(119979) 2002 WC19

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The correct title of this article is (119979) 2002 WC19. It features superscript or subscript characters that are substituted or omitted because of technical limitations.
(119979) 2002 WC19
Discovery
Discovered by Palomar Observatory
Discovery date November 16, 2002
Designations
MPC designation (119979) 2002 WC19
Alternative names none
Minor planet
category
Twotino[1]
Epoch December 31, 2006 (JD 2454100.5)
Aphelion 8989.786 Gm (60.093 AU)
Perihelion 5269.094 Gm (35.222 AU)
Semi-major axis 7129.440 Gm (47.657 AU)
Eccentricity 0.261
Orbital period 120169.272 d (329.01 a)
Average orbital speed 4.24 km/s
Mean anomaly 305.041°
Inclination 9.191°
Longitude of ascending node 109.692°
Argument of perihelion 45.322°
Satellites 1 (127 km)
Physical characteristics
Dimensions 400 km
Surface area 5.5×105 km²
Volume 3.9×107 km³
Mass 7.8×1019? kg
Mean density 2.0? g/cm³
Equatorial surface gravity 0.1174? m/s²
Escape velocity 0.2220? km/s
Sidereal rotation
period
? d
Albedo 0.10?
Temperature ~40 K
Spectral type ?
Absolute magnitude 5.1

(119979) 2002 WC19, also written as (119979) 2002 WC19, is a Trans-Neptunian object (TNO) orbiting beyond Pluto in the Kuiper belt. It was discovered on November 16, 2002 at the Palomar Observatory.

It is in a 2:1 orbital resonance with Neptune, so it has been categorized as a twotino.

[edit] Satellite

A natural satellite was reported to be in orbit of (119979) 2002 WC19 on February 27, 2007. It is estimated to be orbiting at 2700 km from the primary and to be 127 kilometres in diameter.

[edit] References

  1. ^ List of known trans-Neptunian objects

http://www.johnstonsarchive.net/astro/astmoons/am-119979.html