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2003 YN107 is a tiny asteroid, classified as a near-Earth object of the Aten group moving in a 1:1 mean-motion resonance with Earth. Because of that, it is in a co-orbital configuration relative to Earth.[2][3][4]

2003 YN107
Discovery
Discovered byLINEAR
Discovery date20 December 2003
Designations
Minor planet category
Orbital characteristics[1]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 0
Observation arc467 days (1.28 yr)
Aphelion1.00244 AU (149.963 Gm)
Perihelion0.974906 AU (145.8439 Gm)
Semi-major axis
0.988674 AU (147.9035 Gm)
Eccentricity0.0139259
Orbital period (sidereal)
0.98 yr (359.1 d)
Average orbital speed
29.82 km/s
Mean anomaly
176.9658°
Mean motion
1.00259°/day
Inclination4.32078°
Longitude of ascending node
264.41926°
Argument of perihelion
87.50070°
Earth MOID0.0045919 AU (686,940 km)
Physical characteristics
Mean diameter
10–30 m
Absolute magnitude (H)
26.5[1]

    Discovery, orbit and physical properties


    2003 YN107 was discovered by the Lincoln Near Earth Asteroid Research (LINEAR) system in orbit around the Sun on 20 December 2003. Its diameter is approximately 10 to 30 metres. The object is on NASA's Earth Close Approach list, and is estimated to miss Earth by 0.01 AU. It revolves around the Sun on an Earth-like, almost circular, orbit. Its orbital period of 363.846 days also is very close to the sidereal year.


    Co-orbital with Earth and orbital evolution


    From approximately 1997 to 2006, the asteroid remained within 0.1 AU (15,000,000 km; 9,300,000 mi) of Earth and it appeared to slowly orbit Earth.[2] However, 2003 YN107 is no second moon, as it is not bound to Earth. It is the first discovered member of a postulated group of coorbital objects, or quasi-satellites, which show these path characteristics.[2][3] Other members of this group include 10563 Izhdubar, 54509 YORP, (66063) 1998 RO1, (85770) 1998 UP1, and (85990) 1999 JV6. Before 1996, the asteroid had been on a so-called horseshoe orbit around the Sun, along the Earth's orbit. After 2006, it had regained such an orbit. This makes it very similar to 2002 AA29, which will become a quasi-satellite of Earth in approximately 600 years.[2][3][4]

    Animation of 2003 YN107 orbit from 1900-2100
    Relative to Sun and Earth
    Around Earth
    Around Sun
       Sun ·    Earth ·    2003 YN107

    See also



    References


    1. "JPL Small-Body Database Browser: (2003 YN107)". Jet Propulsion Laboratory. Retrieved 30 March 2016.
    2. Connors, M.; Veillet, C.; Brasser, R.; Wiegert, P.; Chodas, P.; Mikkola, S.; Innanen, K. (August 2004). "Discovery of Earth's quasi-satellite". Meteoritics & Planetary Science. 39 (8): 1251–1255. Bibcode:2004M&PS...39.1251C. doi:10.1111/j.1945-5100.2004.tb00944.x.
    3. Brasser, R.; Innanen, K. A.; Connors, M.; Veillet, C.; Wiegert, P.; Mikkola, S.; Chodas, P. W. (September 2004). "Transient co-orbital asteroids". Icarus. 171 (1): 102–109. Bibcode:2004Icar..171..102B. doi:10.1016/j.icarus.2004.04.019.
    4. de la Fuente Marcos, C.; de la Fuente Marcos, R. (July 2013). "A resonant family of dynamically cold small bodies in the near-Earth asteroid belt". Monthly Notices of the Royal Astronomical Society: Letters. 434 (1): L1–L5. arXiv:1305.2825. Bibcode:2013MNRAS.434L...1D. doi:10.1093/mnrasl/slt062.



    На других языках


    [de] 2003 YN107

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    - [en] 2003 YN107

    [es] 2003 YN107

    El asteroide 2003 YN107 es uno de los denominados asteroides coorbitantes de la Tierra o cuasisatélites, y el primero que se ha conocido. Estos son asteroides que al acercarse a la Tierra permanecen capturados por la gravedad terrestre, durante algunos años, y luego se alejan nuevamente.

    [ru] 2003 YN107

    2003 YN107 — небольшой околоземный астероид из группы атонов, который движется в орбитальном резонансе с Землёй 1:1. Из-за особенностей его движения вокруг Солнца этот астероид также называют квазиспутником Земли[1][2][3].



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