The layered bedrock in this image was brought from several kilometers of depth during the formation of this 44 kilometer wide crater in the volcanic plains of Lunae Planum.

As these layers were exhumed and brought to nearly vertical orientations, faulting and fracturing occurred and breccia dikes formed. Breccias are rocks consisting of angular and sharp fragments, and a dike is a fracture that has been widened by forces pulling apart the rock while simultaneously filling it with rocky materials. Breccia dikes are a common feature in terrestrial craters and can now be recognized in brilliant preservation on Mars.

This high-resolution, false-color image cutout above allows us to see a cross-cutting breccia dike near the bottom of the image. (Blue represents basaltic material.)

ID: ESP_017833_1975
date: 17 May 2010
altitude: 277 km

https://uahirise.org/hipod/ESP_017833_1975
NASA/JPL-Caltech/UArizona
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