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Mojave Desert map. The Mojave Desert is a desert within the United States that is often used for testing Mars rovers. [43] It also has useful biological analogues for Mars. Some arid conditions and chemical processes are similar to Mars. [2] Has extremophiles within the soils. [2] Desert varnish similar to Mars. [2] [44]
CRISM was being used to identify locations on Mars that may have hosted water, [1] a solvent considered important in the search for past or present life on Mars.In order to do this, CRISM was mapping the presence of minerals and chemicals that may indicate past interaction with water - low-temperature or hydrothermal. [2]
Map showing estimated water depth in different parts of Eridania Sea This map is about 530 miles across. Features around Eridania Sea labeled Research with CRISM found thick deposits, greater than 400 meters thick, that contained the minerals saponite , talc-saponite, Fe-rich mica (for example, glauconite - nontronite ), Fe- and Mg-serpentine ...
There may be much more water further below the surface; the instruments aboard the Mars Odyssey are only able to study the top meter or so of soil. If all holes in the soil were filled by water, this would correspond to a global layer of water 0.5 to 1.5 km deep. [9] The Phoenix lander confirmed the initial findings of the Mars Odyssey. [10]
The MDRS station is situated on the San Rafael Swell of Southern Utah, [4] 11.63 kilometres (7.23 mi) by road northwest of Hanksville, Utah. [5] It is the second such analogue research station to be built by the Mars Society, following the Flashline Mars Arctic Research Station or FMARS [6] on Devon Island in Canada's high Arctic.
The upper deck's shared space is used for both computing and dining, and the galley consists of a stove, microwave, and a water container. The crew quarter's rooms have staggered bunk beds and are not equal in volume. A nearby river a few hundred meters away provides freshwater, and a gas generator provides electricity. [9]: 98–100
The Mars Desert Research Station (MDRS) is the second Mars analog habitat established by the Mars Society. Located on the San Rafael Swell in Utah , the MDRS has been inhabited by 130 individual crews (of roughly 6 members each) between the first field season in December 2001 and the twelfth field season ending in May 2013. [ 7 ]
A low-resolution map across all of Mars of surface hematite levels. Data for this map was produced by the thermal emission spectrometer (TES) on the Mars Global Surveyor between 1997 and 2002. The green and red blob in the center of the map is shown in high resolution in Figure 1b. Mapped from 1997 to 2002.
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