Jupiter

Jupiters Rings

Jupiter's main ring system is formed by dust kicked up as interplanetary meteoroids smash into the giant planet's four small inner moons Almathea, Thebe, Adrastea and Metis. The ring system begins about 92,000 kilometers (55,000 miles) from Jupiter's center and extends to about 250,000 kilometers (150,000 miles) from the planet. NASA's Voyager 2 detected an uneven dust ring around Jupiter in 1979. One Voyager image seemed to indicate a third, faint outer ring. The Galileo spacecraft found a flattened main ring and an inner, cloud-like ring, called the halo, both composed of small, dark particles, and a third ring known as the Gossamer Ring. The third ring is actually two very thin rings made up of debris from Amalthea and Thebe. Unlike Saturn's rings, there are no signs of ice in Jupiter's rings.

The planet contains 71% of the planetary matter in the solar system