Comet Hale Bopp taken by Auvo Korpi from Huhtamo, Finland |
Comet 1P/Halley as taken March 8, 1986 by W. Liller, Easter Island, part of the International Halley Watch (IHW) Large Scale Phenomena Network. |
The white tail above is the dust tail and the blue tail is the ion table. The dust tail is composed of slightly heavier particles, so this tail bends just a bit, whereas the ion tail points directly away from the Sun. Thus even when the comet is moving away from the Sun, the tails point away, leading the comet. The tail is not always trailing the nucleus of the comet.
Comets orbit the Sun repeatedly, although each passing of the Sun results in a bit of mass loss. Eventually a comet, after a few thousand years and several orbits of the Sun, will break apart. Some comets come from the Kuiper Belt, out near Neptune and Pluto's orbit. These are called short period comets. A famous short period comet is Halley's comet, with an orbital period of 76 years. Long period comets come from the Oort cloud, and several tens of thousands of astronomical units from the Sun. These comets have orbital periods of several hundred to possibly several tens of thousands of years.
Most comets require a telescope to observe, but occasionally comets are visible to the naked eye. The last really good naked eye comet I remember was Comet McNaught, which flew by Earth in 2007. I took my astronomy class out a couple of times to view this comet. Comet McNaught has an orbital period estimated to be about 93,000 years, so I won't be seeing that one again. LOL!
Comets are beautiful objects in the sky, so if you ever have a chance to view one, definitely take advantage.
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