Great Comet of 1843
Kreutz sungrazer comet that appeared in 1843
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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, specifically the Population I subgroup that originated from the breakup of a large parent comet in February 1106.[5] These comets pass extremely close to the surface of the Sunâwithin a few solar radiiâand often become very bright as a result.
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A painting of the Great Comet of 1843, as seen from Tasmania, by Mary Morton Allport | |
| Discovery | |
|---|---|
| Discovery date | 5 February 1843 |
| Designations | |
| 1843 I | |
| Orbital characteristics[1][2] | |
| Epoch | 27 February 1843 (JD 2394259.411) |
| Observation arc | 45 days |
| Number of observations | 200 |
| Orbit type | Kreutz sungrazer (Population I) |
| Aphelion | ~156 AU |
| Perihelion | 0.00553 AU (1.19 Râ)[3][a] |
| Semi-major axis | ~78 AU |
| Eccentricity | 0.99993 |
| Orbital period | ~600â800 years[4] |
| Max. orbital speed | 566.6 km/s[3] |
| Inclination | 144.36° |
| 3.527° | |
| Argument of periapsis | 82.639° |
| Last perihelion | 27 February 1843[3] |
| TJupiter | 0.006 |
| Physical characteristics | |
Mean radius | 24.75 km (15.38 mi)[5] |
| Mass | 7.30Ã1017 kg[6] |
| Comet total magnitude (M1) | 4.9[7] |
Perihelion
First observed in early February, 1843, it raced toward an incredibly close perihelion of about 827,000 km (~132,000 km from the surface of the Sun) on February 27, 1843;[a] at this time it was observed in broad daylight roughly a degree away from the Sun.[8] It passed closest to Earth on March 6, 1843, at a distance of 0.84 AU,[8] 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.[9] 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 â21:59 | 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° |
Physical characteristics
Nucleus size
Estimates in 2022 based on reconstructions of the origin of Kreutz sungrazers revealed that the nucleus of the Great Comet of 1843 possibly was about 24.75 km (15.38 mi) in effective radius, with a mass of approximately 7.30Ã1017 kg before it disintegrated upon perihelion.[5][6]
Tail
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.
Orbit
Estimates for the orbital period of the comet have varied from 512±105 years (Kreutz's classical work from 1901),[10] 654±103 years,[4] 687 years,[1] and 742 years.[4] 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.[4]
Recent studies in 2022 and 2025 further solidified the link between the comets of 1106 and 1843 after their orbits were traced back to the comet witnessed by Ammianus Marcellinus in 363 AD.[11][12]
Musical depiction
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).[citation needed]
See also
Notes
- The comet passed about 0.00553 AU (1.19 Râ) from the center of the Sun[3] which is (0.19 solar radii * 695700 km) = 132,000 km (82,000 mi) from the surface of the Sun.
