Comets: Ice, Dust and Long Tails

Frozen travelers from the outer Solar System that grow glowing tails when the Sun warms them.

A comet is a small body of ice, dust and rock. For most of its orbit it is a dark, quiet nucleus, often only a few kilometers across. When it moves closer to the Sun, ice turns to gas and sets dust free. That forms a cloud called the coma and, often, two tails. One tail is made of electrically charged gas and points straight away from the Sun. The other is made of dust and curves gently along the orbit. Both point away from the Sun, not behind the comet, whichever way it is traveling.

Comets come from two cold reservoirs. Short-period comets, which return within about 200 years, mostly come from the Kuiper Belt beyond Neptune. Long-period comets arrive from the Oort Cloud, a far larger and much more distant shell that no spacecraft has seen directly. Halley's Comet is the best-known periodic visitor. It returns about every 76 years, and its next visit is expected in 2061.

The guides in this category explain how comets are built, why tails behave as they do, how comets differ from asteroids and which ones have earned the name great comet. They also cover Rosetta, the European Space Agency mission that orbited Comet 67P and put a lander on its surface.

A practical guide explains how to see a comet with your eyes or binoculars. One rule comes first and applies everywhere on this site: never point binoculars or a telescope at the Sun without a solar filter made for that purpose. Comets that pass very close to the Sun are best left to spacecraft.

Not sure where to begin? Read what a comet is, then how comet tails work.

The nine guides

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