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<p>preliminary theoretical work was carried out prior to the planetary missions of the 1970s. In particular, Lewis showed in 1971 that <a href="page.php?w=radioactive_decay">radioactive decay</a> alone was likely sufficient to produce subsurface oceans in large moons, especially if ammonia (<a href="page.php?w=Ammonia">{{chem</a>) were present. Peale and Cassen figured out in 1979 the important role of <a href="page.php?w=tidal_heating">tidal heating</a> (aka: tidal flexing) on satellite evolution and structure. The first confirmed detection of</p><p>
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