Patapsco Vallis

Scaled Image

Image Credit: NASA/JPL/ASU

About this image

This VIS image shows a section of Patapsco Vallis, a channel located east of Elysium Mons. 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: 
V81192012 (View data in Mars Image Explorer)
23.6547
153.166
81192
2020-04-03 16:07
Tue, 2020-06-02
VIS
1024 pixels (19 km)
3648 pixels (67 km)
0.018637 km/pixel
0.0186228 km/pixel

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