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barry barry
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10 years ago
Contrast the internal structures of the four Galilean moons.  How are their internal differences reflected in the nature of their surfaces and other factors like their mean densities?
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10 years ago
Io: Molten to core, high density (3600 kg/m3), abundance of sulfur. Surface very active.
Europa: Water ice crust over liquid water ocean over rocky core.  Lower density than Io (3000 kg/m3).  Surface somewhat active, with only a few fairly new impact craters.
Ganymede, Callisto: Water ice, frozen.  Low density (1900 kg/m3). Surface dead and inactive, with many craters.
Would you know my name, if I saw you in heaven?

Eric Clapton
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barry Authorbarry
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10 years ago
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