Kaph-Nun Asteroid Belt: Difference between revisions
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*they orbit there star at approximately | *they orbit there star at approximately 136 to 141 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 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 | ||
Revision as of 02:41, 30 October 2008
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| Kivis Sector |
|---|
| Sigma Dorphus Sector |
| Free Haven Sector |
| Territory |
| Local Species |
| Stellar Phenomenae |
| Federation Presence |
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| Kaph-Nun system | Star · I · II · Belt · III · IV |
- they orbit there star at approximately 136 to 141 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