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1 Orbit and classification  





2 Numbering and naming  





3 Physical characteristics  





4 References  





5 External links  














(523759) 2014 WK509






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From Wikipedia, the free encyclopedia
 

(Redirected from 2014 WK509)

(523759) 2014 WK509
Discovery[1]
Discovered byPan-STARRS1
Discovery siteHaleakala Obs.
Discovery date14 September 2010
Designations

MPC designation

(523759) 2014 WK509

Minor planet category

TNO[2] · SDO[3]
distant[1]
Orbital characteristics[2]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter5[2] · 3[1]
Observation arc3.24 yr (1,185 days)
Aphelion61.579 AU
Perihelion40.098 AU

Semi-major axis

50.838 AU
Eccentricity0.2113

Orbital period (sidereal)

362.49 yr (132,399 days)

Mean anomaly

271.50°

Mean motion

0° 0m 9.72s / day
Inclination14.542°

Longitude of ascending node

41.033°

Argument of perihelion

135.10°
Physical characteristics

Mean diameter

574 km (est.)[4]
584 km (est.)[3]

Geometric albedo

0.09 (assumed)[3][4]

Absolute magnitude (H)

4.4[1][2]
4.5[4]

(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-STARRSatHaleakala Observatory on the island of Maui, Hawaii, in the United States.[1] The object's diameter has been estimated to measure approximately 600 kilometers.[3][4]

Orbit and classification[edit]

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.[2] The body's observation arc begins on 14 September 2011 at Haleakala, more than 3 years prior to its official first observation.[1] Its orbit still has a high uncertainty.[1][2]

Numbering and naming[edit]

This minor planet was numbered by the Minor Planet Center on 25 September 2018 (M.P.C. 111779).[5] As of 2018, it has not been named.[1]

Physical characteristics[edit]

Based on an absolute magnitude of 4.4,[2] and an assumed albedo of 0.09, the Johnston's archive estimates a mean diameter of approximately 584 kilometers (363 mi).[3]

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.[2]

References[edit]

  1. ^ a b c d e f g h "2014 WK509". Minor Planet Center. Retrieved 8 February 2018.
  • ^ a b c d e f g h "JPL Small-Body Database Browser: (2014 WK509)" (2015-01-21 last obs.). Jet Propulsion Laboratory. Retrieved 8 February 2018.
  • ^ a b c d e Johnston, Wm. Robert (30 December 2017). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 8 February 2018.
  • ^ a b c d Michael E. Brown. "How many dwarf planets are there in the outer solar system?". California Institute of Technology. Retrieved 8 February 2018.
  • ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 7 October 2018.
  • External links[edit]



    Retrieved from "https://en.wikipedia.org/w/index.php?title=(523759)_2014_WK509&oldid=1229652442"

    Categories: 
    Minor planet object articles (numbered)
    Scattered disc and detached objects
    Discoveries by Pan-STARRS
    Possible dwarf planets
    Astronomical objects discovered in 2014
    Hidden categories: 
    Use dmy dates from February 2018
    Articles with JPL SBDB identifiers
    Articles with MPC identifiers
     



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