翻訳と辞書 Words near each other ・ Iota and Jot ・ Iota Andromedae ・ Iota Antliae ・ Iota Apodis ・ Iota Aquarii ・ Iota Aquilae ・ Iota Arae ・ Iota Arietis ・ Iota Aurigae ・ Iota Beta Chi ・ Iota Boötis ・ Iota Cancri ・ Iota Canis Majoris ・ Iota Capricorni ・ Iota Carinae ・ Iota Cassiopeiae ・ Iota Centauri ・ Iota Cephei ・ Iota Ceti ・ Iota Chamaeleontis ・ Iota Coronae Borealis ・ Iota Crucis ・ Iota Cygni ・ Iota Delphini ・ Iota Delta ・ Iota Draconis ・ Iota Draconis b ・ Iota Eridani ・ Iota Geminorum ・ Iota Gruis Dictionary Lists mini英和辞書 mini和英辞書 Webster 1913 Latin-English FOLDOC Wikipedia English ウィキペディア

翻訳と辞書　辞書検索 [ 開発暫定版 ] スポンサード リンク Iota Cassiopeiae ： ウィキペディア英語版 Iota Cassiopeiae Iota Cassiopeiae (ι Cas, ι Cassiopeiae) is a star system in the constellation Cassiopeia. It is approximately 141.6 light years from Earth. The primary component, ι Cassiopeiae A, is a white A-type main sequence dwarf with a mean apparent magnitude of +4.64. It is classified as an α² Canum Venaticorum type variable star and the brightness of the system varies from magnitude +4.45 to +4.53 with a period of 1.74 days. Component A is a spectroscopic binary. Its unresolved companion has an orbital period of 52.4 years and is separated from the primary by 0.113 arcseconds, or at least 5 AU. The second astrometric component, ι Cassiopeiae B, is a yellow-white F-type main sequence dwarf with an apparent magnitude of +6.89. It is 2.27 arcseconds, or at least 100 AU, from the primary. It has an orbital period of 840 years. The third astrometric component, ι Cassiopeiae C, is a yellow G-type dwarf, with an apparent magnitude of +8.40. It is 7.3 arcseconds (at least 300 AU) from the primary. 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 Cassiopeiae」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.