A meteorite is an asteroid that is pulled into the Earth's atmosphere.
Meteorites help us understand the composition of asteroids because meteorites are small asteroids.
Most meteorites come from asteroids, which are rocky bodies orbiting the sun. Some meteorites could also come from comets, which are icy bodies. Both asteroids and comets can collide with Earth, resulting in meteorites.
Asteroids are objects smaller then planets that orbit the Sun. Meteorites are (usually) smaller objects that enter the atmosphere and reach the ground.
Asteroids and Meteorites
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Rock debree from other galaxy's
They are all very hot.
Stone meteorites are formed from the solidification of molten rock within asteroids. Iron meteorites are likely remnants of the metallic cores of differentiated asteroids. Carbonaceous chondrite asteroids are primitive bodies that have preserved materials from the early solar system due to minimal heating and alteration processes.
Meteorites were originally asteroids or fragments of other celestial bodies that were orbiting in space. When they collided with other objects or were influenced by gravitational forces, they were knocked out of their orbit and eventually fell to Earth's surface as meteorites.
Iron meteorites originate from the cores of asteroids that broke apart due to collisions in space. These fragments eventually make their way to Earth as meteorites.
Meteorites can from asteroids that landed on Earth's surface. They were originally chipped off larger planetary bodies by bolide impact.
asteroids comets meteoroids meteor meteorites