Miri (star): Difference between revisions
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{{Miri}} | {{Miri}} | ||
The Miri star is a [[wp:Main sequence|class V main sequence star]], [[wp:Stellar classification#Class G|type G7 (yellow spectrum)]] with a | The Miri star is a [[wp:Main sequence|class V main sequence star]], [[wp:Stellar classification#Class G|type G7 (yellow spectrum)]] with a temperature of 5,000 to 6,000 Kelvin and with a stellar mass of about 1 to 1.1. (in relation to Sol) It has a solar radius of about 1.1, a luminosity of 1.2L and hydrogen lines falling in the weak range. | ||
[[Category:Stars]] | [[Category:Stars]] | ||
[[Category:Miri system]] | [[Category:Miri system]] | ||
[[Category:Trinity Sector]] | [[Category:Trinity Sector]] | ||
Revision as of 14:42, 6 June 2008
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| Serellan Sector |
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| Jenatris Cloud Sector |
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| Miri system | Star · I · II · III · IV · V · VI · VII |
The Miri star is a class V main sequence star, type G7 (yellow spectrum) with a temperature of 5,000 to 6,000 Kelvin and with a stellar mass of about 1 to 1.1. (in relation to Sol) It has a solar radius of about 1.1, a luminosity of 1.2L and hydrogen lines falling in the weak range.