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55P/Tempel–Tuttle

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For other comets discovered by Wilhelm Tempel and Horace Tuttle, see Comet Tempel (disambiguation) and Comet Tuttle (disambiguation).
55P/Tempel–Tuttle
Comet Tempel–Tuttle photographed by the Hubble Space Telescope on 9 January 1998
Discovery
Discovered byWilhelm Tempel
Horace Parnell Tuttle
Discovery date19 December 1865
Designations
  • P/1366 U1, P/1699 U1
  • P/1865 Y1, P/1965 M2
  • P/1997 E1
1699 II, 1866 I, 1965 IV
Orbital characteristics[2][3]
Epoch25 February 2023 (JD 2460000.5)
Observation arc631.69 years
Earliest precovery date25 October 1366[1]
Number of
observations		471
Aphelion19.732 AU
Perihelion0.975 AU
Semi-major axis10.354 AU
Eccentricity0.90587
Orbital period33.318 years
Inclination162.48°
235.41°
Argument of
periapsis		172.45°
Mean anomaly271.09°
Last perihelion28 February 1998
Next perihelion20 May 2031
TJupiter–0.637
Earth MOID0.008 AU
Physical characteristics
Mean radius
1.8 ± 0.2 km (1.12 ± 0.12 mi)[4][5]
14.79–15.31 hours[6]
  • (B−V) = 0.75±0.05[7]
  • (V–R) = 0.51±0.05[8]
Comet total
magnitude (M1)		10.0
Comet nuclear
magnitude (M2)		16.0

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 19 December 1865, and by Horace Parnell Tuttle on 6 January 1866. It is the parent body of the Leonid meteor shower.

Observational history

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Sketch of the comet as it was discovered by Wilhelm Tempel on 19 December 1865.

In 1699, it was observed by Gottfried Kirch,[9] however it 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.[10] On 26 October 1366, the comet passed 0.0229 AU (3.43 million km; 2.13 million mi) from Earth.[11] It is possible the comet was also observed in October 1234, however it is only mentioned briefly by a single Japanese source, and also a comet observed in China in January 1035 could be comet Temple–Tuttle, however unless it had undergone a major outburst, it would have been too dim to observe with the naked eye.[12]

Comet Tempel–Tuttle was recovered by J. Schubart in images taken by Michiel John Bester on 30 June 1965 using the 10-inch telescope of Boyden Observatory, South Africa. At that time the comet had an apparent magnitude of 16.[13] The presence of the comet was confirmed in plates obtained by Palomar Observatory on 30 June. These were the only two observations of the comet during the 1965 apparition.[14]

The comet was recovered on 4 March 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.[15] During the 1998 apparition the comet brightened more than predicted and reached an apparent magnitude of 7.4–7.8 in late February and could be observed with binoculars. It was last observed on 5 July 1998.[16]

Physical characteristics

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The nucleus of the comet was observed by Hubble Space Telescope during the 1998 apparition, and assuming an albedo of 0.04, its nucleus was estimated to have a mean radius of 1.8 km.[17] Spectrometric observations of its nucleus reveal that it has a reddish color, with a B−V of 0.75±0.05 and V−R of 0.51±0.05.[7][8] A jet was observed emanating from the nucleus and based on its movement the rotation period was calculated to be between 14.79±0.02 and 15.31±0.03 hours.[6]

The spectrum of the comet revealed the presence of diatomic carbon, NH2 and [Oi]. The relative production rates indicate that the comet is depleted in diatomic carbon, with the gas-to-dust ratio also indicated it was gas rich compared with Halley's Comet.[18] The infrared spectrum of the comet closely resembled that of a black body with a temperature of 330 K and lacked silicate emission that has been detected in other comets.[19]

William Huggins observed the spectrum of the comet in January 1866, making it the second time spectrographic observations of a comet were obtained.[20]

55P/Tempel–Tuttle is estimated to have a total nuclear mass of 1.2×1013 kg,[21] with its meteoroid stream is estimated to have a mass of 5×1012 kg in total.[21]

Orbit

[edit]
55P/Tempel–Tuttle Earth approaches
Year Nominal geocentric
distance (AU)
1366 0.023 AU (3.4 million km)[11][16]
1699 0.064 AU (9.6 million km)[22][16]
1832 0.171 AU (25.6 million km)[23][22]
1998 0.356 AU (53.3 million km)[24][22]
2031 0.791 AU (118.3 million km)[25][22]
2163 0.132 AU (19.7 million km)[2]

Orbital calculations in 2014 suggested that Tempel–Tuttle was at one point about 5,000 years before discovery, the comet made a close encounter with Uranus, which reduced its orbital period from that of a long-period comet out to the Kuiper Belt to its present-day 33-year retrograde orbit around the Sun, however this remains unconfirmed.[26]

The comet currently has an Earth-MOID of about 0.008 AU (1.2 million km).[2]

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

Meteor shower

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Tempel–Tuttle is the parent body of the Leonid meteor shower. 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. 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.[27] Between 2021–2030, Earth will often pass through the meteoroid stream left behind from the 1733 orbit.[28]

See also

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References

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  1. ^ Kronk, Meyer & Seargent 1999, pp. 246–248.
  2. ^ a b c "55P/Tempel–Tuttle – JPL Small-Body Database Lookup". ssd.jpl.nasa.gov. Jet Propulsion Laboratory. Retrieved 2 February 2017.
  3. ^ "55P/Tempel–Tuttle Orbit". Minor Planet Center. Retrieved 16 June 2014.
  4. ^ O. R. Hainaut; K. J. Meech; H. Boehnhardt; R. M. West (1998). "Early recovery of Comet 55P/Tempel–Tuttle". Astronomy & Astrophysics. 333: 746–752. Bibcode:1998A&A...333..746H.
  5. ^ K. J. Meech; O. R. Hainaut; B. G. Marsden (2000). A. Fitzsimmons; D. C. Jewitt; R. M. West (eds.). Comet Size Distributions and Distant Activity. Minor Bodies in the Outer Solar System. Berlin, Germany. pp. 75–80. Bibcode:2000mbos.work...75M. doi:10.1007/10651968_10. ISBN 3-540-41152-6.
  6. ^ a b L. Jorda; J. Lecacheux; F. Colas; et al. (30 January 1998). D. W. Green (ed.). "Comet 55P/Tempel–Tuttle". IAU Circular. 6816 (2). Bibcode:1998IAUC.6816....2J. ISSN 0081-0304.
  7. ^ a b P. Lamy; I. Toth (2009). "The colors of cometary nuclei—Comparison with other primitive bodies of the Solar System and implications for their origin". Icarus. 201 (2): 674–713. Bibcode:2009Icar..201..674L. doi:10.1016/j.icarus.2009.01.030.
  8. ^ a b M. M. Knight; R. Kokotanekova; N. H. Samarasinha (2023). "Physical and Surface Properties of Comet Nuclei from Remote Observations". arXiv:2304.09309 [astro-ph.EP].
  9. ^ Kronk, Meyer & Seargent 1999, p. 385.
  10. ^ J. Schubart (1966). "Comet Tempel–Tuttle: Recovery of the Long-Lost Comet of the November Meteors". Science. 152 (3726): 1236–1237. Bibcode:1966Sci...152.1236S. doi:10.1126/science.152.3726.1236. PMID 17769538.
  11. ^ a b "Closest Approaches to the Earth by Comets". Minor Planet Center. Retrieved 28 June 2012.
  12. ^ D. K. Yeomans; K. K. Yau; P. R. Weissman (1996). "The Impending Appearance of Comet Tempel–Tuttle and the Leonid Meteors". Icarus. 124 (2): 407–413. Bibcode:1996Icar..124..407Y. doi:10.1006/icar.1996.0218.
  13. ^ J. Schubart; M. J. Bester; E. Geyer (4 October 1965). O. Gingerich (ed.). "Periodic Comet Tempel–Tuttle (1965i)". IAU Circular. 1926 (3). Bibcode:1965IAUC.1926....3S. ISSN 0081-0304.
  14. ^ J. Schubart; E. Geyer (1 November 1966). O. Gingerich (ed.). "Periodic Comet Tempel–Tuttle (1965i)". IAU Circular. 1979 (1). Bibcode:1966IAUC.1979....1S. ISSN 0081-0304.
  15. ^ "Comet 55P/Tempel–Tuttle Through History".
  16. ^ a b c C&MS: 55P/Tempel–Tuttle
  17. ^ P. Lamy; V. Znojil; N. Biver (27 March 1998). D. W. Green (ed.). "Comet 55P/Tempel–Tuttle". IAU Circular. 6851 (2). Bibcode:1998IAUC.6851....2L. ISSN 0081-0304.
  18. ^ T. Hamane; H. Kawakita; B. Suzuki; et al. (2003). "Gas-to-dust ratio and chemical composition in comet 55P/Tempel–Tuttle". The Institute of Space and Astronautical Science Report. S.P: 17–22.
  19. ^ D. Lynch (2000). "3- to 14- μm Spectroscopy of Comet 55P/Tempel–Tuttle, Parent Body of the Leonid Meteors". Icarus. 144 (1): 187–190. Bibcode:2000Icar..144..187L. doi:10.1006/icar.1999.6260.
  20. ^ Huggins, William (31 December 1867). "II. On the spectrum of comet 1, 1866". Proceedings of the Royal Society of London. 15: 5–7. doi:10.1098/rspl.1866.0004.
  21. ^ a b D. C. Jewitt (2004). "From Cradle To Grave: The Rise and Demise of the Comets" (PDF). Comets II. University of Arizona Press. pp. 659–676. Bibcode:2004come.book..659J.
  22. ^ a b c d 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.
  23. ^ "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.
  24. ^ "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.
  25. ^ "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)
  26. ^ R. A. Guliyev (2014). "About the Origin of Comet 55P" (PDF). Astronomical School's Report (in Azerbaijani). 10 (2): 179–182. Bibcode:2014AstSR..10..179G. doi:10.18372/2411-6602.10.2179.
  27. ^ Archive of Leonid dust trail positions in 1833
  28. ^ Mikhail, Maslov. "Leonids 2021–2030". Archived from the original on 10 June 2021. Retrieved 10 June 2021.

Bibliography

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  • Kronk, Gary W.; Meyer, Maik; Seargent, David A. J. (1999). Cometography: A Catalog of Comets. Vol. 1: Ancient–1799. Cambridge University Press. ISBN 978-0-521-58504-0.
[edit]


Numbered comets
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