Fig. 12
From: Thermal evolution of icy planetesimals in the solar nebula
Temperature evolutions at the centers of different-sized icy plan-etesimals and rocky planetesimals. Results for model 50–10A (thin dashed line), 100–10A (thin dot-dashed line) and 500–10A (thin solid line), and for rocky planetesimals with radii of 23 km (thick dashed line), 53 km (thick dot-dashed line), and 270 km (thick solid line) formed 1.5 Myr after CAI formation with 273 K for the initial temperature are shown. The abscissa, the ordinate and the horizontal dotted lines are the same as in Fig. 5.