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Dissipation of ocean potential energy is proposed by Tyler (2020) as a newmechanism leading to possible high-power states for Enceladus. I show here thatthis process actually results from viscoelastic dissipation within the crust.For plausible values of Enceladus's ocean thickness, crustal dissipation can becomputed with the standard approach of static deformations of solid layers byequilibrium tides.

Comment on `Heating of Enceladus due to the dissipation of ocean tides' by R. Tyler