Discovery | |
---|---|
Discovered by | Pan-STARRS |
Discovery date | 12 June 2013 |
Designations | |
2013 LX28 | |
Orbital characteristics [2] [3] [4] | |
Epoch 13 January 2016 (JD 2457400.5) | |
Uncertainty parameter 1 | |
Aphelion | 1.4543719 AU (217.57094 Gm) |
Perihelion | 0.5488609 AU (82.10842 Gm) |
1.00161641 AU (149.839682 Gm) | |
Eccentricity | 0.4520249 |
1.00 yr (366.14 d) | |
61.458811° | |
0° 58m 59.602s /day | |
Inclination | 49.97420° |
76.679354° | |
345.77666° | |
Earth MOID | 0.373137 AU (55.8205 Gm) |
Jupiter MOID | 3.8786 AU (580.23 Gm) |
Physical characteristics | |
Dimensions | 130–300 m [a] [5] |
21.7 [2] | |
2013 LX28, is an asteroid, classified as near-Earth object of the Apollo group that is a temporary quasi-satellite of the Earth, the third known Earth quasi-satellite. [6] [7]
2013 LX28 was discovered on 12 June 2013. As of September 2014, it has been observed 26 times with a data-arc span of 349 days. It is an Apollo asteroid and its semi-major axis (1.0016 AU) is very similar to that of the Earth but it has relatively high eccentricity (0.4521) and high orbital inclination (49.9761°). With an absolute magnitude of 21.7, it has a diameter in the range 130–300 m (for an assumed albedo range of 0.04–0.20).
2013 LX28 has been identified as an Earth quasi-satellite following a kidney-shaped retrograde orbit around the Earth. [6] [7]