Recurring Slope Lineae in Coprates Chasma
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.
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Details
NASA ID
PIA18119
Date Created
April 9, 2014
Center
JPL
Media Type
image
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