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翻訳と辞書　辞書検索 [ 開発暫定版 ] スポンサード リンク Iota Andromedae ： ウィキペディア英語版 Iota Andromedae Iota Andromedae (ι And, ι Andromedae) is a star in the constellation Andromeda. It has an apparent magnitude of +4.29〔 and is approximately 500 light years from Earth.〔 Iota Andromedae is a B-type main sequence star with a stellar classification of B8 V. It is among the least variable stars observed during the Hipparcos mission.〔 ==Name== *In the catalogue of stars in the ''Calendarium of Al Achsasi Al Mouakket'', this star was designated Keff al-Salsalat (كف المسلسلة - ''kaf al-musalsala''), which was translated into Latin as Manus Catenata, meaning ''palm of chained woman''. *In Chinese, (), meaning ''Flying Serpent'', refers to an asterism consisting of ι Andromedae, α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae, 9 Lacertae, 3 Andromedae, 7 Andromedae, 8 Andromedae, λ Andromedae, κ Andromedae and ψ Andromedae. Consequently, ι Andromedae itself is known as (, (英語:the Twenty Second Star of Flying Serpent))〔 (AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 7 日 )〕 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「Iota Andromedae」の詳細全文を読む スポンサード リンク 翻訳と辞書 : 翻訳のためのインターネットリソース Copyright(C) kotoba.ne.jp 1997-2016. All Rights Reserved.