Ice cliffs spotted on Mars

Fora ASTRO-FORUM NYT FRA VIDENSKABEN Ice cliffs spotted on Mars

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    Bjarne
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      • Super Nova

      Ice cliffs spotted on Mars

      What Dundas saw that day, and subsequently found at seven other sites, are steep cliffs, up to 100 meters tall, that expose what appears to be nearly pure ice. The discovery points to large stores of underground ice buried only a meter or two below the surface at surprisingly low martian latitudes. “This kind of ice is more widespread than previously thought,” says Dundas, who, with his co-authors, describes the cliffs this week in Science. Each cliff seems to be the naked face of a glacier, tantalizing scientists with the promise of a layer-cake record of past martian climates and space enthusiasts with a potential resource for future human bases.

       

      #315683

      Bjarne
      Moderator
        • Super Nova

        Exposed subsurface ice sheets in the Martian mid-latitudes

        Some locations on Mars are known to have water ice just below the surface, but how much has remained unclear. Dundas et al. used data from two orbiting spacecraft to examine eight locations where erosion has occurred. This revealed cliffs composed mostly of water ice, which is slowly sublimating as it is exposed to the atmosphere. The ice sheets extend from just below the surface to a depth of 100 meters or more and appear to contain distinct layers, which could preserve a record of Mars’ past climate. They might even be a useful source of water for future human exploration of the red planet.

        Abstract
        Thick deposits cover broad regions of the Martian mid-latitudes with a smooth mantle; erosion in these regions creates scarps that expose the internal structure of the mantle. We investigated eight of these locations and found that they expose deposits of water ice that can be >100 meters thick, extending downward from depths as shallow as 1 to 2 meters below the surface. The scarps are actively retreating because of sublimation of the exposed water ice. The ice deposits likely originated as snowfall during Mars’ high-obliquity periods and have now compacted into massive, fractured, and layered ice. We expect the vertical structure of Martian ice-rich deposits to preserve a record of ice deposition and past climate.

         

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        nightsky
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          • Neutron star
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