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Epsilon Volantis : ウィキペディア英語版 | Epsilon Volantis
Epsilon Volantis (ε Vol, ε Volantis) is a triple star system in the constellation Volans. It is approximately 642 light years from Earth. The primary component, Epsilon Volantis A, is a spectroscopic binary. It is classified a blue-white B-type subgiant and has an apparent magnitude of +4.35. The binary system has an orbital period of 14.17 days. The binary's companion, Epsilon Volantis B, is 6.05 arcseconds away and has an apparent magnitude of +8.1.
抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)』 ■ウィキペディアで「Epsilon Volantis」の詳細全文を読む
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