翻訳と辞書 Words near each other ・ Epsilon Pavonis ・ Epsilon Pegasi ・ Epsilon Persei ・ Epsilon Phoenicis ・ Epsilon photography ・ Epsilon Pi Tau ・ Epsilon Piscis Austrini ・ Epsilon Piscium ・ Epsilon Pyxidis ・ Epsilon radiation ・ Epsilon Reticuli ・ Epsilon Reticuli b ・ Epsilon Sagittae ・ Epsilon Sagittarii ・ Epsilon Scorpii ・ Epsilon Sculptoris ・ Epsilon Scuti ・ Epsilon Serpentis ・ Epsilon Sextantis ・ Epsilon Sigma Alpha ・ Epsilon Tau Pi ・ Epsilon Tauri ・ Epsilon Tauri b ・ Epsilon Telescopii ・ Epsilon transition ・ Epsilon Trianguli ・ Epsilon Trianguli Australis ・ Epsilon Tucanae ・ Epsilon TV ・ Epsilon Ursae Majoris 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 Epsilon Sculptoris ： ウィキペディア英語版 Epsilon Sculptoris Epsilon Sculptoris (ε Scl, ε Sculptoris) is a star system in the constellation Sculptor. It is approximately 89.5 light years from Earth. The primary component, Epsilon Sculptoris A, is a yellow-white F-type subgiant with an apparent magnitude of +5.29 with an angular diameter of 000509 arcseconds. Orbiting it with a separation of 4.6 arcseconds, or at least 125 Astronomical Units, is Epsilon Sculptoris B, a yellow G-type main sequence dwarf with an apparent magnitude of +8.6. A and B make one orbit around their centre of mass once every 1200 years. They are accompanied by two more distant and dimmer companions, the 15th magnitude Epsilon Sculptoris C at a separation of 15 arcseconds and the 11th magnitude Epsilon Sculptoris D, at a separation of 142 arcseconds. ε Scl A Solar radius = 1.5. ref. Solar luminosity = 5.0. ref. Starry Night software This star will be in constellation Fornax around 2920 CE.〔p. 296, (''Patrick Moore's Data Book of Astronomy'' ), Patrick Moore and Robin Rees, Cambridge, Cambridge University Press, 2011.〕 ==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「Epsilon Sculptoris」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.