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C/1983 H1 (IRAS–Araki–Alcock)

From Wikipedia, the free encyclopedia
(Redirected fromComet IRAS–Araki–Alcock)
Long-period comet

For the other comets discovered by George E. D. Alcock and the Infrared Astronomical Satellite, seeComet Alcock andComet IRAS.
C/1983 H1
(IRAS–Araki–Alcock)
Comet IRAS–Araki–Alcock photographed by Russell E. Milton on 11 May 1983
Discovery[1][2]
Discovered byIRAS
George E. D. Alcock
Genichi Araki
Discovery date25 April 1983
Designations
1983d[3]
1983 VII
Orbital characteristics[4]
Epoch13 May 1983 (JD 2445467.5)
Observation arc160 days
Number of
observations
347
Aphelion195.08 AU
Perihelion0.9913 AU
Semi-major axis98.034 AU
Eccentricity0.98989
Orbital period970.49 years
Inclination73.251°
49.102°
Argument of
periapsis
192.85°
Last perihelion21 May 1983
TJupiter0.408
EarthMOID0.0058 AU
JupiterMOID3.0838 AU
Physical characteristics[4][5]
Dimensions9.2 km (5.7 mi)
51.3±0.3 hours
0.02
Comet total
magnitude
(M1)
12.6
3–4
(1983 apparition)

Comet IRAS–Araki–Alcock (formal designationC/1983 H1, formerly1983 VII) is a long-periodcomet that, in 1983, made the closest known approach to Earth of any comet in the last 200 years, at a distance of about 0.0312 AU (4.67 million km; 2.90 million mi).[3]

Discovery and observations

[edit]
A false colour image of Comet IRAS–Araki–Alcock in 1983, viewed ininfrared light by theInfrared Astronomical Satellite (IRAS)
This figure combines anInternational Ultraviolet Explorer FES image showing its diffuse tail, and the long-wavelength redundant (LWR) spectrum depicting the molecular emission lines of sulfur (S2) and hydroxyl (OH).

The comet was named after its discoverers – theInfrared Astronomical Satellite and two amateurastronomers,George Alcock of theUnited Kingdom and Genichi Araki ofJapan. Both men were schoolteachers by profession, although Alcock was retired. Alcock had made his discovery simply by observing through the window of his home, usingbinoculars.[6][7] During the closest approach, the comet appeared as a circular cloud about the size of the full moon, having no discernible tail, and shining at a naked eyemagnitude of 3–4. It swept across the sky at an angular speed of about 30 degrees per day. On May 11 the comet was detected on radar byArecibo Observatory andGoldstone Solar System Radar making it the first comet detected by two different radar systems.[8] A second detection was made by Goldstone on 14 May.[8]

It is a long-period comet, with an orbital period of about 970 years,[4] and is the parent comet of the minorEta Lyridmeteor shower.[9] This shower'sradiant lies betweenVega andCygnus and produces 1 or 2 meteors an hour in mid-May with a peak between 9 May and 11 May.

Flyby

[edit]
The comet passed from north to south between 9 May to 13 May, passing throughUrsa Major towardsCancer. Its motion is marked every 2 hours here.
Moving north to south, it crossed just inside the Earth's orbit on 11 May.

Comet IRAS–Araki–Alcock made its closest approach to Earth in 1983, at a distance of about 0.0312 AU (4.67 million km; 2.90 million mi). It was the closest approach up to that time of any comet in the last 200 years; onlyLexell's Comet (1770) and55P/Tempel–Tuttle (1366) are thought to have come closer.[4][10] Subsequently, on 12 June 1999, the small cometP/1999 J6 (SOHO) passed about 0.012 AU (1.8 million km; 1.1 million mi) from Earth.[11] What was thought to be a small fragment of252P/LINEAR,460P/PANSTARRS, passed at a distance of 0.0237 AU (3.55 million km; 2.20 million mi) on 22 March 2016.[12]

See also

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References

[edit]
  1. ^B. G. Marsden (4 May 1983)."Comet IRAS-Araki-Alcock (1983d)".Central Bureau for Astronomical Telegrams.3796: 1.Bibcode:1983IAUC.3796....1D.
  2. ^"IRAS–Araki–Alcock, Comet (C/1983 H1)".Oxford Reference.Oxford University Press. Retrieved19 December 2024.
  3. ^abA. Hale (9 May 2020)."Comet of the Week: IRAS-Araki-Alcock (1983d)".RocketSTEM.org. Retrieved19 December 2024.
  4. ^abcd"C/1983 H1 (IRAS–Araki–Alcock) – JPL Small-Body Database Lookup".ssd.jpl.nasa.gov.Jet Propulsion Laboratory. Retrieved28 June 2012.
  5. ^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].
  6. ^"Obituary of George Alcock".BBC News. 21 December 2000.
  7. ^"Outbreak of Comet Fever".Time. 23 May 1983. Archived fromthe original on 14 November 2007.
  8. ^abJ. K. Harmon; D. B. Campbell; S. J. Ostro; M. C. Nolan (1999)."Radar observations of comets"(PDF).Planetary and Space Science.47 (12):1409–1422.Bibcode:1999P&SS...47.1409H.doi:10.1016/S0032-0633(99)00068-9.
  9. ^"Eta Lyrids".Meteor Showers Online.Archived from the original on 5 May 2012. Retrieved21 November 2008.
  10. ^"Closest Approaches to the Earth by Comets".Minor Planet Center. Retrieved28 June 2012.
  11. ^"P/1999 J6 (SOHO) – JPL Small-Body Database Lookup".ssd.jpl.nasa.gov.Jet Propulsion Laboratory. Retrieved28 June 2012.
  12. ^"NEO Earth Close Approaches".neo.jpl.nasa.gov.Jet Propulsion Laboratory. Archived fromthe original on 7 March 2014. Retrieved4 March 2014.

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