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Comets
People have observed comets
orbiting the sun for centuries. Comets are composed of antimatter that enters our solar system.
The comet's nucleus range from less than 100 meters to ten kilometer in
diameter. The solar
wind and dust
blast antimatter off the comet's surface creates the plasma coma and tails. Comets
produce light from the matter and antimatter annihilations on the comet's
surface, coma and tails as shown in the pictures
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Picture of Comet Hale-Bopp
showing a blue plasma tail, by Peter Barvoets, April 1, 1997
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As a comet gets closer to the sun, their coma and tails get
bigger because more solar wind and dust particles are blasting antimatter off
the comet's nucleus. The coma can be from 1,000 to 100,000 kilometers in
diameter; and tails can grow to between a million to 100 million kilometers long
(distance from earth to sun). The comet's tails points away from the sun
and curves with the solar wind. There are over 150 periodic
comets.
The antimatter is a million times less than scientists had
estimated.
The dusty-ice comet model was dispelled when spacecraft took pictures of Halley's
Comet. The
nucleus
was blacker than coal except for where matter and antimatter
annihilations were producing light and other radiation. After analyzing Borrelly's
Comet, the nucleus was found to contain no trace of water. The water
comes from the solar
wind and dust.
During the last
century, Shoemaker-Levy
9 comet broke into 21 fragments that collided with Jupiter and produced
explosions
equivalent to over 200 million Megatons of TNT. In 1908, a fragment from
Encke's comet hit the earth's atmosphere in Russian
Siberia and exploded of over 30 Megatons
of TNT. On July 23, 2002, a team of
researchers used NASA's Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI)
spacecraft to take pictures of a solar flares from a
sungrazer comet that collided with the sun.
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