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・ (11435) 1931 UB
・ (11436) 1969 QR
・ (11671) 1998 BG4
・ (118228) 1996 TQ66
・ (118378) 1999 HT11
・ (118379) 1999 HC12
・ (118702) 2000 OM67
・ (119068) 2001 KC77
・ (119070) 2001 KP77
・ (119878) 2002 CY224
・ (119951) 2002 KX14
・ (119979) 2002 WC19
・ (120132) 2003 FY128
・ (120178) 2003 OP32
・ (120216) 2004 EW95
(120348) 2004 TY364
・ (121514) 1999 UJ7
・ (12377) 1994 PP
・ (12538) 1998 OH
・ (126154) 2001 YH140
・ (126155) 2001 YJ140
・ (12921) 1998 WZ5
・ (130391) 2000 JG81
・ (13060) 1991 EJ
・ (131696) 2001 XT254
・ (131697) 2001 XH255
・ (136120) 2003 LG7
・ (136617) 1994 CC
・ (137108) 1999 AN10
・ (137295) 1999 RB216


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(120348) 2004 TY364 : ウィキペディア英語版
(120348) 2004 TY364

, also written as (120348) 2004 TY364, is a trans-Neptunian object. It is an inner classical Kuiper belt object in the definition by Gladman, Marsden, and Van Laerhoven (e<0.24).〔(Nomenclature in the outer Solar System )〕 Its inclination of almost 25 degrees disqualifies it as such in Marc Buie's definition.〔 It is also not listed as a scattered disc object by the Minor Planet Center.〔 It was discovered by Michael E. Brown, Chad Trujillo and David L. Rabinowitz on October 3, 2004 at the Palomar Observatory.
With an absolute magnitude of 4.5, it is likely a dwarf planet. However, light-curve analysis has questioned whether it really is one.〔 ((Which are the dwarfs in the Solar System?) )〕
, it is 39.2 AU from the Sun.〔
==References==




抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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