Fig. 5From: Inferring the high velocity of landslides in Valles Marineris on Mars from morphological analysisGeomorphological map of the Ophir Labes and Coprates Labes landslides located at the boundary between Melas-Coprates Chasmata of VM, with indicated the most important features of the terrain. The map has been built based both on general examination of the THEMIS images, and on scrutiny of the HRSC images at the detail of 10 m per pixel Points F-I indicate the positions where velocities have been estimated (see Table 2)Back to article page