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  2. Mars ocean theory - Wikipedia

    en.wikipedia.org/wiki/Mars_ocean_theory

    An artist's impression of ancient Mars and its oceans based on geological data The blue region of low topography in the Martian northern hemisphere is hypothesized to be the site of a primordial ocean of liquid water. [1] The Mars ocean theory states that nearly a third of the surface of Mars was covered by an ocean of liquid water early in the ...

  3. Climate of Mars - Wikipedia

    en.wikipedia.org/wiki/Climate_of_Mars

    Orbital measurements showed that this dust storm reduced the average temperature of the surface and raised the temperature of the atmosphere of Mars by 30 K. [31] The low density of the Martian atmosphere means that winds of 18 to 22 m/s (65 to 79 km/h) are needed to lift dust from the surface, but since Mars is so dry, the dust can stay in the ...

  4. Valles Marineris - Wikipedia

    en.wikipedia.org/wiki/Valles_Marineris

    Thermokarst activity may have contributed, but erosion by water is a problematic mechanism because liquid water cannot exist in most current Martian surface conditions, which typically experience about 1% of Earth's atmospheric pressure and a temperature range of 148 K (−125 °C; −193 °F) to 310 K (37 °C; 98 °F).

  5. Water on terrestrial planets of the Solar System - Wikipedia

    en.wikipedia.org/wiki/Water_on_terrestrial...

    The current Venusian atmosphere has only ~200 mg/kg H 2 O(g) in its atmosphere and the pressure and temperature regime makes water unstable on its surface. Nevertheless, assuming that early Venus's H 2 O had a ratio between deuterium (heavy hydrogen, 2H) and hydrogen (1H) similar to Earth's Vienna Standard Mean Ocean Water of 1.6×10 −4, [7] the current D/H ratio in the Venusian atmosphere ...

  6. Mars may be around 140 million miles away from Earth, but the red planet is influencing our oceans, according to new research. Mars could be driving ‘giant whirlpools’ in the Earth’s deep ...

  7. Martian dichotomy - Wikipedia

    en.wikipedia.org/wiki/Martian_dichotomy

    The most conspicuous feature of Mars is a sharp contrast, known as the Martian dichotomy, between the Southern and the Northern hemispheres.The two hemispheres' geography differ in elevation by 1 to 3 km.

  8. New Mars study suggests an ocean's worth of water may be ...

    www.aol.com/news/mars-study-suggests-oceans...

    Mars may be drenched beneath its surface, with enough water hiding in the cracks of underground rocks to form a global ocean, new research suggests. The findings released Monday are based on ...

  9. Underground reservoir on Mars could fill oceans on the planet ...

    www.aol.com/news/evidence-suggests-may-reservoir...

    A new analysis of data collected by NASA’s InSight mission suggests there may be enough water beneath the surface of Mars to cover the planet. Underground reservoir on Mars could fill oceans on ...