2018 RY7, is a small near-Earth object of the Apollo group. It is currently trapped in a 3:5 mean motion resonance with Venus.[6] The object was first observed on 14 September 2018, by astronomer B. M. Africano with the Mount Lemmon Survey at Mount Lemmon Observatory, Arizona, United States.[2][1]
Discovery [1] | |
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Discovered by | MLS M. B. Africano [2] |
Discovery site | Mount Lemmon Obs. |
Discovery date | 14 September 2018 (first observed only) |
Designations | |
MPC designation | 2018 RY7 |
Minor planet category | NEO · Apollo [1][3] Earth crosser |
Orbital characteristics [3] | |
Epoch 27 April 2019 (JD 2458600.5) | |
Uncertainty parameter 4 | |
Observation arc | 89 days |
Aphelion | 1.1656 AU |
Perihelion | 0.8668 AU |
Semi-major axis | 1.0162 AU |
Eccentricity | 0.1470 |
Orbital period (sidereal) | 1.02 yr (374 d) |
Mean anomaly | 80.480° |
Mean motion | 0° 57m 43.92s / day |
Inclination | 13.351° |
Longitude of ascending node | 2.8171° |
Argument of perihelion | 136.88° |
Earth MOID | 0.0938 AU (36.5424 LD) |
Physical characteristics | |
Mean diameter | 23–103 m (est.)[4][5][a] |
Absolute magnitude (H) | 24.4[3] |
The asteroid's orbit determination is in need of some improvement. It orbits the Sun at a distance of 0.87–1.17 AU once every 374 days (semi-major axis of 1.016 AU). Its orbit has an eccentricity of 0.1470 and an inclination of 13.35° with respect to the ecliptic.[3] It is a member of Apollo dynamical class in both the JPL Small-Body Database and the Minor Planet Center.[1][3] Apollo asteroids are Earth-crossing asteroids.
2018 RY7 is currently trapped in a 3:5 mean motion resonance with Venus and follows an orbit very similar to that of 2017 SN16.[6] This pair of near-Earth objects show the highest observed level of dynamical coherence among the NEO-population.
2018 RY7 has an absolute magnitude of 24.4 which gives a calculated mean diameter between 23 and 103 meters for an assumed geometric albedo of 0.60 and 0.03, respectively.[4][5]
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