Planetary Classification: Difference between revisions
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==Classifications== | ==Classifications== | ||
===Class A=== | ===Class A=== | ||
* Geothermal rocky body | |||
* Young world not yet solidified | |||
* Insufficiently large to maintain atmosphere, heat following solidification | |||
* Primarily hydrogen-based atmosphere | |||
* Eventually cools to class C | |||
===Class B=== | ===Class B=== | ||
* Geomorteus rocky body | |||
* Orbits close to primary | |||
* Surface temperature high; portions of surface potentially molten | |||
* Little to no atmosphere due to heat and solar ablation | |||
===Class C=== | ===Class C=== | ||
* Geoinactive rocky body | |||
* Transition from Class A | |||
* Geological processes largely halted | |||
* Atmosphere cooled, potentially frozen | |||
===Class D=== | ===Class D=== | ||
* Airless body, often an asteroid or moon | * Airless body, often an asteroid or moon | ||
===Class E=== | ===Class E=== | ||
* Geoplastic rocky body | |||
* Young world not yet solidified | |||
* Essentially a large class A | |||
* Transitions to class F | |||
===Class F=== | ===Class F=== | ||
* Geometallic rocky body | |||
* Transition from class E | |||
* Surface partially solidified, geological and geothermal activity still high | |||
* Largely uninhabitable by humanoid life | |||
* Transitions to class G | |||
===Class G=== | ===Class G=== | ||
* Geocrystalline rocky body | |||
* Transition from class F | |||
* Surface essentially solidified | |||
* Temperatures cooling, potentially survivable range | |||
* Thick atmosphere | |||
** Often low oxygen content due to oxygen binding in crust | |||
* Potentially habitable with technological aid | |||
* Transition to class H, K-P | |||
===Class H=== | ===Class H=== | ||
* | * Rocky body | ||
* | * Very arid world | ||
** High surface temperature | |||
* Little to no surface water | |||
* Atmosphere often saturated with heavy gasses or metallic vapors | * Atmosphere often saturated with heavy gasses or metallic vapors | ||
* Generally uninhabitable to humanoid life | * Generally uninhabitable to humanoid life | ||
===Class I=== | ===Class I=== | ||
* Ice giant | |||
* Atmospheric envelope dominated by ammonia, water, methane | |||
** Hydrogen levels very low (20% or lower) as compared to class J planets | |||
===Class J=== | ===Class J=== | ||
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*** Type 2: 150K-250K, dominated by water vapor clouds | *** Type 2: 150K-250K, dominated by water vapor clouds | ||
*** Type 3: 250K-800K, cloudless | *** Type 3: 250K-800K, cloudless | ||
* Known as [[Fesoan]]-class by [[Andorian Empire|Andorian]]s (ENT Novel: ''Live by the Code'') | |||
===Class K=== | ===Class K=== | ||
* Adaptable | |||
* Adaptable | |||
* Generally thin atmopshere | * Generally thin atmopshere | ||
* Little to no surface water | * Little to no surface water | ||
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===Class L=== | ===Class L=== | ||
* | * Marginal | ||
* Transitioned from class G | |||
* Barely habitable or habitable with minimal technological aid | * Barely habitable or habitable with minimal technological aid | ||
** Often pre-terraforming state | ** Often pre-terraforming state | ||
* Native life often limited to flora | |||
** Possibly in process of transitioning to class M | |||
===Class M=== | ===Class M=== | ||
* Terrestrial | * Terrestrial | ||
* Previously known as [[Vulcan (planet)|Minshara]]-class by | * Previously known as [[Vulcan (planet)|Minshara]]-class by Vulcan Science Directorate, Earth-type by [[UESPA]] (ENT, TOS) | ||
* Significant surface water, below 80% coverage | * Significant surface water, below 80% coverage | ||
* Atmosphere consisting of nitrogen, oxygen, trace elements | * Atmosphere consisting of nitrogen, oxygen, trace elements | ||
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===Class N=== | ===Class N=== | ||
* | * Reducing | ||
* Thick atmosphere, often saturated with sulfur compounds | * Thick atmosphere, often saturated with sulfur compounds | ||
* High surface temperature due to atmospheric greenhouse effect | * High surface temperature due to atmospheric greenhouse effect | ||
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===Class O=== | ===Class O=== | ||
* Pelagic | |||
* Largely identical in composition and habitability to class M | |||
* Liquid water covers 80+% of surface | |||
* Life generally only present if sufficient landmasses to allow for mineral circulation | |||
* Common alternative to class M planets in systems with gravitational disruption of protoplanetary disk leading to increased cometary bombardment (TNG Novel: ''The Buried Age'') | |||
** Examples include distant stellar companions, multiple inward-migrating Jovians (TNG Novel: ''The Buried Age'') | |||
===Class P=== | ===Class P=== | ||
* Glaciated | |||
* Largely identical in composition to class M | |||
* Surface temperatures below freezing | |||
* Generally covered in water ice | |||
* Often transitioning from prior class due to changes in available surface heat | |||
* Scientific study often based from subglacial bases constructed on rocky core beneath planetary ocean/slush mantle, ice crust (TNG Novel: ''The Buried Age'') | |||
===Class Q=== | ===Class Q=== | ||
* Variable | |||
* Previously known as Quaris-class by Vulcan Science Directorate | |||
* Unpredictable surface and environmental conditions | |||
** Generally wide variations from region to region | |||
* Often caused by variable star output, highly eccentric orbit | |||
===Class R=== | ===Class R=== | ||
* Rogue | |||
* Generally uninhabitable | |||
** Geothermal heat can sometimes maintain ecosystem on surface | |||
===Class S=== | ===Class S=== | ||
* Gas dwarf | |||
* Generally protoplanetary stage progressing towards class I | |||
===Class T=== | ===Class T=== | ||
* Hot gas giant | |||
** Divided into [https://en.wikipedia.org/wiki/Sudarsky%27s_gas_giant_classification two subtypes] by temperature, predominant cloud formation | |||
*** Type 4: 900K-1400K, dominated by alkali clouds | |||
*** Type 5: 1400+K, dominated by silicate clouds | |||
===Class X=== | |||
* Miscellaneous classification | |||
* Any planetary status not falling under standard natural planetary development | |||
* ''Unsubstantiated'' | |||
===Class Y=== | ===Class Y=== | ||
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** ''Class I ice giant'' | ** ''Class I ice giant'' | ||
** ''Class J cold gas giant'' | ** ''Class J cold gas giant'' | ||
*** ''Type | *** ''Type 1 through 3 using [https://en.wikipedia.org/wiki/Sudarsky%27s_gas_giant_classification Sudarsky's schema]'' | ||
** ''Class S gas dwarf'' | ** ''Class S gas dwarf'' | ||
*** ''[http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?bibcode=1989A&A...215..177S&db_key=AST&page_ind=0&data_type=GIF&type=SCREEN_VIEW&classic=YES Theoretical protoplanet state] leading to ice giants, potentially also gas giant that has lost atmosphere to solar wind ablation'' | *** ''[http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?bibcode=1989A&A...215..177S&db_key=AST&page_ind=0&data_type=GIF&type=SCREEN_VIEW&classic=YES Theoretical protoplanet state] leading to ice giants, potentially also gas giant that has lost atmosphere to solar wind ablation'' | ||
** ''Class T hot gas giant (fka hot Jupiter)'' | ** ''Class T hot gas giant (fka hot Jupiter)'' | ||
*** ''Type | *** ''Type 4 through 5 using Sudarsky's schema'' | ||
(''Star Charts'' unless otherwise referenced) | (''Star Charts'' unless otherwise referenced) | ||
[[Category:Astronomy]] | [[Category:Astronomy]] |
Latest revision as of 07:42, 26 April 2018
Facts
- Planetary classification system established by mid-23rd century
- Descends from similar classification systems established by Vulcan Science Directorate, UESPA (ENT, TOS)
Classifications
Class A
- Geothermal rocky body
- Young world not yet solidified
- Insufficiently large to maintain atmosphere, heat following solidification
- Primarily hydrogen-based atmosphere
- Eventually cools to class C
Class B
- Geomorteus rocky body
- Orbits close to primary
- Surface temperature high; portions of surface potentially molten
- Little to no atmosphere due to heat and solar ablation
Class C
- Geoinactive rocky body
- Transition from Class A
- Geological processes largely halted
- Atmosphere cooled, potentially frozen
Class D
- Airless body, often an asteroid or moon
Class E
- Geoplastic rocky body
- Young world not yet solidified
- Essentially a large class A
- Transitions to class F
Class F
- Geometallic rocky body
- Transition from class E
- Surface partially solidified, geological and geothermal activity still high
- Largely uninhabitable by humanoid life
- Transitions to class G
Class G
- Geocrystalline rocky body
- Transition from class F
- Surface essentially solidified
- Temperatures cooling, potentially survivable range
- Thick atmosphere
- Often low oxygen content due to oxygen binding in crust
- Potentially habitable with technological aid
- Transition to class H, K-P
Class H
- Rocky body
- Very arid world
- High surface temperature
- Little to no surface water
- Atmosphere often saturated with heavy gasses or metallic vapors
- Generally uninhabitable to humanoid life
Class I
- Ice giant
- Atmospheric envelope dominated by ammonia, water, methane
- Hydrogen levels very low (20% or lower) as compared to class J planets
Class J
- Cold gas giant
- Divided into three subtypes by temperature, predominant cloud formation
- Type 1: 150K or lower, dominated by ammonia clouds
- Type 2: 150K-250K, dominated by water vapor clouds
- Type 3: 250K-800K, cloudless
- Divided into three subtypes by temperature, predominant cloud formation
- Known as Fesoan-class by Andorians (ENT Novel: Live by the Code)
Class K
- Adaptable
- Generally thin atmopshere
- Little to no surface water
- Surface conditions suitable for life with aid of pressure domes or life support technology (TOS: "I, Mudd")
- Often pre-terraforming state
Class L
- Marginal
- Transitioned from class G
- Barely habitable or habitable with minimal technological aid
- Often pre-terraforming state
- Native life often limited to flora
- Possibly in process of transitioning to class M
Class M
- Terrestrial
- Previously known as Minshara-class by Vulcan Science Directorate, Earth-type by UESPA (ENT, TOS)
- Significant surface water, below 80% coverage
- Atmosphere consisting of nitrogen, oxygen, trace elements
- Habitable by humanoid life
- Subdivided into type 1-4, indicating most to least suitable for humanoid life (TNG: "The Bonding")
Class N
- Reducing
- Thick atmosphere, often saturated with sulfur compounds
- High surface temperature due to atmospheric greenhouse effect
- Generally uninhabitable for humanoid life
Class O
- Pelagic
- Largely identical in composition and habitability to class M
- Liquid water covers 80+% of surface
- Life generally only present if sufficient landmasses to allow for mineral circulation
- Common alternative to class M planets in systems with gravitational disruption of protoplanetary disk leading to increased cometary bombardment (TNG Novel: The Buried Age)
- Examples include distant stellar companions, multiple inward-migrating Jovians (TNG Novel: The Buried Age)
Class P
- Glaciated
- Largely identical in composition to class M
- Surface temperatures below freezing
- Generally covered in water ice
- Often transitioning from prior class due to changes in available surface heat
- Scientific study often based from subglacial bases constructed on rocky core beneath planetary ocean/slush mantle, ice crust (TNG Novel: The Buried Age)
Class Q
- Variable
- Previously known as Quaris-class by Vulcan Science Directorate
- Unpredictable surface and environmental conditions
- Generally wide variations from region to region
- Often caused by variable star output, highly eccentric orbit
Class R
- Rogue
- Generally uninhabitable
- Geothermal heat can sometimes maintain ecosystem on surface
Class S
- Gas dwarf
- Generally protoplanetary stage progressing towards class I
Class T
- Hot gas giant
- Divided into two subtypes by temperature, predominant cloud formation
- Type 4: 900K-1400K, dominated by alkali clouds
- Type 5: 1400+K, dominated by silicate clouds
- Divided into two subtypes by temperature, predominant cloud formation
Class X
- Miscellaneous classification
- Any planetary status not falling under standard natural planetary development
- Unsubstantiated
Class Y
- Terrestrial
- Colloquially known as "demon"-class (VOY: "Demon")
- Extremely high surface temperatures
- Corrosive and/or toxic atmosphere
- Thermionic discharges from surface-level metallic hydrogen deposits common (VOY: "Demon")
- Planetary conditions can lead to vessel hazards even at standard orbital altitude (VOY: "Demon")
Notes
- Star Charts classifications flawed w.r.t. giant planets
- Radii are physically impossible
- Jupiter diameter ~140,000km, maximum theoretical possible planetary diameter ~400,000km, but class T planets go up to 120m km?
- Adding more mass generally tends to increase density, not radius; proximity to sun increases size but only so far
- No acknowledgement of ice giants (not widespread distinction yet at time of writing) despite physically distinct characteristics
- All Star charts giant classes are predominantly hydrogen-based, ice giants (i.e. Neptune, Uranus) are water/ammonia-based with very slim hydrogen envelopes
- All gas giants listed as being in "cold zone" beyond ecosphere, which doesn't fit later discoveries
- Written before discovery of numerous hot Jupiters by various exoplanet surveys
- Radii are physically impossible
- Alteration:
- Class I ice giant
- Class J cold gas giant
- Type 1 through 3 using Sudarsky's schema
- Class S gas dwarf
- Theoretical protoplanet state leading to ice giants, potentially also gas giant that has lost atmosphere to solar wind ablation
- Class T hot gas giant (fka hot Jupiter)
- Type 4 through 5 using Sudarsky's schema
(Star Charts unless otherwise referenced)