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Heth-Gimel Outer Asteroid Belt: Difference between revisions
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Heth-Gimel Outer Asteroid Belt (view source)
Revision as of 16:56, 19 October 2008
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{{Sigma Dorphus Sector}} | {{Sigma Dorphus Sector}} | ||
{{Heth-Gimel}} | {{Heth-Gimel}} | ||
*they orbit there star at approximately | *they orbit there star at approximately 543 to 549 million km | ||
*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 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 | *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 | ||
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[[Category:Asteroid belts]] | [[Category:Asteroid belts]] | ||
[[Category:Heth-Gimel system]] | |||