Sigma Corvi asteroid field: Difference between revisions
Jump to navigation
Jump to search
m (added data) |
(No difference)
|
Revision as of 00:00, 1 May 2008
Serellan Sector |
---|
Trinity Sector |
Jenatris Cloud Sector |
(Sector 118 map) |
Territory |
Local Species |
Stellar Phenomenae |
Federation Presence |
|
Sigma Corvi system | Star · Belt |
- they orbit there star at approximately 38 to 573 million km
- over half of the asteroids have abnormal orbits or are rogue'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
- most of these asteroids are S-Type asteroids and have a stony, iron composition
- long range scans show abnormal readings for some of the asteroid debrie, readings are more closely linked with planetary bodies
- see Asteroid Data for more information