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  2. Atmosphere of Mars - Wikipedia

    en.wikipedia.org/wiki/Atmosphere_of_Mars

    The surface pressure measured by Mars rovers showed clear signals of thermal tides, although the variation also depends on the shape of the planet's surface and the amount of suspended dust in the atmosphere. [169] The atmospheric waves can also travel vertically and affect the temperature and water-ice content in the middle atmosphere of Mars ...

  3. Areography - Wikipedia

    en.wikipedia.org/wiki/Areography

    The datum for Mars was defined initially in terms of a constant atmospheric pressure. From the Mariner 9 mission up until 2001, this was chosen as 610.5 Pa (6.105 mbar), on the basis that below this pressure liquid water can never be stable (i.e., the triple point of water is at this pressure).

  4. Aeolis quadrangle - Wikipedia

    en.wikipedia.org/wiki/Aeolis_quadrangle

    Download as PDF; Printable version; ... (Mars Chart-23). [1] ... scientists found that the annual average concentration of methane in Mars' atmosphere is 0.41 ppb ...

  5. Hellas Planitia - Wikipedia

    en.wikipedia.org/wiki/Hellas_Planitia

    The crater's depth of 7,152 m (23,465 ft) [1] below the topographic datum of Mars explains the atmospheric pressure at the bottom: 12.4 mbar (1240 Pa or 0.18 psi) during winter, when the air is coldest and reaches its highest density.

  6. Casius quadrangle - Wikipedia

    en.wikipedia.org/wiki/Casius_quadrangle

    Studies have shown that when the tilt of Mars reaches 45 degrees from its current 25 degrees, ice is no longer stable at the poles. [24] Furthermore, at this high tilt, stores of solid carbon dioxide (dry ice) sublimate, thereby increasing the atmospheric pressure. This increased pressure allows more dust to be held in the atmosphere.

  7. Hellas quadrangle - Wikipedia

    en.wikipedia.org/wiki/Hellas_quadrangle

    The Hellas quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program. The Hellas quadrangle is also referred to as MC-28 (Mars Chart-28). [1] The Hellas quadrangle covers the area from 240° to 300° west longitude and 30° to 65° south latitude on the planet Mars.

  8. Climate of Mars - Wikipedia

    en.wikipedia.org/wiki/Climate_of_Mars

    One effect of this is that Mars' atmosphere can react much more quickly to a given energy input than Earth's atmosphere. [51] As a consequence, Mars is subject to strong thermal tides produced by solar heating rather than a gravitational influence. These tides can be significant, being up to 10% of the total atmospheric pressure (typically ...

  9. Arabia quadrangle - Wikipedia

    en.wikipedia.org/wiki/Arabia_quadrangle

    At that time, Mars is 40% closer to the Sun. The orbit of Mars is much more elliptical then the Earth's. That is the difference between the farthest point from the Sun and the closest point to the Sun is very great for Mars, but only a slight amount for the Earth. Also, every few years, the entire planet is engulfed in global dust storms.