Sigma Corvi asteroid field: Difference between revisions

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{{Trinity}}
{{Jenatris Cloud}}
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{{Sigma Corvi}}



Revision as of 15:19, 9 July 2008

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Serellan Sector
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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