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Thermally Regulated Viscoelastic Tidal Migration of Eccentric Planets

  • Authors: Cristobal Petrovich, Hareesh Gautham Bhaskar

Cristobal Petrovich and Hareesh Gautham Bhaskar 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 8.

High-eccentricity collapse of the equilibrium spin, normalized by the Hut value, as a function of x = M. The points show numerical zero-torque equilibria for 0.7 ≤ e ≤ 0.9, selecting the highest-frequency stable branch when multiple stable roots exist. The black curve shows the empirical envelope fit in Equation (B7). The lower panel shows the fractional residuals. The fit is intended for the early high-eccentricity transition from solid-like to fluid-like response.

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