Sigma Corvi: Difference between revisions
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The Sigma Corvi star is a [[wp:Supergiant|class IIb]], [[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. | The Sigma Corvi star is a [[wp:Supergiant|class IIb]], [[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]] | |||
Revision as of 04:47, 22 April 2008
The Sigma Corvi star is a class IIb, 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.