Ql'tu Outer Asteroid Belt II: Difference between revisions
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Latest revision as of 15:46, 9 July 2008
Serellan Sector |
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Trinity Sector |
Jenatris Cloud Sector |
(Sector 118 map) |
Territory |
Local Species |
Stellar Phenomenae |
Federation Presence |
|
QI'tu system | Star · Belt I · I · Belt II |
Stats
- they orbit there star at approximately 183 to 203 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
Resources
- unknown at this time, as the only known survey was conducted by the Klingons