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An artist's impression of what ancient Mars may have looked like, based on geological data
An artist's impression of what ancient Mars may have looked like, based on geological data
Global
Global
Planar
Planar
Martian terrain
Martian terrain
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Curiosity's view of Martian soil and boulders after crossing the "Dingo Gap" sand dune (February 9, 2014; image transformed to Earth-like atmospheric
Curiosity's view of Martian soil and boulders after crossing the "Dingo Gap" sand dune (February 9, 2014; image transformed to Earth-like atmospheric view, original image).
Comparison of Soils on Mars - Samples by Curiosity, Opportunity, and Spirit rovers (December 3, 2012). (SiO2 and FeO are divided by 10, and Ni, Zn, an
Comparison of Soils on Mars - Samples by Curiosity, Opportunity, and Spirit rovers (December 3, 2012). (SiO2 and FeO are divided by 10, and Ni, Zn, and Br are multiplied by 100.)
First X-ray diffraction view of Martian soil - CheMin analysis reveals feldspar, pyroxenes, olivine and more (Curiosity rover at "Rocknest", October 1
First X-ray diffraction view of Martian soil - CheMin analysis reveals feldspar, pyroxenes, olivine and more (Curiosity rover at "Rocknest", October 17, 2012).
Mars without a dust storm in June 2001 (on left) and with a global dust storm in July 2001 (on right), as seen by Mars Global Surveyor
Mars without a dust storm in June 2001 (on left) and with a global dust storm in July 2001 (on right), as seen by Mars Global Surveyor