(523727) 2014 NW65

(523727) 2014 NW65
Discovery[1]
Discovered byPan-STARRS 1
Discovery siteHaleakala Obs.
Discovery date14 July 2010
Designations
(523727) 2014 NW65
centaur[2][3][4] · distant[1]
Orbital characteristics[2]
Epoch 25 February 2023 (JD 2460000.5)
Uncertainty parameter 2
Observation arc12.45 yr (4,546 d)
Aphelion35.388 AU
Perihelion11.185 AU
23.286 AU
Eccentricity0.5197
112.37 yr (41,044 d)
311.34°
0° 0m 31.68s / day
Inclination20.424°
216.01°
232.73°
Physical characteristics
212 km[3]
213 km[5]
0.08 (est.)[5]
0.09 (est.)[3]
6.5[1][2]
6.8[5]

(523727) 2014 NW65 (provisional designation 2014 NW65) is a large centaur from the outer Solar System, approximately 220 kilometers (140 miles) in diameter. It was discovered on 14 July 2010 by astronomers with the Pan-STARRS-1 survey at Haleakala Observatory, Hawaii, in the United States.[1] The minor planet was numbered in 2018 and has not been named.

  1. ^ a b c d Cite error: The named reference MPC-object was invoked but never defined (see the help page).
  2. ^ a b c Cite error: The named reference jpldata was invoked but never defined (see the help page).
  3. ^ a b c Cite error: The named reference johnstonsarchive-TNO-list was invoked but never defined (see the help page).
  4. ^ Cite error: The named reference MPC-CEN-SDO-list was invoked but never defined (see the help page).
  5. ^ a b c Brown, Michael E. "How many dwarf planets are there in the outer solar system?". California Institute of Technology. Retrieved 29 June 2023.