Melas Dorsa 3D anaglyph

Melas Dorsa imaged during revolution 10532 on 17 April 2012 by ESA’s Mars Express using the High-Resolution Stereo Camera (HRSC). Data from HRSC’s nadir channel and one stereo channel are combined to produce this anaglyph 3D image that can be viewed using stereoscopic glasses with red–green or red–blue filters. The image clearly shows the wrinkle ridges bisected by the en echelon fault lines. Centred at around 18°S and 288°E, the image has a ground resolution of about 18 m per pixel.