Zeta Pictoris (star): Difference between revisions
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{{Zeta Pictoris | {{Zeta Pictoris}} | ||
The Zeta Pictoris star is a [[wp:Subgiant|class IV Subgiant star]], [[wp:Stellar classification#Class A|type A6 (white spectrum)]] with an average temperature of between 7,500 to 10,000 Kelvin and with a stellar mass of about 3.1 to 4.0 (in relation to Sol) It has a solar radius of 2.1 and a luminosity of 40L with hydrogen lines falling within the strong range. | The Zeta Pictoris star is a [[wp:Subgiant|class IV Subgiant star]], [[wp:Stellar classification#Class A|type A6 (white spectrum)]] with an average temperature of between 7,500 to 10,000 Kelvin and with a stellar mass of about 3.1 to 4.0 (in relation to Sol) It has a solar radius of 2.1 and a luminosity of 40L with hydrogen lines falling within the strong range. | ||
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[[Category:Stars]] | [[Category:Stars]] | ||
[[Category:Giants]] | [[Category:Giants]] | ||
[[Category:Zeta Pictoris | [[Category:Zeta Pictoris system|*]] | ||
[[Category:Trinity Sector]] | [[Category:Trinity Sector]] | ||
Latest revision as of 14:47, 2 May 2008
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| Serellan Sector |
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| Trinity Sector |
| Jenatris Cloud Sector |
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| Zeta Pictoris system | Star · I · II · Belt I · III · Belt II |
The Zeta Pictoris star is a class IV Subgiant star, type A6 (white spectrum) with an average temperature of between 7,500 to 10,000 Kelvin and with a stellar mass of about 3.1 to 4.0 (in relation to Sol) It has a solar radius of 2.1 and a luminosity of 40L with hydrogen lines falling within the strong range.