80P/Peters–Hartley
| Discovery[1][2] | |
|---|---|
| Discovered by | Christian H. F. Peters Malcolm Hartley |
| Discovery site | Capodimonte Observatory, Italy |
| Discovery date | 26 June 1846 11 July 1982 |
| Designations | |
| P/1846 M1 P/1982 N1 | |
| |
| Orbital characteristics[4][5] | |
| Epoch | 21 November 2025 (JD 2461000.5) |
| Observation arc | 177.15 years |
| Number of observations | 186 |
| Aphelion | 6.424 AU |
| Perihelion | 1.618 AU |
| Semi-major axis | 4.021 AU |
| Eccentricity | 0.59769 |
| Orbital period | 8.063 years |
| Inclination | 29.928° |
| 259.77° | |
| Argument of periapsis | 339.26° |
| Mean anomaly | 131.89° |
| Last perihelion | 8 December 2022 |
| Next perihelion | 28 December 2030[3] |
| TJupiter | 2.513 |
| Earth MOID | 0.619 AU |
| Jupiter MOID | 0.454 AU |
| Comet total magnitude (M1) | 11.8 |
80P/Peters–Hartley is a Jupiter-family comet with an orbital period of 8.06 years around the Sun. It is the first of two comets discovered by German–American astronomer, Christian Heinrich Friedrich Peters,[a] later becoming lost and subsequently recovered by Australian astronomer, Malcolm Hartley.
Observational history
It was originally discovered by Christian Heinrich Friedrich Peters of Capodimonte Observatory, Naples, Italy.[1] There was insufficient data to accurately compute the orbit, and the comet was lost for well over 136 years.[6]
It was accidentally rediscovered by Malcolm Hartley at the UK Schmidt Telescope Unit, Siding Spring, Australia on a photographic plate exposed on 11 July 1982.[7] He estimated its brightness at a magnitude of 15. The sighting was confirmed from the Perth Observatory, where Michael P. Candy calculated the orbit and concluded that Hartley had indeed relocated the lost Peters' Comet.[2] Ichiro Hasegawa and Syuichi Nakano had simultaneously reached the same conclusion.
It was observed at its next apparition in 1990 by Robert H. McNaught of the Siding Spring observatory, who described as diffuse with a brightness of magnitude 14, indicating that the comet had faded over the last 150 years.[8] It was subsequently observed on every apparition since its recovery.
Notes
- ^ The second comet discovered by C. H. F. Peters was C/1857 O1 (Peters)
References
- ^ a b M. Peters (1846). "Announcement of Discovery of a Comet, June 26, 1846" (PDF). Monthly Notices of the Royal Astronomical Society. 7 (9): 159–160. Bibcode:1846MNRAS...7R.159P. doi:10.1093/mnras/7.9.159.
- ^ a b M. Hartley; M. P. Candy; V. Flynn; et al. (22 July 1982). B. G. Marsden (ed.). "Periodic Comet Peters-Hartley (1846 VI = 1982h)". IAU Circular. 3715 (1). Bibcode:1982IAUC.3715....1H.
- ^ "Horizons Batch for 80P/Peters-Hartley (90000849) on 2030-Dec-28" (Perihelion occurs when rdot flips from negative to positive). JPL Horizons. Retrieved 6 July 2023. (JPL#28/Soln.date: 2023-Jun-26)
- ^ "80P/Peters–Hartley – JPL Small-Body Database Lookup". ssd.jpl.nasa.gov. Jet Propulsion Laboratory. Retrieved 2 February 2026.
- ^ "80P/Peters–Hartley Orbit". Minor Planet Center. Retrieved 24 February 2019.
- ^ Z. Sekanina (1984). "Disappearance and Disintegration of Comets". Icarus. 58 (1): 81–100. Bibcode:1984Icar...58...81S. doi:10.1016/0019-1035(84)90099-X.
- ^ B. A. Skiff; E. Bowell; A. C. Gilmore; et al. (19 July 1982). B. G. Marsden (ed.). "Comet Hartley (1982h)". IAU Circular. 3713 (1). Bibcode:1982IAUC.3713....1S.
- ^ J. D. Shanklin (1996). "The Comets of 1990". Journal of the British Astronomical Association. 106 (2): 86–91. Bibcode:1996JBAA..106...86S.
External links
- 80P/Peters–Hartley at the JPL Small-Body Database
- 80P/Peters–Hartley at Gary W. Kronk's Cometography
- 80P/Peters–Hartley at Seiichi Yoshida's website