(Top) The inclination of current day asteroids with absolute magnitude H < 9.7, corresponding to D ≳ 50 km, plotted as a function of their semimajor axis. The long-dashed lines show the location of the major mean motion resonances with Jupiter and the short-dashed curves the location of the ν₆ and ν₁₆ secular resonances. (Bottom) Surviving planetesimals from the 12 simulations, showing a strong depletion of low inclination bodies in the inner part of the asteroid belt region.