Only in the late 18th century did scientist begin to recognize that meteorites were extraterrestrial matter. Some come from the Moon and others from Mars. When a huge meteorite carves a big crater, especially if hitting the surface with a low angle, little rock fragments can escape the gravity field of the parent body. They orbit the Sun during millenia, and if some are finally intercepted by the Earths' orbit, they fall as meteorites. Today we know that most meteorites are remnants of the formation of the solar system 4.6 billion years ago. A lot are fragments produced when asteroids collide.
The smallests burn and disintegrate when enter the Earth's atmosphere, but some are big enough to resist air friction and aerodinamic pressure, crashing and sometimes producing a crater. Meteor showers happen when our planet crosses the trail of a comet, often densely populated with little fragments of rock, most the size of sand grains or smaller.
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Meteorites are classified as follows:
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