Article ID Journal Published Year Pages File Type
10701543 Icarus 2012 11 Pages PDF
Abstract
► We present 3D spherical models of convection in Enceladus' ice shell. ► We implement a mechanically weak lithosphere within Enceladus' SPT. ► We find vigorous convection in the ice underneath the SPT. ► Stagnant lid convection or no convection occurs elsewhere over the satellite. ► Our models explain high heat flow, intense tectonism, and young ages in SPT.
Keywords
Related Topics
Physical Sciences and Engineering Earth and Planetary Sciences Space and Planetary Science
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The impact of a weak south pole on thermal convection in Enceladus' ice shell
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