91P/Russell
Appearance
| Discovery[1] | |
|---|---|
| Discovered by | Kenneth S. Russell |
| Discovery site | Siding Spring Observatory, Australia |
| Discovery date | 14 June 1983 |
| Designations | |
| P/1983 L1 P/1989 A4 | |
| |
| Orbital characteristics[2][3] | |
| Epoch | 21 November 2025 (JD 2461000.5) |
| Observation arc | 38.21 years |
| Number of observations | 423 |
| Aphelion | 5.207 AU |
| Perihelion | 3.106 AU |
| Semi-major axis | 4.156 AU |
| Eccentricity | 0.25276 |
| Orbital period | 8.473 years |
| Inclination | 16.015° |
| 242.12° | |
| Argument of periapsis | 356.97° |
| Mean anomaly | 235.59° |
| Last perihelion | 9 November 2020 |
| Next perihelion | 26 October 2028[4] |
| TJupiter | 2.921 |
| Earth MOID | 1.593 AU |
| Jupiter MOID | 0.084 AU |
| Physical characteristics[2] | |
Mean radius | 1.26 km (0.78 mi)[5] |
| Comet total magnitude (M1) | 7.7 |
| Comet nuclear magnitude (M2) | 15.6 |
91P/Russell, also known as Russell 3, is a Jupiter-family comet with an 8.47-year orbit around the Sun. It was discovered by Kenneth S. Russell in 1983.
References
[edit]- ↑ K. S. Russell (17 June 1983). B. G. Marsden (ed.). "Comet Russell (1983i)". IAU Circular. 3828 (1). Bibcode:1983IAUC.3828....1R.
- 1 2 "91P/Russell – JPL Small-Body Database Lookup". ssd.jpl.nasa.gov. Jet Propulsion Laboratory. Retrieved 13 April 2026.
- ↑ "91P/Russell Orbit". Minor Planet Center. Retrieved 16 June 2014.
- ↑ "Horizons Batch for 91P/Russell (90000904) on 2028-Oct-26" (Perihelion occurs when rdot flips from negative to positive). JPL Horizons. Retrieved 29 April 2023. (Soln.date: 2021-Sep-07)
- ↑ G. Tancredi; J. A. Fernández; H. Rickman; J. Licandro (2006). "Nuclear magnitudes and the size distribution of Jupiter family comets". Icarus. 182 (2): 527–549. Bibcode:2006Icar..182..527T. doi:10.1016/j.icarus.2006.01.007.
External links
[edit]- 91P/Russell at the JPL Small-Body Database
- 91P/Russell at Seiichi Yoshida's website
- 91P/Russell at Gary W. Kronk's Cometography