翻訳と辞書 Words near each other ・ (136120) 2003 LG7 ・ (136617) 1994 CC ・ (137108) 1999 AN10 ・ (137295) 1999 RB216 ・ (13780) 1998 UZ8 ・ (13790) 1998 UF31 ・ (137924) 2000 BD19 ・ (13E)-labda-7,13-dien-15-ol synthase ・ (143649) 2003 QQ47 ・ (144897) 2004 UX10 ・ (144898) 2004 VD17 ・ (144908) 2004 YH32 ・ (145451) 2005 RM43 ・ (145452) 2005 RN43 ・ (145453) 2005 RR43 ・ (145480) 2005 TB190 ・ (148209) 2000 CR105 ・ (148975) 2001 XA255 ・ (152680) 1998 KJ9 ・ (153201) 2000 WO107 ・ (153591) 2001 SN263 ・ (153814) 2001 WN5 ・ (15430) 1998 UR31 ・ (15760) 1992 QB1 ・ (15788) 1993 SB ・ (15789) 1993 SC ・ (15807) 1994 GV9 ・ (15809) 1994 JS ・ (15810) 1994 JR1 ・ (15820) 1994 TB 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 (145480) 2005 TB190 ： ウィキペディア英語版 (145480) 2005 TB190 , provisionally known as 2005 TB190, is a trans-Neptunian object (TNO) with an absolute magnitude of 4.4,〔 making it a likely dwarf planet.〔 == Orbit == is classified as scattered-extended by the Deep Ecliptic Survey (DES), because its orbit appears to be beyond significant gravitational interactions with Neptune's current orbit.〔 However, if Neptune migrated outward, there would have been a period when Neptune had a higher eccentricity. The aphelion of lies at 104 AU.〔 Simulations by Emel’yanenko and Kiseleva in 2007 showed that appears to have less than a 1% chance of being in a 4:1 resonance with Neptune.〔 It has been observed 202 times over seven oppositions.〔 It will come to perihelion in January 2017.〔 There are precovery observations dating back to November 2001. 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「(145480) 2005 TB190」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.