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・ (415029) 2011 UL21
・ (415713) 1998 XX2
・ (416151) 2002 RQ25
・ (417634) 2006 XG1
・ (419624) 2010 SO16
・ (420356) 2012 BX85
・ (42301) 2001 UR163
・ (42493) 1991 TG14
・ (432949) 2012 HH2
・ (433953) 1997 XR2
・ (434326) 2004 JG6
・ (434620) 2005 VD
・ (436724) 2011 UW158
・ (444004) 2004 AS1
・ (444030) 2004 NT33
(445473) 2010 VZ98
・ (44594) 1999 OX3
・ (4489) 1988 AK
・ (4715) 1989 TS1
・ (47171) 1999 TC36
・ (48438) 1989 WJ2
・ (48639) 1995 TL8
・ (4953) 1990 MU
・ (4S)-beta-phellandrene synthase (geranyl-diphosphate-cyclizing)
・ (4S)-limonene synthase
・ (5025) 1986 TS6
・ (5119) 1988 RA1
・ (52246) 1981 EQ5
・ (52747) 1998 HM151
・ (52760) 1998 ML14


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(445473) 2010 VZ98 : ウィキペディア英語版
(445473) 2010 VZ98

is a trans-Neptunian object (TNO) orbiting the Sun in the scattered disc. It was discovered in November 2010 when it was 38 AU from the Sun. With an absolute magnitude of 5.0,〔 it is likely a dwarf planet and might be around in diameter.
Small number statistics suggest may be trapped in a 3:2 orbital resonance with an unseen planet beyond Neptune with a semi-major axis of 195–215 AU.
In May 2015, precovery images of 2010 VZ98 from 1998 were found, and have been accepted by the Minor Planet Center but not the JPL. Therefore, the JPL orbit for the asteroid is less accurate.
==See also==

*List of Solar System objects by greatest aphelion

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