Planet Classification - Revision history

Cyclops at 21:46, 13 July 2023

2023-07-13T21:46:32Z

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	~~This is~~ a ~~comprehensive guide~~ to the ~~various~~ types of planets ~~that can be found~~ in the ~~cosmos~~. ~~It provides a general overview of each planet type~~, ~~along with their average~~ conditions. ~~Please note that there can be exceptions~~ and ~~outliers~~ to ~~these~~ classifications.		Planet classifications exist to provide a systematic and organized way of categorizing and understanding the diverse range of celestial bodies found throughout the universe. These classifications serve several important purposes. Firstly, they allow scientists and researchers to study and compare planets based on their shared characteristics, such as size, composition, and environmental conditions. This aids in the identification of patterns, trends, and relationships between different types of planets. Secondly, classifications help in the exploration and colonization of space by providing valuable information about the suitability of planets for human habitation and resource extraction. They guide astronomers, explorers, and future settlers in identifying planets that may have the necessary conditions to support life or provide valuable resources. Additionally, planet classifications aid in communication and the dissemination of knowledge about planets. They provide a common language for scientists, enabling them to share information, conduct research, and collaborate on a global scale. Overall, planet classifications play a crucial role in expanding our understanding of the cosmos and shaping our exploration and utilization of space resources.

	{{Planet Class		{{Planet Class

Cyclops at 21:45, 13 July 2023

2023-07-13T21:45:22Z

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Cyclops at 18:41, 4 June 2022

2022-06-04T18:41:54Z

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	{{Planet Class		{{Planet Class
	\|type=Gas Giant		\|type=Gas Giant
			\|age=2-10 Billion Years
	\|radius=25,000 to 250,000 km		\|radius=25,000 to 250,000 km
	\|class=J / Jovian		\|class=J / Jovian

Cyclops at 00:35, 31 December 2021

2021-12-31T00:35:33Z

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	\|atmosphere=None		\|atmosphere=None
	\|surface=Barren and Cratered		\|surface=Barren and Cratered
	\|composition=Anthracite and Basalt		\|composition=Anthracite and Basalt / Layers of Frozen Hydrocarbons & Water
	\|hab=None		\|hab=None
	\|type=Rock		\|type=Rock
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	These dead worlds can appear anywhere in a star system, most Class A and B worlds eventually cool to become Class C. Other worlds such as Class E worlds that evolve too close to their parent star will eventually cool into Class C, losing their atmosphere to the stars heat or gravitational pull. The key feature of a Class C is the lack of any geological activity whatsoever and no atmosphere. These worlds are rocky and barren worlds which can exist in any zone of a star system, their surface temperature largely depends on the zone which they reside, generally speaking it runs between -150 to -120 degree's Celsius since most are located far enough away from the central star to absorb enough heat to bake the surface. However, it is possible for these planets to be close enough to the central star to have surface temperatures much higher, though generally below that of a Class B world.		These dead worlds can appear anywhere in a star system, most Class A and B worlds eventually cool to become Class C. Other worlds such as Class E worlds that evolve too close to their parent star will eventually cool into Class C, losing their atmosphere to the stars heat or gravitational pull. The key feature of a Class C is the lack of any geological activity whatsoever and no atmosphere. These worlds are rocky and barren worlds which can exist in any zone of a star system, their surface temperature largely depends on the zone which they reside, generally speaking it runs between -150 to -120 degree's Celsius since most are located far enough away from the central star to absorb enough heat to bake the surface. However, it is possible for these planets to be close enough to the central star to have surface temperatures much higher, though generally below that of a Class B world.

	Class E typically do not cool to Class C unless they are too close to the star to retain an atmosphere. Without volcanic outgassing the atmosphere will burn away leaving a geologically dead world with no atmosphere. Such evolutions are more rare than the smaller variations which evolve from Class A and B worlds.		Class E typically do not cool to Class C unless they are too close to the star to retain an atmosphere. Without volcanic outgassing the atmosphere will burn away leaving a geologically dead world with no atmosphere. Such evolutions are more rare than the smaller variations which evolve from Class A and B worlds. When a Class P world is too far away from the star, it can eventually evolve into a Class C world with thick layers of frozen hydrocarbons and ice clinging to the surface but no atmosphere to speak of. These worlds are too far away from the parent star for heat to melt / sublimate the frozen surface into an atmosphere. When geological activity ceases on a Class P world sufficiently far from the parent star, it can turn into a Class C if stellar heat is not sufficient to prevent the atmosphere from freezing.

	These worlds are often rich in minerals and make incredibly good candidates for mining operations. Some can even have semi-molten iron cores with rich deposits of minerals produced either by steady impact of meteorites during the early phases of their existence (usually these worlds begin as Class A worlds or similar and then become more inactive as they cool over several billion years). Examples include Psi 2000.		These worlds are often rich in minerals and make incredibly good candidates for mining operations. Some can even have semi-molten iron cores with rich deposits of minerals produced either by steady impact of meteorites during the early phases of their existence (usually these worlds begin as Class A worlds or similar and then become more inactive as they cool over several billion years). Examples include Psi 2000.

Cyclops at 00:30, 31 December 2021

2021-12-31T00:30:35Z

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	\|age=2-10 Billion Years		\|age=2-10 Billion Years
	\|radius=5,000 to 7,500 km		\|radius=5,000 to 7,500 km
	\|location=~~Hot Zone and Ecosphere~~		\|location=Any
	\|surface=Molten with High Surface Temperature		\|surface=Molten with High Surface Temperature
	\|atmosphere=Hydrogen Compounds		\|atmosphere=Hydrogen Compounds
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	Class E planets represent the earliest stage in the evolution of a habitable planet. The core and crust is completely molten, making the planets susceptible to solar winds and radiation and subject to extremely high surface temperatures. The atmosphere is very thin, composed of hydrogen and helium. If the world has formed in the ecosphere of a star system, as the planet cools it will develop into a Class F world and continue its evolution to potentially become a life sustaining world. This is true of the majority of Class E worlds.		Class E planets represent the earliest stage in the evolution of a habitable planet. The core and crust is completely molten, making the planets susceptible to solar winds and radiation and subject to extremely high surface temperatures. The atmosphere is very thin, composed of hydrogen and helium. If the world has formed in the ecosphere of a star system, as the planet cools it will develop into a Class F world and continue its evolution to potentially become a life sustaining world. This is true of the majority of Class E worlds.

	~~In some cases the~~ Class E world ~~forms~~ too close to its parent star and within the Hot Zone. The planet then takes a different path, it never develops into a Class F world and eventually cools to become a Class C world. As geological activity slows to a halt, its thin atmosphere begins to either dissipate (either burned away by the heat of the star or drawn away by gravitational forces). These hot Class E worlds continue to be classified as Class E until geological activity ceases, the atmospheres are gone, and they become Class C.		A Class E world can also form too close to its parent star and within the Hot Zone. The planet then takes a different path, it never develops into a Class F world and eventually cools to become a Class C world. As geological activity slows to a halt, its thin atmosphere begins to either dissipate (either burned away by the heat of the star or drawn away by gravitational forces). These hot Class E worlds continue to be classified as Class E until geological activity ceases, the atmospheres are gone, and they become Class C.

			Finally, a Class E planet can develop just outside of a star's habitable zone in the cold zone. Such formations have a similar trajectory as their more common counterparts with the ecosphere of a star. The Class E world cools into a cold Class F world on a trajectory to becoming a Class P world. If such a world is too far outside of the ecosphere of a star, it dies as the geological heat dies and will eventually develop into a dead Class C world losing its atmosphere to condensation and eventual freezing of hydrocarbons in the atmosphere or lighter elemental gasses such as hydrogen and helium eventually bleed away into space.

	{{Planet Class		{{Planet Class
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	\|age=1-3 Billion Years		\|age=1-3 Billion Years
	\|radius=5,000 to 7,500 km		\|radius=5,000 to 7,500 km
	\|location=Ecosphere		\|location=Ecosphere or Cold Zone
	\|surface=Volcanic and Barren		\|surface=Volcanic and Barren
	\|atmosphere=Carbon Dioxide, Ammonia, Methane		\|atmosphere=Carbon Dioxide, Ammonia, Methane
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	}}		}}
	A Class E planet makes the transition to Class F once the crust and core have begun to harden. Volcanic activity is also commonplace on Class F worlds; the steam expelled from volcanic eruptions eventually condenses into water, giving rise to shallow seas in which simple bacteria thrive. When the planet's core is sufficiently cool, the volcanic activity ceases and the planet is considered Class G. Examples include Janus IV.		A Class E planet makes the transition to Class F once the crust and core have begun to harden. Volcanic activity is also commonplace on Class F worlds; the steam expelled from volcanic eruptions eventually condenses into water, giving rise to shallow seas in which simple bacteria thrive. When the planet's core is sufficiently cool, the volcanic activity ceases and the planet is considered Class G. Examples include Janus IV.

			When the world forms just inside the cold zone of a star, the planet's condensing water begins to form a layer of protective ice. The interior is kept warm and simple bacteria can still develop, transforming the atmosphere far more slowly than a world found in the ecosphere. Instead of developing into a Class G world, it will develop into a frozen glaciated Class P world with minimal simple life forms.

	{{Planet Class		{{Planet Class
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	{{Planet Class		{{Planet Class
	\|class=P / Glaciated		\|class=P / Glaciated
	\|location=Ecosphere, Cold Zone		\|location=Ecosphere and Cold Zone
	\|atmosphere=Oxygen, Nitrogen, Argon		\|atmosphere=Oxygen, Nitrogen, Argon
	\|surface=Cold, Glaciated		\|surface=Cold, Glaciated
	\|composition=Silicon, Iron, Magnesium, Ice		\|composition=Silicon, Iron, Magnesium, Ice
	\|hab=Cold-Resistant Vegetation, Animal, and Humanoid		\|hab=Varied; Cold-Resistant Vegetation, Animal, and Humanoid / Bioluminescent Single-Celled Organisms / Possibly None
	\|age=3-10 Billion Years		\|age=3-10 Billion Years
	\|radius=5,000 to 7,500 km		\|radius=5,000 to 7,500 km
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	}}		}}
	On the distant edge of a star system's ecosphere, habitable planets are still numerous, but they are a far cry from the lush garden worlds closer in. Cold, barren, and glaciated planet is covered in solid ice, and while many possess narrow stripes of green along the equator, where hearty plant and animal life may flourish, many glaciated worlds are entirely frozen. Despite the harsh conditions, humanoid life can thrive on a glaciated world. Any planet whose surface is more than 80% frozen is considered Class P. These glaciated worlds are typically very cold, with temperatures rarely exceeding the freezing point. Though not prime conditions for life, hearty plants and animals are not uncommon, and some species, such as the Aenar and the Andorians, have evolved on Class P worlds. Examples include Andorra and Rita Penthe.		On the distant edge of a star system's ecosphere, habitable planets are still numerous, but they are a far cry from the lush garden worlds closer in. Cold, barren, and glaciated planet is covered in solid ice, and while many possess narrow stripes of green along the equator, where hearty plant and animal life may flourish, many glaciated worlds are entirely frozen. Despite the harsh conditions, humanoid life can thrive on a glaciated world. Any planet whose surface is more than 80% frozen is considered Class P. These glaciated worlds are typically very cold, with temperatures rarely exceeding the freezing point. Though not prime conditions for life, hearty plants and animals are not uncommon, and some species, such as the Aenar and the Andorians, have evolved on Class P worlds. Examples include Andorra and Rita Penthe.

			When a Class P world forms in the ecosphere of a star, they tend to develop some kind of cold-resistant life forms which can develop when the planet is still kept warm by geological activity rather than the sun. In such cases bioluminescent bacteria and other single-celled organisms can stay alive deep within the planet where geological heat maintains a layer of liquid water. Eventually when the planet cools sufficiently the layer of liquid water freezes and the world effectively dies. Worlds of this type typically hold onto their atmosphere with heavier diatomic elements like Oxygen and Nitrogen and will build up thick layers of permafrost. Such worlds have the potential to be terraformed, if the ice was to thaw many single-celled bacteria and similar life forms may revive and propagate.

	{{Planet Class		{{Planet Class

Cyclops at 23:00, 30 December 2021

2021-12-30T23:00:30Z

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	These dead worlds can appear anywhere in a star system, most Class A and B worlds eventually cool to become Class C. Other worlds such as Class E worlds that evolve too close to their parent star will eventually cool into Class C, losing their atmosphere to the stars heat or gravitational pull. The key feature of a Class C is the lack of any geological activity whatsoever and no atmosphere. These worlds are rocky and barren worlds which can exist in any zone of a star system, their surface temperature largely depends on the zone which they reside, generally speaking it runs between -150 to -120 degree's Celsius since most are located far enough away from the central star to absorb enough heat to bake the surface. However, it is possible for these planets to be close enough to the central star to have surface temperatures much higher, though generally below that of a Class B world.		These dead worlds can appear anywhere in a star system, most Class A and B worlds eventually cool to become Class C. Other worlds such as Class E worlds that evolve too close to their parent star will eventually cool into Class C, losing their atmosphere to the stars heat or gravitational pull. The key feature of a Class C is the lack of any geological activity whatsoever and no atmosphere. These worlds are rocky and barren worlds which can exist in any zone of a star system, their surface temperature largely depends on the zone which they reside, generally speaking it runs between -150 to -120 degree's Celsius since most are located far enough away from the central star to absorb enough heat to bake the surface. However, it is possible for these planets to be close enough to the central star to have surface temperatures much higher, though generally below that of a Class B world.

	Class E typically do not cool to Class C unless they are too close to the star to retain an atmosphere~~. If a Class G world is too hot and too close to its parent star, it can evolve into a Class C as the planet cools~~. Without volcanic outgassing the atmosphere will burn away leaving a geologically dead world with no atmosphere. Such evolutions are more rare than the smaller variations which evolve from Class A and B worlds.		Class E typically do not cool to Class C unless they are too close to the star to retain an atmosphere. Without volcanic outgassing the atmosphere will burn away leaving a geologically dead world with no atmosphere. Such evolutions are more rare than the smaller variations which evolve from Class A and B worlds.

	These worlds are often rich in minerals and make incredibly good candidates for mining operations. Some can even have semi-molten iron cores with rich deposits of minerals produced either by steady impact of meteorites during the early phases of their existence (usually these worlds begin as Class A worlds or similar and then become more inactive as they cool over several billion years). Examples include Psi 2000.		These worlds are often rich in minerals and make incredibly good candidates for mining operations. Some can even have semi-molten iron cores with rich deposits of minerals produced either by steady impact of meteorites during the early phases of their existence (usually these worlds begin as Class A worlds or similar and then become more inactive as they cool over several billion years). Examples include Psi 2000.

Cyclops at 22:58, 30 December 2021

2021-12-30T22:58:56Z

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	\|radius=500 to 7,500 km		\|radius=500 to 7,500 km
	}}		}}
	~~When all volcanic activity on~~ a Class A ~~planet ceases, it is considered~~ Class C. ~~Essentially dead, these small~~ worlds ~~have cold~~, ~~barren surfaces~~ and ~~possess~~ no ~~geological activity~~. These worlds are rocky and barren worlds which can exist in any zone of a star system, their surface temperature largely depends on the zone which they reside, generally speaking it runs between -150 to -120 degree's Celsius since most are located far enough away from the central star to absorb enough heat to bake the surface. However, it is possible for these planets to be close enough to the central star to have surface temperatures much higher, though generally below that of a Class B world. ~~They tend to run smaller than~~ a Class M world, ~~with sizes ranging from that of moons up to just~~ a ~~bit smaller than an M~~ Class ~~world~~. ~~The primary classification of this class is~~ the ~~lack of an~~ atmosphere, no ~~geological activity,~~ and ~~the lack of any ability to support life~~.		These dead worlds can appear anywhere in a star system, most Class A and B worlds eventually cool to become Class C. Other worlds such as Class E worlds that evolve too close to their parent star will eventually cool into Class C, losing their atmosphere to the stars heat or gravitational pull. The key feature of a Class C is the lack of any geological activity whatsoever and no atmosphere. These worlds are rocky and barren worlds which can exist in any zone of a star system, their surface temperature largely depends on the zone which they reside, generally speaking it runs between -150 to -120 degree's Celsius since most are located far enough away from the central star to absorb enough heat to bake the surface. However, it is possible for these planets to be close enough to the central star to have surface temperatures much higher, though generally below that of a Class B world.

			Class E typically do not cool to Class C unless they are too close to the star to retain an atmosphere. If a Class G world is too hot and too close to its parent star, it can evolve into a Class C as the planet cools. Without volcanic outgassing the atmosphere will burn away leaving a geologically dead world with no atmosphere. Such evolutions are more rare than the smaller variations which evolve from Class A and B worlds.

	These worlds are often rich in minerals and make incredibly good candidates for mining operations. Some can even have semi-molten iron cores with rich deposits of minerals produced either by steady impact of meteorites during the early phases of their existence (usually these worlds begin as Class A worlds or similar and then become more inactive as they cool over several billion years). Examples include Psi 2000.		These worlds are often rich in minerals and make incredibly good candidates for mining operations. Some can even have semi-molten iron cores with rich deposits of minerals produced either by steady impact of meteorites during the early phases of their existence (usually these worlds begin as Class A worlds or similar and then become more inactive as they cool over several billion years). Examples include Psi 2000.
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	\|age=2-10 Billion Years		\|age=2-10 Billion Years
	\|radius=5,000 to 7,500 km		\|radius=5,000 to 7,500 km
	\|location=Ecosphere		\|location=Hot Zone and Ecosphere
	\|surface=Molten with High Surface Temperature		\|surface=Molten with High Surface Temperature
	\|atmosphere=Hydrogen Compounds		\|atmosphere=Hydrogen Compounds
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	\|composition=Silicone, Iron, Magnesium, Aluminum		\|composition=Silicone, Iron, Magnesium, Aluminum
	}}		}}
	Class E planets represent the earliest stage in the evolution of a habitable planet. The core and crust is completely molten, making the planets susceptible to solar winds and radiation and subject to extremely high surface temperatures. The atmosphere is very thin, composed of hydrogen and helium. As the ~~surface cools~~, the ~~core~~ and ~~crust begin~~ to ~~harden,~~ and the planet ~~evolves~~ into a Class F world.		Class E planets represent the earliest stage in the evolution of a habitable planet. The core and crust is completely molten, making the planets susceptible to solar winds and radiation and subject to extremely high surface temperatures. The atmosphere is very thin, composed of hydrogen and helium. If the world has formed in the ecosphere of a star system, as the planet cools it will develop into a Class F world and continue its evolution to potentially become a life sustaining world. This is true of the majority of Class E worlds.

			In some cases the Class E world forms too close to its parent star and within the Hot Zone. The planet then takes a different path, it never develops into a Class F world and eventually cools to become a Class C world. As geological activity slows to a halt, its thin atmosphere begins to either dissipate (either burned away by the heat of the star or drawn away by gravitational forces). These hot Class E worlds continue to be classified as Class E until geological activity ceases, the atmospheres are gone, and they become Class C.

	{{Planet Class		{{Planet Class
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	\|composition=Silicone, Iron, Magnesium, Aluminum		\|composition=Silicone, Iron, Magnesium, Aluminum
	}}		}}
	A planet is considered Class H if less than 20% of its surface is water. Though many Class H worlds are covered in sand, it is not required to be considered a desert; it must, however, receive little in the way of precipitation. These worlds are usually between 8,000 and 15,000 km in diameter. Drought-resistant plants and animals are common on Class H worlds, and many are inhabited by humanoid populations. Most Class H worlds are hot and arid, but conditions can vary greatly. Examples include Nimbus III and Ocampa.		A planet is considered Class H if less than 20% of its surface is water. Though many Class H worlds are covered in sand, it is not required to be considered a desert; it must, however, receive little in the way of precipitation. These worlds are usually between 8,000 and 15,000 km in diameter. Drought-resistant plants and animals are common on Class H worlds, and many are inhabited by humanoid populations. Most Class H worlds are hot and arid, but conditions can vary greatly. Examples include Nimbus III and Ocampa.

	{{Planet Class		{{Planet Class

Cyclops at 22:32, 30 December 2021

2021-12-30T22:32:28Z

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	\|type=Rock		\|type=Rock
	\|age=2-10 Billion Years		\|age=2-10 Billion Years
	\|radius=500 to 5,~~000~~ km		\|radius=500 to 7,500 km
	}}		}}
	When all volcanic activity on a Class A planet ceases, it is considered Class C. Essentially dead, these small worlds have cold, barren surfaces and possess no geological activity. These worlds are rocky and barren worlds which can exist in any zone of a star system, their surface temperature largely depends on the zone which they reside, generally speaking it runs between -150 to -120 degree's Celsius since most are located far enough away from the central star to absorb enough heat to bake the surface. However, it is possible for these planets to be close enough to the central star to have surface temperatures much higher, though generally below that of a Class B world. They tend to run smaller than a Class M world, with sizes ranging from that of moons up to just a bit smaller than an M Class world. The primary classification of this class is the lack of an atmosphere, no geological activity, and the lack of any ability to support life.		When all volcanic activity on a Class A planet ceases, it is considered Class C. Essentially dead, these small worlds have cold, barren surfaces and possess no geological activity. These worlds are rocky and barren worlds which can exist in any zone of a star system, their surface temperature largely depends on the zone which they reside, generally speaking it runs between -150 to -120 degree's Celsius since most are located far enough away from the central star to absorb enough heat to bake the surface. However, it is possible for these planets to be close enough to the central star to have surface temperatures much higher, though generally below that of a Class B world. They tend to run smaller than a Class M world, with sizes ranging from that of moons up to just a bit smaller than an M Class world. The primary classification of this class is the lack of an atmosphere, no geological activity, and the lack of any ability to support life.

Cyclops at 22:03, 29 December 2021

2021-12-29T22:03:50Z

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	Such planets are classified as ''Class I3'', ''Ejected Class I'', or ''Rogue Class I''.		Such planets are classified as ''Class I3'', ''Ejected Class I'', or ''Rogue Class I''.

	=== 4 / Artificial Ocean ===		=== 4 / Large / Heavy ===
			Applicable to nearly any rock type world, class A, B, C, D, E, F, G, H, K, L, M, N, O, P, Q, and Y.

			Some planets do not exactly fit into an existing classification. This subclass specifically identifies a planet as being otherwise fitting with an existing classification but otherwise too large or too heavy to be classified as such. For these class worlds the planet fits all categories except size / mass. Such worlds are not rare, this subclass is mostly for precise cataloguing purposes. Although can be referred too explicitly to differentiate with other classifications, especially when other planets in the system share the same class but fit within size / mass guidelines. These worlds often have thicker atmospheres and higher gravity than their more common contemporaries. This classification is not terribly uncommon, though tends to not be into the more ideal Class M or O but instead tend toward Class N. Class H, K, L, or P are also somewhat common.

			Examples include; ''Class E4'', ''Heavy Class E'', or ''Large Class E''.

			=== 5 / Small / Light ===
			Applicable to nearly any rock type world, class A, B, C, D, E, F, G, H, K, L, M, N, O, P, Q, and Y.

			Some planets do not exactly fit into an existing classification. This subclass specifically identifies a planet as being otherwise fitting with an existing classification but otherwise too small or too light to be classified as such. For these class worlds the planet fits all categories except size / mass. Such worlds are not rare, this subclass is mostly for precise cataloguing purposes. Although can be referred too explicitly to differentiate with other classifications, especially when other planets in the system share the same class but fit within size / mass guidelines. These worlds often have thinner atmospheres and lower gravity than their more common contemporaries. In contrast to a subclass 4 world, many of these planets do not reach Class M or O status tending more toward Class H, K, L, N, or P. This is primarily due to the gravitational pull of the world being too small for the thicker atmosphere required for a Class M / O. These planets are more rare than their larger cousins unless they have an unusually dense core which can hold onto more atmosphere and water.

			Examples include; ''Class L5'', ''Light Class L'', or ''Small Class L''. While occasionally the term ''Dwarf'' is used in colloquial terms, it is not considered an official designation to avoid confusion with ''Class D''.

			=== 6 / Artificial Ocean ===
	Applicable to only Class O worlds.		Applicable to only Class O worlds.

	This is a specific type of classification. Class O worlds require greater than 80% of the surface be made of water, even with worlds that have 100% water coverage there is still a dense molten rock core which creates the gravitational field to maintain an atmosphere and pressure for liquid water. With a subtype of 4 this is not the case. Also called a ''Class O4'' or ''Artificial Class O'' these are worlds that are not naturally occurring. Such "Ocean Worlds" are held together not by gravity but by a containment field generated at their core and is otherwise entirely made of water. As such the age, size, and evolutionary history of the world do not conform to most known standards. The size will be entirely dependent on the size of the containment field, though even if life is seeded in this artificial ocean world it will have a unique evolutionary path, just like any planet.		This is a specific type of classification. Class O worlds require greater than 80% of the surface be made of water, even with worlds that have 100% water coverage there is still a dense molten rock core which creates the gravitational field to maintain an atmosphere and pressure for liquid water. With a subtype of 4 this is not the case. Also called a ''Class O6'' or ''Artificial Class O'' these are worlds that are not naturally occurring. Such "Ocean Worlds" are held together not by gravity but by a containment field generated at their core and is otherwise entirely made of water. As such the age, size, and evolutionary history of the world do not conform to most known standards. The size will be entirely dependent on the size of the containment field, though even if life is seeded in this artificial ocean world it will have a unique evolutionary path, just like any planet.

	Only one such world has ever been located, called ''The Waters'' by the Monean in the Delta Quadrant.		Only one such world has ever been located, called ''The Waters'' by the Monean in the Delta Quadrant.

	[[Category:Blazing Umbra]]		[[Category:Blazing Umbra]]

Cyclops at 02:58, 27 December 2021

2021-12-27T02:58:54Z

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	\|type=Rock		\|type=Rock
	}}		}}
	These rare planetoids typically develop with a highly eccentric orbit, or near stars with a variable output. As such, conditions on the planet's surface are widely varied. Deserts and [[rain]] forests exist within a few kilometers of each other, while glaciers can simultaneously lie very near the equator. Given the constant instability, is virtually impossible for life to exist on Class-Q worlds. Examples include the Genesis Planet.		These rare planetoids typically develop with a highly eccentric orbit, or near stars with a variable output. As such, conditions on the planet's surface are widely varied. Deserts and rain forests exist within a few kilometers of each other, while glaciers can simultaneously lie very near the equator. Given the constant instability, is virtually impossible for life to exist on Class-Q worlds. Examples include the Genesis Planet.

	{{Planet Class		{{Planet Class