Asteroids and the Asteroid Belt

Rocky and metal leftovers from the birth of the planets, and the spacecraft that brought pieces of them home.

Asteroids are rocky or metallic bodies left over from the early Solar System. Most travel in the main asteroid belt between Mars and Jupiter, but others share Jupiter's orbit, cross the paths of the inner planets or pass near Earth. They range from boulders to bodies hundreds of kilometers wide, and many are loose piles of rubble held together by weak gravity.

The belt is far emptier than movies suggest. Its total mass is less than that of the Moon, and the rocks are spread across an enormous region, so spacecraft cross it without special maneuvers. Astronomers sort asteroids by what they are made of, mostly dark carbon-rich types, stony types and metal-rich types, and by where they orbit.

This category covers both the science and the missions. NASA's Dawn studied Vesta and then Ceres. Japan's Hayabusa and Hayabusa2 brought back material from the asteroids Itokawa and Ryugu. NASA's OSIRIS-REx delivered a sample from Bennu to Earth in 2023, and NASA's DART spacecraft hit the small moonlet Dimorphos in 2022 to test whether a collision can change an asteroid's path.

Planetary defense gets its own guide because the topic attracts exaggeration. Space agencies track near-Earth asteroids, publish their orbits and explain the odds openly. Our guides report those statements with the date they were checked, and they leave out scenarios that no agency has put forward.

Start with what asteroids are for the basics. After that, follow your curiosity: a giant like Vesta, a sample mission like OSIRIS-REx and Bennu, or the 2029 flyby of Apophis.

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