Veqlargh Chu (star): Difference between revisions

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{{Trinity}}
{{Serellan}}
{{Veqlargh Chu}}
{{Veqlargh Chu}}


The Veqlargh Chu star is a [[wp:Main sequence|class V main sequence star]], [[wp:Stellar classification#Class K|type K3 (red spectrum)]] with a temerature of 3,500 to 5,000 Kelvin and with a stellar mass of about 0.8 to 0.9. (in relation to Sol) It has a solar radius of about 0.9, a luminosity of 0.4L and hydrogen lines falling in the very weak range.
The Veqlargh Chu star is a [[wp:Main sequence|class V main sequence star]], [[wp:Stellar classification#Class K|type K3 (orange spectrum)]] with a temerature of 3,500 to 5,000 Kelvin and with a stellar mass of about 0.8 to 0.9. (in relation to Sol) It has a solar radius of about 0.9, a luminosity of 0.4L and hydrogen lines falling in the very weak range.


[[Category:Stars]]
[[Category:Stars]]
[[Category:Veqlargh Chu system]]
[[Category:Veqlargh Chu system]]
[[Category:Trinity Sector]]
[[Category:Serellan Sector]]

Latest revision as of 14:59, 3 July 2008

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Veqlargh Chu system Star  · I  · II · Belt I  · III  · IV  · Belt II

The Veqlargh Chu star is a class V main sequence star, type K3 (orange spectrum) with a temerature of 3,500 to 5,000 Kelvin and with a stellar mass of about 0.8 to 0.9. (in relation to Sol) It has a solar radius of about 0.9, a luminosity of 0.4L and hydrogen lines falling in the very weak range.