(118702) 2000 OM67
Discovery | |
---|---|
Discovered by |
Marc W. Buie and Susan D. Kern[1] |
Discovery date | 31 July 2000 |
Designations | |
MPC designation | (118702) 2000 OM67 |
none | |
SDO | |
Orbital characteristics[2] | |
Epoch 13 January 2016 (JD 2457400.5) | |
Uncertainty parameter 3 | |
Observation arc | 2916 days (7.98 yr) |
Aphelion | 155.57 AU (23.273 Tm) |
Perihelion | 39.16692 AU (5.859288 Tm) |
97.367124 AU (14.5659144 Tm) | |
Eccentricity | 0.59774 |
960.79 yr (350927 d) | |
Average orbital speed | 2.71 km/s |
10.1863° | |
0° 0m 3.693s / day | |
Inclination | 23.3955° |
327.164° | |
348.434° | |
Earth MOID | 38.1548 AU (5.70788 Tm) |
Jupiter MOID | 34.1095 AU (5.10271 Tm) |
Physical characteristics | |
Dimensions | 201 km[3] |
Mass | 8.5×1018? kg |
Mean density | 2.0? g/cm³ |
Equatorial surface gravity | 0.0562? m/s² |
Equatorial escape velocity | 0.1063? km/s |
Sidereal rotation period | ? d |
0.10? | |
Temperature | ~28 K |
? | |
6.8 | |
|
(118702) 2000 OM67, also written as (118702) 2000 OM67, is a trans-Neptunian object that resides in the scattered disc region of the Solar System. It was discovered on July 31, 2000 by Marc Buie and Susan Kern.
See also
References
- ↑ List Of Centaurs and Scattered-Disk Objects
- ↑ "JPL Small-Body Database Browser: 118702 (2000 OM67)". NASA/Jet Propulsion Laboratory. Retrieved 7 April 2016.
- ↑ List of known trans-Neptunian objects Archived June 21, 2007, at WebCite
External links
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