Evidence of flow?
About this image
The striations on the floor of this sinuous channel adjacent to Protonilus Mensae look like they result from the flow of lava or perhaps even glacial ice. However, it is also possible that they result from some process acting on permafrost confined within the channel having nothing to do with flow.
Please see the THEMIS Data Citation Note for details on crediting THEMIS images.
Context
Image ID:
V04442004 (View data in Mars Image Explorer)
33.7307
56.8222
4442
2002-12-14 23:36
Fri, 2003-01-17
VIS
1024 pixels (19 km)
3648 pixels (67 km)
0.018621 km/pixel
0.018756 km/pixel