(496315) 2013 GP136

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(496315) 2013 GP136
Discovery [1] [2]
Discovered by OSSOS
Discovery site Mauna Kea Obs.
Discovery date8 February 2013
Designations
(496315) 2013 GP136
o3e39 [3]
TNO [1]  · SDO [4]
Orbital characteristics [1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 3
Observation arc 4.29 yr (1,566 days)
Aphelion 268.46 AU
Perihelion 41.073 AU
154.76 AU
149.8 AU [5]
Eccentricity 0.7346
1925 yr (703,239 days)
356.44°
0° 0m 1.8s / day
Inclination 33.467°
210.71°
42.316°
Physical characteristics
Dimensions 212 km [4]
6.6 [1]

    2013 GP136 is a trans-Neptunian object from the scattered disc in the outermost reaches of the Solar System. It is approximately 212 kilometers in diameter. It was discovered on 8 February 2013, by the Outer Solar System Origins Survey at the Mauna Kea Observatories on the island of Hawaii, United States. [2]

    Contents

    Orbit and classification

    2013 GP136 orbits the Sun at a distance of 41.1–268.5 AU once every 1925 years and 4 months (703,239 days). Its orbit has an eccentricity of 0.73 and an inclination of 33° with respect to the ecliptic. [1]

    It was mentioned in a 2016 paper by Malhotra of the Lunar and Planetary Laboratory, at the University of Arizona, as a detached object with a perihelion greater than 40 AUs, a 6:1 orbital period ratio with 90377 Sedna, and in a possible 9:1 mean-motion resonance with a hypothetical large Planet Nine. [5]

    See also

    References

    1. 1 2 3 4 5 "JPL Small-Body Database Browser: 496315 (2013 GP136)" (2017-05-24 last obs.). Jet Propulsion Laboratory . Retrieved 30 July 2017.
    2. 1 2 "496315 (2013 GP136)". Minor Planet Center. Retrieved 30 July 2017.
    3. ↑ Shankman, Cory; et al. (2017). "OSSOS. VI. Striking Biases in the Detection of Large Semimajor Axis Trans-Neptunian Objects". The Astronomical Journal . 154 (2): 50. arXiv: 1706.05348 . Bibcode:2017AJ....154...50S. doi: 10.3847/1538-3881/aa7aed . hdl:10150/625487. S2CID   3535702.
    4. 1 2 "List of Known Trans-Neptunian Objects". Johnston's Archive. 22 July 2017. Retrieved 30 July 2017.
    5. 1 2 Malhotra, Renu; Volk, Kathryn; Wang, Xianyu (2016). "Corralling a distant planet with extreme resonant Kuiper belt objects". The Astrophysical Journal Letters . 824 (2): L22. arXiv: 1603.02196 . Bibcode:2016ApJ...824L..22M. doi: 10.3847/2041-8205/824/2/L22 . S2CID   118422279.


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