Io

3,643 kmdiameter

Updated

3,643km
Visual creditGalileo 1999 / NASA / JPL / University of Arizona / Public domainSource: Wikimedia Commons

Details

Io is Jupiter's third-largest moon and the most volcanically active world in the Solar System. Tidal flexing by Jupiter, sustained by orbital resonance with Europa and Ganymede, keeps its interior hot enough to renew the surface with lava flows and sulfur-rich deposits.

Io’s 4:2:1 orbital resonance with Europa and Ganymede prevents its orbit from becoming circular. As its distance from Jupiter changes, solid-body tides flex the moon by as much as about 100 meters and generate enough internal heat to power hundreds of volcanoes. Repeated lava flows and sulfur-rich deposits resurface Io so rapidly that few impact craters remain visible.

Key facts

Category
Moons
Object class
Galilean moon
Mass
~0.015 Earth masses
Scale fact
3,643 kmdiameter
Estimated age
~4.5 billion years
Composition
Silicate rock with sulfur-rich surface deposits
Embed

Size neighbors

Objects near Io on the scale

On the logarithmic size axis, Io falls between Moon and Callisto. The band uses nearby Galilean moon records.

Shared physical scale
4,022km
Io3,643 km
Callisto4,821 km
Ganymede5,260 km

Sources

References for Io

Measurements and descriptive context are compiled by the Scale of Space team from the references below. If you find an error, please let us know.

Continue with nearby objects or open the full scale.

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