| Discovery | |
|---|---|
| Discovered by | Pan-STARRS |
| Discovery date | 29 October 2011 |
| Designations | |
| Martian L5 | |
| Orbital characteristics | |
| 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 is a small asteroid and Mars trojan orbiting near the L5 point of Mars (60 degrees behind Mars on its orbit).
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. Its orbit is characterized by low eccentricity (0.071), moderate inclination (24.3°) and a semi-major axis of 1.52 AU. 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. 2011 UB256 has an absolute magnitude of 19.9 which gives a characteristic diameter of 300 m.
Recent calculations indicate that it is a stable L5 Mars trojan. It may not be a member of the so-called Eureka family.
L4 (leading):
L5 (trailing):