(78799) 2002 XW93

(78799) 2002 XW93
Discovery [1][2]
Discovered by Palomar team
Discovery site Palomar Obs.
Discovery date 10 December 2002
Designations
MPC designation (78799) 2002 XW93
2002 XW93
TNO
Orbital characteristics[1]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 3
Observation arc 6852 days (18.76 yr)
Aphelion 46.788 AU (6.9994 Tm)
Perihelion 28.270 AU (4.2291 Tm)
37.529 AU (5.6143 Tm)
Eccentricity 0.24673
229.91 yr (83974.5 d)
140.32°
 0m 15.433s / day
Inclination 14.376°
46.903°
247.41°
Earth MOID 27.2797 AU (4.08099 Tm)
Jupiter MOID 23.2578 AU (3.47932 Tm)
Physical characteristics
Dimensions 584 km[3]
565 km[4]
5.5[1]

    (78799) 2002 XW93 is an unnamed minor planet in the outer Solar System, classified as a trans-Neptunian object, about 550–600 kilometers in diameter. It was discovered by and at the U.S Palomar observatory, California, on 10 December 2002. According to American astronomer Michael Brown, the minor planet is a likely dwarf planet.[3]

    The minor planet orbits the Sun at a distance of 28.3–46.8 AU once every 229 years and 11 months (83,974 days). Its orbit has an eccentricity of 0.25 and an inclination of 14° with respect to the ecliptic. As of 2016, its orbital uncertainty parameter is still at 3.[1] It most recently reached perihelion, when it was nearest to the Sun, on 10 August 1926. Prior to its discovery, it was observed 29 times between 17 December 1989, and 20 September 2008.[2][5] It is a near 5:7 resonant trans-Neptunian object.

    References

    1. 1 2 3 4 "JPL Small-Body Database Browser: 78799 (2002 XW93)" (2008-09-20 last obs.). Jet Propulsion Laboratory. Retrieved 7 April 2016.
    2. 1 2 Marsden, Brian G. (2003-12-24). "MPEC 2003-Y55 : 2002 XW93". IAU Minor Planet Center. Harvard-Smithsonian Center for Astrophysics. Retrieved 2015-01-02.
    3. 1 2 "How many dwarf planets are there in the outer solar system?". Retrieved 2015-01-02.
    4. "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 2015-01-02.
    5. "78799 (2002 XW93)". Minor Planet Center. Retrieved February 2016.

    External links

    This article is issued from Wikipedia - version of the Friday, April 08, 2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.