Veqlargh Bal (star): Difference between revisions

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{{Veqlargh Bal}}
{{Veqlargh Bal}}


The Veqlargh Bal star is a [[wp:Main sequence|class V main sequence star]], [[wp:Stellar classification#Class M|type M6 (red spectrum)]] with a temerature of 2,000 to 3,500 Kelvin and with a stellar mass of about 0.3 to 0.4. (in relation to Sol) It has a solar radius of about 0.5, a luminosity of 0.04L and hydrogen lines falling in the very weak range.
The Veqlargh Bal star is a [[wp:Main sequence|class V main sequence star]], [[wp:Stellar classification#Class M|type M6 (red spectrum)]] with a temerature of 2,000 to 3,500 Kelvin and with a stellar mass of about 0.3 to 0.4. (in relation to Sol) It has a solar radius of about 0.5, a luminosity of 0.04L and hydrogen lines falling in the very weak range.


[[Category:Stars]]
[[Category:Stars]]
[[Category:Veqlargh Bal system]]
[[Category:Veqlargh Bal system]]
[[Category:Trinity Sector]]
[[Category:Trinity Sector]]
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