(42301) 2001 UR163

(42301) 2001 UR163
Discovery[1]
Discovered by Kitt Peak (695)
Discovery date 21 October 2001
Designations
MPC designation (42301) 2001 UR163

TNO (SDO)[2]

4:9 resonance[3]
Orbital characteristics[4]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 3
Observation arc 9591 days (26.26 yr)
Aphelion 65.876 AU (9.8549 Tm)
Perihelion 36.825 AU (5.5089 Tm)
51.351 AU (7.6820 Tm)
Eccentricity 0.28287
367.98 yr (134405 d)
4.07 km/s
77.675°
0° 0m 9.643s / day
Inclination 0.75238°
302.085°
342.203°
Earth MOID 35.807 AU (5.3567 Tm)
Jupiter MOID 31.6187 AU (4.73009 Tm)
Physical characteristics
Dimensions 636 km (assumed)[5]
0.09? (assumed)
Temperature ≈39 K
(Super red; highest B−R)
B−V=1.44; V−R=0.84;
B−R=2.28
21.3[6]
4.5[4]

    (42301) 2001 UR163, also written as (42301) 2001 UR163, is likely a dwarf planet[7] that resides in the scattered disc. It was discovered on October 21, 2001 by the Deep Ecliptic Survey (DES) program at Kitt Peak. Light-curve-amplitude analysis shows only small deviations, suggesting that (42301) 2001 UR163 is a spheroid with small albedo spots.[8] Michael Brown's website lists it as a highly likely dwarf planet, but the diameter of the object has never been measured.[9]

    (42301) 2001 UR163 has the reddest color index of any object in the Solar System. On October 31, 2002, the 3.6-meter Canada–France–Hawaii Telescope observed (42301) 2001 UR163 set a record red reading of B−R=2.28. This makes (42301) 2001 UR163 even redder than Pholus, (119070) 2001 KP77, Sedna and comet C/2001 T4.

    Reddening of the spectrum is caused by cosmic irradiation by ultraviolet radiation and charged particles. Becoming bluer in the spectrum is caused by impact collisions exposing the interior of an object. In the visible spectrum, (42301) 2001 UR163 would appear orange-brown, depending on its albedo.

    It came to perihelion around 1937.[4] In 2006, it moved beyond 50 AU from the Sun. It is currently 51.9 AU from the Sun.[6]

    See also

    References

    1. ↑ Marsden, Brian G. (2001-11-14). "MPEC 2001-V57: 2001 QX322, 2001 UR163, 2001 VN71". IAU Minor Planet Center. Harvard-Smithsonian Center for Astrophysics. Retrieved 2010-01-06. (K01UG3R*)
    2. ↑ "List Of Centaurs and Scattered-Disk Objects". Minor Planet Center. Retrieved 2008-09-25.
    3. ↑ Marc W. Buie (2003-10-23). "Orbit Fit and Astrometric record for 42301". SwRI (Space Science Department). Retrieved 2008-09-25.
    4. 1 2 3 "JPL Small-Body Database Browser: 42301 (2001 UR163)" (2003-10-23 last obs). Retrieved 5 April 2016.
    5. ↑ Wm. Robert Johnston. "List of Known Trans-Neptunian Objects". Johnston's Archive. Archived from the original on 24 June 2009. Retrieved 2009-08-28.
    6. 1 2 "AstDyS (42301) 2001UR163 Ephemerides". Department of Mathematics, University of Pisa, Italy. Archived from the original on 2009-04-18. Retrieved 2009-03-19.
    7. ↑ Gonzalo Tancredi & Sofía Favre (October 13, 2008). "Dwarf Planet & Plutoid Headquarters". Portal Uruguayo de Astronomía. Retrieved 2010-09-22. (Which are the dwarfs in the Solar System?)
    8. ↑ Tancredi, G., & Favre, S. (2008) Which are the dwarfs in the Solar System?. Depto. Astronomía, Fac. Ciencias, Montevideo, Uruguay; Observatorio Astronómico Los Molinos, MEC, Uruguay. Retrieved 10-08-2011
    9. ↑ Michael E. Brown. "How many dwarf planets are there in the outer solar system? (updates daily)". California Institute of Technology. Retrieved 31 August 2016.
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