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2011 UB256

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2011 UB256
Discovery
Discovered byPan-STARRS
Discovery date29 October 2011
Designations
MPC designation2011 UB256
Minor planet categoryMartian L5 Martian L5
Orbital characteristics
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc6265 days (17.15 yr)
Aphelion1.631894031 AU (244.1278722 Gm)
Perihelion1.4154896 AU (211.75423 Gm)
Semi-major axis1.523691798 AU (227.9410486 Gm)
Eccentricity0.0710132
Orbital period (sidereal)1.88 yr (686.980044 d)
Mean anomaly180.60444°
Mean motion0° 31 26.518 /day
Inclination24.30270°
Longitude of ascending node58.781126°
Argument of perihelion7.58178°
Earth MOID0.428887 AU (64.1606 Gm)
Jupiter MOID3.5641 AU (533.18 Gm)
Physical characteristics
Mean diameter300 m
Geometric albedo0.5-0.05 (assumed)
Absolute magnitude (H)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).

Discovery, orbit and physical properties

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.

Mars trojan and orbital evolution

Recent calculations indicate that it is a stable L5 Mars trojan. It may not be a member of the so-called Eureka family.

Mars trojan

L4 (leading):

L5 (trailing):

See also

References

  1. ^ "JPL Small-Body Database Browser: (2011 UB256)". Jet Propulsion Laboratory. Retrieved 12 January 2021.
  2. ^ Christou, Apostolos A.; Borisov, Galin; Dell'Oro, Aldo; Jacobson, Seth A.; Cellino, Alberto; Unda-Sanzana, Eduardo (January 2020). "Population control of Mars Trojans by the Yarkovsky & YORP effects". Icarus. 335 (1): 113370 (34 pages). arXiv:1907.12858. Bibcode:2020Icar..33513370C. doi:10.1016/j.icarus.2019.07.004. S2CID 198985887.
  3. Christou, Apostolos A.; Borisov, Galin; Dell'Oro, Aldo; Cellino, Alberto; Devogèle, Maxime (January 2021). "Composition and origin of L5 Trojan asteroids of Mars: Insights from spectroscopy". Icarus. 354 (1): 113994 (22 pages). arXiv:2010.10947. Bibcode:2021Icar..35413994C. doi:10.1016/j.icarus.2020.113994. S2CID 224814529.
  4. de la Fuente Marcos, Carlos; de la Fuente Marcos, Raúl (March 2021). "Using Mars co-orbitals to estimate the importance of rotation-induced YORP break-up events in Earth co-orbital space". Monthly Notices of the Royal Astronomical Society. 501 (4): 6007–6025. arXiv:2101.02563. Bibcode:2021MNRAS.501.6007D. doi:10.1093/mnras/stab062.
  5. ^ MPC data on 2011 SP189
Further reading

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