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From Wikipedia, the free encyclopedia
2011 UB256 is a small asteroid and Mars trojan orbiting near the L5 point of Mars (60 degrees behind Mars on its orbit).[2][3][4]
Discovery | |
---|---|
Discovered by | Pan-STARRS |
Discovery date | 29 October 2011 |
Designations | |
2011 UB256 | |
Martian L5 | |
Orbital characteristics[1] | |
Epoch 31 May 2020 (JD 2459000.5) | |
Uncertainty parameter 0 | |
Observation arc | 6265 days (17.15 yr) |
Aphelion | 1.631894031 AU (244.1278722 Gm) |
Perihelion | 1.4154896 AU (211.75423 Gm) |
1.523691798 AU (227.9410486 Gm) | |
Eccentricity | 0.0710132 |
1.88 yr (686.980044 d) | |
180.60444° | |
0° 31m 26.518s /day | |
Inclination | 24.30270° |
58.781126° | |
7.58178° | |
Earth MOID | 0.428887 AU (64.1606 Gm) |
Jupiter MOID | 3.5641 AU (533.18 Gm) |
Physical characteristics | |
300 m | |
0.5-0.05 (assumed) | |
19.9 | |
2011 UB256 was first observed on 29 October 2011 by the Pan-STARRS 1 telescope system at Haleakala; the Apache Point-Sloan Digital Sky Survey had imaged this object on 31 March 2003 without identifying it as an asteroid.[5] Its orbit is characterized by low eccentricity (0.071), moderate inclination (24.3°) and a semi-major axis of 1.52 AU.[5] Upon discovery, it was classified as Mars-crosser by the Minor Planet Center. Its orbit is well determined as it is currently (January 2021) based on 64 observations with a data-arc span of 6265 days.[1] 2011 UB256 has an absolute magnitude of 19.9 which gives a characteristic diameter of 300 m.[1]
Recent calculations indicate that it is a stable L5 Mars trojan.[2] It may not be a member of the so-called Eureka family.
L4 (leading):
L5 (trailing):
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