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Fig. 7

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Mass of planetesimals formed at different locations in the disk. Left panel: Total mass of ‘rocky’ planetesimals as a function of the infall timescale, Tinfall, and the viscosity, α0. Rocky planetesimals are the ones that form around the silicate condensation line. White areas are disks that do not produce any planetesimals, while grey squares indicate disks that produce between zero and two Earth masses of planetesimals. Centre panel: Total mass of ‘icy’ planetesimals for a given disk. Icy planetesimals are the ones formed near the water snow line, typically beyond it. Right panel: Number of locations, i.e. rings, where planetesimals form.

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