Sigma Corvi: Difference between revisions
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The Sigma Corvi star is a [[wp:Supergiant|class | {{Jenatris Cloud}} | ||
{{Sigma Corvi}} | |||
The Sigma Corvi star is a [[wp:Supergiant|class Ib]], [[wp:Stellar classification#Class O|type O (blue spectrum)]] with a temperature between 30,000 and 60,000 Kelvin with a stellar mass of about 60 to 64. (in relation to Sol) It has a solar radius of 16 and a luminosity of 1,400,000L with very weak hydrogen lines. | |||
[[Category:Stars]] | |||
[[Category:Sigma Corvi system]] | |||
[[Category:Jenatris Cloud Sector]] | |||
Latest revision as of 15:19, 9 July 2008
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| Serellan Sector |
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| Trinity Sector |
| Jenatris Cloud Sector |
| (Sector 118 map) |
| Territory |
| Local Species |
| Stellar Phenomenae |
| Federation Presence |
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| Sigma Corvi system | Star · Belt |
The Sigma Corvi star is a class Ib, type O (blue spectrum) with a temperature between 30,000 and 60,000 Kelvin with a stellar mass of about 60 to 64. (in relation to Sol) It has a solar radius of 16 and a luminosity of 1,400,000L with very weak hydrogen lines.