Angustus Labyrinthus
Image Credit: NASA/JPL/ASU
About this image
The ridges in this VIS image are part of Angustus Labyrinthus. The intersecting ridges were most likely formed due to tectonic activity.
Please see the THEMIS Data Citation Note for details on crediting THEMIS images.
Context
Image ID:
V67279005 (View data in Mars Image Explorer)
-81.43
296.558
67279
2017-02-12 16:12
Wed, 2017-04-05
VIS
512 pixels (16 km)
1824 pixels (57 km)
0.031699 km/pixel
0.032025 km/pixel
