Sigma Corvi asteroid field: Difference between revisions
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[[Category:Asteroid belts]] | [[Category:Asteroid belts]] | ||
[[Category:Sigma Corvi system]] | [[Category:Sigma Corvi system]] | ||
[[Category: | [[Category:Jenatris Cloud Sector]] |
Revision as of 05:22, 27 June 2008
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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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