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 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.
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]]
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