Discovery[1]
|
|
---|---|
Discovered by | Lincoln Laboratory ETS, New Mexico (704) |
Discovery date | 5 October 1999 |
Designations
|
|
MPC designation | (237442) 1999 TA10 |
Minor planet category |
Amor asteroid (NEO)[2] |
Epoch July 23, 2010 (2455400.5) | |
Aphelion | 1.8694 AU (Q) |
Perihelion | 1.1420 AU (q) |
Semi-major axis | 1.5057 AU (a) |
Eccentricity | 0.24155 |
Orbital period | 1.85 yr 674.85 days |
Mean anomaly | 355.60° (M) |
Inclination | 20.842° |
Longitude of ascending node | 214.71° |
Argument of perihelion | 84.739° |
Physical characteristics
|
|
Dimensions | 500-1500 meters[2][3] |
Sidereal rotation period |
14 hr(?)[2] |
Albedo | unknown |
Apparent magnitude | 16.77 (close approach) to 22.29 |
Absolute magnitude (H) | 17.9[2] |
(237442) 1999 TA10, provisionally known as 1999 TA10, is a near-Earth object (NEO) from the Amor asteroid group.[2] It is suspected of being an inner fragment of the differentiated asteroid 4 Vesta.[4]
Given an absolute magnitude (H) of 17.9,[2] and that the albedo is unknown, this NEO could vary from 500 to 1500 meters in diameter.[3]
1999 TA10 was discovered on 5 October 1999 at apparent magnitude 17.7,[1] when it was only 0.39 AU from the Earth.[5] In 2010, it came within 0.3 AU of the Earth.[5] During the 2010 close approach, NASA Infrared Telescope Facility (NASA IRTF) studies suggested that 1999 TA10 originated from the interior of Vesta.[4] The next close approach will be in 2023.[5] In 2086, it will come within 0.017 AU (2,500,000 km; 1,600,000 mi) of Mars.[5]