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The following is a chart of the standard planetary classification system used by the United Federation of Planets.

Planetary Classification Chart
Class Description Diameter Zone Surface Atmosphere Examples Notes
Class A geothermal 1,000 - 10,000 km Ecosphere / Cold Zone partially molten, volcanic hydrogen compounds Gothos, Io cools to become Class C


(FASA: Class H)

Class B geomorteus 1,000 - 10,000 km Hot Zone partially molten, high temperature extremely tenuous, chemically inactive Mercury (FASA: Class I)
Class C geoinactive 1,000 - 10,000 km Ecosphere / Cold Zone low temperature partially frozen Pluto
Class D dwarf / asteroid / moon 100 - 1,000 km Hot Zone / Ecosphere / Cold Zone barren and cratered metallic, iron-nickel-silicate none or very tenuous Luna,

Regula, Weytahn

generally found in orbit of larger planets or in asteroid fields


(FASA: Class D or Class J)

Class E geoplastic 10,000 - 15,000 km Ecosphere molten, high temperature hydrogen compounds and reactive gasses Excalbia surface cools to become Class F


(FASA: Class I)

Class F geometallic 10,000 - 15,000 km Ecosphere volcanic hydrogen compounds Janus VI molten core cools to become Class G
Class G geocrystalline 10,000 - 15,000 km Ecosphere crystalizing carbon dioxide, some toxic gasses, possible oxygen and nitrogen Delta Vega evolves into Class H, K, L, M, O or P


(FASA: Class F)

Class H desert 8,000 - 15,000 km Hot Zone / Echosphere / Cold Zone hot and arid, little or no water may contain heavy gasses and metal vapors Rigel XII, Tau Cygna V (FASA: Class G)
Class I ice giant 25,000 - 100,000 km Cold Zone tenuous, heavier gasses surrounding an ice or iron core variable pressure and composition, may contain ammonia, methane, water vapor, carbon, or other heavy gasses, with little hydrogen or helium Neptune, Uranus "Uranian" giants


(FASA: Class B)

Class J1 gas giant 50,000 - 140,000 km Cold Zone tenuous, comprised of gaseous hydrogen and hydrogen compounds, radiates heat variable pressure and composition Jupiter, Saturn, Ba'Syladon "Jovians" are often remnants of a failed star


(FASA: Class A)

Class J2 gas giant 50,000 - 140,000 km Hot Zone tenuous, lower density than Class J variable pressure and composition "Hot Jovians", extremely close to primary, tidally locked; possibly failed brown dwarfs
Class K adaptable 5,000 - 10,000 km Ecosphere barren, little or no water thin, mostly carbon dioxide Mars, Mudd
Class L marginal 10,000 - 15,000 kkm Ecosphere rocky and barren, little water oxygen/argon, high concentration of carbon dioxide Gateway, Indri VIII, Kaijur XII, Mestiko
Class M terrestrial 10,000 - 15,000 km Ecosphere abundant water nitrogen, oxygen and trace elements Andoria, Earth, Vulcan, Qo'noS,Cardassia Prime
Class N1 hot reducing 10,000 - 15,000 km Ecosphere, Hot Zone extreme high temperature extremely dense, carbon dioxide and sulfides Medusa,Venus, Tholia (possibly) (FASA: Class C)
Class N2 cold reducing 3,000 - 10,000 km Cold Zone extreme low temperature, liquid methane lakes, ice extremely dense, nitrogen, methane Titan (pre-terraforming)
Class O pelagic 10,000 - 15,000 km Ecosphere liquid water covers 80% or more; few, small landmasses nitrogen, oxygen and trace elements Argo, Chal, Droplet, Tazi Prime (FASA: Class N)
Class P glaciated 10,000 - 15,000 km Ecosphere, Cold Zone water ice covers 80% or more; possible equatorial habitable zone nitrogen, oxygen and trace elements Exo III, Psi 2000, Rigel X Sometimes former Class M or N2 or P worlds
Class Q variable 4,000 - 15,000 km Hot Zone / Ecosphere / Cold Zone various tenuous to very dense Crateris, Delta Canaris IV, Genesis Planet, Remus, Vor II Extremely variable conditions, sometimes partially habitable, sometimes home to extremophiles, sometimes unstable
Class R rogue 4,000 - 500,000 km Interstellar space or cometary halos various - terrestrial or gaseous tenuous to very dense Dakala "Rogue" planets, extremely variable in composition
Class S gas supergiant 140,000 - 10mil km Cold Zone tenuous, comprised of gaseous hydrogen and helium compounds, may radiate considerable heat variable pressure and composition, may contain water vapor Q'tahL Includes "Class 9 gas giants"; failed protostars; depending on mass, could migrate and become a Hot Jovian, reduce into Class X, or ignite into a red dwarf


(SC: "Class I")

Class T gas ultragiant 10mil - 50mil km Cold Zone tenuous, comprised of gaseous hydrogen and helium compounds, may radiate considerable heat variable pressure and composition, may contain water vapor Kern III failed protostars; depending on mass, could migrate and become a Hot Jovian, reduce into Class X, or ignite into a red dwarf


(SC: "Class S")

Class U gas ultragiant 50mil - 120mil km Cold Zone or Hot Zone tenuous, hydrogen and helium compounds, may radiate considerable heat variable pressure and composition, may contain water vapor Beta Orionis VI, Deneb Kaitos VI failed protostars; depending on mass, could migrate and become a Hot Jovian, reduce into Class X, or ignite into a red dwarf


(SC: "Class T")

Class X chthonian 1,000 - 10,000 km Hot Zone barren, rich in resources none leftover core of a former gas super- or ultragiant after migration into hot zone, usually destroyed by parent star
Class Y demon 10,000 - 50,000 km Hot Zone / Ecosphere / Cold Zone barren, rocky or molten iron, deuterium and/or silicate; temperature can exceed 500 K turbulent, saturated with toxic chemicals and therionic radiation Nukara Prime, Tholia (possibly) could support crystalline/silicon or biomimetic life


Notes[]

  • This chart is mostly derived from classification system presented in Star Trek: Star Charts, and subsequently (mostly) adopted by canon, though some alterations have been made to incorporate additional data, including several sub-classes postulated by The Final Frontier fan fiction series. Notations have been made allowing conversion from the earlier classification system used by FASA and other earlier licensed sources.

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