Fig. 2
Secular evolution of the eccentricity of GJ 436b starting from the present-day orbit and assuming a standard perturber (m′ = 0.1 MJup, T′ = 10 yr) in different conditions (see text): a) perturbing planet, but no tides nor relativity; b) tides and relativity but no perturbing planet; c) perturbing planet, relativity but no tides; d) perturbing planet, relativity and tides.
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