Tidally heated convection: Constraints on Europa's ice shell thickness

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Titan's internal structure inferred from a coupled thermal-orbital model (2005, background): “In both cases, the temperature dependence of both ice Ih viscosity (Eq. (1)) and thermal diffusivity (Table 1) as well as the viscosity dependence of tidal dissipation ( Tobie et al., 2003 ) are included in our calculations.”
Ceres’ evolution and present state constrained by shape data (2010, background): “Certainly large variations of temperature between the equator and the poles can be the source of lateral variations of Ceres’ shell outer shell properties, as has been modeled for Europa (Tobie et al., 2003).”