54598 Bienor

54598 Bienor
Discovery
Discovered byDES
Discovery siteCerro Tololo Obs.
Discovery date27 August 2000
Designations
(54598) Bienor
Pronunciation/bˈnɔːr/
Named after
Biēnor
2000 QC243
Centaur
AdjectivesBienorian /b.ɪˈnɔːriən/
Symbol (astrological)
Orbital characteristics
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc24775 days (67.83 yr)
Aphelion19.715 AU (2.9493 Tm)
Perihelion13.172 AU (1.9705 Tm)
16.444 AU (2.4600 Tm)
Eccentricity0.19894
66.68 yr (24355 d)
7.26 km/s
318.473°
0° 0m 53.039s / day
Inclination20.745°
337.728°
153.374°
Earth MOID12.199 AU (1.8249 Tm)
Jupiter MOID7.873 AU (1.1778 Tm)
TJupiter3.575
Physical characteristics
Dimensionsa,b,c=127±5, 55±4, 45±4 km
187.5±15.5 km
198 km
207±30 km
9.1736 ± 0.0002 h
9.14 h (0.381 d)
0.03–0.05
0.05±0.019 0.065±0.005
Temperature~ 69 K
BR
B–V = 0.711±0.059
V–R = 0.476±0.046
~ 19.2
7.5

    54598 Bienor /bˈnɔːr/ is a centaur that grazes the orbit of Uranus. It is named after the mythological centaur Bienor. Its closest approach to the Sun (perihelion) is 13.2 AU. As of 2020, Bienor is 14.2 AU from the Sun and will reach perihelion in January 2028. It measured approximately 198 kilometers (120 miles) in diameter. Through the analysis of rotational light curves and stellar occultations, it has been determined that the object has a highly elongated ellipsoidal shape. Its light curve is consistent with surface deformations, regions with significant albedo variations, or even the possible presence of a moon.