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  2. History of Mars observation - Wikipedia

    en.wikipedia.org/wiki/History_of_Mars_observation

    These observations were primarily made during the time intervals when the planet was located in opposition to the Sun, at which points Mars made its closest approaches to the Earth. Better telescopes developed early in the 19th century allowed permanent Martian albedo features to be mapped in detail.

  3. Mars - Wikipedia

    en.wikipedia.org/wiki/Mars

    Mars is the fourth planet from the Sun.The surface of Mars is orange-red because it is covered in iron(III) oxide dust, giving it the nickname "the Red Planet". [22] [23] Mars is among the brightest objects in Earth's sky, and its high-contrast albedo features have made it a common subject for telescope viewing.

  4. Valles Marineris - Wikipedia

    en.wikipedia.org/wiki/Valles_Marineris

    Valles Marineris (/ ˈ v æ l ɪ s m ær ɪ ˈ n ɛər ɪ s /; [1] Latin for Mariner Valleys, named after the Mariner 9 Mars orbiter of 1971–72 which discovered it) is a system of canyons that runs along the Martian surface east of the Tharsis region. [2]

  5. Geological history of Mars - Wikipedia

    en.wikipedia.org/wiki/Geological_history_of_Mars

    Methods dating back to 17th-century techniques developed by Nicholas Steno, including the so-called law of superposition and stratigraphy, used to estimate the geological histories of Earth and the Moon, are being actively applied to the data available from several Martian observational and measurement resources.

  6. Cydonia (Mars) - Wikipedia

    en.wikipedia.org/wiki/Cydonia_(Mars)

    Small part of the Cydonia region, taken by the Viking 1 orbiter and released by NASA/JPL on July 25, 1976. Cydonia (/ s ɪ ˈ d oʊ n i ə /, / s aɪ ˈ d oʊ n i ə /) is a region on the planet Mars that has attracted both scientific [1] and popular interest.

  7. Geology of Mars - Wikipedia

    en.wikipedia.org/wiki/Geology_of_Mars

    The northern part is an enormous topographic depression. About one-third of the surface (mostly in the northern hemisphere) lies 3–6 km lower in elevation than the southern two-thirds. This is a first-order relief feature on par with the elevation difference between Earth's continents and ocean basins. [12]

  8. Mars rover data confirms ancient lake sediments on red planet

    www.aol.com/news/mars-rover-data-confirms...

    LOS ANGELES (Reuters) -NASA's rover Perseverance has gathered data confirming the existence of ancient lake sediments deposited by water that once filled a giant basin on Mars called Jerezo Crater ...

  9. Mars ocean theory - Wikipedia

    en.wikipedia.org/wiki/Mars_ocean_theory

    However, early in its history Mars may have had conditions more conducive to retaining liquid water at the surface. Mars without a dust storm in June 2001 (on left) and with a global dust storm in July 2001 (on right), as seen by Mars Global Surveyor. Early Mars had a carbon dioxide atmosphere similar in thickness to present-day Earth (1000 hPa ...