Odd Channel
About this image
This usual channel feature is located south of Tooting Crater near Lycus Sulci. It most likely formed by the release of melted sub-surface ice. The impact crater event may have caused the heating, or volcanic activity from Olympus Mons.
Please see the THEMIS Data Citation Note for details on crediting THEMIS images.
Context
Image ID:
V95004003 (View data in Mars Image Explorer)
21.9884
208.652
95004
2023-05-15 22:29
Fri, 2023-12-01
VIS
512 pixels (19 km)
1824 pixels (68 km)
0.037391 km/pixel
0.0377089 km/pixel