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・ (10115) 1992 SK
・ (101429) 1998 VF31
・ (101869) 1999 MM
・ (10302) 1989 ML
・ (11351) 1997 TS25
・ (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


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(119951) 2002 KX14 : ウィキペディア英語版
(119951) 2002 KX14

, also written as 2002 KX14, is a trans-Neptunian object (TNO) residing within the Kuiper belt. It was discovered on 17 May 2002 by Michael E. Brown and Chad Trujillo.
It has a semi-major axis, orbital period and orbital eccentricity close to that of a plutino. The orbital periods of plutinos cluster around 247.2 years (1.5 times Neptune's orbital period). However, is not a plutino, because is not in resonance with Neptune, and it may have formed near its present nearly circular orbit lying almost perfectly on the ecliptic. It may have remained dynamically cold and thus its orbit may not be a direct result of significant perturbations during Neptune's outward planetary migration. The Deep Ecliptic Survey (DES) currently shows it as a cubewano (classical) based on a 10-million-year integration of the orbit.〔
File:2002KX14-orbit.png
It comes to opposition in late May at an apparent magnitude of 20.4.〔〔 This makes it about 360 times fainter than Pluto.〔(5th root of 100)^(20.4-(14 )=363)〕
==See also==

* Nice model

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