Fig. 13
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Tidal evolution of the WASP-148 system. Starting with the nominal solution from Table 4, we show the evolution of the mutual inclination (top), the eccentricities (middle), and semi-major axes (bottom) over 800 Myr. We used a direct three-body model with linear tides (Correia 2018) with general relativity corrections, and adopted k2 = 0.5 and Δt = 1 s for both planets.
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