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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 61 Virginis d ： ウィキペディア英語版 61 Virginis d 61 Virginis d (abbreviated 61 Vir d) is a proposed exoplanet orbiting the 5th apparent-magnitude G-type main-sequence star 61 Virginis in the constellation Virgo. 61 Virginis d would have a minimum mass of 22.9 times that of Earth and orbits nearly one-half the distance to the star as Earth orbits the Sun with an eccentricity of 0.35. This planet would most likely be a gas giant like Uranus and Neptune. This planet was induced on 14 December 2009 from using a precise radial velocity method taken at Keck and Anglo-Australian Observatories. As of 2012 it has not been confirmed by other measurements such as from HARPS.〔 File:61VirginisSystem.svg|61VirginisSystem File:Artist's impression of 61 Virginis d.jpg|Artist's impression of 61 Virginis d. == 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「61 Virginis d」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.