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

Author:

Wogsland B. V.1ORCID,Minitti M. E.2ORCID,Kah L. C.1ORCID,Yingst R. A.3ORCID,Abbey W.4ORCID,Bhartia R.5,Beegle L.6,Bleefeld B. L.7,Cardarelli E. L.4ORCID,Conrad P. G.8,Edgett K.6ORCID,Hickman‐Lewis K.9,Hugget J.7ORCID,Imbeah S.7,Kennedy M. R.7ORCID,Lee C.10,Nixon B. E.7,Núñez J. I.11ORCID,Pascuzzo A.7,Robinson M.4,Sanchez‐Vahamonde C. Rodriguez7ORCID,Scheller E.12,Sharma S.4,Siljeström S.13ORCID,Steadman K.4ORCID,Winchell K.7,Ravine Michael A.7ORCID

Affiliation:

1. University of Tennessee Knoxville MD USA

2. Framework Silver Spring MD USA

3. Planetary Science Institute San Diego CA USA

4. Jet Propulsion Laboratory California Institute of Technology Pasadena CA USA

5. Photon Systems Incorporated Covina CA USA

6. Formerly with NASA Jet Propulsion Laboratory California Institute of Technology Pasadena CA USA

7. Malin Space Science Systems San Diego CA USA

8. Carnegie Institution for Science Washington DC USA

9. The Natural History Museum Università di Bologna Bologna Italy

10. NASA Johnson Space Center Houston TX USA

11. Johns Hopkins University Applied Physics Laboratory Laurel MD USA

12. Massachusetts Institute of Technology Cambridge MA USA

13. RISE Research Institutes of Sweden Stockholm Sweden

Abstract

AbstractDuring 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.

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Environmental Science (miscellaneous)

Cited by 1 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Evidence of Sulfate‐Rich Fluid Alteration in Jezero Crater Floor, Mars;Journal of Geophysical Research: Planets;2024-01

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