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The ChemCam Instrument Suite on the Mars Science Laboratory (MSL) Rover: Science Objectives and Mast Unit Description

hal.structure.identifierCentre d'étude spatiale des rayonnements [CESR]
dc.contributor.authorMAURICE, S.
dc.contributor.authorWIENS, R. C.
dc.contributor.authorSACCOCCIO, M.
dc.contributor.authorBARRACLOUGH, B.
hal.structure.identifierCentre d'étude spatiale des rayonnements [CESR]
dc.contributor.authorGASNAULT, O.
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorFORNI, O.
hal.structure.identifierLaboratoire de Planétologie et Géodynamique [UMR 6112] [LPG]
dc.contributor.authorMANGOLD, N.
hal.structure.identifierServices communs OMP [UMS 831]
dc.contributor.authorBARATOUX, David
dc.contributor.authorBENDER, S.
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorBERGER, G.
dc.contributor.authorBERNARDIN, J.
dc.contributor.authorBERTHÉ, M.
dc.contributor.authorBRIDGES, N.
dc.contributor.authorBLANEY, D.
dc.contributor.authorBOUYÉ, M.
hal.structure.identifierFORMATION STELLAIRE 2012
dc.contributor.authorCAIS, Ph.
hal.structure.identifierLockheed Martin Corporation
dc.contributor.authorCLARK, B.
dc.contributor.authorCLEGG, S.
dc.contributor.authorCOUSIN, A.
dc.contributor.authorCREMERS, D.
dc.contributor.authorCROS, A.
dc.contributor.authorDEFLORES, L.
dc.contributor.authorDERYCKE, C.
dc.contributor.authorDINGLER, B.
dc.contributor.authorDROMART, G.
hal.structure.identifierFranche-Comté Électronique Mécanique, Thermique et Optique - Sciences et Technologies (UMR 6174) [FEMTO-ST]
dc.contributor.authorDUBOIS, B.
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorDUPIEUX, M.
dc.contributor.authorDURAND, E.
hal.structure.identifierCentre d'étude spatiale des rayonnements [CESR]
dc.contributor.authorD'USTON, L.
dc.contributor.authorFABRE, C.
dc.contributor.authorFAURE, Jean-Baptiste
dc.contributor.authorGABORIAUD, A.
dc.contributor.authorGHARSA, T.
dc.contributor.authorHERKENHOFF, K.
dc.contributor.authorKAN, E.
dc.contributor.authorKIRKLAND, L.
dc.contributor.authorKOUACH, D.
hal.structure.identifierSpectroscopie de l'atmosphère, Service de Chimie Quantique et Photophysique
dc.contributor.authorLACOUR, J.-L.
hal.structure.identifierInstitut d'astrophysique spatiale [IAS]
dc.contributor.authorLANGEVIN, Y.
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorLASUE, Jérémie
hal.structure.identifierLaboratoire de Planétologie et Géodynamique [UMR 6112] [LPG]
dc.contributor.authorLE MOUÉLIC, S.
dc.contributor.authorLESCURE, M.
hal.structure.identifierUniversité Joseph Fourier - Grenoble 1 [UJF]
dc.contributor.authorLEWIN, E.
dc.contributor.authorLIMONADI, D.
hal.structure.identifierInstitut de Physique du Globe de Paris [IPGP]
dc.contributor.authorMANHÈS, G.
hal.structure.identifierLaboratoire d'Interaction Laser Matière [LILM]
dc.contributor.authorMAUCHIEN, P.
dc.contributor.authorMCKAY, C.
hal.structure.identifierLaboratoire de Météorologie Dynamique (UMR 8539) [LMD]
dc.contributor.authorMESLIN, P.-Y.
hal.structure.identifierLaboratoire de Physique Théorique et Hautes Energies [LPTHE]
dc.contributor.authorMICHEL, Y.
dc.contributor.authorMILLER, E.
dc.contributor.authorNEWSOM, H. E.
dc.contributor.authorORTTNER, G.
dc.contributor.authorPAILLET, A.
dc.contributor.authorPARÈS, L.
dc.contributor.authorPAROT, Y.
dc.contributor.authorPÉREZ, R.
hal.structure.identifierServices communs OMP [UMS 831]
dc.contributor.authorPINET, P.
dc.contributor.authorPOITRASSON, F.
hal.structure.identifierFORMATION STELLAIRE 2012
dc.contributor.authorQUERTIER, Benjamin
dc.contributor.authorSALLÉ, B.
hal.structure.identifierLaboratoire de Planétologie et Géodynamique [UMR 6112] [LPG]
hal.structure.identifierJet Propulsion Laboratory [JPL]
dc.contributor.authorSOTIN, C.
dc.contributor.authorSAUTTER, V.
dc.contributor.authorSÉRAN, H.
dc.contributor.authorSIMMONDS, J. J.
dc.contributor.authorSIRVEN, J.-B.
dc.contributor.authorSTIGLICH, R.
hal.structure.identifierInstitut de Physique du Globe de Paris [IPGP]
dc.contributor.authorSTRIEBIG, N.
dc.contributor.authorTHOCAVEN, J.-J.
dc.contributor.authorTOPLIS, M. J.
dc.contributor.authorVANIMAN, D.
dc.date.issued2012-07
dc.identifier.issn0038-6308
dc.description.abstractEnChemCam is a remote sensing instrument suite on board the "Curiosity" rover (NASA) that uses Laser-Induced Breakdown Spectroscopy (LIBS) to provide the elemental composition of soils and rocks at the surface of Mars from a distance of 1.3 to 7 m, and a telescopic imager to return high resolution context and micro-images at distances greater than 1.16 m. We describe five analytical capabilities: rock classification, quantitative composition, depth profiling, context imaging, and passive spectroscopy. They serve as a toolbox to address most of the science questions at Gale crater. ChemCam consists of a Mast-Unit (laser, telescope, camera, and electronics) and a Body-Unit (spectrometers, digital processing unit, and optical demultiplexer), which are connected by an optical fiber and an electrical interface. We then report on the development, integration, and testing of the Mast-Unit, and summarize some key characteristics of ChemCam. This confirmed that nominal or better than nominal performances were achieved for critical parameters, in particular power density (>1 GW/cm2). The analysis spot diameter varies from 350 μm at 2 m to 550 μm at 7 m distance. For remote imaging, the camera field of view is 20 mrad for 1024×1024 pixels. Field tests demonstrated that the resolution (˜90 μrad) made it possible to identify laser shots on a wide variety of images. This is sufficient for visualizing laser shot pits and textures of rocks and soils. An auto-exposure capability optimizes the dynamical range of the images. Dedicated hardware and software focus the telescope, with precision that is appropriate for the LIBS and imaging depths-of-field. The light emitted by the plasma is collected and sent to the Body-Unit via a 6 m optical fiber. The companion to this paper (Wiens et al. this issue) reports on the development of the Body-Unit, on the analysis of the emitted light, and on the good match between instrument performance and science specifications.
dc.language.isoen
dc.publisherSpringer Verlag
dc.subject.enMars
dc.subject.enSpectroscopy
dc.subject.enLIBS
dc.subject.enInstruments
dc.subject.enPlanetary surfaces
dc.subject.enChemical composition
dc.title.enThe ChemCam Instrument Suite on the Mars Science Laboratory (MSL) Rover: Science Objectives and Mast Unit Description
dc.typeArticle de revue
dc.identifier.doi10.1007/S11214-012-9912-2
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
bordeaux.journalSpace Science Reviews
bordeaux.page95-166
bordeaux.volume170
bordeaux.issue1-4
bordeaux.peerReviewedoui
hal.identifierhal-00732883
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00732883v1
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