Gamma Taboa outer asteroid belt: Difference between revisions
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(New page: {{Trinity}} {{Gamma Taboa}} *they orbit there star at approximately 392 to 438 million km *there are C-Type asteroids mixed in with the majority of S=type asteroids. These asteroids are ...) |
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|style="width:11.0em;"| '''[[Gamma Taboa system]]''' | |||
| [[Gamma Taboa (star)|Star]] '''·''' [[Gamma Taboa inner asteroid belt|Belt I]] '''·''' [[Gamma Taboa|I]] '''·''' [[Gamma Taboa outer asteroid belt|Belt II]] | |||
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*they orbit there star at approximately 392 to 438 million km | *they orbit there star at approximately 392 to 438 million km | ||
Revision as of 01:43, 17 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 392 to 438 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