翻訳と辞書 Words near each other ・ List of Executive Council of Hong Kong unofficial members 1896–1941 ・ List of exercise prescription software ・ List of Exeter City F.C. seasons ・ List of exhibitions by Olafur Eliasson ・ List of Exiles characters ・ List of existentialists ・ List of existing model dwellings ・ List of exit examinations in the United States ・ List of Exo members ・ List of exonerated death row inmates ・ List of exoplanet extremes ・ List of exoplanet firsts ・ List of exoplanet search projects ・ List of exoplanetary host stars ・ List of exoplanets ・ List of exoplanets detected by microlensing ・ List of exoplanets detected by radial velocity ・ List of exoplanets detected by timing ・ List of exoplanets discovered using the Kepler spacecraft ・ List of exorcists ・ List of Exosquad episodes ・ List of expatriate Afghan football clubs ・ List of expatriate Irish populations ・ List of expatriate players who have played in Korea Baseball Championship ・ List of expeditions of Muhammad ・ List of expenses claims in the United Kingdom parliamentary expenses scandal ・ List of experimental aircraft ・ List of experimental and computational labs focusing on IDPs ・ List of Experimental Bands ・ List of experimental big bands 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 List of exoplanets detected by microlensing ： ウィキペディア英語版 List of exoplanets detected by microlensing This is the list of 19 extrasolar planets detected by microlensing, sorted by projected separations. To find planets using that method, the background star is temporarily magnified by a foreground star because of the gravity that bends light. If the foreground star has a planet, the light from background star would be slightly brighter than the star with no planet. Studying the brightness difference of background star between the foreground star with planets and foreground star with no planets, then mass can be estimated. The projected separation can be determined from how much the light bended. The most massive planet detected by microlensing is MOA-bin-1b, which masses ; the least massive is MOA-2007-BLG-192Lb, which masses or . The widest separation between a planet and a star is MOA-bin-1b, which is 8.3 AU; the shortest separation is MOA-2007-BLG-192Lb, which is 0.66 AU. There are 2 members of the multi-planet systems. ''Yellow rows denote the members of the multi-planet system'' ==See also== * List of exoplanets 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「List of exoplanets detected by microlensing」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.