Image Credit: NASA/JPL/ASU
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Context image credit: NASA/JPL/MOLA
View on map Detailed information on this image is available at the
THEMIS Data Releases website.
Please see the THEMIS Data Citation Note for details on crediting THEMIS images.
Valley networks are a relatively common feature in the southern highlands of Mars. This THEMIS visible image contains several of these small channels. Some appear clustered near the smaller crater at the top of the image. There is still some debate over the origin of these enigmatic martian
landforms. Were they caused by overland flow after precipitation, underground sapping, or a combination of both?
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