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Chemical, Mineralogical, and Physical Properties of Martian Dust and SoilGlobal and regional dust storms on Mars have been observed from Earth-based telescopes, Mars orbiters, and surface rovers and landers. Dust storms can be global and regional. Dust is material that is suspended into the atmosphere by winds and has a particle size of 1-3 micrometer. Planetary scientist refer to loose unconsolidated materials at the surface as "soil." The term ''soil'' is used here to denote any loose, unconsolidated material that can be distinguished from rocks, bedrock, or strongly cohesive sediments. No implication for the presence or absence of organic materials or living matter is intended. Soil contains local and regional materials mixed with the globally distributed dust by aeolian processes. Loose, unconsolidated surface materials (dust and soil) may pose challenges for human exploration on Mars. Dust will no doubt adhere to spacesuits, vehicles, habitats, and other surface systems. What will be the impacts on human activity? The objective of this paper is to review the chemical, mineralogical, and physical properties of the martian dust and soil.
Document ID
20170005414
Document Type
Conference Paper
Authors
Ming, D. W. (NASA Johnson Space Center Houston, TX, United States)
Morris, R. V. (NASA Johnson Space Center Houston, TX, United States)
Date Acquired
June 8, 2017
Publication Date
June 13, 2017
Subject Category
Lunar and Planetary Science and Exploration
Report/Patent Number
JSC-CN-39581
Meeting Information
Dust in the Atmosphere of Mars and Its Impact on Human Exploration Workshop(Houston, TX)
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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