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



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Ruiz Pérez, Javier and Álvarez Gómez, José Antonio and Tejero López, Rosa and Sánchez, Nieves (2007) Heat flow and thickness of a convective ice shell on Europa for grain size-dependent rheologies. Icarus (New York, N.Y. 1962) , 190 . pp. 145-154. ISSN 0019-1035

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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 mWm−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.

Item Type:Article
Uncontrolled Keywords:Europa; Jupiter, satellites; Thermal histories; Tides, solid body
Subjects:Sciences > Geology > Geodynamics
ID Code:10509
Deposited On:23 Apr 2010 11:04
Last Modified:05 May 2015 16:47

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