Heat flow and thickness of a convective ice shell on Europa for grain size-dependent rheologies

Details Heat flow and thickness of a convective ice shell on Europa for grain size-dependent rheologies Heat flow and thickness of a convective ice shell on Europa for grain size-dependent rheologies

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007icar..190..145r&link_type=abstract

Icarus, Volume 190, Issue 1, p. 145-154.

Mathematics

Logic

3

Scientific paper

Although it is mostly accepted that the lower part of the ice shell of Europa is actively convective, there is still much uncertainty about the flow mechanism dominating the rheology of this convective layer, which largely depends on the grain size of the ice. In this work, we examined thermal equilibrium states in a tidally heated and strained convective shell, for two rheologies sensitive to grain size, grain boundary sliding and diffusion creep. If we take a lower limit of 70 mW m-2 for the surface heat flow, according to some geological features observed, the ice grain size should be less than 2 or 0.2 mm for grain boundary sliding or diffusion creep respectively. If in addition the thickness of the ice shell is constrained to a few tens of kilometers and it is assumed that the thickness of the convective layer is related to lenticulae spacing, then grain sizes between 0.2 and 2 mm for grain boundary sliding, and between 0.1 and 0.2 mm for diffusion creep are obtained. Also, local convective layer thicknesses deduced from lenticulae spacing are more similar to those here derived for grain boundary sliding. Our results thus favor grain boundary sliding as the dominant rheology for the water ice in Europa's convective layer, since this flow mechanism is able to satisfy the imposed constraints for a wider range of grain sizes.

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