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Elemental geochemistry of sedimentary rocks at Yellowknife Bay, Gale crater, Mars

  • MSL Science Team
  • Stony Brook University
  • United States Geological Survey
  • Arizona State University
  • University of Leicester
  • California Institute of Technology
  • University of Guelph
  • Space Science Institute
  • United States Department of Energy
  • NASA Goddard Space Flight Center
  • NASA Ames Research Center
  • Université Lyon
  • Mount Holyoke College
  • Faculté des Sciences
  • Institute de Recherche en Astrophysique et Planétologie
  • University of New Mexico
  • Smithsonian Institution
  • Imperial College London
  • Australian National University
  • Nantes Université
  • Rensselaer Polytechnic Institute
  • Canadian Space Agency
  • Princeton University
  • Université de Toulouse
  • NASA Johnson Space Center
  • Brock University
  • Open University Milton Keynes
  • University of California at Davis
  • Lunar Planetary Science Institute
  • Planetary Science Institute
  • Los Alamos National Laboratory

Research output: Contribution to journal › Article › peer-review

305 Scopus citations

Abstract

Sedimentary rocks examined by the Curiosity rover at Yellowknife Bay, Mars, were derived from sources that evolved from an approximately average martian crustal composition to one influenced by alkaline basalts. No evidence of chemical weathering is preserved, indicating arid, possibly cold, paleoclimates and rapid erosion and deposition. The absence of predicted geochemical variations indicates that magnetite and phyllosilicates formed by diagenesis under low-temperature, circumneutral pH, rock-dominated aqueous conditions. Analyses of diagenetic features (including concretions, raised ridges, and fractures) at high spatial resolution indicate that they are composed of iron- and halogen-rich components, magnesium-iron-chlorine - rich components, and hydrated calcium sulfates, respectively. Composition of a cross-cutting dike-like feature is consistent with sedimentary intrusion. The geochemistry of these sedimentary rocks provides further evidence for diverse depositional and diagenetic sedimentary environments during the early history of Mars.

Original languageEnglish
Article number1244734
JournalScience
Volume343
Issue number6169
DOIs
StatePublished - 2014

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