Sigma Corvi asteroid field

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Sigma Corvi system Star  · Belt
  • Orbits their star at approximately 38 to 573 million km.
  • Over half of the asteroids have abnormal orbits or are rogue asteroids.
  • Most of the asteroids are S-Type asteroid and have a stony, iron composition.
  • There are C-Type asteroids mixed into the field. These asteroids are dark and not very reflective, with brittle bodies made of fine opaque materials and water-rich minerals.
  • There are also M-Type asteroids mixed in. These asteroids are made of nickel/iron compositions and other rare types of metals. Any of these may have usable amounts of ice on the surface or within them.
  • Long range scans show abnormal readings for some of the asteroid debris; these readings are of a sort that is more often linked with planetary bodies.