Gamma Taboa inner asteroid belt: Difference between revisions
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*they orbit there star at approximately 238 to 273 million km | *they orbit there star at approximately 238 to 273 million km |
Revision as of 01:50, 17 April 2008
Serellan Sector |
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Trinity Sector |
Jenatris Cloud Sector |
(Sector 118 map) |
Territory |
Local Species |
Stellar Phenomenae |
Federation Presence |
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Gamma Taboa system | Star ·Belt I · I · Belt II |
- they orbit there star at approximately 238 to 273 million km
- there are C-Type asteroids mixed in with the majority of S=type asteroids. These asteroids are dark, low reflective, with brittle bodies made of fine opaque material and hydrated (water-rich) minerals
- there are M-Type asteroids mixed in with the majority of S-type asteroids. These asteroids have nickel/iron compositions and other rare types of metals. Any of these may have useable amounts of ice on the surface or within them
- most of these asteroids are S-Type asteroids and have a stony, iron composition
- see Asteroid Data for more information