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  2. Composition of Mars - Wikipedia

    en.wikipedia.org/wiki/Composition_of_Mars

    It is supposed that billions of years ago Mars was much warmer and wetter. At that time, carbonates would have formed from water and the carbon dioxide-rich atmosphere. Later the deposits of carbonate would have been buried. The double impact has now exposed the minerals. Earth has vast carbonate deposits in the form of limestone. [67]

  3. Tectonics of Mars - Wikipedia

    en.wikipedia.org/wiki/Tectonics_of_Mars

    Topographic map of Mars showing the highland-lowland boundary marked in yellow, and the Tharsis rise outlined in red (USGS, 2014).[1]Like the Earth, the crustal properties and structure of the surface of Mars are thought to have evolved through time; in other words, as on Earth, tectonic processes have shaped the planet.

  4. Water on Mars - Wikipedia

    en.wikipedia.org/wiki/Water_on_Mars

    Rocks on Mars have been found to frequently occur as layers, called strata, in many different places. [380] Layers form by various ways, including volcanoes, wind, or water. [381] Light-toned rocks on Mars have been associated with hydrated minerals like sulfates and clay. [382] Layers on the west slope of Asimov Crater. Location is Noachis ...

  5. Geology of Mars - Wikipedia

    en.wikipedia.org/wiki/Geology_of_Mars

    Mars also has an atmosphere that plays a role in ejecta emplacement and subsequent erosion. Moreover, Mars has a rate of volcanic and tectonic activity low enough that ancient, eroded craters are still preserved, yet high enough to have resurfaced large areas, producing a diverse range of crater populations of widely differing ages.

  6. Evidence found that supports current existence of liquid ...

    www.aol.com/news/2015-04-14-evidence-found-that...

    The soil's composition is key in allowing for such promise as it shows high quantities of perchlorate salts, which would enable water to exist in a liquid form despite the Red Planet's punishing ...

  7. Atmosphere of Mars - Wikipedia

    en.wikipedia.org/wiki/Atmosphere_of_Mars

    The atmosphere of Mars is the layer of gases surrounding Mars.It is primarily composed of carbon dioxide (95%), molecular nitrogen (2.85%), and argon (2%). [3] It also contains trace levels of water vapor, oxygen, carbon monoxide, hydrogen, and noble gases.

  8. Mars May Have Far More Water Than We Thought - AOL

    www.aol.com/mars-may-far-more-water-195315919.html

    The deepest hole ever drilled on Earth is the Kola superdeep borehole in northwest Russia, which extends down about 12 km. That may be deep enough to touch the Red Planet water, but nobody ...

  9. Groundwater on Mars - Wikipedia

    en.wikipedia.org/wiki/Groundwater_on_Mars

    Sometimes water flows through Earth's aquifers, and then evaporates at the surface just as is hypothesized for Mars. One location this occurs on Earth is the Great Artesian Basin of Australia. [30] On Earth the hardness of many sedimentary rocks, like sandstone, is largely due to the cement that was put in place as water passed through.