Great Comet of 1843

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C/1843 D1
Great Comet of 1843 (cropped).jpg
A painting of the sungrazing Great Comet of 1843, as seen from Tasmania, by Mary Morton Allport
Discovery
Discovery dateFebruary 5, 1843
Alternative
designations		Great Comet of 1843, Great March Comet, 1843 I, 1843 D1
Orbital characteristics A
Epoch2394259.411
Aphelion156 AU
Perihelion.005460 AU
Semi-major axis78 AU
Eccentricity0.99993
Orbital period742? yr[1]
Inclination144.4°
Last perihelionFebruary 27, 1843
Next perihelionunknown

The Great Comet of 1843, formally designated C/1843 D1 and 1843 I, was a long-period comet which became very bright in March 1843 (it is also known as the Great March Comet). It was discovered on February 5, 1843 and rapidly brightened to become a great comet. It was a member of the Kreutz Sungrazers, a family of comets resulting from the breakup of a parent comet (X/1106 C1) into multiple fragments in about 1106. These comets pass extremely close to the surface of the Sun—within a few solar radii—and often become very bright as a result.

Perihelion[]

First observed in early February, 1843, it raced toward an incredibly close perihelion of less than 830,000 km on February 27, 1843; at this time it was observed in broad daylight roughly a degree away from the Sun.[2] It passed closest to Earth on March 6, 1843, and was at its greatest brilliance the following day; unfortunately for observers north of the equator, at its peak it was best visible from the Southern Hemisphere.[3] It was last observed on April 19, 1843. At that time this comet had passed closer to the Sun than any other known object.

Tail[]

Charles Piazzi Smyth: The Great Comet of 1843

The Great Comet of 1843 developed an extremely long tail during and after its perihelion passage. At over two astronomical units in length, it was the longest known cometary tail until measurements in 1996 showed that Comet Hyakutake's tail was almost twice as long. There is a painting in the National Maritime Museum that was created by astronomer Charles Piazzi Smyth. The purpose of the painting is to show the overall brightness and size of the tail of the comet.

Orbit[]

Estimates for the orbital period of the comet have varied from 512 ± 105 years (Kreutz's classical work from 1901),[1] 654 ± 103 years (Chodas2008 unforced solution),[1] 688 years (JPL Horizons barycentric epoch 1852 solution), and 742 years (Chodas2008 forced solution based on a presumed identity with X/1106 C1).[1] But the comet was only observed over a period of 45 days from March 5 to April 19, and the uncertainties mean it likely has an orbital period of 600 to 800 years.[1]

Musical depiction[]

The Mexican composer composed a waltz for piano, El cometa de 1843. It appeared as no. 13 in Instructor filarmónico, periódico semanario musical, Tomo primero (Mexico, 1843)

See also[]

  • Charles Piazzi Smyth

References[]

  1. ^ a b c d e Sekanina, Zdenek; Chodas, Paul W. (2008). "A New Orbit Determination for Bright Sungrazing Comet of 1843". the Astrophysical Journal. 687 (2): 1415–1422. Bibcode:2008ApJ...687.1415S. doi:10.1086/592081.
  2. ^ Donald K. Yeomans (April 2007). "Great Comets in History". Jet Propulsion Laboratory/California Institute of Technology (Solar System Dynamics). Retrieved 2011-02-02.
  3. ^ "Great Comets in History". Archived from the original on 2004-08-22. Retrieved 2006-02-07.

External links[]

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