Is Titan in hydrostatic equilibrium?

Physics

Scientific paper

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Scientific paper

The observed ratio of the degree-2 gravity coefficients of Titan, J2/C22 10/3, is consistent with a degree-2 gravity field and moments of inertia dominated by hydrostatic rotational and tidal deformation. We consider the effect of non-hydrostatic contributions to validate the significance of this ratio. We illustrate that the observed ratio is also consistent with a degree-2 gravity field and moments of inertia dominated by fossil figure and/or mass anomaly contributions. However, a dominant fossil figure contribution is unlikely since the expected orbital migration is small, and a dominant mass anomaly contribution can be rule out given the observed power spectrum of the gravity field.

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