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(523759) 2014 WK509

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(523759) 2014 WK509
Discovery
Discovered byPan-STARRS 1
Discovery siteHaleakala Obs.
Discovery date14 September 2010
Designations
MPC designation(523759) 2014 WK509
Minor planet categoryTNO · SDO
distant
Orbital characteristics
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter· 3
Observation arc3.24 yr (1,185 days)
Aphelion61.579 AU
Perihelion40.098 AU
Semi-major axis50.838 AU
Eccentricity0.2113
Orbital period (sidereal)362.49 yr (132,399 days)
Mean anomaly271.50°
Mean motion0° 0 9.72 / day
Inclination14.542°
Longitude of ascending node41.033°
Argument of perihelion135.10°
Physical characteristics
Mean diameter574 km (est.)
584 km (est.)
Geometric albedo0.09 (assumed)
Absolute magnitude (H)4.4
4.5

(523759) 2014 WK509 (provisional designation 2014 WK509) is a trans-Neptunian object in the scattered disc, located in the outermost regions of the Solar System. It was discovered on 14 September 2010, by Pan-STARRS at Haleakala Observatory on the island of Maui, Hawaii, in the United States. The object's diameter has been estimated to measure approximately 600 kilometers.

Orbit and classification

2014 WK509 belongs to the scattered disc population. It orbits the Sun at a distance of 40.1–61.6 AU once every 362 years and 6 months (132,399 days; semi-major axis of 50.8 AU). Its orbit has an eccentricity of 0.21 and an inclination of 15° with respect to the ecliptic. The body's observation arc begins on 14 September 2011 at Haleakala, more than 3 years prior to its official first observation. Its orbit still has a high uncertainty.

Numbering and naming

This minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111779). As of 2018, it has not been named.

Physical characteristics

Based on an absolute magnitude of 4.4, and an assumed albedo of 0.09, the Johnston's archive estimates a mean diameter of approximately 584 kilometers (363 mi).

As of 2018, no rotational lightcurve of this object has been obtained from photometric observations. The object's rotation period, pole and shape remain unknown.

References

  1. ^ "2014 WK509". Minor Planet Center. Retrieved 8 February 2018.
  2. ^ "JPL Small-Body Database Browser: (2014 WK509)" (2015-01-21 last obs.). Jet Propulsion Laboratory. Retrieved 8 February 2018.
  3. ^ Johnston, Wm. Robert (30 December 2017). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 8 February 2018.
  4. ^ Michael E. Brown. "How many dwarf planets are there in the outer solar system?". California Institute of Technology. Retrieved 8 February 2018.
  5. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 7 October 2018.

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