Eccentricity and mean anomaly maps from the dataset BIN10100. We only plot the particles that met with Jupiter at least once during the 2000 years of integration. On the eccentricity map, we plot the width of the MMR (1:3 with Jupiter). The resonance is too wide for our set of initial conditions. The black line represents the limit of the MMR on its left side (see Fig. 4 for the full resonance width).