Heth-Gimel Inner Asteroid Belt: Difference between revisions
m (adding Template) |
mNo edit summary |
||
| (One intermediate revision by the same user not shown) | |||
| Line 1: | Line 1: | ||
{{Sigma Dorphus Sector}} | {{Sigma Dorphus Sector}} | ||
{{Heth-Gimel}} | {{Heth-Gimel}} | ||
*they orbit there star at approximately 284 to 293 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 [[wp:Asteroid|Asteroid Data]] for more information | |||
[[Category:Asteroid belts]] | |||
[[Category:Heth-Gimel system]] | |||
Latest revision as of 16:55, 19 October 2008
|
| Kivis Sector |
|---|
| Sigma Dorphus Sector |
| Free Haven Sector |
| Territory |
| Local Species |
| Stellar Phenomenae |
| Federation Presence |
|
| Heth-Gimel system | Star I · Star II · Star III · Belt I · I · Belt II |
- they orbit there star at approximately 284 to 293 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