Sigma Corvi: Difference between revisions
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{{Sigma Corvi}} | {{Sigma Corvi}} | ||
The Sigma Corvi star is a [[wp:Supergiant|class | 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:Stars]] | ||
[[Category:Sigma Corvi system]] | [[Category:Sigma Corvi system]] | ||
Revision as of 05:22, 22 April 2008
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| Serellan Sector |
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| Trinity Sector |
| Jenatris Cloud Sector |
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| Territory |
| Local Species |
| Stellar Phenomenae |
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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.