Gamma Taboa inner asteroid belt: Difference between revisions
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*see [[wp:Asteroid|Asteroid Data]] for more information | *see [[wp:Asteroid|Asteroid Data]] for more information | ||
[[Category: | [[Category:Asteroid belts]] | ||
[[Category:Gamma Taboa system]] | [[Category:Gamma Taboa system]] | ||
[[Category:Trinity Sector]] | [[Category:Trinity Sector]] | ||
Latest revision as of 12:25, 30 April 2008
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| 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