Minorplanet: | yes |
Background: |
|
52872 Okyrhoe | |
Symbol: | (astrological) |
Discovered: | 19 September 1998 |
Mpc Name: | (52872) Okyrhoe |
Named After: | Ωκυρόη, Ωκυρρόη Ōkyroē, Ōkyrroē |
Epoch: | 13 January 2016 (JD 2457400.5) |
Semimajor: | 8.3478AU |
Perihelion: | 5.7875AU |
Aphelion: | 10.908abbr=onNaNabbr=on |
Eccentricity: | 0.30670 |
Period: | 24.12 yr (8809.66 d) |
Inclination: | 15.665° |
Asc Node: | 173.03° |
Arg Peri: | 337.79° |
Abs Magnitude: | 10.8 |
Albedo: | 0.03 |
Mean Motion: | / day |
Observation Arc: | 5393 days (14.77 yr) |
Uncertainty: | 0 |
Jupiter Moid: | 0.468729AU |
Tisserand: | 2.945 |
52872 Okyrhoe is a centaur orbiting in the outer Solar System between Jupiter and Saturn. It was discovered on 19 September 1998, by the Spacewatch survey at Kitt Peak Observatory in Arizona, United States, and named after Ocyrhoe from Greek mythology.
Centaurs have short dynamical lives due to strong interactions with the giant planets. Okyrhoe is estimated to have an orbital half-life of about 670 thousand years. Of objects listed as a centaur by the Minor Planet Center (MPC), JPL, and the Deep Ecliptic Survey (DES), Okyrhoe has the second smallest perihelion distance of a numbered centaur. Numbered centaur has a smaller perihelion distance.
It was named after Ocyrhoe, the daughter of Chiron and Chariclo from Greek mythology.
Okyrhoe passed perihelion in early 2008, and exhibited significant magnitude variations during March and April 2008. This could be a sign of sublimation of volatiles.