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Composition and Density Stratification Observed by SuperCam in the First 300 Sols in Jezero CraterThe Perseverance rover has traveled > 2.5 km since leaving its Octavia Butler landing site in
Jezero crater ~300 sols ago. The SuperCam remote sensing instrument suite has made > 1000 observations of bedrock along the traverse to provide a comprehensive picture of Jezero crater floor’s chemistry and mineralogy. SuperCam combines high resolution imaging, visible and near-infrared (VISIR) reflectance spectroscopy (0.4-0.85, 1.3-2.6 µm), remote time-resolved green-laser Raman and fluorescence spectroscopy, laser-induced breakdown spectroscopy (LIBS), and acoustic sensing into a single co-boresighted package [1, 2]. Derivation of the major element abundances as oxide wt% for this part of the mission is presented in [3], while calibration of the VIS and IR spectrometers are given in [4-7].
Document ID
20220000504
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
External Source(s)
https://mars.nasa.gov/mars2020/spacecraft/instruments/supercam/
Authors
R.C. Wiens (Los Alamos National Laboratory Los Alamos, New Mexico, United States)
A. Udry (University of Nevada, Las Vegas Las Vegas, Nevada, United States)
N. Mangold (Laboratoire de Planétologie et Géodynamique de Nantes Nantes, France)
O. Beyssac (Institute of Mineralogy, Materials Physics and Cosmochemistry Paris, France)
C. Quantin (University of Lyon System Lyon, France)
V. Sautter (Sorbonne University Paris, France)
A. Cousin (Institute de Recherche en Astrophysique et Planetologie)
A. Brown (National Aeronautics and Space Administration Washington D.C., District of Columbia, United States)
T. Bosak (Massachusetts Institute of Technology Cambridge, Massachusetts, United States)
L. Mandon (Paris Observatory Paris, Île-de-France, France)
O. Forni (Research Institute in Astrophysics and Planetology Toulouse, France)
J.R. Johnson (Johns Hopkins University Applied Physics Laboratory North Laurel, Maryland, United States)
S. McLennan (Stony Brook University Stony Brook, New York, United States)
C. Legett IV (Los Alamos National Laboratory Los Alamos, New Mexico, United States)
S. Maurice (Research Institute in Astrophysics and Planetology Toulouse, France)
L. Mayhew (University of Colorado Boulder Boulder, Colorado, United States)
L. Crumpler (New Mexico Museum of Natural History and Science Albuquerque, New Mexico, United States)
R.B. Anderson (University of Colorado Boulder Boulder, Colorado, United States)
S.M. Clegg (Los Alamos National Laboratory Los Alamos, New Mexico, United States)
A.M. Ollila (Los Alamos National Laboratory Los Alamos, New Mexico, United States)
J. Hall (Massachusetts Institute of Technology Cambridge, Massachusetts, United States)
P.-Y. Meslin (Research Institute in Astrophysics and Planetology Toulouse, France)
L.C. Kah (University of Tennessee at Knoxville Knoxville, Tennessee, United States)
T.S.J. Gabriel (United States Geological Survey Reston, Virginia, United States)
P. Gasda (Los Alamos National Laboratory Los Alamos, New Mexico, United States)
J.I. Simon (Johnson Space Center Houston, Texas, United States)
E.M. Hausrath (University of Nevada, Las Vegas Las Vegas, Nevada, United States)
B. Horgan (Purdue University West Lafayette West Lafayette, Indiana, United States)
F. Poulet (Institut d'Astrophysique Spatiale Bures-sur-Yvette, France)
P. Beck (Grenoble Alpes University Saint-Martin-d'Hères, France)
S. Gupta (Imperial College London London, Westminster, United Kingdom)
B. Chide (Los Alamos National Laboratory Los Alamos, New Mexico, United States)
E. Clavé (University of Bordeaux Bordeaux, France)
S. Connell (University of Winnipeg Winnipeg, Manitoba, Canada)
E. Dehouck (Catholic University of Lyon Lyon, France)
G. Dromart (Catholic University of Lyon Lyon, France)
T. Fouchet (Laboratory of Space Studies and Instrumentation in Astrophysics Meudon, France)
C. Royer (Lockheed Martin (United States) Bethesda, Maryland, United States)
J. Frydenvang (Paris Observatory Paris, Île-de-France, France)
O. Gasnault (Research Institute in Astrophysics and Planetology Toulouse, France)
E. Gibbons (McGill University Montreal, Quebec, Canada)
H. Kalucha (California Institute of Technology Pasadena, California, United States)
N. Lanza (Los Alamos National Laboratory Los Alamos, New Mexico, United States)
J. Lasue (Research Institute in Astrophysics and Planetology Toulouse, France)
S. Le Mouelic (Laboratoire de Planétologie et Géodynamique de Nantes Nantes, France)
R. Leveillé (McGill University Montreal, Quebec, Canada)
E. Cloutis (University of Winnipeg Winnipeg, Manitoba, Canada)
G. Lopez Reyes (University of Valladolid Valladolid, Castilla y León, Spain)
G. Arana (University of the Basque Country Leioa, Spain)
K. Castro (University of the Basque Country Leioa, Spain)
J.M. Madariaga (University of the Basque Country Leioa, Spain)
J.-A. Manrique (University of Valladolid Valladolid, Castilla y León, Spain)
C. Pilorget (Institut d'Astrophysique Spatiale Bures-sur-Yvette, France)
P. Pinet (Research Institute in Astrophysics and Planetology Toulouse, France)
J. Laserna (University of Malaga Málaga, Spain)
S.K. Sharma (University of Hawaii at Manoa Honolulu, Hawaii, United States)
T. Acosta-Maeda (University of Hawaii at Manoa Honolulu, Hawaii, United States)
E. Kelly (University of Hawaii at Manoa Honolulu, Hawaii, United States)
F. Montmessin (Atmospheres Laboratory Environments, Observations Spatiales Guyancourt, France)
W. Fischer (California Institute of Technology Pasadena, California, United States)
R. Francis (Jet Propulsion Lab La Cañada Flintridge, California, United States)
K. Stack (Jet Propulsion Lab La Cañada Flintridge, California, United States)
K. Farley (California Institute of Technology Pasadena, California, United States)
Date Acquired
January 25, 2022
Subject Category
Lunar And Planetary Science And Exploration
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Houston, TX
Country: US
Start Date: March 7, 2022
End Date: March 11, 2022
Sponsors: Lunar and Planetary Institute
Funding Number(s)
WBS: 203959
PROJECT: Mars 2020 Project
Distribution Limits
Public
Copyright
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