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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 Cyllene (moon) ： ウィキペディア英語版 Cyllene (moon) Cyllene ( ; Greek: ''Κυλλήνη''), also known as , is a natural satellite of Jupiter. It was discovered by a team of astronomers from the University of Hawaii led by Scott S. Sheppard in 2003, receiving the temporary designation .〔(IAUC 8116: ''Satellites of Jupiter and Saturn'' ) 2003 April (discovery)〕〔(MPEC 2003-G09: ''S/2003 J 13'' ) 2003 April (discovery and ephemeris)〕 Cyllene is about 2 kilometres in diameter, and orbits Jupiter at an average distance of 23,396 Mm in 731.099 days, at an inclination of 140° to the ecliptic (140° to Jupiter's equator), in a retrograde direction and with an eccentricity of 0.4116. It was named in March 2005 after Cyllene, a naiad (stream nymph) or oread (mountain nymph) associated with Mount Kyllini, Greece.〔(IAUC 8502: ''Satellites of Jupiter'' ) 2005 March (naming the moon)〕 She was a daughter of Zeus (Jupiter). It belongs to the Pasiphae group, irregular retrograde moons orbiting Jupiter at distances ranging between 22.8 and 24.1 Gm, and with inclinations ranging between 144.5° and 158.3°. ==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「Cyllene (moon)」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.