
Main Menu > The Solar System > Discovering Meteorites > Where Do We Find Meteorites?


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Meteorites fall everywhere on Earth.
Most plunge into the oceans that cover three-quarters of the
surface and are lost. Even those that fall on land can be
difficult to recognize unless you see them hit the ground.
The best places to look for meteorites have few Earth rocks
and little or no vegetation to camouflage them. That's why
glaciers, deserts, and rock-free plains are prime meteorite
hunting grounds.
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More meteorites have been discovered in Antarctica than anywhere
else on Earth. Not only are meteorites relatively easy to
recognize against the ice, but the moving glacial ice actually
concentrates the rocks in a few, small areas. As a bonus,
the Antarctic deep freeze helps protect meteorites from the
effects of weathering for thousands of years.
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The first Antarctic meteorites were found by Japanese scientists
in 1969. Beginning in the 1970s, the United States and Japan
each sponsored numerous expeditions to the continent and brought
back thousands of meteorites.
The United States's Antarctic Search for Meteorites program
falls under the joint sponsorship of the National Science
Foundation, the National Aeronautics and Space Administration,
and the Smithsonian Institution.
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How are the meteorites concentrated? Over time, many meteorites
land on a glacier and are buried by accumulating snow and
ice. Like a slow-moving river, the glacier transports the
meteorites until hills or mountains cause the flowing ice
to buckle or flow up and over the obstacle. Wind erodes the
uplifted ice and strands the cargo of meteorites on the surface.
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