Minerals (May 2024)

The Chemistry and Mineralogy (CheMin) X-ray Diffractometer on the MSL Curiosity Rover: A Decade of Mineralogy from Gale Crater, Mars

  • David Blake,
  • Valerie Tu,
  • Thomas Bristow,
  • Elizabeth Rampe,
  • David Vaniman,
  • Steve Chipera,
  • Philippe Sarrazin,
  • Richard Morris,
  • Shaunna Morrison,
  • Albert Yen,
  • Robert Downs,
  • Robert Hazen,
  • Allan Treiman,
  • Douglas Ming,
  • Gordon Downs,
  • Cherie Achilles,
  • Nicholas Castle,
  • Tanya Peretyazhko,
  • David De Marais,
  • Patricia Craig,
  • Barbara Lafuente,
  • Benjamin Tutolo,
  • Elisabeth Hausrath,
  • Sarah Simpson,
  • Richard Walroth,
  • Michael Thorpe,
  • Johannes Meusburger,
  • Aditi Pandey,
  • Marc Gailhanou,
  • Przemyslaw Dera,
  • Jeffrey Berger,
  • Lucy Thompson,
  • Ralf Gellert,
  • Amy McAdam,
  • Catherine O’Connell-Cooper,
  • Brad Sutter,
  • John Michael Morookian,
  • Abigail Fraeman,
  • John Grotzinger,
  • Kirsten Siebach,
  • Soren Madsen,
  • Ashwin Vasavada

DOI
https://doi.org/10.3390/min14060568
Journal volume & issue
Vol. 14, no. 6
p. 568

Abstract

Read online

For more than a decade, the CheMin X-ray diffraction instrument on the Mars Science Laboratory rover, Curiosity, has been returning definitive and quantitative mineralogical and mineral–chemistry data from ~3.5-billion-year-old (Ga) sediments in Gale crater, Mars. To date, 40 drilled rock samples and three scooped soil samples have been analyzed during the rover’s 30+ km transit. These samples document the mineralogy of over 800 m of flat-lying fluvial, lacustrine, and aeolian sedimentary rocks that comprise the lower strata of the central mound of Gale crater (Aeolis Mons, informally known as Mt. Sharp) and the surrounding plains (Aeolis Palus, informally known as the Bradbury Rise). The principal mineralogy of the sedimentary rocks is of basaltic composition, with evidence of post-depositional diagenetic overprinting. The rocks in many cases preserve much of their primary mineralogy and sedimentary features, suggesting that they were never strongly heated or deformed. Using aeolian soil composition as a proxy for the composition of the deposited and lithified sediment, it appears that, in many cases, the diagenetic changes observed are principally isochemical. Exceptions to this trend include secondary nodules, calcium sulfate veining, and rare Si-rich alteration halos. A surprising and yet poorly understood observation is that nearly all of the ~3.5 Ga sedimentary rocks analyzed to date contain 15–70 wt.% of X-ray amorphous material. Overall, this >800 m section of sedimentary rock explored in lower Mt. Sharp documents a perennial shallow lake environment grading upward into alternating lacustrine/fluvial and aeolian environments, many of which would have been habitable to microbial life.

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