2020 SL1 is a near-Earth asteroid of the Apollo group, discovered by the Pan-STARRS 1 survey at Haleakala Observatory, Hawaii on 18 September 2020. With an estimated diameter of 0.9–2.0 km (0.56–1.24 mi), it is the largest potentially hazardous asteroid discovered in 2020.[8]
| Discovery [1][2] | |
|---|---|
| Discovered by | Pan-STARRS 1 |
| Discovery site | Haleakala Obs. |
| Discovery date | 18 September 2020 |
| Designations | |
| 2020 SL1 | |
| P116Atg [3][4] | |
| NEO · Apollo · PHA [5] | |
| Orbital characteristics [5] | |
| Epoch 31 May 2020 (JD 2459000.5) | |
| Uncertainty parameter 1 | |
| Observation arc | 12.04 yr (4,396 days) |
| Earliest precovery date | 25 October 2008 |
| Aphelion | 4.121 AU |
| Perihelion | 0.9091 AU |
| 2.515 AU | |
| Eccentricity | 0.63856 |
| 3.99 yr | |
| 34.497° | |
| 0° 14m 49.48s / day | |
| Inclination | 13.764° |
| 275.182° | |
| 12 January 2020 09:09 UT [5] | |
| 331.910° | |
| Earth MOID | 0.04732 AU |
| TJupiter | 3.108 |
| Physical characteristics | |
| 0.9–2.0 km (assumed albedo 0.05–0.25)[6] | |
| 23.6 (current)[7] 22.3 (at discovery)[1] | |
| 17.353±0.567[5] 17.1[2] | |
Discovery
edit2020 SL1 was discovered by the Pan-STARRS 1 survey at Haleakala Observatory, Hawaii on 18 September 2020. It was first observed in the constellation Triangulum at an apparent magnitude of 22.3.[1] The asteroid was moving at an on-sky rate of 0.56 arcseconds per minute, from a distance of 1.94 AU (290 million km; 180 million mi) from Earth.[9]
The asteroid was subsequently listed on the Minor Planet Center's Near-Earth Object Confirmation Page (NEOCP) as P116Atg.[4] Follow-up observations were carried out by the Astronomical Research Observatory (H21) and the asteroid was identified in earlier Mount Lemmon Survey (G96) observations from 28 August and 17 September 2020. The listing was confirmed and publicly announced as 2020 SL1 on 19 September 2020.[1]
Since discovery, 2020 SL1 has been identified in several precovery observations from Pan-STARRS 1 between November 2012 and January 2015 as well as October 2012 observations from the Mount Lemmon Survey. The earliest known precovery observations were identified in three Sloan Digital Sky Survey images from 25 October 2008.[2]
Orbit and classification
edit
2020 SL1 orbits the Sun at an average distance of 2.52 AU once every 3.99 years. Its orbit has a high eccentricity of 0.64 and an inclination of 14° with respect to the ecliptic plane. Over the course of its orbit, its distance from the Sun ranges from 0.91 AU at perihelion to 4.1 AU at aphelion, crossing the orbits of Earth and Mars.[5] Since its orbit crosses that of Earth's while having a semi-major axis greater than 1 AU, 2020 SL1 is classified as an Apollo asteroid.
Having a long observation arc over 12 years, the orbit of 2020 SL1 is well-defined with a condition code of 1.[5] Although it is classified as a potentially hazardous asteroid due to its large size combined with its small minimum orbit intersection distance of 0.047 AU (7.0 million km; 4.4 million mi) from Earth's orbital path, the asteroid will not make any close approaches within 0.1 astronomical units (15×106 km; 9.3×106 mi) over the next 200 years. The closest Earth encounter by 2020 SL1 in the last 200 years was on 10 July 1972, when it passed within 0.073 AU (10.9 million km; 6.8 million mi) of Earth at closest approach.[5]
Physical characteristics
editDiameter and albedo
editBased on an magnitude-to-diameter conversion and a measured absolute magnitude of 17.35, 2020 SL1 measures between 0.9 and 2.0 kilometers in diameter for an assumed geometric albedo of 0.25 and 0.05, respectively.[2][6] It is the largest potentially hazardous asteroid discovered in 2020, followed by 2020 QF6 with an absolute magnitude of 17.8.[8]
References
edit- ^ a b c d "MPEC 2020-S98 : 2020 SL1". Minor Planet Electronic Circular. Minor Planet Center. 19 September 2020. Retrieved 19 January 2021.
- ^ a b c d "2020 SL1". Minor Planet Center. International Astronomical Union. Retrieved 19 January 2021.
- ^ "2020 SL1". NEO Exchange. Las Cumbres Observatory. 19 September 2020. Retrieved 19 January 2021.
- ^ a b Gray, Bill (19 September 2020). ""Pseudo-MPEC" for P116Atg". Project Pluto. Retrieved 19 January 2021.
- ^ a b c d e f g "JPL Small-Body Database Browser: 2020 SL1" (2020-11-07 last obs.). Jet Propulsion Laboratory. Retrieved 19 January 2021.
- ^ a b Bruton, Dan. "Conversion of Absolute Magnitude to Diameter for Minor Planets". Department of Physics, Engineering, and Astronomy. Stephen F. Austin State University. Archived from the original on 23 July 2011. Retrieved 19 January 2021.
- ^ "2020SL1". Near Earth Objects – Dynamic Site. Department of Mathematics, University of Pisa, Italy. Retrieved 19 January 2021.
- ^ a b "JPL Small-Body Database Search Engine: PHAs and H < 18 (mag)". JPL Solar System Dynamics. Jet Propulsion Laboratory. Retrieved 19 January 2021.
- ^ "2020SL1 Ephemerides". Near Earth Objects – Dynamic Site (Ephemerides at discovery (obs. code F51)). Department of Mathematics, University of Pisa, Italy. Retrieved 19 January 2021.
External links
edit- "Pseudo-MPEC" for P116Atg[permanent dead link], Project Pluto, 19 September 2020
- 2020 SL1 at NeoDyS-2, Near Earth Objects—Dynamic Site
- 2020 SL1 at ESA–space situational awareness
- 2020 SL1 at the JPL Small-Body Database
