Sediments rich in hydrated sulfates may have filled central Valles Marineris, but debates persist as to how these deposits grew or formed.

If they formed from deposition in a deep lake then the layers should be nearly horizontal. If the layers formed from airfall deposits such as volcanic pyroclastics or windblown dust, then the layers should drape over the pre-existing topography.

Another possibility is that the layers were deformed by slumping. Stereo topographic data can be used to test these hypotheses. The cutout shows an area at full resolution. There are no detectable color variations within these layers, suggesting a uniform composition or the presence of a thin cover of dust over all surfaces.

ID: ESP_072546_1725
date: 17 January 2022
altitude: 262 km

https://uahirise.org/hipod/ESP_072546_1725
NASA/JPL-Caltech/UArizona
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