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Mars Gullies Produced by Dry Granular Debris and Not by Recent Water Flow

March 01, 2008 | Ian O'Neill | Comments 0

Simulations of dry debris flow and water flow when compared with HiRISE observations (credit: Jon Pelletier, University of Arizona)
The High Resolution Imaging Science Experiment (HiRISE) on board NASA’s Mars Reconnaissance Orbiter (MRO) observed what appeared to be fresh gullies formed by a rapid release of water on the Martian surface in 2006. However, new computer models simulating the creation of gullies on the surface of Mars suggest that they are in fact created by the flow of dry debris (i.e. landslides) and not by the flow of water. A blow for the microbial life hunters and a huge blow for mission planners looking for easy sources of water for manned missions…
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