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153P/Ikeya–Zhang

From Wikipedia, the free encyclopedia
Long-period comet
For other comets discovered by Kaoru Ikeya, seeComet Ikeya.
153P/Ikeya-Zhang
Comet Ikeya–Zhang photographed by Philipp Salzgeber on 1 April 2002
Discovery
Discovered byKaoru Ikeya
Zhang Daqing
Discovery date1 February 2002
Designations
Orbital characteristics[6]
Epoch8 May 2002 (JD 2452402.5)
Observation arc341–1,125 years
Earliestprecovery dateFebruary 877[1]
3 February 1661[5]
Number of
observations
1,893
Aphelion101.73 AU
Perihelion0.507 AU
Semi-major axis51.119 AU
Eccentricity0.99008
Orbital period365.49 years
Max.orbital speed59 km/s
(2002-03-18)
Min.orbital speed0.29 km/s[a]
(2182-Nov-24)
Inclination28.121°
93.369°
Argument of
periapsis
34.668°
Mean anomaly0.135°
Last perihelion18 March 2002[6][7]
29 January 1661[8]
Next perihelion1 September 2362[8]
14 March 2363[9]
TJupiter0.879
EarthMOID0.332 AU
JupiterMOID0.011 AU
Physical characteristics[6]
Mean diameter
5.09 km (3.16 mi)[10]
1.48±0.2 days[11]
Comet total
magnitude
(M1)
4.0
2.9
(2002 apparition)

Comet Ikeya–Zhang (Japanese, Chinese: 池谷-張彗星, officially designated153P/Ikeya–Zhang) is along-period comet discovered independently by two astronomers fromJapan andChina in 2002. It has by far the longest orbital period of thenumbered periodic comets. It was last observed in October 2002 when it was about 3.3 AU (490 million km) from the Sun.[6]

Discovery and observations

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On 1 February 2002, Chinese astronomerZhang Daqing fromKaifeng discovered a new comet in theconstellationCetus, and reported it to theIAU. He found that Japanese astronomerKaoru Ikeya had discovered it earlier than he had, as the time of sunset is earlier than China. According to tradition, since they discovered the new comet independently, the comet was named after both of them. The comet was initially designated asC/2002 C1 (Ikeya–Zhang).

The comet was observed in 1661, 341 years earlier, by Polish astronomerJohannes Hevelius.[12][5] A bright comet had also been recorded by Chinese astronomers in 1661.[5] Further research byIchiro Hasegawa andShuichi Nakano concluded that historical comets recorded in A.D. 877[2] and 1273[3] were likely previous apparitions of Ikeya–Zhang as well.[1]

The permanent designation "153P" was given to the comet. It has the longest known orbital period of anyperiodic comet (366.51 years). Itsorbital speed around the Sun varies from 59 km/s (37 mi/s) atperihelion to 0.29 km/s (0.18 mi/s) at aphelion.[a]

The comet passed perihelion on 18 March 2002, and withapparent magnitude 2.9. With a multi-hundred year orbit involving asymmetric outgassing the next perihelion passage is expected between 2362–2363. During March–April 2002, protons from the comet tail may have been detected by theCassini–Huygens spacecraft. This data suggested the comet tail had a length greater than 7.5 AU (1.12 billion km), making it the longest yet detected.[13]

Orbit

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The orbital paths of three comets, outlined in turquoise, against the orbits of Jupiter, Saturn, Uranus and Neptune, outlined in green
The orbits of threeperiodic comets,Halley,Borrelly and Ikeya–Zhang, set against the orbits of theouter planets. Ikeya–Zhang is to the right.

See also

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Notes

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  1. ^abv = 42.12191/r − 0.5/a, wherer is the distance from the Sun, anda is the major semi-axis.

References

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  1. ^abcdI. Hasegawa; S. Nakano (2003)."Orbit of periodic comet 153P/Ikeya–Zhang".Monthly Notices of the Royal Astronomical Society.345 (3):883–888.Bibcode:2003MNRAS.345..883H.doi:10.1046/j.1365-8711.2003.07009.x.
  2. ^abKronk, Meyer & Seargent 1999, pp. 138–139.
  3. ^abKronk, Meyer & Seargent 1999, p. 223.
  4. ^G. W. Kronk."153P/Ikeya–Zhang".Cometography.com. Retrieved19 October 2017.
  5. ^abcdKronk, Meyer & Seargent 1999, pp. 348–350.
  6. ^abcd"153P/Ikeya–Zhang – JPL Small-Body Database Lookup".ssd.jpl.nasa.gov.Jet Propulsion Laboratory. Retrieved20 April 2011.
  7. ^"153P/Ikeya–Zhang".www.minorplanetcenter.net.Minor Planet Center. Retrieved25 February 2019.
  8. ^abS. Nakano (13 August 2002)."153P/Ikeya-Zhang". OAA Computing and Minor Planet Sections. Retrieved4 October 2009.
  9. ^"Horizons Batch for 153P/Ikeya–Zhang (90001080) on 2363-Mar-14" (Perihelion occurs when rdot flips from negative to positive).JPL Horizons. Retrieved10 April 2021. (JPL#74/Soln.date: 2020-Jun-17)
  10. ^E. Rondón; F. Roig; D. Lazzaro; F. Fernandez."Secular light curves of periodic comets observed by SWAN/SOHO"(PDF).Monthly Notices of the Royal Astronomical Society.538 (4):2869–2904.Bibcode:2025MNRAS.538.2869R.doi:10.1093/mnras/staf454.
  11. ^F. Manzini; G. Schwarz; C. B. Cosmovici; C. Guaita; et al. (2007)."Comet Ikeya-Zhang (C/2002 C1): Determination of the Rotation Period From Observations of Morphological Structures"(PDF).Earth, Moon, and Planets.100 (1–2):1–16.Bibcode:2007EM&P..100....1M.doi:10.1007/s11038-005-9062-6.
  12. ^D. W. Green (2004).Assessment of early-modern observations of Comets and Supernovae: Focus on Pre-telescopic European astrometric and physical data(PDF) (Doctoral thesis). Durham University. pp. 213–228.
  13. ^G. H. Jones; H. A. Elliott; D. J. McComas; M. E. Hill; et al. (2020)."Cometary Ions detected by the Cassini spacecraft 6.5 AU downstream of Comet 153P/Ikeya-Zhang"(PDF).Icarus.388 15199.arXiv:2006.00500.Bibcode:2022Icar..38815199J.doi:10.1016/j.icarus.2022.115199.

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.

External links

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154P/Brewington
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