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Spain - Toledo - You'll Want to Come Back

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In addition, the volatile-containing upper crust of Mars (Fig. 11) provides conditions and environments conducive to instability development. Although there is a wide range in the morphometric characteristics of volcanoes on Mars (Pike 1978), the Tharsis shield volcanoes provide good examples of the array of features related to volcanic instability observed on Mars. Comer et al. (1985) used the deformational structures surrounding several Tharsis volcanoes to assess lithospheric flexure caused by volcano loading and to estimate the thickness of the elastic lithosphere (Fig.

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