Asteroids, Meteors, and
Meteorites
A million
asteroids populate the zone between
Mars and Jupiter known as the Asteroid Belt. Asteroids are
essentially chunks of rock but they range in size from dust particles
to 1,000 km across. Darker asteroids are probably made of carbon
materials and the brighter ones may contain such metals as iron and
nickel. Astronomers know of some 2,200 asteroids. The largest of
these are Ceres (about the width of France), Pallas, Vesta, and
Juno.
Shown here: the asteroid 243 Ida and its moon Dactyl (the
small dot on it's right)
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We find out about the
composition of asteroids by analyzing meteorites, which are essentially
asteroids that have fallen out of orbit and survived the fiery
passage through Earth's atmosphere. There are about 2,500 meteorites
known. the largest is in Namibia, Africa and weighs 53.5 metric tons.
The second largest, which landed in Greenland, weighs 53.5 metric
tons and is on display at the Hayden Planetarium in New York City.
An example of a meteorite
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When these chunks of
rock are still in space they are called meteoroids. they strike the Earth's
atmosphere at speeds up to 40 km/second. At a height of about 128 km,
friction with the atmosphere surrounds the object with hot, glowing
air. This fireball streaks toward Earth, becoming visible as a bright
meteor. If it does not break up, the
meteoroid will strike the surface and become a meteorite.
Meteors from much
smaller particles, about as large as grains of sand, can be seen
almost any dark night. the best chance of seeing meteors occurs
during meteor showers, when Earth passes through streams of dust left
behind by comets.