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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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