Tidal Love numbers of membrane worlds: Europa, Titan, and Co

Abstract

Under tidal forcing, icy satellites with subsurface oceans deform as if the surface were a membrane stretched around a fluid layer. `Membrane worlds' is thus a fitting name for these bodies and membrane theory provides the perfect toolbox to predict tidal effects. I describe here a new membrane approach to tidal perturbations based on the general theory of viscoelastic-gravitational deformations of spherically symmetric bodies. The massive membrane approach leads to explicit formulas for viscoelastic tidal Love numbers which are exact in the limit of zero crust thickness. Formulas for load Love numbers come as a bonus. The accuracy on $k_2$ and $h_2$ is better than one percent if the crust thickness is less than five percents of the surface radius, which is probably the case for Europa and Titan. The new approach allows for density differences between crust and ocean and correctly includes crust compressibility. This last feature makes it more accurate than the incompressible propagator matrix method. Membrane formulas factorize shallow and deep interior contributions, the latter affecting Love numbers mainly through density stratification. I show that a screening effect explains why ocean stratification typically increases Love numbers instead of reducing them. For Titan, a thin and dense liquid layer at the bottom of a light ocean can raise $k_2$ by more than ten percents. The membrane approach can also deal with dynamical tides in a non-rotating body. I show that a dynamical resonance significantly decreases the tilt factor and may thus lead to underestimating Europa's crust thickness. Finally, the dynamical resonance increases tidal deformations and tidal heating in the crust if the ocean thickness is of the order of a few hundred meters.

71 pages, 15 figures, 11 tables, submitted to Icarus. Revision includes load Love numbers, dynamical propagator matrix, and other minor corrections

References in corpus (3)

• Tidal dissipation in stars and giant planets
• Spatial patterns of tidal heating
• Tides on Europa: the membrane paradigm

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• Powering the Galilean Satellites with Moon-Moon Tides
• Two-layer compact stars with crystalline quark matter: Screening effect on the tidal deformability
• Exomoon Climate Models with the Carbonate-Silicate Cycle and Viscoelastic Tidal Heating
• Tidal Love numbers and moment-Love relations of polytropic stars
• Isostasy with Love: I Elastic equilibrium
• Librations of a body composed of a deformable mantle and a fluid core
• Love-C relations for elastic hybrid stars
• Exploring the Interior Structure and Mode of Tidal Heating in Enceladus