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10-4 10-3 10-2 10-1 10° 101 102 103 104 105 106 107 Diameter, cm

Fig. 5.24 Evolution of the size distribution of particles with a disk as a function of time. Initially, the grains have a diameter of 1 |m. The conditions in the protoplanetary disk are those in the primordial solar nebula, for a distance of 1 AU from the Sun (After Weidenschilling, 2000)

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