Discovery[1]
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Discovered by | Michael E. Brown, Chad Trujillo |
Discovery date | May 17, 2002 |
Designations
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MPC designation | (119951) 2002 KX14 |
Alternate name(s) | none |
Minor planet category |
TNO cubewano[2] plutino-like |
Epoch December 31, 2006 (JD 2454100.5) | |
Aphelion | 6081.698 Gm (40.654 AU) |
Perihelion | 5594.029 Gm (37.394 AU) |
Semi-major axis | 5837.864 Gm (39.024 AU) |
Eccentricity | 0.042 |
Orbital period | 89041.246 d (243.78 a) |
Average orbital speed | 4.77 km/s |
Mean anomaly | 253.196° |
Inclination | 0.401° |
Longitude of ascending node | 286.961° |
Argument of perihelion | 66.276° |
Physical characteristics
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Dimensions | 180 km (2010)[3] <562+220 −182 (2007) km[4] |
Mass | 2.0×1020? kg |
Mean density | 2.0? g/cm3 |
Equatorial surface gravity | 0.1621? m/s2 |
Escape velocity | 0.3066? km/s |
Sidereal rotation period |
? d |
Albedo | >0.08+0.09 −0.04[4] |
Temperature | ~45 K |
Spectral type | ? |
Apparent magnitude | 20.4 (opposition)[5][6] |
Absolute magnitude (H) | 4.5[1] |
(119951) 2002 KX14, also written as 2002 KX14, is a trans-Neptunian object (TNO) residing within the Kuiper belt. It was discovered on May 17, 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.[7] The orbital periods of plutinos cluster around 247.2 years (1.5 x Neptune's orbital period). But (119951) 2002 KX14 is not classified as a plutino since is not in resonance with Neptune and it may have formed near its present quasi-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.[2]
It comes to opposition in late May at an apparent magnitude of 20.4.[5][6] This makes it about 360 times fainter than Pluto.[8]
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