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Science and Science-Enabling Activities of the SHERLOC and WATSON Imaging Systems in Jezero Crater, MarsDuring 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.
Document ID
20230015706
Acquisition Source
Johnson Space Center
Document Type
Reprint (Version printed in journal)
Authors
B. V. Wogsland ORCID
(University of Tennessee at Knoxville Knoxville, Tennessee, United States)
M. E. Minitti ORCID
(Framework (United States) Silver Spring, Maryland, United States)
L. C. Kah ORCID
(University of Tennessee at Knoxville Knoxville, Tennessee, United States)
R. A. Yingst ORCID
(Planetary Science Institute Tucson, Arizona, United States)
W. Abbey ORCID
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
R. Bhartia
(Photon Systems (United States) Covina, California, United States)
L. Beegle
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
B. L. Bleefeld
(Malin Space Science Systems (United States) San Diego, California, United States)
E. L. Cardarelli ORCID
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
P. G. Conrad
(Carnegie Institution for Science Washington D.C., District of Columbia, United States)
K. Edgett ORCID
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
K. Hickman-Lewis
(University of Bologna Bologna, Emilia-Romagna, Italy)
J. Huggett ORCID
(Malin Space Science Systems (United States) San Diego, California, United States)
S. Imbeah
(Malin Space Science Systems (United States) San Diego, California, United States)
M. R. Kennedy ORCID
(Malin Space Science Systems (United States) San Diego, California, United States)
C. Lee
(Jacobs (United States) Dallas, Texas, United States)
B. E. Nixon
(Malin Space Science Systems (United States) San Diego, California, United States)
J. I. Núñez ORCID
(Johns Hopkins University Applied Physics Laboratory North Laurel, Maryland, United States)
A. Pascuzzo
(Malin Space Science Systems (United States) San Diego, California, United States)
M. Robinson
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
C. Rodiguez Sanchez-Vahamonde ORCID
(Malin Space Science Systems (United States) San Diego, California, United States)
E. Scheller
(Massachusetts Institute of Technology Cambridge, Massachusetts, United States)
S. Sharma
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
S. Siljeström ORCID
(RISE Research Institutes of Sweden Gothenburg, Sweden)
K. Steadman ORCID
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
K. Winchell
(Malin Space Science Systems (United States) San Diego, California, United States)
Michael A. Ravine ORCID
(Malin Space Science Systems (United States) San Diego, California, United States)
Date Acquired
October 31, 2023
Publication Date
October 27, 2023
Publication Information
Publication: Earth and Space Science
Publisher: Wiley Open Access
Volume: 10
Issue: 11
Issue Publication Date: November 1, 2023
e-ISSN: 2333-5084
Subject Category
Instrumentation and Photography
Funding Number(s)
TASK: J20092254100001
PROJECT: M2020-SHERLOC
CONTRACT_GRANT: 80NM0018D0004
CONTRACT_GRANT: SNSA 137/19 and 2021-00092
CONTRACT_GRANT: ASI 2017-48-H-0
CONTRACT_GRANT: 80GSFC21M0002
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
Professional Review
Keywords
WATSON
SHERLOC
Perseverance
Mars 2020
Rover
Jezero
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