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Oort cloud
(redirected from Ort cloud)

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Oort cloud: see comet comet [Gr.,=longhaired], a small celestial body consisting mostly of dust and gases that moves in an elongated elliptical or nearly parabolic orbit around the sun. Comets visible from the earth can be seen for periods ranging from a few days to several months.
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Oort cloud

Vast spherical cloud of small, icy bodies orbiting the Sun at distances ranging from about 0.3 light-year to one light-year or more that is probably the source of most long-period comets. In 1950 the Dutch astronomer Jan Hendrik Oort (1900–92) noted that no comets have orbits that would indicate an interstellar origin. He proposed that the Sun is surrounded by billions of these objects, which are only occasionally detectable when they enter the inner solar system. The Oort cloud is believed to be composed of primordial bodies dating from the formation of the solar system (see solar nebula). Whether the Oort cloud merges, in its inner region, into the disk-shaped Kuiper belt is not known.



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The orbit of the comet indicates that it is coming from the outermost edge of the solar system, the so-called Ort Cloud, which is about 100,000 times more distant from the sun than the Earth," said Donald Yeomans, a senior research scientist who oversees NASA's Near-Earth Object program office at the Jet Propulsion Laboratory in Pasadena, California.
Modern comet theory dates back to 1950, when two highly significant models -- the "dirty snowball" and the Ort cloud -- emerged to enliven the field.
 
 
 
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