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Recurring Slope Lineae in Coprates Chasma
NASA/JPL-Caltech/Univ. of Arizona2014-04-09
NASA
Washington, DC, United States
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
- Title: Recurring Slope Lineae in Coprates Chasma
- Creator: NASA/JPL-Caltech/Univ. of Arizona
- Date Created: 2014-04-09
- Rights: JPL
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