Volcanism on Io, a moon of
Jupiter, produces
lava flows,
volcanic pits, and plumes of
sulfur and
sulfur dioxide hundreds of kilometres high. This volcanic activity was discovered in 1979 by
Voyager 1 imaging scientists. Observations of
Io by passing spacecraft and Earth-based astronomers have revealed more than 150 active volcanoes. Io's volcanism makes the satellite one of only four known volcanically active worlds in the solar system. First predicted shortly before the
Voyager 1 flyby, the heat source for Io's volcanism comes from
tidal heating produced by Io's forced
orbital eccentricity. Io's volcanism has led to the formation of hundreds of volcanic centres and extensive lava formations, making the moon the most volcanically active body in the solar system. Three different types of volcanic eruptions have been identified, differing in duration, intensity, lava effusion rate, and whether the eruption occurs within a volcanic pit. Lava flows on Io, tens or hundreds of kilometres long, have primarily
basaltic composition, similar to lavas seen on Earth at shield volcanoes such as
Kīlauea in
Hawaii. As a result of the presence of significant quantities of sulfurous materials in Io's crust and on its surface, during some eruptions, sulfur, sulfur dioxide gas, and
pyroclastic material are blown up to 500 kilometres (310 mi) into space, producing large, umbrella-shaped volcanic plumes. (
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