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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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