2010 RF12 is a very small asteroid, classified as near-Earth object of the Apollo group, that passed between Earth and the Moon on 8 September 2010, at 21:12 UTC, approaching Earth within 79,000 kilometres (49,000 mi) above Antarctica.[5] The asteroid was discovered by the Mount Lemmon Survey near Tucson, Arizona on 5 September 2010 along with 2010 RX30.[1][6] Based on a short 7-day observation arc from that apparation, it was listed for 12 years on the Sentry Risk Table as the asteroid with the greatest known probability (5%) of impacting Earth.[7][note 1] 2010 RF12 was recovered in August 2022,[8][1] and now has a 12 year observation arc and a much better known orbit. There is an insignificant 1-in-63,000 chance of an Earth impact on 5 September 2120.[4]
Date | Impact probability |
JPL Horizons nominal geocentric distance (AU) |
uncertainty region (3-sigma) |
---|---|---|---|
2095-09-05 23:39 ± 00:07 | none | 0.00088 AU (132 thousand km)[3] | ±15 thousand km[9] |
Discovery[1][2] | |
---|---|
Discovered by | Mount Lemmon Srvy. |
Discovery site | Mount Lemmon Obs. |
Discovery date | 5 September 2010 |
Designations | |
MPC designation | 2010 RF12 |
Minor planet category | NEO · Apollo[1][3] |
Orbital characteristics[3] | |
Epoch 2022-Aug-09 (JD 2459800.5) | |
Uncertainty parameter 0[1][3] | |
Observation arc | 11.98 years |
Aphelion | 1.26 AU |
Perihelion | 0.86075 AU |
Semi-major axis | 1.060 AU |
Eccentricity | 0.18825 |
Orbital period (sidereal) | 1.09 yr (399 d) |
Mean anomaly | 264° |
Mean motion | 0° 54m 9s / day |
Inclination | 0.88352° |
Longitude of ascending node | 163.8° |
Time of perihelion | 2022-Nov-23[3] |
Argument of perihelion | 267.6° |
Earth MOID | 0.00067 AU (100 thousand km; 0.26 LD) |
Physical characteristics | |
Mean diameter | 7 m[4] 6–12 meters (CNEOS) |
Absolute magnitude (H) | 28.4[1][3] |
NASA's Near Earth Program estimates its size to be 7 meters (23 feet) in diameter with a mass of around 500 tonnes.[4] 2010 RF12 will make many more close approaches to Earth.[3] On 5 September 2095 it will pass 131000 ± 15000 km from Earth.[3][9] When an asteroid roughly 7-meters in diameter does impact Earth, there is very little danger of harm arising from such an impact; rather there is expected to be an impressive fireball (estimated in the Risk table as nearly 9 KT of energy release[4]) as the rock air bursts in the upper atmosphere and pebble sized fragments would likely fall to the ground at terminal velocity.[10] The power of the airburst would be somewhere between the 2–4 m Sutter's Mill meteorite and the 17 m Chelyabinsk meteor (which was 440 KT equivalent energy).[11]
Date | Impact probability (1 in) |
JPL Horizons nominal geocentric distance (AU) |
NEODyS nominal geocentric distance (AU) |
MPC nominal geocentric distance (AU) |
Find_Orb nominal geocentric distance (AU) |
uncertainty region (3-sigma) |
---|---|---|---|---|---|---|
2095-09-05 23:46 | 22 | 0.000201 AU (30.1 thousand km) | 0.0001 AU (15 thousand km)[12] | 0.00055 AU (82 thousand km) | 0.00096 AU (143,000 km)[13] | ±700 thousand km[14] |
2096-09-04 21:50 | 12000 | 1.27 AU (190 million km) | 1.47 AU (220 million km) | 0.49 AU (73 million km) | 0.14 AU (21 million km) | ±2 billion km[15] |
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