Reported March 2008

WHAT ARE ASTEROIDS? Asteroids are not the same as comets. Comets are essentially large, dirty snowballs. They are made of ice and frozen gases, mixed with rocky material and dust, and travel in large oval orbits, sometimes leaving our solar system. In contrast, asteroids are metallic, rocky bodies, without atmospheres, that orbit the Sun, just like planets, but are too small to be considered planets themselves. There are tens of thousands of them gathered into the main asteroid belt, a donut-shaped ring located between the orbits of Mars and Jupiter. Astronomers conclude they are made from primordial rock. Jupiter's strong gravity prevented these small bodies from forming into a planet when the solar system began 4.6 billion years ago.

DEEP IMPACT: Asteroids and comets have routinely collided with Earth since our planet was formed four billion years ago, although these are rarely catastrophic, because most aren't large enough. The total mass of all the asteroids combined is less than that of the Moon. But occasionally a very large asteroid -- a quarter mile wide or more -- will strike with devastating effects, such as the extinction of the dinosaurs. When an asteroid, or part of it, crashes into Earth, it is called a meteorite. There are currently two programs in the US to actively search for these near-earth objects: NASA's Near Earth Asteroid Tracking program and Spacewatch at the University of Arizona.

The American Astronomical Society contributed to the information contained in the TV portion of this report.

If you would like more information, please contact:

Andrew Becker, Ph.D.
University of Washington
Seattle WA 98195-1580
(206) 685 0542
becker@astro.washington.edu

American Astronomical Society
Washington, DC 20009-1231
(202) 328-2010
http://www.aas.org
aas@aas.org

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