Resonance breaking due to dissipation in planar planetary systems

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Fig. 7

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Same as Fig. 6 but for GJ 581b, and c (5:2 MMR). The top x-axis (Δt₂/ Δt₁) is scaled using the value κ ≈ 15 obtained in Eq. (87). We note that M₁ varies only between 0° (center of libration) and 90° (separatrix), because the resonant combination is 5M₂ − 2M₁ (factor 2 in front of M₁).

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