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Chemical composition of Martian fines
Abstract
Of the 21 samples acquired for the Viking X ray fluorescence spectrometer, 17 were analyzed to high precision. Compared to typical terrestrial continental soils and lunar mare fines, the Martian fines are lower in Al, higher in Fe, and much higher in S and Cl concentrations. Protected fines at the two lander sites are almost indistinguishable, but concentration of the element S is somewhat higher at Utopia. Duricrust fragments, successfully acquired only at the Chryse site, invariably contained about 50% higher S than fines. No elements correlate positively with S, except Cl and possibly Mg. A sympathetic variation is found among the triad Si, Al, Ca; positive correlation occurs between Ti and Fe. Sample variabilities are as great within a few meters as between lander locations (4500 km apart), implying the existence of a universal Martian regolith component of constant average composition. The nature of the source materials for the regolith fines must be mafic to ultramafic.
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“Martian dust of almost uniform composition on the basis of Viking and Pathfinder results [Clark e! al., 1982; Rieder et al., 1997].”
From A chemical model for evaporites on early Mars: Possible sedimentary tracers of the early climate and implications for exploration (1999) · cites this paper as Clark et al., 1982
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Mahaney, W. C., Dohm, J. M., Schwartz, S., Findling, N., Hart, K. M., Conway, S. J., Allen, C. C. R., Miyamoto, H., & Fairén, A. G. (2014) · Planetary and Space Science · doi:10.1016/j.pss.2014.10.008 · Cited by 10
Amundson, R. (2013) · Treatise on Geochemistry · doi:10.1016/b978-0-08-095975-7.00501-5 · Cited by 10
Planetary Surface Instruments Workshop
Meyer, C. E., Treiman, A. H., & Kostiuk, T. (1996) · NASA Technical Reports Server (NASA) · Cited by 10
Fan, C., Schulze‐Makuch, D., Fairén, A. G., & Wolff, J. A. (2008) · Geophysical Research Letters · doi:10.1029/2007gl033079 · Cited by 10
Martian surface chemistry: APXS results from the Pathfinder landing site
Foley, C. N., Economou, T. E., Clayton, R. N., Brückner, J., DREIBUS, G., Rieder, R., & Wänke, H. (2008) · Cambridge University Press eBooks · doi:10.1017/cbo9780511536076.004 · Cited by 9
Marchant, D. R., & Head, J. W., III (2010) · Cambridge University Press eBooks · doi:10.1017/cbo9780511712258.002 · Cited by 9
Spectral detectability of Ca- and Mg-sulfates in Martian bright soils in the 4–5μm wavelength range
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Metadata
- Authors
- Clark, B. C., Baird, A. K., Weldon, R. J., Tsusaki, D. M., Schnabel, L., & Candelaria, M. P.
- Affiliations
- Martin Marietta (United States) (US)
- Pomona College (US)
- Venue
- Journal of Geophysical Research: Solid Earth
- Publisher
- American Geophysical Union (AGU)
- Published
- 1982-01
- Volume
- 87
- Issue
- B12
- Pages
- 10059-10067
- ISSN
- 0148-0227 (ISSN-L)
- OpenAlex
- W2087792793
- Cited by
- 409
- References
- 25
- Citations by year
- 2026: 8 · 2025: 13 · 2024: 6 · 2023: 9 · 2022: 15 · 2021: 10 · 2020: 3 · 2019: 7 · 2018: 8 · 2017: 5 · 2016: 3 · 2015: 9 · 2014: 14 · 2013: 18 · 2012: 8
- FWCI
- 3.01
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Journal of Geophysical Research Atmospheres (publishedVersion)
- Topics
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Planetary Science and Exploration
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Physical Sciences › Earth and Planetary Sciences › Geochemistry and Petrology › Geochemistry and Elemental Analysis
- Keywords
- Martian regolith, chemical composition, Viking landers, X-ray fluorescence, sulfur, chlorine, iron, aluminum, duricrusts, Utopia Planitia, Chryse Planitia
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