Elysium Mons
Image Credit: NASA/JPL/ASU
About this image
This VIS image shows part of the eastern flank of Elysium Mons. The small channels were likely created due to the flow of lava, rather than water.
Please see the THEMIS Data Citation Note for details on crediting THEMIS images.
Context
Image ID:
V44248005 (View data in Mars Image Explorer)
24.2191
151.509
44248
2011-12-05 16:06
Mon, 2012-01-02
VIS
1024 pixels (20 km)
3648 pixels (69 km)
0.019163 km/pixel
0.020176 km/pixel
