The Mysterious Inner Workings of Io, Jupiter’s Volcanic Moon
Crucially, unlike Io’s odd magnetic field, which seemed to indicate that it concealed an ocean’s worth of fluid, Europa’s own Galileo-era magnetic signal remains robust. “It’s a pretty clean result at Europa,” said Robert Pappalardo, the Europa mission’s project scientist at the Jet Propulsion Laboratory. The icy moon is far enough from Jupiter and the intense plasma-flooded space environment of Io that Europa’s own magnetic induction signal “really sticks out.” But if both moons are tidally heated, why does only Europa have an inner ocean? According to Nimmo, “there’s a fundamental difference between a liquid-water ocean and a magma ocean. The magma wants to escape; the water really doesn’t.” Liquid rock is less dense than solid rock, so it wants to rise and erupt quickly; the new study suggests that it doesn’t linger at depth long enough inside Io to form a massive, interconnected ocean. But liquid water is, unusually, denser than its solid icy form. “Liquid water is heavy, so it collects into an ocean,” Sori said. “I think that’s the big-picture message from …