(52872) Okyrhoe
Asteroid (52872) Okyrhoe |
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Properties of the orbit ( animation ) | |
Orbit type | centaur |
Major semi-axis | 8.35 AU |
eccentricity | 0.306 |
Perihelion - aphelion | 5.795 AU - 10.905 AU |
Inclination of the orbit plane | 15.7 ° |
Sidereal period | 24.13 years |
Mean orbital velocity | 10.06 km / s |
Physical Properties | |
Absolute brightness | 10.8 mag |
history | |
Explorer | Spacewatch |
Date of discovery | September 19, 1998 |
Another name | 1998 SG 35 |
Source: Unless otherwise stated, the data comes from JPL Small-Body Database Browser . The affiliation to an asteroid family is automatically determined from the AstDyS-2 database . Please also note the note on asteroid items. |
(52872) Okyrhoe is a planetoid that was discovered on September 19, 1998 as part of the Spacewatch program and belongs to the group of centaurs . The asteroid will orbit the sun on a moderately eccentric orbit in a good 24 years . The orbital eccentricity of its orbit is 0.306, which is 15.67 ° inclined to the ecliptic .
It is assumed that the Okyrhoe, like the two centaurs (2060) Chiron and (60558) Echeclus, also has cometary activities.
In mythology, Okyrhoe was the daughter of the centaur (2060) Chiron and the nymph (10199) Chariklo , which are the two largest confirmed centaurs in astronomy, both of which also have a fine ring system. The name means "quickly running" or "quickly flowing".
See also
Individual evidence
- ^ Trigo-Rodríguez: A continuous follow-up of Centaurs, and dormant comets: looking for cometary activity. (PDF) European Planetary Science Congress. 2008. Retrieved October 12, 2008.