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52872 Okyrhoe

Centaur


Centaur

FieldValue
minorplanetyes
background#C7FF8F
name52872 Okyrhoe
symbol[[File:Okyrhoe symbol (bold).svg24px]] (astrological)
discovererSpacewatch
discovery_siteKitt Peak Obs.
discovered19 September 1998
mpc_name(52872) Okyrhoe
pronounced
named_afterΩκυρόη, Ωκυρρόη *Ōkyroē, Ōkyrroē*
alt_names
mp_categorycentaur
epoch13 January 2016 (JD 2457400.5)
semimajor8.3478 AU
perihelion5.7875 AU
aphelion10.908 AU
eccentricity0.30670
period24.12 yr (8809.66 d)
inclination15.665°
asc_node173.03°
arg_peri337.79°
mean_anomaly118.92°
mean_diameter
rotation
abs_magnitude10.8
albedo0.03
mean_motion/ day
orbit_ref
observation_arc5393 days (14.77 yr)
uncertainty0
jupiter_moid0.468729 AU
tisserand2.945
spectral_typeB–V

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.

Orbit and classification

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.

Naming

It was named after Ocyrhoe, the daughter of Chiron and Chariclo from Greek mythology.

Physical characteristics

Sublimation

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.

References

References

  1. 'Ocyroe' in Noah Webster (1884) ''A Practical Dictionary of the English Language''
Info: Wikipedia Source

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