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Fig. 14 | Earth, Planets and Space

Fig. 14

From: Thermal evolution of icy planetesimals in the solar nebula

Fig. 14

Comparison of the radii of the inner and outer boundaries of water mantles (see Fig. 1) for three values of thermal conductivity: twice (dot lines), half (dot-dashed lines), and just equal to (solid lines), the standard value. Each icy planetesimal has the same parameters as model 50–10A. The abscissa and the ordinate are the same as in Fig. 8.

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