Fig. 4

Growth timescale tgrowth as function of planetesimal radius R for a constant internal density ρ• = 1 g cm-3. Crosses indicate numerical data, while the solid lines are fits. The color scale extends from dark blue to light blue, transitioning from lowest particle radius to highest particle radius. a) tgrowth obtained with the potential flow solution at 1 AU orbital distance and a pebble density of ρp = ρg/ 100, showing maxima at Rgr,max ~ 100 km. b) tgrowth with the Stokes flow solution at 1 AU orbital distance and a pebble density of ρp = ρg/ 100 , showing early settling and flattening out of the curves. c) tgrowth with the potential flow solution at 3 AU orbital distance and a pebble density of ρp = ρg/ 100. d) tgrowth with the potential flow solution at 10 AU orbital distance and a pebble density of ρp = ρg/ 100 (top, blue) and a pebble density of ρp = ρg (bottom, red).
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