Great Comet of 1744
.jpg) The tails of C/1743 X1, the Great Comet of 1744, extending above the horizon before sunrise on March 8, 1744 | |
| Discovery | |
|---|---|
| Discovered by | Jan de Munck Dirk Klinkenberg Jean-Philippe de Chéseaux |
| Discovery date | 29 November 1743 |
| Designations | |
| Great Comet of 1743 | |
| Orbital characteristics[1] | |
| Observation arc | 71 days |
| Number of observations | 76 |
| Perihelion | 0.222 AU |
| Eccentricity | ~1.000 |
| Inclination | 47.142° |
| 49.297° | |
| Argument of periapsis | 151.486° |
| Last perihelion | 1 March 1744 |
| Physical characteristics[2] | |
| Comet total magnitude (M1) | 0.5 |
| –7.0 (1744 apparition) | |
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.[2] 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.
Discovery
[edit]The comet was discovered on November 29, 1743, by Jan de Munck at Middelburg,[3] and was independently sighted on December 9, 1743 by Klinkenberg at Haarlem, and by Chéseaux from the observatory at Lausanne on December 13. Chéseaux said it lacked a tail and resembled a nebulous star of the third magnitude; he measured the coma as five minutes across.[4]
The comet brightened steadily as it approached perihelion. By February 18, 1744, it reportedly was as bright as the planet Venus (with an apparent magnitude of −4.6) and at this time displayed a double tail.
Perihelion, "six tails"
[edit]The comet reached perihelion about March 1, 1744, when it was 0.2 astronomical units from the Sun.[1] At about this time it was bright enough to be observed in daylight with the naked eye.[5] As it moved away from perihelion, a spectacular tail developed — extending well above the horizon while the comet's head remained invisible due to the morning twilight. In early March 1744, Chéseaux and several other observers reported an extremely unusual phenomenon — a 'fan' of six separate tails rose above the horizon.[5]
An engraving illustration of "COMET-STERNS" (Comet-Stars) by astronomer & master engraver Johann Georg Puschner (1680–1749) of Comet Klinkenberg
The tail structure was a puzzle to astronomers for many years. Although other comets had displayed multiple tails on occasion, the 1744 comet was unique in having six. It has been suggested that the 'fan' of tails was generated by as many as three active sources on the cometary nucleus, exposed in turn to solar radiation as the nucleus rotated.[6] It also has been proposed that the tail phenomenon was a very prominent example of the "dust striae" seen in the tails of some comets, such as Comet West and C/2006 P1 (McNaught).
Other observations
[edit]Chéseaux, on March 9, was the last known observer in the northern hemisphere to see the comet, but it remained visible for observers in the southern hemisphere, some of whom reported a tail length of approximately 90 degrees on March 18.[6] The comet was not seen after April 22, 1744.
The comet also was noted in Japanese astronomical records in the Nihon Odai Ichiran of the Kanpō era.[7] Researchers have found in Chinese astronomical records that some Chinese observations describe audible sounds associated with the comet, which may, if true, have resulted from the interaction of particles with the Earth's magnetosphere, as sometimes described for the aurora.[8]
Among those who saw the comet was the thirteen-year-old Charles Messier, on whom it had a profound and inspirational effect. He went on to become one of the founding figures of modern astronomy, and later discovered many comets during his observations.
Catherine the Great, then Sophia, also observed the brilliant comet as a young girl as she was travelling to Russia to be wed.[9]
References
[edit]- ^ a b "JPL Small-Body Database Browser: C/1743 X1" (1744-03-01 last obs used (2-body dynamics used in orbit determination)). Jet Propulsion Laboratory. Retrieved 2011-07-18.
- ^ a b M. Kidger (3 April 1997). "Comet Hale-Bopp Light Curve". jpl.nasa.gov. NASA / JPL. Archived from the original on 7 April 2023. Retrieved 17 November 2008.
- ^ De Munck, J., Sterrekundige Waarneemingen op de Comeet of Staart-Sterre; Sedert den 29 November des Jaars 1743. tot op den 1 Maart van den Jaare 1744, Amsterdam/Middelburg: Isaak Tirion/Hendrik van Hoekke, 1744.
- ^ Kronk, G. W. Cometography: A Catalog of Comets, I, Cambridge: Cambridge University Press, 1999, p. 408.
- ^ a b Kronk, p.410
- ^ a b Kronk, p.411
- ^ Titsingh, Isaac. (1834). Nihon Odai Ichiran; or, Annales des empereurs du Japon. Paris: Royal Asiatic Society, Oriental Translation Fund of Great Britain and Ireland, p. 418. OCLC 5850691.
- ^ Keay, C. Explanation of Auroral Sounds Archived 2015-09-24 at the Wayback Machine, Australian Space Weather Agency, accessed 17-11-08
- ^ Robert K. Massie (2012). Catherine the Great: Portrait of a Woman. Random House Trade Paperbacks. ISBN 978-0-345-40877-8.
External links
[edit]- Orbit Diagram, C/1743 X1 NASA Jet Propulsion Laboratory
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