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  2. 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 ...

  3. Scientists explore how to improve crop yields - on Mars - AOL

    www.aol.com/news/scientists-explore-improve-crop...

    The crops were grown in simulated Martian regolith - soil with no organic matter - developed by NASA researchers that is a near-perfect physical and chemical match to real Martian soil.

  4. Atmosphere of Mars - Wikipedia

    en.wikipedia.org/wiki/Atmosphere_of_Mars

    The average surface emission temperature of Mars is just 215 K (−58 °C; −73 °F), which is comparable to inland Antarctica. [ 2 ] [ 4 ] Although Mars' atmosphere consists primarily of carbon dioxide, the greenhouse effect in the Martian atmosphere is much weaker than Earth's: 5 °C (9.0 °F) on Mars, versus 33 °C (59 °F) on Earth due to ...

  5. Martian surface - Wikipedia

    en.wikipedia.org/wiki/Martian_surface

    The study of surface characteristics (or surface properties and processes [1]) is a broad category of Mars science that examines the nature of the materials making up the Martian surface. The study evolved from telescopic and remote-sensing techniques developed by astronomers to study planetary surfaces.

  6. Scientists propose warming up Mars by using heat-trapping ...

    www.aol.com/news/scientists-propose-warming-mars...

    The median Martian surface temperature is about minus-85 degrees Fahrenheit (minus-65 degrees Celsius). With its tenuous atmosphere, solar heat on the Martian surface readily escapes into space.

  7. Martian regolith - Wikipedia

    en.wikipedia.org/wiki/Martian_regolith

    However, each new lander has confirmed their presence in the regoltih locally and the Mars Odyssey orbiter confirmed they are spread globally across the entire surface of the planet. [4] "Sutton Inlier" soil on Mars – target of ChemCam's laser – Curiosity rover (May 11, 2013)

  8. Heat Flow and Physical Properties Package - Wikipedia

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

    The mole is first allowed to cool down for two days, then it is heated to about 10 °C (50 °F) over 24 hours. Temperature sensors within the tether measure how rapidly this happens, which tells scientists the thermal conductivity of the soil. [22] Together, these measurements yield the rate of heat flowing from the interior.

  9. Scientific information from the Mars Exploration Rover mission

    en.wikipedia.org/wiki/Scientific_information...

    Temperature profile taken by MGS over the MER-B site During a press conference on March 11, 2004, mission scientists presented the first temperature profile of the martian atmosphere ever measured. It was obtained by combining data taken from the Opportunity Mini-TES infrared spectrometer with data from the TES instrument on board the Mars ...