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(118702) 2000 OM67

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This is an old revision of this page, as edited by Tom.Reding (talk | contribs) at 18:07, 7 April 2016 (Update infobox with JPL data (code) using AWB). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

(118702) 2000 OM67
Discovery
Discovered byMarc W. Buie and
Susan D. Kern[1]
Discovery date31 July 2000
Designations
(118702) 2000 OM67
none
SDO
Orbital characteristics[2]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 3
Observation arc2916 days (7.98 yr)
Aphelion155.57 AU (23.273 Tm)
Perihelion39.16692 AU (5.859288 Tm)
97.367124 AU (14.5659144 Tm)
Eccentricity0.59774
960.79 yr (350927 d)
2.71 km/s
10.1863°
0° 0m 3.693s / day
Inclination23.3955°
327.164°
348.434°
Earth MOID38.1548 AU (5.70788 Tm)
Jupiter MOID34.1095 AU (5.10271 Tm)
Physical characteristics
Dimensions201 km[3]
Mass8.5×1018? kg
Mean density
2.0? g/cm³
Equatorial surface gravity
0.0562? m/s²
Equatorial escape velocity
0.1063? km/s
? 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

  1. ^ List Of Centaurs and Scattered-Disk Objects
  2. ^ "JPL Small-Body Database Browser: 118702 (2000 OM67)". NASA/Jet Propulsion Laboratory. Retrieved 7 April 2016.
  3. ^ List of known trans-Neptunian objects Template:WebCite


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