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Evidence for Multiple Diagenetic Episodes in Ancient Fluvial-Lacustrine Sedimentary Rocks in Gale Crater, Mars.
Achilles, C N; Rampe, E B; Downs, R T; Bristow, T F; Ming, D W; Morris, R V; Vaniman, D T; Blake, D F; Yen, A S; McAdam, A C; Sutter, B; Fedo, C M; Gwizd, S; Thompson, L M; Gellert, R; Morrison, S M; Treiman, A H; Crisp, J A; Gabriel, T S J; Chipera, S J; Hazen, R M; Craig, P I; Thorpe, M T; Des Marais, D J; Grotzinger, J P; Tu, V M; Castle, N; Downs, G W; Peretyazhko, T S; Walroth, R C; Sarrazin, P; Morookian, J M.
Afiliação
  • Achilles CN; NASA Goddard Space Flight Center Greenbelt MD USA.
  • Rampe EB; NASA Johnson Space Center Houston TX USA.
  • Downs RT; Department of Geosciences University of Arizona Tucson AZ USA.
  • Bristow TF; NASA Ames Research Center Moffett Field CA USA.
  • Ming DW; NASA Johnson Space Center Houston TX USA.
  • Morris RV; NASA Johnson Space Center Houston TX USA.
  • Vaniman DT; Planetary Science Institute Tucson AZ USA.
  • Blake DF; NASA Ames Research Center Moffett Field CA USA.
  • Yen AS; Jet Propulsion Laboratory California Institute of Technology Pasadena CA USA.
  • McAdam AC; NASA Goddard Space Flight Center Greenbelt MD USA.
  • Sutter B; Jacobs at NASA Johnson Space Center Houston TX USA.
  • Fedo CM; Department of Earth and Planetary Sciences University of Tennessee, Knoxville Knoxville TN USA.
  • Gwizd S; Department of Earth and Planetary Sciences University of Tennessee, Knoxville Knoxville TN USA.
  • Thompson LM; Department of Earth Sciences University of New Brunswick Fredericton New Brunswick Canada.
  • Gellert R; Department of Physics University of Guelph Guelph Ontario Canada.
  • Morrison SM; Carnegie Institute for Science Washington DC USA.
  • Treiman AH; Lunar and Planetary Institute Houston TX USA.
  • Crisp JA; Jet Propulsion Laboratory California Institute of Technology Pasadena CA USA.
  • Gabriel TSJ; School of Earth and Space Exploration Arizona State University Tempe AZ USA.
  • Chipera SJ; Chesapeake Energy Oklahoma City OK USA.
  • Hazen RM; Carnegie Institute for Science Washington DC USA.
  • Craig PI; Planetary Science Institute Tucson AZ USA.
  • Thorpe MT; NASA Johnson Space Center Houston TX USA.
  • Des Marais DJ; NASA Ames Research Center Moffett Field CA USA.
  • Grotzinger JP; Division of Geological and Planetary Sciences California Institute of Technology Pasadena CA USA.
  • Tu VM; Jacobs at NASA Johnson Space Center Houston TX USA.
  • Castle N; Planetary Science Institute Tucson AZ USA.
  • Downs GW; Department of Geosciences University of Arizona Tucson AZ USA.
  • Peretyazhko TS; Jacobs at NASA Johnson Space Center Houston TX USA.
  • Walroth RC; NASA Ames Research Center Moffett Field CA USA.
  • Sarrazin P; SETI Institute Mountain View CA USA.
  • Morookian JM; Jet Propulsion Laboratory California Institute of Technology Pasadena CA USA.
J Geophys Res Planets ; 125(8): e2019JE006295, 2020 Aug.
Article em En | MEDLINE | ID: mdl-32999799
ABSTRACT
The Curiosity rover's exploration of rocks and soils in Gale crater has provided diverse geochemical and mineralogical data sets, underscoring the complex geological history of the region. We report the crystalline, clay mineral, and amorphous phase distributions of four Gale crater rocks from an 80-m stratigraphic interval. The mineralogy of the four samples is strongly influenced by aqueous alteration processes, including variations in water chemistries, redox, pH, and temperature. Localized hydrothermal events are evidenced by gray hematite and maturation of amorphous SiO2 to opal-CT. Low-temperature diagenetic events are associated with fluctuating lake levels, evaporative events, and groundwater infiltration. Among all mudstones analyzed in Gale crater, the diversity in diagenetic processes is primarily captured by the mineralogy and X-ray amorphous chemistry of the drilled rocks. Variations indicate a transition from magnetite to hematite and an increase in matrix-associated sulfates suggesting intensifying influence from oxic, diagenetic fluids upsection. Furthermore, diagenetic fluid pathways are shown to be strongly affected by unconformities and sedimentary transitions, as evidenced by the intensity of alteration inferred from the mineralogy of sediments sampled adjacent to stratigraphic contacts.
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Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2020 Tipo de documento: Article

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2020 Tipo de documento: Article