(336756) 2010 NV1

(336756) 2010 NV1, provisional designation 2010 NV1, is a highly eccentric planet crossing trans-Neptunian object, approximately 44 kilometers in diameter. It is on a retrograde cometary orbit. It has a barycentric semi-major axis (average distance from the Sun) of approximately 286 AU.[lower-alpha 1]

(336756) 2010 NV1
Discovery [1][2]
Discovered byWISE
Discovery sitespace-based
Discovery date1 July 2010
Designations
(336756) 2010 NV1
2010 NV1
Distant [2] · TNO [1] · SDO
Centaur (DES)[3]
Orbital characteristics [1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 1
Observation arc5.87 yr (2,143 days)
Aphelion608.44 AU
563 AU (barycentric 2050)[lower-alpha 1]
Perihelion9.4004 AU
308.92 AU
286 AU (barycentric 2050)[lower-alpha 1]
Eccentricity0.9696
5429.66 yr (1,983,183 days)
4830 yr (barycentric 2050)[lower-alpha 1]
0.4463°
0° 0m 0.72s / day
Inclination140.78°
136.17°
132.76°
Saturn MOID1.17 AU[2]
Physical characteristics
Mean diameter
44.2±8.0 km[4]
0.057±0.030[4]
22[5]
10.6[1]

    Discovery

    This trans-Neptunian object was discovered on 1 July 2010, by NASA's space-based Wide-field Infrared Survey Explorer (WISE). It was first observed by the Mount Lemmon Survey in 2009, extending the body's observation arc by 8 months prior to its official discovery observation by WISE.[2]

    Orbit
    Orbital evolution
    EpochAphelion [lower-alpha 1]Orbital period
    1950561 AU4820 yrs
    2050563 AU4830 yrs

    2010 NV1 came to perihelion in December 2010 at a distance of 9.4 AU from the Sun.[1] As of 2016, it is 14 AU from the Sun.[5]

    It will not be 50 AU from the Sun until late 2044. After leaving the planetary region of the Solar System, 2010 NV1 will have a barycentric aphelion of 563 AU with an orbital period of 4830 years.

    In a 10 million year integration of the orbit, the nominal (best-fit) orbit and both 3-sigma clones remain outside 7.7AU (qmin) from the Sun.[3]

    Physical characteristics

    According to the surveys carried out by the NEOWISE mission, 2010 NV1 measures 44.2 kilometers in diameter and its surface has a low albedo of 0.057.[4]

    Numbering and naming

    This minor planet was numbered by the Minor Planet Center on 31 August 2012.[7] As of 2018, it has not been named.[2]

    Notes
    1. Given the orbital eccentricity of this object, different epochs can generate quite different heliocentric unperturbed two-body best-fit solutions to the semi-major axis and orbital period. For objects at such high eccentricity, the Sun's barycentric coordinates are more stable than heliocentric coordinates. Using JPL Horizons, the barycentric semi-major axis is approximately 286 AU.[6]
    gollark: Good, exactly as planned.
    gollark: Do you know about thesauri, gnobody?
    gollark: Enjoy your existential horror!
    gollark: Strictly speaking it *would* be possible to just read that information out of nondestructive neural scans of you, but this is more fun.
    gollark: Well, not my mind exactly, but since 21/01/2020 CE, 18:00 UTC, your world has been a simulation created by GTech™ to work out exactly who made which entry.

    References
    1. "JPL Small-Body Database Browser: 336756 (2010 NV1)" (2015-08-12 last obs.). Jet Propulsion Laboratory. Retrieved 1 June 2017.
    2. "336756 (2010 NV1)". Minor Planet Center. Retrieved 8 February 2017.
    3. Marc W. Buie. "Orbit Fit and Astrometric record for 336756". SwRI (Space Science Department). Retrieved 2016-02-18.
    4. Bauer, James M.; Grav, Tommy; Blauvelt, Erin; Mainzer, A. K.; Masiero, Joseph R.; Stevenson, Rachel; et al. (August 2013). "Centaurs and Scattered Disk Objects in the Thermal Infrared: Analysis of WISE/NEOWISE Observations". The Astrophysical Journal. 773 (1): 11. arXiv:1306.1862. Bibcode:2013ApJ...773...22B. doi:10.1088/0004-637X/773/1/22. Retrieved 3 February 2017.
    5. "AstDyS (418993) 2010NV1 Ephemerides". Department of Mathematics, University of Pisa, Italy. Retrieved 2016-02-18.
    6. Horizons output. "Barycentric Osculating Orbital Elements for 2010 NV1". Retrieved 2016-02-18. (Solution using the Solar System Barycenter and barycentric coordinates. Select Ephemeris Type:Elements and Center:@0)
    7. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 25 February 2018.
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