46P/Wirtanen is a small short-period comet with a current orbital period of 5.4 years. It was the original target for close investigation by the Rosetta spacecraft, planned by the European Space Agency, but an inability to meet the launch window caused Rosetta to be sent to 67P/Churyumov–Gerasimenko instead. It belongs to the Jupiter family of comets, all of which have aphelia between 5 and 6 AU. Its diameter is estimated at 1.2 kilometres (0.75 mi). In December 2019, astronomers reported capturing an outburst of the comet in substantial detail by the TESS space telescope.
|Discovered by||Carl A. Wirtanen|
|Discovery date||January 17, 1948|
|1961 IV; 1960m;|
1967 XIV; 1967k;
1974 XI; 1974i;
1986 VI; 1985q;
1991 XVI; 1991s;
1947 XIII; 1948b;
|Orbital characteristics A|
|Epoch||September 3, 2002 (JDT 2452520.5)|
|Semi-major axis||3.0943529 AU|
|Orbital period||5.44 a|
|Earth MOID||0.068 AU (10,200,000 km)|
|Rotation period||8.9 hours|
|Last perihelion||December 12, 2018|
July 9, 2013
February 2, 2008
46P/Wirtanen was discovered photographically on January 17, 1948, by the American astronomer Carl A. Wirtanen. The plate was exposed on January 15 during a stellar proper motion survey for the Lick Observatory. Due to a limited number of initial observations, it took more than a year to recognize this object as a short-period comet.
On 16 December 2018 the comet passed 0.0774 AU (11,580,000 km; 7,190,000 mi) (≈30.1 LD) from Earth, reaching an estimated magnitude of 4.2, making this pass the brightest one predicted, and the brightest close approach for the next 20 years. Its magnitude could peak as bright as magnitude 3 near its December 16, 2018 closest approach. It was one of the 10 closest comet flybys of Earth in 70 years.
The 2018 close approach, combined with Wirtanen's brightness provides an opportunity to study a potential future spacecraft mission target in detail. A worldwide observing campaign has been organized to capitalize on the favorable circumstances of this apparition.
View from the Hubble Space Telescope on December 13, 2018
The comet was the target for the proposed Comet Hopper mission, which reached the finalist stage in the NASA Discovery program. It was one of only three missions in that selection to have a more detailed study. The selection process was ultimately won in 2012 by the InSight mission, a Mars lander. The Comet Hopper was designed to use the ASRG, the Advanced Stirling Radioisotope Generator.
The Comet Hopper mission, if it were selected, would have had multiple science goals over the 7.3 years of its nominal lifetime. At roughly 4.5 AU the spacecraft would rendezvous with Comet Wirtanen and begin to map the spatial heterogeneity of surface solids as well as gas and dust emissions from the coma - the nebulous envelope around the nucleus of a comet. The remote mapping would also allow for any nucleus structure, geologic processes, and coma mechanisms to be determined. After arriving at the comet, the spacecraft would approach and land, then subsequently hop to other locations on the comet. As the comet approached the Sun, the spacecraft would land and hop multiple times. The final landing would occur at 1.5 AU. As the comet approached the Sun and became more active, the spacecraft would be able to record surface changes.
Also, 46P/Wirtanen was the original destination of the European Space Agency's Rosetta spacecraft mission, but launch delays meant that the comet was no longer easily reachable and another periodic comet, 67P/Churyumov–Gerasimenko, was chosen as the mission's target instead.
Associated Piscid meteor showerEdit
Russian forecaster Mikhail Maslov had predicted that the Earth's orbit would cross Comet Wirtanen's debris stream as many as four times between December 10 and December 14, 2012. As there had not previously been an encounter with this debris stream, it was not certain whether or not a meteor shower would be visible from Earth, but there was speculation that a shower with as many as 30 meteors per hour might occur.
In popular cultureEdit
- "46P/Wirtanen Orbit". Minor Planet Center. Retrieved 2019-02-23.
- Syuichi Nakano (2010-04-09). "46P/Wirtanen (NK 1909)". OAA Computing and Minor Planet Sections. Retrieved 2012-02-18.
- "JPL Small-Body Database Browser: 46P/Wirtanen" (last observation: 2018-11-26; arc: 202 days). Retrieved 2018-12-06.
- Goddard Space Flight Center (3 December 2019). "NASA's exoplanet-hunting mission catches a natural comet outburst in unprecedented detail". EurekAlert!. Retrieved 3 December 2019.
- University of Maryland (3 December 2019). "UMD astronomers catch a natural comet outburst in unprecedented detail - Data from NASA's Transiting Exoplanet Survey Satellite (TESS) reveal start-to-finish sequence of an outburst from comet 46P/Wirtanen". EurekAlert!. Retrieved 3 December 2019.
- Ulamec, S.; Espinasse, S.; Feuerbacher, B.; Hilchenbach, M.; Moura, D.; et al. (April 2006). "Rosetta Lander—Philae: Implications of an alternative mission". Acta Astronautica. 58 (8): 435–441. Bibcode:2006AcAau..58..435U. doi:10.1016/j.actaastro.2005.12.009.
- Kronk, Gary W. "46P/Wirtanen". Retrieved 2019-03-03. (Cometography Home Page)
- "Comet 46P/Wirtanen Information". theskylive.com. Retrieved 2017-11-26.
- "Look Up! Comet 46P/Wirtanen to Flyby in December 2018". timeanddate.com. Retrieved 2018-12-06.
- "See a Passing Comet This Sunday". JPL. Retrieved 2019-03-03.
- "The Comet Wirtanen Observing Campaign". wirtanen.astro.umd.edu. Retrieved 2018-06-05.
- "Picturesque poison". www.eso.org. Retrieved 19 February 2019.
- "Maryland scientists vie for NASA missions". The Baltimore Sun. Archived from the original on 2012-09-26. Retrieved 2011-06-02.
- "Planetary Science Division Update" (PDF). NASA. Archived from the original (PDF) on 2011-11-14. Retrieved 2011-05-23.
- "Comet 67P/Churyumov-Gerasimenko". Rosetta. ESA. 18 December 2013. Retrieved 20 May 2014.
- "Hubble Assists Rosetta Comet Mission" (Press release). Hubble Space Telescope. September 5, 2003. Retrieved May 20, 2014.
- "A New Meteor Shower in December?". NASA. Retrieved 2012-12-13.
- "Comet Wirtanen meteors report". IceInSpace. Retrieved 2012-12-17.