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・ (415713) 1998 XX2
・ (416151) 2002 RQ25
・ (417634) 2006 XG1
・ (419624) 2010 SO16
・ (420356) 2012 BX85
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・ (42493) 1991 TG14
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(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
・ (53319) 1999 JM8


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(44594) 1999 OX3 : ウィキペディア英語版
(44594) 1999 OX3

is a trans-Neptunian object with a centaur-like orbit.
==Classification==
Neptune has a semi-major axis of 30 AU and has a semi-major axis of 32 AU. The Minor Planet Center (MPC) does not classify this object as a centaur because the MPC defines centaurs as having a semi-major axis of less than 30.066 AU. crosses the orbits of both Neptune and Uranus and has an inclination of only 2.62°. The Deep Ecliptic Survey (DES) defines centaurs using a dynamical classification scheme, based on the behavior of orbital integrations over 10 million years. The DES defines centaurs as nonresonant objects whose osculating perihelia are less than the osculating semimajor axis of Neptune at any time during the integration. Using the dynamical definition of a centaur, is a centaur.〔

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