Great Comet of 1811
Great Comet of 1811
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Great Comet of 1811

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Great Comet of 1811

The Great Comet of 1811, formally designated C/1811 F1, is a comet that was visible to the naked eye for around 260 days, the longest recorded period of visibility until the appearance of Comet Hale–Bopp in 1997. In October 1811, at its brightest, and when it was 1.2 AU from Earth, it displayed an apparent magnitude of 0, with an easily-visible coma.

The comet was discovered on March 25, 1811, by Honoré Flaugergues at 2.7 AU from the Sun in the now-defunct constellation of Argo Navis. After being obscured for several days by moonlight, it was also found by Jean-Louis Pons on April 11, while Franz Xaver, Baron Von Zach was able to confirm Flaugergues' discovery the same night.

The first provisional orbit was computed in June by Johann Karl Burckhardt. Based on those calculations, Heinrich Wilhelm Matthäus Olbers predicted that the comet would go on to become extremely bright later that year.

From May to August, the comet's position made it difficult to spot because of its low altitude and the evening twilight. Both Flaugergues and Olbers were able to recover it in Leo Minor during August, Olbers noting a small but distinct tail, consisting of two rays forming a parabola, when viewing through a comet seeker. In August, the comet was first sighted in the United Kingdom by James Veitch of Inchbonny. By September, in Ursa Major, it was becoming a conspicuous object in the evening sky as it approached perihelion: William Herschel noted that a tail 25° long had developed by October 6.

By January 1812, the comet's brightness had faded. Several astronomers continued to obtain telescopic observations for some months, the last being Vincent Wisniewski at Novocherkassk, who noted it as barely reaching an apparent magnitude of 11 by August 12.

The Great Comet of 1811 was thought to have had an exceptionally large coma, perhaps reaching over 1 million miles across, 50% larger than the Sun. The comet's nucleus was later estimated at 30–40 km in diameter. In many ways, the comet was quite similar to Comet Hale–Bopp; it became spectacular without passing particularly close to either the Earth or the Sun but had an extremely large and active nucleus.

Astronomers also found the comet a memorable sight. William Henry Smyth, comparing his recollections of the Great Comet of 1811 to the spectacular Donati's Comet, stated that "as a mere sight-object, the branched tail was of greater interest, the nucleus with its 'head-veil' was more distinct, and its circumpolarity was a fortunate incident for gazers".

The comet was apparently visible during the New Madrid earthquakes in December 1811. A report on the first steamship to descend the Ohio River as it approached the confluence with the Mississippi River states, "December 18, 1811.—The anniversary of this day the people of Cairo [Illinois] and its vicinity should never forget. It was the coming of the first steamboat to where Cairo now is—the New Orleans, Capt. Roosevelt, Commanding. It was the severest day of the great throes of the New Madrid earthquake; at the same time, a fiery comet was rushing athwart the horizon".

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