Astronomy:2017 DB120
| Discovery[1][2] | |
|---|---|
| Discovered by | Pan-STARRS |
| Discovery site | Haleakala Obs. |
| Discovery date | 25 February 2017 (first observation only) |
| Designations | |
| 2017 DB120 | |
| Minor planet category | NEO–Amor[1][2] |
| Orbital characteristics[2] | |
| Epoch 26 February 2017 (JD 2457810.5) | |
| Uncertainty parameter 9[2] · E[1] | |
| Observation arc | 2.4 days[3] |
| |{{{apsis}}}|helion}} | 3.34±0.99 astronomical unit|AU |
| |{{{apsis}}}|helion}} | 1.07±0.23 AU |
| 2.20±0.65 AU | |
| Eccentricity | 0.52±0.25 |
| Orbital period | 3.3±1.5 years |
| Mean anomaly | 339°±9° |
| Mean motion | 0° 18m 3.6s / day |
| Inclination | 4.1°±1.4° |
| Longitude of ascending node | 193°±15° |
| 31°±33° | |
| Earth MOID | 0.0697 AU (27 LD) |
| Physical characteristics | |
| Mean diameter | |
| Absolute magnitude (H) | |
2017 DB120 (also written 2017 DB120) is a near-Earth object, meaning that it has an orbit which brings it into proximity with Earth. It is an Amor asteroid, meaning that its orbit does not cross Earth's orbit, but its perihelion is close to, but greater than, the aphelion of Earth. It was first observed on February 25, 2017, when the asteroid was less than 1 AU from Earth[1] and had a solar elongation of 169°.[5]
This asteroid is a lost asteroid.[6] It has a short observation arc of 2.4 days and has not been seen since 2017, so it has an orbit that is only roughly calculated. Also, there are variations in the absolute magnitude cataloged by various organizations, leading to variations in the estimated size of the asteroid (Sentry list H 23.0 implies 86 m[3] vs MPC H 22.3 implies 120 m[1]). These variations are in addition to the uncertainty in the size estimate caused by the uncertainty in the albedo.[7]
This asteroid is in both the Risk List[4] of the European Space Agency (ESA) - Space Situational Awareness (SSA) and in the Sentry List[8] of the Jet Propulsion Laboratory (JPL) – Center for Near Earth Object Studies (CNEOS). According to the Sentry List, of the possible close encounters with Earth in the foreseeable future, an encounter on 26 March 2061 has the highest Palermo Technical Impact Hazard Scale value.[3]
According to the Near Earth Objects Dynamic Site (NEODyS), of the possible close encounters with Earth in the foreseeable future, an encounter on 25 April 2031 is the most likely.[9] This encounter has a minimum possible distance of zero, meaning that an impact onto Earth is possible.
See also
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 "2017 DB120". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=2017+DB120. Retrieved 11 September 2020.
- ↑ 2.0 2.1 2.2 2.3 2.4 "JPL Small-Body Database Browser: (2017 DB120)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=3771593. Retrieved 11 September 2020.
- ↑ 3.0 3.1 3.2 3.3 3.4 "Sentry: Earth Impact Monitoring - Object Details 2017 DB120". Jet Propulsion Laboratory. https://cneos.jpl.nasa.gov/sentry/details.html#?des=2017%20DB120.
- ↑ 4.0 4.1 4.2 "ESA space situational awareness 2017DB120". European Space Agency. http://neo.ssa.esa.int/search-for-asteroids?tab=summary&des=2017DB120.
- ↑ "JPL HORIZONS Web-Interface (2017 DB120)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/horizons.cgi?find_body=1&body_group=sb&sstr=2017%20DB120.
- ↑ "NEODyS-2 Risk List". SpaceDys. https://newton.spacedys.com/neodys/index.php?pc=4.1.
- ↑ "Asteroid Size Estimator". CNEOS NASA/JPL. https://cneos.jpl.nasa.gov/tools/ast_size_est.html. Retrieved 11 September 2020.
- ↑ "Sentry: Earth Impact Monitoring - Impact Risk Data". Jet Propulsion Laboratory. https://cneos.jpl.nasa.gov/sentry/.
- ↑ "NEODyS-2 - Near Earth Objects - Dynamic Site - 2017DB120 - Close Approaches". SpaceDys. https://newton.spacedys.com/neodys/index.php?pc=1.1.8&n=2017DB120.
External links
- 2017 DB120 at NeoDyS-2, Near Earth Objects—Dynamic Site
- Ephemeris · Obs prediction · Orbital info · MOID · Proper elements · Obs info · Close · Physical info · NEOCC
- 2017 DB120 at ESA–space situational awareness
- 2017 DB120 at the JPL Small-Body Database
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