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Chemistry of diagenetic features analyzed by ChemCam at Pahrump Hills, Gale crater, Mars

Journal Article · · Icarus
 [1];  [1];  [2];  [3];  [2];  [4];  [5];  [6];  [7];  [6];  [4];  [8];  [9];  [2];  [10];  [3];  [4];  [2];  [1];  [1] more »;  [2];  [2];  [11];  [8];  [2];  [12];  [6];  [13] « less
  1. Univ. of Nantes (France). Lab. of Planetology and Geodynamics
  2. Univ. of Toulouse (France). Center for Space Studies of Radiation
  3. Univ. of Tennessee, Knoxville, TN (United States). Dept. of Earth and Planetary Sciences
  4. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
  5. U.S. Geological Survey Astrogeology Science Center, Flagstaff, AZ (United States)
  6. California Inst. of Technology (CalTech), Pasadena, CA (United States). Jet Propulsion Lab.
  7. NASA Ames Research Center (ARC), Moffett Field, Mountain View, CA (United States)
  8. Univ. of Lorraine, Nancy (France). Geo Ressources
  9. Oregon State Univ., Corvallis, OR (United States). College of Earth Ocean and Atmospheric Sciences
  10. California Inst. of Technology (CalTech), Pasadena, CA (United States). Division of Geologic and Planetary Sciences
  11. NASA Johnson Space Center, Houston, TX (United States). Astromaterials Research and Exploration Science Division
  12. Univ. of Toulouse (France). Center for Space Studies of Radiation; German Aerospace Center (DLR), Berlin (Germany)
  13. Univ. of California, Davis, CA (United States). Earth and Planetary Sciences
The Curiosity rover's campaign at Pahrump Hills provides the first analyses of lower Mount Sharp strata. We report ChemCam elemental composition of a diverse assemblage of post-depositional features embedded in, or cross-cutting, the host rock. ChemCam results demonstrate their compositional diversity, especially compared to the surrounding host rock: (i) Dendritic aggregates and relief enhanced features, characterized by a magnesium enhancement and sulfur detection, and interpreted as Mg-sulfates; (ii) A localized observation that displays iron enrichment associated with sulfur, interpreted as Fe-sulfate; (iii) Dark raised ridges with varying Mg- and Ca-enriched compositions compared to host rock; (iv) Several dark-toned veins with calcium enhancement associated with fluorine detection, interpreted as fluorite veins. (v) Light-toned veins with enhanced calcium associated with sulfur detection, and interpreted as Ca-sulfates. The diversity of the Pahrump Hills diagenetic assemblage suggests a complex post-depositional history for fine-grained sediments for which the origin has been interpreted as fluvial and lacustrine. Assessment of the spatial and relative temporal distribution of these features shows that the Mg-sulfate features are predominant in the lower part of the section, suggesting local modification of the sediments by early diagenetic fluids. Conversely, light-toned Ca-sulfate veins occur in the whole section and cross-cut all other features. A relatively late stage shift in geochemical conditions could explain this observation. The Pahrump Hills diagenetic features have no equivalent compared to targets analyzed in other locations at Gale crater. Only the light-toned Ca-sulfate veins are present elsewhere, along Curiosity's path, suggesting they formed through a common late-stage process that occurred at over a broad area.
Research Organization:
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
National Aeronautics and Space Administration (NASA)
Grant/Contract Number:
AC52-06NA25396
OSTI ID:
1412864
Report Number(s):
LA-UR--17-27694
Journal Information:
Icarus, Journal Name: Icarus Journal Issue: C Vol. 281; ISSN 0019-1035
Publisher:
ElsevierCopyright Statement
Country of Publication:
United States
Language:
English

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Cited By (16)

Using ChemCam LIBS data to constrain grain size in rocks on Mars: Proof of concept and application to rocks at Yellowknife Bay and Pahrump Hills, Gale crater journal March 2019
Extraformational sediment recycling on Mars journal October 2020
Characterization of LIBS emission lines for the identification of chlorides, carbonates, and sulfates in salt/basalt mixtures for the application to MSL ChemCam data: LIBS OF CL, C, S IN SALT-BASALT MIXTURES journal April 2017
Geological Analysis of Martian Rover-Derived Digital Outcrop Models Using the 3-D Visualization Tool, Planetary Robotics 3-D Viewer-PRo3D journal July 2018
Geologic Constraints on Early Mars Climate journal January 2019
In Situ Analysis of Opal in Gale Crater, Mars journal August 2018
Mineral-Filled Fractures as Indicators of Multigenerational Fluid Flow in the Pahrump Hills Member of the Murray Formation, Gale Crater, Mars journal February 2019
Major Volatiles Evolved From Eolian Materials in Gale Crater journal October 2018
Extensive Polygonal Fracture Network in Siccar Point group Strata: Fracture Mechanisms and Implications for Fluid Circulation in Gale Crater, Mars journal October 2019
An interval of high salinity in ancient Gale crater lake on Mars journal October 2019
The potential science and engineering value of samples delivered to Earth by Mars sample return journal March 2019
The potential science and engineering value of samples delivered to Earth by Mars sample return: International MSR Objectives and Samples Team (iMOST) journal March 2019
Organic matter preserved in 3-billion-year-old mudstones at Gale crater, Mars journal June 2018
Ichnofossils, Cracks or Crystals? A Test for Biogenicity of Stick-Like Structures from Vera Rubin Ridge, Mars journal January 2020
Geological Analysis of Martian Rover-Derived Digital Outcrop Models Using the 3-D Visualization Tool, Planetary Robotics 3-D Viewer—PRo3D text January 2018
The potential science and engineering value of samples delivered to Earth by Mars sample return text January 2019

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