Thermal equilibrium in Europa's ice shell |
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| Authors: | William B Moore |
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| Institution: | Department of Earth and Space Sciences, Institute of Geophysics and Planetary Physics, University of California, Los Angeles, 3806 Geology Bldg., Box 951567, Los Angeles, CA 90095-1567, USA |
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| Abstract: | Models of tidal-convective equilibrium for Europa's ice shell are computed using a laboratory-derived composite flow law for ice. Volume diffusion creep is found to dominate the flow law at equilibrium, and thus the thickness of the shell is strongly dependent on the poorly known grain size of the ice. This grain size is, however, constrained to be less than a few millimeters if equilibrium is achieved at the current eccentricity. Europa's ice shell cannot be thinner than about 16 km in equilibrium at present, since tidal dissipation cannot generate enough heat in such a thin shell to balance the heat transport. No conductive equilibria are found; this is likely due to the fact that most of a conductive shell must be cold if temperature gradients are to be large enough to carry the heat. A minimum eccentricity of about 0.0025 (about 1/4 the present value) below which there are no equilibria is also found. |
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| Keywords: | Europa Interiors Thermal histories |
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