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Comet Donati

Non-periodic comet

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Through Comet, Italy and Earth

Discovery and observations

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" of Leo. By mid-August it had brightened sufficiently to be visible to the naked eye.

In September it passed into Ursa Major. For much of its apparition it occupied a unique position (among great comets) in the sky and was particularly well placed for Northern Hemisphere viewers.

It was nearest the Earth 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. The final observation was by William Mann, chief assistant at the Royal Observatory, Cape of Good Hope, who detected it as a faint nebulosity on March 4, 1859.

During its apparition the comet was particularly closely studied by the astronomer George Phillips Bond and his father William 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 the Royal Astronomical Society, being the first American to receive the award.

Comet photographed

Donati's Comet was successfully photographed on September 27 by W. Usherwood, a portrait photographer at Walton-on-the-Hill, Surrey, using a 7-second exposure with an f/2.4 portrait lens, the first time a comet had been photographed. Usherwood's photograph, which is in archival storage at Harvard College Observatory’s Astronomical Photographic Glass Plate Collection at the Center for Astrophysics, 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 at Harvard 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".

Orbital calculations

Orbits for the comet were calculated by Friedrich Emil von Asten and George William Hill, the latter's based on nearly 1000 positions. The comet had an orbital inclination of 116.9°. With an epoch 2200 barycentric orbital period approximated at 1739 years, it is estimated that Donati's Comet will not be seen passing by Earth again until somewhere around the year 3600. As of 2023, 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).

The comet's orbit lies very close to that of Venus, 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 strong meteor shower at the northern hemisphere.

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