Fig. 9
From: Thermal evolution of icy planetesimals in the solar nebula
The temperature evolution of model 500–10A. Line graphs represent 1.2 Myr (dashed line), 2.0 Myr (dot-dashed line), 2.8 Myr (dot-dot-dashed line) and 6.0 Myr after CAI formation (solid line), respectively. The abscissa shows the radius from the center in km and theordinate shows the temperature in kelvin. The horizontal dotted lines are the same as in Fig. 5.