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  2. Martian polar ice caps - Wikipedia

    en.wikipedia.org/wiki/Martian_polar_ice_caps

    1995 photo of Mars showing approximate size of the polar caps. The planet Mars has two permanent polar ice caps of water ice and some dry ice (frozen carbon dioxide, CO 2).Above kilometer-thick layers of water ice permafrost, slabs of dry ice are deposited during a pole's winter, [1] [2] lying in continuous darkness, causing 25–30% of the atmosphere being deposited annually at either of the ...

  3. Medusae Fossae Formation - Wikipedia

    en.wikipedia.org/wiki/Medusae_Fossae_Formation

    In some places, the formation appears as a smooth and gently undulating surface, while in others it is wind-sculpted into ridges and grooves. [1] Radar imaging has suggested that the region may contain either extremely porous rock (for example volcanic ash) or deep layers of glacier-like ice deposits amounting to about the same quantity as is stored in Mars' south polar cap.

  4. Common surface features of Mars - Wikipedia

    en.wikipedia.org/.../Common_surface_features_of_Mars

    Dry ice behaves in a similar fashion on the Earth. On Mars sublimation has been observed when the Phoenix lander uncovered chunks of ice that disappeared in a few days. [59] [60] In addition, HiRISE has seen fresh craters with ice at the bottom. After a time, HiRISE saw the ice deposit disappear. [61]

  5. NASA spacecraft spots stunning flow of ice on Mars - AOL

    www.aol.com/news/nasa-spacecraft-spots-stunning...

    Mars, a world that once gushed with water, is today 1,000 times drier than Earth's driest desert. Yet some ice still flows, slowly, on the Martian ground.NASA's Mars-orbiting satellite, the Mars ...

  6. Mare Acidalium quadrangle - Wikipedia

    en.wikipedia.org/wiki/Mare_Acidalium_quadrangle

    The "Face on Mars", of great interest to the general public, is located near 40.8 degrees north and 9.6 degrees west, in an area called Cydonia. When Mars Global Surveyor examined it with high resolution, the face turned out to just be an eroded mesa. [8] Mare Acidalium contains the Kasei Valles system of canyons.

  7. Martian surface - Wikipedia

    en.wikipedia.org/wiki/Martian_surface

    Ground-penetrating radar instruments on the Mars Express orbiter and the Mars Reconnaissance Orbiter are currently providing stunning echo-return data on subsurface materials and structures to depths of up to 5 km. Results have shown that the polar layered deposits are composed of almost pure ice, with no more than 10% dust by volume [23] and ...

  8. Glaciers on Mars - Wikipedia

    en.wikipedia.org/wiki/Glaciers_on_Mars

    [32] [33] Ice was found both in the southern hemisphere [34] and in the northern hemisphere. [35] Researchers at the Niels Bohr Institute combined radar observations with ice flow modelling to say that ice in all of the Martian glaciers is equivalent to what could cover the entire surface of Mars with 1.1 meters of ice.

  9. Lobate debris apron - Wikipedia

    en.wikipedia.org/wiki/Lobate_debris_apron

    The floors of some channels show ridges and grooves that seem to flow around obstacles; these features are called lineated floor deposits or lineated valley fill (LVF). Like lobate debris aprons, they are believed to be ice-rich. Some glaciers on the Earth show such features. It has been suggested that lineated floor deposits began as LDAs.