 Comet Russell–LINEAR on 9 December 2020 byNEOWISE | |
| Discovery[1] | |
|---|---|
| Discovered by | Kenneth S. Russell |
| Discovery site | Siding Spring Observatory |
| Discovery date | 3 September 1986 |
| Designations | |
| P/1986 R1, P/1993 WU,P/2000 QD181,P/2000 XV43 | |
| Orbital characteristics[3][4] | |
| Epoch | 20 March 2020 (JD 2458928.5) |
| Observation arc | 35.57 years |
| Number of observations | 2,317 |
| Aphelion | 5.591 AU |
| Perihelion | 1.333 AU |
| Semi-major axis | 3.462 AU |
| Eccentricity | 0.61492 |
| Orbital period | 6.442 years |
| Inclination | 17.264° |
| 35.397° | |
| Argument of periapsis | 0.378° |
| Mean anomaly | 322.84° |
| Last perihelion | 18 November 2020 |
| Next perihelion | 30 April 2027[2] |
| TJupiter | 2.732 |
| EarthMOID | 0.339 AU |
| JupiterMOID | 0.100 AU |
| Physical characteristics[3] | |
Mean radius | 2.0 ± 0.2 km (1.24 ± 0.12 mi)[5] |
| Comet total magnitude (M1) | 12.7 |
156P/Russell–LINEAR is aJupiter-family comet with anorbital period of 6.4 years. It was discovered by Kenneth S. Russell in September 1986.[6]
The comet was found by Australian astronomerKenneth S. Russell in September 1986 on a plate exposed on 3 September 1986 using the U.K.Schmidt Telescope ofSiding Spring Observatory, Australia.[6] The comet had anapparent magnitude of 17. Follow up observations on 25 September failed to recover the comet.[1] The comet was spotted again in a plate exposed using the 0.46-m Schmidt telescope ofPalomar Observatory byCarolyn S. Shoemaker on 19 November 1993. The comet had asteroidal appearance and was given the provisional designation1993 WU.[1]
The comet was observed again during the 2000 perihelion. The comet was noted as an asteroidal object byLincoln Near-Earth Asteroid Research on 31 August and 5 November and was given the provisional designation2000 QD181, and was observed again in November 2000-January 2001 and named2000 XV43.Timothy B. Spahr noted that these objects were the same as the 1986 comet.[1] It was then given the number156P.[7]
The comet had passed 0.70 AU from Jupiter in November 1970 and its perihelion distance decreased from 1.73 AU to 1.56 AU. The comet approached again to Jupiter in March 2018 at a distance of 0.36 AU and its perihelion distance decreased to 1.33 AU, while the orbital period decreased from 6.85 years to 6.44 years.[6][3]
During the 2020 perihelion, the comet approached to 0.48 AU from Earth on 24 October 2020.[6] It brightened to an apparent magnitude of 9.7 in mid November 2020.[8]
Thecyanide anddiatomic carbon production rate was estimated to be(2.85±0.51)×1024 mol/s and(3.44±0.62)×1024 mol/s respectively on 14 October 2020, when the comet was located at an heliocentrical distance of 1.40 AU.[9] The production rates are comparable to those of other Jupiter-family comets. Two strong jets were observed during perihelion and persisted until December, indicating increased activity after perihelion.[10]
The size of itsnucleus is estimated to be less than 2.0 ± 0.2 km (1.24 ± 0.12 mi) in radius.[5]
| Numbered comets | ||
|---|---|---|
| Previous 155P/Shoemaker | 156P/Russell–LINEAR | Next 157P/Tritton |
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