C/1874 H1

Last updated
C/1874 H1 (Coggia)
Comet Coggia, 1874.jpg
Drawing of the comet C/1874 H1 (Coggia) (as seen on June 10th and July 9th, 1874
Discovery
Discovered by Jérôme Eugène Coggia
Discovery date17 April 1874
Designations
Comet Coggia, 1874 III, 1874c
Orbital characteristics
Epoch 2405720.5
1874-Jul-09.3583 [1]
Aphelion 1144.7 AU
Perihelion 0.676 AU [1]
Semi-major axis 572.7 AU
Eccentricity 0.9988 [1]
Orbital period ~13708 a [1]
Inclination 66.3° [1]

C/1874 H1 (Coggia) is a non-periodic comet, which in the summer of 1874 could be seen by the naked eye. On the basis of its brightness, the comet has been called the Great Comet of 1874; on July 13 of that year its apparent magnitude peaked at between 0 and 1. [2]

Contents

Discovery and observations

The astronomer Jérôme Eugène Coggia discovered this comet on 17 April 1874 at the Marseille Observatory. During the remainder of April and in May the comet was closely observed by many astronomers, including Winnecke in Straßburg, Tempel in Arcetri, Rayet in Paris, Schulhof in Vienna, Rümker in Hamburg, Schmidt in Athens, Bruhns in Leipzig, Christie in Greenwich and Dreyer in Copenhagen. In mid-May telescopes revealed the development of a faint tail.

In early June the comet became visible to the naked eye [3] [4] and by the end of June its brightness reached magnitude 4. By the beginning of July the tail had grown to 6° and by the 16th of July to 45°. The tail was straight and narrow, stretching across from 1° to 2° of the sky at the tail's end. [5]

According to David A. J. Seargent, [6]

Without doubt, C/1874 H1 (Coggia) was a beauty; a true great comet. At its brightest, it probably exceeded the first magnitude and displayed a series of envelopes within its coma that astronomers compared with Donati's Comet 16 years earlier. Suitably placed observers also noted maximum naked-eye tail lengths reaching 70 degrees as the comet passed near Earth in July.

From 16 July to 23 July, the comet accelerated and moved rapidly southward in the observer's sky, making the comet more difficult to observe in the northern hemisphere. Reports indicate that the tail length was about 60° to 70°; the tail was at least 63°. [7] On 23 July in Athens, Schmidt made the last observation of the comet from the northern hemisphere.

On July 27 [8] the comet became visible in the southern hemisphere, with observations made in South Africa and by Robert L. J. Ellery [9] in Australia. According to a newspaper report from pre-dawn observations by H. C. Russell on July 29, "The nucleus was as bright as a first magnitude star, and the head about half the diameter of the moon." [10] John Tebbutt in Windsor, New South Wales made observations of the comet from 1 August to 7 October. On 19 October, John M. Thome at Córdoba, Argentina made the last observation of Comet Coggia. [5]

Undulations in the tail

On the evening of July 21 with a first quarter moon and a very clear sky, Trouvelot observed undulations in the comet's tail. Trouvelot wrote that he "... saw the comet's tail shortening and extending, lightening up and extinguishing like the rays of certain auroras. Extended undulations, rapid vibrations, ran along it in succession from the horizon to its extremity, giving it the appearance of a fine gauze wavering in a strong breeze. The pulsations and waves of light were of unequal duration; some being rapid, while others lasted a longer time. For over one hour, the comet's tail kindled and extinguished more than one hundred times; the extinction being sometimes so complete that it was impossible to see any trace of the comet; while sometimes it became so bright that, in spite of the light of the moon, it could be distinguished easily in all its contours, even to its very extremity, which was then a little to the south of γ Ursa Minoris. ..." [11]

Scientific analysis

From May to July 1874, Huggins, Secchi, Lockyer, Rayet and Wolf made spectrographic observations of the comet. At first only a continuum was found, but by mid-June the three typical comet spectral bands were found. [12] According to Huggins, Comet Coggia was "the first bright comet which has appeared since the spectroscope has become an instrument of scientific research." [13]

Orbit

Using 638 observations of Comet Coggia made over a period of 185 days, Josef von Hepperger in 1882 calculated an elliptical orbit inclined about 66° to the ecliptic. [14] On 9 July 1874 the comet reached perihelion at about .6758 AU from the Sun. On 23 July the comet made its closest approach to planet Earth at about .29 AU. [15]

Comet of 1874 in literature

Gerard Manley Hopkins wrote on 13 July 1874 a journal entry concerning Coggia's comet. [16]

The public scare regarding the comet was satirized by Mark Twain in his short story "A Curious Pleasure Excursion." [17]

The comet was observed by members of the Custer 1874 expedition to the Black Hills of South Dakota. It was observed for 3 or 4 days by white and Native American members of the expedition ending July 2. Accounts of the observations were included in the diary of James Calhoun and in a newspaper article in the New York World. Lieutenant Calhoun was Custer's brother-in-law and acting adjutant on the expedition and later died at the Little Big Horn. [18]

Related Research Articles

<span class="mw-page-title-main">Great Comet of 1811</span> Astronomical object

The Great Comet of 1811, formally designated C/1811 F1, is a comet that was visible to the naked eye for around 260 days, the longest recorded period of visibility until the appearance of Comet Hale–Bopp in 1997. In October 1811, at its brightest, and when it was 1.2 AU from Earth, it displayed an apparent magnitude of 0, with an easily visible coma.

Jérôme Eugène Coggia was a 19th-century French astronomer and discoverer of asteroids and comets, who was born in the Corsican town of Ajaccio.

<span class="mw-page-title-main">Comet Donati</span> Long-Period Comet named after the Italian astronomer Giovanni Battista Donati

Comet Donati, or Donati's Comet, formally designated C/1858 L1 and 1858 VI, is a long-period comet named after the Italian astronomer Giovanni Battista Donati who first observed it on June 2, 1858. After the Great Comet of 1811, it was the most brilliant comet that appeared in the 19th century. It was also the first comet to be photographed.

<span class="mw-page-title-main">Great Comet of 1882</span> Astronomical object

The Great Comet of 1882 formally designated C/1882 R1, 1882 II, and 1882b, was a comet which became very bright in September 1882. It was a member of the Kreutz Sungrazers, a family of comets which pass within 1 R of the Sun's photosphere at perihelion. The comet was bright enough to be visible next to the Sun in the daytime sky at its perihelion. The comet made its closest approach to Earth on 16 September 1882 at 0.99 AU and then came to perihelion the next day on 17 September.

<span class="mw-page-title-main">C/1861 J1</span> Astronomical object

The Great Comet of 1861, formally designated C/1861 J1 and 1861 II, is a long-period comet that was visible to the naked eye for approximately 3 months. It was categorized as a great comet—one of the eight greatest comets of the 19th century.

The Comet of 1729, also known as C/1729 P1 or Comet Sarabat, was an assumed parabolic comet with an absolute magnitude of −3, the brightest ever observed for a comet; it is therefore considered to be potentially the largest comet ever seen. With an assumed eccentricity of 1, it is unknown if this comet will return in a hundred thousand years or be ejected from the Solar System.

<span class="mw-page-title-main">23P/Brorsen–Metcalf</span> Periodic comet with 70 year orbit

23P/Brorsen–Metcalf is a periodic comet with an orbital period of 70 years. It fits the classical definition of a Halley-type comet with. It was first discovered by Theodor Brorsen at the Altona Observatory on July 20, 1847, and again by Kaspar Schweizer (Moscow) on August 11, 1847. It was predicted that it would reappear between 1919 and 1922.

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. 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 around May 27, 2039 when it will be near a maximum near-perihelion distance from Earth.

<span class="mw-page-title-main">Great Comet of 1744</span> Non-periodic comet

The Great Comet of 1744, whose official designation is C/1743 X1, and which is also known as Comet de Chéseaux or Comet Klinkenberg-Chéseaux, was a spectacular comet that was observed during 1743 and 1744. It was discovered independently in late November 1743 by Jan de Munck, in the second week of December by Dirk Klinkenberg, and, four days later, by Jean-Philippe de Chéseaux. It became visible with the naked eye for several months in 1744 and displayed dramatic and unusual effects in the sky. Its absolute magnitude – or intrinsic brightness – of 0.5 was the sixth highest in recorded history. Its apparent magnitude may have reached as high as −7, leading it to be classified as a Great Comet. This comet is noted especially for developing a 'fan' of six tails after reaching its perihelion.

<span class="mw-page-title-main">C/2002 T7 (LINEAR)</span>

C/2002 T7 (LINEAR) is a non-periodic comet discovered in 2002 by LINEAR project. The comet brightened to a magnitude of 2.2.

X/1872 X1, occasionally referred to as "Pogson's Comet", was a probable cometary astronomical object seen from Madras on December 3 and 4, 1872, by astronomer N. R. Pogson.

<span class="mw-page-title-main">Great Southern Comet of 1887</span> Kreutz comet

The Great Southern Comet of 1887, or C/1887 B1 using its International Astronomical Union (IAU) designation, was a bright comet seen from the Southern Hemisphere during January 1887. Later calculations indicated it to be part of the Kreutz Sungrazing group. It came to perihelion on 11 January 1877 at a distance of 0.00483 AU (723 thousand km) with a velocity of 606.1 km/s. Since the Sun has a radius of 696000 km, the comet passed about 27000 km from the surface of the Sun.

<span class="mw-page-title-main">Great Comet of 1901</span>

The Great Comet of 1901, sometimes known as Comet Viscara, formally designated C/1901 G1, was a comet which became bright in the spring of 1901. Visible exclusively from the southern hemisphere, it was discovered on the morning of April 12, 1901 as a naked-eye object of second magnitude with a short tail. On the day of perihelion passage, the comet's head was reported as deep yellowish in color, trailing a 10-degree tail. It was last seen by the naked eye on May 23.

<span class="mw-page-title-main">C/2011 L4 (PanSTARRS)</span>

C/2011 L4 (PanSTARRS), also known as Comet PANSTARRS, is a non-periodic comet discovered in June 2011 that became visible to the naked eye when it was near perihelion in March 2013. It was discovered using the Pan-STARRS telescope located near the summit of Haleakalā, on the island of Maui in Hawaii. Comet C/2011 L4 probably took millions of years to come from the Oort cloud. After leaving the planetary region of the Solar System, the post-perihelion orbital period is estimated to be roughly 107000 years. Dust and gas production suggests the comet nucleus is roughly 1 kilometer (0.62 mi) in diameter, while based on the absolute nuclear magnitude and a geometric albedo of 0.04 the diameter of the nucleus is over 2.4 kilometers (1.5 mi). A method based on coma magnitude decay function estimated the effective radius at 2.317 ± 0.190 km.

<span class="mw-page-title-main">C/1807 R1</span> Long-period comet

C/1807 R1, also known as the Great Comet of 1807, is a long-period comet. It was visible to naked-eye observers in the northern hemisphere from early September 1807 to late December, and is ranked among the great comets due to its exceptional brightness.

<span class="mw-page-title-main">C/1769 P1</span>

C/1769 P1 (Messier) is a long-period comet that was visible to the naked eye at its last apparition in 1769. The comet is classified as a great comet due to its superlative brightness.

C/1865 B1 was a non-periodic comet, which in 1865 was so bright that it was visible to unaided-eye observations in the Southern Hemisphere. The comet could not be seen from the Northern Hemisphere.

<span class="mw-page-title-main">Great Comet of 1819</span> Comet discovered by German astronomer Johann Georg Tralles

The Great Comet of 1819, officially designated as C/1819 N1, also known as Comet Tralles, was an exceptionally bright and easily visible comet, approaching an apparent magnitude of 1–2, discovered July 1, 1819 by the German astronomer Johann Georg Tralles in Berlin. It was the first comet analyzed using polarimetry, by French mathematician François Arago.

<span class="mw-page-title-main">C/1963 A1 (Ikeya)</span> Comet

C/1963 A1 (Ikeya), also known as Comet 1963I and 1963a, is a long period comet discovered by Kaoru Ikeya on 2 January 1963. The comet last passed perihelion on 21 March 1963, when it reached an apparent magnitude of 2.8.

C/1989 W1 (Aarseth–Brewington) is a non-periodic comet discovered on 16 November 1989 independently by Knut Aarseth and Howard Brewington. It reached an apparent magnitude of 2.8.

References

  1. 1 2 3 4 5 Kronk, G. W. (2003). "J. von Heppeger's orbital calculation for C/1874 H1". Cometography: A Catalog of Comets. Vol. 2: 1800–1899. Cambridge University Press. p. 411. ISBN   0-521-58505-8.
  2. Donald K. Yeomans. "NASA JPL Solar System Dynamics: Great Comets in History".
  3. "Coggia's Comet". Haydn's Dictionary of Dates and Universal Information (17th ed.). NY: Harper and Brothers. 1884. p. 175. To the casual observer near London the comet became readily visible about July 4th.
  4. Bailey, Greg, ed. (2014). "The Voyage of the F. H. Moore" and Other 19th Century Whaling Accounts. McFarland. p. 60. ISBN   9780786478668. According to Samuel Grant Williams’s journal entry for July 10, 1874, “… About the 3d this month we began to see a beautiful comet in the southern sky. It has been visible every night since. We see it a little after sundown and about midnight it fades from sight. …” Williams’s whaling ship (under the command of Captain Soper) might have been near 24.22°N, 85.40°W.
  5. 1 2 Kronk, G. W. (2003). "C/1874 H1 (Coggia)". Cometography: A Catalog of Comets. Vol. 2: 1800–1899. Cambridge University Press. pp. 405–412. ISBN   0-521-58505-8.
  6. Seargent, David A. J. (2008). "C/1874 H1 (Coggia)". The greatest comets in history. Springer. p. 126. ISBN   9780387095134.
  7. Moore, P.; Rees, R. (2011). "Table 14.8 Selected list of brilliant comets, 1500–1900". Patrick Moore's Data Book of Astronomy. Cambridge: Cambridge University Press. p. 270. ISBN   978-0-521-89935-2.
  8. Hayter, Henry Heylyn (1875). "alleged sightings near Melbourne". Victorian Year Book for 1874. p. 226. "July 26.—Coggia's comet first seen in Victoria from Wilson's Promontory, Point Lonsdale, and the suburbs of Melbourne."
  9. A. Guillemin, trans. & ed. by J. Glaisher (1877). "comet observed by R. L. J. Ellery". The world of comets. London. p. 353.{{cite book}}: CS1 maint: location missing publisher (link)
  10. "The Comet". The Evening News, Sydney, New South Wales. 31 July 1874. p. 2.
  11. Trouvelot, L. (1878). "Undulations observed in the tail of Coggia's comet, 1874". Proceedings of the American Academy of Arts and Sciences. 13, May 1877 – May 1878 (86): 185–186. Bibcode:1878AmJS...15...84T. doi:10.2475/ajs.s3-15.86.84. S2CID   130981641.
  12. Grego, Peter (2013). Blazing a Ghostly Trail: ISON and Great Comets of the Past and Future. Springer. pp. 118–119. ISBN   978-3-319-01774-7.
  13. "Comet Coggia". The Astronomical Register (140): 183–193. August 1874.
  14. "NASA JPL Small-Body Database Browser: C/1874 H1".
  15. Vitagliano, A. "SOLEX 11.0". Archived from the original on 2008-12-20.
  16. David H. Levy: Poet and Observer: Gerard Manley Hopkins and some mid-19th Century Comets. In: Journal of the Royal Astronomical Society of Canada. Vol. 75, No. 3, 1981, pp. 139–150. (PDF; 974 kB).
  17. Mark Twain (2013). Delphi Complete Works of Mark Twain (Illustrated). Delphi Classics. p. 2604. ISBN   978-1-908909-12-1.
  18. Horstead, Paul (2009). Crossing the Plains with Custer. Golden Valley Press. pp. 29–33. ISBN   978-0-9718053-5-4.