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41P/Tuttle–Giacobini–Kresák
Periodic comet
Periodic comet
| Field | Value |
|---|---|
| name | 41P/Tuttle–Giacobini–Kresák |
| image | 41P Tuttle-Giacobini-Kresak near M108 and M97 - 2017-03-22.jpg |
| caption | Comet 41P/Tuttle–Giacobini–Kresák on March 3, 2017 near Messier 108 and the Owl Nebula. |
| discoverer | Horace Parnell Tuttle |
| Michel Giacobini | |
| Ľubor Kresák | |
| discovery_date | May 3, 1858 |
| mpc_name | P/1858 J1, P/1907 O1 |
| P/1951 H1, P/1989b1 | |
| designations | |
| orbit_ref | |
| epoch | September 13, 2023 (JD 2460200.5) |
| observation_arc | 72.38 years |
| earliest_precovery_date | April 26, 1951 |
| obs | 5,250 |
| perihelion | 1.051 AU |
| aphelion | 5.126 AU |
| semimajor | 3.088 AU |
| eccentricity | 0.65981 |
| period | 5.428 years |
| inclination | 9.219° |
| asc_node | 140.99° |
| arg_peri | 62.227° |
| mean | 66.147° |
| tjup | 2.827 |
| Earth_moid | 0.134 AU |
| Jupiter_moid | 0.488 AU |
| physical_ref | |
| dimensions | 1.4 km |
| M1 | 16.9 |
| last_p | 12 September 2022 |
| next_p | 15 February 2028 |
Michel Giacobini Ľubor Kresák P/1951 H1, P/1989b1
41P/Tuttle–Giacobini–Kresák is a periodic comet in the Solar System. The comet nucleus is estimated to be 1.4 km in diameter.
Observational history
Discovery
Discovered by Horace Parnell Tuttle on May 3, 1858, and re-discovered independently by Michel Giacobini and Ľubor Kresák in 1907 and 1951 respectively, it is a member of the Jupiter family of comets.
2006 apparition
As of June 1, 2006, Comet 41P was a 10th magnitude object for telescopes, located on the Cancer-Leo border, with a predicted maximum of about 10 at perihelion on June 11. This comet is of interest as it has been noted to flare dramatically. In 1973 the flare was 10 magnitudes brighter than predicted, reaching easy naked-eye visibility at apparent magnitude 4. However, by June 22, the comet had diminished to about magnitude 11, having produced no flare of note.
2011 apparition
The comet was not observed during the 2011 unfavorable apparition since the perihelion passage occurred when the comet was on the far side of the Sun.
2017 apparition
41P was recovered on November 10, 2016, at apparent magnitude 21 by Pan-STARRS. On April 1, 2017, the comet passed 0.142 AU from the Earth. The comet was expected to brighten to around magnitude 7 and be visible in binoculars.
Proposed exploration
In the 1960s, the European Space Research Organisation investigated sending a probe to the comet.
References
| access-date= 28 February 2010 }}
| access-date= 16 June 2014 }}
|access-date=2012-02-18}}
|archive-url=https://archive.today/20121213142035/http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=41P;cad=1%23cad |archive-date=December 13, 2012 |url-status=live |access-date=2012-02-22}}
|access-date=2017-03-02}}
References
- (2007). "Robotic Exploration of the Solar System Part I: The Golden Age 1957-1982". Springer.
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