| |
| Discovery | |
|---|---|
| Discovery date | February 5, 1843 |
| Designations | |
| Great Comet of 1843, Great March Comet, 1843 I, 1843 D1 | |
| Orbital characteristics | |
| Observation arc | 45 days |
| Number of observations | 200 |
| Orbit type | Kreutz sungrazer |
| Aphelion | 156 AU[1] |
| Perihelion | 0.00553 AU (827 thousand km) |
| Semi-major axis | 78 AU[1] |
| Eccentricity | 0.99993[1] |
| Orbital period | 600–800? yr[2] |
| Max. orbital speed | 566.6 km/s[3] |
| Inclination | 144.4° |
| Last perihelion | February 27, 1843 |
| Next perihelion | unknown |
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.
First observed in early February, 1843, it raced toward an incredibly close perihelion of about 827,000 km (~131,000 km from the surface of the Sun) on February 27, 1843; at this time it was observed in broad daylight roughly a degree away from the Sun.[4] It passed closest to Earth on March 6, 1843, at a distance of 0.84 AU,[4] 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.[5] It was last observed on April 19, 1843. At that time this comet had passed closer to the Sun than any other known object.
| Perihelion (Sun approach) |
Earth distance (AU) |
Sun centerpoint distance (AU) |
Velocity relative to Earth (km/s) |
Velocity relative to Sun (km/s) |
Solar elongation |
|---|---|---|---|---|---|
| 27 February 1843 ≈21:59 | 0.993 AU (148.6 million km; 92.3 million mi; 386 LD) | 0.00553 AU (827 thousand km; 514 thousand mi; 2.15 LD) | 552.4 | 566.6 | 0.29° |
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 with the purpose of showing the overall brightness and size of the tail of the comet.
Estimates for the orbital period of the comet have varied from 512 ± 105 years (Kreutz's classical work from 1901),[2] 654 ± 103 years (Chodas2008 unforced solution),[2] 687 years (JPL Horizons barycentric epoch 1900 solution),[1] and 742 years (Chodas2008 forced solution based on a presumed identity with X/1106 C1).[2] 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.[2]
The Mexican composer Luis Baca composed a waltz for piano, El cometa de 1843. It appeared as no. 13 in Instructor filarmónico, periódico semanario musical, Tomo primero (Mexico, 1843)
