2010 RF43
Discovery[1] | |
---|---|
Discovered by | S. D. Benecchi |
Discovery site | Las Campanas Observatory, Chile |
Discovery date | September 6, 2010[2] |
Designations | |
MPC designation | 2010 RF43 |
Scattered disc[3][4] | |
Orbital characteristics[3] | |
Epoch 13 January 2016 (JD 2457400.5) | |
Uncertainty parameter 5 | |
Observation arc | 743 days (2.03 yr) |
Aphelion | 61.726 AU (9.2341 Tm) |
Perihelion | 36.853 AU (5.5131 Tm) |
49.290 AU (7.3737 Tm) | |
Eccentricity | 0.25231 |
346.05 yr (126396 d) | |
94.491° | |
0° 0m 10.254s /day | |
Inclination | 30.698° |
25.208° | |
191.70° | |
Known satellites | none |
Earth MOID | 35.8518 AU (5.36335 Tm) |
Jupiter MOID | 31.4497 AU (4.70481 Tm) |
Proper orbital elements | |
Precession of the ascending node | 24.527 arcsec / yr |
Physical characteristics | |
Dimensions |
380–860[5] 581 km in diameter.[6] |
4.1 | |
|
2010 RF43, also written 2010 RF43, is a trans-Neptunian object with an absolute magnitude of 4.1.[3] It was discovered in 2010 by S. D. Benecchi at the Las Campanas Observatory in Chile.[1] 2010 RF43 is currently classified as a scattered disc object.[3][4] Astronomer Mike Brown lists it as highly likely a dwarf planet.[6]
References
- 1 2 "MPEC 2011-U09 : 2010 RF43". Minorplanetcenter.net. Retrieved 2014-06-13.
- ↑ (2010 RF43). "Small Solar System Body (2010 RF43)". Comets-asteroids.findthedata.org. Retrieved 2014-06-13.
- 1 2 3 4 Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Retrieved 31 March 2016.
- 1 2 Marc W. Buie. "Orbit Fit and Astrometric record for 10RF43" (2013-02-13 using 34 of 36 observations). SwRI (Space Science Department). Retrieved 2013-02-13.
- ↑ "Absolute Magnitude (H)". NASA / JPL. Retrieved 2010-02-13.
- 1 2 Michael E. Brown. "How many dwarf planets are there in the outer solar system? (updates daily)". California Institute of Technology. Archived from the original on 2011-10-18. Retrieved 2011-08-25.
External links
- 2010 RF43 at the JPL Small-Body Database
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