Miri (star): Difference between revisions
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(New page: {{stub}} {{Trinity}} {{Miri}} The Miri star is a class V main sequence star, type G (yellow spectrum) with a stellar mass of abo...) |
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The Miri star is a [[wp:Main sequence|class V main sequence star]], [[wp:Stellar classification#Class G|type | The Miri star is a [[wp:Main sequence|class V main sequence star]], [[wp:Stellar classification#Class G|type G7 (yellow spectrum)]] with a temerature 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]] | ||
Revision as of 03:52, 22 April 2008
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The Miri star is a class V main sequence star, type G7 (yellow spectrum) with a temerature 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.