Dark Light
These lovely linear dunes at Meroe Patera identified in Context Camera images that have developed in a sand starved region of the dune field, elongating from behind a cliff.

HiRISE was asked to obtain this observation in order to compare morphology to other linear dunes elsewhere on Mars.


Image: NASA/JPL/University of Arizona https://www.uahirise.org/hipod/ESP_065194_1875
Related Posts

Wind Carved Rock

The distinctively fluted surface and elongated hills in this image in Medusae Fossae are caused by wind erosion of a soft fine-grained rock.

River of Sand

A dominant driver of surface processes on Mars today is aeolian (wind) activity. In many cases, sediment from this activity is trapped in low-lying areas, such as craters.