(119951) 2002 KX14

(119951) 2002 KX14
Discovery[1]
Discovered by Michael E. Brown, Chad Trujillo
Discovery date May 17, 2002
Designations
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
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]

See also

References

  1. ^ a b c "JPL Small-Body Database Browser: 119951 (2002 KX14)". 2006-04-26 last obs. http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=119951. Retrieved 2008-07-16. 
  2. ^ a b c Marc W. Buie (2006-04-26). "Orbit Fit and Astrometric record for 119951". SwRI (Space Science Department). http://www.boulder.swri.edu/~buie/kbo/astrom/119951.html. Retrieved 2008-07-16. 
  3. ^ Wm. Robert Johnston (7 August 2010). "List of Known Trans-Neptunian Objects". Johnston's Archive. http://www.johnstonsarchive.net/astro/tnoslist.html. Retrieved 2011-03-03. 
  4. ^ a b Stansberry, John; et al. (2007). "Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope". arXiv:astro-ph/0702538 [astro-ph]. 
  5. ^ a b "(119951) 2002 KX14". Minor Planet Center. 2010-07-23 epoch. http://scully.cfa.harvard.edu/~cgi/ReturnPrepEph?d=d&o=B9951. Retrieved 2010-10-24. 
  6. ^ a b "HORIZONS Web-Interface". JPL Solar System Dynamics. http://ssd.jpl.nasa.gov/horizons.cgi?find_body=1&body_group=sb&sstr=119951. Retrieved 2008-07-20. 
  7. ^ John S. Lewis (2004). "Plutinos 2nd paragraph on page 410". Physics and Chemistry of the Solar System. Academic Press. ISBN 012446744X, 9780124467446. http://books.google.com/books?id=zm3ChHeFJn8C&pg=PA410&lpg=PA410&dq=centaur+%22Neptune+resonance%22. 
  8. ^ (5th root of 100)^(20.4-14=363)

External links