MIRS: an imaging spectrometer for the MMX mission

Barucci, M. A.*; Reess, J.-M.*; Bernardi, P.*; Doressoundiram, A.*; Fornasier, S.*; Le Du, M.*; Iwata, Takahiro*; Nakagawa, Hiromu*; Nakamura, Tomoki*; Andr, Y.*; Aoki, Shohei*; Arai, Takehiko*; Baldit, E.*; Beck, P.*; Buey, J.-T.*; Canalias, E.*; Castelnau, M.*; Charnoz, S.*; Chaussidon, M.*; Chapron, F.*; Ciarletti, V.*; Delbo, M,*; Dubois, B.*; Gauffre, S.*; Gautier, T.*; Genda, Hidenori*; Hassen-Khodja, R.*; Hervet, G.*; Hyodo, Ryuki*; Imbert, C.*; Imamura, Takeshi*; Jorda, L.*; Kameda, Shingo*; Kouach, D.*; Koyama, Toru*; Kuroda, Takeshi*; Kurokawa, Hiroyuki*; Lapaw, L.*; Lasue, J.*; Le Deit, L.*; Ledot, A.*; Leyrat, C.*; Le Ruyet, B.*; Matsuoka, Moe*; Merlin, F.*; Miyamoto, Hideaki*; Moynier, F.*; Nguyen Tuong, N.*; Ogohara, Kazunori*; Osawa, Takahito  ; Parisot, J.*; Pistre, L.*; Quertier, B,*; Raymond, S. N.*; Rocard, F.*; Sakanoi, Takeshi*; Sato, Takao*; Sawyer, E.*; Tache, F.*; Trmoliers, S.*; Tsuchiya, Fuminori*; Vernazza, P.*; Zeganadin, D.*

The MMX InfraRed Spectrometer (MIRS) is an imaging spectrometer on board of MMX JAXA mission. MIRS is built at LESIA-Paris Observatory in collaboration with four other French laboratories, collaboration and financial support of CNES and close collaboration with JAXA and MELCO. The instrument is designed to fully accomplish MMX's scientific and measurement objectives. MIRS will remotely provide near-infrared spectral maps of Phobos and Deimos containing compositional diagnostic spectral features that will be used to analyze the surface composition and to support the sampling site selection. MIRS will also study Mars atmosphere, in particular to spatial and temporal changes such as clouds, dust and water vapor.