Veqlargh Bal (star): Difference between revisions
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{{Veqlargh Bal}} | {{Veqlargh Bal}} | ||
The Veqlargh Bal | The Veqlargh Bal 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 about 0.5, a luminosity of 0.04L and hydrogen lines falling in the very weak range. | ||
[[Category:Stars]] | [[Category:Stars]] | ||
[[Category:Veqlargh Bal system]] | [[Category:Veqlargh Bal system]] | ||
[[Category:Trinity Sector]] | [[Category:Trinity Sector]] | ||
Latest revision as of 03:44, 1 May 2008
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| Serellan Sector |
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| Trinity Sector |
| Jenatris Cloud Sector |
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| Territory |
| Local Species |
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| Veqlargh Bal system | Star · I · II · III · IV · V |
The Veqlargh Bal 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 about 0.5, a luminosity of 0.04L and hydrogen lines falling in the very weak range.