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Zeta Phoenicis : ウィキペディア英語版 | Zeta Phoenicis
Zeta Phoenicis (ζ Phe, ζ Phoenicis) is a 280 light-year distant star in the constellation Phoenix. It is an Algol-type eclipsing binary star and its apparent magnitude fluctuates between 3.9 and 4.4 with a period of 1.66977 days. Zeta Phoenicis is most likely a four-star system: it has two other telescopic components with an apparent magnitude of 7.2 and 8.2 at an angular separation of 0.8 and 6.4 arcseconds from the main pair.〔 ==References==
* ''Der Brockhaus. Astronomie''. 2006, p. 334.
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「Zeta Phoenicis」の詳細全文を読む
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