HiRISE: Beautiful Mars explains how small ancient craters in Aeolis Dorsa can constrain Mars paleoatmospheric pressure and sediment accumulation rates, showing how imagery supports quantitative climate reconstruction.
HiRISE 3D: Small Exhumed Craters in Aeolis Dorsa
Small ancient craters can directly constrain the paleoatmospheric pressure on Mars via crater sizes and additionally constrain sediment accumulation rate via exhumed-crater frequency.
This finding is one of many signals tracked across Space. The live feed updates every few hours with new authority voices, debates, and emerging ideas.
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