27P/Crommelin

Last updated
27P/Crommelin
Comet Forbes 1928c - F. Quenisset - 28-10-1928.jpg
The comet on 28 October 1928, by Ferdinand Quénisset
Discovery
Discovered by J.-L. Pons
Discovery dateFebruary 23, 1818
Designations
1818 D1, 1873 V1, 1928 W1, 1956 S1
Orbital characteristics
Epoch July 18, 2011
Observation arc 84 years (1928-2012)
Number of
observations
392 [1]
Aphelion 17.660 AU
Perihelion 0.748 AU
Semi-major axis 9.204 AU
Eccentricity 0.919
Orbital period 27.9 yr
27y 10m 2d (perihelion to perihelion)
Inclination 28.96°
Last perihelionAugust 3, 2011 [2] [1]
February 20, 1984 [2]
Next perihelionMay 27, 2039 [2] [1] [3]

Comet Crommelin, also known as Comet Pons-Coggia-Winnecke-Forbes, is a periodic comet with an orbital period of almost 28 years. It fits the classical definition of a Halley-type comet with (20 years < period < 200 years). It is named after the British astronomer Andrew C. D. Crommelin who calculated its orbit in 1930. It is one of only four comets not named after their discoverer(s), the other three being Comets Halley, Encke, and Lexell. It next comes to perihelion (closest approach to the Sun) around May 27, 2039 when it will be near a maximum near-perihelion distance from Earth.

Contents

Observational history

The first observation was by Jean-Louis Pons (Marseille, France) on February 23, 1818, he followed the comet until February 27 but was prevented further by bad weather. Johann Franz Encke attempted to calculate the orbit but was left with very large errors.

In 1872, John R. Hind produced a rough orbital calculation and observed it was close to that of Comet Biela, based on these observations, Edmund Weiss later speculated it may have been part of Biela's comet.

The next observation was on November 10, 1873, by Jérôme E. Coggia (Marseille, France), and again on November 11 by Friedrich A. T. Winnecke (Strasbourg, France), but it was lost by November 16. Weiss and Hind took up the calculations and tried to match it again with the 1818 appearance.

A third discovery was by Alexander F. I. Forbes (Cape Town, South Africa) on November 19, 1928, and confirmed by Harry E. Wood (Union Observatory, South Africa) on November 21. It was Crommelin who eventually established the orbit and finally linked the 1818 (Pons) and 1873 (Coggia-Winnecke) comets to it (also see Lost comet).

On its latest return, 27P/Crommelin was recovered on May 12, 2011, at apparent magnitude 18.7 [4] and peaked at magnitude 10.7 at perihelion on August 3. [5] 27P/Crommelin was last observed in January 2012 and passed 1.5 AU from Saturn on July 11, 2015. [6]

The next perihelion will be on May 27, 2039. [2] [3] Near perihelion the comet will be 0.74 AU from the Sun and 1.73 AU from Earth. [3] This is about as far from Earth as the comet can get during perihelion.

On December 22, 2120 it will pass 0.297  AU (44.4 million  km ) from Earth. [6]

Related Research Articles

<span class="mw-page-title-main">Jean-Louis Pons</span> French astronomer (1761–1831)

Jean-Louis Pons was a French astronomer. Despite humble beginnings and being self-taught, he went on to become the greatest visual comet discoverer of all time: between 1801 and 1827 Pons discovered thirty-seven comets, more than any other person in history.

<span class="mw-page-title-main">Comet Encke</span> Periodic comet with 3-year orbit

Comet Encke, or Encke's Comet, is a periodic comet that completes an orbit of the Sun once every 3.3 years. Encke was first recorded by Pierre Méchain on 17 January 1786, but it was not recognized as a periodic comet until 1819 when its orbit was computed by Johann Franz Encke. Like Halley's Comet, it is unusual in its being named after the calculator of its orbit rather than its discoverer. Like most comets, it has a very low albedo, reflecting only 4.6% of the light its nucleus receives, although comets generate a large coma and tail that can make them much more visible during their perihelion. The diameter of the nucleus of Encke's Comet is 4.8 km.

<span class="mw-page-title-main">12P/Pons–Brooks</span> Periodic comet with 71-year orbit

12P/Pons–Brooks is a periodic comet with an orbital period of 71 years. Comets with an orbital period of 20–200 years are referred to as Halley-type comets. It is one of the brightest known periodic comets, reaching an absolute visual magnitude of about 5 in its approach to perihelion. Comet Pons-Brooks was conclusively discovered at Marseilles Observatory in July 1812 by Jean-Louis Pons, and on its next appearance in 1883 by William Robert Brooks. There are ancient records of comets that are suspected of having been apparitions of 12P/Pons–Brooks.

<span class="mw-page-title-main">Biela's Comet</span> Disintegrated periodic comet

Biela's Comet or Comet Biela was a periodic Jupiter-family comet first recorded in 1772 by Montaigne and Messier and finally identified as periodic in 1826 by Wilhelm von Biela. It was subsequently observed to split in two and has not been seen since 1852. As a result, it is currently considered to have been destroyed, although remnants have survived for some time as a meteor shower, the Andromedids which may show increased activity in 2023.

<span class="mw-page-title-main">10P/Tempel</span> Periodic comet with 5 year orbit

10P/Tempel, also known as Tempel 2, is a periodic Jupiter-family comet with a 5-year orbital period. It was discovered on July 4, 1873 by Wilhelm Tempel. At the perihelion passage on 2 August 2026 the solar elongation is calculated at 164 degrees, with apparent magnitude approximately 8, with closest approach to Earth on 3 August 2026 at a distance of 0.414 AU (61.9 million km).

<span class="mw-page-title-main">28P/Neujmin</span> Periodic comet with 18 year orbit

28P/Neujmin, also known as Neujmin 1, is a large periodic comet in the Solar System. With a perihelion distance of 1.5AU, this comet does not make close approaches to the Earth.

<span class="mw-page-title-main">88P/Howell</span> Periodic comet with 5 year orbit

88P/Howell is a periodic comet with a 5.5 year orbital period. It was discovered on 29 August 1981, by Ellen Howell. In 1975 the comet's perihelion was 1.9 AU, but a close approach to Jupiter in 1978 perturbed the perihelion distance closer to the Sun. During the 2009 apparition the comet became as bright as apparent magnitude 8.

<span class="mw-page-title-main">7P/Pons–Winnecke</span> Periodic comet with 6-year orbit

7P/Pons–Winnecke is a periodic Jupiter-family comet with a six-year orbit. Early calculations for the 1921 apparition suggested that the orbit of the comet might collide with Earth in June, but observations on 10 April ruled out an impact. It made a very close approach to Earth in June 1927. The outward migration of perihelion created impressive meteor showers in 1916, 1921 and 1927.

<span class="mw-page-title-main">13P/Olbers</span> Periodic comet with 70 year orbit

13P/Olbers is a periodic comet with an orbital period of 69 years. It fits the classical definition of a Halley-type comet with a period between 20 and 200 years. The comet last passed perihelion 30 June 2024 and it was previously seen in 1956. The next perihelion is in 2094.

<span class="mw-page-title-main">15P/Finlay</span> Periodic comet with 6 year orbit

Comet Finlay is a periodic comet with an orbital period of 6 years discovered by William Henry Finlay on September 26, 1886. The next perihelion passage is July 13, 2021 when the comet will have a solar elongation of 54 degrees at approximately apparent magnitude 10. It last came to perihelion on December 27, 2014, at around magnitude 10. Of the numbered periodic comets, the orbit of 15P/Finlay has one of the smallest minimum orbit intersection distances with the orbit of Earth (E-MOID). In October 2060 the comet will pass about 5 million km from Earth.

Comet 177P/Barnard, also known as Barnard 2, is a periodic comet with an orbital period of 122 years. It fits the classical definition of a Halley-type comet with. It orbits near the ecliptic plane and has aphelion near the Kuiper cliff at 48 AU (7.2 billion km).

<span class="mw-page-title-main">22P/Kopff</span> Periodic comet with 6 year orbit

Comet Kopff or 22P/Kopff is a periodic comet in the Solar System. Discovered on August 23, 1906, it was named after August Kopff who discovered the comet. The comet was missed on its November 1912 return, but was recovered on its June 1919 return and has been seen at every apparition since. Close approaches to Jupiter in 1938 and 1943 decreased the perihelion distance and orbital period. 22P/Kopff’s last perihelion passage was 18 March 2022. On 13 July 2028 it will pass 0.353 AU (52.8 million km) from Earth.

<span class="mw-page-title-main">35P/Herschel–Rigollet</span> Periodic comet with 155 year orbit

35P/Herschel–Rigollet is a periodic comet with an orbital period of 155 years and an orbital inclination of 64 degrees. It fits the classical definition of a Halley-type comet with. It was discovered by Caroline Herschel on 21 December 1788. Given that the comet has a 155-year orbit involving asymmetric outgassing, and astrometric observations in 1939 were not as precise as modern observations, predictions for the next perihelion passage in 2092 vary by about a month.

<span class="mw-page-title-main">38P/Stephan–Oterma</span> Periodic comet with 38 year orbit

38P/Stephan–Oterma is a periodic comet with an orbital period of 38 years. It fits the classical definition of a Halley-type comet with. It was discovered on 22.9 January 1867, by Jérôme Eugène Coggia at Marseilles Observatory, France. On 25.86 January Édouard Stephan confirmed it was a comet. It was recovered in 6 November 1942 by the Finnish astronomer Liisi Oterma.

<span class="mw-page-title-main">94P/Russell</span> Periodic comet with 6 year orbit

94P/Russell 4 is a periodic comet in the Solar System. It fits the definition of an Encke-type comet with. It was discovered by Ken Rusell on photographic plates taken by M. Hawkins on March 7, 1984. In the discovery images, Russell estimated that the comet had an apparent magnitude of 13 and a noticeable tail of 5 arc minutes. In the year of discovery, the comet had come to perihelion in January 1984.

<span class="mw-page-title-main">43P/Wolf–Harrington</span> Periodic comet with 6 year orbit

43P/Wolf–Harrington is a periodic comet discovered on December 22, 1924, by Max Wolf in Heidelberg, Germany. In 2019 it passed within 0.065 AU of Jupiter, which lifted the perihelion point and increased the orbital period to 9 years.

82P/Gehrels is a periodic comet that was discovered on October 27, 1975, by Tom Gehrels at the Palomar Mountain Observatory in California having a faint nuclear brightness of magnitude 17.

C/2000 W1 (Utsunomiya–Jones) is a long-period comet from the Oort cloud discovered on November 18, 2000, by Syogo Utsunomiya and Albert F. A. L. Jones. The comet reached up to apparent magnitude 5.5, but was only 27 degrees from the Sun in mid-December 2000.

163P/NEAT is a periodic comet discovered on November 5, 2004 by Near-Earth Asteroid Tracking (NEAT) using the 1.2 meter Samuel Oschin telescope at Palomar Observatory.

<span class="mw-page-title-main">62P/Tsuchinshan</span> Periodic comet with 6 year orbit

62P/Tsuchinshan, also known as Tsuchinshan 1, is a periodic comet first discovered January 1, 1965 at the Purple Mountain Observatory in Nanking. It last came to perihelion on 25 December 2023 at around apparent magnitude 8, and was then 0.53 AU (79 million km) from Earth and 110 degrees from the Sun.

References

  1. 1 2 3 Syuichi Nakano (2012-02-04). "27P/Crommelin (NK 2190)". OAA Computing and Minor Planet Sections. Retrieved 2012-02-18.
  2. 1 2 3 4 MPC
  3. 1 2 3 "Horizons Batch for 27P/Crommelin (90000381) on 2039-May-27" (Perihelion occurs when rdot flips from negative to positive). JPL Horizons . Retrieved 2023-05-12. (JPL#6 Soln.date: 2023-May-12)
  4. "MPEC 2011-L11 : OBSERVATIONS AND ORBITS OF COMETS". IAU Minor Planet Center. 2011-06-02. Retrieved 2011-06-13.
  5. Seiichi Yoshida (2013-02-10). "27P/Crommelin (2011) - Magnitudes Graph" . Retrieved 2016-03-19.
  6. 1 2 "JPL Small-Body Database Browser: 27P/Crommelin" (last observation: 2012-01-26). Jet Propulsion Laboratory . Retrieved 2023-05-12.
Numbered comets
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