A meteor is a bright streak of light that appears briefly in the sky.
Observers often call meteors shooting stars or falling stars because
they look like stars falling from the sky. People sometimes call the
brightest meteors fireballs. A meteor appears when a particle or chunk
of metallic or stony matter called a meteoroid enters the earth's
atmosphere from outer space. Air friction heats the meteoroid so that it
glows and creates a shining trail of gases and melted meteoroid
particles. The gases include vaporized meteoroid material and
atmospheric gases that heat up when the meteoroid passes through the
atmosphere. Most meteors glow for about a second.
Most meteoroids disintegrate before reaching the earth. But some
leave a trail that lasts several minutes. Meteoroids that reach the
earth are called meteorites.
Millions of meteors occur in the earth's atmosphere every day.
Most meteoroids that cause meteors are about the size of a pebble. They
become visible between about 40 and 75 miles (65 and 120 kilometers)
above the earth. They disintegrate at altitudes of 30 to 60 miles (50 to
95 kilometers).
Meteoroids travel around the sun in a variety of orbits and at
various velocities. The fastest ones move at about 26 miles per second
(42 kilometers per second). The earth travels at about 18 miles per
second (29 kilometers per second). Thus, when meteoroids meet the
earth's atmosphere head-on, the combined speed may reach about 44 miles
per second (71 kilometers per second).
Meteor showers
The earth meets a number of streams (trails) or swarms (clusters)
of tiny meteoroids at certain times every year. At such times, the sky
seems filled with a shower of sparks. Streams and swarms have orbits
like those of comets and are believed to be fragments of comets.
The most brilliant meteor shower known took place on Nov. 12-13,
1833. It was one of the Leonid showers, which occur every November and
seem to come from the direction of the constellation Leo.
Meteorites
There are three kinds of meteorites, stony, iron, and stony-iron.
Stony meteorites consist of minerals rich in silicon and oxygen, with
smaller amounts of iron, magnesium, and other elements. One group of
stony meteorites, called chondrites, are pieces of the same material
from which the planets formed. Another group of stony meteorites, the
achondrites, were once part of a parent body, such as an asteroid, that
was large enough to have melted and separated into an iron-rich core and
a stony crust. Achondrites come from the outer crust; stony-iron
meteorites, from the inner crust; and iron meteorites, from the metallic
core. Iron meteorites consist mostly of iron and nickel. Stony-iron
meteorites have nearly equal amounts of silicon-based stone and
iron-nickel metal.
The size of meteorites varies greatly. Most of them are
relatively small. The largest meteorite ever found weighs about 66 short
tons (60 metric tons). It fell at Hoba West, a farm near Grootfontein,
Namibia. However, much larger bodies, such as asteroids and comets, can
also strike the earth and become meteorites.
Meteorites reach the earth's surface because they are the right
size to travel through the atmosphere. If they are too small, they will
disintegrate in the atmosphere. If they are too large, they may explode
before reaching the earth's surface. One such object exploded about 6
miles (10 kilometers) above the Tunguska River in Siberia in 1908,
leaving a 20-mile (32-kilometer) area of felled and scorched trees.
Thousands of small meteorites have been found in Antarctica,
providing a rich supply of specimens for scientists to study. Scientists
study meteorites for clues to the types of material that formed the
planets.
Impact craters and basins
When large bodies such as asteroids and comets strike a planet, they produce
an impact crater or impact basin. Impact craters are bowl-shaped depressions
that measure up to about 10 miles (25 kilometers) in diameter. They have shallow,
flat floors and uplifted centers. Impact basins are larger, and inside their
rims there are one or more rings on the planet's surface.
Scientists have found more than 120 impact craters and basins on
the earth. One of the most famous, the Meteor Crater in Arizona, is
about 4,180 feet (1,275 meters) across and 570 feet (175 meters) deep.
It formed nearly 50,000 years ago when an iron meteorite weighing
330,000 short tons (300,000 metric tons) struck the earth.
Most impact craters and basins larger than the Meteor Crater are heavily worn
away or have been buried by rocks and dirt as the earth's surface changed. The
largest known of these is the Chicxulub (CHEEK shoo loob) Basin centered in
Mexico's Yucatan Peninsula. The diameter of the basin is about 190 miles (300
kilometers). Rock samples obtained by drilling into the basin indicate that
an asteroid struck the earth there about 65 million years ago. This was about
the time the last dinosaurs became extinct. The impact hurled much debris into
the sky. Many scientists believe this debris caused climate changes that the
dinosaurs could not survive.
Contributor: Virgil L. Sharpton, Ph.D., President's Professor, Geophysical Institute, University of Alaska Fairbanks.
How to cite this article:To cite this article, World Book recommends the following format:
Sharpton, Virgil L. "Meteor." World Book Online Reference Center. 2005.
World Book, Inc. http://www.worldbookonline.com/wb/Article?id=ar358140.