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  2. Climate of Mars - Wikipedia

    en.wikipedia.org/wiki/Climate_of_Mars

    One such cyclonic storm was recently captured by the Hubble Space Telescope (pictured below). One of the major differences between Mars' and Earth's Hadley circulations is their speed [55] which is measured on an overturning timescale. The overturning timescale on Mars is about 100 Martian days while on Earth, it is over a year.

  3. Atmosphere of Mars - Wikipedia

    en.wikipedia.org/wiki/Atmosphere_of_Mars

    SO 2 has also been one of the proposed effective greenhouse gases in the early history of Mars. [48] [49] [50] However, other studies suggested that high solubility of SO 2, efficient formation of H 2 SO 4 aerosol and surface deposition prohibit the long-term build-up of SO 2 in the Martian atmosphere, and hence reduce the potential warming ...

  4. Martian lava tube - Wikipedia

    en.wikipedia.org/wiki/Martian_lava_tube

    The thin atmosphere allows Mars to radiate heat energy away more easily, so temperatures near the equator can get up to 21 °C (70 °F) during a summer day, and then drop down to −73 °C (−99 °F) at night. [10] Subsurface conditions on Mars are dramatically more benign than those on the surface, which lead researchers to believe that if ...

  5. Evidence of hot water that’s essential to life points to Mars ...

    www.aol.com/evidence-hot-water-essential-life...

    Researchers have uncovered what may be the oldest direct evidence of hot water activity on Mars, suggesting the red planet could have supported life billions of years ago.. Scientists at Australia ...

  6. 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 ...

  7. Mars Is About To Be at Its Brightest Since 2022—Here ... - AOL

    www.aol.com/lifestyle/mars-brightest-since-2022...

    Spotting Mars at opposition is easier than you might think because the planet will stand out due to its color and radiance. Instead of appearing a whitish yellow shade like the stars, it will be a ...

  8. Composition of Mars - Wikipedia

    en.wikipedia.org/wiki/Composition_of_Mars

    The Independence class showed some signs of clay (perhaps montmorillonite a member of the smectite group). Clays require fairly long term exposure to water to form. One type of soil, called Paso Robles, from the Columbia Hills, may be an evaporate deposit because it contains large amounts of sulfur, phosphorus, calcium, and iron. [78]

  9. Suddenly, Mars Is Spinning Faster. No One Knows Why. - AOL

    www.aol.com/suddenly-mars-spinning-faster-no...

    Researchers have discovered that Mars’s rotation is speeding up. Here's what's happening.