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・ Zeta Cancri
・ Zeta Canis Majoris
・ Zeta Canis Minoris
・ Zeta Capricorni
・ Zeta Cassiopeiae
・ Zeta Centauri
・ Zeta Cephei
・ Zeta Ceti
・ Zeta Chamaeleontis
・ Zeta Chi
・ Zeta Chi Phi
・ Zeta Circini
・ Zeta Coronae Australis
・ Zeta Coronae Borealis
・ Zeta Corse
Zeta Corvi
・ Zeta Crateris
・ Zeta Crucis
・ Zeta Cygni
・ Zeta Delphini
・ Zeta Delta Xi
・ Zeta distribution
・ Zeta Doradus
・ Zeta Draconis
・ Zeta Equulei
・ Zeta Eridani
・ Zeta function (operator)
・ Zeta function regularization
・ Zeta function universality
・ Zeta Geminorum


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Zeta Corvi : ウィキペディア英語版
Zeta Corvi


Zeta Corvi (ζ Crv, ζ Corvi) is a star in the constellation Corvus. It is a blue-white main sequence star of apparent magnitude 5.21. Located around 420 light-years distant, it shines with a luminosity approximately 154 times that of the Sun and has a surface temperature of 10,695 K. It is a Be star, the presence of hydrogen emission lines in its spectrum indicating it has a circumstellar disk. It is separated by 7 arcseconds from the star HR 4691. The two may be an optical double or a true multiple star system, with a separation of at least 50,000 astronomical units and the stars taking 3.5 million years to orbit each other. HR 4691 is itself double, composed of an ageing yellow-orange giant whose spectral type has been calculated at K0 or G3, and an F-type main sequence star.

==Reference==



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 Corvi」の詳細全文を読む



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