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Tidal heating9/18/2023 The generation of heat due to friction produced by the strong tidal forces exerted by a very massive parent body on a body moving about it in an elliptical orbit. Io has a similar mass and size as the Moon, but Io is the most geologically active body in the Solar System. Orbital and rotational energy are dissipated as heat in the crust of the moon. Tidal heating of Io (also known as tidal working) occurs through the tidal friction processes between Jupiter and its moon. Why does Io experiences strong internal tidal heating? Why are there no visible impact craters on the surface of Io quizlet?.Why are there no craters on Io and few on Europa?.What evidence do you see for tectonic activity on Ganymede?.What is the difference between Io and Europa satellites?.Why are Ganymede and Callisto geologically dead while the other two Galilean moons are not?.Why are Jupiter’s Galilean moons geologically active?.Why are numerous impact craters found on Ganymede and Callisto but not on Io or Europa?.What evidence supports the hypothesis that Europa has an active surface and liquid sub surface ocean?.What causes the geological activity seen on Europa and Io?.Which forces cause tidal heating of Jupiter’s moon?.Which statement about Jupiter’s moon Io is true?.What causes the heating of Io that gives rise to volcanic activity?.What is the relevance of tidal heating to the possibility of life on Jovian moons?.Why does Io experience a much more substantial tidal force compared to the moon?.Why does Io experiences strong internal tidal heating?.
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