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2014 YX49 is a centaur and Uranus co-orbital, approximately 77 kilometers (48 miles) in diameter, first observed on December 26, 2014, by the Pan-STARRS survey.[4] It is the second known centaur on a tadpole orbit with Uranus, and the fourth Uranus co-orbital discovered after 83982 Crantor, 2011 QF99 and (472651) 2015 DB216.[5]

2014 YX49
Discovery[1]
Discovered byPan-STARRS
Discovery siteHaleakala Obs.
Discovery dateDecember 26, 2014
Designations
MPC designation
2014 YX49
Minor planet category
Uranus trojan centaur[2][3] · distant[1]
Orbital characteristics[2]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 1
Observation arc4876 days (13.35 yr)
Aphelion24.4207 AU (3.65328 Tm)
Perihelion13.8401 AU (2.07045 Tm)
Semi-major axis
19.1304 AU (2.86187 Tm)
Eccentricity0.276539
Orbital period (sidereal)
83.67 yr (30562 d)
Mean anomaly
75.587°
Inclination25.55097°
Longitude of ascending node
91.44425°
Argument of perihelion
280.584°
Earth MOID12.9424 AU (1.93616 Tm)
Jupiter MOID9.47006 AU (1.416701 Tm)
Physical characteristics
Mean diameter
77 km (est. at 0.09)[3]
Apparent magnitude
21.6
Absolute magnitude (H)
8.8

    Description


    Centaur 2014 YX49 is a temporary L4 trojan of Uranus, the second one (2011 QF99 was identified first) to be confirmed as currently trapped in such a resonant state. This object may have remained as a L4 Uranian Trojan for about 60,000 years and it can continue that way for another 80,000 years. Numerical integrations suggest that it may stay within Uranus' co-orbital zone for nearly one million years.[5]

    Besides being a L4 Uranian trojan, 2014 YX49 is trapped in the 7:20 mean motion resonance with Saturn as well; therefore, this minor body is currently subjected to a three-body resonance.[5] The other known Uranian trojan, 2011 QF99, is also in this resonant configuration.

    Animation of 2014 YX49 relative to Sun and Uranus 1600-2500.mw-parser-output .legend{page-break-inside:avoid;break-inside:avoid-column}.mw-parser-output .legend-color{display:inline-block;min-width:1.25em;height:1.25em;line-height:1.25;margin:1px 0;text-align:center;border:1px solid black;background-color:transparent;color:black}.mw-parser-output .legend-text{}  2014 YX49 ·   Uranus ·   Sun
    Animation of 2014 YX49 relative to Sun and Uranus 1600-2500
      2014 YX49 ·   Uranus ·   Sun

    See also



    References


    1. "2014 YX49 - Minor Planet Center". Minor Planet Center. International Astronomical Union. Retrieved January 20, 2017.
    2. "JPL Small Body Database Browser". JPL (2015-01-28 last obs.). NASA. Retrieved January 20, 2017.
    3. Johnston, Wm. Robert (August 18, 2020). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved August 12, 2021.
    4. "MPEC 2016-O10 : 2014 YX49". Minor Planet Center. International Astronomical Union. Retrieved January 20, 2017.
    5. de la Fuente Marcos, Carlos; de la Fuente Marcos, Raúl (May 15, 2017). "Asteroid 2014 YX49: a large transient Trojan of Uranus". Monthly Notices of the Royal Astronomical Society. 467 (2): 1561–1568. arXiv:1701.05541. Bibcode:2017MNRAS.467.1561D. doi:10.1093/mnras/stx197.




    На других языках


    - [en] 2014 YX49

    [ru] 2014 YX49

    2014 YX49 — астероид, кентавр, коорбитальный спутник Урана, впервые наблюдавшийся 26 декабря 2014 года в рамках обзора Pan-STARRS.[3] Второй из известных кентавров на подковообразной орбите относительно Урана, четвёртый открытый коорбитальный спутник Урана наряду с объектами (83982) Крантор, 2011 QF99 и (472651) 2015 DB216.[4]



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