Fig. B.4
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Frequency distribution of the torques exerted on the least massive planets plotted in green in Figure 14, e.g., for the runs 10Me-β3 and 10Me-β4. These two histograms show the stochasticity of the torques experienced by the 10 Earth mass planets, via a Gaussian distribution with standard deviation of σ3 ≃ 4 × 10−2 and σ4 ≃ 2 × 10−2 for an initial β0 of 103 and 104 respectively.
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