“…The stability against convection of a layer (in this case, Callisto's outer ice shell) can be estimated by means of the Rayleigh number de®ned at the layer base, Ra base ; for non-newtonian viscosity, this is These regimes are associated with premelting effects 18 , or with recrystallization under stress 30 , and have still higher values 18 of Q; they dominate at temperatures above ,240±260 K (different reports give different temperatures in this range 18,29 given by 7 Ra base agrh n 2 =n DT k 1=n b 1=n exp v=n 1 where a is the volumetric thermal expansion coef®cient, g is the acceleration due to gravity (taken in general as the surface value, 1.24 m s -2 for Callisto), r is the density (930 kg m -3 for water ice I), h is the effective layer thickness, DT ( T base 2 T s ) is the temperature difference between the base and the surface of the layer, k is the thermal diffusion coef®cient, b is a parameter that depends on creep mechanism and temperature, and n is a constant that depends on creep mechanism. v ( QDT=RT 2 i ) is the Frank±Kamenetskii parameter (which is related to the viscosity contrast through the layer caused by temperature differences), where Q is the activation enthalpy of creep deformation (which, because of experimental uncertainty, can be taken as the activation energy), R is the gas constant, and T i is the adiabatic temperature (approximately constant) in the case of convection.…”