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2016 CP31

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2016 CP31
Discovery
Discovered byCatalina Sky Survey
Discovery date7 February 2016
Designations
MPC designation2016 CP31
Minor planet categoryMartian L5 Martian L5
Orbital characteristics
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc1652 days (4.52 yr)
Aphelion1.61311791 AU (241.319005 Gm)
Perihelion1.4341118 AU (214.54007 Gm)
Semi-major axis1.52361487 AU (227.929540 Gm)
Eccentricity0.0587439
Orbital period (sidereal)1.88 yr (686.92802 d)
Mean anomaly122.0549°
Mean motion0° 31 26.661 /day
Inclination23.130505°
Longitude of ascending node154.488290°
Argument of perihelion329.2083°
Earth MOID0.455015 AU (68.0693 Gm)
Jupiter MOID3.39497 AU (507.880 Gm)
Physical characteristics
Mean diameter400 m
Geometric albedo0.5-0.05 (assumed)
Absolute magnitude (H)19.5

2016 CP31 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

2016 CP31 was first observed on 7 February 2016 by the Catalina Sky Survey; the Pan-STARRS 1 telescope system at Haleakala had imaged this object on 14 January 2016 without identifying it as an asteroid. Its orbit is characterized by low eccentricity (0.059), moderate inclination (23.1°) 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 131 observations with a data-arc span of 1652 days. 2016 CP31 has an absolute magnitude of 19.5 which gives a characteristic diameter of 400 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: (2016 CP31)". 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 2016 CP31

Further reading

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