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Comet Swift–Tuttle

From Wikipedia, the free encyclopedia
Halley-type comet and parent body of the Perseid meteors
For other comets discovered by Lewis A. Swift, seeComet Swift.
109P/Swift–Tuttle
Sketch of the comet on 23 August 1862 by G. J. Chambers
Discovery
Discovered byLewis Swift
Horace Parnell Tuttle
Discovery date16–19 July 1862
Designations
P/1737 N1; P/1862 O1
P/1992 S2
1737 II; 1862 III;
1992 XXVIII
Orbital characteristics[1][2][3]
Epoch4 December 1995 (JD 2448960.5)
Observation arc257 years
Earliestprecovery date69 BC
Number of
observations
652
Aphelion51.225 AU
Perihelion0.9595 AU
Semi-major axis26.092 AU
Eccentricity0.9632
Orbital period133.28 years
Max.orbital speed42.6 km/s (26.5 mi/s)[a]
Min.orbital speed0.8 km/s (0.50 mi/s) (2059-Dec-12)
Inclination113.45°
139.44°
Argument of
periapsis
153.00°
Last perihelion12 December 1992
Next perihelion12 July 2126
TJupiter–0.280
EarthMOID0.0009 AU (130,000 km; 84,000 mi)
Physical characteristics[4]
Dimensions26 km (16 mi)
Comet total
magnitude
(M1)
4.5
Comet nuclear
magnitude (M2)
8.5
Orbital period
at different passages
[3]
Perihelion
date
Orbital
period

(years)
2392-09-16132.7
2261-08-10134.6
2126-07-12136.2
1992-12-12135.0
1862-08-23131.7
1737-06-15127.8
1610-02-06130.5
1479-10-18133.4
1348-05-02135.0

Comet Swift–Tuttle (formally designated109P/Swift–Tuttle) is a largeperiodiccomet with a 1995 (osculating)orbital period of 133 years that is in a 1:11orbital resonance withJupiter. It fits the classical definition of aHalley-type comet, which has anorbital period between 20 and 200 years.[4] The comet was independently discovered byLewis Swift on 16 July 1862 and byHorace Parnell Tuttle on 19 July 1862.

Itsnucleus is 26 km (16 mi) in diameter.[4] Swift–Tuttle is the parent body of thePerseidmeteor shower, perhaps the best known shower and among the most reliable in performance.[5]

The comet made a return appearance in 1992, when it was rediscovered by Japaneseastronomer Tsuruhiko Kiuchi and became visible with binoculars.[6] It was last observed in April 1995 when it was 8.6 AU (1.3 billion km) from the Sun.[1] In 2126, it will be a bright naked-eye comet reaching anapparent magnitude of about 0.7.[3]

Historical observations

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Older passages[3]
CE/BCEDate
188 CE188-07-10
69 BCE–68-08-27
322 BCE–321-09-27

Chinese records indicate that, in 188, the comet reachedapparent magnitude 0.1.[3] Observation was also recorded in 69BCE, and it was probably visible to the naked eye in 322 BCE.[7]

In the discovery year of 1862, the comet was as bright asPolaris.[8]

After the 1862 observations, it was incorrectly theorized that the comet would return between 1979 and 1983. However, it had been suggested in 1902 that this was the same comet as that observed byIgnatius Kegler on 3 July 1737[9] and on this basisBrian Marsden calculated correctly that it would return in 1992.[7]

Orbit

[edit]
Animation of 109P/Swift–Tuttle orbit from 1850 to 2150 (  Sun ·  Earth ·  Jupiter ·  Saturn ·  Uranus ·  109P/Swift–Tuttle)
Animation of 109P/Swift–Tuttle's close approach to Earth in 2126

The comet's perihelion is just under that ofEarth, while its aphelion is just over that ofPluto. An unusual aspect of its orbit is that it was recently captured into a 1:11orbital resonance withJupiter; it completes one orbit for every 11 of Jupiter.[7] It was the first comet in aretrograde orbit to be found in a resonance.[7] In principle this would mean that itsproper long-term average period would be 130.48 years, as itlibrates about the resonance. Over the short term, betweenepochs 1737 and 2126 the orbital period varies between 128 and 136 years.[1] However, it only entered this resonance about 1000 years ago, and will probably exit the resonance in several thousand years.[7]

Threat to Earth

[edit]

The comet is on anorbit that makes repeated close approaches to theEarthMoon system,[7] and has an Earth-MOID (Minimum orbit intersection distance) of 0.0009 AU (130,000 km; 84,000 mi).<[4] Upon its September 1992 rediscovery, the comet's date ofperihelion passage was off from the 1973 prediction by 17 days.[10] It was then noticed that if its next perihelion passage (July 2126) was also off by another 15 days (July 26), the comet could impact the Earth or the Moon on 14 August 2126 (IAUC 5636: 1992t).[11]

Distance of Comet Swift–Tuttle from Earth in Astronomical Units and millions of kilometres (gigametres) from 800 BCE to 2500 CE. Approaches in the shaded area are not visible to the unaided eye. The dashed line shows approximately the current year.

Given the size of the nucleus of Swift–Tuttle, this was of some concern. This prompted amateur astronomer and writerGary W. Kronk to search for previous apparitions of this comet. He found the comet was most likely observed by the Chinese at least twice, first in 69 BCE and later in 188 CE;[12] these two sightings were quickly confirmed by Brian Marsden and added to the list of perihelion passages at theMinor Planet Center.[1] Around 25 July 188 CE the comet passed about 0.129 AU (19.3 million km) from Earth.[3]

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.[10] It is now known that the comet will pass 0.153 AU (22.9 million km; 14.2 million mi) from Earth on August 5, 2126.[4][b] and within 0.147 AU (22.0 million km; 13.7 million mi) from Earth on August 24, 2261.[3]

APerseid meteor, originating from Comet Swift–Tuttle, from theISS

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 0.011 AU (1.0 million mi; 1.6 million km).[13] Another close encounter is predicted for the year 4479, around Sept. 15; the close approach is estimated to be less than 0.05AU, with a probability of impact of 1 in a million.[7] 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%).[7]

Comet Swift–Tuttle is by far the largestnear-Earth object (Apollo orAten asteroid orshort-period comet) to cross Earth's orbit and make repeated close approaches to Earth.[4] With a relative velocity of 60 km/s,[14][15] an Earth impact would have an estimated energy of ~27 times that of theCretaceous–Paleogene impactor.[c] 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 to433 Eros and about 3000 other kilometer-sized objects of concern.[16]

Comet Swift–Tuttle Closest Earth Approach on 2126-Aug-05 15:50 UT[4]
Date & time of
closest approach
Earth distance
(AU)
Sun distance
(AU)
Velocity
wrt Earth
(km/s)
Velocity
wrt Sun
(km/s)
Uncertainty
region
(3-sigma)
Reference
2126-08-05 15:500.15337 AU (22.944 million km; 14.257 million mi; 59.69 LD)1.04 AU (156 million km; 97 million mi; 400 LD)58.340.8± 11000 kmHorizons

See also

[edit]

Notes

[edit]
  1. ^v = 42.12191/r − 0.5/a, wherer is the distance from the Sun, anda is thesemimajor axis.
  2. ^The3-sigma uncertainty in the comet's closest approach to Earth on 5 August 2126 is about±10 thousand km.
  3. ^This calculation can be carried out in the manner given by Weissman forComet 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 1.15×1032ergs, or 2.75×109megatons, about 27.5 times the estimated energy of theK–T impact event.

References

[edit]
  1. ^abcd"109P/Swift–Tuttle".www.minorplanetcenter.net.Minor Planet Center. Retrieved17 June 2014.
  2. ^Nakano, Syuichi (1999-11-18)."109P/Swift–Tuttle (NK 798)". OAA Computing and Minor Planet Sections. Retrieved2011-05-09.
  3. ^abcdefgK. Yau; D. K. Yeomans; P. Weissman (1994)."The Past and Future Motion of Comet P/Swift-Tuttle"(PDF).Monthly Notices of the Royal Astronomical Society.266 (2):305–316.Bibcode:1994MNRAS.266..305Y.doi:10.1093/mnras/266.2.305.
  4. ^abcdefg"109P/Swift–Tuttle – JPL Small-Body Database Lookup".ssd.jpl.nasa.gov.Jet Propulsion Laboratory. Retrieved9 May 2011.
  5. ^J. Bedient (20 June 2010)."Meteor Showers".American Meteor Society. Retrieved31 July 2010.
  6. ^Britt, Robert (2005-08-11)."Top 10 Perseid Meteor Shower Facts".Space.com. Retrieved2009-08-10.
  7. ^abcdefghJ. E. Chambers (1995). "The long-term dynamical evolution of Comet Swift–Tuttle".Icarus.114 (2):372–386.Bibcode:1995Icar..114..372C.doi:10.1006/icar.1995.1069.
  8. ^Levy, David H. (2008).David Levy's Guide to Observing Meteor Showers. Cambridge University Press. p. 12.ISBN 978-0-521-69691-3.
  9. ^G. W. Kronk; M. Meyer; D. A. J. Seargent (1999).Cometography: A Catalog of Comets. Vol. 1: Ancient–1799.Cambridge University Press. pp. 400–402.ISBN 978-0-521-58504-0.
  10. ^abStephens, Sally (1993)."on Swift–Tuttle's possible collision".Astronomical Society of the Pacific.Archived from the original on 2012-05-25. Retrieved2008-08-25.
  11. ^Marsden, Brian G. (1992-10-15)."IAUC 5636: Periodic Comet Swift–Tuttle (1992t)".Central Bureau for Astronomical Telegrams. Retrieved2009-06-19.
  12. ^Marsden, Brian G. (1992-12-05)."IAUC 5670: Periodic Comet Swift–Tuttle (1992t)".Central Bureau for Astronomical Telegrams. Retrieved2009-06-19.
  13. ^"ASP: Cosmic Collisions". Archived fromthe original on 2012-12-19.
  14. ^P. R. Weissman (2006). A. Milani; G. B. Valsecchi; D. Vokrouhlicky (eds.).The Cometary Impactor Flux at the Earth(PDF). Near Earth Objects, our Celestial Neighbors: Opportunity and Risk; IAU Symposium No. 236.Proceedings of the International Astronomical Union. Vol. 2, no. 236. pp. 441–450.doi:10.1017/S1743921307003559.
  15. ^abG. L. Verschuur (1997).Impact!: The Threat of Comets and Asteroids.Oxford University Press. p. 216.ISBN 978-0-19-511919-0.
  16. ^M. W. Browne (25 April 1996)."Mathematicians Say Asteroid May Hit Earth in a Million Years".The New York Times. Retrieved16 November 2018.

Bibliography

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External links

[edit]


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