123P/West–Hartley
Periodic comet
From Wikipedia, the free encyclopedia
Comet WestâHartley is a periodic comet roughly 4 km in diameter with a 7.67-year orbit around the Sun. The current orbit does not bring it closer than about 1.2 AU (180 million km) from Earth.[2] It will next come to perihelion on 21 September 2026, when the comet will have a solar elongation of 22 degrees.[5]
Discoverydate11 May 1989
P/1989 E3, P/1995 S2
| Discovery | |
|---|---|
| Discovered by | Richard M. West Malcolm Hartley |
| Discovery site | European Southern Observatory |
| Discovery date | 11 May 1989 |
| Designations | |
| P/1989 E3, P/1995 S2 | |
| 1988 XVI, 1989k | |
| Orbital characteristics[2][3] | |
| Epoch | 7 October 2026 (JD 2461320.5) |
| Observation arc | 30.39 years |
| Number of observations | 4,399 |
| Aphelion | 5.616 AU |
| Perihelion | 2.159 AU |
| Semi-major axis | 3.887 AU |
| Eccentricity | 0.44469 |
| Orbital period | 7.665 years |
| Inclination | 15.281° |
| 45.848° | |
| Argument of periapsis | 103.88° |
| Mean anomaly | 1.945° |
| Last perihelion | 5 February 2019[4] |
| Next perihelion | 21 September 2026[4][5] |
| TJupiter | 2.832 |
| Earth MOID | 1.197 AU |
| Jupiter MOID | 0.704 AU |
| Physical characteristics[2][6][7] | |
Mean radius | 2.18±0.23 km |
| 3.7 hours | |
| Comet total magnitude (M1) | 8.2 |
| Comet nuclear magnitude (M2) | 13.8 |
| 17.5 (2026-04-03)[8] | |
Physical characteristics
The first attempts to measure the effective radius of its nucleus in 2000 were not successful due to too much scatter data in light curves obtained to provide reliable estimates.[9] Recent attempts to measure the comet's light curves between 2004 and 2015 revealed that the nucleus is about 2.18 km (1.35 mi) in radius, rotating once every 3.7 hours.[6]