Miri (star): Difference between revisions
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{{ | {{Serellan}} | ||
{{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 | 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: | [[Category:Serellan Sector]] | ||
Latest revision as of 15:33, 9 July 2008
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| Serellan Sector |
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| Trinity Sector |
| Jenatris Cloud Sector |
| (Sector 118 map) |
| Territory |
| Local Species |
| Stellar Phenomenae |
| Federation Presence |
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| Miri system | Star · I · II · III · IV · V · VI · VII |
The Miri star is a class V main sequence star, 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.