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Kuiper belt

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Kuiper belt

Ring of small, icy bodies orbiting the Sun beyond the outermost planet. The Kuiper belt, named after Dutch-born US astronomer Gerard Kuiper, who proposed its existence in 1951, is thought to be the source of comets that orbit the Sun with periods of less than 200 years. The first member of the Kuiper belt was seen in 1992. In 1995 the first comet-sized objects were discovered; previously the only objects found had diameters of at least 100 km/62 mi (comets generally have diameters of less than 10 km/6.2 mi). An object named Xena, discovered in 2003, is larger than the dwarf planet Pluto.



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? Mentioned in ? References in periodicals archive
 
Agnor's theory builds on recent studies showing that about 10 percent of Kuiper belt bodies, including Pluto, have satellites.
Most previously observed disks have been cool and lie much farther from their parent stars, in the region that corresponds in the solar system to the locale of Pluto and the reservoir of comets known as the Kuiper belt.
The craft will explore Pluto and its large moon, Charon, and, continuing on a trajectory away from the sun, will probe additional icy and rocky bodies of the Kuiper Belt as part of a possible extended mission.
 
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