Case (1): tidal evolution of a planet of mass 1 M⊕ orbiting a 0.08 M⊙ BD calculated with the secular code (blue dashed line) and the Mercury-T code (full red line). Graph a) from top to bottom: evolution of the semi-major axis of the planet, evolution of its eccentricity and evolution of the tidal heat flux. Graph b) from top to bottom: evolution of the obliquity of the planet, evolution of its rotation period (the pseudo-synchronization period is represented in long red dashes), and conservation of total angular momentum.
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