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  2. Lyot (Martian crater) - Wikipedia

    en.wikipedia.org/wiki/Lyot_(Martian_crater)

    Images from Mars Reconnaissance Orbiter show valleys carved by rivers on the floor of Lyot crater. Scientists are excited because the rivers seem to have formed more recently than others on Mars; water could have flowed in them only 1.25 million years ago. The source of the water is believed to have been ice from nearby glaciers.

  3. 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.

  4. Chasma Boreale - Wikipedia

    en.wikipedia.org/wiki/Chasma_Boreale

    Chasma Boreale is a large canyon in Mars's north polar ice cap in the Mare Boreum quadrangle of Mars at 83° north latitude and 47.1° west longitude. It is about 560 km (350 mi) long and was named after a classical albedo feature name. [ 1 ]

  5. Lineated valley fill - Wikipedia

    en.wikipedia.org/wiki/Lineated_Valley_Fill

    Lineated valley fill (LVF), also called lineated floor deposit, is a feature of the floors of some channels on Mars, exhibiting ridges and grooves that seem to flow around obstacles. Shadow measurements show that at least some of the ridges are several metres high. LVF is believed to be ice-rich.

  6. 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 ...

  7. 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]

  8. The Best Skin Secret? Try Putting Ice on Your Face (Yes ... - AOL

    www.aol.com/lifestyle/best-skin-secret-try...

    From blemishes to facial sculpting, here are all the expert-approved ways you can use ice cubes for skin care. Skip to main content. Lifestyle. 24/7 help. For premium support please call: ...

  9. Mare Acidalium quadrangle - Wikipedia

    en.wikipedia.org/wiki/Mare_Acidalium_quadrangle

    Changes in Mars' orbit and tilt cause significant changes in the distribution of water ice from polar regions down to latitudes equivalent to Texas. During certain climate periods water vapor leaves polar ice and enters the atmosphere. The water comes back to ground at lower latitudes as deposits of frost or snow mixed generously with dust.