Cited by 607Planetary Science and ExplorationAstro and Planetary ScienceGeochemistry and Elemental Analysis

The Chemical Composition of Martian Soil and Rocks Returned by the Mobile Alpha Proton X-ray Spectrometer: Preliminary Results from the X-ray Mode

Rieder, R., Economou, T., Wänke, H., Turkevich, A., Crisp, J., Brückner, J., Dreibus, G., McSween, H. Y.·1997·Science

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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Crossref · 10.1126/science.278.5344.1771

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Each is checked against this paper’s own text: does it say what the citing paper says it does?

  • 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].”
  • 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]

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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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