SuperCam Calibration Targets: Design and Development.

Calibration Infrared spectroscopy Jezero crater LIBS Perseverance rover Raman spectroscopy SuperCam

Journal

Space science reviews
ISSN: 0038-6308
Titre abrégé: Space Sci Rev
Pays: Netherlands
ID NLM: 100971458

Informations de publication

Date de publication:
2020
Historique:
received: 04 06 2020
accepted: 09 11 2020
entrez: 7 12 2020
pubmed: 8 12 2020
medline: 8 12 2020
Statut: ppublish

Résumé

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.

Identifiants

pubmed: 33281235
doi: 10.1007/s11214-020-00764-w
pii: 764
pmc: PMC7691312
doi:

Types de publication

Journal Article Review

Langues

eng

Pagination

138

Informations de copyright

© The Author(s) 2020.

Déclaration de conflit d'intérêts

Conflicts of interest/Competing interestsThe authors declare that there are no conflicts of interest or competing interests.

Références

Talanta. 2015 Mar;134:627-639
pubmed: 25618716
Opt Express. 2014 Mar 10;22(5):6040-6
pubmed: 24663939
Earth Space Sci. 2015 May;2(5):144-172
pubmed: 27981072
Phys Chem Chem Phys. 2014 Sep 7;16(33):17551-9
pubmed: 25025655
Sci Rep. 2018 Dec 4;8(1):17576
pubmed: 30514860
Opt Express. 2015 Mar 9;23(5):6187-208
pubmed: 25836841

Auteurs

J A Manrique (JA)

Unidad Asocida UVA-CSIC-CAB, University of Valladolid (UVA), Valladolid, Spain.

G Lopez-Reyes (G)

Unidad Asocida UVA-CSIC-CAB, University of Valladolid (UVA), Valladolid, Spain.

A Cousin (A)

Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS, CNES, Université de Toulouse, Toulouse, France.

F Rull (F)

Unidad Asocida UVA-CSIC-CAB, University of Valladolid (UVA), Valladolid, Spain.

S Maurice (S)

Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS, CNES, Université de Toulouse, Toulouse, France.

R C Wiens (RC)

Los Alamos National Laboratory, Los Alamos, NM USA.

M B Madsen (MB)

Niels Bohr Institute (NBI), University of Copenhagen, Copenhagen, Denmark.

J M Madariaga (JM)

University of the Basque Country (UPV/EHU), Leioa, Spain.

O Gasnault (O)

Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS, CNES, Université de Toulouse, Toulouse, France.

J Aramendia (J)

University of the Basque Country (UPV/EHU), Leioa, Spain.

G Arana (G)

University of the Basque Country (UPV/EHU), Leioa, Spain.

P Beck (P)

CNRS, Institut de Planetologie et d'Astrophysique de Grenoble (IPAG), Universite Grenoble Alpes, Saint-Martin d'Heres, France.

S Bernard (S)

Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie (IMPMC), CNRS, MNHN, Sorbonne Université, Paris, France.

P Bernardi (P)

Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris-PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France.

M H Bernt (MH)

Niels Bohr Institute (NBI), University of Copenhagen, Copenhagen, Denmark.

A Berrocal (A)

Ingeniería de Sistemas para la Defensa de España S.A. (ISDEFE), Madrid, Spain.

O Beyssac (O)

Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie (IMPMC), CNRS, MNHN, Sorbonne Université, Paris, France.

P Caïs (P)

Laboratoire d'astrophysique de Bordeaux, CNRS, Univ. Bordeaux, Bordeaux, France.

C Castro (C)

Added Value Solutions (AVS), Elgóibar, Spain.

K Castro (K)

University of the Basque Country (UPV/EHU), Leioa, Spain.

S M Clegg (SM)

Los Alamos National Laboratory, Los Alamos, NM USA.

E Cloutis (E)

U. Winnipeg, Winnipeg, Canada.

G Dromart (G)

Univ Lyon, ENSL, CNRS, LGL-TPE, Univ Lyon 1, 69007 Lyon, France.

C Drouet (C)

CIRIMAT, Université de Toulouse, CNRS/UT3/INP, Ensiacet, Toulouse, France.

B Dubois (B)

Observatoire Midi-Pyrénées, Toulouse, France.

D Escribano (D)

Instituto Nacional de Técnica Aeroespacial, Torrejón de Ardoz, Spain.

C Fabre (C)

GeoRessources, Vandoeuvre les Nancy, France.

A Fernandez (A)

Added Value Solutions (AVS), Elgóibar, Spain.

O Forni (O)

Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS, CNES, Université de Toulouse, Toulouse, France.

V Garcia-Baonza (V)

Instituto de Geociencias CSIC, Universidad Complutense de Madrid, Madrid, Spain.

I Gontijo (I)

Jet Propulsion Laboratory, Pasadena, CA USA.

J Johnson (J)

Applied Physics Laboratory, Johns Hopkins University, Laurel, MD USA.

J Laserna (J)

University of Malaga (UMA), Málaga, Spain.

J Lasue (J)

Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS, CNES, Université de Toulouse, Toulouse, France.

S Madsen (S)

Jet Propulsion Laboratory, Pasadena, CA USA.

E Mateo-Marti (E)

Centro de Astrobiología-CSIC-INTA, Torrejón de Ardoz, Spain.

J Medina (J)

Unidad Asocida UVA-CSIC-CAB, University of Valladolid (UVA), Valladolid, Spain.

P-Y Meslin (PY)

Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS, CNES, Université de Toulouse, Toulouse, France.

G Montagnac (G)

Univ Lyon, ENSL, CNRS, LGL-TPE, Univ Lyon 1, 69007 Lyon, France.

A Moral (A)

Instituto Nacional de Técnica Aeroespacial, Torrejón de Ardoz, Spain.

J Moros (J)

University of Malaga (UMA), Málaga, Spain.

A M Ollila (AM)

Los Alamos National Laboratory, Los Alamos, NM USA.

C Ortega (C)

Added Value Solutions (AVS), Elgóibar, Spain.

O Prieto-Ballesteros (O)

Centro de Astrobiología-CSIC-INTA, Torrejón de Ardoz, Spain.

J M Reess (JM)

Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris-PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France.

S Robinson (S)

Los Alamos National Laboratory, Los Alamos, NM USA.

J Rodriguez (J)

Ingeniería de Sistemas para la Defensa de España S.A. (ISDEFE), Madrid, Spain.

J Saiz (J)

Unidad Asocida UVA-CSIC-CAB, University of Valladolid (UVA), Valladolid, Spain.

J A Sanz-Arranz (JA)

Unidad Asocida UVA-CSIC-CAB, University of Valladolid (UVA), Valladolid, Spain.

I Sard (I)

Added Value Solutions (AVS), Elgóibar, Spain.

V Sautter (V)

Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie (IMPMC), CNRS, MNHN, Sorbonne Université, Paris, France.

P Sobron (P)

SETI Institute, Mountain View, CA USA.

M Toplis (M)

Observatoire Midi-Pyrénées, Toulouse, France.

M Veneranda (M)

Unidad Asocida UVA-CSIC-CAB, University of Valladolid (UVA), Valladolid, Spain.

Classifications MeSH