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Words near each other
・ Mu Arae
・ Mu Arae b
・ Mu Arae c
・ Mu Arae d
・ Mu Arae e
・ Mu Arietis
・ Mu Aurigae
・ Mu Beta Psi
・ Mu Boötis
・ Mu Cancri
・ Mu Canis Majoris
・ Mu Capricorni
・ Mu Cassiopeiae
・ Mu Centauri
・ Mu Cephei
Mu Ceti
・ Mu chord
・ Mu Chun
・ Mu Columbae
・ Mu Coronae Australis
・ Mu Coronae Borealis
・ Mu Crucis
・ Mu Cygni
・ Mu Dan
・ Mu Draconis
・ Mu Eka Tumara
・ Mu Epsilon Delta
・ Mu Epsilon Kappa
・ Mu Epsilon Theta
・ Mu Eridani


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Mu Ceti : ウィキペディア英語版
Mu Ceti


Mu Ceti (μ Ceti) is a binary system located in the constellation Cetus. Mu Ceti is a quadruple visual star system. The combined apparent magnitude of the system is +4.27, and is located 84 light years from the Sun.
In Chinese, (), meaning ''Circular Celestial Granary'', refers to an asterism consisting of α Ceti, κ1 Ceti, λ Ceti, μ Ceti, ξ1 Ceti, ξ2 Ceti, ν Ceti, γ Ceti, δ Ceti, 75 Ceti, 70 Ceti, 63 Ceti and 66 Ceti. Consequently, Mu Ceti itself is known as the Fourth Star of Circular Celestial Granary.〔 (AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 11 日 )〕
Mu Ceti A is an F0V subgiant, believed to be a Delta Scuti variable star.
The other components, Mu Ceti B, C and D are G3V, G2V and G6V respectively. The dimmer components were all discovered during occultations of Mu Ceti by the Moon. One of them orbits at a period of 1202 days.
== References ==



抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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