M. OLLILA, Ann; WIENS, Roger C.; PEREZ, René; NELSON, Andrew; BODINE, M.; MAURICE, Sylvestre; SHARMA, Shiv; GASDA, P.; REESS, Jean-Michel; FOUCHET, T.; CLOUTIS, Edward; JOHNSON, Jeffrey R.; BENDER, S.; MONTMESSIN, Franck; BERNARDI, Pernelle; FRYDENVANG, J.; MCCABE, K.; CAIS, Ph.

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M. OLLILA, Ann
Los Alamos National Laboratory [LANL]

WIENS, Roger C.
Los Alamos National Laboratory [LANL]

PEREZ, René
Centre National d’Études Spatiales [Paris] [CNES]

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Ce document a été publié dans

48th Lunar and Planetary Science Conference, 2017-03-20, The Woodlands. p. id.2339

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Scheduled to be launched in July/August 2020, the next Mars rover will continue the geological and astrobiological exploration of the martian surface. One of the selected instrument suites on its science payload is called SuperCam. SuperCam will have five science techniques that it will deploy remotely to study the chemistry, mineralogy, and small scale morphology of Mars. These techniques include laser-induced breakdown spectroscopy (LIBS) for chemistry, Raman/time resolved fluorescence (TRF) and visible-near infrared (VISIR) spectroscopy for mineralogy, a microphone to support the LIBS analyses, and a color remote micro imager (RMI) for context imagery and textural analyses [1].< Réduire

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Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804