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Sigma Corvi asteroid field: Difference between revisions
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{{Sigma Corvi}} | {{Sigma Corvi}} | ||
* | *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. | |||
[[Category:Asteroid belts]] | [[Category:Asteroid belts]] | ||
[[Category:Sigma Corvi system]] | [[Category:Sigma Corvi system]] | ||
[[Category:Jenatris Cloud Sector]] | [[Category:Jenatris Cloud Sector]] | ||