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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 5.

Quasi-steady thermal regulation along a constant angular momentum migration track at fixed eccentricity, e = 0.7. Columns correspond to cooling indices β = 1, 4, and 8 in Equation (28). Colored curves show solutions of the thermal balance equation for three values of the dimensionless normalization A0. In each column, the cooling normalization Lcool,0 is chosen so that the middle model, A0 = 10−5, has te = 5 Gyr at af = 0.06 au; the dashed gray fixed-Δt comparison is normalized at the same point. Upper panels show the eccentricity damping time te, middle panels show the representative tidal quality factor Qeff, and lower panels show the corresponding equilibrium temperature X = Tc/Tref. Thermal regulation weakens the dependence of te on af relative to the standard constant time lag scaling, ﹩{t}_{e}\propto {a}_{f}^{8}﹩, by driving larger Qeff at smaller circularization radii.

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