Seasonal Flows in Palikir Crater

NASA/JPL-Caltech/Univ. of Arizona2013-05-15

NASA
Washington, DC, United States

Seasonal flows on warm Martian slopes may be caused by the flow of salty water on Mars, active today when the surface is warm above the freezing point of the solution. This observation is from NASA Mars Reconnaissance Orbiter.

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Details

Title: Seasonal Flows in Palikir Crater
Creator: NASA/JPL-Caltech/Univ. of Arizona
Date Created: 2013-05-15
Rights: JPL

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