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  2. Climate of Mars - Wikipedia

    en.wikipedia.org/wiki/Climate_of_Mars

    While Mars's climate has similarities to Earth's, including periodic ice ages, there are also important differences, such as much lower thermal inertia. Mars' atmosphere has a scale height of approximately 11 km (36,000 ft), 60% greater than that on Earth. The climate is of considerable relevance to the question of whether life is or ever has ...

  3. Category:Climate of Mars - Wikipedia

    en.wikipedia.org/wiki/Category:Climate_of_Mars

    Mars Climate Orbiter; Mars general circulation model; T. Temperature and Winds for InSight; Terraforming of Mars This page was last edited on 19 April 2024, at 23:07 ...

  4. Mars general circulation model - Wikipedia

    en.wikipedia.org/wiki/Mars_General_Circulation_Model

    Mars climate simulation models date as far back as the Viking missions to Mars. Most Mars climate simulation models were written by individual researchers that were never reused or open-sourced. By the 1990s the need for a unified model codebase came into being, due to the general impact of the internet on climate modelling and research. This ...

  5. Martian polar ice caps - Wikipedia

    en.wikipedia.org/wiki/Martian_polar_ice_caps

    1995 photo of Mars showing approximate size of the polar caps. The planet Mars has two permanent polar ice caps of water ice and some dry ice (frozen carbon dioxide, CO 2).Above kilometer-thick layers of water ice permafrost, slabs of dry ice are deposited during a pole's winter, [1] [2] lying in continuous darkness, causing 25–30% of the atmosphere being deposited annually at either of the ...

  6. Argyre quadrangle - Wikipedia

    en.wikipedia.org/wiki/Argyre_quadrangle

    The climate of Mars may have been such in the past that water ran on its surface. It has been known for some time that Mars undergoes many large changes in its tilt or obliquity because its two small moons lack the gravity to stabilize it, as the Moon stabilizes Earth; at times the tilt of Mars has even been greater than 80 degrees [48] [49]

  7. Category:Climates of the Solar System - Wikipedia

    en.wikipedia.org/wiki/Category:Climates_of_the...

    Climate of Mars; P. Climate of Pluto; T. Climate of Titan; Climate of Triton; U. Climate of Uranus This page was last edited on 19 April 2024, at 23:03 ...

  8. Phaethontis quadrangle - Wikipedia

    en.wikipedia.org/wiki/Phaethontis_quadrangle

    Most dunes on Mars are black because of the weathering of the volcanic rock basalt. [79] [80] Black sand can be found on Earth on Hawaii and on some tropical South Pacific islands. [81] Sand is common on Mars due to the old age of the surface that has allowed rocks to erode into sand. Dunes on Mars have been observed to move many meters.

  9. Candor Chasma - Wikipedia

    en.wikipedia.org/wiki/Candor_Chasma

    The climate of Mars may have been such in the past that water ran on its surface. It has been known for some time that Mars undergoes many large changes in its tilt or obliquity because its two small moons lack the gravity to stabilize it, as the Moon stabilizes Earth; at times the tilt of Mars has even been greater than 80 degrees [3] [4]