11P/Tempel–Swift–LINEAR
![]() Infrared image of Comet T–S–L taken by NEOWISE on 4 January 2021. | |
Discovery[1] | |
---|---|
Discovered by | |
Discovery date |
|
Designations | |
| |
| |
Orbital characteristics[4][2] | |
Epoch | 17 October 2024 (JD 2460600.5) |
Observation arc | 154.75 years |
Number of observations | 1,337 |
Aphelion | 5.18 AU |
Perihelion | 1.388 AU |
Semi-major axis | 3.284 AU |
Eccentricity | 0.57756 |
Orbital period | 5.95 years |
Inclination | 14.435° |
238.87° | |
Argument of periapsis | 168.04° |
Mean anomaly | 235.14° |
Last perihelion | 26 November 2020[2] |
Next perihelion | 9 November 2026[3] |
TJupiter | 2.839 |
Earth MOID | 0.403 AU |
Jupiter MOID | 0.326 AU |
Comet total magnitude (M1) | 15.2 |
Comet nuclear magnitude (M2) | 18.6 |
11P/Tempel–Swift–LINEAR is a periodic comet with a 5.95-year orbit around the Sun.
Observational history
Discovery
In 1869, the comet's perihelion was around 1.063 AU (159.0 million km) from the Sun.[5] Ernst Wilhelm Leberecht Tempel originally discovered the comet on 27 November 1869, from his observatory at Marseille. It was later observed by Lewis Swift from the Warner Observatory on 11 October 1880, and he realised that it is the same comet as Tempel's.[6]
Loss and recovery
After 1908, the comet became an unobservable lost comet due to a series of four close flybys of Jupiter between 1911 and 1946[a] perturbing its orbit significantly enough that made subsequent apparitions of the comet unfavorable for observations in decades.[7] Nevertheless, Brian G. Marsden computed the resulting orbit based on the observations between 1891 and 1908, and predicted a favorable return in 1963, however the comet remained unobserved.[7] Despite this, additional predictions of the comet's favorable returns were later attempted by Marsden and Zdenek Sekanina in 1971,[8] and Shuichi Nakano in 1995.
On 7 December 2001, an object designated as P/2001 X3 was found by the Lincoln Near-Earth Asteroid Research (LINEAR) program.[9] Analysis of images taken between 10 September and 17 October 2001 later confirmed that P/2001 X3 is the recovery of the previously lost comet Tempel–Swift.[1]
Recent observations
The comet was not observed during the 2008 unfavorable apparition[10][2] because the perihelion passage occurred when the comet was on the far side of the Sun. The comet was observed during the 2014 and 2020 apparitions.[2] The comet will next come to perihelion on 9 November 2026,[3] then two days later on the 11th, make a closest approach to Earth of 0.4012 AU (60.02 million km).[4]
References
Notes
Citations
- ^ a b C. Hergenrother; K. Muraoka; S. Nakano (20 December 2001). D. W. Green (ed.). "Comet 11D (Tempel–Swift) = P/2001 X3 (LINEAR)". IAU Circular. 7779 (1). Bibcode:2001IAUC.7779....1H.
- ^ a b c d "11P/Tempel–Swift–LINEAR Orbit". Minor Planet Center. Retrieved 28 October 2014.
- ^ a b "Horizons Batch for 11P/Tempel-Swift-LINEAR (90000219) on 2026-Nov-09" (Perihelion occurs when rdot flips from negative to positive). JPL Horizons. Retrieved 27 June 2022. (JPL#K204/11 Soln.date: 2022-May-23)
- ^ a b "11P/Tempel–Swift–LINEAR – JPL Small-Body Database". ssd.jpl.nasa.gov. Jet Propulsion Laboratory. Retrieved 12 July 2023.
- ^ Kinoshita, Kazuo (2 December 2014). "11P/Tempel-Swift-LINEAR past, present and future orbital elements". Comet Orbit. Archived from the original on 20 May 2011. Retrieved 27 July 2023.
- ^ G. W. Kronk. "11P/Tempel–Swift–LINEAR". Cometography.com. Retrieved 28 October 2014.
- ^ a b c B. G. Marsden (3 August 1963). K. A. Thernöe (ed.). "Periodic Comet Tempel–Swift". IAU Circular. 1838 (2).
- ^ a b B. G. Marsden; Z. Sekanina (1971). "Comets and Nongravitational Forces. IV". The Astronomical Journal. 76 (10): 1135–1152. Bibcode:1971AJ.....76.1135M. doi:10.1086/111232.
- ^ R. Huber; G. Hug (19 December 2001). D. W. Green (ed.). "Comet P/2001 X3 (LINEAR)". IAU Circular. 7779 (2). Bibcode:2001IAUC.7778....2H.
- ^ Seiichi Yoshida (7 April 2009). "Tempel–Swift–LINEAR". Seiichi Yoshida's Comet Catalog. Retrieved 19 February 2012.
External links
- 11P/Tempel–Swift–LINEAR at the JPL Small-Body Database
- 11P/Tempel–Swift–LINEAR at Gary W. Kronk's Cometography