Tides on Europa: The membrane paradigm
Author:
Beuthe
Abstract:
Jupiter’s moon Europa has a thin icy crust which is decoupled from the mantle by a subsurface ocean. The crust thus responds to tidal forcing as a deformed membrane, cold at the top and near melting point at the bottom. In this paper I develop the membrane theory of viscoelastic shells with depth-dependent rheology with the dual goal of predicting tidal tectonics and computing tidal dissipation. Two parameters characterize the tidal response of the membrane: the effective Poisson’s ratio View the MathML sourceν¯ and the membrane spring constant Λ , the latter being proportional to the crust thickness and effective shear modulus. I solve membrane theory in terms of tidal Love numbers, for which I derive analytical formulas depending on View the MathML sourceΛ,ν¯, the ocean-to-bulk density ratio and the number View the MathML sourcek2∘ representing the influence of the deep interior. Membrane formulas predict h2h2 and k2k2 with an accuracy of a few tenths of percent if the crust thickness is less than one hundred kilometers, whereas the error on l2l2 is a few percents. Benchmarking with the thick-shell software SatStress leads to the discovery of an error in the original, uncorrected version of the code that changes stress components by up to 40%. Regarding tectonics, I show that different stress-free states account for the conflicting predictions of thin and thick shell models about the magnitude of tensile stresses due to nonsynchronous rotation. Regarding dissipation, I prove that tidal heating in the crust is proportional to Im(Λ)Im(Λ) and that it is equal to the global heat flow (proportional to Im(k2)Im(k2)) minus the core-mantle heat flow (proportional to View the MathML sourceIm(k2∘)). As an illustration, I compute the equilibrium thickness of a convecting crust. More generally, membrane formulas are useful in any application involving tidal Love numbers such as crust thickness estimates, despinning tectonics or true polar wander.
Tuesday, November 25, 2014
Tides on Europa
Labels:
Europa,
Galilean moons,
jovian system,
jupiter,
planetary science,
tidal forces
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