Asteroids

Overview

Asteroids are small, rocky bodies left over from the early formation of the solar system. More than 1 million asteroids orbit the sun—primarily in the asteroid belt between Mars and Jupiter—ranging in size from bus-length to hundreds of miles in diameter. Astronomers catalog and study these objects to identify threats to Earth and better understand the solar system's history.

The search for asteroids began somewhat accidentally at the turn of the 19th century, when a group of scientists calling themselves the "Celestial Police" began searching for a suspected missing planet between the orbits of Mars and Jupiter. After Giuseppe Piazzi independently discovered Ceres, various members discovered three smaller celestial bodies: Pallas, Juno, and Vesta. All four were initially described as planets, but subsequent discoveries of smaller bodies prompted a new classification term: asteroids.

NASA's NEO Observations Program has detected over 40,000 near-Earth asteroids—those orbiting within 30 million miles of Earth. NASA has identified 95% of near-Earth asteroids over 0.6 miles in length, which are capable of causing global extinction events, though it continues to work toward identifying at least 90% of smaller, city-killing asteroids.

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