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  2. Caves of Mars Project - Wikipedia

    en.wikipedia.org/wiki/Caves_of_Mars_Project

    Caves of Mars Project. THEMIS image of probable cave entrances on Arsia Mons. The pits have been informally named (A) Dena, (B) Chloe, (C) Wendy, (D) Annie, (E) Abby (left) and Nikki, and (F) Jeanne. The Caves of Mars Project was an early 2000s program funded through Phase II [clarification needed] by the NASA Institute for Advanced Concepts [1 ...

  3. Martian lava tube - Wikipedia

    en.wikipedia.org/wiki/Martian_lava_tube

    Gravity on Mars is about 38% that of Earth, [8] allowing Martian lava tubes to be much larger in comparison. [9] Lava tubes represent prime locations for direct observation of pristine bedrock where keys to the geological, paleohydrological, and possible biological history of Mars could be found.

  4. Arsia Mons - Wikipedia

    en.wikipedia.org/wiki/Arsia_Mons

    Arsia Mons is a shield volcano with a relatively low slope and a massive caldera at its summit. The southernmost of the three Tharsis Montes volcanoes, it is the only major Tharsis volcano south of the equator. [2] Topographic map of Arsia Mons. The volcano is 435 kilometres (270 mi) in diameter, almost 20 kilometres (12 mi) high (more than 9 ...

  5. File:Complete map of 1,000+ cave-entrances on Mars.png ...

    en.wikipedia.org/wiki/File:Complete_map_of_1,000...

    The Mars Global Cave Candidate Catalog (MGC3) provides latitude and longitude coordinates, feature type, priority (confidence) rating, and a brief comment about each candidate. Types of cave entrances identified in the catalog include lava tube skylights, deep fractures, Atypical Pit Craters (APCs), and other void spaces in karst-similar terrains.

  6. Valles Marineris - Wikipedia

    en.wikipedia.org/wiki/Valles_Marineris

    Valles Marineris (/ ˈvælɪs mærɪˈnɛərɪs /; [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] At more than 4,000 km (2,500 mi) long, 200 km (120 mi) wide and up to 7 km (23,000 ft) deep, [3][4 ...

  7. Mars habitability analogue environments on Earth - Wikipedia

    en.wikipedia.org/wiki/Mars_habitability_analogue...

    Ice caves, or ice preserved under the surface in cave systems protected from the surface conditions, may exist on Mars. The ice caves near the summit of Mount Erebus in Antarctica, are associated with fumaroles in a polar alpine environments starved in organics and with oxygenated hydrothermal circulation in highly reducing host rock.

  8. Geology of Mars - Wikipedia

    en.wikipedia.org/wiki/Geology_of_Mars

    The geology of Mars is the scientific study of the surface, crust, and interior of the planet Mars. It emphasizes the composition, structure, history, and physical processes that shape the planet. It is analogous to the field of terrestrial geology. In planetary science, the term geology is used in its broadest sense to mean the study of the ...

  9. List of caves - Wikipedia

    en.wikipedia.org/wiki/List_of_caves

    Possible cave entrances on Mars. The pits have been informally named (A) Dena, (B) Chloe, (C) Wendy, (D) Annie, (E) Abby (left) and Nikki, and (F) Jeanne. As of 2007 [update] seven putative cave entrances have been identified in satellite imagery of the planet Mars , all so far located on the flanks of Arsia Mons . [ 53 ]