Planetary Classes: Difference between revisions
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=<h2><center>Planet classes and their particular properties</center></h2>= | =<h2><center>Planet classes and their particular properties</center></h2>= |
Revision as of 07:58, 30 January 2010
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Planet classes and their particular properties
A-Class Planet
B-Class Planet
C-Class Planet
D-Class Planet
Class E Planets are the same size as Earth. They are recently formed, having been Class D, with a very thin crust. They will cool to Class F, and they still have Hydrogen left in the atmosphere. |
E-Class Planet
Class E Planets are the same size as Earth. They are recently formed, having been Class D, with a very thin crust. They will cool to Class F, and they still have Hydrogen left in the atmosphere. |
F-Class Planet
G-Class Planet
H-Class Planet
Smaller than earth (about 1 to 1/10 the size of Earth), Class H Planets are newly formed, with Hydrogen atmospheres . They are located in the Suns Cold Zone, and will cool to Class L Planets. |
I-Class Planet
Tiny planets, 1/100 the size of Earth or less, Class I Planets are generally lifeless. They have no atmosphere due to the low gravity, and consequently are very cratered. |
J-Class Planet
K-Class Planet
Although small (1/10 Earth), Class K Planets, located in the Suns Habitable Zone, do have water despite their weak atmosphere. |
L-Class Planet
M-Class Planet (Terra)
N-Class Planet
S-Class Planet
For additional information see: Star Classes, Star Structure
T-Class Planet
Class T Planets are Gas Super Giants, about 3,000 times the size of Earth. They are located in the Suns Cold Zone, and have a thick atmosphere. Water is present on Class T Planets. |
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