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1 Discovery  





2 Orbit and orbital evolution  





3 Physical properties  





4 See also  





5 References  





6 External links  














2014 OL339






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From Wikipedia, the free encyclopedia
 


2014 OL339
Discovery[1]
Discovered byEURONEAR
(unofficial credits)
Discovery siteLa Palma Obs.
(first observed)
Discovery date29 July 2014
Designations

MPC designation

2014 OL339

Minor planet category

  • Aten[1][2]
  • Venus crosser
  • Earth crosser
  • Orbital characteristics[1]
    Epoch 16 February 2017 (JD 2457800.5)
    Uncertainty parameter1
    Observation arc2.10 yr (768 days)
    Aphelion1.4598 AU
    Perihelion0.5388 AU

    Semi-major axis

    0.9993 AU
    Eccentricity0.4608

    Orbital period (sidereal)

    1.00 yr (365 days)

    Mean anomaly

    285.00°

    Mean motion

    0° 59m 12.12s / day
    Inclination10.187°

    Longitude of ascending node

    252.18°

    Argument of perihelion

    289.69°
    Earth MOID0.0179 AU
    Physical characteristics
    Dimensions170 m (est. at 0.25)[3]

    Absolute magnitude (H)

    22.9[1]

    2014 OL339 (also written 2014 OL339) is an Aten asteroid that is a temporary quasi-satelliteofEarth, the fourth known Earth quasi-satellite.[4]

    Discovery[edit]

    2014 OL339 was discovered on 29 July 2014 by Farid Char of the Chilean University of Antofagasta. The actual observers were O. Vaduvescu and V. Tudor, observing from the Roque de los Muchachos Observatory for the EURONEAR project with the Isaac Newton Telescope. The intended target of the program was the Apollo asteroid 2013 VQ4 but F. Char identified 2014 OL339 as a streak near the edge of the observed field.[5] As of 14 August 2015, it has been observed 39 times with an observation arc of 381 days.[1]

    Orbit and orbital evolution[edit]

    2014 OL339 is currently an Aten asteroid (Earth-crossing but with a period less than a year). Its semi-major axis (currently 0.9994 AU) is similar to that of Earth (0.9992 AU), but it has a relatively high eccentricity (0.4607) and moderate orbital inclination (10.1910°). Gravitational interaction with Earth causes its orbit to change so that its average period is one year (This means it alternates between being an Aten asteroid and being an Apollo asteroid.) Its mean longitude (around the Sun) is similar to that of Earth, which means that it is fairly close to Earth (less than about 1.5 AU). This makes it a quasi-satellite. It moves in a kidney-shaped path going from east to west relative to Earth ("retrograde", the opposite way from the Moon). The relative mean longitude compared to Earth (that is, its mean longitude minus that of Earth) librates around zero. This means that the center of the "kidney" moves back and forth over a period of years, from being in front of Earth to being behind Earth, but this movement is centered on Earth.[4]

    It became a quasi-satellite at least 775 years ago and will stop being that 165 years from now after a "close" encounter with Earth (0.13 AU). This quasi-satellite episode will have had a duration of around a thousand years or more, but less than 2,500 years. Before and after this episode it passes in and out of other types of co-orbital orbits, such as being a trojan or a "passing object" (one whose relative longitude to Earth can attain any value, which is not the case for a quasi-satellite or a Trojan).[4]

    Physical properties[edit]

    With an absolute magnitude of 22.9,[1] it has an estimated diameter of approximately 170 meters for an albedo of 0.25, which is typical for stony asteroids.[3]

    See also[edit]

    References[edit]

    1. ^ a b c d e f "JPL Small-Body Database Browser: (2014 OL339)" (2016-09-04 last obs.). Jet Propulsion Laboratory. Retrieved 23 March 2017.
  • ^ "2014 OL339". Minor Planet Center. Retrieved 23 March 2017.
  • ^ a b "Absolute Magnitude (H)". NASA/JPL. Archived from the original on 2 March 2001. Retrieved 23 March 2017.
  • ^ a b c de la Fuente Marcos, Carlos; de la Fuente Marcos, Raúl (2014). "Asteroid 2014 OL339: yet another Earth quasi-satellite". Monthly Notices of the Royal Astronomical Society. 445 (3): 2985–2994. arXiv:1409.5588. Bibcode:2014MNRAS.445.2961D. doi:10.1093/mnras/stu1978.
  • ^ Discovery account
  • Further reading

    External links[edit]


    Retrieved from "https://en.wikipedia.org/w/index.php?title=2014_OL339&oldid=1187134352"

    Categories: 
    Aten asteroids
    Minor planet object articles (unnumbered)
    Venus-crossing asteroids
    Earth-crossing asteroids
    Earth co-orbital asteroids
    Astronomical objects discovered in 2014
    Discoveries by EURONEAR
    Hidden categories: 
    Use dmy dates from February 2018
    Articles with Spanish-language sources (es)
    JPL Small-Body Database ID same as Wikidata
    Articles with JPL SBDB identifiers
    Articles with MPC identifiers
     



    This page was last edited on 27 November 2023, at 17:58 (UTC).

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