(523794) 2015 RR245

(523794) 2015 RR245
2015 RR245 imaged by the Hubble Space Telescope in October 2020
Discovery
Discovered byOSSOS
Michele T. Bannister et al.
Discovery siteMauna Kea Obs.
Discovery date9 September 2015
Designations
(523794) 2015 RR245
TNO · SDO · resonant (2:9)
p-DP · distant
Orbital characteristics
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 3
Observation arc13.10 yr (4,786 d)
Earliest precovery date15 October 2004
Aphelion128.80 AU
Perihelion33.943 AU
81.373 AU
Eccentricity0.5829
734.05 yr (268,113 d)
323.86°
0° 0m 4.68s / day
Inclination7.5755°
211.68°
≈ 21 August 2092
±3 days
261.02°
Physical characteristics
≈500 km
≈630 km
500–870 km assuming a single object
0.12 (assumed)
0.11 (assumed)
0.135 (assumed)
neutral
G–R=0.59±0.11
21.2 (perihelic)
3.6±0.1 (Hr)
4.01
4.1

    (523794) 2015 RR245, provisional designation 2015 RR245, is a large trans-Neptunian object of the Kuiper belt in the outermost regions of the Solar System. It was discovered on 9 September 2015, by the Outer Solar System Origins Survey at Mauna Kea Observatories on the Big island of Hawaii, in the United States. The object is in a rare 2:9 resonance with Neptune and measures approximately 600 kilometers in diameter. 2015 RR245 was suspected to have a satellite according to a study announced by Noyelles et al. in a European Planetary Science Congress meeting in 2019.