The Chemical Composition of Martian Soil and Rocks Returned by the Mobile Alpha Proton X-ray Spectrometer: Preliminary Results from the X-ray Mode
Abstract
The alpha proton x-ray spectrometer (APXS) on board the rover of the Mars Pathfinder mission measured the chemical composition of six soils and five rocks at the Ares Vallis landing site. The soil analyses show similarity to those determined by the Viking missions. The analyzed rocks were partially covered by dust but otherwise compositionally similar to each other. They are unexpectedly high in silica and potassium, but low in magnesium compared to martian soils and martian meteorites. The analyzed rocks are similar in composition to terrestrial andesites and close to the mean composition of Earth's crust. Addition of a mafic component and reaction products of volcanic gases to the local rock material is necessary to explain the soil composition.
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Martian dust is of almost uniform composition on the basis of Viking and Pathfinder results.
“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 Rieder et al., 1997
Perchlorate salts are hypothesized to be present over the entire surface of Mars due to atmospheric circulation and wind transport of sediments.
“With atmospheric circulation and wind transport of sediments, perchlorate salts are hypothesized to be present over the entire surface of Mars [16][17][18].”
From Perchlorate and Agriculture on Mars (2021) · cites this paper as [16]
Cites
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Exploring for a record of ancient Martian life
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First demonstration on direct laser fabrication of lunar regolith parts
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Perchlorate and Agriculture on Mars
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- Authors
- Rieder, R., Economou, T., Wänke, H., Turkevich, A., Crisp, J., Brückner, J., Dreibus, G., & McSween, H. Y.
- Affiliations
- California Institute of Technology (US)
- R. Rieder, H. Wänke, J. Brückner, G. Dreibus, Max-Planck-Institut für Chemie, P.O. Box 3060, D-55020 Mainz, Germany.
- Venue
- Science
- Published
- 1997-12-05
- Volume
- 278
- Issue
- 5344
- Pages
- 1771-1774
- ISSN
- 0036-8075 (ISSN-L)
- 1095-9203
- OpenAlex
- W1982898366
- Cited by
- 607
- References
- 1
- Citations by year
- 2026: 4 · 2025: 14 · 2024: 17 · 2023: 10 · 2022: 15 · 2021: 13 · 2020: 18 · 2019: 9 · 2018: 14 · 2017: 9 · 2016: 74 · 2015: 11 · 2014: 7 · 2013: 10 · 2012: 15
- FWCI
- 31.62
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Science (publishedVersion)
- PubMed (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Planetary Science and Exploration
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
- Physical Sciences › Earth and Planetary Sciences › Geochemistry and Petrology › Geochemistry and Elemental Analysis
- Keywords
- Martian soil, Martian rocks, chemical composition, Mars Pathfinder, Ares Vallis, silica, potassium, magnesium, andesite, Earth's crust, volcanic gases, Martian meteorites
- MeSH terms
- Aluminum, Extraterrestrial Environment, Iron, Magnesium, Oxides, Potassium, Silicon Dioxide, Mars, Geologic Sediments, Meteoroids
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