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Beta Crateris : ウィキペディア英語版 | Beta Crateris
Beta Crateris (β Crt, β Crateris) is a star in the constellation Crater. Beta Crateris is a white sub-giant belonging to the spectral class A2, has apparent magnitude 4.48, and is about 265 light years from Earth. ==Name==
Shared with κ Hya, this star was Al Tizini's Al Sharāsīf (ألصرسىف), the Ribs, — i.e. of the Hydra, — and the first of the set〔(Star Name - R.H.Allen p. 182 )〕〔(Star Name - R.H.Allen p. 246 )〕 In Chinese, (), meaning ''Wings (asterism)'', refers to an asterism consisting of β Crateris, α Crateris, γ Crateris, ζ Crateris, λ Crateris, ν Hydrae, η Crateris, δ Crateris, ι Crateris, κ Crateris, ε Crateris, HD 95808, HD 93833, θ Crateris, HD 102574, HD 100219, HD 99922, HD 100307, HD 96819, χ1 Hydrae, HD 102620 and HD 103462.〔 ''中國星座神話'', written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 978-986-7332-25-7.〕 Consequently, β Crateris itself is known as (, (英語:the Sixteenth Star of Wings).)〔 (AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 31 日 )〕〔 ( 夢之大地 @ 國立成功大學 WebBBS DreamLand @ National Cheng Kung University WebBBS System )〕
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