Rotation and figure evolution in the creep tide theory. A new approach and application to Mercury
Gabriel O. Gomes, Hugo A. Folonier, Sylvio Ferraz-Mello

TL;DR
This paper introduces a new differential equation formulation of the creep tide theory to study planetary rotation and figure evolution, applying it to Mercury to estimate its relaxation factor and compare with observational data.
Contribution
It presents a coupled system of equations for rotation and figure evolution, and a method to determine the relaxation factor gamma for non-rigid bodies in spin-orbit resonance.
Findings
Derived gamma range for Mercury's rotational evolution
Found Mercury's figure coefficients match Darwin-Kaula model
Observed current Mercury flattenings exceed tidal theory predictions
Abstract
This paper deals with the rotation and figure evolution of a planet near the 3/2 spin-orbit resonance and the exploration of a new formulation of the creep tide theory (Folonier et al. 2018). This new formulation is composed by a system of differential equations for the figure and the rotation of the body simultaneously (which is the same system of equations used in Folonier et al. 2018), different from the original one (Ferraz-Mello, 2013, 2015a) in which rotation and figure were considered separately. The time evolution of the figure of the body is studied for both the 3/2 and 2/1 spin-orbit resonances. Moreover, we provide a method to determine the relaxation factor gamma of non-rigid homogeneous bodies whose endpoint of rotational evolution from tidal interactions is the 3/2 spin-orbit resonance, provided that (i) an initially faster rotation is assumed and (ii) no permanent…
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