Planet Classification: Difference between revisions

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|surface=Barren / Molten in Places
|surface=Barren / Molten in Places
|composition=Iron / Potassium / Silicon
|composition=Iron / Potassium / Silicon
|habitability=None
|habitability=None}}


Class B planets are generally very small, very rocky worlds located within a star system's hot zone. In the harsh daylight, these planets are scorched by their parent star, often to the point of rock becoming molten. Because Class B worlds have little to no atmosphere, this heat quickly radiates away at night, leaving the dark side of the planet a frigid wasteland. As a result, these planets are highly unsuitable for humanoid life.
Class B planets are generally very small, very rocky worlds located within a star system's hot zone. In the harsh daylight, these planets are scorched by their parent star, often to the point of rock becoming molten. Because Class B worlds have little to no atmosphere, this heat quickly radiates away at night, leaving the dark side of the planet a frigid wasteland. As a result, these planets are highly unsuitable for humanoid life.
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Class B planets are fairly common in the universe.
Class B planets are fairly common in the universe.
== Class M ==
{{Planet Class
|location=Ecosphere
|atmosphere=Oxygen, Nitrogen, Argon
|surface=Abundant Surface Water, Temperate Climate
|composition=Silicone, Iron, Magnesium, Aluminium
|habitability=Prime conditions for large populations of animal, planet, and humanoid life.
}}
These planets are robust and varied worlds composed primarily of silicate rocks. Located in a star system's habitable zone, most are temperate worlds with vast blue oceans and wide swaths of verdant forest. However, conditions can vary greatly between worlds and still be considered Class M; as long as the surface is between 20 and 80 percent water, the climate is generally temperate, and the atmosphere made of oxygen and nitrogen, even dry rocky worlds and cold snowy planets can be Class M.
== Class P ==
{{Planet Class
|location=Ecosphere, Cold Zone
|atmosphere=Oxygen, Nitrogen, Argon
|surface=Cold, Glaciated
|composition=Silicon, Iron, Magnesium, Ice
|habitability=Hearty flora and fauna capable of withstanding extreme cold.
}}
}}
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 and barren, more than eighty percent of a Class P: 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.


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

Revision as of 20:16, 8 November 2017

Planets are classified according to their predominant properties. While there is, at times, overlap in some of the classifications the primary classification of a planet assists travelers through space in identifying the primary characteristics of a planet more easily.

Class A

Type: Unknown
Age: Unknown
Atmosphere: Sulfer Dioxide / Carbon Dioxide
Radius: Unknown
Surface: Rocky / Partially Molten
Composition: Igneous Silica / Basalt
Location: Any
Habitability: Unknown

These planets are generally young, rocky worlds that are rife with volcanic activity. This volcanic activity spews vast amounts of sulfur and carbon dioxide into the atmosphere, causing a greenhouse effect that keeps temperatures relatively hot. Such worlds have tenuous and toxic atmospheres and are unsuitable to any kind of life.

When this extreme volcanic activity eventually ceases, the planet "dies" and becomes a Class C world.

Class A planets are common in the universe; Jupiter's moon Io is a prime example.

Class B

Type: Unknown
Age: Unknown
Atmosphere: Oxygen / Sodium / Hydrogen
Radius: Unknown
Surface: Barren / Molten in Places
Composition: Iron / Potassium / Silicon
Location: Hot Zone
Habitability: Unknown

Class B planets are generally very small, very rocky worlds located within a star system's hot zone. In the harsh daylight, these planets are scorched by their parent star, often to the point of rock becoming molten. Because Class B worlds have little to no atmosphere, this heat quickly radiates away at night, leaving the dark side of the planet a frigid wasteland. As a result, these planets are highly unsuitable for humanoid life.

Despite their small size, Class B planets are often extremely dense, with a large inner core, up to 55% of the planet's volume, that is made of molten iron.

Class B planets are fairly common in the universe.

Class M

Type: Unknown
Age: Unknown
Atmosphere: Oxygen, Nitrogen, Argon
Radius: Unknown
Surface: Abundant Surface Water, Temperate Climate
Composition: Silicone, Iron, Magnesium, Aluminium
Location: Ecosphere
Habitability: Unknown

These planets are robust and varied worlds composed primarily of silicate rocks. Located in a star system's habitable zone, most are temperate worlds with vast blue oceans and wide swaths of verdant forest. However, conditions can vary greatly between worlds and still be considered Class M; as long as the surface is between 20 and 80 percent water, the climate is generally temperate, and the atmosphere made of oxygen and nitrogen, even dry rocky worlds and cold snowy planets can be Class M.

Class P

Type: Unknown
Age: Unknown
Atmosphere: Oxygen, Nitrogen, Argon
Radius: Unknown
Surface: Cold, Glaciated
Composition: Silicon, Iron, Magnesium, Ice
Location: Ecosphere, Cold Zone
Habitability: Unknown

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 and barren, more than eighty percent of a Class P: 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.