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Fig. 8 | Progress in Earth and Planetary Science

Fig. 8

From: Strength models of the terrestrial planets and implications for their lithospheric structure and evolution

Fig. 8

Effect of thermal gradient on elastic thickness for each planet for various models. Dashed, solid, and dotted lines indicate calculation results using strain rates of 10−16, 10−17, and 10−18 s−1, respectively. In the calculations, a tensional stress field is assumed at shallow depths, which shifts to compression at greater depths. The parameters for the calculations are listed in Tables 1 and 2

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