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Beta Circini b : ウィキペディア英語版 | Beta Circini b
Location of parent star β Circini (Circled, Marked simply as β) in the constellation of Circinus.
Beta Circini b (also known as Beta Cir b, β Circini b, β Cir b)〔(Discovery of a brown dwarf companion to the A3V star β Circini. ) Retrieved 2015-11-9.〕 is an exoplanet〔 or Brown dwarf〔 orbiting the A-type star β Circini, in the constellation of Circinus.〔 It has a surface temperature of 2084.0 K. Its mass was discovered using the Spectrum method which concluded that the object has a mass of 56.0±7.0 MJ.〔 ==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「Beta Circini b」の詳細全文を読む
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