(119951) 2002 KX14
(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, (119951) 2002 KX14 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
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(119951) 2002 KX14
(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, (119951) 2002 KX14 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
apoapsis (km)
6.0573673825137E9
average speed (km/s)
orbital period (μ)
periapsis (km)
5.5716230963508E9
temperature (K)
absolute magnitude
has abstract
(119951) 2002 KX14 est un objet transneptunien de la famille des cubewanos.
@fr
(119951) 2002 KX14 — транснепт ...... 12 года составляет 404 ± 1 км.
@ru
(119951) 2002 KX14, also writt ...... 360 times fainter than Pluto.
@en
(119951) 2002 KX14, também esc ...... idato a possível planeta anão.
@pt
小行星119951((119951) 2002 KX14)是 ...... 119951的半長軸,軌道週期,軌道偏心率都接近冥族小天體。
@zh
apoapsis (μ)
6.0573673825137e+12
apparent magnitude
average speed (kmh)
discovery date
2002-05-17
epoch
13 January 2016 (JD2457400.5)
orbital period (s)
7.64697024e+9
periapsis (μ)
5.5716230963508e+12
temperature (K)
thumbnail
Link from a Wikipage to an external page
Wikipage page ID
Wikipage revision ID
738,565,105
arg peri
asc node
2.86686e+2
background
eccentricity
inclination
mean anomaly
2.61303e+2
mean motion
minorplanet
mp category
observation arc
8.805888E8
uncertainty
subject
hypernym
comment
(119951) 2002 KX14 est un objet transneptunien de la famille des cubewanos.
@fr
(119951) 2002 KX14 — транснепт ...... лассический), расположенный уж
@ru
(119951) 2002 KX14, also writt ...... ws it as a cubewano (classical
@en
(119951) 2002 KX14, também esc ...... idato a possível planeta anão.
@pt
小行星119951((119951) 2002 KX14)是 ...... 119951的半長軸,軌道週期,軌道偏心率都接近冥族小天體。
@zh
label
(119951) 2002 KX14
@en
(119951) 2002 KX14
@fr
(119951) 2002 KX14
@pt
(119951) 2002 KX14
@ru
小行星119951
@zh