Fig. 8From: Strength models of the terrestrial planets and implications for their lithospheric structure and evolutionEffect 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 2Back to article page