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  2. Climate of Mars - Wikipedia

    en.wikipedia.org/wiki/Climate_of_Mars

    Colaprete et al. conducted simulations with the Mars General Circulation Model which show that the local climate around the Martian south pole may currently be in an unstable period. The simulated instability is rooted in the geography of the region, leading the authors to speculate that the sublimation of the polar ice is a local phenomenon ...

  3. 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 ...

  4. Mars regional atmospheric modeling system - Wikipedia

    en.wikipedia.org/wiki/Mars_regional_atmospheric...

    The Mars Regional Atmospheric Modeling System (MRAMS) is a computer program that simulates the circulations of the Martian atmosphere at regional and local scales. [1] MRAMS, developed by Scot Rafkin and Timothy Michaels, is derived from the Regional Atmospheric Modeling System (RAMS) developed by William R. Cotton and Roger A. Pielke to study atmospheric circulations on the Earth.

  5. Category:Climate of Mars - Wikipedia

    en.wikipedia.org/wiki/Category:Climate_of_Mars

    Climate of Mars; 0–9. 2018 Mars global dust storm; M. Mars Climate Orbiter; Mars general circulation model; T. Temperature and Winds for InSight; Terraforming of Mars

  6. File:PIA22737-Mars-2018DustStorm-MCS-MRO-Animation-20181030 ...

    en.wikipedia.org/wiki/File:PIA22737-Mars-2018...

    The animation shows the optical depth tau-- a measure of how much light is being blocked by atmospheric dust as measured by the Mars Climate Sounder instrument onboard NASA's Mars Reconnaissance Orbiter. NASA's Opportunity rover is marked with a RED DOT. The dust is mapped to two opposite hemispheres of Mars, giving a view of the full globe.

  7. Heat Flow and Physical Properties Package - Wikipedia

    en.wikipedia.org/wiki/Heat_Flow_and_Physical...

    The mole is described as a "self-hammering nail" and was designed to burrow below the Martian surface while trailing a tether with embedded heaters and temperature sensors. The goal was to measure the thermal properties of Mars' interior, and thus reveal unique information about the planet's geologic history. [4]

  8. 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 ...

  9. Mars Observer - Wikipedia

    en.wikipedia.org/wiki/Mars_Observer

    The Mars Observer spacecraft, also known as the Mars Geoscience/Climatology Orbiter, was a robotic space probe launched by NASA on September 25, 1992, to study the Martian surface, atmosphere, climate and magnetic field.