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A Mars 2020 Perseverance SuperCam Perspective on the Igneous Nature of the Máaz Formation at Jezero Crater, MarsThe Mars2020 Perseverance rover landed in Jezero crater in February 2020,and first encountered the Máaz formation (or Crater floor-fractured rough(Cf-fr) unit previously mapped based on orbital data[1]).In this study, we use data from the SuperCam instrument(SCAM) to show that the Máaz formation has an igneous origin. SuperCam is a remote-sensing instrument onboard Perseverance, and investigates the texture, mineralogy, and chemistry of rocks and soils, as well as atmospheric features [2,3]. SuperCam comprises the Remote Micro Imager (RMI) to provide high-resolution images, laser-induced breakdown spectroscopy (LIBS)to investigate the major and minor element chemistry of materials, Raman, and passive visible-near infrared (VISIR) spectroscopy to analyze the mineralogy of targets, and time-resolved luminescence spectroscopy (TRLS)to measure organic fluorescence and inorganic luminescence. In addition, the microphone (MIC) can constrain the rock hardness through measurements of the shockwave of LIBS shots. In this study, we use LIBS-based major-oxide compositions (MOC),quantified using the calibration in [2].
Document ID
20220000502
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
A Udry
(University of Nevada, Las Vegas Las Vegas, Nevada, United States)
V Sautter
(Institute de Recherche en Astrophysique et Planetologie)
A Cousin
(Institute de Recherche en Astrophysique et Planetologie)
R C Wiens
(Los Alamos National Laboratory Los Alamos, New Mexico, United States)
O Forni
(Institute de Recherche en Astrophysique et Planetologie)
K Benzerara
(Centre national de la recherche scientifique Rabat, Morocco)
O Beyssac
(Institute of Mineralogy, Materials Physics and Cosmochemistry Paris, France)
M Nachon
(Texas A&M University)
G Dromart
(ENS Lyon)
C Quantin
(ENS Lyon Lyon, France)
L Mandon
(Centre national de la recherche scientifique Rabat, Morocco)
E Clave
(Centre national de la recherche scientifique Rabat, Morocco)
P Pinet
(Institute de Recherche en Astrophysique et Planetologie)
A Ollila
(Los Alamos National Laboratory Los Alamos, New Mexico, United States)
T Bosak
(Massachusetts Institute of Technology Cambridge, Massachusetts, United States)
N Mangold
(Laboratoire de Planétologie et Géodynamique de Nantes Nantes, France)
E Dehouck
(ENS Lyon)
J Johnson
(Johns Hopkins University Applied Physics Laboratory North Laurel, Maryland, United States)
M Schmidt
(Brock University St. Catharines, Ontario, Canada)
B Horgan
(Purdue University West Lafayette West Lafayette, Indiana, United States)
T Gabriel
(United States Geological Survey Reston, Virginia, United States)
S Mclennan
(Stony Brook University Stony Brook, New York, United States)
S Maurice
(Institute de Recherche en Astrophysique et Planetologie)
J I Simon
(Johnson Space Center Houston, Texas, United States)
C D K Herd
(University of Alberta Edmonton, Alberta, Canada)
J M Madiaraga
(University of the Basque Country Leioa, Spain)
Date Acquired
January 25, 2022
Subject Category
Spacecraft Instrumentation And Astrionics
Meeting Information
Meeting: 53rd Lunar and Planetary Science Conference
Location: The Woodlands, TX
Country: US
Start Date: March 7, 2022
End Date: March 11, 2022
Sponsors: Lunar and Planetary Institute
Funding Number(s)
WBS: 203959
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Keywords
Mars 2020
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