Veqlargh Bal (star): Difference between revisions

no edit summary
m (added data)
 
No edit summary
 
Line 2: Line 2:
{{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]]
15,085

edits