Cited by 200Planetary Science and ExplorationAstro and Planetary ScienceGeochemistry and Geologic Mapping

The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.

Compositional stratigraphy of clay‐bearing layered deposits at Mawrth Vallis, Mars

Wray, J. J., Ehlmann, B. L., Squyres, S. W., Mustard, J. F., Kirk, R. L.·2008·Geophysical Research Letters

Abstract

Phyllosilicates have previously been detected in layered outcrops in and around the Martian outflow channel Mawrth Vallis. CRISM spectra of these outcrops exhibit features diagnostic of kaolinite, montmorillonite, and Fe/Mg‐rich smectites, along with crystalline ferric oxide minerals such as hematite. These minerals occur in distinct stratigraphic horizons, implying changing environmental conditions and/or a variable sediment source for these layered deposits. Similar stratigraphic sequences occur on both sides of the outflow channel and on its floor, with Al‐clay‐bearing layers typically overlying Fe/Mg‐clay‐bearing layers. This pattern, combined with layer geometries measured using topographic data from HiRISE and HRSC, suggests that the Al‐clay‐bearing horizons at Mawrth Vallis postdate the outflow channel and may represent a later sedimentary or altered pyroclastic deposit that drapes the topography.

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Crossref · 10.1029/2008gl034385

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1 of 1 references verified0 citation errors · 0 not checkable

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  • Al-rich clays such as kaolinite are observed alongside or overlying Fe/Mg clays at several sites on Mars.

    “At several sites, Al-rich clays such as kaolinite are observed alongside or overlying Fe/Mg clays (Poulet et al. 2005; Wray et al. 2008; Ehlmann et al. 2009; Carter et al. 2015).”

    From The Climate of Early Mars (2016) · cites this paper as Wray et al. 2008

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Research works printed but not linked: 19

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  14. 10.1029/2006JE002682 · DOI
  15. Neukum G., 2004, Mars Express: The Scientific Payload, 17
  16. Noe Dobrea E. Z., 2008, Clay bearing units in the region around Mawrth Vallis: Stratigraphy, extent, and possible alteration fronts, Lunar Planet. Sci.
  17. 10.1126/science.1136855 · DOI
  18. 10.1029/2006JE002831 · DOI
  19. 10.1038/nature04274 · DOI

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Metadata

Authors
Wray, J. J., Ehlmann, B. L., Squyres, S. W., Mustard, J. F., & Kirk, R. L.
Affiliations
  • Cornell University (US)
  • Brown University (US)
  • United States Geological Survey (US)
Venue
Geophysical Research Letters
Published
2008-06-21
Volume
35
Issue
12
ISSN
  • 0094-8276 (ISSN-L)
  • 1944-8007
OpenAlex
W2158914315
Cited by
200
References
1
Citations by year
2026: 5 · 2025: 11 · 2024: 5 · 2023: 5 · 2022: 9 · 2021: 7 · 2020: 6 · 2019: 51 · 2018: 6 · 2017: 8 · 2016: 8 · 2015: 9 · 2014: 7 · 2013: 6 · 2012: 19
FWCI
7.39
Type
journal article
Language
en
Open access
closed
Locations
  • Geophysical Research Letters (publishedVersion)
  • CaltechAUTHORS (California Institute of Technology) (submittedVersion)
  • DOAJ (DOAJ: Directory of Open Access Journals) (submittedVersion)
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 Geologic Mapping
Keywords
Mawrth Vallis, phyllosilicates, kaolinite, montmorillonite, smectite, hematite, outflow channels, sedimentary deposits, pyroclastic deposits, Mars

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