 Donati's Comet, Oxford, 7:30 p.m., 5 Oct. 1858 byWilliam Turner | |
| Discovery | |
|---|---|
| Discovered by | Giovanni Battista Donati |
| Discovery date | 1858 |
| Designations | |
| 1858 VI | |
| Orbital characteristics[1][2] | |
| Epoch | 8 October 1858 (JD 2399960.5) |
| Observation arc | 270 days |
| Number of observations | 1,000 |
| Aphelion | ~289AU |
| Perihelion | 0.578 AU |
| Semi-major axis | ~145 AU |
| Eccentricity | 0.996295 |
| Orbital period | ~1,739yr (outbound) |
| Inclination | 116.951° |
| 167.304° | |
| Argument of periapsis | 129.144° |
| Last perihelion | 30 September 1858 |
| Next perihelion | ≈3600 |
| TJupiter | –0.394 |
| Physical characteristics[3][5] | |
Mean radius | 2.96 km (1.84 mi)[a] |
| 4.6 hours | |
| Comet total magnitude (M1) | 3.3 |
| 0.0–1.0 (1858 apparition)[4] | |
Comet Donati, orDonati's Comet,formally designatedC/1858 L1 and1858 VI, is along-periodcomet named after theItalianastronomerGiovanni Battista Donati who first observed it on June 2, 1858. After theGreat Comet of 1811, it was the most brilliant comet that appeared in the 19th century. It was also the first comet to be photographed.
Donati first observed the comet on 2 June from the Florence Observatory: it was initially visible as a small nebula-like object of magnitude 7 near the "head" ofLeo.[6] By mid-August it had brightened sufficiently to be visible to the naked eye.[7]
In September it passed intoUrsa Major. For much of its apparition it occupied a unique position (among great comets) in the sky[7] and was particularly well placed for Northern Hemisphere viewers.[6]
It was nearest theEarth on October 10, 1858, and for much of October was a brilliant object with a long,scimitar-like dust tail and prominent gas tail. It remained a naked-eye object until November for Southern Hemisphere observers.[7] The final observation was by William Mann, chief assistant at theRoyal Observatory, Cape of Good Hope, who detected it as a faint nebulosity on March 4, 1859.[8]
During its apparition the comet was particularly closely studied by the astronomerGeorge Phillips Bond and his fatherWilliam Cranch Bond. G. P. Bond incorporated these observations and those of many other astronomers into a monograph,An Account of the Great Comet of 1858, which remains his most important scientific work and for which he was awarded the Gold Medal of theRoyal Astronomical Society, being the first American to receive the award.[9]
Donati's Comet was successfully photographed on September 27 by W. Usherwood, a portrait photographer atWalton-on-the-Hill, Surrey, using a 7-second exposure with anf/2.4 portrait lens, the first time a comet had been photographed.[10] Usherwood's photograph, which has not survived, showed the bright region around the comet's nucleus and a part of the tail. G. P. Bond also successfully photographed the comet on September 28 atHarvard College Observatory, the first comet photograph through a telescope. He made several attempts with increasing exposure times, finally achieving a discernible image. He later wrote, "only the nucleus and a little nebulosity 15" in diameter acted on the plate in an exposure of six minutes".[11]
| Epoch 1600 | Epoch 2200 | |
|---|---|---|
| Orbital period | 1966 yr | 1739 yr |
| Orbital eccentricity | 0.9963 | 0.9960 |
| Aphelion | 313AU | 289 AU |
Orbits for the comet were calculated by Friedrich Emil von Asten andGeorge William Hill, the latter's based on nearly 1000 positions.[12] The comet had anorbital inclination of 116.9°.[2] With an epoch 2200 barycentric orbital period approximated at 1739 years,[1] it is estimated that Donati's Comet will not be seen passing by Earth again untilsomewhere around the year 3600. As of 2023[update],JPL Horizons estimates that the comet is 147 AU (22 billion km) from the Sun and continuing to move away from the Sun at 2.4 km/s (5,400 mph).[13]
The comet's orbit lies very close to that ofVenus, with the minimum intersection distance being 0.0047 astronomical units (700,000 km; 440,000 mi), which is smallest known distance a great comet can approach a terrestrial planet. It is possible the comet produces a strongmeteor shower at the northern hemisphere.[14]
Donati's Comet is considered to be one of the most beautiful comets observed,[15] and was one of the brightest of the century, making a strong impression both on artists and the general public. After a prior period of hysteria on the subject of comets, especially inParis (caused partly by incorrect calculations byJohn Russell Hind which suggested that one would strike the Earth in June 1857) Donati's Comet went on to be the most-observed of the century due to its excellent visibility in dark skies for Northern Hemisphere viewers, particularly in Europe, and fine weather in September and October.[16]William Henry Smyth, an English astronomer, recalled it as "one of the most beautiful objects that I have ever seen".[16] Donati himself, a relatively obscure figure, was propelled to the status of an astronomical hero, and the comet helped cultivate a general enthusiasm for astronomy among the public.[17]
Donati's Comet appears as a streak and star in the early evening sky of a painting byWilliam Dyce,Pegwell Bay, Kent – a Recollection of October 5th 1858.[18] It was featured in a number of sketches and at least one painting byWilliam Turner of Oxford, and in a painting, "The Comet of 1858, as seen from the Heights of Dartmoor", bySamuel Palmer.The Comet at Yell'ham, a 1902 poem byThomas Hardy, was inspired by his recollections of Donati's Comet.[19]
Abraham Lincoln, then a candidate for a seat in theU.S. Senate, sat up on the porch of his hotel inJonesboro, Illinois, to see "Donti's Comet" on September 14, 1858, the night before the third of hishistoric debates withStephen Douglas.[20]
In his journals of the Malay Archipelago, naturalistAlfred Russel Wallace writes of seeing the comet in October 1858 off the island ofTidore in Indonesia. "I observed what seemed a fire of remarkable whiteness on the very summit of the hill ... the magnificent comet which was at the same time, astonishing all Europe. The nucleus presented to the naked eye a distinct disc of brilliant white light, from which the tail rose at an angle of about 30° or 35° with the horizon, curving slightly downwards, and terminating in a broad brush of faint light, the curvature of which diminished till it was nearly straight at the end. The portion of the tail next the comet appeared three or four times as bright as the most luminous portion of the milky way, and what struck me as a singular feature was that its upper margin, from the nucleus to very near the extremity, was clearly and almost sharply defined, while the lower side gradually shaded off into obscurity."[21]
The influence of the comet, particularly in visual and design terms, was such that traces of its appearance can be found in magazine and commercial illustrations, household objects, children's books and other items up until the early years of the 20th century.[17]
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