(52760) 1998 ML14 (provisional designation 1998 ML14) is a stony asteroid, classified as near-Earth object of the Apollo group and potentially hazardous asteroid, approximately 1 kilometer in diameter. It was discovered on 24 June 1998, by the LINEAR survey at the Lincoln Laboratory's Experimental Test Site in Socorro, New Mexico.[2]
Discovery[1] | |
---|---|
Discovered by | LINEAR |
Discovery site | Lincoln Lab's ETS |
Discovery date | 24 June 1998 |
Designations | |
(52760) 1998 ML14 | |
1998 ML14 | |
NEO · Apollo[1][2] · PHA[1][2] | |
Orbital characteristics[1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 15.54 yr (5,676 days) |
Aphelion | 3.9104 AU |
Perihelion | 0.9071 AU |
2.4088 AU | |
Eccentricity | 0.6234 |
3.74 yr (1,366 days) | |
21.557° | |
0° 15m 48.96s / day | |
Inclination | 2.4274° |
338.72° | |
20.324° | |
Earth MOID | 0.0167 AU · 6.5 LD |
Physical characteristics | |
Dimensions | 1.0±0.05 km[3] 0.81±0.16 km[4] 1.17 km (derived)[5] |
14.98±0.06 h[6] 14.98±0.06 h[7] 14.28±0.01 h[8] | |
0.27±0.24[4] 0.20 (assumed)[5] | |
S (Tholen)[5] | |
16.93±0.01[7] · 17.02[5][6] · 17.5[1] | |
1998 ML14 orbits the Sun at a distance of 0.9–3.9 AU once every 3 years and 9 months (1,366 days). Its orbit has an eccentricity of 0.62 and an inclination of 2° with respect to the ecliptic.[1] It is also a Mars-crossing asteroid.
Shortly after its discovery, 1998 ML14 was imaged by radar at Goldstone and Arecibo.[9]
The study showed that the asteroid has a rotation period of 15 hours, and a shape that is roughly spherical, with some steep protrusions and large craters.[6][7][8]
On 24 August 2013 it passed at a distance of 21.9 Lunar distances.[1] It was hoped to be observed by Goldstone radar.[10]
This minor planet was numbered by the Minor Planet Center on 16 February 2003.[11] As of 2018, it has not been named.[2]