A TWO-DIMENSIONAL, LINEAR–ELASTIC MODEL TO EXPLAIN RADIAL EXTENSIONAL FRACTURES, PANTHEON FOSSAE, CALORIS BASIN, MERCURY
The model presented here attempts to describe the state of the stress field, independent of the physical mechanism that produced it. The first part of the analysis uses a model with azimuthal symmetry, consisting of a two-dimensional infinite plate with a hole in the center to represent the crater and a constant horizontal pressure applied along the crater wall. This model produces a stress field with compressive stresses in the radial direction and tensional stresses in the azimuthal direction, which is consistent with the formation of radial extensional fractures. However, this simple model cannot explain the observed asymmetry of the fractures distribution, where fractures extend further and are more abundant along a preferred azimuth of approximately N30°E. The second part of the analysis superposes a regional stress field, with the maximum horizontal compressive stress aligned with this direction of maximum fracture extent. This analysis shows that the yield strength of the lithosphere is minimal along the direction of the maximum compressive stress. Therefore, a stress field with constant pressure applied horizontally along the crater wall superimposed upon a regional stress field with maximum horizontal compressive stress aligned along a N30°E azimuth can adequately explain the observed fracture distribution.