翻訳と辞書 Words near each other ・ Dyspessa dueldueli ・ Dyspessa elbursensis ・ Dyspessa emilia ・ Dyspessa fantolii ・ Dyspessa fuscula ・ Dyspessa hethitica ・ Dyspessa infuscata ・ Dyspessa kabylaria ・ Dyspessa karatavica ・ Dysmorphococcus ・ Dysmorphopsia ・ Dysna ・ Dysnectes brevis ・ Dysnomia ・ Dysnomia (deity) ・ Dysnomia (moon) ・ Dysnymphus ・ Dysochrysa ・ Dysocnemis ・ Dysodia ・ Dysodia zellerii ・ Dysodiopsis ・ Dysolobium ・ Dysomma ・ Dysomma bucephalus ・ Dysomma dolichosomatum ・ Dysomma fuscoventralis ・ Dysomma goslinei ・ Dysomma longirostrum ・ Dysomma melanurum 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 Dysnomia (moon) ： ウィキペディア英語版 Dysnomia (moon) Dysnomia (Greek: ''Δυσνομία'')—officially (136199) Eris I Dysnomia—is the only known moon of the dwarf planet Eris (the most massive known dwarf planet in the Solar System). It was discovered in 2005 by Mike Brown and the laser guide star adaptive optics team at the W. M. Keck Observatory, and carried the provisional designation of until officially named ''Dysnomia''〔 (from the Ancient Greek word meaning "lawlessness") after the daughter of the Greek goddess Eris. == Discovery == During 2005, the adaptive optics team at the Keck telescopes in Hawaii carried out observations of the four brightest Kuiper belt objects (Pluto, , , and ), using the newly commissioned laser guide star adaptive optics system. Observations taken on 10 September revealed a moon in orbit around Eris, provisionally designated . In keeping with the ''Xena'' nickname that was already in use for Eris, the moon was nicknamed "Gabrielle" by its discoverers, after Xena's sidekick.〔〔 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「Dysnomia (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.