Stability of Ice/Rock Mixtures with Application to a Partially Differentiated Titan
Joseph G. O'Rourke, David J. Stevenson

TL;DR
This study models the thermal evolution of Titan's ice/rock interior, showing that compositional gradients delay but do not prevent differentiation, challenging the idea of a partially differentiated Titan.
Contribution
It introduces a parameterized model of double-diffusive convection to assess Titan's internal differentiation, considering compositional heterogeneity and heat removal over time.
Findings
Double-diffusive convection delays ice melting in Titan's interior.
Realistic density gradients cannot prevent complete differentiation.
Titan is likely fully differentiated despite compositional heterogeneity.
Abstract
Titan's moment of inertia, calculated assuming hydrostatic equilibrium from gravity field data obtained during the Cassini-Huygens mission, implies an internal mass distribution that may be incompatible with complete differentiation. This suggests that Titan may have a mixed ice/rock core, possibly consistent with slow accretion in a gas-starved disk, which may initially spare Titan from widespread ice melting and subsequent differentiation. A partially differentiated Titan, however, must still efficiently remove radiogenic heat over geologic time. We argue that compositional heterogeneity in the major Saturnian satellites indicates that Titan formed from planetesimals with disparate densities. The resulting compositional anomalies would quickly redistribute to form a vertical density gradient that would oppose thermal convection. We use elements of the theory of double-diffusive…
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