Image Credit: NASA/JPL/ASU
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Context image credit: NASA/JPL/MOLA
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Please see the THEMIS Data Citation Note for details on crediting THEMIS images.
The fluidized impact crater ejecta and flat crater floors observed in this THEMIS image suggest near surface volatiles once played an important role in modifying the martian surface. Gullies observed in crater walls could possibly point to more recent volatile-rock interactions.
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