Comet_Tempel-Tuttle

55P/Tempel–Tuttle

55P/Tempel–Tuttle

Periodic comet with an orbital period of 33 years, parent body of the Leonid meteor shower


55P/Tempel–Tuttle (commonly known as Comet Tempel–Tuttle) is a retrograde periodic comet with an orbital period of 33 years. It fits the classical definition of a Halley-type comet with a period of between 20 and 200 years. It was independently discovered by Wilhelm Tempel on December 19, 1865, and by Horace Parnell Tuttle on January 6, 1866.

Quick Facts Discovery, Discovered by ...

It is the parent body of the Leonid meteor shower. In 1699, it was observed by Gottfried Kirch[6] but was not recognized as a periodic comet until the discoveries by Tempel and Tuttle during the 1866 perihelion. In 1933, S. Kanda deduced that the comet of 1366 was Tempel–Tuttle, which was confirmed by Joachim Schubart in 1965.[6] On 26 October 1366, the comet passed 0.0229 AU (3,430,000 km; 2,130,000 mi; 8.9 LD) from Earth.[7]

Comet Tempel-Tuttle was recovered on March 4, 1997 by Karen Meech, Olivier Hainaut and James "Gerbs" Bauer, at the University of Hawai`i. At the time it was very faint (22.5 mag), but the recovery proved that it was returning on schedule and that its orbit was very well determined.[8]

The retrograde orbit of 55P/Tempel–Tuttle causes meteors to impact Earth at a high speed of 70 km/s. The orbit intersects that of Earth nearly exactly, hence streams of material ejected from the comet during perihelion passages do not have to spread out much over time to encounter Earth. The comet currently has an Earth-MOID of 0.008 AU (1,200,000 km; 740,000 mi).[5] This coincidence means that past streams from the comet at perihelion are still dense when they encounter Earth, resulting in the 33-year cycle of Leonid meteor storms. For example, the 1833 meteor storm was created by the previous 1800 perihelion passage.[9] Between 2021–2030, Earth will often pass through the meteoroid stream left behind from the 1733 orbit.[10]

More information Year, Nominal geocentric distance (AU) ...

55P/Tempel–Tuttle is estimated to have a nucleus of mass 1.2×1013 kg[14] and radius 1.8 km[14] and a stream of mass 5×1012 kg.[14]

Animation of 55P/Tempel–Tuttle's orbit from 1990 to 2180
Around Sun
Around Earth
   Sun ·    Earth ·    Mars ·    Jupiter ·   55P/Tempel–Tuttle

See also


References

  1. Kinoshita, Kazuo (16 September 1999). "55P/Tempel-Tuttle past, present and future orbital elements". Comet Orbit. Archived from the original on 20 May 2011. Retrieved 6 September 2023.
  2. Seiichi Yoshida (12 December 2005). "55P/Tempel-Tuttle". Seiichi Yoshida's Comet Catalog. Retrieved 18 February 2012.
  3. "Horizons Batch for 55P/Tempel-Tuttle (90000621) at 2031-May-20 23:45:52" (Perihelion occurs when rdot flips from negative to positive). JPL Horizons. Retrieved 26 August 2023. (JPL#J985/69 Soln.date: 2002-Jan-03)
  4. "JPL Small-Body Database Browser: 55P/Tempel-Tuttle" (last observation: 1998-07-05). Jet Propulsion Laboratory. Archived from the original on 2 February 2017.
  5. "Closest Approaches to the Earth by Comets". Minor Planet Center. Retrieved 28 June 2012.
  6. Mikhail, Maslov. "Leonids 2021-2030". Archived from the original on 10 June 2021. Retrieved 10 June 2021.
  7. "Horizons Batch for 55P/Tempel-Tuttle (90000621) at 1832-Dec-16" (J985 fits data all the way back to 1865). JPL Horizons. Retrieved 6 September 2023.
  8. "Horizons Batch for 55P/Tempel-Tuttle (90000621) at 1998-Jan-17" (Closest Earth approach occurs when deldot flips from negative to positive). JPL Horizons. Retrieved 6 September 2023.
  9. "Horizons Batch for 55P/Tempel-Tuttle (90000621) at 2031-Feb-25" (Closest Earth approach occurs when deldot flips from negative to positive). JPL Horizons. Retrieved 5 September 2023. (JPL#J985/69 Soln.date: 2002-Jan-03)
  10. David C. Jewitt. "From Cradle To Grave: The Rise and Demise of the Comets" (PDF). Comets II. Retrieved 12 November 2009.
More information Numbered comets ...



Share this article:

This article uses material from the Wikipedia article Comet_Tempel-Tuttle, and is written by contributors. Text is available under a CC BY-SA 4.0 International License; additional terms may apply. Images, videos and audio are available under their respective licenses.