Difference between revisions of "Planetary Classes (FASA)"

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'''Classes'''<br/>
 
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==Class A==
 
==Class A==
 
{{ImageBox2|file=jupiter-tng-101-102.jpg|caption=[[Jupiter (FASA)|Jupiter]], a Class A world ([[Star Trek: The Next Generation|TNG]]&nbsp;[[Encounter at Farpoint (Episode)|101-102]])}}
 
{{ImageBox2|file=jupiter-tng-101-102.jpg|caption=[[Jupiter (FASA)|Jupiter]], a Class A world ([[Star Trek: The Next Generation|TNG]]&nbsp;[[Encounter at Farpoint (Episode)|101-102]])}}
 
Class A planets were gas giants with a tenuous surface, which may not have been present at all. The atmosphere was reducing, and composed of elements such as methane. Class A planets radiated their own heat, and could also be considered "failed" stars. An example of a Class A planet is [[Jupiter (FASA)|Jupiter]].<ref name="WoF"/>
 
Class A planets were gas giants with a tenuous surface, which may not have been present at all. The atmosphere was reducing, and composed of elements such as methane. Class A planets radiated their own heat, and could also be considered "failed" stars. An example of a Class A planet is [[Jupiter (FASA)|Jupiter]].<ref name="WoF"/>
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==Class B==
 
==Class B==
 
Class B planets were gas giants with a tenuous surface, which may not have been present at all. The atmosphere was reducing. Class B planets did not radiate their own heat. An example of a Class B planet is [[Neptune (FASA)|Neptune]].<ref name="WoF"/>
 
Class B planets were gas giants with a tenuous surface, which may not have been present at all. The atmosphere was reducing. Class B planets did not radiate their own heat. An example of a Class B planet is [[Neptune (FASA)|Neptune]].<ref name="WoF"/>
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{{Clear}}
 
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==Class G==
 
==Class G==
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{{ImageBox2|float=left|file=rigel-12-tos03.jpg|caption=[[Rigel XII (FASA)|Rigel XII]], a Class G world ([[Star Trek|TOS]]&nbsp;[[Mudd's Women (Episode)|03]])}}
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{{ImageBox2|file=rigel-12-tos03_original.jpg|caption=[[Rigel XII (FASA)|Rigel XII]], a Class G world ([[Star Trek|TOS]]&nbsp;[[Mudd's Women (Episode)|03]])}}
 
Class G planets had a silicate surface. The atmosphere was thin and oxidizing. Class G planets were desert worlds. An example of a Class G planet is [[Rigel XII (FASA)|Rigel XII]].<ref name="WoF"/>
 
Class G planets had a silicate surface. The atmosphere was thin and oxidizing. Class G planets were desert worlds. An example of a Class G planet is [[Rigel XII (FASA)|Rigel XII]].<ref name="WoF"/>
 
{{Clear}}
 
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==Class H==
 
==Class H==
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{{ImageBox2|file=gothos-tos-18.jpg|caption=[[Gothos (FASA)|Gothos]], a Class H world ([[Star Trek|TOS]]&nbsp;[[The Squire of Gothos (Episode)|18]])}}
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{{ImageBox2|file=gothos-tos18_original.jpg|caption=[[Gothos (FASA)|Gothos]], a Class H world ([[Star Trek|TOS]]&nbsp;[[The Squire of Gothos (Episode)|18]])}}
 
Class H planets had a silicate surface. The atmosphere was variable. Class H planets were geologically active. An example of a Class H planet is [[Gothos (FASA)|Gothos]].<ref name="WoF"/>
 
Class H planets had a silicate surface. The atmosphere was variable. Class H planets were geologically active. An example of a Class H planet is [[Gothos (FASA)|Gothos]].<ref name="WoF"/>
 
{{Clear}}
 
{{Clear}}
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==Class I==
 
==Class I==
 
Class I planets had a metallic/silicate surface. The atmosphere was fluid and very dense. Class I planets were small and young. An example of a Class I planet is [[Excalbia (FASA)|Excalbia]].<ref name="WoF"/>
 
Class I planets had a metallic/silicate surface. The atmosphere was fluid and very dense. Class I planets were small and young. An example of a Class I planet is [[Excalbia (FASA)|Excalbia]].<ref name="WoF"/>
 
{{Clear}}
 
{{Clear}}
 
==Class J==
 
==Class J==
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{{ImageBox2|float=left|file=moon-stsc.jpg|caption=[[Earth (FASA)|Earth]]'s [[Luna (FASA)|moon]], a Class J world ([[Star Trek: Star Charts (Book)|STSC]])}}
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{{ImageBox2|file=moon-stsc.jpg|caption=[[Earth (FASA)|Earth]]'s [[Luna (FASA)|moon]], a Class J world ([[Star Trek: Star Charts (Book)|STSC]])}}
 
Class J planets had a silicate surface. The atmosphere was very tenuous, with noble gases. Class J planets were often moons. An example of a Class J planet is [[Luna (FASA)|Luna]].<ref name="WoF"/>
 
Class J planets had a silicate surface. The atmosphere was very tenuous, with noble gases. Class J planets were often moons. An example of a Class J planet is [[Luna (FASA)|Luna]].<ref name="WoF"/>
 
{{Clear}}
 
{{Clear}}
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==Class K==
 
==Class K==
 
{{ImageBox2|file=mars-stsc.jpg|caption=[[Mars (FASA)|Mars]], a Class K world ([[Star Trek: Star Charts (Book)|STSC]])}}
 
{{ImageBox2|file=mars-stsc.jpg|caption=[[Mars (FASA)|Mars]], a Class K world ([[Star Trek: Star Charts (Book)|STSC]])}}
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{{Clear}}
 
{{Clear}}
 
==Class L==
 
==Class L==
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{{ImageBox2|float=left|file=psi2000-tos06.jpg|caption=[[Psi 2000 (FASA)|Psi 2000]], a Class L world ([[Star Trek|TOS]]&nbsp;[[The Naked Time (Episode)|06]])}}
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{{ImageBox2|file=psi2000-tos06_original.jpg|caption=[[Psi 2000 (FASA)|Psi 2000]], a Class L world ([[Star Trek|TOS]]&nbsp;[[The Naked Time (Episode)|06]])}}
 
Class L planets had a silicate/water surface. The atmosphere was oxidizing. Class L planets were geologically inactive. An example of a Class L planet is [[Psi 2000 (FASA)|Psi 2000]].<ref name="WoF"/>
 
Class L planets had a silicate/water surface. The atmosphere was oxidizing. Class L planets were geologically inactive. An example of a Class L planet is [[Psi 2000 (FASA)|Psi 2000]].<ref name="WoF"/>
 
{{Clear}}
 
{{Clear}}
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==Class M==
 
==Class M==
 
{{ImageBox2|file=earth-tos-21.jpg|caption=[[Earth (FASA)|Earth]], a Class M world ([[Star Trek|TOS]]&nbsp;[[Tomorrow is Yesterday (Episode)|21]])}}
 
{{ImageBox2|file=earth-tos-21.jpg|caption=[[Earth (FASA)|Earth]], a Class M world ([[Star Trek|TOS]]&nbsp;[[Tomorrow is Yesterday (Episode)|21]])}}
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[[Category:Astrometrics]]
 
[[Category:Astrometrics]]
 
[[Category:Planets]]
 
[[Category:Planets]]
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[[Category:Planetary Classes]]
 
 
[[Category:TOS]]
 
[[Category:TOS]]
 
[[Category:Film]]
 
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[[Category:Books]]
 
[[Category:Books]]
 
[[Category:FASA Timeline]]
 
[[Category:FASA Timeline]]

Latest revision as of 06:05, 5 September 2023

Planetary Classes
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Class A

Jupiter, a Class A world (TNG 101-102)

Jupiter, a Class A world (TNG 101-102)

Class A planets were gas giants with a tenuous surface, which may not have been present at all. The atmosphere was reducing, and composed of elements such as methane. Class A planets radiated their own heat, and could also be considered "failed" stars. An example of a Class A planet is Jupiter.[1]

Class B

Class B planets were gas giants with a tenuous surface, which may not have been present at all. The atmosphere was reducing. Class B planets did not radiate their own heat. An example of a Class B planet is Neptune.[1]

Class C

Class C planets had an iron/silicate surface. The atmosphere was reducing and dense. Class C planets also had high surface temperatures. An example of a Class C planet is Venus.[1]

Class D

Class D planets had a nickel-iron/silicate surface. The atmosphere was tenuous, if one existed at all. Class D planets were typically moons or large meteroids.[2] An example of a Class D planet is Ceres.[1]

Class E

Class E planets had a silicate surface with some metals. The atmosphere was reducing or oxidizing. Class E planets had large, molten cores. An example of a Class E planet is Janus VI.[1]

Class F

Delta Vega, a Class F world (TOS 01)

Delta Vega, a Class F world (TOS 01)

Class F planets had a silicate surface with some metals. The atmosphere was oxidizing. Class F planets were very young, typically less than 109 years. An example of a Class F planet is Delta Vega.[1]

Class G

Rigel XII, a Class G world (TOS 03)

Rigel XII, a Class G world (TOS 03)

Class G planets had a silicate surface. The atmosphere was thin and oxidizing. Class G planets were desert worlds. An example of a Class G planet is Rigel XII.[1]


Class H

Gothos, a Class H world (TOS 18)

Gothos, a Class H world (TOS 18)

Class H planets had a silicate surface. The atmosphere was variable. Class H planets were geologically active. An example of a Class H planet is Gothos.[1]


Class I

Class I planets had a metallic/silicate surface. The atmosphere was fluid and very dense. Class I planets were small and young. An example of a Class I planet is Excalbia.[1]

Class J

Earth's moon, a Class J world (STSC)

Earth's moon, a Class J world (STSC)

Class J planets had a silicate surface. The atmosphere was very tenuous, with noble gases. Class J planets were often moons. An example of a Class J planet is Luna.[1]


Class K

Mars, a Class K world (STSC)

Mars, a Class K world (STSC)

Class K planets had a silicate surface. The atmosphere was tenuous, with some water. Class K planets were adaptable with the use of pressure domes. An example of a Class K planet is Mars.[1]

Class L

Psi 2000, a Class L world (TOS 06)

Psi 2000, a Class L world (TOS 06)

Class L planets had a silicate/water surface. The atmosphere was oxidizing. Class L planets were geologically inactive. An example of a Class L planet is Psi 2000.[1]


Class M

Earth, a Class M world (TOS 21)

Earth, a Class M world (TOS 21)

Class M planets had a silicate/water surface. The atmosphere was oxidizing,[1] and consisted largely of nitrogen and oxygen.[3] Class M planets were geologically active. An example of a Class M planet is Earth.[1]

Class N

Class N planets had a surface covered entirely in water. The atmosphere was oxidizing. Class N planets were pelagic planets. An example of a Class N planet is Argo.[1]

Notes and References

  1. ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 1.10 1.11 1.12 1.13 1.14 Johnson, Shane. Star Trek: The Worlds of the Federation. Pocket Books, 1989.
  2. ↑ Salin, Robert (Producer). Star Trek II: The Wrath of Khan. Directed by Nicholas Meyer. Story by Harve Bennett and Jack B. Sowards. Screenplay by Nicholas Meyer (Uncredited). Paramount Pictures. 4 June 1982.
  3. ↑ Roddenberry, Gene (Executive Producer). "The Cage". Star Trek, season 0, episode 0 (Production number 01). Directed by Robert Butler. Written by Gene Roddenberry. Released 1986. Desilu Productions. 1965.
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