Patapsco Vallis
Image Credit: NASA/JPL/ASU
About this image
This VIS image shows where Patapsco Vallis enters the largest depression of Elysium Fossae. Patapsco Vallis, as other valley systems on the Elysium Mons volcanic complex, was likely formed by the flow of lava rather than water.
Please see the THEMIS Data Citation Note for details on crediting THEMIS images.
Context
Image ID:
V52938012 (View data in Mars Image Explorer)
23.8099
153.968
52938
2013-11-19 20:20
Wed, 2014-01-08
VIS
1024 pixels (18 km)
3648 pixels (66 km)
0.018328 km/pixel
0.018462 km/pixel
