000005233 001__ 5233
000005233 005__ 20210129100814.0
000005233 0247_ $$2DOI$$a10.1016/j.icarus.2020.113934
000005233 037__ $$aSCART-2021-0042
000005233 100__ $$aBeuthe, Mikael
000005233 245__ $$aComment on `Heating of Enceladus due to the dissipation of ocean tides’ by R. Tyler
000005233 260__ $$c2020
000005233 520__ $$aDissipation of ocean potential energy is proposed by Tyler (2020) as a new mechanism leading to possible high-power states for Enceladus. I show here that this process actually results from viscoelastic dissipation within the crust. For plausible values of Enceladus’s ocean thickness, crustal dissipation can be computed with the standard approach of static deformations of solid layers by equilibrium tides.
000005233 536__ $$aPRODEX program managed by the European Space Agency in collaboration with BELSPO/$$cPRODEX program managed by the European Space Agency in collaboration with BELSPO/$$fPRODEX program managed by the European Space Agency in collaboration with BELSPO
000005233 594__ $$aNO
000005233 773__ $$n113934$$pIcarus$$v350$$y2020
000005233 8560_ $$fmikael.beuthe@observatoire.be
000005233 85642 $$ahttps://www.sciencedirect.com/science/article/abs/pii/S0019103520303092
000005233 85642 $$ahttps://arxiv.org/abs/2011.14800
000005233 905__ $$apublished in
000005233 980__ $$aREFERD