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SuperCam Calibration Targets: Design and Development.
Manrique, J A; Lopez-Reyes, G; Cousin, A; Rull, F; Maurice, S; Wiens, R C; Madsen, M B; Madariaga, J M; Gasnault, O; Aramendia, J; Arana, G; Beck, P; Bernard, S; Bernardi, P; Bernt, M H; Berrocal, A; Beyssac, O; Caïs, P; Castro, C; Castro, K; Clegg, S M; Cloutis, E; Dromart, G; Drouet, C; Dubois, B; Escribano, D; Fabre, C; Fernandez, A; Forni, O; Garcia-Baonza, V; Gontijo, I; Johnson, J; Laserna, J; Lasue, J; Madsen, S; Mateo-Marti, E; Medina, J; Meslin, P-Y; Montagnac, G; Moral, A; Moros, J; Ollila, A M; Ortega, C; Prieto-Ballesteros, O; Reess, J M; Robinson, S; Rodriguez, J; Saiz, J; Sanz-Arranz, J A; Sard, I.
Affiliation
  • Manrique JA; Unidad Asocida UVA-CSIC-CAB, University of Valladolid (UVA), Valladolid, Spain.
  • Lopez-Reyes G; Unidad Asocida UVA-CSIC-CAB, University of Valladolid (UVA), Valladolid, Spain.
  • Cousin A; Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS, CNES, Université de Toulouse, Toulouse, France.
  • Rull F; Unidad Asocida UVA-CSIC-CAB, University of Valladolid (UVA), Valladolid, Spain.
  • Maurice S; Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS, CNES, Université de Toulouse, Toulouse, France.
  • Wiens RC; Los Alamos National Laboratory, Los Alamos, NM USA.
  • Madsen MB; Niels Bohr Institute (NBI), University of Copenhagen, Copenhagen, Denmark.
  • Madariaga JM; University of the Basque Country (UPV/EHU), Leioa, Spain.
  • Gasnault O; Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS, CNES, Université de Toulouse, Toulouse, France.
  • Aramendia J; University of the Basque Country (UPV/EHU), Leioa, Spain.
  • Arana G; University of the Basque Country (UPV/EHU), Leioa, Spain.
  • Beck P; CNRS, Institut de Planetologie et d'Astrophysique de Grenoble (IPAG), Universite Grenoble Alpes, Saint-Martin d'Heres, France.
  • Bernard S; Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie (IMPMC), CNRS, MNHN, Sorbonne Université, Paris, France.
  • Bernardi P; Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris-PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France.
  • Bernt MH; Niels Bohr Institute (NBI), University of Copenhagen, Copenhagen, Denmark.
  • Berrocal A; Ingeniería de Sistemas para la Defensa de España S.A. (ISDEFE), Madrid, Spain.
  • Beyssac O; Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie (IMPMC), CNRS, MNHN, Sorbonne Université, Paris, France.
  • Caïs P; Laboratoire d'astrophysique de Bordeaux, CNRS, Univ. Bordeaux, Bordeaux, France.
  • Castro C; Added Value Solutions (AVS), Elgóibar, Spain.
  • Castro K; University of the Basque Country (UPV/EHU), Leioa, Spain.
  • Clegg SM; Los Alamos National Laboratory, Los Alamos, NM USA.
  • Cloutis E; U. Winnipeg, Winnipeg, Canada.
  • Dromart G; Univ Lyon, ENSL, CNRS, LGL-TPE, Univ Lyon 1, 69007 Lyon, France.
  • Drouet C; CIRIMAT, Université de Toulouse, CNRS/UT3/INP, Ensiacet, Toulouse, France.
  • Dubois B; Observatoire Midi-Pyrénées, Toulouse, France.
  • Escribano D; Instituto Nacional de Técnica Aeroespacial, Torrejón de Ardoz, Spain.
  • Fabre C; GeoRessources, Vandoeuvre les Nancy, France.
  • Fernandez A; Added Value Solutions (AVS), Elgóibar, Spain.
  • Forni O; Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS, CNES, Université de Toulouse, Toulouse, France.
  • Garcia-Baonza V; Instituto de Geociencias CSIC, Universidad Complutense de Madrid, Madrid, Spain.
  • Gontijo I; Jet Propulsion Laboratory, Pasadena, CA USA.
  • Johnson J; Applied Physics Laboratory, Johns Hopkins University, Laurel, MD USA.
  • Laserna J; University of Malaga (UMA), Málaga, Spain.
  • Lasue J; Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS, CNES, Université de Toulouse, Toulouse, France.
  • Madsen S; Jet Propulsion Laboratory, Pasadena, CA USA.
  • Mateo-Marti E; Centro de Astrobiología-CSIC-INTA, Torrejón de Ardoz, Spain.
  • Medina J; Unidad Asocida UVA-CSIC-CAB, University of Valladolid (UVA), Valladolid, Spain.
  • Meslin PY; Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS, CNES, Université de Toulouse, Toulouse, France.
  • Montagnac G; Univ Lyon, ENSL, CNRS, LGL-TPE, Univ Lyon 1, 69007 Lyon, France.
  • Moral A; Instituto Nacional de Técnica Aeroespacial, Torrejón de Ardoz, Spain.
  • Moros J; University of Malaga (UMA), Málaga, Spain.
  • Ollila AM; Los Alamos National Laboratory, Los Alamos, NM USA.
  • Ortega C; Added Value Solutions (AVS), Elgóibar, Spain.
  • Prieto-Ballesteros O; Centro de Astrobiología-CSIC-INTA, Torrejón de Ardoz, Spain.
  • Reess JM; Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris-PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France.
  • Robinson S; Los Alamos National Laboratory, Los Alamos, NM USA.
  • Rodriguez J; Ingeniería de Sistemas para la Defensa de España S.A. (ISDEFE), Madrid, Spain.
  • Saiz J; Unidad Asocida UVA-CSIC-CAB, University of Valladolid (UVA), Valladolid, Spain.
  • Sanz-Arranz JA; Unidad Asocida UVA-CSIC-CAB, University of Valladolid (UVA), Valladolid, Spain.
  • Sard I; Added Value Solutions (AVS), Elgóibar, Spain.
Space Sci Rev ; 216(8): 138, 2020.
Article in En | MEDLINE | ID: mdl-33281235
ABSTRACT
SuperCam is a highly integrated remote-sensing instrumental suite for NASA's Mars 2020 mission. It consists of a co-aligned combination of Laser-Induced Breakdown Spectroscopy (LIBS), Time-Resolved Raman and Luminescence (TRR/L), Visible and Infrared Spectroscopy (VISIR), together with sound recording (MIC) and high-magnification imaging techniques (RMI). They provide information on the mineralogy, geochemistry and mineral context around the Perseverance Rover. The calibration of this complex suite is a major challenge. Not only does each technique require its own standards or references, their combination also introduces new requirements to obtain optimal scientific output. Elemental composition, molecular vibrational features, fluorescence, morphology and texture provide a full picture of the sample with spectral information that needs to be co-aligned, correlated, and individually calibrated. The resulting hardware includes different kinds of targets, each one covering different needs of the instrument. Standards for imaging calibration, geological samples for mineral identification and chemometric calculations or spectral references to calibrate and evaluate the health of the instrument, are all included in the SuperCam Calibration Target (SCCT). The system also includes a specifically designed assembly in which the samples are mounted. This hardware allows the targets to survive the harsh environmental conditions of the launch, cruise, landing and operation on Mars during the whole mission. Here we summarize the design, development, integration, verification and functional testing of the SCCT. This work includes some key results obtained to verify the scientific outcome of the SuperCam system.
Key words

Full text: 1 Collection: 01-internacional Database: MEDLINE Type of study: Prognostic_studies Language: En Journal: Space Sci Rev Year: 2020 Document type: Article Affiliation country: Spain

Full text: 1 Collection: 01-internacional Database: MEDLINE Type of study: Prognostic_studies Language: En Journal: Space Sci Rev Year: 2020 Document type: Article Affiliation country: Spain