Comet Swift–Tuttle

Comet Swift–Tuttle (formally designated 109P/Swift–Tuttle) is a periodic comet with a current (osculating) orbital period of 133 years. It fits the classical definition of a Halley-type comet with a period between 20 and 200 years.[1] It was independently discovered by Lewis Swift on July 16, 1862 and by Horace Parnell Tuttle on July 19, 1862. It has a well determined orbit and has a comet nucleus 26 km in diameter.[1]

109P/Swift–Tuttle
Perseid meteor, originating from Comet Swift-Tuttle, from the ISS
Discovery
Discovered byLewis Swift
Horace Parnell Tuttle
Discovery dateJuly 16, 1862
Alternative
designations		1737 N1; 1737 II; 1862 O1;
1862 III; 1992 S2; 1992 XXVIII
Orbital characteristics A
EpochOctober 10, 1995
(JD 2450000.5)
Aphelion51.225 AU
Perihelion0.9595 AU
Semi-major axis26.092 AU
Eccentricity0.9632
Orbital period133.28 yr
Max. orbital speed42.6 km/s[lower-alpha 1]
Min. orbital speed0.8 km/s (2059-Dec-12)
Inclination113.45°
Earth MOID0.0009 AU (130,000 km)
Dimensions26 km[1]
Last perihelionDecember 11, 1992[1]
Next perihelionJuly 12, 2126[2][3]
Animation of 109P/Swift–Tuttle orbit from 1875 to 2100
  Sun ·   Earth ·   Jupiter  ·   Saturn ·   Uranus ·   109P/Swift–Tuttle
Animation of 109P/Swift–Tuttle's close approach to Earth in 1992

Chinese records indicate that, in 188, the comet reached apparent magnitude 0.1.[4] Observation was also recorded in 69 BC, and it was probably visible to the naked eye in 322 BC.[5] In the discovery year of 1862, the comet was as bright as Polaris.[6] The comet made a return appearance in 1992, when it was rediscovered by Japanese astronomer Tsuruhiko Kiuchi and became visible with binoculars.[7] In 2126 it will be a bright naked-eye comet reaching about apparent magnitude 0.7.[4]

After the 1862 observations it was thought that the comet would return between 1979 and 1983, but it didn't show up. However, it had been suggested in 1902 that this was the same comet as that observed by Ignatius Kegler on July 3, 1737,[8] and on this basis Brian Marsden calculated that it would return only in 1992, which in fact it did.[5]

It is the parent body of the Perseid meteor shower, perhaps the best known shower and among the most reliable in performance.[9]

The comet's perihelion is just under that of Earth, while its aphelion is just over that of Pluto. An unusual aspect of its orbit is that it is captured into a 1:11 orbital resonance with Jupiter; it completes one orbit for every 11 of Jupiter.[5] In principle this would mean that its proper long-term average period would be 130.48 years. However, it only entered this resonance about 1000 years ago, and will probably exit the resonance in several thousand years.[5]

Threat to Earth
Distance of Comet Swift-Tuttle from Earth in Astronomical Units and gigametres from 800 BC to AD 2500 . Approaches in the shaded area are not visible to the unaided eye. The dashed line shows approximately the current year.

The comet is on an orbit that makes repeated close approaches to the Earth-Moon system,[5] and has an Earth-MOID (Minimum orbit intersection distance) of 0.0009 AU (130,000 km; 84,000 mi).[1] Upon its 1992 rediscovery, the comet's date of perihelion passage was off from the then-current prediction by 17 days. It was then noticed that if its next perihelion passage (July 11, 2126) was also off by another 15 days (July 26), the comet would pass perilously close to Earth or the Moon on August 14, 2126 (IAUC 5636: 1992t). Given the size of the nucleus of Swift–Tuttle, this was of some concern. This prompted amateur astronomer and writer Gary W. Kronk to search for previous apparitions of this comet. He found the comet was most likely observed by the Chinese in 69 BC and AD 188, which was quickly confirmed by Brian Marsden.[10] This information and subsequent observations have led to recalculation of its orbit, which indicates the comet's orbit is sufficiently stable that there is absolutely no threat over the next two thousand years.[11] It is now known that the comet will pass 0.153 AU (22,900,000 km; 14,200,000 mi) from Earth on August 5, 2126.[1] and within 0.147 AU (22,000,000 km; 13,700,000 mi) from Earth on August 24, 2261.[12]

A close encounter with Earth is predicted for the comet's return to the inner Solar System in the year 3044, with the closest approach estimated to be one million miles (1,600,000 km; 0.011 AU).[13] Another close encounter is predicted for the year 4479, around Sept. 15; the close approach is estimated to be less than 0.05 AU, with a probability of impact of 1 in a million.[5] Subsequent to 4479, the orbital evolution of the comet is more difficult to predict; the probability of Earth impact per orbit is estimated as 2×10−8 (0.000002%).[5]

Comet Swift–Tuttle is the largest Solar System object that makes repeated close approaches to Earth. With a relative velocity of 60 km/s,[14][15] an Earth impact would have an estimated energy of ~27 times that of the Cretaceous–Paleogene impactor.[16] The comet has been described as "the single most dangerous object known to humanity".[15] In 1996, the long-term possibility of Comet Swift–Tuttle impacting Earth was compared to 433 Eros, and they were compared to about 3000 other kilometer sized objects as objects of concern.[17]

Notes
  1. v = 42.1219 √1/r − 0.5/a, where r is the distance from the Sun, and a is the semimajor axis.

References
  1. "JPL Small-Body Database Browser: 109P/Swift–Tuttle" (last observation: 1995-03-29). Jet Propulsion Laboratory. Retrieved 2011-05-09.
  2. "109P/Swift-Tuttle Orbit". Minor Planet Center. Retrieved 2014-06-17.
  3. Syuichi Nakano (1999-11-18). "109P/Swift–Tuttle (NK 798)". OAA Computing and Minor Planet Sections. Retrieved 2011-05-09.
  4. Yau, K.; Yeomans, D.; Weissman, P. (1994). "The past and future motion of Comet P/Swift-Tuttle". Monthly Notices of the Royal Astronomical Society. 266 (2): 305–316. Bibcode:1994MNRAS.266..305Y. doi:10.1093/mnras/266.2.305.
  5. Chambers, J. E. (1995). "The long-term dynamical evolution of Comet Swift–Tuttle". Icarus. Academic Press. 114 (2): 372–386. Bibcode:1995Icar..114..372C. doi:10.1006/icar.1995.1069.
  6. Levy, David H. (2008). David Levy's Guide to Observing Meteor Showers. Cambridge University Press. p. 12. ISBN 978-0-521-69691-3.
  7. Britt, Robert (2005-08-11). "Top 10 Perseid Meteor Shower Facts". Space.com. Retrieved 2009-08-10.
  8. Gary W. Kronk (1999). "109P/1737 N1". Cometography. 1. pp. 400–2.
  9. Bedient, John. "AMS Meteor Showers page", American Meteor Society, 20 June 2010. Retrieved 2010-7-31.
  10. Kronk, Gary; Marsden, Brian G. (1992). "Periodic Comet Swift–Tuttle (1992t)". Central Bureau for Astronomical Telegrams. Retrieved 2009-06-19.
  11. Stephens, Sally (1993). "on Swift–Tuttle's possible collision". Astronomical Society of the Pacific. Archived from the original on 2012-05-25. Retrieved 2008-08-25.
  12. Yau, Kevin; Paul, Weissman; Yeomans, Donald (1994). "The past and future motion ofComet P/Swift-Tuttle". Monthly Notices of the Royal Astronomical Society. Jet Propulsion Laboratory, California Institute of Technology. 266 (2): 305–316. Bibcode:1994MNRAS.266..305Y. doi:10.1093/mnras/266.2.305.
  13. https://astrosociety.org/edu/publications/tnl/23/23.html
  14. Weissman, Paul R. (2007). Milani, A.; Valsecchi, G.B.; Vokrouhlicky, D. (eds.). "Near Earth Objects, our Celestial Neighbors: Opportunity and Risk; Proceedings IAU Symposium No. 236, 2006". Proceedings of the International Astronomical Union. Cambridge University Press. 2: 441–450. doi:10.1017/S1743921307003559. Archived from the original on 2009-08-15. Retrieved 2009-08-13. |contribution= ignored (help)
  15. Verschuur, Gerrit L. (1997). Impact!: the threat of comets and asteroids. Oxford University Press. pp. 256 (see p. 116). ISBN 978-0-19-511919-0.
  16. This calculation can be carried out in the manner given by Weissman for Comet Hale–Bopp, as follows: A radius of 13.5 km and an estimated density of 0.6 g/cm3 gives a cometary mass of 6.2×1018 g. An encounter velocity of 60 km/s yields an impact velocity of 61 km/s, giving an impact energy of 1.15×1032 ergs, or 2.75×109 megatons, about 27.5 times the estimated energy of the K–T impact event.
  17. Browne, Malcolm W. "Mathematicians Say Asteroid May Hit Earth in a Million Years". Retrieved 2018-11-16.
Numbered comets
Previous
108P/Ciffreo		 Comet Swift–Tuttle Next
110P/Hartley
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.