(179806) 2002 TD66 (also written 2002 TD66) is a sub-kilometer asteroid, classified as near-Earth object of the Apollo group. It was discovered on 5 October 2002, by the LINEAR project at Lincoln Laboratory's ETS in Socorro, New Mexico.[1] It was announced on 7 October 2002 and appeared later that day on the JPL current risk page.
Discovery | |
---|---|
Discovered by | LINEAR |
Discovery site | Lincoln Lab ETS |
Discovery date | 5 October 2002 |
Designations | |
NEO · Apollo | |
Orbital characteristics[1] | |
Epoch 13 January 2016 (JD 2457400.5) | |
Uncertainty parameter 0 | |
Observation arc | 2017 days (5.52 yr) |
Aphelion | 2.8505 AU (426.43 Gm) |
Perihelion | 0.86543 AU (129.466 Gm) |
1.8580 AU (277.95 Gm) | |
Eccentricity | 0.53421 |
2.53 yr (925.03 d) | |
55.037° | |
0° 23m 21.048s / day | |
Inclination | 4.9211° |
335.73° | |
125.66° | |
Earth MOID | 0.00603808 AU (903,284 km) |
Jupiter MOID | 2.35661 AU (352.544 Gm) |
Physical characteristics | |
Dimensions | 300 meters[2] 270–590 meters H |
9.455 h (0.3940 d)[2][1] | |
20.2[1] | |
Due to the proximity of its orbit to Earth and its estimated size, this object has been classified as a potentially hazardous asteroid (PHA) by the Minor Planet Center in Cambridge, Massachusetts. In November 2006 there were 823 PHAs known. As of October 2011[update], there are 1261 PHAs known.[3] 2002 TD66 was removed from the Sentry Risk Table on October 10, 2002.[4] A Doppler observation[1] has helped produce a well known trajectory with a condition code (Uncertainty Parameter U) of 0.[1]
Based on an absolute magnitude (H) of 20.2,[1] the asteroid is estimated to be between 270 and 590 meters in diameter. Radar astronomy shows it is a contact binary asteroid with a diameter of 300 meters and a rotation period of 9.5 hours.[2]
On February 26, 2008, 2002 TD66 passed 0.04282 AU (6,406,000 km; 3,980,000 mi) from Earth.[5] The asteroid also comes close to Venus, Mars, and dwarf planet Ceres.[5]