| Discovery[1][2] | |
|---|---|
| Discovered by | Pan-STARRS 1 |
| Discovery site | Haleakalā Obs. |
| Discovery date | 18 February 2015 |
| Designations | |
| 2015 DR215 | |
| NEO · Atira · PHA[3][1] | |
| Orbital characteristics[3] | |
| Epoch 21 January 2022 (JD 2459600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 7.12 yr (2,602 days) |
| Aphelion | 0.9809AU |
| Perihelion | 0.3522 AU |
| 0.6665 AU | |
| Eccentricity | 0.4716 |
| 0.54 yr (199 days) | |
| 74.459° | |
| 1° 48m 40.325s / day | |
| Inclination | 4.085° |
| 314.961° | |
| 42.298° | |
| Earth MOID | 0.044412 AU (6,643,900 km) |
| Physical characteristics | |
| 205 m[4] | |
| 0.266[4] | |
| Sr[4] | |
| 20.51[3] | |
2015 DR215 is astonynear-Earth asteroid of theAtira class residing withinEarth's orbit. It was discovered on 18 February 2015 by thePan-STARRS 1 survey atHaleakalā Observatory atMaui,Hawaiʻi.[1][2] The asteroid has a diameter of about 200 m (660 ft)[4] and makes close approaches within 0.05 AU (7.5 million km; 4.6 million mi) of Earth, making it apotentially hazardous object.[3] On 11 March 2022, it made a close approach 0.045 AU (6.7 million km; 4.2 million mi) from Earth,[3] reaching a peakapparent magnitude of 17 as it streaked across thesouthern sky.[1]
2015 DR215 was discovered on 18 February 2015 by thePan-STARRS 1 survey atHaleakalā Observatory atMaui,Hawaiʻi.[2] It was first observed atapparent magnitude 20.7, located in thesouthern sky 28 degrees below theecliptic with an angular separation (solar elongation) of 76 degrees from the Sun.[2] Follow-up observations from theMauna Kea Observatory andCerro Tololo Inter-American Observatory commenced, establishing anobservation arc of 12 days until its discovery announcement by theMinor Planet Center on 2 March 2015.[2]
On 5 March 2016,2015 DR215 was recovered by theESA Optical Ground Station at apparent magnitude 19, at solar elongations below 56 degrees.[5] It was observed to be about 0.5 degrees away from its predicted positions in March 2016.[5] The recovery observations significantly reduced the asteroid's orbital uncertainty, bringing itsuncertainty parameter down from 9 to 3.[2][5]
As of 2022[update],2015 DR215 has been observed for over 7 years, with a well-determined orbit at an uncertainty parameter of 0.[3]
2015 DR215 is one of a small number ofAtira class asteroids that are orbiting entirely within the Earth's orbit.[6] Thetaxonomic class of2015 DR215 in theBus–DeMeo scheme isSr, indicating a stony composition.[4]
As of 2023, thisminor planet has neither beennumbered nornamed by theMinor Planet Center.
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