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 | ||
*there are C-Type asteroids mixed in with the majority of S | *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 | *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 | *most of these asteroids are S-Type asteroids and have a stony, iron composition | ||
Revision as of 01:57, 17 April 2008
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| Serellan Sector |
|---|
| 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