Rumaiy (star): Difference between revisions
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{{ | {{Promell Sector}} | ||
{{Rumaiy}} | {{Rumaiy}} | ||
The Rumaiy star is a [[wp:Main sequence|class V main sequence star]], [[wp:Stellar classification#Class M|type M9 (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 about 0.5, a luminosity of 0.04L and hydrogen lines falling in the very weak range. | The Rumaiy star is a [[wp:Main sequence|class V main sequence star]], [[wp:Stellar classification#Class M|type M9 (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 about 0.5, a luminosity of 0.04L and hydrogen lines falling in the very weak range. | ||
Latest revision as of 22:16, 30 July 2008
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| Alrakis Sector |
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| Promell Sector |
| Gavaria Sector |
| Territory |
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| Local Species |
| Stellar Phenomenae |
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| Federation Presence |
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| Rumaiy system | Star · Belt I · I · II · Belt II · III · IV · Belt III · V |
The Rumaiy star is a class V main sequence star, type M9 (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 about 0.5, a luminosity of 0.04L and hydrogen lines falling in the very weak range.