Recurring Slope Lineae on Hale Crater

Recurring Slope Lineae on Hale Crater
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Dark, narrow streaks on Martian slopes such as these at Hale Crater are inferred to have been formed by seasonal flow of water on contemporary Mars. Detection of hydrated salts at the streaks supports that interpretation. The features are called Recurring Slope Lineae

ID #:

PIA19916

Source:

NASA/JPL-Caltech/Arizona State University

Copyright/Owner:

NASA/JPL-Caltech/University of Arizona

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