Overslaan en naar de inhoud gaan
Publicaties | Personen | Instituten | Projecten
[ meld een fout in dit record ]mandje (1): toevoegen | toon Print deze pagina

one publication added to basket [295828]
Tides on Europa: the membrane paradigm
Beuthe, M. (2015). Tides on Europa: the membrane paradigm. Icarus 248: 109-134. https://dx.doi.org/10.1016/j.icarus.2014.10.027
In: Icarus. Elsevier. ISSN 0019-1035; e-ISSN 1090-2643, meer
Peer reviewed article  

Beschikbaar in  Auteur 

Author keywords
    Europa; Tides, solid body; Tectonics; Planetary dynamics

Auteur  Top 

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 theology 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 9 and the membrane spring constant A, 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 A, 9, the ocean-to-bulk density ratio and the number 14 representing the influence of the deep interior. Membrane formulas predict h(2) and k(2) with an accuracy of a few tenths of percent if the crust thickness is less than one hundred kilometers, whereas the error on 12 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(A) and that it is equal to the global heat flow (proportional to Im(k(2))) minus the core-mantle heat flow (proportional to Im(k(2)degrees)). 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.

Alle informatie in het Integrated Marine Information System (IMIS) valt onder het VLIZ Privacy beleid Top | Auteur