2014 FC69

2014 FC69
Discovery[1]
Discovery date 25 March 2014
Designations
MPC designation 2014 FC69
SDO[2]
Orbital characteristics[1]
Epoch 27 June 2015 (JD 2457200.5)
Uncertainty parameter 7
Observation arc 302 days
Aphelion 106.917 AU
Perihelion 40.222 AU
73.569 AU
Eccentricity 0.45328
631.04 yr (230,490 days)
83.561°
Inclination 30.066°
250.19°
191.279°
Physical characteristics
Dimensions 300–700 km
4.6[1]

    2014 FC69 is a trans-Neptunian object that resides in the scattered disc. It was discovered on 25 March 2014. Because of its great distance and short observation arc of 302 days, 2014 FC69's orbit is too poorly determined to know whether it is in an orbital resonance with Neptune.

    Distance

    Based on the best-fit (albeit uncertain) orbital solution, 2014 FC69 last came to perihelion around 1869,[1] and is currently about 84.0 AU from the Sun. Other than long-period comets, it is currently about the fifth-most-distant known large body in the Solar System, after V774104 (~103 AU), Eris and Dysnomia (96.3 AU), 2007 OR10 (87.4 AU), and Sedna (85.9 AU).

    Most-distant known Trans-Neptunian objects (TNOs) in the Solar System at present time
    Solar System body V774104 Eris 2007 OR10 Sedna 2014 FC69 2006 QH181 2012 VP113 2013 FY27 2010 GB174 2000 CR105
    Distance
    from the Sun
    (AU)
    Current ~103 96.3 87.4 85.8 84.1 83.3 83.3 80.2 70.6 60.4
    Perihelion ? 37.9 33.0 76.1 40.2 38.3 80.5 35.5 48.5 44.2
    Aphelion ? 97.7 100.7 ~936 106.9 96.7 ~446 83.7 ~673 ~416
    Magnitude (vmag) 24? 18.7 21.4 21.0 23.8 23.5 23.4 22.2 25.2 24.1
    Current distance from Sun is at least twice Neptune's semimajor axis [3]

    See also

    References

    1. 1 2 3 4 "JPL Small-Body Database Browser: (2014 FC69)" (2015-01-21 last obs). Retrieved 2015-11-12.
    2. "MPEC 2015-C52 : 2014 FC69". IAU Minor Planet Center. 2015-02-11. Retrieved 2015-11-12.
    3. AstDyS, Objects at least two Neptune distances from Sun

    External links


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