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  2. 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.

  3. 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 ...

  4. Mars habitability analogue environments on Earth - Wikipedia

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

    Mines on Earth give access to deep subsurface environments which turn out to be inhabited, and deep caves may possibly exist on Mars, although without the benefits of an atmosphere. Basaltic lava tubes. The only caves found so far on Mars are lava tubes. These are insulated to some extent from surface conditions and may retain ice also when ...

  5. Columbia Hills (Mars) - Wikipedia

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

    The Columbia Hills are a range of low hills inside Gusev crater on Mars. They were observed by the Mars Exploration Rover Spirit when it landed within the crater in 2004. They were promptly given an unofficial name by NASA since they were the most striking nearby feature on the surface. The hills lie approximately 3 kilometres (1.9 mi) away ...

  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. 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 ...

  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. 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.