Rumaiy (star): Difference between revisions
Jump to navigation
Jump to search
(added data) |
mNo edit summary |
||
| (2 intermediate revisions by the same user not shown) | |||
| Line 1: | Line 1: | ||
{{ | {{Promell Sector}} | ||
{{Rumaiy}} | {{Rumaiy}} | ||
The Rumaiy star is a [[wp:Main sequence|class V main sequence star]], [[wp:Stellar classification#Class M|type M9 (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 Rumaiy star is a [[wp:Main sequence|class V main sequence star]], [[wp:Stellar classification#Class M|type M9 (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:Rumaiy system]] | |||
Latest revision as of 22:16, 30 July 2008
|
| Alrakis Sector |
|---|
| Promell Sector |
| Gavaria Sector |
| Territory |
|
| Local Species |
| Stellar Phenomenae |
|
| Federation Presence |
|
| Rumaiy system | Star · Belt I · I · II · Belt II · III · IV · Belt III · V |
The Rumaiy star is a class V main sequence star, type M9 (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.