Discovery | |
---|---|
Discovered by | Pan-STARRS 1 |
Discovery site | Haleakala Obs. |
Discovery date | 14 September 2010 |
Designations | |
MPC designation | (523759) 2014 WK509 |
Minor planet category | TNO · SDO distant |
Orbital characteristics | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 5 · 3 | |
Observation arc | 3.24 yr (1,185 days) |
Aphelion | 61.579 AU |
Perihelion | 40.098 AU |
Semi-major axis | 50.838 AU |
Eccentricity | 0.2113 |
Orbital period (sidereal) | 362.49 yr (132,399 days) |
Mean anomaly | 271.50° |
Mean motion | 0° 0 9.72 / day |
Inclination | 14.542° |
Longitude of ascending node | 41.033° |
Argument of perihelion | 135.10° |
Physical characteristics | |
Mean diameter | 574 km (est.) 584 km (est.) |
Geometric albedo | 0.09 (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
- ^ "2014 WK509". Minor Planet Center. Retrieved 8 February 2018.
- ^ "JPL Small-Body Database Browser: (2014 WK509)" (2015-01-21 last obs.). Jet Propulsion Laboratory. Retrieved 8 February 2018.
- ^ Johnston, Wm. Robert (30 December 2017). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 8 February 2018.
- ^ 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
- List Of Centaurs and Scattered-Disk Objects, Minor Planet Center
- (523759) 2014 WK509 at AstDyS-2, Asteroids—Dynamic Site
- (523759) 2014 WK509 at the JPL Small-Body Database
Trans-Neptunian objects | |
---|---|
TNO classes | |
Dwarf planets (moons) | |
Sednoids |
Minor planets navigator | |
---|---|
Small Solar System bodies | |||||||
---|---|---|---|---|---|---|---|
Minor planets |
| ||||||
Comets | |||||||
Other |