Earth and Space Science (Nov 2023)

Science and Science‐Enabling Activities of the SHERLOC and WATSON Imaging Systems in Jezero Crater, Mars

  • B. V. Wogsland,
  • M. E. Minitti,
  • L. C. Kah,
  • R. A. Yingst,
  • W. Abbey,
  • R. Bhartia,
  • L. Beegle,
  • B. L. Bleefeld,
  • E. L. Cardarelli,
  • P. G. Conrad,
  • K. Edgett,
  • K. Hickman‐Lewis,
  • J. Hugget,
  • S. Imbeah,
  • M. R. Kennedy,
  • C. Lee,
  • B. E. Nixon,
  • J. I. Núñez,
  • A. Pascuzzo,
  • M. Robinson,
  • C. Rodriguez Sanchez‐Vahamonde,
  • E. Scheller,
  • S. Sharma,
  • S. Siljeström,
  • K. Steadman,
  • K. Winchell,
  • Michael A. Ravine

DOI
https://doi.org/10.1029/2022EA002544
Journal volume & issue
Vol. 10, no. 11
pp. n/a – n/a

Abstract

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Abstract During its first year of operation, the Perseverance rover explored the cratered and fractured floor of Jezero crater on Mars. Here, we report the use of the Scanning Habitability Environments with Raman and Luminescence for Organics and Chemicals (SHERLOC) imaging system that includes two high‐resolution cameras, the Autofocus and Contextual Imager (ACI) and Wide Angle Topographic Sensor for Operations and eNgineering (WATSON). ACI is a fixed focus gray scale imager with a resolution of 10.1 μm/pixel whereas WATSON is a variable field of view, variable focus imager capable of resolution down to 14 μm/pixel. WATSON is a reflight of the MArs Hand Lens Imager (MAHLI) imager and has similar capabilities. During first‐time activities, WATSON was used to support both science and engineering operations related to sample and abrasion patch assessment and sample collection and caching. WATSON also documented the deployment of the Ingenuity helicopter. The Crater Floor Campaign identified two primary rock units, the Máaz formation and the Séítah formation, which have been interpreted as lava flows and an olivine cumulate, respectively. Interpretation of rock textures with WATSON and ACI images was limited to abraded surfaces because unmodified outcrop surfaces (herein termed “natural surfaces”) show high degrees of dust covering, wind abrasion, and coating by secondary mineral products. WATSON and ACI images support the hypothesis that the material of both the Máaz and Séítah formations consists of largely aqueously altered mafic materials with varying igneous origins.

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