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In a final burst of glory in November, Galileo will plunge into Io’s highly charged atmosphere, searching for close-ups of that molten moon’s surface. The flight is likely to be the end for Galileo but just the beginning of reasons to keep going back to these compelling worlds.
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Callisto has one of the most battered and scarred surfaces in the solar system, the result of 4.6 billion years of abuse from incoming asteroids. Unlike its sibling moons, Callisto has no large-scale processes for erasing craters; some may fade as the underlying ice evaporates, but most simply sit on top of earlier scars. Still, something mysterious is going on beneath the dusty crust of this ball of ice and rock. During a recent flyby, Galileo detected a magnetic field that indicates a salty ocean.
The interiors of Io, Europa, Ganymede, and Callisto (clockwise from top left): While three of the moons have metallic cores similar to Earth’s, Callisto has a mixture of ice and rock at its heart. Europa, Ganymede, and Callisto may contain hidden oceans.
Images of a shattered landscape (right) led researchers to a remarkable conclusion: Europa’s surface is littered with icebergs frozen in place. |








