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Very early collisional evolution in the asteroid belt

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Figure

Fig. 2. Same as Fig. 1, for a 200 km planetesimal that encounters the 3:2resonance. Multiple resonances increase e while the orbit decays
Fig. 3.Results of a collisional simulation involving two populations of asteroids: low-velocity (non resonant), and high-velocity (resonant)
Fig. 4.For the case shown in Fig. 1, trapping in the 2:1 resonance of a300 km planetesimal, its velocity relative to the nebular gas is plotted.Each curve shows the variation during an orbital period, from perihelionto aphelion, at intervals of 10000 y, during a total time of 1.5 × 105 y.

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