Flowing Water On Mars

  • Released Thursday, March 3, 2016

Mars is drier than the most arid deserts on Earth, yet scientists now know it harbors liquid water just beneath its surface. Images from the HiRISE camera aboard NASA’s Mars Reconnaissance Orbiter spacecraft reveal seeps of moisture sliding down steep Martian cliffs that come and go with the seasons. These dark streaks, called recurring slope lineae, appear on sun-facing hillsides, often inside craters. They usually advance slowly, over days or weeks, before fading away at summer’s end. Dissolved salts lower the water's freezing point, perhaps explaining why flows are seen even at low temperatures. The water doesn’t collect into streams or lakes like it might on Earth. Instead, it evaporates into the dry Martian air, leaving behind telltale traces of salt. Using instruments aboard the spacecraft, scientists detected those salts on the same cliffs where they had spied seasonal flows, confirming their aqueous nature. Watch the video to learn more.

Mars’ flows extend downslope over time. The above images, captured about two weeks apart, show the growth of flows seen near the equator.

Mars’ flows extend downslope over time. The above images, captured about two weeks apart, show the growth of flows seen near the equator.

During warm seasons, seeping moisture carves lines (shown above) into the steep walls of Juventae Chasma, a giant canyon on Mars.

During warm seasons, seeping moisture carves lines (shown above) into the steep walls of Juventae Chasma, a giant canyon on Mars.

The flows in this image begin where bedrock meets sand. As the water evaporates, it leaves behind traces of salt that can be detected from orbit.

The flows in this image begin where bedrock meets sand. As the water evaporates, it leaves behind traces of salt that can be detected from orbit.



Credits

Please give credit for this item to:
NASA's Goddard Space Flight Center
Video and images courtesy of NASA/JPL/University of Arizona

Release date

This page was originally published on Thursday, March 3, 2016.
This page was last updated on Wednesday, May 3, 2023 at 1:48 PM EDT.