Mars: Dune Diversity in Renaudot Crater | NASA's Mars Reconnaissance Orbiter
Dark and light-toned dunes are located on the floor of Renaudot crater. The dark-toned dunes are likely basaltic sand, while the light-toned dunes source from other materials. The floor underlying the dunes is an eroded lighter-toned surface consisting of rougher, angular blocky material or cracked, cemented surface materials.
It is likely that the sources for these dunes are outside of the crater and sediment was blown in by prevailing winds. Windward-facing dune slopes tend to have lower slopes, while those pointing in the downwind direction are steeper. This suggests that the windward direction for the basaltic and larger light-toned dunes is generally towards the south, although there are smaller sets of differently aligned dunes suggesting varying wind directions.
This HiRISE image was captured when NASA's Mars Reconnaissance Orbiter (MRO) was at an altitude of 297 km (184 mi).
The University of Arizona, in Tucson, operates the High Resolution Imaging Science Experiment (HiRISE). It was built by BAE Systems in Boulder, Colorado. NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate (SMD), Washington.
Image Date: October 15, 2024
Release Date: July 8, 2025
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