Rocky objects from space that strike the Earth.
When meteorites pass through Earth’s atmosphere, they get
heated and their surfaces become ionized, causing them to
glow brightly and form a streak moving across the atmosphere
known as a shooting star or fireball.
At certain times of the year, the Earth passes through
parts of our solar system that are rich in meteorites, and the
night skies become filled with shooting stars and fireballs,
sometimes as frequently as several per minute. These times of
high-frequency meteorite encounters are known as meteor
showers and include the Perseid showers that appear around
August 11 and the Leonid showers that appear about November
14 (both occur annually).
There is ample evidence that many small meteorites have
hit the Earth frequently throughout time. Eyewitness
accounts describe many events, and fragments of meteorites
are regularly recovered from places like the Antarctic ice
sheets, where rocky objects on the surface have no place to
come from but space. Although meteorites may appear as
flaming objects moving across the night skies, they are generally
cold icy bodies when they land on Earth, and only their
outermost layers get heated from the deep freeze of space
during their short transit though the atmosphere.
Meteorites consist of several different main types. Stony
meteorites include chondrites, which are very primitive and
ancient meteorites made of silicate minerals, like those common
in the Earth’s crust and mantle, but chondrites contain
small spherical objects known as chondrules. These chondrules
contain frozen droplets of material that is thought to
be remnants of the early solar nebula from which the Earth
and other planets initially condensed. Achondrites are similar
to chondrites in mineralogy, except that they do not contain
the chondritic spheres. Iron meteorites are made of an ironnickel
alloy with textures that suggest they formed from slow
crystallization inside a large asteroid or small planet that has
since been broken into billions of small pieces, probably by
an impact with another object. Stony-irons are meteorites
that contain mixtures of stony and iron components and
probably formed near the core-mantle boundary of the broken
planet or asteroid. Almost all meteorites found on Earth
are stony varieties.














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