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5145 Pholus

5145 Pholus
Discovery 
Discovered by Spacewatch
unaccredited:
D. L. Rabinowitz
Discovery site Kitt Peak National Obs.
Discovery date 9 January 1992
Designations
MPC designation 5145 Pholus
Pronunciation /ˈfləs/ (foe'-ləs)
Named after
Pholus
(Greek mythology)
1992 AD
Centaur
Saturn crosser
Uranus crosser
Neptune crosser
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 1
Observation arc 31.74 yr (11,593 days)
Aphelion 32.038 AU
Perihelion 8.7184 AU
20.378 AU
Eccentricity 0.5722
91.99 yr (33,601 days)
Average orbital speed
6.01 km/s
97.208°
0° 0m 38.52s / day
Inclination 24.705°
119.30°
355.10°
Jupiter MOID 3.469 AU
Jupiter Tisserand parameter 3.20
Physical characteristics
Dimensions 99±15 km
165.03 km (derived)
185±16 km
190 km
9.977 h
9.980 h
9.982 h
9.983 h
0.04
0.044±0.013
0.057 (assumed)
0.155±0.076
Tholen = Z  · C
RR  · RR-U 
B−V=1.19
V−R=0.78
21.45
7.1
7.198±0.056 (R)
7.63
7.64
7.68±0.28
7.78±0.09
7.83±0.12

5145 Pholus (/ˈfləs/; from Greek: Φόλος) provisional designation 1992 AD, is an eccentric centaur in the outer Solar System, approximately 100 to 200 kilometers in diameter, that crosses the orbit of both Saturn and Neptune. It was discovered on 9 January 1992, by American astronomer David L. Rabinowitz (unaccredited) of UA's Spacewatch Project at Kitt Peak National Observatory, and named after the mythological creature Pholus.

The minor planet orbits the Sun at a distance of 8.7–32.0 AU once every 91 years and 12 months (33,601 days). Its orbit has an eccentricity of 0.57 and an inclination of 25° with respect to the ecliptic. The first precovery was taken at the Australian Siding Spring Observatory in 1977, extending the centaur's observation arc by 15 years prior to its discovery. Pholus has not come within one astronomical unit of a planet since 764 BC, and will not until 5290. It is believed that Pholus originated in the Kuiper belt.


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