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HiPOD 26 Apr 2023: A Flow-Like Feature within Chryse Planitia

This image covers a flow-like feature that is hypothesized to be the result of subsurface sediment mobilization. With it, we can investigate details about the associated mud movement over the Martian surface. The flow is showing an interesting shape that might be evidence of the former presence of an icy-muddy crust.

uahirise.org/hipod/ESP_072993_
NASA/JPL-Caltech/UArizona

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