Comet Halley
Comet Halley, officially designated 1P/Halley, more generally known as Halley's Comet after Edmond Halley, is the best-known and the brightest of the "short-period" comets from the Kuiper belt that visit the inner solar system in years or decades-long orbits rather than the millennial periods of comets from the Oort cloud.
Composition
The nucleus of Halley's comet is potato-shaped with dimensions around
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8 by 8 by 16 kilometers. The density of the nucleus is between
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one tenth and one quarter times the density of water. The nucleus is very
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dark, reflecting only around 4% of incident light.
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http://www.astronomynotes.com/solfluf/s7.htm
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The Giotto space probe found the comet's surface to be rich in carbon. Of the volume of material ejected by Halley, 80% was water, 10% carbon monoxide, and 2.5% a mix of methane and ammonia. Other hydrocarbons, iron, and sodium were detected in trace amounts.
Related Topics:
Giotto space probe - Carbon - Water - Carbon monoxide - Methane - Ammonia - Hydrocarbons - Iron - Sodium
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Cyanogen gas is present in trace amounts.
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Material from the comet is responsible for two meteor showers each year, the Eta Aquarids in May and the Orionids in October.
Related Topics:
Meteor showers - Eta Aquarids - Orionids
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~ Table of Content ~
| ► | Introduction |
| ► | Composition |
| ► | Early history |
| ► | Recent history |
| ► | Dates of perihelia |
| ► | Trivia |
| ► | Halley's Comet in fiction |
| ► | External links |
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