Do tidally-generated inertial waves heat the subsurface oceans of Europa and Enceladus?
Abstract
Some of the moons of the outer solar system harbour subsurface liquid oceans. Tidal dissipation plays an important role in preventing these oceans from freezing. In the past, most studies considered only tidal dissipation in the solid layers of these bodies (rock and ice). Recently, new studies considering tidal dissipation in the oceans of these moons have appeared. All of them make use of the shallow water approximation. However, the use of...
Paper Details
Title
Do tidally-generated inertial waves heat the subsurface oceans of Europa and Enceladus?
Published Date
Mar 1, 2019
Journal
Volume
321
Pages
126 - 140
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Notes
History