2017 DR109, is a micro-asteroid, classified as near-Earth object of the Apollo group and Aten group, respectively. It is currently trapped in a 1:1 mean motion resonance with the Earth of the horseshoe type.[5] The object was first observed on 27 February 2017, by astronomers of the Catalina Sky Survey conducted at Mount Lemmon Observatory, Arizona, United States.[2]
Discovery[1] | |
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Discovered by | Catalina Sky Srvy. |
Discovery site | Mount Lemmon Obs. |
Discovery date | 27 February 2017 |
Designations | |
MPC designation | 2017 DR109 |
Minor planet category | NEO · Apollo[1] · Aten[2] |
Orbital characteristics[1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 6 | |
Observation arc | (5 days) |
Aphelion | 1.2422 AU |
Perihelion | 0.7591 AU |
Semi-major axis | 1.0006 AU |
Eccentricity | 0.2414 |
Orbital period (sidereal) | 1.00 yr (366 days) |
Mean anomaly | 263.04° |
Mean motion | 0° 59m 4.92s / day |
Inclination | 3.0600° |
Longitude of ascending node | 341.31° |
Argument of perihelion | 72.094° |
Earth MOID | 0.0062 AU (2.4 LD) |
Physical characteristics | |
Mean diameter | 9–20 m (estimate)[3][4][a] |
Absolute magnitude (H) | 27.6[1] |
2017 DR109 was first observed by astronomer D. C. Fuls on 27 February 2017, using the 0.68-meter Schmidt camera of the Catalina Sky Survey at a visual apparent magnitude of 19.6.[5]: 6
The asteroid's orbit has still a high uncertainty; with a very short observation arc of just 5 days. It orbits the Sun at a distance of 0.76–1.24 AU once every 366 days (semi-major axis of 1.00 AU). Its orbit has an eccentricity of 0.24 and an inclination of 3° with respect to the ecliptic.[1] With a semi-major axis of that of Earth, the object is both classified as a member of Apollo and Aten in the JPL Small-Body Database and by the Minor Planet Center, respectively.[1][2] Both Apollo and Aten asteroids are Earth-crossing asteroids.
2017 DR109 is currently trapped in a 1:1 mean motion resonance with the Earth of the horseshoe type and follows an orbit similar to those of 54509 YORP, 2017 FZ2 and several other near-Earth asteroids.[5]
2017 DR109 has an absolute magnitude of 27.6 which gives a calculated mean diameter between 9 and 20 meters for an assumed geometric albedo of 0.20 and 0.04, respectively, which are typical values for stony S-type and carbonaceous C-type asteroids.[3][4]
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