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  2. Chloride-bearing deposits on Mars - Wikipedia

    en.wikipedia.org/wiki/Chloride-Bearing_Deposits...

    On Earth, chlorides are known to form through aqueous processes. [2] Similar processes are expected to be responsible for the formation of chloride deposits on Mars. The finding of these deposits is significant in that it provides further evidence for the presence of surface or subsurface water in ancient Mars. [3]

  3. Evidence of water on Mars found by Mars Reconnaissance ...

    en.wikipedia.org/wiki/Evidence_of_water_on_Mars...

    Using data from Mars Global Surveyor, Mars Odyssey and the Mars Reconnaissance Orbiter, scientists have found widespread deposits of chloride minerals. Some of these chloride deposits have been identified to be a mixture of anhydrous chloride salt and regional basaltic regolith. These are located in the southern highlands of Mars. [36]

  4. Chronology of discoveries of water on Mars - Wikipedia

    en.wikipedia.org/wiki/Chronology_of_discoveries...

    Evidence of water from chloride deposits in Phaethontis quadrangle. Picture from HiRISE. Rocks on Mars have been found to frequently occur as layers, called strata, in many different places. Columbus Crater is one of many craters that contain layers. Rock can form layers in a variety of ways. Volcanoes, wind, or water can produce layers. [83]

  5. Composition of Mars - Wikipedia

    en.wikipedia.org/wiki/Composition_of_Mars

    Mars is differentiated, which—for a terrestrial planet—implies that it has a central core made up of high density matter (mainly metallic iron and nickel) surrounded by a less dense, silicate mantle and crust. [4] Like Earth, Mars appears to have a molten iron core, or at least a molten outer core. [5]

  6. Terra Sirenum - Wikipedia

    en.wikipedia.org/wiki/Terra_Sirenum

    Based on chloride deposits and hydrated phyllosilicates, Alfonso Davila and others believe there is an ancient lakebed in Terra Sirenum that had an area of 30,000 km 2 and was 200 meters deep. Other evidence that supports this lake are normal and inverted channels like ones found in the Atacama Desert .

  7. Martian regolith - Wikipedia

    en.wikipedia.org/wiki/Martian_regolith

    Curiosity 's view of Martian soil and boulders after crossing the "Dingo Gap" sand dune (February 9, 2014; image transformed to Earth-like atmospheric view, original image). Martian regolith is the fine blanket of unconsolidated, loose, heterogeneous superficial deposits covering the surface of Mars.

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  9. Lakes on Mars - Wikipedia

    en.wikipedia.org/wiki/Lakes_on_Mars

    So, samples of material from the Eridania may give us insight into the environment of the early Earth. Chloride deposits were found where a shoreline existed. They were deposited as water evaporated from the sea. These chloride deposits are thought to be thin (less than 30 meters), because some craters do not display the chemical in their ejecta.