(65407) 2002 RP120
Appearance
Discovery | |
---|---|
Discovered by | Brian A. Skiff (LONEOS) |
Discovery date | 4 September 2002 |
Designations | |
Damocloid Scattered disk object | |
Orbital characteristics [1] | |
Epoch 13 January 2016 (JD 2457400.5) | |
Uncertainty parameter 2 | |
Observation arc | 1225 days (3.35 yr) |
Aphelion | 107.08 AU (16.019 Tm) |
Perihelion | 2.4759 AU (370.39 Gm) |
54.780 AU (8.1950 Tm) | |
Eccentricity | 0.95480 |
405.45 yr (148092 d) | |
Average orbital speed | 3.98 km/s |
11.779° | |
0° 0m 8.751s / day | |
Inclination | 119.00° |
39.238° | |
357.99° | |
Earth MOID | 1.48322 AU (221.887 Gm) |
Jupiter MOID | 2.50008 AU (374.007 Gm) |
Physical characteristics | |
Dimensions | 14.6 km[1] |
7.3 ± 1.4 km | |
Mass | 3.1×1015 kg |
200 h (8.3 d)[1] | |
0.098 ± 0.036[1] | |
Temperature | ~ 37 K |
12.3[1] | |
(65407) 2002 RP120 (also written (65407) 2002 RP120) is a damocloid, which means it is also a member of a small group of retrograde minor planets. Aside from being a damocloid, it is also a scattered-disc object – a trans-Neptunian object with a very eccentric orbit, probably ejected from the ecliptic by Neptune.
References
External links
- Orbital simulation from JPL (Java)
- Horizons Ephemeris
- (65407) 2002 RP120 at the JPL Small-Body Database