The large dark feature is a classic Martian sand dune. Most sand on Earth is made from the mineral quartz, which is white and bright. On Mars, most sand is composed of dark basalt, a volcanic rock. For this reason, dunes on Mars are darker than those on Earth.
The dunes in this observation , within Wirtz Crater, are known as “barchans.” The steepest slope is on the eastern (right) side, partially in shadow, and represents the direction the dune is migrating as the sand is blown and transported by the wind. Small ripples are visible on much of the dune surface. The dark streaks on the dune are tracks left by passing vortices known to us as dust devils. These raise dust off the dune, revealing a darker substrate.
Written by: Nathan Bridges (19 January 2017)
This is a stereo pair with ESP_021893_1315 .
More info and image formats at http://hirise.lpl.arizona.edu/ESP_021603_1315
Image: NASA/JPL/University of Arizona