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.

1440 Findings

Hours of research by our editors, distilled into minutes of clarity.

  • Earth is constantly bombarded by material from space

    Most of this matter is composed of small particles, with any smaller than 33 feet in diameter burning up in the atmosphere. Larger asteroids can reach the ground, and those larger than several thousand feet cause global damage, including earthquakes and tsunamis.

  • Only 40% of city-destroying asteroids have been detected

    Statistical modeling shows that while we have identified the majority of extinction-level asteroids, smaller asteroids that can cause significant damage remain elusive. Some asteroids, like the one that exploded over Chelyabinsk in 2013, can't be detected ahead of time since they come from the sun's direction.

  • NASA's DART mission successfully deflected an asteroid

    The Double Asteroid Redirection Test crashed into asteroid moonlet Dimorphos in 2022, altering its orbital radius. The project required precise astrodynamics to strike the moonlet from 11 million kilometers away while traveling 22,530 kilometers per hour.

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