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出典:『Wikipedia』 (2010/12/25 04:33 UTC 版)

英語による解説

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Lambda Muscae (λ Mus, λ Muscae), often catalogued HD 102249 or HIP 57363, is the fourth brightest star in the southern hemisphere constellation of Musca (the Fly). Lambda Muscae visibly makes up the far end of the tail of the visual Musca constellation. It is a star in a dual system according to studies, and one of the stars catalogued in astronomer Johann Bayer's 1603 publications Uranometria. Lambda Muscae more recently has been recorded as having a stellar classification of A7III. Thus, Lambda Muscae has a white tint and burns significantly hotter than our own sun.