Class |
Description |
| Class
A
Gas Supergiant |
Planets
of this class are usually found in a star's outer or "cold zone".
They are typically 140 thousand to 10 million kilometers in
diameter and have high core temperatures causing them to radiate
heat. Low stellar radiation and high planet gravity enables
them to keep a tenuous surface comprised of gaseous hydrogen
and hydrogen compounds. |
| |
| Class
B
Gas Giant |
Class
B Planets are usually found in a star's outer or "cold zone".
They are typically 50 thousand to 140 thousand kilometers in
diameter and have high core temperatures but do not radiate
much heat. Low stellar radiation and high planet gravity enables
them to keep a tenuous surface comprised of gaseous hydrogen
and hydrogen compounds. |
| |
| Class
C
Reducing |
Planets
of this class are usually found in a star's "habitable zone".
They are typically 10 to 15 thousand kilometers in diameter.
They have high surface temperatures due to the "greenhouse effect"
caused by their dense atmospheres. The only water found is in
vapor form. |
| |
| Class
D
Geo-Plastic |
Planets
of this class are usually found in a star's "habitable zone".
They are typically 10,000 to 15,000 kilometers in diameter.
They have a molten surface because they have been recently formed.
The atmosphere contains many hydrogen compounds and reactive
gases. Class D planets eventually cool, becoming Class E. |
| |
| Class
E
Geo-Metalic |
Planets
of this class have a molten core and are usually found in a
star's "habitable zone". They are typically 10,000 to 15,000
kilometers in diameter. Their atmospheres still contain hydrogen
compounds. They will cool further eventually becoming Class
F. |
| |
| Class
F
Geo-Crystaline |
Class
F planets are usually found in a star's "habitable zone". They
are typically 10 to 15 thousand kilometers in diameter and have
surfaces that are still crystalizing. Their atmospheres still
contain some toxic gases. They will cool eventually becoming
Class C, M or N. |
| |
| Class
G
Desert |
Planets
of this class can be found in any of a star's zones. They are
typically 8 to 15 thousand kilometers in diameter. Their surfaces
are usually hot. Their atmospheres contain heavy gases and metal
vapors. |
| |
| Class
H
Geo-Thermal |
Planets
of this class are usually found in a star's "habitable zone"
or "cold zone". They are typically 1,000 to 10,000 kilometers
in diameter. They have partially molten surfaces and atmospheres
that contain many hydrogen compounds. They cool becoming Class
L. |
| |
| Class
I
Asteroid
/ Moon |
Planetary
bodies of this class can be found in any of a star's zones.
They are usually found in orbit of larger planets or in asteroid
fields. They are typically 100 to 1,000 kilometers in diameter.
They have no atmospheres. Their surfaces are barren and cratered. |
| |
| Class
J
Geo-Morteus |
Planets
of this class are found in a star's "hot zone". They are typically
1,000 to 10,000 kilometers in diameter. They have high surface
temperatures due to the proximity to the star. Their atmospheres
are extremely tenuous with few chemically active gases. |
| |
| Class
K
Adaptable |
Planets
of this class are usually found in a star's "habitable zone".
They are adaptable for humanoid colonization through the use
of pressure domes and other life support devices. They are typically
5,000 to 10,000 kilometers in diameter. They have thin atmospheres.
Small amounts of water are present. |
| |
| Class
L
Geo-Inactive |
Planets
of this class are usually found in a star's "habitable zone"
or "cold zone". They are typically 1,000 to 10,000 kilometers
in diameter. Low solar radiation and minimal internal heat usually
result in a frozen atmosphere. |
| |
| Class
M
Terrestrial |
Planets
of this class are found in a star's "habitable zone". They are
typically 10,000 to 15 thousand kilometers in diameter. They
have atmospheres that contain oxygen and nitrogen . Water and
life-forms are typically abundant. If water covers more than
97% of the surface, then they are considered Class N. |
| |
| Class
N
Pelagic |
Class
N planets are usually found in a star's "habitable zone". They
are typically 10,000 to 15 thousand kilometers in diameter.
They have atmospheres that contain oxygen and nitrogen . Water
and life-forms are typically abundant. If water covers less
than 97% of the surface, then they are considered Class M. |
| |
| Class
S
Near
Star |
Planets
of this class are usually found in a star's "cold zone". They
are typically 50 million to 120 million kilometers in diameter
and have high core temperatures causing them to radiate heat
and light. These are the largest possible planets, because most
planetary bodies that reach this size do become stars. |
| |
| Class
T
Gas
Ultragiant |
Planets
of this class are usually found in a star's "cold zone". They
are typically 10 to 50 million kilometers in diameter. They
have high core temperatures causing them to radiate enough heat
to keep water in a liquid state. |
| |
| Class
Y
Demon |
Class
Y - Demon Planets and planetoids of this class can be found
in any of a star's zones. They are typically 10,000 to 15 thousand
kilometers in diameter. Atmospheric conditions are often turbulent
and saturated with poisonous chemicals and thermionic radiation.
Surface temperatures can reach in excess of 500 K. |