2012 FC71

2012 FC71, also written 2012 FC71, is a small asteroid trapped in a Kozai resonance with the Earth.[4]

2012 FC71
Discovery[1]
Discovered byMt. Lemmon Survey
A. Boattini
(unofficial credits)
Discovery date31 March 2012
Designations
2012 FC71
Orbital characteristics[2]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter
Observation arc21 days
Aphelion1.0750 AU
Perihelion0.9008 AU
0.9879 AU
Eccentricity0.0882
0.98 yr (359 days)
150.11°
 0m 13.68s / day
Inclination4.9430°
38.142°
348.30°
Earth MOID0.0566 AU (22.1 LD)
Physical characteristics
Dimensions20–40 m[a][3]
25.2[2]

    Discovery, orbit and physical properties

    It was first observed on 31 March 2012 by Andrea Boattini, observing for the Mt. Lemmon Survey.[5][6] Its orbit is characterized by low eccentricity (0.088), low inclination (4.97º) and a semi-major axis of 0.9895 AU.[6] It is an Aten asteroid but also an Earth crosser. As of 11 May 2013 its orbit is based on 35 observations spanning a data-arc of 21 days.

    Kozai resonator and future orbital evolution

    2012 FC71 is locked in a Kozai resonance and as such it has a very slow orbital evolution and it will remain relatively unperturbed for hundreds of thousands of years.[4] It had a close encounter with the Earth on 18 April 2012 at 0.076 AU and another on 17 May 2013 at 0.0581 AU.

    Origin

    It may have been originated within the Venus-Earth-Mars region or in the main asteroid belt like other Near-Earth Objects, then transitioned to an Amor-class asteroid before entering Earth's co-orbital region.[4]

    gollark: Velvet: do you still have that 3G SAltkin thing? I'd prefer that.
    gollark: I'm working on my stupidly messy SAltkin prizekin madness lineage.
    gollark: A 2G GoN from SAltkin.
    gollark: Free for a CB *ND*.
    gollark: I like that.

    See also

    Notes

    • ^ This is assuming an albedo of 0.20–0.04.

    References

    1. "2012 FC71". Minor Planet Center. Retrieved 2 February 2017.
    2. "JPL Small-Body Database Browser: 2012 FC71" (2012-04-21 last obs.). Jet Propulsion Laboratory. Retrieved 2 February 2017.
    3. "Absolute Magnitude (H)". NASA/JPL. Retrieved 2 February 2017.
    4. de la Fuente Marcos, C.; de la Fuente Marcos, R. (July 2013). "A resonant family of dynamically cold small bodies in the near-Earth asteroid belt". Monthly Notices of the Royal Astronomical Society: Letters. 434 (1): L1–L5. arXiv:1305.2825. Bibcode:2013MNRAS.434L...1D. doi:10.1093/mnrasl/slt062.
    5. Discovery MPEC
    6. MPC data on 2012 FC71
    Further reading
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