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2017 FZ2
From Wikipedia, the free encyclopedia
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2017 FZ2 (also written 2017 FZ2) is a micro-asteroid and near-Earth object of the Apollo group that was a quasi-satellite of the Earth until March 23, 2017.[6]
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Discovery, orbit and physical properties
2017 FZ2 was discovered by American astronomer Gregory Leonard on March 19, 2017, observing for the Mt. Lemmon Survey from Mount Lemmon Observatory.[7][8] Its orbit is moderately eccentric (0.26), low inclination (1.81º) and a semi-major axis of 1.007 AU.[8] Upon discovery, it was classified as an Apollo asteroid but also an Earth crosser by the Minor Planet Center. Its orbit is very chaotic but it is relatively well determined; as of September 26, 2017, its orbit is based on 52 observations (1 Doppler) spanning a data-arc of 8 days.[2] 2017 FZ2 has an absolute magnitude of 26.7 which gives a characteristic diameter of 20 m.[5]
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Quasi-satellite
2017 FZ2 was until very recently an Earth co-orbital, the sixth known terrestrial quasi-satellite and the smallest by far. Its most recent quasi-satellite episode may have started over 225 years ago and certainly ended after a close encounter with the Earth on March 23, 2017.[6]
Candidate asteroid family
A number of other near-Earth asteroids move in orbits similar to that of 2017 FZ2, the largest being 54509 YORP. There is an apparent excess of small bodies moving in orbits similar to that of YORP and this could be the result of mass shedding from the YORP effect.[6]
See also
Notes
- ^ This is assuming an albedo of 0.20–0.04.
References
External links
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