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What evidence suggests that Europa has a liquid-water ocean beneath its ice?

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Evidence suggesting that Europa harbors a subsurface liquid-water ocean includes several key observations:

  • Induced Magnetic Field: Europa possesses an induced magnetic field that requires the presence of an electrically conducting fluid medium within the moon, implying a layer of salty liquid water beneath the icy crust.12
  • Surface Geology: The moon’s surface is remarkably smooth and features few impact craters, indicating it is geologically young and has undergone recent resurfacing. High-resolution images show fractured ice blocks that appear to have rotated and refrozen, suggesting the subsurface was once—and perhaps still is—semifluid.12
  • Surface Deposits: Mottled regions on the surface contain salt deposits, which scientists interpret as evidence of evaporation from a reservoir located below the crust. Additionally, spatter cones along surface grooves suggest fluid eruptions from the interior.12
  • Tidal Heating: Models indicate that tidal energy generated by Jupiter’s gravitational pull could provide the heat necessary to maintain a liquid ocean beneath the ice.12