Sigma Corvi asteroid field: Difference between revisions

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Sigma Corvi asteroid field (view source)

Revision as of 20:16, 9 September 2016

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grammar fixes, adjusted phrasing.

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 {{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:Sigma Corvi system]]
 [[Category:Jenatris Cloud Sector]]