'Softened' impact craters on Mars - Implications for ground ice and the structure of the Martian megaregolith

Physics

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Mars Surface, Planetary Craters, Ice, Regolith, Soil Mechanics, Creep Properties, Topography, Temperature Dependence, Finite Element Method

Scientific paper

FEM is here used to investigate the relaxation of impact craters on Mars, due to creep deformation of subsurface ice, that has been hypothesized as a basis for the 'terrain softening' type of landform degradation. A non-Newtonian viscoelastic rheology derived from experiments on frozen solids is asummed. The results thus obtained imply a Martian midlatitude softened terrain morphology consistent with relaxation in a deforming layer that is no more than 1 km in depth. The total amount of Martian subsurface ice is estimated on this basis.

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