prograde	|| 12.21 || Dark red/carbon, inclined (20º, eccentric orbit (0.1)&lt;br /&gt;
|-&lt;br /&gt;
! V &lt;br /&gt;
| 710,000 ||	55.7 Rₚ	||~350	|| Captured/retrograde	|| 36.83 || Highly inclined (130º), Split terrain—half rugged highlands, half smooth resurfaced plain&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==== g: Stripped Sub-Neptune Remnant ====&lt;br /&gt;
&lt;br /&gt;
Basic Parameters&lt;br /&gt;
* Mass: 2.6 Earth masses (M⊕)&lt;br /&gt;
* Radius: 1.7 Earth radii (R⊕)&lt;br /&gt;
* Mean Density: ~2.92 g/cm³&lt;br /&gt;
* Orbital Distance: 0.4 AU &lt;br /&gt;
* Albedo: ~0.5 (moderately high)&lt;br /&gt;
* Rotation: Tidally locked &lt;br /&gt;
&lt;br /&gt;
Origin and Evolution&lt;br /&gt;
* Formed beyond the snow line (~0.8–1.2 AU) from a mix of rock, iron, and ices&lt;br /&gt;
* Migrated inward early during protoplanetary disk phase&lt;br /&gt;
* Accreted a modest hydrogen-helium envelope (&amp;gt;1% by mass)&lt;br /&gt;
* Exposed to intense stellar X-ray and UV radiation during the M dwarf&#039;s pre-main-sequence phase&lt;br /&gt;
* Lacked a magnetic dynamo (metal-poor and early core freezing)&lt;br /&gt;
* Entire atmosphere lost over ~100 Myr via photoevaporation, core-powered mass loss, and sputtering&lt;br /&gt;
&lt;br /&gt;
Current State&lt;br /&gt;
* Atmosphere: None (trace mineral vapors possible in hot regions)&lt;br /&gt;
* Surface: Stark contrast between hemispheres due to tidal locking&lt;br /&gt;
** Dayside: ~700–1000 K; high-silica lava fields, salt flats, exposed alumino-silicates&lt;br /&gt;
** Nightside: ~100–150 K; gypsum and calcite in cold traps, frozen regolith&lt;br /&gt;
* Magnetosphere: Absent&lt;br /&gt;
* Volcanism:episodic; high-silica flows, volcanic glass, sodium-rich crusts&lt;br /&gt;
* Geological Activity: Tectonically inactive; thermally fractured plains, impact craters&lt;br /&gt;
&lt;br /&gt;
Surface Composition&lt;br /&gt;
* Titanium dioxide (rutile): bright, high-albedo mineral condensate&lt;br /&gt;
* Calcite (CaCO₃): carbonate deposits in cold traps&lt;br /&gt;
* Gypsum (CaSO₄·2H₂O): hydration mineral, stable only on the nightside&lt;br /&gt;
* Sodium chloride: salt flats, especially in evaporated basins&lt;br /&gt;
* High-silica volcanic deposits: glassy, oxidized, and light-colored&lt;br /&gt;
&lt;br /&gt;
Visual and Observational Notes&lt;br /&gt;
&lt;br /&gt;
* High visual contrast between molten and frozen hemispheres&lt;br /&gt;
* Surface appears mottled: obsidian-black lava, gleaming salt flats, white calcium deposits&lt;br /&gt;
* No clouds, auroras, or magnetic activity&lt;br /&gt;
* Extreme day/night temperature gradient&lt;br /&gt;
* Reflective phase curve possible in photometric observations&lt;br /&gt;
* Surface pressure: effectively 0 bar&lt;br /&gt;
&lt;br /&gt;
Planet g is the airless skeleton of a once-sub-Neptune world. Born icy and distant, it migrated into the young star&#039;s wrath, where its fragile envelope boiled away under a sky of flares. Bereft of a magnetic shield, it was slowly stripped to bare rock. Today, one hemisphere bakes in molten silence while the other freezes in shadow. No air, no oceans, only salt, stone, and the echo of a lost atmosphere.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property !!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~75,000 km (~0.26 R&amp;lt;sub&amp;gt;hill&amp;lt;/sub&amp;gt;)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~1,400 km (~0.22 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass	&lt;br /&gt;
| ~0.01 M⊕ (~1.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~3.0 g/cm³ (rock–ice mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temp&lt;br /&gt;
|	~150–180 K&lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
| 0.20g&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere&lt;br /&gt;
|	Trace O₂, from radiolysis and outgassing&lt;br /&gt;
|-&lt;br /&gt;
! Subsurface Ocean&lt;br /&gt;
|	heated by tidal flexing&lt;br /&gt;
|-&lt;br /&gt;
! Surface Features	&lt;br /&gt;
|Fractured ice crust, chaos terrain, cryogeysers, lenticulae&lt;br /&gt;
|}&lt;br /&gt;
gI is a cracked glass orb, rimed with frost and laced with luminous fissures. Below its crust, tides flex a hidden ocean in rhythmic silence. Its faint oxygen exosphere is ghostly but present.  It is frosted quartz with cobwebbed streaks and mineral discoloration.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property!!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~150,000 km (~0.5 Rₕill)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~2,100 km (~0.33 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass&lt;br /&gt;
|	~0.035 M⊕ (~4.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~2.1 g/cm³ (icy-rocky mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes &lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
|	~0.35 g&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temperature&lt;br /&gt;
|	~115–130 K (pressure and greenhouse effects)&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere	&lt;br /&gt;
| ~0.18 bar N₂ + ~0.1 bar Ar + ~0.02 bar CH₄, minor CO, trace haze &lt;br /&gt;
|}&lt;br /&gt;
gII is a muted blue-green crescent veiled in gold. Its sky glows with the weight of argon and the shimmer of methane haze, and its surface smolders with the memory of internal warmth. Liquid hydrocarbons shine like ink in the basins, while glaciers ebb across the uplands. To the star it shows only one face, but beneath that still gaze lies the soft breath of a world more welcoming than its master.&lt;br /&gt;
&lt;br /&gt;
==== h ====&lt;br /&gt;
h is a twin-planet system, 1.5 AU from the star, with a period of 4.1 years&lt;br /&gt;
&lt;br /&gt;
Mutual Orbital Configuration&lt;br /&gt;
* Type: True binary planet pair, gravitationally bound, equal mass&lt;br /&gt;
* Masses: 5.0 M⊕ each&lt;br /&gt;
* Radii: 2.3 R⊕ each&lt;br /&gt;
* Mutual Orbit: Essentially circular, ~1 million km separation (~8–10 planetary radii)&lt;br /&gt;
* Period (mutual orbit): ~4.5 days&lt;br /&gt;
* Orbital Plane: Perpendicular to system ecliptic &lt;br /&gt;
* Tidal State: Tidally locked to each other (mutual synchronous rotation)&lt;br /&gt;
&lt;br /&gt;
Planet A — &amp;quot;Sapphire&amp;quot;&lt;br /&gt;
* Coloration: Deep sapphire blue with white high-altitude methane ice hazes&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: H₂, He&lt;br /&gt;
** Methane (CH₄): high&lt;br /&gt;
** Ammonia: trace&lt;br /&gt;
** Argon: moderate&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: slightly enriched&lt;br /&gt;
* Magnetosphere: Strong, symmetric; supports brilliant blue-violet aurorae&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Superionic water mantle&lt;br /&gt;
** Stratified silicate-ice alloy core&lt;br /&gt;
** Radiogenic heating and layered convection&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar hexagonal jet (stronger than Saturn&#039;s)&lt;br /&gt;
** Methane plasma flares at terminator&lt;br /&gt;
** Iridescent methane cirrus clouds&lt;br /&gt;
** Massive auroral crowns aligned with spin-magnetic axis misalignment&lt;br /&gt;
&lt;br /&gt;
Planet B — &amp;quot;Rust&amp;quot;&lt;br /&gt;
* Coloration: Dark crimson to rust-red, streaked with black and violet haze bands&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: N₂, CO&lt;br /&gt;
** CH₄: trace&lt;br /&gt;
** Tholins: abundant&lt;br /&gt;
** Argon: high&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: moderate&lt;br /&gt;
** Magnetosphere: Weak, multipolar and intermittent&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Dense iron-rich core with impact inclusions (e.g., iridium, ruthenium)&lt;br /&gt;
** Volcanically active mantle with carbon-rich inclusions&lt;br /&gt;
** Higher internal heat flow than Sapphire&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar cyclonic basins with geyser-like haze columns&lt;br /&gt;
** Frequent UV lightning within organic clouds&lt;br /&gt;
** Faint auroral echoes from Sapphire’s magnetospheric tail&lt;br /&gt;
** Surface glow from argon emissions during conjunction&lt;br /&gt;
&lt;br /&gt;
Mutual Phenomena &amp;amp; Sky Effects&lt;br /&gt;
* Eclipse Cycles: Frequent, due to short mutual period and perpendicular orbit; cause wave-like haze patterns and shadow bands&lt;br /&gt;
* Filamentary Atmosphere Bridges: Transient stratospheric strands near L1, illuminated during eclipses&lt;br /&gt;
* Auroral Flux Tubes: Occasionally connect the two with violet-green flickering arcs&lt;br /&gt;
* Gravitational Stability: Mutual orbit stable within Hill sphere; resistant to long-term disruption&lt;br /&gt;
&lt;br /&gt;
* Legacy of the Comet Shield&lt;br /&gt;
* Each planet’s core contains embedded relics of the system’s ancient bombardment:&lt;br /&gt;
** Sapphire: interstellar dust, primordial isotopes, deep xenon pockets&lt;br /&gt;
** Rust: impact-derived siderophiles, compressed organics, rare isotopic anomalies&lt;br /&gt;
* Capture Events: Both planets have intercepted and redirected hundreds of large icy bodies over system history&lt;br /&gt;
&lt;br /&gt;
They each have 2 small irregular moons, &amp;lt;100 km diameter, retrograde, on distant orbits.  Negligible.&lt;br /&gt;
== Planet C ==&lt;br /&gt;
&lt;br /&gt;
* With an albedo of 0.2, the global average temp is 263ºK.  Because of modest greenhouse effects, surface temperatures are higher, on the sun-side.&lt;br /&gt;
# Mass: 1.5M⊕&lt;br /&gt;
# Gravity: 1g⊕&lt;br /&gt;
# Radius = 1.225⊕, or 7805km&lt;br /&gt;
Terminator Zone&lt;br /&gt;
# +/-30º: 1.28 E8 km&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; (slightly less than all the land of the Earth)&lt;br /&gt;
# Escape velocity is 12.4km/s, 11% higher than Earth&lt;br /&gt;
# Orbital velocity is 8.79km/s&lt;br /&gt;
=== Atmosphere ===&lt;br /&gt;
Water content is low because&lt;br /&gt;
* Water vapor is a potent greenhouse gas; vast surface water can trap too much heat, especially near the substellar point.&lt;br /&gt;
* Water leads to climate homogenization&lt;br /&gt;
* Lack of exposed silicate rock: Necessary for carbon-silicate weathering feedback, which stabilizes climate on geological timescales.&lt;br /&gt;
Earth has ~1.4 billion km³ of water.  In our habitable zone, we have no more than 10% of that, or 100 million km³, though there is much more on the night side, both liquid and ice.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Factor !! Ɬiʔa atm !! Ɬiʔa % !! Earth atm !! Earth % !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! Total Pressure &lt;br /&gt;
| 1.6 atm || || 1.0 atm || || Enhanced convective heat transfer, increased IR trapping&lt;br /&gt;
|-&lt;br /&gt;
! Nitrogen (N₂) &lt;br /&gt;
| 1.00 || 62.50% || 0.7808 || 78.08% || Reduced; still inert, still dominant&lt;br /&gt;
|-&lt;br /&gt;
! Oxygen (O₂) &lt;br /&gt;
| 0.21 || 13.13% || 0.2095 || 20.95% || Earth-normal partial pressure &lt;br /&gt;
|-&lt;br /&gt;
! Argon (Ar)&lt;br /&gt;
| 0.40 || 25.00% || 0.0093 || 0.93% || Major heat distribution enhancement, inert&lt;br /&gt;
|-&lt;br /&gt;
! Krypton + Xenon&lt;br /&gt;
| 0.005 || 0.31% || trace || trace || High molecular mass → improved heat retention, still safe&lt;br /&gt;
|-&lt;br /&gt;
! CO₂&lt;br /&gt;
| 0.005 || 0.31% || 0.004 || 0.04% || slightly elevated; sub-greenhouse threshold&lt;br /&gt;
|-&lt;br /&gt;
! H₂O vapor &lt;br /&gt;
| 0.015 || ~1% || || 0-4% || Maintains greenhouse without excess moisture&lt;br /&gt;
|}&lt;br /&gt;
==== Atmospheric Effects on Clouds ====&lt;br /&gt;
# Increased Pressure (1.6 atm) compresses gases, raising the dew point at which water vapor condenses. Clouds form closer to the surface, and are denser than similar altitudes compared to Earth.&lt;br /&gt;
# Low Water Inventory (~20% of Earth&#039;s): less frequent and less massive cloud systems than on Earth, but still present—especially over &amp;quot;hotspots&amp;quot; on the day side.&lt;br /&gt;
# Tidally Locked Climate: Cloud formation concentrate along the substellar point, where warm, moist air rises and cools.&lt;br /&gt;
#* A permanent “eyewall” storm system has formed at the subsolar point, like a giant hurricane.&lt;br /&gt;
#* As air rises and is advected to the night side, thin cloud bands or ice hazes form as it descends and cools.&lt;br /&gt;
&lt;br /&gt;
Appearance:&lt;br /&gt;
* The presence of noble gases (Ar, Kr, Xe) and higher pressure enhance Mie scattering, making clouds appear whiter and more silvered, especially at sunrise/sunset boundaries.&lt;br /&gt;
* Night side clouds are thin, high-altitude icy sheets, glowing faintly in aurorae or thermal emissions.&lt;br /&gt;
&lt;br /&gt;
==== Sky Color ====&lt;br /&gt;
The color of the sky is shaped by Rayleigh scattering, which depends on:&lt;br /&gt;
# Molecular composition: Heavier gases like Ar, Kr, and Xe scatter light less efficiently than N₂.&lt;br /&gt;
# Spectral output of the star: the red dwarf emits predominantly infrared and red light, with very little blue or violet.&lt;br /&gt;
&lt;br /&gt;
Consequence:&lt;br /&gt;
* Even with atmospheric scattering, there is insufficient blue light in the stellar spectrum to produce a blue sky.&lt;br /&gt;
* Day sky would likely appear:&lt;br /&gt;
** Dark peach, dusky rose, or reddish beige near zenith,&lt;br /&gt;
** Grading to deep salmon or mauve near the horizon,&lt;br /&gt;
** A slight metallic sheen due to noble gas content and high pressure.&lt;br /&gt;
&lt;br /&gt;
Twilight &amp;amp; Limb Scattering:&lt;br /&gt;
* The terminator (twilight zone) sees a diffuse, ruddy light, scattering through haze and clouds into luminous reds, purples, and copper tones.&lt;br /&gt;
* Aurorae are spectacular on the night side, especially since stellar flares are frequent.&lt;br /&gt;
&lt;br /&gt;
==== Sound Propagation ====&lt;br /&gt;
: &#039;&#039;Sound is profoundly affected by atmospheric pressure and composition.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Compared to Earth:&lt;br /&gt;
* Higher pressure → greater air density → faster transmission of sound and less attenuation.&lt;br /&gt;
* Argon and Xenon are heavy gases, which:&lt;br /&gt;
** Lower the speed of sound relative to air at the same pressure (despite the pressure increase).&lt;br /&gt;
** Shift resonance frequencies downward, resulting in deeper, rounder sounds.&lt;br /&gt;
&lt;br /&gt;
Consequences:&lt;br /&gt;
* Voices sound subtly lower-pitched and richer, especially for consonants and low vowels.&lt;br /&gt;
* Ambient sounds (wind, water, animals) would carry farther and sound more muffled or sonorous.&lt;br /&gt;
* Music or speech would resonate more warmly, especially indoors or in enclosed spaces.&lt;br /&gt;
&lt;br /&gt;
In short: it sounds like it’s wrapped in velvet.&lt;br /&gt;
&lt;br /&gt;
==== Heat Transport to the Night Side ====&lt;br /&gt;
Mechanisms:&lt;br /&gt;
# Thick Atmosphere (1.6 atm) increases:&lt;br /&gt;
#* Advection efficiency: Warm air masses can move more heat horizontally.&lt;br /&gt;
#* Radiative time constant: The atmosphere holds heat longer before releasing it.&lt;br /&gt;
# Noble Gases (especially Kr/Xe):&lt;br /&gt;
#* High molecular mass → more IR opacity → trapping and radiating heat more evenly.&lt;br /&gt;
# Slow Rotation / Tidal Locking:&lt;br /&gt;
#* Global Hadley-like cells dominate circulation, carrying warm air from the day side to the night side and descending it there.&lt;br /&gt;
&lt;br /&gt;
Result:&lt;br /&gt;
* The night side is not so freezing.  Temperatures differ by tens of degrees, not hundreds.&lt;br /&gt;
* There are still ice caps and a cold deserts at the anti-stellar point, but not a glaciated wasteland.&lt;br /&gt;
&lt;br /&gt;
=== Magnetosphere ===&lt;br /&gt;
* Larger mass --&amp;gt; larger iron core, generating more internal heat&lt;br /&gt;
* Larger radius --&amp;gt; Vigorous convection in the core&lt;br /&gt;
* Tidal Flexing --&amp;gt; still drives magnetic activity&lt;br /&gt;
&lt;br /&gt;
# Aurorae at lower latitudes&lt;br /&gt;
## higher magnetic rigidity, wider magnetotail, and greater reconnection energy.&lt;br /&gt;
## Combined with a higher flux of stellar particles, this means:&lt;br /&gt;
### Auroral ovals expand, reaching mid-latitudes sometimes equator.&lt;br /&gt;
### The skies are alive with rippling green, violet, and crimson aurorae, especially on the night side.&lt;br /&gt;
### Daily auroral activity occur during stellar flare cycles.&lt;br /&gt;
# Compasses&lt;br /&gt;
## compasses respond more sharply, with:&lt;br /&gt;
### Faster alignment.&lt;br /&gt;
### Greater resistance to local perturbations.&lt;br /&gt;
## However, frequent magnetic storms from stellar activity cause sudden declinations, reversals, or local anomalies.  In short, lots of aurorae equals dead compasses at the same time.&lt;br /&gt;
# Magnetic Field Strength &amp;gt; 100 μT &lt;br /&gt;
# Electromagnetism is more basic than chemistry or almost any other natural philosophy&lt;br /&gt;
&lt;br /&gt;
=== Substellar Point ===&lt;br /&gt;
The maximum incoming flux is very nearly the same as Earth&#039;s solar constant (≈1361 W/m²), but concentrated over one point rather than averaged over a rotating sphere.  Temperatures should be above 500ºK most of the time.  &lt;br /&gt;
&lt;br /&gt;
The magnetic north is also here. The thick atmosphere prevents too much loss here, but &lt;br /&gt;
* Charged particle influx&lt;br /&gt;
** Maximized at the substellar point—intense auroral and energetic particle precipitation&lt;br /&gt;
* Atmospheric ionization&lt;br /&gt;
** Constant production of high-energy ions and NOx compounds—UV fluorescence in upper sky&lt;br /&gt;
* Localized heating&lt;br /&gt;
** Augments already extreme temperatures—600–700 K surface&lt;br /&gt;
&lt;br /&gt;
== Artificially Tethered Moon ==&lt;br /&gt;
* 670,000 km up&lt;br /&gt;
* 7805 km in radius = same as the planet&lt;br /&gt;
* 1.33º of the sky, same as the sun&lt;br /&gt;
&lt;br /&gt;
A network of tethers/tension lines from the moon to multiple anchor points on the planet’s surface (a tripod or hexapod structure), woven like hair&lt;br /&gt;
* Uses active tension management and orbital station-keeping to stabilize the moon&lt;br /&gt;
* Counterweights and inward-pointing mass drivers on the moon to oppose drift&lt;br /&gt;
&lt;br /&gt;
The tethers are not bearing the full weight, but merely damping drift, providing restoring force, and enabling long-term stability through active compensation.  The moon&lt;br /&gt;
* Blocks the worst of the heat&lt;br /&gt;
* Blocks the worst of the solar radiation&lt;br /&gt;
The moon has &lt;br /&gt;
* low mass&lt;br /&gt;
* high albedo - enormous reflectivity&lt;br /&gt;
* scatters charges particles, UV, X-rays, auroral flux tubes&lt;br /&gt;
* sunward - crazy hot, high emissivity&lt;br /&gt;
* earthward - crazy cool, low emissivity&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=File:Ringed_Neptune_with_four_moons.png&amp;diff=168162</id>
		<title>File:Ringed Neptune with four moons.png</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=File:Ringed_Neptune_with_four_moons.png&amp;diff=168162"/>
		<updated>2025-03-27T23:36:13Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: mini neptune&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Summary ==&lt;br /&gt;
mini neptune&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168161</id>
		<title>Ɬiʔa/Conworlding</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168161"/>
		<updated>2025-03-27T23:19:53Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* e: The Tortured Near-Sphere */ pic&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Star ==&lt;br /&gt;
Our star is a red-dwarf.&lt;br /&gt;
# Type: M5V&lt;br /&gt;
## M: This indicates it&#039;s a cool, red star with a surface temperature less than 3,500ºK&lt;br /&gt;
## 5: Within the M class, stars are further divided into subclasses 0-9, with 0 being the hottest and 9 the coolest. An M5 star is in the middle of this range.&lt;br /&gt;
## V: Denotes that it&#039;s a main sequence star, also known as a dwarf star&lt;br /&gt;
# Stellar luminosity (L*) ≈ 0.01 𝐿⊙ (1/100th Sol&#039;s brightness)&lt;br /&gt;
# Stellar mass (M*) ≈ 0.2 𝑀⊙ (1/5 the mass of Sol)&lt;br /&gt;
# Stellar radius (R*) ≈ 0.25 𝑅⊙ (1/4 as wide as Sol)&lt;br /&gt;
# Effective temperature (T*) ≈ 3500 K&lt;br /&gt;
​The habitable zone (a) is about square root of L* over L⊙, so ~0.1 AU.&lt;br /&gt;
&lt;br /&gt;
=== Solar System ===&lt;br /&gt;
There are seven planets in the system&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Planet !!	Mass (M🜨)!!	Radius (R🜨)!! Moons/Rings	!!Resonance !!	Semi-Major Axis (AU)!!	Rings !! Moons !! Period !! Size&lt;br /&gt;
|-&lt;br /&gt;
| b ||	2.17 ||	1.1 ||	No ||	2:3 with c	|| 0.0763 ||	No || No || 17.2 || 13.6&#039; to 1.5&#039;&lt;br /&gt;
|-&lt;br /&gt;
| c ||	1.5	 ||1.225 ||	1* ||	—	        || 0.100 || No || No || 25.8 || -&lt;br /&gt;
|-&lt;br /&gt;
| d ||	2.0	 ||1.4 ||No ||	2:3 with c	 ||0.131 ||	No || No || 38.7 || 13.1&#039; to 1.8&#039;&lt;br /&gt;
|-&lt;br /&gt;
| e ||	0.9 ||	1.0 || No	 ||	2:3 with d	 ||0.172 ||	No || No || 58 || 4.1&#039; to 1.1&#039;&lt;br /&gt;
|-&lt;br /&gt;
| f ||	3.5 ||	2.0 ||	Yes! ||	2:3 with e	 ||0.227 || Yes || Junk || 87 || 4.6&#039; to 1.8&#039;&lt;br /&gt;
|-&lt;br /&gt;
| g ||	2.6 ||	1.7 ||	2 ||	-	 ||0.40 ||	Yes || Junk || 206 || 1.6&#039; to 1.0&#039;&lt;br /&gt;
|-&lt;br /&gt;
| h ||	5.0x2 ||2.3x2 || yes	 || -	 ||1.5 ||	Yes || No || 1500 || 0.5&#039; 16.4&#039; apart (at max)&lt;br /&gt;
|}&lt;br /&gt;
==== b: super Mercury with a ring of fire  ====&lt;br /&gt;
[[File:planet b by GPT.png|thumb|right|An artistic rendering of planet b]]&lt;br /&gt;
b is a super-Mercury, tidally locked, and incredibly dense.  ~700ºK on the day side, ~50ºK on the night.  2.1 Earth Masses, 1.1 Earth radii (~7000km) in size.  Orbital period 17.2 days.  Density 9.0 g/cm&amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt;.  Gravity is ~1.8g.  &lt;br /&gt;
&lt;br /&gt;
The iron core is huge, being 75% of the mass.  A thin silicate mantle, with metallic plains and exhumed ultramafic crust, with frequent iron meteorite craters, lacking typical “stone” breccias.&lt;br /&gt;
&lt;br /&gt;
The night side is intense, as simple hydrocarbons (methane, ethane, propane) condense and freeze into layered deposits.  Complex organics (tholins, polycyclic aromatics) accumulate on the sea floor, under miles of nitrogen ice.  Massive slush layers slosh around above cryovolcanic brines of ammonia.&lt;br /&gt;
&lt;br /&gt;
There is a crucial layer of Superionic Ice XI above the core, which acts as an electromagnetic insulator, and ionic heat bridge.  The crust is ultramafic silicates (olivine, pyroxene, perovskite) riddled with with sulfide veins, iron alloys, and graphite networks.  The poles of the magnetosphere are sideways, like Uranus, with poles at the equator in the Terminator Zone.  Persistent surface charges develop, because the whole planet is basically a ginormous Leyden jar!&lt;br /&gt;
&lt;br /&gt;
A planetary flux rope forms and un-forms with the star and planet b.  This induces electric jets at the terminator.  This is where temps are Earth-like.  Hydrocarbons sublimate and eject into the atmosphere, even while aurorae come right down to the ground.  A small, low pressure atmosphere prevents photodissociation, even while electrothermal instabilities lift molecules, forming an anomalous haze, a standing, glowing ring.  Coronal events cause localized lightning geysers with magnetic arcing.&lt;br /&gt;
&lt;br /&gt;
In short, b is visible with a blinding bright sun side (glowing orange bronze), a utterly black night side, and a burning, glowing, erupting, arcing ring at the terminator (all colors).  At biggest, it&#039;s half the size of Earth&#039;s moon in the sky, shrinking down to a star at it&#039;s furthest away.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== d: the wet eye with depths ====&lt;br /&gt;
[[File:wet eye planet.png|thumb|right|An reasonable approximation of d&#039;s appearance]]&lt;br /&gt;
From the outside, d is a &amp;quot;wet eye&amp;quot; just outside the habitable zone.  It is a water world, twice the mass of Earth, 1.4 times the radius, tidally locked.  The substellar point is the only place without surface ice.  However, it is better to think of the planet top-to-bottom.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;atmosphere&#039;&#039;&#039; is tenuous, less than 0.2 bars.  It is thin, N₂-rich with traces of H₂O, NH₃ vapor, and transient geyser outputs.  It is highly UV-irradiated, and Mars-like in its inability to retain volatiles.&lt;br /&gt;
&lt;br /&gt;
Next, there is a &#039;&#039;&#039;surface ice shell&#039;&#039;&#039;, ~20 km of thick Ice I.  Swirling currents beneath have cracked continent-sized ice plates, similar to Europa&#039;s crust.  It is permanently frozen except at the substellar furnace.  It accumulates chemical stains, mineral deposits, and cryovolcanic eruption plumes.  Accumulations of complex hydrates—like methanol clathrates—precipitate out and form false reefs, rising like coral from beneath. Transient thermal vents push hot plumes into the thin air, freezing instantly and snowing down crystals that form mineral spires.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;subglacial ocean&#039;&#039;&#039; is hundreds of kilometers thick.  It is super-pressurized liquid H₂O mixed with NH₃, CH₃OH, H₂O₂, and trace salts.  The movement is slow, planetary-scale currents originating from the Furnace and Coriolis force.  Strong layers exist: the surface is oxidized; the abyssal layer is reducing.&lt;br /&gt;
&lt;br /&gt;
A new &amp;quot;surface&amp;quot; is next.  The &#039;&#039;&#039;Ice Mantle&#039;&#039;&#039; is solid Ice VI and VII.  There are massive, slowly shifting &amp;quot;sub-oceanic continents&amp;quot;. It is periodically fractured and resurfaced by cryoquakes and brine-driven eruptions.  Some regions have developed elevated domes or ridges, continental “shelves” under the ocean.&lt;br /&gt;
&lt;br /&gt;
Finally, underneath is the &#039;&#039;&#039;core&#039;&#039;&#039;. Temperatures exceed 2000–3000 K locally.  Pressures range from 100 to 300 GPa.  The core is rich in heavy elements.  This makes radiogenic hotspots, localized magnetic eddies.  Heat gradients + ion flows = thermoelectric currents.  These make magnetic storms within the ocean itself, not the sky.  When uranium-rich corium pods shift or explode upward through the mantle, their heat and conductivity disturb the local magnetic field, generating geomagnetic quakes.  These pulse through the ocean, creating short-lived magnetic lenses.  These interact with atmospheric charged particles above the Furnace, giving rise to transient magnetic halos visible from orbit—false auroras without a sunstorm.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== e: The Tortured Near-Sphere ====&lt;br /&gt;
[[File:Blasting and shattered.png|thumb|right|An axial recoil event in progress]]&lt;br /&gt;
Orbital and Physical Characteristics&lt;br /&gt;
* Mass: 0.9 Earth masses&lt;br /&gt;
* Radius: 1.0 Earth radii&lt;br /&gt;
* Orbital Period: 58 Earth days&lt;br /&gt;
* Surface Gravity: ~0.9 g&lt;br /&gt;
* Semimajor Axis: ~0.17 AU &lt;br /&gt;
* Spin State: In the &#039;&#039;process&#039;&#039; of becoming tidally locked&lt;br /&gt;
* Obliquity: Extreme, experiencing chaotic realignment events&lt;br /&gt;
&lt;br /&gt;
Internal Structure and Composition&lt;br /&gt;
* &#039;&#039;&#039;Crust:&#039;&#039;&#039; A thick, rigid outer shell of water ice I mixed with clathrates (CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; and CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; hydrates), underlain by layers of ammonia-water ice eutectics. Inclusions of carbon under extreme pressure form diamond strata in the lower crust, lending rigidity and brittle behavior.&lt;br /&gt;
* &#039;&#039;&#039;Mantle:&#039;&#039;&#039; Comprised of Ice VI and Ice VII, with ammonia- and methane-rich brines forming localized conduits and pockets of unstable volatiles.&lt;br /&gt;
* &#039;&#039;&#039;Core:&#039;&#039;&#039; Differentiated and semi-molten. Inner core of iron-nickel alloy spins at a different rate. Outer core is a highly viscous slurry of silicate, iron, carbon, sulfur, and dissolved volatiles. Chemical veins (e.g., uranium silicates, perovskites) act as mechanical shear zones. Tidal torque leads to periodic frictional heating.&lt;br /&gt;
&lt;br /&gt;
Tectonic and Cryovolcanic Behavior&lt;br /&gt;
* The planet resists tidal locking due to core-crust decoupling and uneven angular momentum transfer.&lt;br /&gt;
* High obliquity experiences &#039;&#039;&#039;&#039;&#039;Axial Recoil Events&#039;&#039;&#039;&#039;&#039;, where the entire planet jerks between metastable orientations (e.g., from 110° to 70°) in sudden spasms.&lt;br /&gt;
* These events generate:&lt;br /&gt;
** Global-scale crustal cracking&lt;br /&gt;
** Venting of pressurized subsurface gases (H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;O, CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt;)&lt;br /&gt;
** Surface deformation and glacial faulting&lt;br /&gt;
* Volatiles erupt ballistically into space (200+lm) from exposed fissures and calderas, driven by phase-change explosions.&lt;br /&gt;
&lt;br /&gt;
Surface Conditions&lt;br /&gt;
* Global temperature well below freezing; warmest zones around cryovolcanic hotspots&lt;br /&gt;
* Crustal coloration varies by volatile deposition:&lt;br /&gt;
** Pale blue-white from water ice&lt;br /&gt;
** Red-brown from CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; frostfields&lt;br /&gt;
** Green-black CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; stains from plume fallout&lt;br /&gt;
* Surface features include:&lt;br /&gt;
** Cryovolcanic calderas&lt;br /&gt;
** Diamond-studded impact-like basins&lt;br /&gt;
** Faulted plains crossed by salt-streaked rift zones&lt;br /&gt;
&lt;br /&gt;
Atmosphere and Ejected Material&lt;br /&gt;
* Thin transient exosphere formed from eruptive events&lt;br /&gt;
* Gases often escape to space or freeze back out in polar regions&lt;br /&gt;
* Fallback material creates uneven surface mass distributions, altering moment of inertia and prolonging instability&lt;br /&gt;
&lt;br /&gt;
Appearance from Planet c&lt;br /&gt;
&lt;br /&gt;
* Angular Size: ~4-1 arcminutes&lt;br /&gt;
* Coloration: Overall dusky grey-white, with changing colored bands due to volatile fallout; craterless but mottled&lt;br /&gt;
&lt;br /&gt;
Transient visible phenomena:&lt;br /&gt;
&lt;br /&gt;
* Cryovolcanic plumes visible as fan-like arcs at the limb during outburst events&lt;br /&gt;
* Infrared brightening during Axial Recoil Events&lt;br /&gt;
* Occasional light-scattering halos from plume particles&lt;br /&gt;
&lt;br /&gt;
Event Cycle Summary&lt;br /&gt;
&lt;br /&gt;
# Tidal torque builds due to obliquity misalignment&lt;br /&gt;
# Core resists, crust locks tension&lt;br /&gt;
# Critical stress threshold breached&lt;br /&gt;
# Obliquity lurches to new orientation&lt;br /&gt;
# Crust fractures globally, vents open&lt;br /&gt;
# Supersonic cryovolcanism hurls volatiles into space&lt;br /&gt;
# Fallback modifies crustal mass distribution&lt;br /&gt;
# Obliquity rebuilds instability over decades&lt;br /&gt;
# Repeat.&lt;br /&gt;
&lt;br /&gt;
Planet e is a tortured world caught in an unending cycle of self-correcting failure—its body unable to align, its gases unable to stay contained, its appearance in the sky a visible signature of internal catastrophe.&lt;br /&gt;
&lt;br /&gt;
==== f: Ringed Mini-Neptune ====&lt;br /&gt;
This planet is a substantial mini-Neptune, with a mass of approximately 3.5 Earth masses and a radius of 2.0 Earth radii, orbiting at 0.227 AU. Its low mean density (~0.44 ρ⊕) signals the presence of a deep, volatile-rich envelope overlying a denser core. The bulk of its volume is composed of hydrogen and helium, accreted from the protoplanetary disk, with trace amounts of methane (CH₄) and ammonia (NH₃)—gases that dominate its photochemical and radiative behavior. Beneath this envelope, the planet hosts a water–rock–metal core layered in complex phases, with high-pressure ices and possibly superionic water enveloping a metallic center.  Lower atmosphere reaches 300–500 K (27–227°C) near the bottom of the troposphere, depending on opacity and convection.&lt;br /&gt;
&lt;br /&gt;
Visually, the planet exhibits a blue-to-cyan atmospheric hue, governed by Rayleigh scattering and methane absorption in the red and near-infrared spectrum. While not as banded or storm-laced as Jupiter, it features broad zonal flows, high-altitude methane ice clouds, and long-lived anticyclonic storms akin to Neptune’s Great Dark Spot. Due to its tidal locking to the host star, the planet presents hemispheric climatic asymmetry: a sunlit dayside prone to atmospheric upwelling and cloud formation, and a cooler, darker nightside. While colder, the backside is not freezing— in the 150–250 K range, depending on circulation efficiency. Atmospheric circulation is dominated by slow, large-scale overturning cells, moderated by planetary-scale waves and a subdued Coriolis force. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Rings =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Ring!!	Range (Rₚ)!!	Approx.! Range (km)!!	Description&lt;br /&gt;
|-&lt;br /&gt;
! C&lt;br /&gt;
| 	1.5–1.65 Rₚ	||19,100–21,000	||Faint, dusty interior ring&lt;br /&gt;
|-&lt;br /&gt;
! B&lt;br /&gt;
| 	1.65–1.96 Rₚ	||21,000–25,000||	Bright, dense primary ring&lt;br /&gt;
|-&lt;br /&gt;
! Division&lt;br /&gt;
|	1.96–2.04 Rₚ ||25,000–26,000 || a low-density gap&lt;br /&gt;
|-&lt;br /&gt;
!  A&lt;br /&gt;
|	2.04–2.3 Rₚ||26,000–29,300||	Sharp-edged outer ring&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Moon !!	Orbit (km) !!	Orbit (Rₚ) !!	Diameter (km) !!	Type	!! Period !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! I&lt;br /&gt;
|	60,000	||4.7 Rₚ	||~400	||Rocky	|| 0.9 ||Cratered&lt;br /&gt;
|-&lt;br /&gt;
! II&lt;br /&gt;
| 	110,000	|| 8.6 Rₚ	|| ~800	|| Mixed rock/ice	|| 2.25|| Cracked surface, frozen ocean&lt;br /&gt;
|-&lt;br /&gt;
! III &lt;br /&gt;
| 190,000	|| 14.9 Rₚ ||	~1200 ||	Icy major moon ||	5.1|| Cryovolcanism, smooth plains&lt;br /&gt;
|-&lt;br /&gt;
! IV &lt;br /&gt;
|340,000	||26.7 Rₚ	||~200	||Irregular/prograde	|| 12.21 || Dark red/carbon, inclined (20º, eccentric orbit (0.1)&lt;br /&gt;
|-&lt;br /&gt;
! V &lt;br /&gt;
| 710,000 ||	55.7 Rₚ	||~350	|| Captured/retrograde	|| 36.83 || Highly inclined (130º), Split terrain—half rugged highlands, half smooth resurfaced plain&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==== g: Stripped Sub-Neptune Remnant ====&lt;br /&gt;
&lt;br /&gt;
Basic Parameters&lt;br /&gt;
* Mass: 2.6 Earth masses (M⊕)&lt;br /&gt;
* Radius: 1.7 Earth radii (R⊕)&lt;br /&gt;
* Mean Density: ~2.92 g/cm³&lt;br /&gt;
* Orbital Distance: 0.4 AU &lt;br /&gt;
* Albedo: ~0.5 (moderately high)&lt;br /&gt;
* Rotation: Tidally locked &lt;br /&gt;
&lt;br /&gt;
Origin and Evolution&lt;br /&gt;
* Formed beyond the snow line (~0.8–1.2 AU) from a mix of rock, iron, and ices&lt;br /&gt;
* Migrated inward early during protoplanetary disk phase&lt;br /&gt;
* Accreted a modest hydrogen-helium envelope (&amp;gt;1% by mass)&lt;br /&gt;
* Exposed to intense stellar X-ray and UV radiation during the M dwarf&#039;s pre-main-sequence phase&lt;br /&gt;
* Lacked a magnetic dynamo (metal-poor and early core freezing)&lt;br /&gt;
* Entire atmosphere lost over ~100 Myr via photoevaporation, core-powered mass loss, and sputtering&lt;br /&gt;
&lt;br /&gt;
Current State&lt;br /&gt;
* Atmosphere: None (trace mineral vapors possible in hot regions)&lt;br /&gt;
* Surface: Stark contrast between hemispheres due to tidal locking&lt;br /&gt;
** Dayside: ~700–1000 K; high-silica lava fields, salt flats, exposed alumino-silicates&lt;br /&gt;
** Nightside: ~100–150 K; gypsum and calcite in cold traps, frozen regolith&lt;br /&gt;
* Magnetosphere: Absent&lt;br /&gt;
* Volcanism:episodic; high-silica flows, volcanic glass, sodium-rich crusts&lt;br /&gt;
* Geological Activity: Tectonically inactive; thermally fractured plains, impact craters&lt;br /&gt;
&lt;br /&gt;
Surface Composition&lt;br /&gt;
* Titanium dioxide (rutile): bright, high-albedo mineral condensate&lt;br /&gt;
* Calcite (CaCO₃): carbonate deposits in cold traps&lt;br /&gt;
* Gypsum (CaSO₄·2H₂O): hydration mineral, stable only on the nightside&lt;br /&gt;
* Sodium chloride: salt flats, especially in evaporated basins&lt;br /&gt;
* High-silica volcanic deposits: glassy, oxidized, and light-colored&lt;br /&gt;
&lt;br /&gt;
Visual and Observational Notes&lt;br /&gt;
&lt;br /&gt;
* High visual contrast between molten and frozen hemispheres&lt;br /&gt;
* Surface appears mottled: obsidian-black lava, gleaming salt flats, white calcium deposits&lt;br /&gt;
* No clouds, auroras, or magnetic activity&lt;br /&gt;
* Extreme day/night temperature gradient&lt;br /&gt;
* Reflective phase curve possible in photometric observations&lt;br /&gt;
* Surface pressure: effectively 0 bar&lt;br /&gt;
&lt;br /&gt;
Planet g is the airless skeleton of a once-sub-Neptune world. Born icy and distant, it migrated into the young star&#039;s wrath, where its fragile envelope boiled away under a sky of flares. Bereft of a magnetic shield, it was slowly stripped to bare rock. Today, one hemisphere bakes in molten silence while the other freezes in shadow. No air, no oceans, only salt, stone, and the echo of a lost atmosphere.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property !!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~75,000 km (~0.26 R&amp;lt;sub&amp;gt;hill&amp;lt;/sub&amp;gt;)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~1,400 km (~0.22 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass	&lt;br /&gt;
| ~0.01 M⊕ (~1.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~3.0 g/cm³ (rock–ice mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temp&lt;br /&gt;
|	~150–180 K&lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
| 0.20g&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere&lt;br /&gt;
|	Trace O₂, from radiolysis and outgassing&lt;br /&gt;
|-&lt;br /&gt;
! Subsurface Ocean&lt;br /&gt;
|	heated by tidal flexing&lt;br /&gt;
|-&lt;br /&gt;
! Surface Features	&lt;br /&gt;
|Fractured ice crust, chaos terrain, cryogeysers, lenticulae&lt;br /&gt;
|}&lt;br /&gt;
gI is a cracked glass orb, rimed with frost and laced with luminous fissures. Below its crust, tides flex a hidden ocean in rhythmic silence. Its faint oxygen exosphere is ghostly but present.  It is frosted quartz with cobwebbed streaks and mineral discoloration.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property!!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~150,000 km (~0.5 Rₕill)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~2,100 km (~0.33 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass&lt;br /&gt;
|	~0.035 M⊕ (~4.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~2.1 g/cm³ (icy-rocky mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes &lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
|	~0.35 g&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temperature&lt;br /&gt;
|	~115–130 K (pressure and greenhouse effects)&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere	&lt;br /&gt;
| ~0.18 bar N₂ + ~0.1 bar Ar + ~0.02 bar CH₄, minor CO, trace haze &lt;br /&gt;
|}&lt;br /&gt;
gII is a muted blue-green crescent veiled in gold. Its sky glows with the weight of argon and the shimmer of methane haze, and its surface smolders with the memory of internal warmth. Liquid hydrocarbons shine like ink in the basins, while glaciers ebb across the uplands. To the star it shows only one face, but beneath that still gaze lies the soft breath of a world more welcoming than its master.&lt;br /&gt;
&lt;br /&gt;
==== h ====&lt;br /&gt;
h is a twin-planet system, 1.5 AU from the star, with a period of 4.1 years&lt;br /&gt;
&lt;br /&gt;
Mutual Orbital Configuration&lt;br /&gt;
* Type: True binary planet pair, gravitationally bound, equal mass&lt;br /&gt;
* Masses: 5.0 M⊕ each&lt;br /&gt;
* Radii: 2.3 R⊕ each&lt;br /&gt;
* Mutual Orbit: Essentially circular, ~1 million km separation (~8–10 planetary radii)&lt;br /&gt;
* Period (mutual orbit): ~4.5 days&lt;br /&gt;
* Orbital Plane: Perpendicular to system ecliptic &lt;br /&gt;
* Tidal State: Tidally locked to each other (mutual synchronous rotation)&lt;br /&gt;
&lt;br /&gt;
Planet A — &amp;quot;Sapphire&amp;quot;&lt;br /&gt;
* Coloration: Deep sapphire blue with white high-altitude methane ice hazes&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: H₂, He&lt;br /&gt;
** Methane (CH₄): high&lt;br /&gt;
** Ammonia: trace&lt;br /&gt;
** Argon: moderate&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: slightly enriched&lt;br /&gt;
* Magnetosphere: Strong, symmetric; supports brilliant blue-violet aurorae&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Superionic water mantle&lt;br /&gt;
** Stratified silicate-ice alloy core&lt;br /&gt;
** Radiogenic heating and layered convection&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar hexagonal jet (stronger than Saturn&#039;s)&lt;br /&gt;
** Methane plasma flares at terminator&lt;br /&gt;
** Iridescent methane cirrus clouds&lt;br /&gt;
** Massive auroral crowns aligned with spin-magnetic axis misalignment&lt;br /&gt;
&lt;br /&gt;
Planet B — &amp;quot;Rust&amp;quot;&lt;br /&gt;
* Coloration: Dark crimson to rust-red, streaked with black and violet haze bands&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: N₂, CO&lt;br /&gt;
** CH₄: trace&lt;br /&gt;
** Tholins: abundant&lt;br /&gt;
** Argon: high&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: moderate&lt;br /&gt;
** Magnetosphere: Weak, multipolar and intermittent&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Dense iron-rich core with impact inclusions (e.g., iridium, ruthenium)&lt;br /&gt;
** Volcanically active mantle with carbon-rich inclusions&lt;br /&gt;
** Higher internal heat flow than Sapphire&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar cyclonic basins with geyser-like haze columns&lt;br /&gt;
** Frequent UV lightning within organic clouds&lt;br /&gt;
** Faint auroral echoes from Sapphire’s magnetospheric tail&lt;br /&gt;
** Surface glow from argon emissions during conjunction&lt;br /&gt;
&lt;br /&gt;
Mutual Phenomena &amp;amp; Sky Effects&lt;br /&gt;
* Eclipse Cycles: Frequent, due to short mutual period and perpendicular orbit; cause wave-like haze patterns and shadow bands&lt;br /&gt;
* Filamentary Atmosphere Bridges: Transient stratospheric strands near L1, illuminated during eclipses&lt;br /&gt;
* Auroral Flux Tubes: Occasionally connect the two with violet-green flickering arcs&lt;br /&gt;
* Gravitational Stability: Mutual orbit stable within Hill sphere; resistant to long-term disruption&lt;br /&gt;
&lt;br /&gt;
* Legacy of the Comet Shield&lt;br /&gt;
* Each planet’s core contains embedded relics of the system’s ancient bombardment:&lt;br /&gt;
** Sapphire: interstellar dust, primordial isotopes, deep xenon pockets&lt;br /&gt;
** Rust: impact-derived siderophiles, compressed organics, rare isotopic anomalies&lt;br /&gt;
* Capture Events: Both planets have intercepted and redirected hundreds of large icy bodies over system history&lt;br /&gt;
&lt;br /&gt;
They each have 2 small irregular moons, &amp;lt;100 km diameter, retrograde, on distant orbits.  Negligible.&lt;br /&gt;
== Planet C ==&lt;br /&gt;
&lt;br /&gt;
* With an albedo of 0.2, the global average temp is 263ºK.  Because of modest greenhouse effects, surface temperatures are higher, on the sun-side.&lt;br /&gt;
# Mass: 1.5M⊕&lt;br /&gt;
# Gravity: 1g⊕&lt;br /&gt;
# Radius = 1.225⊕, or 7805km&lt;br /&gt;
Terminator Zone&lt;br /&gt;
# +/-30º: 1.28 E8 km&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; (slightly less than all the land of the Earth)&lt;br /&gt;
# Escape velocity is 12.4km/s, 11% higher than Earth&lt;br /&gt;
# Orbital velocity is 8.79km/s&lt;br /&gt;
=== Atmosphere ===&lt;br /&gt;
Water content is low because&lt;br /&gt;
* Water vapor is a potent greenhouse gas; vast surface water can trap too much heat, especially near the substellar point.&lt;br /&gt;
* Water leads to climate homogenization&lt;br /&gt;
* Lack of exposed silicate rock: Necessary for carbon-silicate weathering feedback, which stabilizes climate on geological timescales.&lt;br /&gt;
Earth has ~1.4 billion km³ of water.  In our habitable zone, we have no more than 10% of that, or 100 million km³, though there is much more on the night side, both liquid and ice.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Factor !! Ɬiʔa atm !! Ɬiʔa % !! Earth atm !! Earth % !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! Total Pressure &lt;br /&gt;
| 1.6 atm || || 1.0 atm || || Enhanced convective heat transfer, increased IR trapping&lt;br /&gt;
|-&lt;br /&gt;
! Nitrogen (N₂) &lt;br /&gt;
| 1.00 || 62.50% || 0.7808 || 78.08% || Reduced; still inert, still dominant&lt;br /&gt;
|-&lt;br /&gt;
! Oxygen (O₂) &lt;br /&gt;
| 0.21 || 13.13% || 0.2095 || 20.95% || Earth-normal partial pressure &lt;br /&gt;
|-&lt;br /&gt;
! Argon (Ar)&lt;br /&gt;
| 0.40 || 25.00% || 0.0093 || 0.93% || Major heat distribution enhancement, inert&lt;br /&gt;
|-&lt;br /&gt;
! Krypton + Xenon&lt;br /&gt;
| 0.005 || 0.31% || trace || trace || High molecular mass → improved heat retention, still safe&lt;br /&gt;
|-&lt;br /&gt;
! CO₂&lt;br /&gt;
| 0.005 || 0.31% || 0.004 || 0.04% || slightly elevated; sub-greenhouse threshold&lt;br /&gt;
|-&lt;br /&gt;
! H₂O vapor &lt;br /&gt;
| 0.015 || ~1% || || 0-4% || Maintains greenhouse without excess moisture&lt;br /&gt;
|}&lt;br /&gt;
==== Atmospheric Effects on Clouds ====&lt;br /&gt;
# Increased Pressure (1.6 atm) compresses gases, raising the dew point at which water vapor condenses. Clouds form closer to the surface, and are denser than similar altitudes compared to Earth.&lt;br /&gt;
# Low Water Inventory (~20% of Earth&#039;s): less frequent and less massive cloud systems than on Earth, but still present—especially over &amp;quot;hotspots&amp;quot; on the day side.&lt;br /&gt;
# Tidally Locked Climate: Cloud formation concentrate along the substellar point, where warm, moist air rises and cools.&lt;br /&gt;
#* A permanent “eyewall” storm system has formed at the subsolar point, like a giant hurricane.&lt;br /&gt;
#* As air rises and is advected to the night side, thin cloud bands or ice hazes form as it descends and cools.&lt;br /&gt;
&lt;br /&gt;
Appearance:&lt;br /&gt;
* The presence of noble gases (Ar, Kr, Xe) and higher pressure enhance Mie scattering, making clouds appear whiter and more silvered, especially at sunrise/sunset boundaries.&lt;br /&gt;
* Night side clouds are thin, high-altitude icy sheets, glowing faintly in aurorae or thermal emissions.&lt;br /&gt;
&lt;br /&gt;
==== Sky Color ====&lt;br /&gt;
The color of the sky is shaped by Rayleigh scattering, which depends on:&lt;br /&gt;
# Molecular composition: Heavier gases like Ar, Kr, and Xe scatter light less efficiently than N₂.&lt;br /&gt;
# Spectral output of the star: the red dwarf emits predominantly infrared and red light, with very little blue or violet.&lt;br /&gt;
&lt;br /&gt;
Consequence:&lt;br /&gt;
* Even with atmospheric scattering, there is insufficient blue light in the stellar spectrum to produce a blue sky.&lt;br /&gt;
* Day sky would likely appear:&lt;br /&gt;
** Dark peach, dusky rose, or reddish beige near zenith,&lt;br /&gt;
** Grading to deep salmon or mauve near the horizon,&lt;br /&gt;
** A slight metallic sheen due to noble gas content and high pressure.&lt;br /&gt;
&lt;br /&gt;
Twilight &amp;amp; Limb Scattering:&lt;br /&gt;
* The terminator (twilight zone) sees a diffuse, ruddy light, scattering through haze and clouds into luminous reds, purples, and copper tones.&lt;br /&gt;
* Aurorae are spectacular on the night side, especially since stellar flares are frequent.&lt;br /&gt;
&lt;br /&gt;
==== Sound Propagation ====&lt;br /&gt;
: &#039;&#039;Sound is profoundly affected by atmospheric pressure and composition.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Compared to Earth:&lt;br /&gt;
* Higher pressure → greater air density → faster transmission of sound and less attenuation.&lt;br /&gt;
* Argon and Xenon are heavy gases, which:&lt;br /&gt;
** Lower the speed of sound relative to air at the same pressure (despite the pressure increase).&lt;br /&gt;
** Shift resonance frequencies downward, resulting in deeper, rounder sounds.&lt;br /&gt;
&lt;br /&gt;
Consequences:&lt;br /&gt;
* Voices sound subtly lower-pitched and richer, especially for consonants and low vowels.&lt;br /&gt;
* Ambient sounds (wind, water, animals) would carry farther and sound more muffled or sonorous.&lt;br /&gt;
* Music or speech would resonate more warmly, especially indoors or in enclosed spaces.&lt;br /&gt;
&lt;br /&gt;
In short: it sounds like it’s wrapped in velvet.&lt;br /&gt;
&lt;br /&gt;
==== Heat Transport to the Night Side ====&lt;br /&gt;
Mechanisms:&lt;br /&gt;
# Thick Atmosphere (1.6 atm) increases:&lt;br /&gt;
#* Advection efficiency: Warm air masses can move more heat horizontally.&lt;br /&gt;
#* Radiative time constant: The atmosphere holds heat longer before releasing it.&lt;br /&gt;
# Noble Gases (especially Kr/Xe):&lt;br /&gt;
#* High molecular mass → more IR opacity → trapping and radiating heat more evenly.&lt;br /&gt;
# Slow Rotation / Tidal Locking:&lt;br /&gt;
#* Global Hadley-like cells dominate circulation, carrying warm air from the day side to the night side and descending it there.&lt;br /&gt;
&lt;br /&gt;
Result:&lt;br /&gt;
* The night side is not so freezing.  Temperatures differ by tens of degrees, not hundreds.&lt;br /&gt;
* There are still ice caps and a cold deserts at the anti-stellar point, but not a glaciated wasteland.&lt;br /&gt;
&lt;br /&gt;
=== Magnetosphere ===&lt;br /&gt;
* Larger mass --&amp;gt; larger iron core, generating more internal heat&lt;br /&gt;
* Larger radius --&amp;gt; Vigorous convection in the core&lt;br /&gt;
* Tidal Flexing --&amp;gt; still drives magnetic activity&lt;br /&gt;
&lt;br /&gt;
# Aurorae at lower latitudes&lt;br /&gt;
## higher magnetic rigidity, wider magnetotail, and greater reconnection energy.&lt;br /&gt;
## Combined with a higher flux of stellar particles, this means:&lt;br /&gt;
### Auroral ovals expand, reaching mid-latitudes sometimes equator.&lt;br /&gt;
### The skies are alive with rippling green, violet, and crimson aurorae, especially on the night side.&lt;br /&gt;
### Daily auroral activity occur during stellar flare cycles.&lt;br /&gt;
# Compasses&lt;br /&gt;
## compasses respond more sharply, with:&lt;br /&gt;
### Faster alignment.&lt;br /&gt;
### Greater resistance to local perturbations.&lt;br /&gt;
## However, frequent magnetic storms from stellar activity cause sudden declinations, reversals, or local anomalies.  In short, lots of aurorae equals dead compasses at the same time.&lt;br /&gt;
# Magnetic Field Strength &amp;gt; 100 μT &lt;br /&gt;
# Electromagnetism is more basic than chemistry or almost any other natural philosophy&lt;br /&gt;
&lt;br /&gt;
=== Substellar Point ===&lt;br /&gt;
The maximum incoming flux is very nearly the same as Earth&#039;s solar constant (≈1361 W/m²), but concentrated over one point rather than averaged over a rotating sphere.  Temperatures should be above 500ºK most of the time.  &lt;br /&gt;
&lt;br /&gt;
The magnetic north is also here. The thick atmosphere prevents too much loss here, but &lt;br /&gt;
* Charged particle influx&lt;br /&gt;
** Maximized at the substellar point—intense auroral and energetic particle precipitation&lt;br /&gt;
* Atmospheric ionization&lt;br /&gt;
** Constant production of high-energy ions and NOx compounds—UV fluorescence in upper sky&lt;br /&gt;
* Localized heating&lt;br /&gt;
** Augments already extreme temperatures—600–700 K surface&lt;br /&gt;
&lt;br /&gt;
== Artificially Tethered Moon ==&lt;br /&gt;
* 670,000 km up&lt;br /&gt;
* 7805 km in radius = same as the planet&lt;br /&gt;
* 1.33º of the sky, same as the sun&lt;br /&gt;
&lt;br /&gt;
A network of tethers/tension lines from the moon to multiple anchor points on the planet’s surface (a tripod or hexapod structure), woven like hair&lt;br /&gt;
* Uses active tension management and orbital station-keeping to stabilize the moon&lt;br /&gt;
* Counterweights and inward-pointing mass drivers on the moon to oppose drift&lt;br /&gt;
&lt;br /&gt;
The tethers are not bearing the full weight, but merely damping drift, providing restoring force, and enabling long-term stability through active compensation.  The moon&lt;br /&gt;
* Blocks the worst of the heat&lt;br /&gt;
* Blocks the worst of the solar radiation&lt;br /&gt;
The moon has &lt;br /&gt;
* low mass&lt;br /&gt;
* high albedo - enormous reflectivity&lt;br /&gt;
* scatters charges particles, UV, X-rays, auroral flux tubes&lt;br /&gt;
* sunward - crazy hot, high emissivity&lt;br /&gt;
* earthward - crazy cool, low emissivity&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=File:Blasting_and_shattered.png&amp;diff=168160</id>
		<title>File:Blasting and shattered.png</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=File:Blasting_and_shattered.png&amp;diff=168160"/>
		<updated>2025-03-27T23:19:34Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: exoplanet&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Summary ==&lt;br /&gt;
exoplanet&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168159</id>
		<title>Ɬiʔa/Conworlding</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168159"/>
		<updated>2025-03-27T22:06:14Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* d: the wet eye with depths */ image&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Star ==&lt;br /&gt;
Our star is a red-dwarf.&lt;br /&gt;
# Type: M5V&lt;br /&gt;
## M: This indicates it&#039;s a cool, red star with a surface temperature less than 3,500ºK&lt;br /&gt;
## 5: Within the M class, stars are further divided into subclasses 0-9, with 0 being the hottest and 9 the coolest. An M5 star is in the middle of this range.&lt;br /&gt;
## V: Denotes that it&#039;s a main sequence star, also known as a dwarf star&lt;br /&gt;
# Stellar luminosity (L*) ≈ 0.01 𝐿⊙ (1/100th Sol&#039;s brightness)&lt;br /&gt;
# Stellar mass (M*) ≈ 0.2 𝑀⊙ (1/5 the mass of Sol)&lt;br /&gt;
# Stellar radius (R*) ≈ 0.25 𝑅⊙ (1/4 as wide as Sol)&lt;br /&gt;
# Effective temperature (T*) ≈ 3500 K&lt;br /&gt;
​The habitable zone (a) is about square root of L* over L⊙, so ~0.1 AU.&lt;br /&gt;
&lt;br /&gt;
=== Solar System ===&lt;br /&gt;
There are seven planets in the system&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Planet !!	Mass (M🜨)!!	Radius (R🜨)!! Moons/Rings	!!Resonance !!	Semi-Major Axis (AU)!!	Rings !! Moons !! Period !! Size&lt;br /&gt;
|-&lt;br /&gt;
| b ||	2.17 ||	1.1 ||	No ||	2:3 with c	|| 0.0763 ||	No || No || 17.2 || 13.6&#039; to 1.5&#039;&lt;br /&gt;
|-&lt;br /&gt;
| c ||	1.5	 ||1.225 ||	1* ||	—	        || 0.100 || No || No || 25.8 || -&lt;br /&gt;
|-&lt;br /&gt;
| d ||	2.0	 ||1.4 ||No ||	2:3 with c	 ||0.131 ||	No || No || 38.7 || 13.1&#039; to 1.8&#039;&lt;br /&gt;
|-&lt;br /&gt;
| e ||	0.9 ||	1.0 || No	 ||	2:3 with d	 ||0.172 ||	No || No || 58 || 4.1&#039; to 1.1&#039;&lt;br /&gt;
|-&lt;br /&gt;
| f ||	3.5 ||	2.0 ||	Yes! ||	2:3 with e	 ||0.227 || Yes || Junk || 87 || 4.6&#039; to 1.8&#039;&lt;br /&gt;
|-&lt;br /&gt;
| g ||	2.6 ||	1.7 ||	2 ||	-	 ||0.40 ||	Yes || Junk || 206 || 1.6&#039; to 1.0&#039;&lt;br /&gt;
|-&lt;br /&gt;
| h ||	5.0x2 ||2.3x2 || yes	 || -	 ||1.5 ||	Yes || No || 1500 || 0.5&#039; 16.4&#039; apart (at max)&lt;br /&gt;
|}&lt;br /&gt;
==== b: super Mercury with a ring of fire  ====&lt;br /&gt;
[[File:planet b by GPT.png|thumb|right|An artistic rendering of planet b]]&lt;br /&gt;
b is a super-Mercury, tidally locked, and incredibly dense.  ~700ºK on the day side, ~50ºK on the night.  2.1 Earth Masses, 1.1 Earth radii (~7000km) in size.  Orbital period 17.2 days.  Density 9.0 g/cm&amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt;.  Gravity is ~1.8g.  &lt;br /&gt;
&lt;br /&gt;
The iron core is huge, being 75% of the mass.  A thin silicate mantle, with metallic plains and exhumed ultramafic crust, with frequent iron meteorite craters, lacking typical “stone” breccias.&lt;br /&gt;
&lt;br /&gt;
The night side is intense, as simple hydrocarbons (methane, ethane, propane) condense and freeze into layered deposits.  Complex organics (tholins, polycyclic aromatics) accumulate on the sea floor, under miles of nitrogen ice.  Massive slush layers slosh around above cryovolcanic brines of ammonia.&lt;br /&gt;
&lt;br /&gt;
There is a crucial layer of Superionic Ice XI above the core, which acts as an electromagnetic insulator, and ionic heat bridge.  The crust is ultramafic silicates (olivine, pyroxene, perovskite) riddled with with sulfide veins, iron alloys, and graphite networks.  The poles of the magnetosphere are sideways, like Uranus, with poles at the equator in the Terminator Zone.  Persistent surface charges develop, because the whole planet is basically a ginormous Leyden jar!&lt;br /&gt;
&lt;br /&gt;
A planetary flux rope forms and un-forms with the star and planet b.  This induces electric jets at the terminator.  This is where temps are Earth-like.  Hydrocarbons sublimate and eject into the atmosphere, even while aurorae come right down to the ground.  A small, low pressure atmosphere prevents photodissociation, even while electrothermal instabilities lift molecules, forming an anomalous haze, a standing, glowing ring.  Coronal events cause localized lightning geysers with magnetic arcing.&lt;br /&gt;
&lt;br /&gt;
In short, b is visible with a blinding bright sun side (glowing orange bronze), a utterly black night side, and a burning, glowing, erupting, arcing ring at the terminator (all colors).  At biggest, it&#039;s half the size of Earth&#039;s moon in the sky, shrinking down to a star at it&#039;s furthest away.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== d: the wet eye with depths ====&lt;br /&gt;
[[File:wet eye planet.png|thumb|right|An reasonable approximation of d&#039;s appearance]]&lt;br /&gt;
From the outside, d is a &amp;quot;wet eye&amp;quot; just outside the habitable zone.  It is a water world, twice the mass of Earth, 1.4 times the radius, tidally locked.  The substellar point is the only place without surface ice.  However, it is better to think of the planet top-to-bottom.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;atmosphere&#039;&#039;&#039; is tenuous, less than 0.2 bars.  It is thin, N₂-rich with traces of H₂O, NH₃ vapor, and transient geyser outputs.  It is highly UV-irradiated, and Mars-like in its inability to retain volatiles.&lt;br /&gt;
&lt;br /&gt;
Next, there is a &#039;&#039;&#039;surface ice shell&#039;&#039;&#039;, ~20 km of thick Ice I.  Swirling currents beneath have cracked continent-sized ice plates, similar to Europa&#039;s crust.  It is permanently frozen except at the substellar furnace.  It accumulates chemical stains, mineral deposits, and cryovolcanic eruption plumes.  Accumulations of complex hydrates—like methanol clathrates—precipitate out and form false reefs, rising like coral from beneath. Transient thermal vents push hot plumes into the thin air, freezing instantly and snowing down crystals that form mineral spires.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;subglacial ocean&#039;&#039;&#039; is hundreds of kilometers thick.  It is super-pressurized liquid H₂O mixed with NH₃, CH₃OH, H₂O₂, and trace salts.  The movement is slow, planetary-scale currents originating from the Furnace and Coriolis force.  Strong layers exist: the surface is oxidized; the abyssal layer is reducing.&lt;br /&gt;
&lt;br /&gt;
A new &amp;quot;surface&amp;quot; is next.  The &#039;&#039;&#039;Ice Mantle&#039;&#039;&#039; is solid Ice VI and VII.  There are massive, slowly shifting &amp;quot;sub-oceanic continents&amp;quot;. It is periodically fractured and resurfaced by cryoquakes and brine-driven eruptions.  Some regions have developed elevated domes or ridges, continental “shelves” under the ocean.&lt;br /&gt;
&lt;br /&gt;
Finally, underneath is the &#039;&#039;&#039;core&#039;&#039;&#039;. Temperatures exceed 2000–3000 K locally.  Pressures range from 100 to 300 GPa.  The core is rich in heavy elements.  This makes radiogenic hotspots, localized magnetic eddies.  Heat gradients + ion flows = thermoelectric currents.  These make magnetic storms within the ocean itself, not the sky.  When uranium-rich corium pods shift or explode upward through the mantle, their heat and conductivity disturb the local magnetic field, generating geomagnetic quakes.  These pulse through the ocean, creating short-lived magnetic lenses.  These interact with atmospheric charged particles above the Furnace, giving rise to transient magnetic halos visible from orbit—false auroras without a sunstorm.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== e: The Tortured Near-Sphere ====&lt;br /&gt;
&lt;br /&gt;
Orbital and Physical Characteristics&lt;br /&gt;
* Mass: 0.9 Earth masses&lt;br /&gt;
* Radius: 1.0 Earth radii&lt;br /&gt;
* Orbital Period: 58 Earth days&lt;br /&gt;
* Surface Gravity: ~0.9 g&lt;br /&gt;
* Semimajor Axis: ~0.17 AU &lt;br /&gt;
* Spin State: In the &#039;&#039;process&#039;&#039; of becoming tidally locked&lt;br /&gt;
* Obliquity: Extreme, experiencing chaotic realignment events&lt;br /&gt;
&lt;br /&gt;
Internal Structure and Composition&lt;br /&gt;
* &#039;&#039;&#039;Crust:&#039;&#039;&#039; A thick, rigid outer shell of water ice I mixed with clathrates (CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; and CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; hydrates), underlain by layers of ammonia-water ice eutectics. Inclusions of carbon under extreme pressure form diamond strata in the lower crust, lending rigidity and brittle behavior.&lt;br /&gt;
* &#039;&#039;&#039;Mantle:&#039;&#039;&#039; Comprised of Ice VI and Ice VII, with ammonia- and methane-rich brines forming localized conduits and pockets of unstable volatiles.&lt;br /&gt;
* &#039;&#039;&#039;Core:&#039;&#039;&#039; Differentiated and semi-molten. Inner core of iron-nickel alloy spins at a different rate. Outer core is a highly viscous slurry of silicate, iron, carbon, sulfur, and dissolved volatiles. Chemical veins (e.g., uranium silicates, perovskites) act as mechanical shear zones. Tidal torque leads to periodic frictional heating.&lt;br /&gt;
&lt;br /&gt;
Tectonic and Cryovolcanic Behavior&lt;br /&gt;
* The planet resists tidal locking due to core-crust decoupling and uneven angular momentum transfer.&lt;br /&gt;
* High obliquity experiences &#039;&#039;&#039;&#039;&#039;Axial Recoil Events&#039;&#039;&#039;&#039;&#039;, where the entire planet jerks between metastable orientations (e.g., from 110° to 70°) in sudden spasms.&lt;br /&gt;
* These events generate:&lt;br /&gt;
** Global-scale crustal cracking&lt;br /&gt;
** Venting of pressurized subsurface gases (H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;O, CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt;)&lt;br /&gt;
** Surface deformation and glacial faulting&lt;br /&gt;
* Volatiles erupt ballistically into space (200+lm) from exposed fissures and calderas, driven by phase-change explosions.&lt;br /&gt;
&lt;br /&gt;
Surface Conditions&lt;br /&gt;
* Global temperature well below freezing; warmest zones around cryovolcanic hotspots&lt;br /&gt;
* Crustal coloration varies by volatile deposition:&lt;br /&gt;
** Pale blue-white from water ice&lt;br /&gt;
** Red-brown from CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; frostfields&lt;br /&gt;
** Green-black CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; stains from plume fallout&lt;br /&gt;
* Surface features include:&lt;br /&gt;
** Cryovolcanic calderas&lt;br /&gt;
** Diamond-studded impact-like basins&lt;br /&gt;
** Faulted plains crossed by salt-streaked rift zones&lt;br /&gt;
&lt;br /&gt;
Atmosphere and Ejected Material&lt;br /&gt;
* Thin transient exosphere formed from eruptive events&lt;br /&gt;
* Gases often escape to space or freeze back out in polar regions&lt;br /&gt;
* Fallback material creates uneven surface mass distributions, altering moment of inertia and prolonging instability&lt;br /&gt;
&lt;br /&gt;
Appearance from Planet c&lt;br /&gt;
&lt;br /&gt;
* Angular Size: ~4-1 arcminutes&lt;br /&gt;
* Coloration: Overall dusky grey-white, with changing colored bands due to volatile fallout; craterless but mottled&lt;br /&gt;
&lt;br /&gt;
Transient visible phenomena:&lt;br /&gt;
&lt;br /&gt;
* Cryovolcanic plumes visible as fan-like arcs at the limb during outburst events&lt;br /&gt;
* Infrared brightening during Axial Recoil Events&lt;br /&gt;
* Occasional light-scattering halos from plume particles&lt;br /&gt;
&lt;br /&gt;
Event Cycle Summary&lt;br /&gt;
&lt;br /&gt;
# Tidal torque builds due to obliquity misalignment&lt;br /&gt;
# Core resists, crust locks tension&lt;br /&gt;
# Critical stress threshold breached&lt;br /&gt;
# Obliquity lurches to new orientation&lt;br /&gt;
# Crust fractures globally, vents open&lt;br /&gt;
# Supersonic cryovolcanism hurls volatiles into space&lt;br /&gt;
# Fallback modifies crustal mass distribution&lt;br /&gt;
# Obliquity rebuilds instability over decades&lt;br /&gt;
# Repeat.&lt;br /&gt;
&lt;br /&gt;
Planet e is a tortured world caught in an unending cycle of self-correcting failure—its body unable to align, its gases unable to stay contained, its appearance in the sky a visible signature of internal catastrophe.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==== f: Ringed Mini-Neptune ====&lt;br /&gt;
This planet is a substantial mini-Neptune, with a mass of approximately 3.5 Earth masses and a radius of 2.0 Earth radii, orbiting at 0.227 AU. Its low mean density (~0.44 ρ⊕) signals the presence of a deep, volatile-rich envelope overlying a denser core. The bulk of its volume is composed of hydrogen and helium, accreted from the protoplanetary disk, with trace amounts of methane (CH₄) and ammonia (NH₃)—gases that dominate its photochemical and radiative behavior. Beneath this envelope, the planet hosts a water–rock–metal core layered in complex phases, with high-pressure ices and possibly superionic water enveloping a metallic center.  Lower atmosphere reaches 300–500 K (27–227°C) near the bottom of the troposphere, depending on opacity and convection.&lt;br /&gt;
&lt;br /&gt;
Visually, the planet exhibits a blue-to-cyan atmospheric hue, governed by Rayleigh scattering and methane absorption in the red and near-infrared spectrum. While not as banded or storm-laced as Jupiter, it features broad zonal flows, high-altitude methane ice clouds, and long-lived anticyclonic storms akin to Neptune’s Great Dark Spot. Due to its tidal locking to the host star, the planet presents hemispheric climatic asymmetry: a sunlit dayside prone to atmospheric upwelling and cloud formation, and a cooler, darker nightside. While colder, the backside is not freezing— in the 150–250 K range, depending on circulation efficiency. Atmospheric circulation is dominated by slow, large-scale overturning cells, moderated by planetary-scale waves and a subdued Coriolis force. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Rings =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Ring!!	Range (Rₚ)!!	Approx.! Range (km)!!	Description&lt;br /&gt;
|-&lt;br /&gt;
! C&lt;br /&gt;
| 	1.5–1.65 Rₚ	||19,100–21,000	||Faint, dusty interior ring&lt;br /&gt;
|-&lt;br /&gt;
! B&lt;br /&gt;
| 	1.65–1.96 Rₚ	||21,000–25,000||	Bright, dense primary ring&lt;br /&gt;
|-&lt;br /&gt;
! Division&lt;br /&gt;
|	1.96–2.04 Rₚ ||25,000–26,000 || a low-density gap&lt;br /&gt;
|-&lt;br /&gt;
!  A&lt;br /&gt;
|	2.04–2.3 Rₚ||26,000–29,300||	Sharp-edged outer ring&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Moon !!	Orbit (km) !!	Orbit (Rₚ) !!	Diameter (km) !!	Type	!! Period !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! I&lt;br /&gt;
|	60,000	||4.7 Rₚ	||~400	||Rocky	|| 0.9 ||Cratered&lt;br /&gt;
|-&lt;br /&gt;
! II&lt;br /&gt;
| 	110,000	|| 8.6 Rₚ	|| ~800	|| Mixed rock/ice	|| 2.25|| Cracked surface, frozen ocean&lt;br /&gt;
|-&lt;br /&gt;
! III &lt;br /&gt;
| 190,000	|| 14.9 Rₚ ||	~1200 ||	Icy major moon ||	5.1|| Cryovolcanism, smooth plains&lt;br /&gt;
|-&lt;br /&gt;
! IV &lt;br /&gt;
|340,000	||26.7 Rₚ	||~200	||Irregular/prograde	|| 12.21 || Dark red/carbon, inclined (20º, eccentric orbit (0.1)&lt;br /&gt;
|-&lt;br /&gt;
! V &lt;br /&gt;
| 710,000 ||	55.7 Rₚ	||~350	|| Captured/retrograde	|| 36.83 || Highly inclined (130º), Split terrain—half rugged highlands, half smooth resurfaced plain&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==== g: Stripped Sub-Neptune Remnant ====&lt;br /&gt;
&lt;br /&gt;
Basic Parameters&lt;br /&gt;
* Mass: 2.6 Earth masses (M⊕)&lt;br /&gt;
* Radius: 1.7 Earth radii (R⊕)&lt;br /&gt;
* Mean Density: ~2.92 g/cm³&lt;br /&gt;
* Orbital Distance: 0.4 AU &lt;br /&gt;
* Albedo: ~0.5 (moderately high)&lt;br /&gt;
* Rotation: Tidally locked &lt;br /&gt;
&lt;br /&gt;
Origin and Evolution&lt;br /&gt;
* Formed beyond the snow line (~0.8–1.2 AU) from a mix of rock, iron, and ices&lt;br /&gt;
* Migrated inward early during protoplanetary disk phase&lt;br /&gt;
* Accreted a modest hydrogen-helium envelope (&amp;gt;1% by mass)&lt;br /&gt;
* Exposed to intense stellar X-ray and UV radiation during the M dwarf&#039;s pre-main-sequence phase&lt;br /&gt;
* Lacked a magnetic dynamo (metal-poor and early core freezing)&lt;br /&gt;
* Entire atmosphere lost over ~100 Myr via photoevaporation, core-powered mass loss, and sputtering&lt;br /&gt;
&lt;br /&gt;
Current State&lt;br /&gt;
* Atmosphere: None (trace mineral vapors possible in hot regions)&lt;br /&gt;
* Surface: Stark contrast between hemispheres due to tidal locking&lt;br /&gt;
** Dayside: ~700–1000 K; high-silica lava fields, salt flats, exposed alumino-silicates&lt;br /&gt;
** Nightside: ~100–150 K; gypsum and calcite in cold traps, frozen regolith&lt;br /&gt;
* Magnetosphere: Absent&lt;br /&gt;
* Volcanism:episodic; high-silica flows, volcanic glass, sodium-rich crusts&lt;br /&gt;
* Geological Activity: Tectonically inactive; thermally fractured plains, impact craters&lt;br /&gt;
&lt;br /&gt;
Surface Composition&lt;br /&gt;
* Titanium dioxide (rutile): bright, high-albedo mineral condensate&lt;br /&gt;
* Calcite (CaCO₃): carbonate deposits in cold traps&lt;br /&gt;
* Gypsum (CaSO₄·2H₂O): hydration mineral, stable only on the nightside&lt;br /&gt;
* Sodium chloride: salt flats, especially in evaporated basins&lt;br /&gt;
* High-silica volcanic deposits: glassy, oxidized, and light-colored&lt;br /&gt;
&lt;br /&gt;
Visual and Observational Notes&lt;br /&gt;
&lt;br /&gt;
* High visual contrast between molten and frozen hemispheres&lt;br /&gt;
* Surface appears mottled: obsidian-black lava, gleaming salt flats, white calcium deposits&lt;br /&gt;
* No clouds, auroras, or magnetic activity&lt;br /&gt;
* Extreme day/night temperature gradient&lt;br /&gt;
* Reflective phase curve possible in photometric observations&lt;br /&gt;
* Surface pressure: effectively 0 bar&lt;br /&gt;
&lt;br /&gt;
Planet g is the airless skeleton of a once-sub-Neptune world. Born icy and distant, it migrated into the young star&#039;s wrath, where its fragile envelope boiled away under a sky of flares. Bereft of a magnetic shield, it was slowly stripped to bare rock. Today, one hemisphere bakes in molten silence while the other freezes in shadow. No air, no oceans, only salt, stone, and the echo of a lost atmosphere.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property !!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~75,000 km (~0.26 R&amp;lt;sub&amp;gt;hill&amp;lt;/sub&amp;gt;)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~1,400 km (~0.22 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass	&lt;br /&gt;
| ~0.01 M⊕ (~1.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~3.0 g/cm³ (rock–ice mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temp&lt;br /&gt;
|	~150–180 K&lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
| 0.20g&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere&lt;br /&gt;
|	Trace O₂, from radiolysis and outgassing&lt;br /&gt;
|-&lt;br /&gt;
! Subsurface Ocean&lt;br /&gt;
|	heated by tidal flexing&lt;br /&gt;
|-&lt;br /&gt;
! Surface Features	&lt;br /&gt;
|Fractured ice crust, chaos terrain, cryogeysers, lenticulae&lt;br /&gt;
|}&lt;br /&gt;
gI is a cracked glass orb, rimed with frost and laced with luminous fissures. Below its crust, tides flex a hidden ocean in rhythmic silence. Its faint oxygen exosphere is ghostly but present.  It is frosted quartz with cobwebbed streaks and mineral discoloration.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property!!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~150,000 km (~0.5 Rₕill)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~2,100 km (~0.33 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass&lt;br /&gt;
|	~0.035 M⊕ (~4.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~2.1 g/cm³ (icy-rocky mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes &lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
|	~0.35 g&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temperature&lt;br /&gt;
|	~115–130 K (pressure and greenhouse effects)&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere	&lt;br /&gt;
| ~0.18 bar N₂ + ~0.1 bar Ar + ~0.02 bar CH₄, minor CO, trace haze &lt;br /&gt;
|}&lt;br /&gt;
gII is a muted blue-green crescent veiled in gold. Its sky glows with the weight of argon and the shimmer of methane haze, and its surface smolders with the memory of internal warmth. Liquid hydrocarbons shine like ink in the basins, while glaciers ebb across the uplands. To the star it shows only one face, but beneath that still gaze lies the soft breath of a world more welcoming than its master.&lt;br /&gt;
&lt;br /&gt;
==== h ====&lt;br /&gt;
h is a twin-planet system, 1.5 AU from the star, with a period of 4.1 years&lt;br /&gt;
&lt;br /&gt;
Mutual Orbital Configuration&lt;br /&gt;
* Type: True binary planet pair, gravitationally bound, equal mass&lt;br /&gt;
* Masses: 5.0 M⊕ each&lt;br /&gt;
* Radii: 2.3 R⊕ each&lt;br /&gt;
* Mutual Orbit: Essentially circular, ~1 million km separation (~8–10 planetary radii)&lt;br /&gt;
* Period (mutual orbit): ~4.5 days&lt;br /&gt;
* Orbital Plane: Perpendicular to system ecliptic &lt;br /&gt;
* Tidal State: Tidally locked to each other (mutual synchronous rotation)&lt;br /&gt;
&lt;br /&gt;
Planet A — &amp;quot;Sapphire&amp;quot;&lt;br /&gt;
* Coloration: Deep sapphire blue with white high-altitude methane ice hazes&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: H₂, He&lt;br /&gt;
** Methane (CH₄): high&lt;br /&gt;
** Ammonia: trace&lt;br /&gt;
** Argon: moderate&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: slightly enriched&lt;br /&gt;
* Magnetosphere: Strong, symmetric; supports brilliant blue-violet aurorae&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Superionic water mantle&lt;br /&gt;
** Stratified silicate-ice alloy core&lt;br /&gt;
** Radiogenic heating and layered convection&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar hexagonal jet (stronger than Saturn&#039;s)&lt;br /&gt;
** Methane plasma flares at terminator&lt;br /&gt;
** Iridescent methane cirrus clouds&lt;br /&gt;
** Massive auroral crowns aligned with spin-magnetic axis misalignment&lt;br /&gt;
&lt;br /&gt;
Planet B — &amp;quot;Rust&amp;quot;&lt;br /&gt;
* Coloration: Dark crimson to rust-red, streaked with black and violet haze bands&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: N₂, CO&lt;br /&gt;
** CH₄: trace&lt;br /&gt;
** Tholins: abundant&lt;br /&gt;
** Argon: high&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: moderate&lt;br /&gt;
** Magnetosphere: Weak, multipolar and intermittent&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Dense iron-rich core with impact inclusions (e.g., iridium, ruthenium)&lt;br /&gt;
** Volcanically active mantle with carbon-rich inclusions&lt;br /&gt;
** Higher internal heat flow than Sapphire&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar cyclonic basins with geyser-like haze columns&lt;br /&gt;
** Frequent UV lightning within organic clouds&lt;br /&gt;
** Faint auroral echoes from Sapphire’s magnetospheric tail&lt;br /&gt;
** Surface glow from argon emissions during conjunction&lt;br /&gt;
&lt;br /&gt;
Mutual Phenomena &amp;amp; Sky Effects&lt;br /&gt;
* Eclipse Cycles: Frequent, due to short mutual period and perpendicular orbit; cause wave-like haze patterns and shadow bands&lt;br /&gt;
* Filamentary Atmosphere Bridges: Transient stratospheric strands near L1, illuminated during eclipses&lt;br /&gt;
* Auroral Flux Tubes: Occasionally connect the two with violet-green flickering arcs&lt;br /&gt;
* Gravitational Stability: Mutual orbit stable within Hill sphere; resistant to long-term disruption&lt;br /&gt;
&lt;br /&gt;
* Legacy of the Comet Shield&lt;br /&gt;
* Each planet’s core contains embedded relics of the system’s ancient bombardment:&lt;br /&gt;
** Sapphire: interstellar dust, primordial isotopes, deep xenon pockets&lt;br /&gt;
** Rust: impact-derived siderophiles, compressed organics, rare isotopic anomalies&lt;br /&gt;
* Capture Events: Both planets have intercepted and redirected hundreds of large icy bodies over system history&lt;br /&gt;
&lt;br /&gt;
They each have 2 small irregular moons, &amp;lt;100 km diameter, retrograde, on distant orbits.  Negligible.&lt;br /&gt;
== Planet C ==&lt;br /&gt;
&lt;br /&gt;
* With an albedo of 0.2, the global average temp is 263ºK.  Because of modest greenhouse effects, surface temperatures are higher, on the sun-side.&lt;br /&gt;
# Mass: 1.5M⊕&lt;br /&gt;
# Gravity: 1g⊕&lt;br /&gt;
# Radius = 1.225⊕, or 7805km&lt;br /&gt;
Terminator Zone&lt;br /&gt;
# +/-30º: 1.28 E8 km&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; (slightly less than all the land of the Earth)&lt;br /&gt;
# Escape velocity is 12.4km/s, 11% higher than Earth&lt;br /&gt;
# Orbital velocity is 8.79km/s&lt;br /&gt;
=== Atmosphere ===&lt;br /&gt;
Water content is low because&lt;br /&gt;
* Water vapor is a potent greenhouse gas; vast surface water can trap too much heat, especially near the substellar point.&lt;br /&gt;
* Water leads to climate homogenization&lt;br /&gt;
* Lack of exposed silicate rock: Necessary for carbon-silicate weathering feedback, which stabilizes climate on geological timescales.&lt;br /&gt;
Earth has ~1.4 billion km³ of water.  In our habitable zone, we have no more than 10% of that, or 100 million km³, though there is much more on the night side, both liquid and ice.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Factor !! Ɬiʔa atm !! Ɬiʔa % !! Earth atm !! Earth % !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! Total Pressure &lt;br /&gt;
| 1.6 atm || || 1.0 atm || || Enhanced convective heat transfer, increased IR trapping&lt;br /&gt;
|-&lt;br /&gt;
! Nitrogen (N₂) &lt;br /&gt;
| 1.00 || 62.50% || 0.7808 || 78.08% || Reduced; still inert, still dominant&lt;br /&gt;
|-&lt;br /&gt;
! Oxygen (O₂) &lt;br /&gt;
| 0.21 || 13.13% || 0.2095 || 20.95% || Earth-normal partial pressure &lt;br /&gt;
|-&lt;br /&gt;
! Argon (Ar)&lt;br /&gt;
| 0.40 || 25.00% || 0.0093 || 0.93% || Major heat distribution enhancement, inert&lt;br /&gt;
|-&lt;br /&gt;
! Krypton + Xenon&lt;br /&gt;
| 0.005 || 0.31% || trace || trace || High molecular mass → improved heat retention, still safe&lt;br /&gt;
|-&lt;br /&gt;
! CO₂&lt;br /&gt;
| 0.005 || 0.31% || 0.004 || 0.04% || slightly elevated; sub-greenhouse threshold&lt;br /&gt;
|-&lt;br /&gt;
! H₂O vapor &lt;br /&gt;
| 0.015 || ~1% || || 0-4% || Maintains greenhouse without excess moisture&lt;br /&gt;
|}&lt;br /&gt;
==== Atmospheric Effects on Clouds ====&lt;br /&gt;
# Increased Pressure (1.6 atm) compresses gases, raising the dew point at which water vapor condenses. Clouds form closer to the surface, and are denser than similar altitudes compared to Earth.&lt;br /&gt;
# Low Water Inventory (~20% of Earth&#039;s): less frequent and less massive cloud systems than on Earth, but still present—especially over &amp;quot;hotspots&amp;quot; on the day side.&lt;br /&gt;
# Tidally Locked Climate: Cloud formation concentrate along the substellar point, where warm, moist air rises and cools.&lt;br /&gt;
#* A permanent “eyewall” storm system has formed at the subsolar point, like a giant hurricane.&lt;br /&gt;
#* As air rises and is advected to the night side, thin cloud bands or ice hazes form as it descends and cools.&lt;br /&gt;
&lt;br /&gt;
Appearance:&lt;br /&gt;
* The presence of noble gases (Ar, Kr, Xe) and higher pressure enhance Mie scattering, making clouds appear whiter and more silvered, especially at sunrise/sunset boundaries.&lt;br /&gt;
* Night side clouds are thin, high-altitude icy sheets, glowing faintly in aurorae or thermal emissions.&lt;br /&gt;
&lt;br /&gt;
==== Sky Color ====&lt;br /&gt;
The color of the sky is shaped by Rayleigh scattering, which depends on:&lt;br /&gt;
# Molecular composition: Heavier gases like Ar, Kr, and Xe scatter light less efficiently than N₂.&lt;br /&gt;
# Spectral output of the star: the red dwarf emits predominantly infrared and red light, with very little blue or violet.&lt;br /&gt;
&lt;br /&gt;
Consequence:&lt;br /&gt;
* Even with atmospheric scattering, there is insufficient blue light in the stellar spectrum to produce a blue sky.&lt;br /&gt;
* Day sky would likely appear:&lt;br /&gt;
** Dark peach, dusky rose, or reddish beige near zenith,&lt;br /&gt;
** Grading to deep salmon or mauve near the horizon,&lt;br /&gt;
** A slight metallic sheen due to noble gas content and high pressure.&lt;br /&gt;
&lt;br /&gt;
Twilight &amp;amp; Limb Scattering:&lt;br /&gt;
* The terminator (twilight zone) sees a diffuse, ruddy light, scattering through haze and clouds into luminous reds, purples, and copper tones.&lt;br /&gt;
* Aurorae are spectacular on the night side, especially since stellar flares are frequent.&lt;br /&gt;
&lt;br /&gt;
==== Sound Propagation ====&lt;br /&gt;
: &#039;&#039;Sound is profoundly affected by atmospheric pressure and composition.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Compared to Earth:&lt;br /&gt;
* Higher pressure → greater air density → faster transmission of sound and less attenuation.&lt;br /&gt;
* Argon and Xenon are heavy gases, which:&lt;br /&gt;
** Lower the speed of sound relative to air at the same pressure (despite the pressure increase).&lt;br /&gt;
** Shift resonance frequencies downward, resulting in deeper, rounder sounds.&lt;br /&gt;
&lt;br /&gt;
Consequences:&lt;br /&gt;
* Voices sound subtly lower-pitched and richer, especially for consonants and low vowels.&lt;br /&gt;
* Ambient sounds (wind, water, animals) would carry farther and sound more muffled or sonorous.&lt;br /&gt;
* Music or speech would resonate more warmly, especially indoors or in enclosed spaces.&lt;br /&gt;
&lt;br /&gt;
In short: it sounds like it’s wrapped in velvet.&lt;br /&gt;
&lt;br /&gt;
==== Heat Transport to the Night Side ====&lt;br /&gt;
Mechanisms:&lt;br /&gt;
# Thick Atmosphere (1.6 atm) increases:&lt;br /&gt;
#* Advection efficiency: Warm air masses can move more heat horizontally.&lt;br /&gt;
#* Radiative time constant: The atmosphere holds heat longer before releasing it.&lt;br /&gt;
# Noble Gases (especially Kr/Xe):&lt;br /&gt;
#* High molecular mass → more IR opacity → trapping and radiating heat more evenly.&lt;br /&gt;
# Slow Rotation / Tidal Locking:&lt;br /&gt;
#* Global Hadley-like cells dominate circulation, carrying warm air from the day side to the night side and descending it there.&lt;br /&gt;
&lt;br /&gt;
Result:&lt;br /&gt;
* The night side is not so freezing.  Temperatures differ by tens of degrees, not hundreds.&lt;br /&gt;
* There are still ice caps and a cold deserts at the anti-stellar point, but not a glaciated wasteland.&lt;br /&gt;
&lt;br /&gt;
=== Magnetosphere ===&lt;br /&gt;
* Larger mass --&amp;gt; larger iron core, generating more internal heat&lt;br /&gt;
* Larger radius --&amp;gt; Vigorous convection in the core&lt;br /&gt;
* Tidal Flexing --&amp;gt; still drives magnetic activity&lt;br /&gt;
&lt;br /&gt;
# Aurorae at lower latitudes&lt;br /&gt;
## higher magnetic rigidity, wider magnetotail, and greater reconnection energy.&lt;br /&gt;
## Combined with a higher flux of stellar particles, this means:&lt;br /&gt;
### Auroral ovals expand, reaching mid-latitudes sometimes equator.&lt;br /&gt;
### The skies are alive with rippling green, violet, and crimson aurorae, especially on the night side.&lt;br /&gt;
### Daily auroral activity occur during stellar flare cycles.&lt;br /&gt;
# Compasses&lt;br /&gt;
## compasses respond more sharply, with:&lt;br /&gt;
### Faster alignment.&lt;br /&gt;
### Greater resistance to local perturbations.&lt;br /&gt;
## However, frequent magnetic storms from stellar activity cause sudden declinations, reversals, or local anomalies.  In short, lots of aurorae equals dead compasses at the same time.&lt;br /&gt;
# Magnetic Field Strength &amp;gt; 100 μT &lt;br /&gt;
# Electromagnetism is more basic than chemistry or almost any other natural philosophy&lt;br /&gt;
&lt;br /&gt;
=== Substellar Point ===&lt;br /&gt;
The maximum incoming flux is very nearly the same as Earth&#039;s solar constant (≈1361 W/m²), but concentrated over one point rather than averaged over a rotating sphere.  Temperatures should be above 500ºK most of the time.  &lt;br /&gt;
&lt;br /&gt;
The magnetic north is also here. The thick atmosphere prevents too much loss here, but &lt;br /&gt;
* Charged particle influx&lt;br /&gt;
** Maximized at the substellar point—intense auroral and energetic particle precipitation&lt;br /&gt;
* Atmospheric ionization&lt;br /&gt;
** Constant production of high-energy ions and NOx compounds—UV fluorescence in upper sky&lt;br /&gt;
* Localized heating&lt;br /&gt;
** Augments already extreme temperatures—600–700 K surface&lt;br /&gt;
&lt;br /&gt;
== Artificially Tethered Moon ==&lt;br /&gt;
* 670,000 km up&lt;br /&gt;
* 7805 km in radius = same as the planet&lt;br /&gt;
* 1.33º of the sky, same as the sun&lt;br /&gt;
&lt;br /&gt;
A network of tethers/tension lines from the moon to multiple anchor points on the planet’s surface (a tripod or hexapod structure), woven like hair&lt;br /&gt;
* Uses active tension management and orbital station-keeping to stabilize the moon&lt;br /&gt;
* Counterweights and inward-pointing mass drivers on the moon to oppose drift&lt;br /&gt;
&lt;br /&gt;
The tethers are not bearing the full weight, but merely damping drift, providing restoring force, and enabling long-term stability through active compensation.  The moon&lt;br /&gt;
* Blocks the worst of the heat&lt;br /&gt;
* Blocks the worst of the solar radiation&lt;br /&gt;
The moon has &lt;br /&gt;
* low mass&lt;br /&gt;
* high albedo - enormous reflectivity&lt;br /&gt;
* scatters charges particles, UV, X-rays, auroral flux tubes&lt;br /&gt;
* sunward - crazy hot, high emissivity&lt;br /&gt;
* earthward - crazy cool, low emissivity&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=File:Wet_eye_planet.png&amp;diff=168158</id>
		<title>File:Wet eye planet.png</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=File:Wet_eye_planet.png&amp;diff=168158"/>
		<updated>2025-03-27T22:05:57Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: A unique exoplanet&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Summary ==&lt;br /&gt;
A unique exoplanet&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168157</id>
		<title>Ɬiʔa/Conworlding</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168157"/>
		<updated>2025-03-27T20:15:40Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* b: super Mercury with a ring of fire */ pic&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Star ==&lt;br /&gt;
Our star is a red-dwarf.&lt;br /&gt;
# Type: M5V&lt;br /&gt;
## M: This indicates it&#039;s a cool, red star with a surface temperature less than 3,500ºK&lt;br /&gt;
## 5: Within the M class, stars are further divided into subclasses 0-9, with 0 being the hottest and 9 the coolest. An M5 star is in the middle of this range.&lt;br /&gt;
## V: Denotes that it&#039;s a main sequence star, also known as a dwarf star&lt;br /&gt;
# Stellar luminosity (L*) ≈ 0.01 𝐿⊙ (1/100th Sol&#039;s brightness)&lt;br /&gt;
# Stellar mass (M*) ≈ 0.2 𝑀⊙ (1/5 the mass of Sol)&lt;br /&gt;
# Stellar radius (R*) ≈ 0.25 𝑅⊙ (1/4 as wide as Sol)&lt;br /&gt;
# Effective temperature (T*) ≈ 3500 K&lt;br /&gt;
​The habitable zone (a) is about square root of L* over L⊙, so ~0.1 AU.&lt;br /&gt;
&lt;br /&gt;
=== Solar System ===&lt;br /&gt;
There are seven planets in the system&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Planet !!	Mass (M🜨)!!	Radius (R🜨)!! Moons/Rings	!!Resonance !!	Semi-Major Axis (AU)!!	Rings !! Moons !! Period !! Size&lt;br /&gt;
|-&lt;br /&gt;
| b ||	2.17 ||	1.1 ||	No ||	2:3 with c	|| 0.0763 ||	No || No || 17.2 || 13.6&#039; to 1.5&#039;&lt;br /&gt;
|-&lt;br /&gt;
| c ||	1.5	 ||1.225 ||	1* ||	—	        || 0.100 || No || No || 25.8 || -&lt;br /&gt;
|-&lt;br /&gt;
| d ||	2.0	 ||1.4 ||No ||	2:3 with c	 ||0.131 ||	No || No || 38.7 || 13.1&#039; to 1.8&#039;&lt;br /&gt;
|-&lt;br /&gt;
| e ||	0.9 ||	1.0 || No	 ||	2:3 with d	 ||0.172 ||	No || No || 58 || 4.1&#039; to 1.1&#039;&lt;br /&gt;
|-&lt;br /&gt;
| f ||	3.5 ||	2.0 ||	Yes! ||	2:3 with e	 ||0.227 || Yes || Junk || 87 || 4.6&#039; to 1.8&#039;&lt;br /&gt;
|-&lt;br /&gt;
| g ||	2.6 ||	1.7 ||	2 ||	-	 ||0.40 ||	Yes || Junk || 206 || 1.6&#039; to 1.0&#039;&lt;br /&gt;
|-&lt;br /&gt;
| h ||	5.0x2 ||2.3x2 || yes	 || -	 ||1.5 ||	Yes || No || 1500 || 0.5&#039; 16.4&#039; apart (at max)&lt;br /&gt;
|}&lt;br /&gt;
==== b: super Mercury with a ring of fire  ====&lt;br /&gt;
[[File:planet b by GPT.png|thumb|right|An artistic rendering of planet b]]&lt;br /&gt;
b is a super-Mercury, tidally locked, and incredibly dense.  ~700ºK on the day side, ~50ºK on the night.  2.1 Earth Masses, 1.1 Earth radii (~7000km) in size.  Orbital period 17.2 days.  Density 9.0 g/cm&amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt;.  Gravity is ~1.8g.  &lt;br /&gt;
&lt;br /&gt;
The iron core is huge, being 75% of the mass.  A thin silicate mantle, with metallic plains and exhumed ultramafic crust, with frequent iron meteorite craters, lacking typical “stone” breccias.&lt;br /&gt;
&lt;br /&gt;
The night side is intense, as simple hydrocarbons (methane, ethane, propane) condense and freeze into layered deposits.  Complex organics (tholins, polycyclic aromatics) accumulate on the sea floor, under miles of nitrogen ice.  Massive slush layers slosh around above cryovolcanic brines of ammonia.&lt;br /&gt;
&lt;br /&gt;
There is a crucial layer of Superionic Ice XI above the core, which acts as an electromagnetic insulator, and ionic heat bridge.  The crust is ultramafic silicates (olivine, pyroxene, perovskite) riddled with with sulfide veins, iron alloys, and graphite networks.  The poles of the magnetosphere are sideways, like Uranus, with poles at the equator in the Terminator Zone.  Persistent surface charges develop, because the whole planet is basically a ginormous Leyden jar!&lt;br /&gt;
&lt;br /&gt;
A planetary flux rope forms and un-forms with the star and planet b.  This induces electric jets at the terminator.  This is where temps are Earth-like.  Hydrocarbons sublimate and eject into the atmosphere, even while aurorae come right down to the ground.  A small, low pressure atmosphere prevents photodissociation, even while electrothermal instabilities lift molecules, forming an anomalous haze, a standing, glowing ring.  Coronal events cause localized lightning geysers with magnetic arcing.&lt;br /&gt;
&lt;br /&gt;
In short, b is visible with a blinding bright sun side (glowing orange bronze), a utterly black night side, and a burning, glowing, erupting, arcing ring at the terminator (all colors).  At biggest, it&#039;s half the size of Earth&#039;s moon in the sky, shrinking down to a star at it&#039;s furthest away.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== d: the wet eye with depths ====&lt;br /&gt;
From the outside, d is a &amp;quot;wet eye&amp;quot; just outside the habitable zone.  It is a water world, twice the mass of Earth, 1.4 times the radius, tidally locked.  The substellar point is the only place without surface ice.  However, it is better to think of the planet top-to-bottom.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;atmosphere&#039;&#039;&#039; is tenuous, less than 0.2 bars.  It is thin, N₂-rich with traces of H₂O, NH₃ vapor, and transient geyser outputs.  It is highly UV-irradiated, and Mars-like in its inability to retain volatiles.&lt;br /&gt;
&lt;br /&gt;
Next, there is a &#039;&#039;&#039;surface ice shell&#039;&#039;&#039;, ~20 km of thick Ice I.  Swirling currents beneath have cracked continent-sized ice plates, similar to Europa&#039;s crust.  It is permanently frozen except at the substellar furnace.  It accumulates chemical stains, mineral deposits, and cryovolcanic eruption plumes.  Accumulations of complex hydrates—like methanol clathrates—precipitate out and form false reefs, rising like coral from beneath. Transient thermal vents push hot plumes into the thin air, freezing instantly and snowing down crystals that form mineral spires.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;subglacial ocean&#039;&#039;&#039; is hundreds of kilometers thick.  It is super-pressurized liquid H₂O mixed with NH₃, CH₃OH, H₂O₂, and trace salts.  The movement is slow, planetary-scale currents originating from the Furnace and Coriolis force.  Strong layers exist: the surface is oxidized; the abyssal layer is reducing.&lt;br /&gt;
&lt;br /&gt;
A new &amp;quot;surface&amp;quot; is next.  The &#039;&#039;&#039;Ice Mantle&#039;&#039;&#039; is solid Ice VI and VII.  There are massive, slowly shifting &amp;quot;sub-oceanic continents&amp;quot;. It is periodically fractured and resurfaced by cryoquakes and brine-driven eruptions.  Some regions have developed elevated domes or ridges, continental “shelves” under the ocean.&lt;br /&gt;
&lt;br /&gt;
Finally, underneath is the &#039;&#039;&#039;core&#039;&#039;&#039;. Temperatures exceed 2000–3000 K locally.  Pressures range from 100 to 300 GPa.  The core is rich in heavy elements.  This makes radiogenic hotspots, localized magnetic eddies.  Heat gradients + ion flows = thermoelectric currents.  These make magnetic storms within the ocean itself, not the sky.  When uranium-rich corium pods shift or explode upward through the mantle, their heat and conductivity disturb the local magnetic field, generating geomagnetic quakes.  These pulse through the ocean, creating short-lived magnetic lenses.  These interact with atmospheric charged particles above the Furnace, giving rise to transient magnetic halos visible from orbit—false auroras without a sunstorm.&lt;br /&gt;
&lt;br /&gt;
==== e: The Tortured Near-Sphere ====&lt;br /&gt;
&lt;br /&gt;
Orbital and Physical Characteristics&lt;br /&gt;
* Mass: 0.9 Earth masses&lt;br /&gt;
* Radius: 1.0 Earth radii&lt;br /&gt;
* Orbital Period: 58 Earth days&lt;br /&gt;
* Surface Gravity: ~0.9 g&lt;br /&gt;
* Semimajor Axis: ~0.17 AU &lt;br /&gt;
* Spin State: In the &#039;&#039;process&#039;&#039; of becoming tidally locked&lt;br /&gt;
* Obliquity: Extreme, experiencing chaotic realignment events&lt;br /&gt;
&lt;br /&gt;
Internal Structure and Composition&lt;br /&gt;
* &#039;&#039;&#039;Crust:&#039;&#039;&#039; A thick, rigid outer shell of water ice I mixed with clathrates (CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; and CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; hydrates), underlain by layers of ammonia-water ice eutectics. Inclusions of carbon under extreme pressure form diamond strata in the lower crust, lending rigidity and brittle behavior.&lt;br /&gt;
* &#039;&#039;&#039;Mantle:&#039;&#039;&#039; Comprised of Ice VI and Ice VII, with ammonia- and methane-rich brines forming localized conduits and pockets of unstable volatiles.&lt;br /&gt;
* &#039;&#039;&#039;Core:&#039;&#039;&#039; Differentiated and semi-molten. Inner core of iron-nickel alloy spins at a different rate. Outer core is a highly viscous slurry of silicate, iron, carbon, sulfur, and dissolved volatiles. Chemical veins (e.g., uranium silicates, perovskites) act as mechanical shear zones. Tidal torque leads to periodic frictional heating.&lt;br /&gt;
&lt;br /&gt;
Tectonic and Cryovolcanic Behavior&lt;br /&gt;
* The planet resists tidal locking due to core-crust decoupling and uneven angular momentum transfer.&lt;br /&gt;
* High obliquity experiences &#039;&#039;&#039;&#039;&#039;Axial Recoil Events&#039;&#039;&#039;&#039;&#039;, where the entire planet jerks between metastable orientations (e.g., from 110° to 70°) in sudden spasms.&lt;br /&gt;
* These events generate:&lt;br /&gt;
** Global-scale crustal cracking&lt;br /&gt;
** Venting of pressurized subsurface gases (H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;O, CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt;)&lt;br /&gt;
** Surface deformation and glacial faulting&lt;br /&gt;
* Volatiles erupt ballistically into space (200+lm) from exposed fissures and calderas, driven by phase-change explosions.&lt;br /&gt;
&lt;br /&gt;
Surface Conditions&lt;br /&gt;
* Global temperature well below freezing; warmest zones around cryovolcanic hotspots&lt;br /&gt;
* Crustal coloration varies by volatile deposition:&lt;br /&gt;
** Pale blue-white from water ice&lt;br /&gt;
** Red-brown from CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; frostfields&lt;br /&gt;
** Green-black CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; stains from plume fallout&lt;br /&gt;
* Surface features include:&lt;br /&gt;
** Cryovolcanic calderas&lt;br /&gt;
** Diamond-studded impact-like basins&lt;br /&gt;
** Faulted plains crossed by salt-streaked rift zones&lt;br /&gt;
&lt;br /&gt;
Atmosphere and Ejected Material&lt;br /&gt;
* Thin transient exosphere formed from eruptive events&lt;br /&gt;
* Gases often escape to space or freeze back out in polar regions&lt;br /&gt;
* Fallback material creates uneven surface mass distributions, altering moment of inertia and prolonging instability&lt;br /&gt;
&lt;br /&gt;
Appearance from Planet c&lt;br /&gt;
&lt;br /&gt;
* Angular Size: ~4-1 arcminutes&lt;br /&gt;
* Coloration: Overall dusky grey-white, with changing colored bands due to volatile fallout; craterless but mottled&lt;br /&gt;
&lt;br /&gt;
Transient visible phenomena:&lt;br /&gt;
&lt;br /&gt;
* Cryovolcanic plumes visible as fan-like arcs at the limb during outburst events&lt;br /&gt;
* Infrared brightening during Axial Recoil Events&lt;br /&gt;
* Occasional light-scattering halos from plume particles&lt;br /&gt;
&lt;br /&gt;
Event Cycle Summary&lt;br /&gt;
&lt;br /&gt;
# Tidal torque builds due to obliquity misalignment&lt;br /&gt;
# Core resists, crust locks tension&lt;br /&gt;
# Critical stress threshold breached&lt;br /&gt;
# Obliquity lurches to new orientation&lt;br /&gt;
# Crust fractures globally, vents open&lt;br /&gt;
# Supersonic cryovolcanism hurls volatiles into space&lt;br /&gt;
# Fallback modifies crustal mass distribution&lt;br /&gt;
# Obliquity rebuilds instability over decades&lt;br /&gt;
# Repeat.&lt;br /&gt;
&lt;br /&gt;
Planet e is a tortured world caught in an unending cycle of self-correcting failure—its body unable to align, its gases unable to stay contained, its appearance in the sky a visible signature of internal catastrophe.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==== f: Ringed Mini-Neptune ====&lt;br /&gt;
This planet is a substantial mini-Neptune, with a mass of approximately 3.5 Earth masses and a radius of 2.0 Earth radii, orbiting at 0.227 AU. Its low mean density (~0.44 ρ⊕) signals the presence of a deep, volatile-rich envelope overlying a denser core. The bulk of its volume is composed of hydrogen and helium, accreted from the protoplanetary disk, with trace amounts of methane (CH₄) and ammonia (NH₃)—gases that dominate its photochemical and radiative behavior. Beneath this envelope, the planet hosts a water–rock–metal core layered in complex phases, with high-pressure ices and possibly superionic water enveloping a metallic center.  Lower atmosphere reaches 300–500 K (27–227°C) near the bottom of the troposphere, depending on opacity and convection.&lt;br /&gt;
&lt;br /&gt;
Visually, the planet exhibits a blue-to-cyan atmospheric hue, governed by Rayleigh scattering and methane absorption in the red and near-infrared spectrum. While not as banded or storm-laced as Jupiter, it features broad zonal flows, high-altitude methane ice clouds, and long-lived anticyclonic storms akin to Neptune’s Great Dark Spot. Due to its tidal locking to the host star, the planet presents hemispheric climatic asymmetry: a sunlit dayside prone to atmospheric upwelling and cloud formation, and a cooler, darker nightside. While colder, the backside is not freezing— in the 150–250 K range, depending on circulation efficiency. Atmospheric circulation is dominated by slow, large-scale overturning cells, moderated by planetary-scale waves and a subdued Coriolis force. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Rings =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Ring!!	Range (Rₚ)!!	Approx.! Range (km)!!	Description&lt;br /&gt;
|-&lt;br /&gt;
! C&lt;br /&gt;
| 	1.5–1.65 Rₚ	||19,100–21,000	||Faint, dusty interior ring&lt;br /&gt;
|-&lt;br /&gt;
! B&lt;br /&gt;
| 	1.65–1.96 Rₚ	||21,000–25,000||	Bright, dense primary ring&lt;br /&gt;
|-&lt;br /&gt;
! Division&lt;br /&gt;
|	1.96–2.04 Rₚ ||25,000–26,000 || a low-density gap&lt;br /&gt;
|-&lt;br /&gt;
!  A&lt;br /&gt;
|	2.04–2.3 Rₚ||26,000–29,300||	Sharp-edged outer ring&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Moon !!	Orbit (km) !!	Orbit (Rₚ) !!	Diameter (km) !!	Type	!! Period !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! I&lt;br /&gt;
|	60,000	||4.7 Rₚ	||~400	||Rocky	|| 0.9 ||Cratered&lt;br /&gt;
|-&lt;br /&gt;
! II&lt;br /&gt;
| 	110,000	|| 8.6 Rₚ	|| ~800	|| Mixed rock/ice	|| 2.25|| Cracked surface, frozen ocean&lt;br /&gt;
|-&lt;br /&gt;
! III &lt;br /&gt;
| 190,000	|| 14.9 Rₚ ||	~1200 ||	Icy major moon ||	5.1|| Cryovolcanism, smooth plains&lt;br /&gt;
|-&lt;br /&gt;
! IV &lt;br /&gt;
|340,000	||26.7 Rₚ	||~200	||Irregular/prograde	|| 12.21 || Dark red/carbon, inclined (20º, eccentric orbit (0.1)&lt;br /&gt;
|-&lt;br /&gt;
! V &lt;br /&gt;
| 710,000 ||	55.7 Rₚ	||~350	|| Captured/retrograde	|| 36.83 || Highly inclined (130º), Split terrain—half rugged highlands, half smooth resurfaced plain&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==== g: Stripped Sub-Neptune Remnant ====&lt;br /&gt;
&lt;br /&gt;
Basic Parameters&lt;br /&gt;
* Mass: 2.6 Earth masses (M⊕)&lt;br /&gt;
* Radius: 1.7 Earth radii (R⊕)&lt;br /&gt;
* Mean Density: ~2.92 g/cm³&lt;br /&gt;
* Orbital Distance: 0.4 AU &lt;br /&gt;
* Albedo: ~0.5 (moderately high)&lt;br /&gt;
* Rotation: Tidally locked &lt;br /&gt;
&lt;br /&gt;
Origin and Evolution&lt;br /&gt;
* Formed beyond the snow line (~0.8–1.2 AU) from a mix of rock, iron, and ices&lt;br /&gt;
* Migrated inward early during protoplanetary disk phase&lt;br /&gt;
* Accreted a modest hydrogen-helium envelope (&amp;gt;1% by mass)&lt;br /&gt;
* Exposed to intense stellar X-ray and UV radiation during the M dwarf&#039;s pre-main-sequence phase&lt;br /&gt;
* Lacked a magnetic dynamo (metal-poor and early core freezing)&lt;br /&gt;
* Entire atmosphere lost over ~100 Myr via photoevaporation, core-powered mass loss, and sputtering&lt;br /&gt;
&lt;br /&gt;
Current State&lt;br /&gt;
* Atmosphere: None (trace mineral vapors possible in hot regions)&lt;br /&gt;
* Surface: Stark contrast between hemispheres due to tidal locking&lt;br /&gt;
** Dayside: ~700–1000 K; high-silica lava fields, salt flats, exposed alumino-silicates&lt;br /&gt;
** Nightside: ~100–150 K; gypsum and calcite in cold traps, frozen regolith&lt;br /&gt;
* Magnetosphere: Absent&lt;br /&gt;
* Volcanism:episodic; high-silica flows, volcanic glass, sodium-rich crusts&lt;br /&gt;
* Geological Activity: Tectonically inactive; thermally fractured plains, impact craters&lt;br /&gt;
&lt;br /&gt;
Surface Composition&lt;br /&gt;
* Titanium dioxide (rutile): bright, high-albedo mineral condensate&lt;br /&gt;
* Calcite (CaCO₃): carbonate deposits in cold traps&lt;br /&gt;
* Gypsum (CaSO₄·2H₂O): hydration mineral, stable only on the nightside&lt;br /&gt;
* Sodium chloride: salt flats, especially in evaporated basins&lt;br /&gt;
* High-silica volcanic deposits: glassy, oxidized, and light-colored&lt;br /&gt;
&lt;br /&gt;
Visual and Observational Notes&lt;br /&gt;
&lt;br /&gt;
* High visual contrast between molten and frozen hemispheres&lt;br /&gt;
* Surface appears mottled: obsidian-black lava, gleaming salt flats, white calcium deposits&lt;br /&gt;
* No clouds, auroras, or magnetic activity&lt;br /&gt;
* Extreme day/night temperature gradient&lt;br /&gt;
* Reflective phase curve possible in photometric observations&lt;br /&gt;
* Surface pressure: effectively 0 bar&lt;br /&gt;
&lt;br /&gt;
Planet g is the airless skeleton of a once-sub-Neptune world. Born icy and distant, it migrated into the young star&#039;s wrath, where its fragile envelope boiled away under a sky of flares. Bereft of a magnetic shield, it was slowly stripped to bare rock. Today, one hemisphere bakes in molten silence while the other freezes in shadow. No air, no oceans, only salt, stone, and the echo of a lost atmosphere.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property !!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~75,000 km (~0.26 R&amp;lt;sub&amp;gt;hill&amp;lt;/sub&amp;gt;)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~1,400 km (~0.22 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass	&lt;br /&gt;
| ~0.01 M⊕ (~1.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~3.0 g/cm³ (rock–ice mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temp&lt;br /&gt;
|	~150–180 K&lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
| 0.20g&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere&lt;br /&gt;
|	Trace O₂, from radiolysis and outgassing&lt;br /&gt;
|-&lt;br /&gt;
! Subsurface Ocean&lt;br /&gt;
|	heated by tidal flexing&lt;br /&gt;
|-&lt;br /&gt;
! Surface Features	&lt;br /&gt;
|Fractured ice crust, chaos terrain, cryogeysers, lenticulae&lt;br /&gt;
|}&lt;br /&gt;
gI is a cracked glass orb, rimed with frost and laced with luminous fissures. Below its crust, tides flex a hidden ocean in rhythmic silence. Its faint oxygen exosphere is ghostly but present.  It is frosted quartz with cobwebbed streaks and mineral discoloration.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property!!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~150,000 km (~0.5 Rₕill)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~2,100 km (~0.33 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass&lt;br /&gt;
|	~0.035 M⊕ (~4.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~2.1 g/cm³ (icy-rocky mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes &lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
|	~0.35 g&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temperature&lt;br /&gt;
|	~115–130 K (pressure and greenhouse effects)&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere	&lt;br /&gt;
| ~0.18 bar N₂ + ~0.1 bar Ar + ~0.02 bar CH₄, minor CO, trace haze &lt;br /&gt;
|}&lt;br /&gt;
gII is a muted blue-green crescent veiled in gold. Its sky glows with the weight of argon and the shimmer of methane haze, and its surface smolders with the memory of internal warmth. Liquid hydrocarbons shine like ink in the basins, while glaciers ebb across the uplands. To the star it shows only one face, but beneath that still gaze lies the soft breath of a world more welcoming than its master.&lt;br /&gt;
&lt;br /&gt;
==== h ====&lt;br /&gt;
h is a twin-planet system, 1.5 AU from the star, with a period of 4.1 years&lt;br /&gt;
&lt;br /&gt;
Mutual Orbital Configuration&lt;br /&gt;
* Type: True binary planet pair, gravitationally bound, equal mass&lt;br /&gt;
* Masses: 5.0 M⊕ each&lt;br /&gt;
* Radii: 2.3 R⊕ each&lt;br /&gt;
* Mutual Orbit: Essentially circular, ~1 million km separation (~8–10 planetary radii)&lt;br /&gt;
* Period (mutual orbit): ~4.5 days&lt;br /&gt;
* Orbital Plane: Perpendicular to system ecliptic &lt;br /&gt;
* Tidal State: Tidally locked to each other (mutual synchronous rotation)&lt;br /&gt;
&lt;br /&gt;
Planet A — &amp;quot;Sapphire&amp;quot;&lt;br /&gt;
* Coloration: Deep sapphire blue with white high-altitude methane ice hazes&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: H₂, He&lt;br /&gt;
** Methane (CH₄): high&lt;br /&gt;
** Ammonia: trace&lt;br /&gt;
** Argon: moderate&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: slightly enriched&lt;br /&gt;
* Magnetosphere: Strong, symmetric; supports brilliant blue-violet aurorae&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Superionic water mantle&lt;br /&gt;
** Stratified silicate-ice alloy core&lt;br /&gt;
** Radiogenic heating and layered convection&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar hexagonal jet (stronger than Saturn&#039;s)&lt;br /&gt;
** Methane plasma flares at terminator&lt;br /&gt;
** Iridescent methane cirrus clouds&lt;br /&gt;
** Massive auroral crowns aligned with spin-magnetic axis misalignment&lt;br /&gt;
&lt;br /&gt;
Planet B — &amp;quot;Rust&amp;quot;&lt;br /&gt;
* Coloration: Dark crimson to rust-red, streaked with black and violet haze bands&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: N₂, CO&lt;br /&gt;
** CH₄: trace&lt;br /&gt;
** Tholins: abundant&lt;br /&gt;
** Argon: high&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: moderate&lt;br /&gt;
** Magnetosphere: Weak, multipolar and intermittent&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Dense iron-rich core with impact inclusions (e.g., iridium, ruthenium)&lt;br /&gt;
** Volcanically active mantle with carbon-rich inclusions&lt;br /&gt;
** Higher internal heat flow than Sapphire&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar cyclonic basins with geyser-like haze columns&lt;br /&gt;
** Frequent UV lightning within organic clouds&lt;br /&gt;
** Faint auroral echoes from Sapphire’s magnetospheric tail&lt;br /&gt;
** Surface glow from argon emissions during conjunction&lt;br /&gt;
&lt;br /&gt;
Mutual Phenomena &amp;amp; Sky Effects&lt;br /&gt;
* Eclipse Cycles: Frequent, due to short mutual period and perpendicular orbit; cause wave-like haze patterns and shadow bands&lt;br /&gt;
* Filamentary Atmosphere Bridges: Transient stratospheric strands near L1, illuminated during eclipses&lt;br /&gt;
* Auroral Flux Tubes: Occasionally connect the two with violet-green flickering arcs&lt;br /&gt;
* Gravitational Stability: Mutual orbit stable within Hill sphere; resistant to long-term disruption&lt;br /&gt;
&lt;br /&gt;
* Legacy of the Comet Shield&lt;br /&gt;
* Each planet’s core contains embedded relics of the system’s ancient bombardment:&lt;br /&gt;
** Sapphire: interstellar dust, primordial isotopes, deep xenon pockets&lt;br /&gt;
** Rust: impact-derived siderophiles, compressed organics, rare isotopic anomalies&lt;br /&gt;
* Capture Events: Both planets have intercepted and redirected hundreds of large icy bodies over system history&lt;br /&gt;
&lt;br /&gt;
They each have 2 small irregular moons, &amp;lt;100 km diameter, retrograde, on distant orbits.  Negligible.&lt;br /&gt;
== Planet C ==&lt;br /&gt;
&lt;br /&gt;
* With an albedo of 0.2, the global average temp is 263ºK.  Because of modest greenhouse effects, surface temperatures are higher, on the sun-side.&lt;br /&gt;
# Mass: 1.5M⊕&lt;br /&gt;
# Gravity: 1g⊕&lt;br /&gt;
# Radius = 1.225⊕, or 7805km&lt;br /&gt;
Terminator Zone&lt;br /&gt;
# +/-30º: 1.28 E8 km&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; (slightly less than all the land of the Earth)&lt;br /&gt;
# Escape velocity is 12.4km/s, 11% higher than Earth&lt;br /&gt;
# Orbital velocity is 8.79km/s&lt;br /&gt;
=== Atmosphere ===&lt;br /&gt;
Water content is low because&lt;br /&gt;
* Water vapor is a potent greenhouse gas; vast surface water can trap too much heat, especially near the substellar point.&lt;br /&gt;
* Water leads to climate homogenization&lt;br /&gt;
* Lack of exposed silicate rock: Necessary for carbon-silicate weathering feedback, which stabilizes climate on geological timescales.&lt;br /&gt;
Earth has ~1.4 billion km³ of water.  In our habitable zone, we have no more than 10% of that, or 100 million km³, though there is much more on the night side, both liquid and ice.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Factor !! Ɬiʔa atm !! Ɬiʔa % !! Earth atm !! Earth % !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! Total Pressure &lt;br /&gt;
| 1.6 atm || || 1.0 atm || || Enhanced convective heat transfer, increased IR trapping&lt;br /&gt;
|-&lt;br /&gt;
! Nitrogen (N₂) &lt;br /&gt;
| 1.00 || 62.50% || 0.7808 || 78.08% || Reduced; still inert, still dominant&lt;br /&gt;
|-&lt;br /&gt;
! Oxygen (O₂) &lt;br /&gt;
| 0.21 || 13.13% || 0.2095 || 20.95% || Earth-normal partial pressure &lt;br /&gt;
|-&lt;br /&gt;
! Argon (Ar)&lt;br /&gt;
| 0.40 || 25.00% || 0.0093 || 0.93% || Major heat distribution enhancement, inert&lt;br /&gt;
|-&lt;br /&gt;
! Krypton + Xenon&lt;br /&gt;
| 0.005 || 0.31% || trace || trace || High molecular mass → improved heat retention, still safe&lt;br /&gt;
|-&lt;br /&gt;
! CO₂&lt;br /&gt;
| 0.005 || 0.31% || 0.004 || 0.04% || slightly elevated; sub-greenhouse threshold&lt;br /&gt;
|-&lt;br /&gt;
! H₂O vapor &lt;br /&gt;
| 0.015 || ~1% || || 0-4% || Maintains greenhouse without excess moisture&lt;br /&gt;
|}&lt;br /&gt;
==== Atmospheric Effects on Clouds ====&lt;br /&gt;
# Increased Pressure (1.6 atm) compresses gases, raising the dew point at which water vapor condenses. Clouds form closer to the surface, and are denser than similar altitudes compared to Earth.&lt;br /&gt;
# Low Water Inventory (~20% of Earth&#039;s): less frequent and less massive cloud systems than on Earth, but still present—especially over &amp;quot;hotspots&amp;quot; on the day side.&lt;br /&gt;
# Tidally Locked Climate: Cloud formation concentrate along the substellar point, where warm, moist air rises and cools.&lt;br /&gt;
#* A permanent “eyewall” storm system has formed at the subsolar point, like a giant hurricane.&lt;br /&gt;
#* As air rises and is advected to the night side, thin cloud bands or ice hazes form as it descends and cools.&lt;br /&gt;
&lt;br /&gt;
Appearance:&lt;br /&gt;
* The presence of noble gases (Ar, Kr, Xe) and higher pressure enhance Mie scattering, making clouds appear whiter and more silvered, especially at sunrise/sunset boundaries.&lt;br /&gt;
* Night side clouds are thin, high-altitude icy sheets, glowing faintly in aurorae or thermal emissions.&lt;br /&gt;
&lt;br /&gt;
==== Sky Color ====&lt;br /&gt;
The color of the sky is shaped by Rayleigh scattering, which depends on:&lt;br /&gt;
# Molecular composition: Heavier gases like Ar, Kr, and Xe scatter light less efficiently than N₂.&lt;br /&gt;
# Spectral output of the star: the red dwarf emits predominantly infrared and red light, with very little blue or violet.&lt;br /&gt;
&lt;br /&gt;
Consequence:&lt;br /&gt;
* Even with atmospheric scattering, there is insufficient blue light in the stellar spectrum to produce a blue sky.&lt;br /&gt;
* Day sky would likely appear:&lt;br /&gt;
** Dark peach, dusky rose, or reddish beige near zenith,&lt;br /&gt;
** Grading to deep salmon or mauve near the horizon,&lt;br /&gt;
** A slight metallic sheen due to noble gas content and high pressure.&lt;br /&gt;
&lt;br /&gt;
Twilight &amp;amp; Limb Scattering:&lt;br /&gt;
* The terminator (twilight zone) sees a diffuse, ruddy light, scattering through haze and clouds into luminous reds, purples, and copper tones.&lt;br /&gt;
* Aurorae are spectacular on the night side, especially since stellar flares are frequent.&lt;br /&gt;
&lt;br /&gt;
==== Sound Propagation ====&lt;br /&gt;
: &#039;&#039;Sound is profoundly affected by atmospheric pressure and composition.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Compared to Earth:&lt;br /&gt;
* Higher pressure → greater air density → faster transmission of sound and less attenuation.&lt;br /&gt;
* Argon and Xenon are heavy gases, which:&lt;br /&gt;
** Lower the speed of sound relative to air at the same pressure (despite the pressure increase).&lt;br /&gt;
** Shift resonance frequencies downward, resulting in deeper, rounder sounds.&lt;br /&gt;
&lt;br /&gt;
Consequences:&lt;br /&gt;
* Voices sound subtly lower-pitched and richer, especially for consonants and low vowels.&lt;br /&gt;
* Ambient sounds (wind, water, animals) would carry farther and sound more muffled or sonorous.&lt;br /&gt;
* Music or speech would resonate more warmly, especially indoors or in enclosed spaces.&lt;br /&gt;
&lt;br /&gt;
In short: it sounds like it’s wrapped in velvet.&lt;br /&gt;
&lt;br /&gt;
==== Heat Transport to the Night Side ====&lt;br /&gt;
Mechanisms:&lt;br /&gt;
# Thick Atmosphere (1.6 atm) increases:&lt;br /&gt;
#* Advection efficiency: Warm air masses can move more heat horizontally.&lt;br /&gt;
#* Radiative time constant: The atmosphere holds heat longer before releasing it.&lt;br /&gt;
# Noble Gases (especially Kr/Xe):&lt;br /&gt;
#* High molecular mass → more IR opacity → trapping and radiating heat more evenly.&lt;br /&gt;
# Slow Rotation / Tidal Locking:&lt;br /&gt;
#* Global Hadley-like cells dominate circulation, carrying warm air from the day side to the night side and descending it there.&lt;br /&gt;
&lt;br /&gt;
Result:&lt;br /&gt;
* The night side is not so freezing.  Temperatures differ by tens of degrees, not hundreds.&lt;br /&gt;
* There are still ice caps and a cold deserts at the anti-stellar point, but not a glaciated wasteland.&lt;br /&gt;
&lt;br /&gt;
=== Magnetosphere ===&lt;br /&gt;
* Larger mass --&amp;gt; larger iron core, generating more internal heat&lt;br /&gt;
* Larger radius --&amp;gt; Vigorous convection in the core&lt;br /&gt;
* Tidal Flexing --&amp;gt; still drives magnetic activity&lt;br /&gt;
&lt;br /&gt;
# Aurorae at lower latitudes&lt;br /&gt;
## higher magnetic rigidity, wider magnetotail, and greater reconnection energy.&lt;br /&gt;
## Combined with a higher flux of stellar particles, this means:&lt;br /&gt;
### Auroral ovals expand, reaching mid-latitudes sometimes equator.&lt;br /&gt;
### The skies are alive with rippling green, violet, and crimson aurorae, especially on the night side.&lt;br /&gt;
### Daily auroral activity occur during stellar flare cycles.&lt;br /&gt;
# Compasses&lt;br /&gt;
## compasses respond more sharply, with:&lt;br /&gt;
### Faster alignment.&lt;br /&gt;
### Greater resistance to local perturbations.&lt;br /&gt;
## However, frequent magnetic storms from stellar activity cause sudden declinations, reversals, or local anomalies.  In short, lots of aurorae equals dead compasses at the same time.&lt;br /&gt;
# Magnetic Field Strength &amp;gt; 100 μT &lt;br /&gt;
# Electromagnetism is more basic than chemistry or almost any other natural philosophy&lt;br /&gt;
&lt;br /&gt;
=== Substellar Point ===&lt;br /&gt;
The maximum incoming flux is very nearly the same as Earth&#039;s solar constant (≈1361 W/m²), but concentrated over one point rather than averaged over a rotating sphere.  Temperatures should be above 500ºK most of the time.  &lt;br /&gt;
&lt;br /&gt;
The magnetic north is also here. The thick atmosphere prevents too much loss here, but &lt;br /&gt;
* Charged particle influx&lt;br /&gt;
** Maximized at the substellar point—intense auroral and energetic particle precipitation&lt;br /&gt;
* Atmospheric ionization&lt;br /&gt;
** Constant production of high-energy ions and NOx compounds—UV fluorescence in upper sky&lt;br /&gt;
* Localized heating&lt;br /&gt;
** Augments already extreme temperatures—600–700 K surface&lt;br /&gt;
&lt;br /&gt;
== Artificially Tethered Moon ==&lt;br /&gt;
* 670,000 km up&lt;br /&gt;
* 7805 km in radius = same as the planet&lt;br /&gt;
* 1.33º of the sky, same as the sun&lt;br /&gt;
&lt;br /&gt;
A network of tethers/tension lines from the moon to multiple anchor points on the planet’s surface (a tripod or hexapod structure), woven like hair&lt;br /&gt;
* Uses active tension management and orbital station-keeping to stabilize the moon&lt;br /&gt;
* Counterweights and inward-pointing mass drivers on the moon to oppose drift&lt;br /&gt;
&lt;br /&gt;
The tethers are not bearing the full weight, but merely damping drift, providing restoring force, and enabling long-term stability through active compensation.  The moon&lt;br /&gt;
* Blocks the worst of the heat&lt;br /&gt;
* Blocks the worst of the solar radiation&lt;br /&gt;
The moon has &lt;br /&gt;
* low mass&lt;br /&gt;
* high albedo - enormous reflectivity&lt;br /&gt;
* scatters charges particles, UV, X-rays, auroral flux tubes&lt;br /&gt;
* sunward - crazy hot, high emissivity&lt;br /&gt;
* earthward - crazy cool, low emissivity&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=File:Planet_b_by_GPT.png&amp;diff=168156</id>
		<title>File:Planet b by GPT.png</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=File:Planet_b_by_GPT.png&amp;diff=168156"/>
		<updated>2025-03-27T20:15:16Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: Exoplanet.  A super-Mercury around a red dwarf&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Summary ==&lt;br /&gt;
Exoplanet.  A super-Mercury around a red dwarf&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168100</id>
		<title>Ɬiʔa/Conworlding</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a/Conworlding&amp;diff=168100"/>
		<updated>2025-03-27T02:53:14Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: Created page with &amp;quot;== Star == Our star is a red-dwarf. # Type: M5V ## M: This indicates it&amp;#039;s a cool, red star with a surface temperature less than 3,500ºK ## 5: Within the M class, stars are further divided into subclasses 0-9, with 0 being the hottest and 9 the coolest. An M5 star is in the middle of this range. ## V: Denotes that it&amp;#039;s a main sequence star, also known as a dwarf star # Stellar luminosity (L*) ≈ 0.01 𝐿⊙ (1/100th Sol&amp;#039;s brightness) # Stellar mass (M*) ≈ 0.2 𝑀⊙...&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Star ==&lt;br /&gt;
Our star is a red-dwarf.&lt;br /&gt;
# Type: M5V&lt;br /&gt;
## M: This indicates it&#039;s a cool, red star with a surface temperature less than 3,500ºK&lt;br /&gt;
## 5: Within the M class, stars are further divided into subclasses 0-9, with 0 being the hottest and 9 the coolest. An M5 star is in the middle of this range.&lt;br /&gt;
## V: Denotes that it&#039;s a main sequence star, also known as a dwarf star&lt;br /&gt;
# Stellar luminosity (L*) ≈ 0.01 𝐿⊙ (1/100th Sol&#039;s brightness)&lt;br /&gt;
# Stellar mass (M*) ≈ 0.2 𝑀⊙ (1/5 the mass of Sol)&lt;br /&gt;
# Stellar radius (R*) ≈ 0.25 𝑅⊙ (1/4 as wide as Sol)&lt;br /&gt;
# Effective temperature (T*) ≈ 3500 K&lt;br /&gt;
​The habitable zone (a) is about square root of L* over L⊙, so ~0.1 AU.&lt;br /&gt;
&lt;br /&gt;
=== Solar System ===&lt;br /&gt;
There are seven planets in the system&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Planet !!	Mass (M🜨)!!	Radius (R🜨)!! Moons/Rings	!!Resonance !!	Semi-Major Axis (AU)!!	Rings !! Moons !! Period !! Size&lt;br /&gt;
|-&lt;br /&gt;
| b ||	2.17 ||	1.1 ||	No ||	2:3 with c	|| 0.0763 ||	No || No || 17.2 || 13.6&#039; to 1.5&#039;&lt;br /&gt;
|-&lt;br /&gt;
| c ||	1.5	 ||1.225 ||	1* ||	—	        || 0.100 || No || No || 25.8 || -&lt;br /&gt;
|-&lt;br /&gt;
| d ||	2.0	 ||1.4 ||No ||	2:3 with c	 ||0.131 ||	No || No || 38.7 || 13.1&#039; to 1.8&#039;&lt;br /&gt;
|-&lt;br /&gt;
| e ||	0.9 ||	1.0 || No	 ||	2:3 with d	 ||0.172 ||	No || No || 58 || 4.1&#039; to 1.1&#039;&lt;br /&gt;
|-&lt;br /&gt;
| f ||	3.5 ||	2.0 ||	Yes! ||	2:3 with e	 ||0.227 || Yes || Junk || 87 || 4.6&#039; to 1.8&#039;&lt;br /&gt;
|-&lt;br /&gt;
| g ||	2.6 ||	1.7 ||	2 ||	-	 ||0.40 ||	Yes || Junk || 206 || 1.6&#039; to 1.0&#039;&lt;br /&gt;
|-&lt;br /&gt;
| h ||	5.0x2 ||2.3x2 || yes	 || -	 ||1.5 ||	Yes || No || 1500 || 0.5&#039; 16.4&#039; apart (at max)&lt;br /&gt;
|}&lt;br /&gt;
==== b: super Mercury with a ring of fire  ====&lt;br /&gt;
b is a super-Mercury, tidally locked, and incredibly dense.  ~700ºK on the day side, ~50ºK on the night.  2.1 Earth Masses, 1.1 Earth radii (~7000km) in size.  Orbital period 17.2 days.  Density 9.0 g/cm&amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt;.  Gravity is ~1.8g.  &lt;br /&gt;
&lt;br /&gt;
The iron core is huge, being 75% of the mass.  A thin silicate mantle, with metallic plains and exhumed ultramafic crust, with frequent iron meteorite craters, lacking typical “stone” breccias.&lt;br /&gt;
&lt;br /&gt;
The night side is intense, as simple hydrocarbons (methane, ethane, propane) condense and freeze into layered deposits.  Complex organics (tholins, polycyclic aromatics) accumulate on the sea floor, under miles of nitrogen ice.  Massive slush layers slosh around above cryovolcanic brines of ammonia.&lt;br /&gt;
&lt;br /&gt;
There is a crucial layer of Superionic Ice XI above the core, which acts as an electromagnetic insulator, and ionic heat bridge.  The crust is ultramafic silicates (olivine, pyroxene, perovskite) riddled with with sulfide veins, iron alloys, and graphite networks.  The poles of the magnetosphere are sideways, like Uranus, with poles at the equator in the Terminator Zone.  Persistent surface charges develop, because the whole planet is basically a ginormous Leyden jar!&lt;br /&gt;
&lt;br /&gt;
A planetary flux rope forms and un-forms with the star and planet b.  This induces electric jets at the terminator.  This is where temps are Earth-like.  Hydrocarbons sublimate and eject into the atmosphere, even while aurorae come right down to the ground.  A small, low pressure atmosphere prevents photodissociation, even while electrothermal instabilities lift molecules, forming an anomalous haze, a standing, glowing ring.  Coronal events cause localized lightning geysers with magnetic arcing.&lt;br /&gt;
&lt;br /&gt;
In short, b is visible with a blinding bright sun side (glowing orange bronze), a utterly black night side, and a burning, glowing, erupting, arcing ring at the terminator (all colors).  At biggest, it&#039;s half the size of Earth&#039;s moon in the sky, shrinking down to a star at it&#039;s furthest away.&lt;br /&gt;
&lt;br /&gt;
==== d: the wet eye with depths ====&lt;br /&gt;
From the outside, d is a &amp;quot;wet eye&amp;quot; just outside the habitable zone.  It is a water world, twice the mass of Earth, 1.4 times the radius, tidally locked.  The substellar point is the only place without surface ice.  However, it is better to think of the planet top-to-bottom.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;atmosphere&#039;&#039;&#039; is tenuous, less than 0.2 bars.  It is thin, N₂-rich with traces of H₂O, NH₃ vapor, and transient geyser outputs.  It is highly UV-irradiated, and Mars-like in its inability to retain volatiles.&lt;br /&gt;
&lt;br /&gt;
Next, there is a &#039;&#039;&#039;surface ice shell&#039;&#039;&#039;, ~20 km of thick Ice I.  Swirling currents beneath have cracked continent-sized ice plates, similar to Europa&#039;s crust.  It is permanently frozen except at the substellar furnace.  It accumulates chemical stains, mineral deposits, and cryovolcanic eruption plumes.  Accumulations of complex hydrates—like methanol clathrates—precipitate out and form false reefs, rising like coral from beneath. Transient thermal vents push hot plumes into the thin air, freezing instantly and snowing down crystals that form mineral spires.&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;subglacial ocean&#039;&#039;&#039; is hundreds of kilometers thick.  It is super-pressurized liquid H₂O mixed with NH₃, CH₃OH, H₂O₂, and trace salts.  The movement is slow, planetary-scale currents originating from the Furnace and Coriolis force.  Strong layers exist: the surface is oxidized; the abyssal layer is reducing.&lt;br /&gt;
&lt;br /&gt;
A new &amp;quot;surface&amp;quot; is next.  The &#039;&#039;&#039;Ice Mantle&#039;&#039;&#039; is solid Ice VI and VII.  There are massive, slowly shifting &amp;quot;sub-oceanic continents&amp;quot;. It is periodically fractured and resurfaced by cryoquakes and brine-driven eruptions.  Some regions have developed elevated domes or ridges, continental “shelves” under the ocean.&lt;br /&gt;
&lt;br /&gt;
Finally, underneath is the &#039;&#039;&#039;core&#039;&#039;&#039;. Temperatures exceed 2000–3000 K locally.  Pressures range from 100 to 300 GPa.  The core is rich in heavy elements.  This makes radiogenic hotspots, localized magnetic eddies.  Heat gradients + ion flows = thermoelectric currents.  These make magnetic storms within the ocean itself, not the sky.  When uranium-rich corium pods shift or explode upward through the mantle, their heat and conductivity disturb the local magnetic field, generating geomagnetic quakes.  These pulse through the ocean, creating short-lived magnetic lenses.  These interact with atmospheric charged particles above the Furnace, giving rise to transient magnetic halos visible from orbit—false auroras without a sunstorm.&lt;br /&gt;
&lt;br /&gt;
==== e: The Tortured Near-Sphere ====&lt;br /&gt;
&lt;br /&gt;
Orbital and Physical Characteristics&lt;br /&gt;
* Mass: 0.9 Earth masses&lt;br /&gt;
* Radius: 1.0 Earth radii&lt;br /&gt;
* Orbital Period: 58 Earth days&lt;br /&gt;
* Surface Gravity: ~0.9 g&lt;br /&gt;
* Semimajor Axis: ~0.17 AU &lt;br /&gt;
* Spin State: In the &#039;&#039;process&#039;&#039; of becoming tidally locked&lt;br /&gt;
* Obliquity: Extreme, experiencing chaotic realignment events&lt;br /&gt;
&lt;br /&gt;
Internal Structure and Composition&lt;br /&gt;
* &#039;&#039;&#039;Crust:&#039;&#039;&#039; A thick, rigid outer shell of water ice I mixed with clathrates (CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; and CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; hydrates), underlain by layers of ammonia-water ice eutectics. Inclusions of carbon under extreme pressure form diamond strata in the lower crust, lending rigidity and brittle behavior.&lt;br /&gt;
* &#039;&#039;&#039;Mantle:&#039;&#039;&#039; Comprised of Ice VI and Ice VII, with ammonia- and methane-rich brines forming localized conduits and pockets of unstable volatiles.&lt;br /&gt;
* &#039;&#039;&#039;Core:&#039;&#039;&#039; Differentiated and semi-molten. Inner core of iron-nickel alloy spins at a different rate. Outer core is a highly viscous slurry of silicate, iron, carbon, sulfur, and dissolved volatiles. Chemical veins (e.g., uranium silicates, perovskites) act as mechanical shear zones. Tidal torque leads to periodic frictional heating.&lt;br /&gt;
&lt;br /&gt;
Tectonic and Cryovolcanic Behavior&lt;br /&gt;
* The planet resists tidal locking due to core-crust decoupling and uneven angular momentum transfer.&lt;br /&gt;
* High obliquity experiences &#039;&#039;&#039;&#039;&#039;Axial Recoil Events&#039;&#039;&#039;&#039;&#039;, where the entire planet jerks between metastable orientations (e.g., from 110° to 70°) in sudden spasms.&lt;br /&gt;
* These events generate:&lt;br /&gt;
** Global-scale crustal cracking&lt;br /&gt;
** Venting of pressurized subsurface gases (H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;O, CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt;)&lt;br /&gt;
** Surface deformation and glacial faulting&lt;br /&gt;
* Volatiles erupt ballistically into space (200+lm) from exposed fissures and calderas, driven by phase-change explosions.&lt;br /&gt;
&lt;br /&gt;
Surface Conditions&lt;br /&gt;
* Global temperature well below freezing; warmest zones around cryovolcanic hotspots&lt;br /&gt;
* Crustal coloration varies by volatile deposition:&lt;br /&gt;
** Pale blue-white from water ice&lt;br /&gt;
** Red-brown from CO&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; frostfields&lt;br /&gt;
** Green-black CH&amp;lt;sub&amp;gt;4&amp;lt;/sub&amp;gt; stains from plume fallout&lt;br /&gt;
* Surface features include:&lt;br /&gt;
** Cryovolcanic calderas&lt;br /&gt;
** Diamond-studded impact-like basins&lt;br /&gt;
** Faulted plains crossed by salt-streaked rift zones&lt;br /&gt;
&lt;br /&gt;
Atmosphere and Ejected Material&lt;br /&gt;
* Thin transient exosphere formed from eruptive events&lt;br /&gt;
* Gases often escape to space or freeze back out in polar regions&lt;br /&gt;
* Fallback material creates uneven surface mass distributions, altering moment of inertia and prolonging instability&lt;br /&gt;
&lt;br /&gt;
Appearance from Planet c&lt;br /&gt;
&lt;br /&gt;
* Angular Size: ~4-1 arcminutes&lt;br /&gt;
* Coloration: Overall dusky grey-white, with changing colored bands due to volatile fallout; craterless but mottled&lt;br /&gt;
&lt;br /&gt;
Transient visible phenomena:&lt;br /&gt;
&lt;br /&gt;
* Cryovolcanic plumes visible as fan-like arcs at the limb during outburst events&lt;br /&gt;
* Infrared brightening during Axial Recoil Events&lt;br /&gt;
* Occasional light-scattering halos from plume particles&lt;br /&gt;
&lt;br /&gt;
Event Cycle Summary&lt;br /&gt;
&lt;br /&gt;
# Tidal torque builds due to obliquity misalignment&lt;br /&gt;
# Core resists, crust locks tension&lt;br /&gt;
# Critical stress threshold breached&lt;br /&gt;
# Obliquity lurches to new orientation&lt;br /&gt;
# Crust fractures globally, vents open&lt;br /&gt;
# Supersonic cryovolcanism hurls volatiles into space&lt;br /&gt;
# Fallback modifies crustal mass distribution&lt;br /&gt;
# Obliquity rebuilds instability over decades&lt;br /&gt;
# Repeat.&lt;br /&gt;
&lt;br /&gt;
Planet e is a tortured world caught in an unending cycle of self-correcting failure—its body unable to align, its gases unable to stay contained, its appearance in the sky a visible signature of internal catastrophe.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==== f: Ringed Mini-Neptune ====&lt;br /&gt;
This planet is a substantial mini-Neptune, with a mass of approximately 3.5 Earth masses and a radius of 2.0 Earth radii, orbiting at 0.227 AU. Its low mean density (~0.44 ρ⊕) signals the presence of a deep, volatile-rich envelope overlying a denser core. The bulk of its volume is composed of hydrogen and helium, accreted from the protoplanetary disk, with trace amounts of methane (CH₄) and ammonia (NH₃)—gases that dominate its photochemical and radiative behavior. Beneath this envelope, the planet hosts a water–rock–metal core layered in complex phases, with high-pressure ices and possibly superionic water enveloping a metallic center.  Lower atmosphere reaches 300–500 K (27–227°C) near the bottom of the troposphere, depending on opacity and convection.&lt;br /&gt;
&lt;br /&gt;
Visually, the planet exhibits a blue-to-cyan atmospheric hue, governed by Rayleigh scattering and methane absorption in the red and near-infrared spectrum. While not as banded or storm-laced as Jupiter, it features broad zonal flows, high-altitude methane ice clouds, and long-lived anticyclonic storms akin to Neptune’s Great Dark Spot. Due to its tidal locking to the host star, the planet presents hemispheric climatic asymmetry: a sunlit dayside prone to atmospheric upwelling and cloud formation, and a cooler, darker nightside. While colder, the backside is not freezing— in the 150–250 K range, depending on circulation efficiency. Atmospheric circulation is dominated by slow, large-scale overturning cells, moderated by planetary-scale waves and a subdued Coriolis force. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Rings =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Ring!!	Range (Rₚ)!!	Approx.! Range (km)!!	Description&lt;br /&gt;
|-&lt;br /&gt;
! C&lt;br /&gt;
| 	1.5–1.65 Rₚ	||19,100–21,000	||Faint, dusty interior ring&lt;br /&gt;
|-&lt;br /&gt;
! B&lt;br /&gt;
| 	1.65–1.96 Rₚ	||21,000–25,000||	Bright, dense primary ring&lt;br /&gt;
|-&lt;br /&gt;
! Division&lt;br /&gt;
|	1.96–2.04 Rₚ ||25,000–26,000 || a low-density gap&lt;br /&gt;
|-&lt;br /&gt;
!  A&lt;br /&gt;
|	2.04–2.3 Rₚ||26,000–29,300||	Sharp-edged outer ring&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Moon !!	Orbit (km) !!	Orbit (Rₚ) !!	Diameter (km) !!	Type	!! Period !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! I&lt;br /&gt;
|	60,000	||4.7 Rₚ	||~400	||Rocky	|| 0.9 ||Cratered&lt;br /&gt;
|-&lt;br /&gt;
! II&lt;br /&gt;
| 	110,000	|| 8.6 Rₚ	|| ~800	|| Mixed rock/ice	|| 2.25|| Cracked surface, frozen ocean&lt;br /&gt;
|-&lt;br /&gt;
! III &lt;br /&gt;
| 190,000	|| 14.9 Rₚ ||	~1200 ||	Icy major moon ||	5.1|| Cryovolcanism, smooth plains&lt;br /&gt;
|-&lt;br /&gt;
! IV &lt;br /&gt;
|340,000	||26.7 Rₚ	||~200	||Irregular/prograde	|| 12.21 || Dark red/carbon, inclined (20º, eccentric orbit (0.1)&lt;br /&gt;
|-&lt;br /&gt;
! V &lt;br /&gt;
| 710,000 ||	55.7 Rₚ	||~350	|| Captured/retrograde	|| 36.83 || Highly inclined (130º), Split terrain—half rugged highlands, half smooth resurfaced plain&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
==== g: Stripped Sub-Neptune Remnant ====&lt;br /&gt;
&lt;br /&gt;
Basic Parameters&lt;br /&gt;
* Mass: 2.6 Earth masses (M⊕)&lt;br /&gt;
* Radius: 1.7 Earth radii (R⊕)&lt;br /&gt;
* Mean Density: ~2.92 g/cm³&lt;br /&gt;
* Orbital Distance: 0.4 AU &lt;br /&gt;
* Albedo: ~0.5 (moderately high)&lt;br /&gt;
* Rotation: Tidally locked &lt;br /&gt;
&lt;br /&gt;
Origin and Evolution&lt;br /&gt;
* Formed beyond the snow line (~0.8–1.2 AU) from a mix of rock, iron, and ices&lt;br /&gt;
* Migrated inward early during protoplanetary disk phase&lt;br /&gt;
* Accreted a modest hydrogen-helium envelope (&amp;gt;1% by mass)&lt;br /&gt;
* Exposed to intense stellar X-ray and UV radiation during the M dwarf&#039;s pre-main-sequence phase&lt;br /&gt;
* Lacked a magnetic dynamo (metal-poor and early core freezing)&lt;br /&gt;
* Entire atmosphere lost over ~100 Myr via photoevaporation, core-powered mass loss, and sputtering&lt;br /&gt;
&lt;br /&gt;
Current State&lt;br /&gt;
* Atmosphere: None (trace mineral vapors possible in hot regions)&lt;br /&gt;
* Surface: Stark contrast between hemispheres due to tidal locking&lt;br /&gt;
** Dayside: ~700–1000 K; high-silica lava fields, salt flats, exposed alumino-silicates&lt;br /&gt;
** Nightside: ~100–150 K; gypsum and calcite in cold traps, frozen regolith&lt;br /&gt;
* Magnetosphere: Absent&lt;br /&gt;
* Volcanism:episodic; high-silica flows, volcanic glass, sodium-rich crusts&lt;br /&gt;
* Geological Activity: Tectonically inactive; thermally fractured plains, impact craters&lt;br /&gt;
&lt;br /&gt;
Surface Composition&lt;br /&gt;
* Titanium dioxide (rutile): bright, high-albedo mineral condensate&lt;br /&gt;
* Calcite (CaCO₃): carbonate deposits in cold traps&lt;br /&gt;
* Gypsum (CaSO₄·2H₂O): hydration mineral, stable only on the nightside&lt;br /&gt;
* Sodium chloride: salt flats, especially in evaporated basins&lt;br /&gt;
* High-silica volcanic deposits: glassy, oxidized, and light-colored&lt;br /&gt;
&lt;br /&gt;
Visual and Observational Notes&lt;br /&gt;
&lt;br /&gt;
* High visual contrast between molten and frozen hemispheres&lt;br /&gt;
* Surface appears mottled: obsidian-black lava, gleaming salt flats, white calcium deposits&lt;br /&gt;
* No clouds, auroras, or magnetic activity&lt;br /&gt;
* Extreme day/night temperature gradient&lt;br /&gt;
* Reflective phase curve possible in photometric observations&lt;br /&gt;
* Surface pressure: effectively 0 bar&lt;br /&gt;
&lt;br /&gt;
Planet g is the airless skeleton of a once-sub-Neptune world. Born icy and distant, it migrated into the young star&#039;s wrath, where its fragile envelope boiled away under a sky of flares. Bereft of a magnetic shield, it was slowly stripped to bare rock. Today, one hemisphere bakes in molten silence while the other freezes in shadow. No air, no oceans, only salt, stone, and the echo of a lost atmosphere.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===== Moons =====&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property !!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~75,000 km (~0.26 R&amp;lt;sub&amp;gt;hill&amp;lt;/sub&amp;gt;)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~1,400 km (~0.22 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass	&lt;br /&gt;
| ~0.01 M⊕ (~1.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~3.0 g/cm³ (rock–ice mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temp&lt;br /&gt;
|	~150–180 K&lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
| 0.20g&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere&lt;br /&gt;
|	Trace O₂, from radiolysis and outgassing&lt;br /&gt;
|-&lt;br /&gt;
! Subsurface Ocean&lt;br /&gt;
|	heated by tidal flexing&lt;br /&gt;
|-&lt;br /&gt;
! Surface Features	&lt;br /&gt;
|Fractured ice crust, chaos terrain, cryogeysers, lenticulae&lt;br /&gt;
|}&lt;br /&gt;
gI is a cracked glass orb, rimed with frost and laced with luminous fissures. Below its crust, tides flex a hidden ocean in rhythmic silence. Its faint oxygen exosphere is ghostly but present.  It is frosted quartz with cobwebbed streaks and mineral discoloration.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Property!!	Value&lt;br /&gt;
|-&lt;br /&gt;
! Orbital Radius&lt;br /&gt;
|	~150,000 km (~0.5 Rₕill)&lt;br /&gt;
|-&lt;br /&gt;
! Radius&lt;br /&gt;
|	~2,100 km (~0.33 R⊕)&lt;br /&gt;
|-&lt;br /&gt;
! Mass&lt;br /&gt;
|	~0.035 M⊕ (~4.2% Earth)&lt;br /&gt;
|-&lt;br /&gt;
! Density&lt;br /&gt;
|	~2.1 g/cm³ (icy-rocky mix)&lt;br /&gt;
|-&lt;br /&gt;
! Tidal Locked&lt;br /&gt;
|	Yes &lt;br /&gt;
|-&lt;br /&gt;
! Surface Gravity&lt;br /&gt;
|	~0.35 g&lt;br /&gt;
|-&lt;br /&gt;
! Surface Temperature&lt;br /&gt;
|	~115–130 K (pressure and greenhouse effects)&lt;br /&gt;
|-&lt;br /&gt;
! Atmosphere	&lt;br /&gt;
| ~0.18 bar N₂ + ~0.1 bar Ar + ~0.02 bar CH₄, minor CO, trace haze &lt;br /&gt;
|}&lt;br /&gt;
gII is a muted blue-green crescent veiled in gold. Its sky glows with the weight of argon and the shimmer of methane haze, and its surface smolders with the memory of internal warmth. Liquid hydrocarbons shine like ink in the basins, while glaciers ebb across the uplands. To the star it shows only one face, but beneath that still gaze lies the soft breath of a world more welcoming than its master.&lt;br /&gt;
&lt;br /&gt;
==== h ====&lt;br /&gt;
h is a twin-planet system, 1.5 AU from the star, with a period of 4.1 years&lt;br /&gt;
&lt;br /&gt;
Mutual Orbital Configuration&lt;br /&gt;
* Type: True binary planet pair, gravitationally bound, equal mass&lt;br /&gt;
* Masses: 5.0 M⊕ each&lt;br /&gt;
* Radii: 2.3 R⊕ each&lt;br /&gt;
* Mutual Orbit: Essentially circular, ~1 million km separation (~8–10 planetary radii)&lt;br /&gt;
* Period (mutual orbit): ~4.5 days&lt;br /&gt;
* Orbital Plane: Perpendicular to system ecliptic &lt;br /&gt;
* Tidal State: Tidally locked to each other (mutual synchronous rotation)&lt;br /&gt;
&lt;br /&gt;
Planet A — &amp;quot;Sapphire&amp;quot;&lt;br /&gt;
* Coloration: Deep sapphire blue with white high-altitude methane ice hazes&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: H₂, He&lt;br /&gt;
** Methane (CH₄): high&lt;br /&gt;
** Ammonia: trace&lt;br /&gt;
** Argon: moderate&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: slightly enriched&lt;br /&gt;
* Magnetosphere: Strong, symmetric; supports brilliant blue-violet aurorae&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Superionic water mantle&lt;br /&gt;
** Stratified silicate-ice alloy core&lt;br /&gt;
** Radiogenic heating and layered convection&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar hexagonal jet (stronger than Saturn&#039;s)&lt;br /&gt;
** Methane plasma flares at terminator&lt;br /&gt;
** Iridescent methane cirrus clouds&lt;br /&gt;
** Massive auroral crowns aligned with spin-magnetic axis misalignment&lt;br /&gt;
&lt;br /&gt;
Planet B — &amp;quot;Rust&amp;quot;&lt;br /&gt;
* Coloration: Dark crimson to rust-red, streaked with black and violet haze bands&lt;br /&gt;
* Atmosphere:&lt;br /&gt;
** Dominant: N₂, CO&lt;br /&gt;
** CH₄: trace&lt;br /&gt;
** Tholins: abundant&lt;br /&gt;
** Argon: high&lt;br /&gt;
** Krypton: balanced&lt;br /&gt;
** Xenon: moderate&lt;br /&gt;
** Magnetosphere: Weak, multipolar and intermittent&lt;br /&gt;
* Internal Structure:&lt;br /&gt;
** Dense iron-rich core with impact inclusions (e.g., iridium, ruthenium)&lt;br /&gt;
** Volcanically active mantle with carbon-rich inclusions&lt;br /&gt;
** Higher internal heat flow than Sapphire&lt;br /&gt;
* Notable Phenomena:&lt;br /&gt;
** Polar cyclonic basins with geyser-like haze columns&lt;br /&gt;
** Frequent UV lightning within organic clouds&lt;br /&gt;
** Faint auroral echoes from Sapphire’s magnetospheric tail&lt;br /&gt;
** Surface glow from argon emissions during conjunction&lt;br /&gt;
&lt;br /&gt;
Mutual Phenomena &amp;amp; Sky Effects&lt;br /&gt;
* Eclipse Cycles: Frequent, due to short mutual period and perpendicular orbit; cause wave-like haze patterns and shadow bands&lt;br /&gt;
* Filamentary Atmosphere Bridges: Transient stratospheric strands near L1, illuminated during eclipses&lt;br /&gt;
* Auroral Flux Tubes: Occasionally connect the two with violet-green flickering arcs&lt;br /&gt;
* Gravitational Stability: Mutual orbit stable within Hill sphere; resistant to long-term disruption&lt;br /&gt;
&lt;br /&gt;
* Legacy of the Comet Shield&lt;br /&gt;
* Each planet’s core contains embedded relics of the system’s ancient bombardment:&lt;br /&gt;
** Sapphire: interstellar dust, primordial isotopes, deep xenon pockets&lt;br /&gt;
** Rust: impact-derived siderophiles, compressed organics, rare isotopic anomalies&lt;br /&gt;
* Capture Events: Both planets have intercepted and redirected hundreds of large icy bodies over system history&lt;br /&gt;
&lt;br /&gt;
They each have 2 small irregular moons, &amp;lt;100 km diameter, retrograde, on distant orbits.  Negligible.&lt;br /&gt;
== Planet C ==&lt;br /&gt;
&lt;br /&gt;
* With an albedo of 0.2, the global average temp is 263ºK.  Because of modest greenhouse effects, surface temperatures are higher, on the sun-side.&lt;br /&gt;
# Mass: 1.5M⊕&lt;br /&gt;
# Gravity: 1g⊕&lt;br /&gt;
# Radius = 1.225⊕, or 7805km&lt;br /&gt;
Terminator Zone&lt;br /&gt;
# +/-30º: 1.28 E8 km&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; (slightly less than all the land of the Earth)&lt;br /&gt;
# Escape velocity is 12.4km/s, 11% higher than Earth&lt;br /&gt;
# Orbital velocity is 8.79km/s&lt;br /&gt;
=== Atmosphere ===&lt;br /&gt;
Water content is low because&lt;br /&gt;
* Water vapor is a potent greenhouse gas; vast surface water can trap too much heat, especially near the substellar point.&lt;br /&gt;
* Water leads to climate homogenization&lt;br /&gt;
* Lack of exposed silicate rock: Necessary for carbon-silicate weathering feedback, which stabilizes climate on geological timescales.&lt;br /&gt;
Earth has ~1.4 billion km³ of water.  In our habitable zone, we have no more than 10% of that, or 100 million km³, though there is much more on the night side, both liquid and ice.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Factor !! Ɬiʔa atm !! Ɬiʔa % !! Earth atm !! Earth % !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! Total Pressure &lt;br /&gt;
| 1.6 atm || || 1.0 atm || || Enhanced convective heat transfer, increased IR trapping&lt;br /&gt;
|-&lt;br /&gt;
! Nitrogen (N₂) &lt;br /&gt;
| 1.00 || 62.50% || 0.7808 || 78.08% || Reduced; still inert, still dominant&lt;br /&gt;
|-&lt;br /&gt;
! Oxygen (O₂) &lt;br /&gt;
| 0.21 || 13.13% || 0.2095 || 20.95% || Earth-normal partial pressure &lt;br /&gt;
|-&lt;br /&gt;
! Argon (Ar)&lt;br /&gt;
| 0.40 || 25.00% || 0.0093 || 0.93% || Major heat distribution enhancement, inert&lt;br /&gt;
|-&lt;br /&gt;
! Krypton + Xenon&lt;br /&gt;
| 0.005 || 0.31% || trace || trace || High molecular mass → improved heat retention, still safe&lt;br /&gt;
|-&lt;br /&gt;
! CO₂&lt;br /&gt;
| 0.005 || 0.31% || 0.004 || 0.04% || slightly elevated; sub-greenhouse threshold&lt;br /&gt;
|-&lt;br /&gt;
! H₂O vapor &lt;br /&gt;
| 0.015 || ~1% || || 0-4% || Maintains greenhouse without excess moisture&lt;br /&gt;
|}&lt;br /&gt;
==== Atmospheric Effects on Clouds ====&lt;br /&gt;
# Increased Pressure (1.6 atm) compresses gases, raising the dew point at which water vapor condenses. Clouds form closer to the surface, and are denser than similar altitudes compared to Earth.&lt;br /&gt;
# Low Water Inventory (~20% of Earth&#039;s): less frequent and less massive cloud systems than on Earth, but still present—especially over &amp;quot;hotspots&amp;quot; on the day side.&lt;br /&gt;
# Tidally Locked Climate: Cloud formation concentrate along the substellar point, where warm, moist air rises and cools.&lt;br /&gt;
#* A permanent “eyewall” storm system has formed at the subsolar point, like a giant hurricane.&lt;br /&gt;
#* As air rises and is advected to the night side, thin cloud bands or ice hazes form as it descends and cools.&lt;br /&gt;
&lt;br /&gt;
Appearance:&lt;br /&gt;
* The presence of noble gases (Ar, Kr, Xe) and higher pressure enhance Mie scattering, making clouds appear whiter and more silvered, especially at sunrise/sunset boundaries.&lt;br /&gt;
* Night side clouds are thin, high-altitude icy sheets, glowing faintly in aurorae or thermal emissions.&lt;br /&gt;
&lt;br /&gt;
==== Sky Color ====&lt;br /&gt;
The color of the sky is shaped by Rayleigh scattering, which depends on:&lt;br /&gt;
# Molecular composition: Heavier gases like Ar, Kr, and Xe scatter light less efficiently than N₂.&lt;br /&gt;
# Spectral output of the star: the red dwarf emits predominantly infrared and red light, with very little blue or violet.&lt;br /&gt;
&lt;br /&gt;
Consequence:&lt;br /&gt;
* Even with atmospheric scattering, there is insufficient blue light in the stellar spectrum to produce a blue sky.&lt;br /&gt;
* Day sky would likely appear:&lt;br /&gt;
** Dark peach, dusky rose, or reddish beige near zenith,&lt;br /&gt;
** Grading to deep salmon or mauve near the horizon,&lt;br /&gt;
** A slight metallic sheen due to noble gas content and high pressure.&lt;br /&gt;
&lt;br /&gt;
Twilight &amp;amp; Limb Scattering:&lt;br /&gt;
* The terminator (twilight zone) sees a diffuse, ruddy light, scattering through haze and clouds into luminous reds, purples, and copper tones.&lt;br /&gt;
* Aurorae are spectacular on the night side, especially since stellar flares are frequent.&lt;br /&gt;
&lt;br /&gt;
==== Sound Propagation ====&lt;br /&gt;
: &#039;&#039;Sound is profoundly affected by atmospheric pressure and composition.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Compared to Earth:&lt;br /&gt;
* Higher pressure → greater air density → faster transmission of sound and less attenuation.&lt;br /&gt;
* Argon and Xenon are heavy gases, which:&lt;br /&gt;
** Lower the speed of sound relative to air at the same pressure (despite the pressure increase).&lt;br /&gt;
** Shift resonance frequencies downward, resulting in deeper, rounder sounds.&lt;br /&gt;
&lt;br /&gt;
Consequences:&lt;br /&gt;
* Voices sound subtly lower-pitched and richer, especially for consonants and low vowels.&lt;br /&gt;
* Ambient sounds (wind, water, animals) would carry farther and sound more muffled or sonorous.&lt;br /&gt;
* Music or speech would resonate more warmly, especially indoors or in enclosed spaces.&lt;br /&gt;
&lt;br /&gt;
In short: it sounds like it’s wrapped in velvet.&lt;br /&gt;
&lt;br /&gt;
==== Heat Transport to the Night Side ====&lt;br /&gt;
Mechanisms:&lt;br /&gt;
# Thick Atmosphere (1.6 atm) increases:&lt;br /&gt;
#* Advection efficiency: Warm air masses can move more heat horizontally.&lt;br /&gt;
#* Radiative time constant: The atmosphere holds heat longer before releasing it.&lt;br /&gt;
# Noble Gases (especially Kr/Xe):&lt;br /&gt;
#* High molecular mass → more IR opacity → trapping and radiating heat more evenly.&lt;br /&gt;
# Slow Rotation / Tidal Locking:&lt;br /&gt;
#* Global Hadley-like cells dominate circulation, carrying warm air from the day side to the night side and descending it there.&lt;br /&gt;
&lt;br /&gt;
Result:&lt;br /&gt;
* The night side is not so freezing.  Temperatures differ by tens of degrees, not hundreds.&lt;br /&gt;
* There are still ice caps and a cold deserts at the anti-stellar point, but not a glaciated wasteland.&lt;br /&gt;
&lt;br /&gt;
=== Magnetosphere ===&lt;br /&gt;
* Larger mass --&amp;gt; larger iron core, generating more internal heat&lt;br /&gt;
* Larger radius --&amp;gt; Vigorous convection in the core&lt;br /&gt;
* Tidal Flexing --&amp;gt; still drives magnetic activity&lt;br /&gt;
&lt;br /&gt;
# Aurorae at lower latitudes&lt;br /&gt;
## higher magnetic rigidity, wider magnetotail, and greater reconnection energy.&lt;br /&gt;
## Combined with a higher flux of stellar particles, this means:&lt;br /&gt;
### Auroral ovals expand, reaching mid-latitudes sometimes equator.&lt;br /&gt;
### The skies are alive with rippling green, violet, and crimson aurorae, especially on the night side.&lt;br /&gt;
### Daily auroral activity occur during stellar flare cycles.&lt;br /&gt;
# Compasses&lt;br /&gt;
## compasses respond more sharply, with:&lt;br /&gt;
### Faster alignment.&lt;br /&gt;
### Greater resistance to local perturbations.&lt;br /&gt;
## However, frequent magnetic storms from stellar activity cause sudden declinations, reversals, or local anomalies.  In short, lots of aurorae equals dead compasses at the same time.&lt;br /&gt;
# Magnetic Field Strength &amp;gt; 100 μT &lt;br /&gt;
# Electromagnetism is more basic than chemistry or almost any other natural philosophy&lt;br /&gt;
&lt;br /&gt;
=== Substellar Point ===&lt;br /&gt;
The maximum incoming flux is very nearly the same as Earth&#039;s solar constant (≈1361 W/m²), but concentrated over one point rather than averaged over a rotating sphere.  Temperatures should be above 500ºK most of the time.  &lt;br /&gt;
&lt;br /&gt;
The magnetic north is also here. The thick atmosphere prevents too much loss here, but &lt;br /&gt;
* Charged particle influx&lt;br /&gt;
** Maximized at the substellar point—intense auroral and energetic particle precipitation&lt;br /&gt;
* Atmospheric ionization&lt;br /&gt;
** Constant production of high-energy ions and NOx compounds—UV fluorescence in upper sky&lt;br /&gt;
* Localized heating&lt;br /&gt;
** Augments already extreme temperatures—600–700 K surface&lt;br /&gt;
&lt;br /&gt;
== Artificially Tethered Moon ==&lt;br /&gt;
* 670,000 km up&lt;br /&gt;
* 7805 km in radius = same as the planet&lt;br /&gt;
* 1.33º of the sky, same as the sun&lt;br /&gt;
&lt;br /&gt;
A network of tethers/tension lines from the moon to multiple anchor points on the planet’s surface (a tripod or hexapod structure), woven like hair&lt;br /&gt;
* Uses active tension management and orbital station-keeping to stabilize the moon&lt;br /&gt;
* Counterweights and inward-pointing mass drivers on the moon to oppose drift&lt;br /&gt;
&lt;br /&gt;
The tethers are not bearing the full weight, but merely damping drift, providing restoring force, and enabling long-term stability through active compensation.  The moon&lt;br /&gt;
* Blocks the worst of the heat&lt;br /&gt;
* Blocks the worst of the solar radiation&lt;br /&gt;
The moon has &lt;br /&gt;
* low mass&lt;br /&gt;
* high albedo - enormous reflectivity&lt;br /&gt;
* scatters charges particles, UV, X-rays, auroral flux tubes&lt;br /&gt;
* sunward - crazy hot, high emissivity&lt;br /&gt;
* earthward - crazy cool, low emissivity&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a&amp;diff=168086</id>
		<title>Ɬiʔa</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a&amp;diff=168086"/>
		<updated>2025-03-26T18:44:14Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* Conworlding */ making a subpage for all this&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Goals ==&lt;br /&gt;
# Endgoal - A truly verbless language I can use&lt;br /&gt;
# Vague phrases&lt;br /&gt;
## Glacial pace&lt;br /&gt;
## Navajo-of-nouns&lt;br /&gt;
## lazy but clever&lt;br /&gt;
## carved in stone&lt;br /&gt;
## complicated rituals&lt;br /&gt;
# Naturalism - 6/10&lt;br /&gt;
#* I want some naturalistic elements&lt;br /&gt;
#* Different setting (parallel Earth)&lt;br /&gt;
#* Different nature (immortal humans)&lt;br /&gt;
#* Irregularities but not many&lt;br /&gt;
#* Idioms within reason&lt;br /&gt;
# Complexity - insane.  Navajo but with only nouns&lt;br /&gt;
# Derivation - clear.  Agglutinative, basically&lt;br /&gt;
# Features&lt;br /&gt;
## Phonology &lt;br /&gt;
### Vowel harmony&lt;br /&gt;
### A couple of clicks, and ejectives (un-earth-like)&lt;br /&gt;
### CV, and CVC &lt;br /&gt;
## Grammar&lt;br /&gt;
### No verbs at all&lt;br /&gt;
### assumed copular between topic and subject&lt;br /&gt;
### 6 nouns classes (genders), like animacy &lt;br /&gt;
### Many cases (12?)&lt;br /&gt;
### Case-stacking&lt;br /&gt;
### word glue, like German&lt;br /&gt;
### mostly agglutinative, touch of fusional&lt;br /&gt;
## Culture&lt;br /&gt;
### things happen, not because someone does them, but because the world unfolds in prescribed patterns&lt;br /&gt;
### discourse is formulaic, ceremonial, or sacred: more on set relational expressions and fixed semantic roles, rather than on active description of novel events&lt;br /&gt;
### agency is less linguistically salient, so predicates assigning blame, initiative, or creativity are avoided&lt;br /&gt;
### Tidally Locked Planet&lt;br /&gt;
#### The sun never moves in the sky.&lt;br /&gt;
#### The world is divided into zones of permanent day, eternal night, and a narrow habitable twilight ring.&lt;br /&gt;
#### People live in a stable band where temperature and light are forever the same.&lt;br /&gt;
### Mountain life&lt;br /&gt;
#### Isolated communities → heavy internal consistency, less external pressure to simplify&lt;br /&gt;
#### Thin air → favoring sharp, closed articulation: ejectives, glottalization, voiceless stops&lt;br /&gt;
#### Cultural inwardness → deep philosophies of stasis and permanence&lt;br /&gt;
### Time is measured in generations, epochs, weathering of stone, growth cycles of ultra-slow plants&lt;br /&gt;
&lt;br /&gt;
{{See also|Ɬiʔa/Conworlding}}&lt;br /&gt;
&lt;br /&gt;
== Morphology ==&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Case !! Function !! Gloss !! Ending&lt;br /&gt;
|+ Existential cases&lt;br /&gt;
|-&lt;br /&gt;
! Topical&lt;br /&gt;
| Frames the referent of the utterance ||	“As for…”&lt;br /&gt;
! -Mp&#039;a&lt;br /&gt;
|-&lt;br /&gt;
! Identity&lt;br /&gt;
| Category, essence, nominal predicate ||	“is a…” / “equals…”&lt;br /&gt;
! -&lt;br /&gt;
|-&lt;br /&gt;
! Possessive&lt;br /&gt;
| ownership, authorship, kinship, part-whole || “X’s Y”&lt;br /&gt;
! -rkI&lt;br /&gt;
|-&lt;br /&gt;
! Genitive	&lt;br /&gt;
| association, content, theme, objective, attribution || “Y of X”&lt;br /&gt;
! -ł(Ɛ)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Where/When Cases&lt;br /&gt;
! Case !!	Function !!	Typical gloss !! Ending&lt;br /&gt;
|-&lt;br /&gt;
! Locative&lt;br /&gt;
| Place, state, context of being, time-within ||	“in,” “at,” “on”, &amp;quot;during&amp;quot;&lt;br /&gt;
! -f&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Dative&lt;br /&gt;
| Target, direction ||	“to,” “for,” “until&amp;quot;, &amp;quot;as far as&amp;quot;&lt;br /&gt;
! -Mk&#039;O&lt;br /&gt;
|-&lt;br /&gt;
! Ablative&lt;br /&gt;
| Source, cause, origin || “from,” “because of,” “due to”&lt;br /&gt;
! -bdI&lt;br /&gt;
|-&lt;br /&gt;
! Benefactive&lt;br /&gt;
| Advantage, interest, concern || “for the benefit of…”, &amp;quot;at the behest of&amp;quot;&lt;br /&gt;
! -aI&lt;br /&gt;
|-&lt;br /&gt;
! Abessive&lt;br /&gt;
| Absence, privation, “lacking”	|| “without,” “lacking,” “free from”, &amp;quot;exclude&amp;quot;&lt;br /&gt;
! -st&#039;Ɛ&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ How Cases&lt;br /&gt;
! Case !! Function 	!! Typical gloss !! Ending&lt;br /&gt;
|-&lt;br /&gt;
! Instrumental &lt;br /&gt;
| Means, medium, material || “by (means of)”, “through,” “with”, &amp;quot;using&amp;quot;&lt;br /&gt;
! -fla&lt;br /&gt;
|-&lt;br /&gt;
! Adverbial&lt;br /&gt;
| Role/state modifier, part of speech shift	|| “as (a) X,” “in a X way”, &amp;quot;like&amp;quot;&lt;br /&gt;
! -Oad&lt;br /&gt;
|-&lt;br /&gt;
! Translative&lt;br /&gt;
| Change of state, transform/manifestation ||	“becoming,” “into,” “turning into”&lt;br /&gt;
! -k&#039;(I)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Noun Classes&lt;br /&gt;
! !! Not &amp;quot;Container&amp;quot; (mass: ?, ??) !! &amp;quot;Container&amp;quot; (count: ?, ??)&lt;br /&gt;
|-&lt;br /&gt;
! Idea + Matter	&lt;br /&gt;
| Animals (also temperaments) || 	Persons / Gods&lt;br /&gt;
|-&lt;br /&gt;
! Matter only	&lt;br /&gt;
| (Diffuse) Substances: air, fire || 	Tools , &amp;quot;rocks&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
! Idea only	&lt;br /&gt;
| Actions	|| Abstracts, Categories, Sets&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Number: Containers are unmarked for number, as in Chinese/Japanese/Korean.  Non-containers default to a collective/mass-noun number, but can take a partitive (which can mean as few as one).&lt;br /&gt;
&lt;br /&gt;
Polypersonal pronouns:&lt;br /&gt;
&lt;br /&gt;
== Phonology/Orthography ==&lt;br /&gt;
{| class=&amp;quot;bluetable&amp;quot; style=&amp;quot;text-align:center; float:left&amp;quot;&lt;br /&gt;
! !!	Labial !!	Labiolingual !!	Alveolar !!	Palatal !! Velar !!	Glottal&lt;br /&gt;
|-&lt;br /&gt;
! Nasal	&lt;br /&gt;
| /m/	&#039;&#039;&#039;m&#039;&#039;&#039; || /n̼/ &#039;&#039;&#039;n&#039;&#039;&#039; || /n/ &#039;&#039;&#039;n&#039;&#039;&#039; || /ŋ/ &#039;&#039;&#039;ŋ&#039;&#039;&#039;			||&lt;br /&gt;
|-&lt;br /&gt;
! Click&lt;br /&gt;
| (/ᵐʘ/ &#039;&#039;&#039;mx&#039;&#039;&#039;) || || (/ŋǃ/ &#039;&#039;&#039;nc&#039;&#039;&#039;) || ||&lt;br /&gt;
|-&lt;br /&gt;
! Voiced Stop&lt;br /&gt;
| &#039;&#039;&#039;b&#039;&#039;&#039; || 	||	&#039;&#039;&#039;d&#039;&#039;&#039; ||	&#039;&#039;&#039;g&#039;&#039;&#039;	||&lt;br /&gt;
|-&lt;br /&gt;
! Eject. Stop&lt;br /&gt;
| /pʼ/ &#039;&#039;&#039;pq&#039;&#039;&#039; ||	|| /t’/ &#039;&#039;&#039;tq&#039;&#039;&#039;	|| /k’/ &#039;&#039;&#039;kq&#039;&#039;&#039; ||	/ʔ/ &#039;&#039;&#039; &#039; &#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Unvoiced Stop&lt;br /&gt;
| &#039;&#039;&#039;p&#039;&#039;&#039; ||	||	&#039;&#039;&#039;t&#039;&#039;&#039; || /k~x/ &#039;&#039;&#039;k&#039;&#039;&#039;	||&lt;br /&gt;
|-&lt;br /&gt;
! Plain Fricative&lt;br /&gt;
| /ɸ~β/ &#039;&#039;&#039;f&#039;&#039;&#039; ||	/θ̼~ð̼/ &#039;&#039;&#039;þ&#039;&#039;&#039;	|| /s~z/ &#039;&#039;&#039;s&#039;&#039;&#039; || (/ʒ/ &#039;&#039;&#039;ž&#039;&#039;&#039;) || ||&lt;br /&gt;
|-&lt;br /&gt;
! Eject. Fricative&lt;br /&gt;
| /fʼ/ &#039;&#039;&#039;fq&#039;&#039;&#039; ||	/θ̼ʼ/ &#039;&#039;&#039;þq&#039;&#039;&#039; || /s’~ts’/ &#039;&#039;&#039;sq&#039;&#039;&#039;		|| ||&lt;br /&gt;
|-&lt;br /&gt;
! Approx./Trill	&lt;br /&gt;
| &#039;&#039;&#039;w&#039;&#039;&#039;	|| || &#039;&#039;&#039;r&#039;&#039;&#039; || &#039;&#039;&#039;j&#039;&#039;&#039; ||	/h~ɦ/ &#039;&#039;&#039;h&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Laterals&lt;br /&gt;
| || /l̼/ &#039;&#039;&#039;l&#039;&#039;&#039; ||	/ɬ/ &#039;&#039;&#039;ł&#039;&#039;&#039;		|| ||&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;bluetable&amp;quot; style=&amp;quot;float:right; text-align:center;&amp;quot;&lt;br /&gt;
! !! Front !! Back !! Underspecified&lt;br /&gt;
|-&lt;br /&gt;
! High&lt;br /&gt;
| &#039;&#039;&#039;i&#039;&#039;&#039; || &#039;&#039;&#039;u&#039;&#039;&#039; || I&lt;br /&gt;
|-&lt;br /&gt;
! High-Mid&lt;br /&gt;
| &#039;&#039;&#039;e&#039;&#039;&#039; || &#039;&#039;&#039;o&#039;&#039;&#039; || O&lt;br /&gt;
|-&lt;br /&gt;
! Low-Mid&lt;br /&gt;
| /ɛ/ &#039;&#039;&#039;ë&#039;&#039;&#039; || /ɔ/ &#039;&#039;&#039;ö&#039;&#039;&#039; || Ö&lt;br /&gt;
|-&lt;br /&gt;
! Low&lt;br /&gt;
| colspan=&amp;quot;2&amp;quot; | /ä/ &#039;&#039;&#039;a&#039;&#039;&#039;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Allophony:&lt;br /&gt;
* nasal + labial ejective -&amp;gt; [m͡ʘ]&lt;br /&gt;
* nasal + non-labial ejective -&amp;gt; [ŋ͡ǃ]&lt;br /&gt;
&lt;br /&gt;
Phonotactics are (C)(G)V(C&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;):&lt;br /&gt;
* any consonant or none can a syllable&lt;br /&gt;
* Glides (/j/ or /w/) after anything&lt;br /&gt;
* hiatus allowed, diphthongs not&lt;br /&gt;
* any coda, except glides&lt;br /&gt;
&lt;br /&gt;
=== Sentences ===&lt;br /&gt;
# The storm scared people&lt;br /&gt;
#* k’ɛthu-Mp’a ʔusɛk närgo-f’&lt;br /&gt;
#* kqëthumxa ’usëk närgofq&lt;br /&gt;
#* As for the storm, (there is) fear in people.&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a&amp;diff=168005</id>
		<title>Ɬiʔa</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a&amp;diff=168005"/>
		<updated>2025-03-26T04:07:48Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: /* Star */ solar system&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Goals ==&lt;br /&gt;
# Endgoal - A truly verbless language I can use&lt;br /&gt;
# Vague phrases&lt;br /&gt;
## Glacial pace&lt;br /&gt;
## Navajo-of-nouns&lt;br /&gt;
## lazy but clever&lt;br /&gt;
## carved in stone&lt;br /&gt;
## complicated rituals&lt;br /&gt;
# Naturalism - 6/10&lt;br /&gt;
#* I want some naturalistic elements&lt;br /&gt;
#* Different setting (parallel Earth)&lt;br /&gt;
#* Different nature (immortal humans)&lt;br /&gt;
#* Irregularities but not many&lt;br /&gt;
#* Idioms within reason&lt;br /&gt;
# Complexity - insane.  Navajo but with only nouns&lt;br /&gt;
# Derivation - clear.  Agglutinative, basically&lt;br /&gt;
# Features&lt;br /&gt;
## Phonology &lt;br /&gt;
### Vowel harmony&lt;br /&gt;
### A couple of clicks, and ejectives (un-earth-like)&lt;br /&gt;
### CV, and CVC &lt;br /&gt;
## Grammar&lt;br /&gt;
### No verbs at all&lt;br /&gt;
### assumed copular between topic and subject&lt;br /&gt;
### 6 nouns classes (genders), like animacy &lt;br /&gt;
### Many cases (12?)&lt;br /&gt;
### Case-stacking&lt;br /&gt;
### word glue, like German&lt;br /&gt;
### mostly agglutinative, touch of fusional&lt;br /&gt;
## Culture&lt;br /&gt;
### things happen, not because someone does them, but because the world unfolds in prescribed patterns&lt;br /&gt;
### discourse is formulaic, ceremonial, or sacred: more on set relational expressions and fixed semantic roles, rather than on active description of novel events&lt;br /&gt;
### agency is less linguistically salient, so predicates assigning blame, initiative, or creativity are avoided&lt;br /&gt;
### Tidally Locked Planet&lt;br /&gt;
#### The sun never moves in the sky.&lt;br /&gt;
#### The world is divided into zones of permanent day, eternal night, and a narrow habitable twilight ring.&lt;br /&gt;
#### People live in a stable band where temperature and light are forever the same.&lt;br /&gt;
### Mountain life&lt;br /&gt;
#### Isolated communities → heavy internal consistency, less external pressure to simplify&lt;br /&gt;
#### Thin air → favoring sharp, closed articulation: ejectives, glottalization, voiceless stops&lt;br /&gt;
#### Cultural inwardness → deep philosophies of stasis and permanence&lt;br /&gt;
### Time is measured in generations, epochs, weathering of stone, growth cycles of ultra-slow plants&lt;br /&gt;
&lt;br /&gt;
== Conworlding ==&lt;br /&gt;
=== Star ===&lt;br /&gt;
Our star is a red-dwarf.&lt;br /&gt;
# Type: M5V&lt;br /&gt;
## M: This indicates it&#039;s a cool, red star with a surface temperature less than 3,500ºK&lt;br /&gt;
## 5: Within the M class, stars are further divided into subclasses 0-9, with 0 being the hottest and 9 the coolest. An M5 star is in the middle of this range.&lt;br /&gt;
## V: Denotes that it&#039;s a main sequence star, also known as a dwarf star&lt;br /&gt;
# Stellar luminosity (L*) ≈ 0.01 𝐿⊙&lt;br /&gt;
# Stellar mass (M*) ≈ 0.2 𝑀⊙&lt;br /&gt;
# Stellar radius (R*) ≈ 0.25 𝑅⊙&lt;br /&gt;
# Effective temperature (T*) ≈ 3000 K&lt;br /&gt;
​The habitable zone (a) is about square root of L* over L⊙, so ~0.1 AU.&lt;br /&gt;
&lt;br /&gt;
==== Solar System ====&lt;br /&gt;
There are seven planets in the system&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Planet !!	Mass (M🜨)!!	Radius (R🜨)!!	Period (d)	!!Resonance !!	Semi-Major Axis (AU)!!	Rings !! Moons !! Period !! Size&lt;br /&gt;
|-&lt;br /&gt;
| b ||	1.2 ||	1.1 ||	11.3 ||	2:3 with c	|| 0.074 ||	No || No || 6 || 13.6&#039;&lt;br /&gt;
|-&lt;br /&gt;
| c ||	1.5	 ||1.225 ||	17.0 ||	—	        ||0.100 || No || No || 26 || -&lt;br /&gt;
|-&lt;br /&gt;
| d ||	2.0	 ||1.4 ||	25.5 ||	2:3 with c	 ||0.13 ||	No || No || 38 || 13.1&#039;&lt;br /&gt;
|-&lt;br /&gt;
| e ||	0.9 ||	1.0 ||	34.0 ||	3:4 with d	 ||0.17 ||	No || No || 57 || 4.1&#039;&lt;br /&gt;
|-&lt;br /&gt;
| f ||	3.5 ||	2.0 ||	45.3 ||	3:4 with e	 ||0.225 || Yes || Junk || 87 || 4.7&#039;&lt;br /&gt;
|-&lt;br /&gt;
| g ||	1.0 ||	1.1 ||	70.0 ||	2:3 with f	 ||0.40 ||	Yes || Junk || 206 || 1.1&#039;&lt;br /&gt;
|-&lt;br /&gt;
| h ||	5.0 ||	2.3 ||	210.0 ||1:3 with g	 ||1.5 ||	OMG || OMG || 1500 || 0.5&#039;&lt;br /&gt;
|}&lt;br /&gt;
; b : b is a Mercury, tidally locked and very hard ~500ºK.  Rocky&lt;br /&gt;
&lt;br /&gt;
=== Planet ===&lt;br /&gt;
Orbital period squared = 4 pi-squared times a-cubed over (G times M*).  For us that is 10.3 days.  Assuming tidal locking (as is common for planets at this distance), the rotation period is the same.  If it were an Earth-like planet, we could calculate the global average, using the effective temperature approximation.&lt;br /&gt;
* For our planet, assuming an albedo of 0.3 (Earth&#039;s), we get 223ºK&lt;br /&gt;
* Assuming an albedo of 0.2, we get 263&lt;br /&gt;
* For an albedo of 0.1, we get 271&lt;br /&gt;
With a modest greenhouse effect, surface temperatures could rise.&lt;br /&gt;
# Mass: 1.5M⊕&lt;br /&gt;
# Gravity: 1g⊕&lt;br /&gt;
# Radius = 1.225⊕, or 7805km&lt;br /&gt;
The area of the terminator is hard to predict&lt;br /&gt;
# +/-10º Guess: 4.253 E 13 m^2, 4.253E7km^2 (much bigger than Africa)&lt;br /&gt;
# +/-30º Guess: 1.28 E8 km^2 (slightly less than the land of the Earth)&lt;br /&gt;
The thicker the atmosphere, the thicker the band.&lt;br /&gt;
# Escape velocity is 12.4km/s, 11% higher than Earth&lt;br /&gt;
# Orbital velocity is 8.79km/s&lt;br /&gt;
==== Atmosphere ====&lt;br /&gt;
Water content is low becaue&lt;br /&gt;
* Water vapor is a potent greenhouse gas; vast surface water can trap too much heat, especially near the substellar point.&lt;br /&gt;
* Water leads to climate homogenization&lt;br /&gt;
* Lack of exposed silicate rock: Necessary for carbon-silicate weathering feedback, which stabilizes climate on geological timescales.&lt;br /&gt;
Earth has ~1.4 billion km³ of water.  In our habitable zone, we have no more than 10% of that, or 100 million km³.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Factor !! Ɬiʔa atm !! Ɬiʔa % !! Earth atm !! Earth % !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! Total Pressure &lt;br /&gt;
| 1.6 atm || || 1.0 atm || || Enhanced convective heat transfer, increased IR trapping&lt;br /&gt;
|-&lt;br /&gt;
! Nitrogen (N₂) &lt;br /&gt;
| 1.00 || 62.50% || 0.7808 || 78.08% || Reduced; still inert, still dominant&lt;br /&gt;
|-&lt;br /&gt;
! Oxygen (O₂) &lt;br /&gt;
| 0.21 || 13.13% || 0.2095 || 20.95% || Earth-normal partial pressure &lt;br /&gt;
|-&lt;br /&gt;
! Argon (Ar)&lt;br /&gt;
| 0.40 || 25.00% || 0.0093 || 0.93% || Major heat distribution enhancement, inert&lt;br /&gt;
|-&lt;br /&gt;
! Krypton + Xenon&lt;br /&gt;
| 0.005 || 0.31% || trace || trace || High molecular mass → improved heat retention, still safe&lt;br /&gt;
|-&lt;br /&gt;
! CO₂&lt;br /&gt;
| 0.005 || 0.31% || 0.004 || 0.04% || slighly elevated; sub-greenhouse threshold&lt;br /&gt;
|-&lt;br /&gt;
! H₂O vapor &lt;br /&gt;
| 0.015 || ~1% || || 0-4% || Maintains greenhouse without excess moisture&lt;br /&gt;
|}&lt;br /&gt;
===== Atmospheric Effects on Clouds =====&lt;br /&gt;
# Increased Pressure (1.6 atm) compresses gases, raising the dew point at which water vapor condenses. Cloudsform closer to the surface, and are denser than similar altitudes compared to Earth.&lt;br /&gt;
# Low Water Inventory (10% of Earth&#039;s): There will be less frequent and less massive cloud systems than on Earth, but still present—especially over &amp;quot;hotspots&amp;quot; on the day side.&lt;br /&gt;
# Tidally Locked Climate: Cloud formation concentrate along the substellar point, where warm, moist air rises and cools.&lt;br /&gt;
#* A permanent “eyewall” storm system has formed at the subsolar point, like a giant hurricane.&lt;br /&gt;
#* As air rises and is advected to the night side, thin cloud bands or ice hazes form as it descends and cools.&lt;br /&gt;
&lt;br /&gt;
Appearance:&lt;br /&gt;
* The presence of noble gases (Ar, Kr, Xe) and higher pressure enhance Mie scattering, making clouds appear whiter and more silvered, especially at sunrise/sunset boundaries.&lt;br /&gt;
* Night side clouds are thin, high-altitude icy sheets, glowing faintly in aurorae or thermal emissions.&lt;br /&gt;
&lt;br /&gt;
===== Sky Color =====&lt;br /&gt;
The color of the sky is shaped by Rayleigh scattering, which depends on:&lt;br /&gt;
# Molecular composition: Heavier gases like Ar, Kr, and Xe scatter light less efficiently than N₂.&lt;br /&gt;
# Spectral output of the star: the red dwarf emits predominantly infrared and red light, with very little blue or violet.&lt;br /&gt;
&lt;br /&gt;
Consequence:&lt;br /&gt;
* Even with atmospheric scattering, there is insufficient blue light in the stellar spectrum to produce a blue sky.&lt;br /&gt;
* Day sky would likely appear:&lt;br /&gt;
** Dark peach, dusky rose, or reddish beige near zenith,&lt;br /&gt;
** Grading to deep salmon or mauve near the horizon,&lt;br /&gt;
** A slight metallic sheen due to noble gas content and high pressure.&lt;br /&gt;
&lt;br /&gt;
Twilight &amp;amp; Limb Scattering:&lt;br /&gt;
* The terminator (twilight zone) sees a diffuse, ruddy light, scattering through haze and clouds into luminous reds, purples, and copper tones.&lt;br /&gt;
* Aurorae are spectacular on the night side, especially since stellar flares are frequent.&lt;br /&gt;
&lt;br /&gt;
===== Sound Propagation =====&lt;br /&gt;
: &#039;&#039;Sound is profoundly affected by atmospheric pressure and composition.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Compared to Earth:&lt;br /&gt;
* Higher pressure → greater air density → faster transmission of sound and less attenuation.&lt;br /&gt;
* Argon and Xenon are heavy gases, which:&lt;br /&gt;
** Lower the speed of sound relative to air at the same pressure (despite the pressure increase).&lt;br /&gt;
** Shift resonance frequencies downward, resulting in deeper, rounder sounds.&lt;br /&gt;
&lt;br /&gt;
Consequences:&lt;br /&gt;
* Voices sound subtly lower-pitched and richer, especially for consonants and low vowels.&lt;br /&gt;
* Ambient sounds (wind, water, animals) would carry farther and sound more muffled or sonorous.&lt;br /&gt;
* Music or speech would resonate more warmly, especially indoors or in enclosed spaces.&lt;br /&gt;
&lt;br /&gt;
In short: it sounds like it’s wrapped in velvet.&lt;br /&gt;
&lt;br /&gt;
===== Heat Transport to the Night Side =====&lt;br /&gt;
Mechanisms:&lt;br /&gt;
# Thick Atmosphere (1.6 atm) increases:&lt;br /&gt;
#* Advection efficiency: Warm air masses can move more heat horizontally.&lt;br /&gt;
#* Radiative time constant: The atmosphere holds heat longer before releasing it.&lt;br /&gt;
# Noble Gases (especially Kr/Xe):&lt;br /&gt;
#* High molecular mass → more IR opacity → trapping and radiating heat more evenly.&lt;br /&gt;
# Slow Rotation / Tidal Locking:&lt;br /&gt;
#* Global Hadley-like cells may dominate circulation, carrying warm air from the day side to the night side and descending it there.&lt;br /&gt;
&lt;br /&gt;
Result:&lt;br /&gt;
* The night side is not freezing.  Temperatures differ by tens of degrees, not hundreds.&lt;br /&gt;
* There are still ice caps and a cold deserts at the anti-stellar point, but not a glaciated wasteland.&lt;br /&gt;
&lt;br /&gt;
==== Magnetosphere ====&lt;br /&gt;
* Larger mass --&amp;gt; larger iron core, generating more internal heat&lt;br /&gt;
* Larger radius --&amp;gt; Vigorous convection in the core&lt;br /&gt;
* Tidal Flexing --&amp;gt; still drives magnetic activity&lt;br /&gt;
&lt;br /&gt;
# Aurorae at lower latitudes&lt;br /&gt;
## higher magnetic rigidity, wider magnetotail, and greater reconnection energy.&lt;br /&gt;
## Combined with a higher flux of stellar particles, this means:&lt;br /&gt;
### Auroral ovals expand, reaching mid-latitudes sometimes equator.&lt;br /&gt;
### The skies are alive with rippling green, violet, and crimson aurorae, especially on the night side.&lt;br /&gt;
### Daily auroral activity occur during stellar flare cycles.&lt;br /&gt;
# Compasses&lt;br /&gt;
## compasses respond more sharply, with:&lt;br /&gt;
### Faster alignment.&lt;br /&gt;
### Greater resistance to local perturbations.&lt;br /&gt;
## However, frequent magnetic storms from stellar activity cause sudden declinations, reversals, or local anomalies.  In short, lots of aurorae equals dead compasses at the same time.&lt;br /&gt;
# Magnetic Field Strength &amp;gt; 100 μT &lt;br /&gt;
# Electromagnetism is more basic than chemistry or almost any other natural philosophy&lt;br /&gt;
&lt;br /&gt;
==== Substellar Point ====&lt;br /&gt;
The maximum incoming flux is very nearly the same as Earth&#039;s solar constant (≈1361 W/m²), but concentrated over one point rather than averaged over a rotating sphere.  Temperatures should be above 500ºK most of the time.  &lt;br /&gt;
&lt;br /&gt;
The magnetic north is also here, The thick atmosphere prevents too much loss here, but &lt;br /&gt;
* Charged particle influx&lt;br /&gt;
** Maximized at the substellar point—intense auroral and energetic particle precipitation&lt;br /&gt;
* Atmospheric ionization&lt;br /&gt;
** Constant production of high-energy ions and NOx compounds—possible UV fluorescence in upper sky&lt;br /&gt;
* Localized heating&lt;br /&gt;
** Augments already extreme temperatures—600–700 K surface possible&lt;br /&gt;
&lt;br /&gt;
=== Artificially Tethered Moon ===&lt;br /&gt;
* 670,000 km up&lt;br /&gt;
* 7805 km in radius = same as the planet&lt;br /&gt;
* 1.33º of the sky, same as the sun&lt;br /&gt;
&lt;br /&gt;
A network of tethers/tension lines from the moon to multiple anchor points on the planet’s surface (a tripod or hexapod structure), woven like hair&lt;br /&gt;
* Uses active tension management and orbital station-keeping to stabilize the moon&lt;br /&gt;
* Counterweights and inward-pointing mass drivers on the moon to oppose drift&lt;br /&gt;
&lt;br /&gt;
The tethers are not bearing the full weight, but merely damping drift, providing restoring force, and enabling long-term stability through active compensation.  The moon&lt;br /&gt;
* Blocks the worst of the heat&lt;br /&gt;
* Blocks the worst of the solar radiation&lt;br /&gt;
The moon has &lt;br /&gt;
* low mass&lt;br /&gt;
* high albedo - enormous reflectivity&lt;br /&gt;
* scatters charges particles, UV, X-rays, auroral flux tubes&lt;br /&gt;
* sunward - crazy hot, high emissivity&lt;br /&gt;
* earthward - crazy cool, low emissivity&lt;br /&gt;
== Morphology ==&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Case !! Function !! Gloss !! Ending&lt;br /&gt;
|+ Existential cases&lt;br /&gt;
|-&lt;br /&gt;
! Topical&lt;br /&gt;
| Frames the referent of the utterance ||	“As for…”&lt;br /&gt;
! -Mp&#039;a&lt;br /&gt;
|-&lt;br /&gt;
! Identity&lt;br /&gt;
| Category, essence, nominal predicate ||	“is a…” / “equals…”&lt;br /&gt;
! -&lt;br /&gt;
|-&lt;br /&gt;
! Possessive&lt;br /&gt;
| ownership, authorship, kinship, part-whole || “X’s Y”&lt;br /&gt;
! -rkI&lt;br /&gt;
|-&lt;br /&gt;
! Genitive	&lt;br /&gt;
| association, content, theme, objective, attribution || “Y of X”&lt;br /&gt;
! -ł(Ɛ)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Where/When Cases&lt;br /&gt;
! Case !!	Function !!	Typical gloss !! Ending&lt;br /&gt;
|-&lt;br /&gt;
! Locative&lt;br /&gt;
| Place, state, context of being, time-within ||	“in,” “at,” “on”, &amp;quot;during&amp;quot;&lt;br /&gt;
! -f&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Dative&lt;br /&gt;
| Target, direction ||	“to,” “for,” “until&amp;quot;, &amp;quot;as far as&amp;quot;&lt;br /&gt;
! -Mk&#039;O&lt;br /&gt;
|-&lt;br /&gt;
! Ablative&lt;br /&gt;
| Source, cause, origin || “from,” “because of,” “due to”&lt;br /&gt;
! -bdI&lt;br /&gt;
|-&lt;br /&gt;
! Benefactive&lt;br /&gt;
| Advantage, interest, concern || “for the benefit of…”, &amp;quot;at the behest of&amp;quot;&lt;br /&gt;
! -aI&lt;br /&gt;
|-&lt;br /&gt;
! Abessive&lt;br /&gt;
| Absence, privation, “lacking”	|| “without,” “lacking,” “free from”, &amp;quot;exclude&amp;quot;&lt;br /&gt;
! -st&#039;Ɛ&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ How Cases&lt;br /&gt;
! Case !! Function 	!! Typical gloss !! Ending&lt;br /&gt;
|-&lt;br /&gt;
! Instrumental &lt;br /&gt;
| Means, medium, material || “by (means of)”, “through,” “with”, &amp;quot;using&amp;quot;&lt;br /&gt;
! -fla&lt;br /&gt;
|-&lt;br /&gt;
! Adverbial&lt;br /&gt;
| Role/state modifier, part of speech shift	|| “as (a) X,” “in a X way”, &amp;quot;like&amp;quot;&lt;br /&gt;
! -Oad&lt;br /&gt;
|-&lt;br /&gt;
! Translative&lt;br /&gt;
| Change of state, transform/manifestation ||	“becoming,” “into,” “turning into”&lt;br /&gt;
! -k&#039;(I)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Noun Classes&lt;br /&gt;
! !! Not &amp;quot;Container&amp;quot; (mass: ?, ??) !! &amp;quot;Container&amp;quot; (count: ?, ??)&lt;br /&gt;
|-&lt;br /&gt;
! Idea + Matter	&lt;br /&gt;
| Animals (also temperaments) || 	Persons / Gods&lt;br /&gt;
|-&lt;br /&gt;
! Matter only	&lt;br /&gt;
| (Diffuse) Substances: air, fire || 	Tools , &amp;quot;rocks&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
! Idea only	&lt;br /&gt;
| Actions	|| Abstracts, Categories, Sets&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Number: Containers are unmarked for number, as in Chinese/Japanese/Korean.  Non-containers default to a collective/mass-noun number, but can take a partitive (which can mean as few as one).&lt;br /&gt;
&lt;br /&gt;
Polypersonal pronouns:&lt;br /&gt;
&lt;br /&gt;
== Phonology/Orthography ==&lt;br /&gt;
{| class=&amp;quot;bluetable&amp;quot; style=&amp;quot;text-align:center; float:left&amp;quot;&lt;br /&gt;
! !!	Labial !!	Labiolingual !!	Alveolar !!	Palatal !! Velar !!	Glottal&lt;br /&gt;
|-&lt;br /&gt;
! Nasal	&lt;br /&gt;
| /m/	&#039;&#039;&#039;m&#039;&#039;&#039; || /n̼/ &#039;&#039;&#039;n&#039;&#039;&#039; || /n/ &#039;&#039;&#039;n&#039;&#039;&#039; || /ŋ/ &#039;&#039;&#039;ŋ&#039;&#039;&#039;			||&lt;br /&gt;
|-&lt;br /&gt;
! Click&lt;br /&gt;
| (/ᵐʘ/ &#039;&#039;&#039;mx&#039;&#039;&#039;) || || (/ŋǃ/ &#039;&#039;&#039;nc&#039;&#039;&#039;) || ||&lt;br /&gt;
|-&lt;br /&gt;
! Voiced Stop&lt;br /&gt;
| &#039;&#039;&#039;b&#039;&#039;&#039; || 	||	&#039;&#039;&#039;d&#039;&#039;&#039; ||	&#039;&#039;&#039;g&#039;&#039;&#039;	||&lt;br /&gt;
|-&lt;br /&gt;
! Eject. Stop&lt;br /&gt;
| /pʼ/ &#039;&#039;&#039;pq&#039;&#039;&#039; ||	|| /t’/ &#039;&#039;&#039;tq&#039;&#039;&#039;	|| /k’/ &#039;&#039;&#039;kq&#039;&#039;&#039; ||	/ʔ/ &#039;&#039;&#039; &#039; &#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Unvoiced Stop&lt;br /&gt;
| &#039;&#039;&#039;p&#039;&#039;&#039; ||	||	&#039;&#039;&#039;t&#039;&#039;&#039; || /k~x/ &#039;&#039;&#039;k&#039;&#039;&#039;	||&lt;br /&gt;
|-&lt;br /&gt;
! Plain Fricative&lt;br /&gt;
| /ɸ~β/ &#039;&#039;&#039;f&#039;&#039;&#039; ||	/θ̼~ð̼/ &#039;&#039;&#039;þ&#039;&#039;&#039;	|| /s~z/ &#039;&#039;&#039;s&#039;&#039;&#039; || (/ʒ/ &#039;&#039;&#039;ž&#039;&#039;&#039;) || ||&lt;br /&gt;
|-&lt;br /&gt;
! Eject. Fricative&lt;br /&gt;
| /fʼ/ &#039;&#039;&#039;fq&#039;&#039;&#039; ||	/θ̼ʼ/ &#039;&#039;&#039;þq&#039;&#039;&#039; || /s’~ts’/ &#039;&#039;&#039;sq&#039;&#039;&#039;		|| ||&lt;br /&gt;
|-&lt;br /&gt;
! Approx./Trill	&lt;br /&gt;
| &#039;&#039;&#039;w&#039;&#039;&#039;	|| || &#039;&#039;&#039;r&#039;&#039;&#039; || &#039;&#039;&#039;j&#039;&#039;&#039; ||	/h~ɦ/ &#039;&#039;&#039;h&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Laterals&lt;br /&gt;
| || /l̼/ &#039;&#039;&#039;l&#039;&#039;&#039; ||	/ɬ/ &#039;&#039;&#039;ł&#039;&#039;&#039;		|| ||&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;bluetable&amp;quot; style=&amp;quot;float:right; text-align:center;&amp;quot;&lt;br /&gt;
! !! Front !! Back !! Underspecified&lt;br /&gt;
|-&lt;br /&gt;
! High&lt;br /&gt;
| &#039;&#039;&#039;i&#039;&#039;&#039; || &#039;&#039;&#039;u&#039;&#039;&#039; || I&lt;br /&gt;
|-&lt;br /&gt;
! High-Mid&lt;br /&gt;
| &#039;&#039;&#039;e&#039;&#039;&#039; || &#039;&#039;&#039;o&#039;&#039;&#039; || O&lt;br /&gt;
|-&lt;br /&gt;
! Low-Mid&lt;br /&gt;
| /ɛ/ &#039;&#039;&#039;ë&#039;&#039;&#039; || /ɔ/ &#039;&#039;&#039;ö&#039;&#039;&#039; || Ö&lt;br /&gt;
|-&lt;br /&gt;
! Low&lt;br /&gt;
| colspan=&amp;quot;2&amp;quot; | /ä/ &#039;&#039;&#039;a&#039;&#039;&#039;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Allophony:&lt;br /&gt;
* nasal + labial ejective -&amp;gt; [m͡ʘ]&lt;br /&gt;
* nasal + non-labial ejective -&amp;gt; [ŋ͡ǃ]&lt;br /&gt;
&lt;br /&gt;
Phonotactics are (C)(G)V(C&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;):&lt;br /&gt;
* any consonant or none can a syllable&lt;br /&gt;
* Glides (/j/ or /w/) after anything&lt;br /&gt;
* hiatus allowed, diphthongs not&lt;br /&gt;
* any coda, except glides&lt;br /&gt;
&lt;br /&gt;
=== Sentences ===&lt;br /&gt;
# The storm scared people&lt;br /&gt;
#* k’ɛthu-Mp’a ʔusɛk närgo-f’&lt;br /&gt;
#* kqëthumxa ’usëk närgofq&lt;br /&gt;
#* As for the storm, (there is) fear in people.&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a&amp;diff=167914</id>
		<title>Ɬiʔa</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=%EA%9E%ADi%CA%94a&amp;diff=167914"/>
		<updated>2025-03-25T03:44:07Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: conworlding&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Goals ==&lt;br /&gt;
# Endgoal - A truly verbless language I can use&lt;br /&gt;
# Vague phrases&lt;br /&gt;
## Glacial pace&lt;br /&gt;
## Navajo-of-nouns&lt;br /&gt;
## lazy but clever&lt;br /&gt;
## carved in stone&lt;br /&gt;
## complicated rituals&lt;br /&gt;
# Naturalism - 6/10&lt;br /&gt;
#* I want some naturalistic elements&lt;br /&gt;
#* Different setting (parallel Earth)&lt;br /&gt;
#* Different nature (immortal humans)&lt;br /&gt;
#* Irregularities but not many&lt;br /&gt;
#* Idioms within reason&lt;br /&gt;
# Complexity - insane.  Navajo but with only nouns&lt;br /&gt;
# Derivation - clear.  Agglutinative, basically&lt;br /&gt;
# Features&lt;br /&gt;
## Phonology &lt;br /&gt;
### Vowel harmony&lt;br /&gt;
### A couple of clicks, and ejectives (un-earth-like)&lt;br /&gt;
### CV, and CVC &lt;br /&gt;
## Grammar&lt;br /&gt;
### No verbs at all&lt;br /&gt;
### assumed copular between topic and subject&lt;br /&gt;
### 6 nouns classes (genders), like animacy &lt;br /&gt;
### Many cases (12?)&lt;br /&gt;
### Case-stacking&lt;br /&gt;
### word glue, like German&lt;br /&gt;
### mostly agglutinative, touch of fusional&lt;br /&gt;
## Culture&lt;br /&gt;
### things happen, not because someone does them, but because the world unfolds in prescribed patterns&lt;br /&gt;
### discourse is formulaic, ceremonial, or sacred: more on set relational expressions and fixed semantic roles, rather than on active description of novel events&lt;br /&gt;
### agency is less linguistically salient, so predicates assigning blame, initiative, or creativity are avoided&lt;br /&gt;
### Tidally Locked Planet&lt;br /&gt;
#### The sun never moves in the sky.&lt;br /&gt;
#### The world is divided into zones of permanent day, eternal night, and a narrow habitable twilight ring.&lt;br /&gt;
#### People live in a stable band where temperature and light are forever the same.&lt;br /&gt;
### Mountain life&lt;br /&gt;
#### Isolated communities → heavy internal consistency, less external pressure to simplify&lt;br /&gt;
#### Thin air → favoring sharp, closed articulation: ejectives, glottalization, voiceless stops&lt;br /&gt;
#### Cultural inwardness → deep philosophies of stasis and permanence&lt;br /&gt;
### Time is measured in generations, epochs, weathering of stone, growth cycles of ultra-slow plants&lt;br /&gt;
&lt;br /&gt;
== Conworlding ==&lt;br /&gt;
=== Star ===&lt;br /&gt;
Our star is a red-dwarf.&lt;br /&gt;
# Type: M5V&lt;br /&gt;
## M: This indicates it&#039;s a cool, red star with a surface temperature less than 3,500ºK&lt;br /&gt;
## 5: Within the M class, stars are further divided into subclasses 0-9, with 0 being the hottest and 9 the coolest. An M5 star is in the middle of this range.&lt;br /&gt;
## V: Denotes that it&#039;s a main sequence star, also known as a dwarf star&lt;br /&gt;
# Stellar luminosity (L*) ≈ 0.01 𝐿⊙&lt;br /&gt;
# Stellar mass (M*) ≈ 0.2 𝑀⊙&lt;br /&gt;
# Stellar radius (R*) ≈ 0.25 𝑅⊙&lt;br /&gt;
# Effective temperature (T*) ≈ 3000 K&lt;br /&gt;
​The habitable zone (a) is about square root of L* over L⊙, so ~0.1 AU.&lt;br /&gt;
&lt;br /&gt;
=== Planet ===&lt;br /&gt;
Orbital period squared = 4 pi-squared times a-cubed over (G times M*).  For us that is 10.3 days.  Assuming tidal locking (as is common for planets at this distance), the rotation period is the same.  If it were an Earth-like planet, we could calculate the global average, using the effective temperature approximation.&lt;br /&gt;
* For our planet, assuming an albedo of 0.3 (Earth&#039;s), we get 223ºK&lt;br /&gt;
* Assuming an albedo of 0.2, we get 263&lt;br /&gt;
* For an albedo of 0.1, we get 271&lt;br /&gt;
With a modest greenhouse effect, surface temperatures could rise.&lt;br /&gt;
# Mass: 1.5M⊕&lt;br /&gt;
# Gravity: 1g⊕&lt;br /&gt;
# Radius = 1.225⊕, or 7805km&lt;br /&gt;
The area of the terminator is hard to predict&lt;br /&gt;
# +/-10º Guess: 4.253 E 13 m^2, 4.253E7km^2 (much bigger than Africa)&lt;br /&gt;
# +/-30º Guess: 1.28 E8 km^2 (slightly less than the land of the Earth)&lt;br /&gt;
The thicker the atmosphere, the thicker the band.&lt;br /&gt;
# Escape velocity is 12.4km/s, 11% higher than Earth&lt;br /&gt;
# Orbital velocity is 8.79km/s&lt;br /&gt;
==== Atmosphere ====&lt;br /&gt;
Water content is low becaue&lt;br /&gt;
* Water vapor is a potent greenhouse gas; vast surface water can trap too much heat, especially near the substellar point.&lt;br /&gt;
* Water leads to climate homogenization&lt;br /&gt;
* Lack of exposed silicate rock: Necessary for carbon-silicate weathering feedback, which stabilizes climate on geological timescales.&lt;br /&gt;
Earth has ~1.4 billion km³ of water.  In our habitable zone, we have no more than 10% of that, or 100 million km³.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Factor !! Ɬiʔa atm !! Ɬiʔa % !! Earth atm !! Earth % !! Notes&lt;br /&gt;
|-&lt;br /&gt;
! Total Pressure &lt;br /&gt;
| 1.6 atm || || 1.0 atm || || Enhanced convective heat transfer, increased IR trapping&lt;br /&gt;
|-&lt;br /&gt;
! Nitrogen (N₂) &lt;br /&gt;
| 1.00 || 62.50% || 0.7808 || 78.08% || Reduced; still inert, still dominant&lt;br /&gt;
|-&lt;br /&gt;
! Oxygen (O₂) &lt;br /&gt;
| 0.21 || 13.13% || 0.2095 || 20.95% || Earth-normal partial pressure &lt;br /&gt;
|-&lt;br /&gt;
! Argon (Ar)&lt;br /&gt;
| 0.40 || 25.00% || 0.0093 || 0.93% || Major heat distribution enhancement, inert&lt;br /&gt;
|-&lt;br /&gt;
! Krypton + Xenon&lt;br /&gt;
| 0.005 || 0.31% || trace || trace || High molecular mass → improved heat retention, still safe&lt;br /&gt;
|-&lt;br /&gt;
! CO₂&lt;br /&gt;
| 0.005 || 0.31% || 0.004 || 0.04% || slighly elevated; sub-greenhouse threshold&lt;br /&gt;
|-&lt;br /&gt;
! H₂O vapor &lt;br /&gt;
| 0.015 || ~1% || || 0-4% || Maintains greenhouse without excess moisture&lt;br /&gt;
|}&lt;br /&gt;
===== Atmospheric Effects on Clouds =====&lt;br /&gt;
# Increased Pressure (1.6 atm) compresses gases, raising the dew point at which water vapor condenses. Cloudsform closer to the surface, and are denser than similar altitudes compared to Earth.&lt;br /&gt;
# Low Water Inventory (10% of Earth&#039;s): There will be less frequent and less massive cloud systems than on Earth, but still present—especially over &amp;quot;hotspots&amp;quot; on the day side.&lt;br /&gt;
# Tidally Locked Climate: Cloud formation concentrate along the substellar point, where warm, moist air rises and cools.&lt;br /&gt;
#* A permanent “eyewall” storm system has formed at the subsolar point, like a giant hurricane.&lt;br /&gt;
#* As air rises and is advected to the night side, thin cloud bands or ice hazes form as it descends and cools.&lt;br /&gt;
&lt;br /&gt;
Appearance:&lt;br /&gt;
* The presence of noble gases (Ar, Kr, Xe) and higher pressure enhance Mie scattering, making clouds appear whiter and more silvered, especially at sunrise/sunset boundaries.&lt;br /&gt;
* Night side clouds are thin, high-altitude icy sheets, glowing faintly in aurorae or thermal emissions.&lt;br /&gt;
&lt;br /&gt;
===== Sky Color =====&lt;br /&gt;
The color of the sky is shaped by Rayleigh scattering, which depends on:&lt;br /&gt;
# Molecular composition: Heavier gases like Ar, Kr, and Xe scatter light less efficiently than N₂.&lt;br /&gt;
# Spectral output of the star: the red dwarf emits predominantly infrared and red light, with very little blue or violet.&lt;br /&gt;
&lt;br /&gt;
Consequence:&lt;br /&gt;
* Even with atmospheric scattering, there is insufficient blue light in the stellar spectrum to produce a blue sky.&lt;br /&gt;
* Day sky would likely appear:&lt;br /&gt;
** Dark peach, dusky rose, or reddish beige near zenith,&lt;br /&gt;
** Grading to deep salmon or mauve near the horizon,&lt;br /&gt;
** A slight metallic sheen due to noble gas content and high pressure.&lt;br /&gt;
&lt;br /&gt;
Twilight &amp;amp; Limb Scattering:&lt;br /&gt;
* The terminator (twilight zone) sees a diffuse, ruddy light, scattering through haze and clouds into luminous reds, purples, and copper tones.&lt;br /&gt;
* Aurorae are spectacular on the night side, especially since stellar flares are frequent.&lt;br /&gt;
&lt;br /&gt;
===== Sound Propagation =====&lt;br /&gt;
: &#039;&#039;Sound is profoundly affected by atmospheric pressure and composition.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Compared to Earth:&lt;br /&gt;
* Higher pressure → greater air density → faster transmission of sound and less attenuation.&lt;br /&gt;
* Argon and Xenon are heavy gases, which:&lt;br /&gt;
** Lower the speed of sound relative to air at the same pressure (despite the pressure increase).&lt;br /&gt;
** Shift resonance frequencies downward, resulting in deeper, rounder sounds.&lt;br /&gt;
&lt;br /&gt;
Consequences:&lt;br /&gt;
* Voices sound subtly lower-pitched and richer, especially for consonants and low vowels.&lt;br /&gt;
* Ambient sounds (wind, water, animals) would carry farther and sound more muffled or sonorous.&lt;br /&gt;
* Music or speech would resonate more warmly, especially indoors or in enclosed spaces.&lt;br /&gt;
&lt;br /&gt;
In short: it sounds like it’s wrapped in velvet.&lt;br /&gt;
&lt;br /&gt;
===== Heat Transport to the Night Side =====&lt;br /&gt;
Mechanisms:&lt;br /&gt;
# Thick Atmosphere (1.6 atm) increases:&lt;br /&gt;
#* Advection efficiency: Warm air masses can move more heat horizontally.&lt;br /&gt;
#* Radiative time constant: The atmosphere holds heat longer before releasing it.&lt;br /&gt;
# Noble Gases (especially Kr/Xe):&lt;br /&gt;
#* High molecular mass → more IR opacity → trapping and radiating heat more evenly.&lt;br /&gt;
# Slow Rotation / Tidal Locking:&lt;br /&gt;
#* Global Hadley-like cells may dominate circulation, carrying warm air from the day side to the night side and descending it there.&lt;br /&gt;
&lt;br /&gt;
Result:&lt;br /&gt;
* The night side is not freezing.  Temperatures differ by tens of degrees, not hundreds.&lt;br /&gt;
* There are still ice caps and a cold deserts at the anti-stellar point, but not a glaciated wasteland.&lt;br /&gt;
&lt;br /&gt;
==== Magnetosphere ====&lt;br /&gt;
* Larger mass --&amp;gt; larger iron core, generating more internal heat&lt;br /&gt;
* Larger radius --&amp;gt; Vigorous convection in the core&lt;br /&gt;
* Tidal Flexing --&amp;gt; still drives magnetic activity&lt;br /&gt;
&lt;br /&gt;
# Aurorae at lower latitudes&lt;br /&gt;
## higher magnetic rigidity, wider magnetotail, and greater reconnection energy.&lt;br /&gt;
## Combined with a higher flux of stellar particles, this means:&lt;br /&gt;
### Auroral ovals expand, reaching mid-latitudes sometimes equator.&lt;br /&gt;
### The skies are alive with rippling green, violet, and crimson aurorae, especially on the night side.&lt;br /&gt;
### Daily auroral activity occur during stellar flare cycles.&lt;br /&gt;
# Compasses&lt;br /&gt;
## compasses respond more sharply, with:&lt;br /&gt;
### Faster alignment.&lt;br /&gt;
### Greater resistance to local perturbations.&lt;br /&gt;
## However, frequent magnetic storms from stellar activity cause sudden declinations, reversals, or local anomalies.  In short, lots of aurorae equals dead compasses at the same time.&lt;br /&gt;
# Magnetic Field Strength &amp;gt; 100 μT &lt;br /&gt;
# Electromagnetism is more basic than chemistry or almost any other natural philosophy&lt;br /&gt;
&lt;br /&gt;
==== Substellar Point ====&lt;br /&gt;
The maximum incoming flux is very nearly the same as Earth&#039;s solar constant (≈1361 W/m²), but concentrated over one point rather than averaged over a rotating sphere.  Temperatures should be above 500ºK most of the time.  &lt;br /&gt;
&lt;br /&gt;
The magnetic north is also here, The thick atmosphere prevents too much loss here, but &lt;br /&gt;
* Charged particle influx&lt;br /&gt;
** Maximized at the substellar point—intense auroral and energetic particle precipitation&lt;br /&gt;
* Atmospheric ionization&lt;br /&gt;
** Constant production of high-energy ions and NOx compounds—possible UV fluorescence in upper sky&lt;br /&gt;
* Localized heating&lt;br /&gt;
** Augments already extreme temperatures—600–700 K surface possible&lt;br /&gt;
&lt;br /&gt;
=== Artificially Tethered Moon ===&lt;br /&gt;
* 670,000 km up&lt;br /&gt;
* 7805 km in radius = same as the planet&lt;br /&gt;
* 1.33º of the sky, same as the sun&lt;br /&gt;
&lt;br /&gt;
A network of tethers/tension lines from the moon to multiple anchor points on the planet’s surface (a tripod or hexapod structure), woven like hair&lt;br /&gt;
* Uses active tension management and orbital station-keeping to stabilize the moon&lt;br /&gt;
* Counterweights and inward-pointing mass drivers on the moon to oppose drift&lt;br /&gt;
&lt;br /&gt;
The tethers are not bearing the full weight, but merely damping drift, providing restoring force, and enabling long-term stability through active compensation.  The moon&lt;br /&gt;
* Blocks the worst of the heat&lt;br /&gt;
* Blocks the worst of the solar radiation&lt;br /&gt;
The moon has &lt;br /&gt;
* low mass&lt;br /&gt;
* high albedo - enormous reflectivity&lt;br /&gt;
* scatters charges particles, UV, X-rays, auroral flux tubes&lt;br /&gt;
* sunward - crazy hot, high emissivity&lt;br /&gt;
* earthward - crazy cool, low emissivity&lt;br /&gt;
== Morphology ==&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
! Case !! Function !! Gloss !! Ending&lt;br /&gt;
|+ Existential cases&lt;br /&gt;
|-&lt;br /&gt;
! Topical&lt;br /&gt;
| Frames the referent of the utterance ||	“As for…”&lt;br /&gt;
! -Mp&#039;a&lt;br /&gt;
|-&lt;br /&gt;
! Identity&lt;br /&gt;
| Category, essence, nominal predicate ||	“is a…” / “equals…”&lt;br /&gt;
! -&lt;br /&gt;
|-&lt;br /&gt;
! Possessive&lt;br /&gt;
| ownership, authorship, kinship, part-whole || “X’s Y”&lt;br /&gt;
! -rkI&lt;br /&gt;
|-&lt;br /&gt;
! Genitive	&lt;br /&gt;
| association, content, theme, objective, attribution || “Y of X”&lt;br /&gt;
! -ł(Ɛ)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Where/When Cases&lt;br /&gt;
! Case !!	Function !!	Typical gloss !! Ending&lt;br /&gt;
|-&lt;br /&gt;
! Locative&lt;br /&gt;
| Place, state, context of being, time-within ||	“in,” “at,” “on”, &amp;quot;during&amp;quot;&lt;br /&gt;
! -f&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Dative&lt;br /&gt;
| Target, direction ||	“to,” “for,” “until&amp;quot;, &amp;quot;as far as&amp;quot;&lt;br /&gt;
! -Mk&#039;O&lt;br /&gt;
|-&lt;br /&gt;
! Ablative&lt;br /&gt;
| Source, cause, origin || “from,” “because of,” “due to”&lt;br /&gt;
! -bdI&lt;br /&gt;
|-&lt;br /&gt;
! Benefactive&lt;br /&gt;
| Advantage, interest, concern || “for the benefit of…”, &amp;quot;at the behest of&amp;quot;&lt;br /&gt;
! -aI&lt;br /&gt;
|-&lt;br /&gt;
! Abessive&lt;br /&gt;
| Absence, privation, “lacking”	|| “without,” “lacking,” “free from”, &amp;quot;exclude&amp;quot;&lt;br /&gt;
! -st&#039;Ɛ&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ How Cases&lt;br /&gt;
! Case !! Function 	!! Typical gloss !! Ending&lt;br /&gt;
|-&lt;br /&gt;
! Instrumental &lt;br /&gt;
| Means, medium, material || “by (means of)”, “through,” “with”, &amp;quot;using&amp;quot;&lt;br /&gt;
! -fla&lt;br /&gt;
|-&lt;br /&gt;
! Adverbial&lt;br /&gt;
| Role/state modifier, part of speech shift	|| “as (a) X,” “in a X way”, &amp;quot;like&amp;quot;&lt;br /&gt;
! -Oad&lt;br /&gt;
|-&lt;br /&gt;
! Translative&lt;br /&gt;
| Change of state, transform/manifestation ||	“becoming,” “into,” “turning into”&lt;br /&gt;
! -k&#039;(I)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Noun Classes&lt;br /&gt;
! !! Not &amp;quot;Container&amp;quot; (mass: ?, ??) !! &amp;quot;Container&amp;quot; (count: ?, ??)&lt;br /&gt;
|-&lt;br /&gt;
! Idea + Matter	&lt;br /&gt;
| Animals (also temperaments) || 	Persons / Gods&lt;br /&gt;
|-&lt;br /&gt;
! Matter only	&lt;br /&gt;
| (Diffuse) Substances: air, fire || 	Tools , &amp;quot;rocks&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
! Idea only	&lt;br /&gt;
| Actions	|| Abstracts, Categories, Sets&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Number: Containers are unmarked for number, as in Chinese/Japanese/Korean.  Non-containers default to a collective/mass-noun number, but can take a partitive (which can mean as few as one).&lt;br /&gt;
&lt;br /&gt;
Polypersonal pronouns:&lt;br /&gt;
&lt;br /&gt;
== Phonology/Orthography ==&lt;br /&gt;
{| class=&amp;quot;bluetable&amp;quot; style=&amp;quot;text-align:center; float:left&amp;quot;&lt;br /&gt;
! !!	Labial !!	Labiolingual !!	Alveolar !!	Palatal !! Velar !!	Glottal&lt;br /&gt;
|-&lt;br /&gt;
! Nasal	&lt;br /&gt;
| /m/	&#039;&#039;&#039;m&#039;&#039;&#039; || /n̼/ &#039;&#039;&#039;n&#039;&#039;&#039; || /n/ &#039;&#039;&#039;n&#039;&#039;&#039; || /ŋ/ &#039;&#039;&#039;ŋ&#039;&#039;&#039;			||&lt;br /&gt;
|-&lt;br /&gt;
! Click&lt;br /&gt;
| (/ᵐʘ/ &#039;&#039;&#039;mx&#039;&#039;&#039;) || || (/ŋǃ/ &#039;&#039;&#039;nc&#039;&#039;&#039;) || ||&lt;br /&gt;
|-&lt;br /&gt;
! Voiced Stop&lt;br /&gt;
| &#039;&#039;&#039;b&#039;&#039;&#039; || 	||	&#039;&#039;&#039;d&#039;&#039;&#039; ||	&#039;&#039;&#039;g&#039;&#039;&#039;	||&lt;br /&gt;
|-&lt;br /&gt;
! Eject. Stop&lt;br /&gt;
| /pʼ/ &#039;&#039;&#039;pq&#039;&#039;&#039; ||	|| /t’/ &#039;&#039;&#039;tq&#039;&#039;&#039;	|| /k’/ &#039;&#039;&#039;kq&#039;&#039;&#039; ||	/ʔ/ &#039;&#039;&#039; &#039; &#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Unvoiced Stop&lt;br /&gt;
| &#039;&#039;&#039;p&#039;&#039;&#039; ||	||	&#039;&#039;&#039;t&#039;&#039;&#039; || /k~x/ &#039;&#039;&#039;k&#039;&#039;&#039;	||&lt;br /&gt;
|-&lt;br /&gt;
! Plain Fricative&lt;br /&gt;
| /ɸ~β/ &#039;&#039;&#039;f&#039;&#039;&#039; ||	/θ̼~ð̼/ &#039;&#039;&#039;þ&#039;&#039;&#039;	|| /s~z/ &#039;&#039;&#039;s&#039;&#039;&#039; || (/ʒ/ &#039;&#039;&#039;ž&#039;&#039;&#039;) || ||&lt;br /&gt;
|-&lt;br /&gt;
! Eject. Fricative&lt;br /&gt;
| /fʼ/ &#039;&#039;&#039;fq&#039;&#039;&#039; ||	/θ̼ʼ/ &#039;&#039;&#039;þq&#039;&#039;&#039; || /s’~ts’/ &#039;&#039;&#039;sq&#039;&#039;&#039;		|| ||&lt;br /&gt;
|-&lt;br /&gt;
! Approx./Trill	&lt;br /&gt;
| &#039;&#039;&#039;w&#039;&#039;&#039;	|| || &#039;&#039;&#039;r&#039;&#039;&#039; || &#039;&#039;&#039;j&#039;&#039;&#039; ||	/h~ɦ/ &#039;&#039;&#039;h&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
! Laterals&lt;br /&gt;
| || /l̼/ &#039;&#039;&#039;l&#039;&#039;&#039; ||	/ɬ/ &#039;&#039;&#039;ł&#039;&#039;&#039;		|| ||&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;bluetable&amp;quot; style=&amp;quot;float:right; text-align:center;&amp;quot;&lt;br /&gt;
! !! Front !! Back !! Underspecified&lt;br /&gt;
|-&lt;br /&gt;
! High&lt;br /&gt;
| &#039;&#039;&#039;i&#039;&#039;&#039; || &#039;&#039;&#039;u&#039;&#039;&#039; || I&lt;br /&gt;
|-&lt;br /&gt;
! High-Mid&lt;br /&gt;
| &#039;&#039;&#039;e&#039;&#039;&#039; || &#039;&#039;&#039;o&#039;&#039;&#039; || O&lt;br /&gt;
|-&lt;br /&gt;
! Low-Mid&lt;br /&gt;
| /ɛ/ &#039;&#039;&#039;ë&#039;&#039;&#039; || /ɔ/ &#039;&#039;&#039;ö&#039;&#039;&#039; || Ö&lt;br /&gt;
|-&lt;br /&gt;
! Low&lt;br /&gt;
| colspan=&amp;quot;2&amp;quot; | /ä/ &#039;&#039;&#039;a&#039;&#039;&#039;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;br clear=&amp;quot;both&amp;quot;&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Allophony:&lt;br /&gt;
* nasal + labial ejective -&amp;gt; [m͡ʘ]&lt;br /&gt;
* nasal + non-labial ejective -&amp;gt; [ŋ͡ǃ]&lt;br /&gt;
&lt;br /&gt;
Phonotactics are (C)(G)V(C&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;):&lt;br /&gt;
* any consonant or none can a syllable&lt;br /&gt;
* Glides (/j/ or /w/) after anything&lt;br /&gt;
* hiatus allowed, diphthongs not&lt;br /&gt;
* any coda, except glides&lt;br /&gt;
&lt;br /&gt;
=== Sentences ===&lt;br /&gt;
# The storm scared people&lt;br /&gt;
#* k’ɛthu-Mp’a ʔusɛk närgo-f’&lt;br /&gt;
#* kqëthumxa ’usëk närgofq&lt;br /&gt;
#* As for the storm, (there is) fear in people.&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
	<entry>
		<id>https://www.frathwiki.com/index.php?title=User:Aquatiki/Sandbox2&amp;diff=167911</id>
		<title>User:Aquatiki/Sandbox2</title>
		<link rel="alternate" type="text/html" href="https://www.frathwiki.com/index.php?title=User:Aquatiki/Sandbox2&amp;diff=167911"/>
		<updated>2025-03-24T23:04:34Z</updated>

		<summary type="html">&lt;p&gt;Aquatiki: Redirected page to User:Aquatiki&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;#REDIRECT [[User:Aquatiki]]&lt;/div&gt;</summary>
		<author><name>Aquatiki</name></author>
	</entry>
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