Aries (star): Difference between revisions
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The Aries star is a [[wp:Main sequence|class V main sequence star]], [[wp:Stellar classification#Class M|type M6 (red spectrum)]] with a temerature of 2,000 to 3,500 Kelvin and with a stellar mass of about 0.3 to 0.4 .(in relation to Sol) It has a solar radius of 0.5 and a luminosity of 0.04 with hydrogen lines falling within the very weak rating. | |||
[[Category:Stars]] | |||
[[Category:Main sequence stars]] | |||
[[Category:Aries system]] | |||
Revision as of 13:41, 27 July 2008
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| Kivis Sector |
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| Sigma Dorphus Sector |
| Free Haven Sector |
| Territory |
| Local Species |
| Stellar Phenomenae |
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| Aries system | Star · I · II · III · IV · V · Belt · VI |
The Aries star is a class V main sequence star, type M6 (red spectrum) with a temerature of 2,000 to 3,500 Kelvin and with a stellar mass of about 0.3 to 0.4 .(in relation to Sol) It has a solar radius of 0.5 and a luminosity of 0.04 with hydrogen lines falling within the very weak rating.