The
Great Comet of 1861 formally designated C/1861 J1 and
1861 II, is a
long-period comet that was visible to the
naked eye for approximately 3 months. It was categorized as a
Great Comet, one of eight in the 19th century.
It was discovered by
John Tebbutt of
Windsor, New South Wales,
Australia, on May 13, 1861, with an
apparent magnitude of +4, a month before
perihelion (June 11). It was not visible in the northern hemisphere until June 29, but it arrived before word of the comet's discovery.
The comet of 1861 interacted with the Earth in an almost unprecedented way. For two days, when the comet was at its closest (0.1326
AU), the Earth was actually within the comet's tail, and streams of cometary material converging towards the distant
nucleus could be seen. By day also the comet's gas and dust even obscured the Sun.
By the middle of August the comet was no longer visible to the naked eye, but it was visible in telescopes until May 1862. An elliptical orbit with a period of about 400 years was calculated, which would indicate a previous appearance about the middle of the 15th century, and a return in the 23rd century.
As of 1992 this Great Comet had traveled more than 100 AU from the Sun, making it even further away than
dwarf planet Eris. It will come to aphelion around 2063.
I. Hasegawa and
S. Nakano suggest that this comet is identical with
C/1500 H1.
Footnotes
External links
- on Cometography.com
- , Gallery of......
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