Public domain
Wind Erosion
From the collection of NASA Image and Video Library. Free to download, adapt and use — no permission needed.
About this work
This VIS image is located between the uplands of Aeolis Mensae and Aeolis Planum. This region of the Martian surface is highly dissected by wind action. The surface materials are poorly cemented and easily eroded. It has been suggested that the surface is comprised of volcanic ash deposits, sourced from the Tharsis and Apollinaris volcanoes.
NASA Image and Video Library’s own descriptionSubjects
Credit lineWind Erosion. NASA/JPL, 2020-06-25. Public domain. ID: PIA23959.
