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  2. Composition of Mars - Wikipedia

    en.wikipedia.org/wiki/Composition_of_Mars

    In the summer of 2008, the TEGA and WCL experiments on the 2007 Phoenix Mars lander found between 3–5wt% (percent by weight) calcite (CaCO 3) and an alkaline soil. [65] In 2010, analyses by the Mars Exploration Rover Spirit identified outcrops rich in magnesium-iron carbonate (16–34 wt%) in the Columbia Hills of Gusev crater. The magnesium ...

  3. Geology of Mars - Wikipedia

    en.wikipedia.org/wiki/Geology_of_Mars

    Generalised geological map of Mars [1] Mars as seen by the Hubble Space Telescope. The geology of Mars is the scientific study of the surface, crust, and interior of the planet Mars. It emphasizes the composition, structure, history, and physical processes that shape the planet. It is analogous to the field of terrestrial geology.

  4. Curiosity rover discovers peculiar metal sphere on Mars - AOL

    www.aol.com/news/2016-11-02-curiosity-rover...

    Part of the reason is that many contain iron which tends to make them more durable and resistant to erosion. This isn't the first strange thing found on Mars and it certainly won't be the last ...

  5. Scientific information from the Mars Exploration Rover mission

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

    Also, MB found that much of the iron in Paso Robles soil was of the oxidized, Fe +++ form, which would happen if water had been present. [13] Towards the middle of the six-year mission (a mission that was supposed to last only 90 days), large amounts of pure silica were found in the soil. The silica could have come from the interaction of soil ...

  6. Geology of solar terrestrial planets - Wikipedia

    en.wikipedia.org/wiki/Geology_of_solar...

    [31] [32] Mars has twice as much iron oxide in its outer layer as Earth does, despite their supposed similar origin. It is thought that Earth, being hotter, transported much of the iron downwards in the 1,800 kilometres (1,118 mi) deep, 3,200 °C (5,792 °F ), lava seas of the early planet, while Mars, with a lower lava temperature of 2,200 °C ...

  7. Martian spherules - Wikipedia

    en.wikipedia.org/wiki/Martian_spherules

    The stainless steel column in the foreground is part of the rover's communications system. The fabrics in the foreground are deflated airbags and parts of the lander system (they are not part of the rover). In the near-middle-ground are soils compacted by the lander's airbags.

  8. Ore resources on Mars - Wikipedia

    en.wikipedia.org/wiki/Ore_resources_on_Mars

    Opportunity found small structures, named "blueberries" which were found to be rich in hematite, a major ore of iron. [49] These blueberries could easily be gathered up and reduced to metallic iron that could be used to make steel. "Blueberries" (hematite spheres) on a rocky outcrop at Eagle Crater. Note the merged triplet in the upper left.

  9. Areostationary orbit - Wikipedia

    en.wikipedia.org/wiki/Areostationary_orbit

    Several factors make placing a spacecraft into an areostationary orbit more difficult than a geostationary orbit. Since the areostationary orbit lies between Mars's two natural satellites, Phobos (semi-major axis: 9,376 km) and Deimos (semi-major axis: 23,463 km), any satellites in the orbit will suffer increased orbital station keeping costs due to unwanted orbital resonance effects.