Jupiter Moon · Most Volcanically Active Body
400+ Active Volcanoes · The Pizza Moon
400+ Active
3,643 km
1,700°C+
1.77 Days
Io is the innermost of Jupiter’s four Galilean moons and the most volcanically active body in the entire solar system. With over 400 active volcanoes, its surface is continuously reshaped by eruptions so frequent that virtually no impact craters remain. Io’s distinctive yellow, orange, red, and black coloring—earning it the nickname “pizza moon”—comes from various forms of sulfur and sulfur dioxide.
Io’s extreme volcanism is driven by tidal heating: Jupiter’s immense gravity, combined with orbital resonance with Europa and Ganymede, flexes Io’s interior, generating enormous friction and heat. Surface temperatures near volcanic vents exceed 1,700°C, hotter than any lava on Earth. Loki Patera, Io’s largest volcanic depression, is a 200-km-wide lava lake that periodically brightens as its surface crust overturns.
NASA’s Juno spacecraft has made multiple close flybys of Io since 2023, capturing stunning images from as close as 1,500 km. These observations revealed that Io’s volcanoes are even more active than previously thought. Despite Io’s extreme environment, studying its volcanism helps scientists understand tidal heating processes that may warm the oceans of Europa and Enceladus.
Largest volcanic depression at 200 km across. Periodically overturning lava lake visible from Earth telescopes.
Iconic volcanic plume rising 300+ km. Creates a massive red sulfur ring 1,200 km in diameter.
Jupiter’s gravity generates enormous internal friction. Produces 100 trillion watts—20× Earth’s total heat flow.
Colorful surface of sulfur compounds at various temperatures. Constantly repainted by volcanic eruptions.
Distinctive yellow-orange-red coloring from sulfur. One of the most recognizable objects in the solar system.
Surface completely renewed every million years. Volcanic resurfacing erases all evidence of impacts.
Io serves as a natural laboratory for understanding volcanism and tidal heating—processes crucial to the habitability of ocean worlds like Europa and Enceladus. By studying how Jupiter’s gravity generates Io’s internal heat, scientists can better model the energy budgets of other tidally heated moons throughout the solar system and around exoplanets.
The Io Volcano Observer (IVO) mission concept has been proposed to orbit Jupiter and make repeated close flybys of Io to map its volcanism, measure tidal heating, and determine whether Io has a magma ocean beneath its surface. Understanding Io’s extremes pushes the boundaries of planetary science and volcanology.
Galileo Galilei discovered Io on January 8, 1610. Named after a priestess of Hera in Greek mythology who was loved by Zeus, Io was first revealed as a volcanic world when Voyager 1 scientist Linda Morabito discovered an eruption plume in 1979—the first active volcanism observed beyond Earth.
NASA’s Galileo orbiter (1995-2003) made numerous close flybys, mapping volcanic activity in detail. The Juno spacecraft began close Io observations in 2023, flying within 1,500 km and revealing volcanic features at unprecedented resolution. Ground-based adaptive optics telescopes regularly monitor Io’s eruptions from Earth.
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