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(472271) 2014 UM33, provisionally designated 2010 TQ182, is a trans-Neptunian object residing in the outer Kuiper belt. It was discovered on October 22, 2014, by the Mount Lemmon Survey.

(472271) 2014 UM33
Discovery[1]
Discovered byMount Lemmon Survey (Pan-STARRS)
Discovery siteMount Lemmon
Discovery date22 October 2014
Designations
MPC designation
(472271) 2014 UM33
Alternative designations
2014 UM33 · 2010 TQ182
Minor planet category
TNO
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 3
Observation arc11.86 yr (4,332 days)
Earliest precovery date16 October 2003
Aphelion49.631 AU
Perihelion36.163 AU
Semi-major axis
42.897 AU
Eccentricity0.1570
Orbital period (sidereal)
280.96 yr (102,622 days)
Mean anomaly
269.23°
Mean motion
0° 0m 12.6s / day
Inclination17.403°
Longitude of ascending node
236.58°
Argument of perihelion
269.24°
Physical characteristics
Dimensions320–720 km[3]
478 km[4]
607 km[5]
220–880[6]
Apparent magnitude
21–22
Absolute magnitude (H)
4.9[1][2]
5.2[4]

    It is approximately the size of 2 Pallas in the asteroid belt. On August 18, 2015, 2014 UM33 was found to have been discovered over four years previously, with the designation 2010 TQ182. This extended its observation arc to over 4 years, and then precovery observations were found using the Sloan Digital Sky Survey from 2009.


    See also



    References


    1. "472271 (2014 UM33)". Minor Planet Center. Retrieved 25 October 2016.
    2. "JPL Small-Body Database Browser: 472271 (2014 UM33)" (2015-08-26 last obs.). Jet Propulsion Laboratory. Retrieved 25 October 2016.
    3. "Glossary: Absolute Magnitude (H)". JPL. NASA. Archived from the original on 2 March 2001. Retrieved 2 January 2015.
    4. Brown, Mike. "How many dwarf planets are there in the outer solar system? (updates daily)". www.gps.caltech.edu. Caltech. Retrieved 21 July 2015.
    5. Wm. Robert Johnston (24 March 2015). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 21 July 2015.
    6. Bruton, Dan. "Conversion of Absolute Magnitude to Diameter". SFASU – Department of Physics and Astronomy. Archived from the original on 18 December 2008. Retrieved 18 August 2015.




    На других языках


    [de] (472271) 2014 UM33

    (472271) 2014 UM33 ist ein großes transneptunisches Objekt, das bahndynamisch als erweitertes Scattered Disc Object (DO) oder als Cubewano eingestuft wird. Aufgrund seiner Größe ist der Asteroid ein Zwergplanetenkandidat.
    - [en] (472271) 2014 UM33



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