Sigma Corvi asteroid field: Difference between revisions

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


*they orbit there star at approximately 38 to 573 million km  
*Orbits their star at approximately 38 to 573 million km.
*over half of the asteroids have abnormal orbits or are rogue's
*Over half of the asteroids have abnormal orbits or are rogue asteroids.
*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
*Most of the asteroids are S-Type asteroid and have a stony, iron composition.
*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
*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.
*most of these asteroids are S-Type asteroids and have a stony, iron composition
*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 debrie, readings are more closely linked with planetary bodies
*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.
*see [[wp:Asteroid|Asteroid Data]] for more information


[[Category:Asteroid belts]]
[[Category:Asteroid belts]]
[[Category:Sigma Corvi system]]
[[Category:Sigma Corvi system]]
[[Category:Jenatris Cloud Sector]]
[[Category:Jenatris Cloud Sector]]

Latest revision as of 20:16, 9 September 2016

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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.