Gamma Taboa outer asteroid belt: Difference between revisions

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{{Trinity}}
{{Trinity}}
{| id="toc" class="toc"
{{Gamma Taboa system}}
|style="width:11.0em;"| '''[[Gamma Taboa system]]'''
| [[Gamma Taboa (star)|Star]]  '''·''' [[Gamma Taboa inner asteroid belt|Belt I]]  '''·''' [[Gamma Taboa|I]]  '''·''' [[Gamma Taboa outer asteroid belt|Belt II]]
|}
 


*they orbit there star at approximately 392 to 438 million km  
*they orbit there star at approximately 392 to 438 million km  

Revision as of 01:51, 17 April 2008

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Gamma Taboa system Star  ·Belt I  · I  · Belt II
  • they orbit there star at approximately 392 to 438 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 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
  • most of these asteroids are S-Type asteroids and have a stony, iron composition
  • see Asteroid Data for more information