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Words near each other
・ MU (musician)
・ Mu (negative)
・ Mu (rocket family)
・ Mu (shaman)
・ MU 90
・ Mu Alpha Phi
・ Mu Alpha Theta
・ Mu Andromedae
・ Mu Aquarii
・ Mu Aquilae
・ 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


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Mu Arietis : ウィキペディア英語版
Mu Arietis


Mu Arietis (μ Ari, μ Arietis) is the Bayer designation for a star system in the northern constellation of Aries. It is approximately distant from Earth, give or take a 30 light-year margin of error, and has a combined apparent visual magnitude of 5.74.〔 According to the Bortle Dark-Sky Scale, this means it is faintly visible to the naked eye from dark suburban skies.
At the heart of this system is a close orbiting pair consisting of a magnitude 6.38 A-type main sequence star with a stellar classification of A0 Vp and a magnitude 8.38 F-type main sequence companion with a classification of F2 V. These two components have an angular separation of 0.04 arcseconds. A third component, consisting of a magnitude 6.72 star with a classification of A1 V, is orbiting the inner pair with a period of 8.845 years and an eccentricity of 0.34. A smaller fourth component, at an angular separation of 19.1 arcseconds, has a magnitude of 12.2.〔
==References==


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「Mu Arietis」の詳細全文を読む



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