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Recurring Slope Lineae in Coprates Chasma
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About this work
Recurring slope lineae RSL may be due to active seeps of water. These dark flows are abundant along the steep slopes of ancient bedrock in Coprates Chasma as seen in this image from NASA Mars Reconnaissance Orbiter.
NASA Image and Video Library’s own descriptionCredit lineRecurring Slope Lineae in Coprates Chasma. NASA/JPL, 2014-04-09. Public domain. ID: PIA18119.