MIRS: an imaging spectrometer for the MMX mission

Barucci, M.A.; Reess, J.-M.; Bernardi, P.; Doressoundiram, A.; Fornasier, S.; Le Du, M.; Iwata, T.; Nakagawa, H.; Nakamura, T.; André, Y.; Aoki, S.; Arai, T.; 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, H.; Hassen-Khodja, R.; Hervet, G.; Hyodo, R.; Imbert, C.; Imamura, T.; Jorda, L.; Kameda, S.; Kouach, D.; Kouyama, T.; Kuroda, T.; Kurokawa, H.; Lapaw, L.; Lasue, J.; Le Deit, L.; Ledot, A.; Leyrat, C.; Le Ruyet, B.; Matsuoka, M.; Merlin, F.; Miyamoto, H.; Moynier, F.; Nguyen Tuong, N.; Ogohara, K.; Osawa, T.; Parisot, J.; Pistre, L.; Quertier, B.; Raymond, S.N.; Rocard, F.; Sakanoi, T.; Sato, T.M.; Sawyer, E.; Tache, F.; Trémolières, S.; Tsuchiya, F.; Vernazza, P.; Zeganadin, D.

View/Open

Barucci(2021a).pdf (3.788Mb)

Authors

Barucci, M.A.

Reess, J.-M.

Bernardi, P.

Show all

Discipline

Physical sciences

Subject

MIRS

MMX

Imaging spectrometer

Phobos

Deimos

Mars

Audience

Scientific

Date

2021

Metadata

Show full item record

Description

The MMX infrared spectrometer (MIRS) is an imaging spectrometer onboard MMX JAXA mission. MMX (Martian Moon eXploration) is scheduled to be launched in 2024 with sample return to Earth in 2029. 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 spatial and temporal changes such as clouds, dust and water vapor.

Citation

Barucci, M.A.; Reess, J.-M.; Bernardi, P.; Doressoundiram, A.; Fornasier, S.; Le Du, M.; Iwata, T.; Nakagawa, H.; Nakamura, T.; André, Y.; Aoki, S.; Arai, T.; 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, H.; Hassen-Khodja, R.; Hervet, G.; Hyodo, R.; Imbert, C.; Imamura, T.; Jorda, L.; Kameda, S.; Kouach, D.; Kouyama, T.; Kuroda, T.; Kurokawa, H.; Lapaw, L.; Lasue, J.; Le Deit, L.; Ledot, A.; Leyrat, C.; Le Ruyet, B.; Matsuoka, M.; Merlin, F.; Miyamoto, H.; Moynier, F.; Nguyen Tuong, N.; Ogohara, K.; Osawa, T.; Parisot, J.; Pistre, L.; Quertier, B.; Raymond, S.N.; Rocard, F.; Sakanoi, T.; Sato, T.M.; Sawyer, E.; Tache, F.; Trémolières, S.; Tsuchiya, F.; Vernazza, P.; Zeganadin, D. (2021). MIRS: an imaging spectrometer for the MMX mission. , Earth, Planets and Space, Vol. 73, A211, DOI: 10.1186/s40623-021-01423-2.

Identifiers

uri: https://orfeo.belnet.be/handle/internal/9674

doi: http://dx.doi.org/10.1186/s40623-021-01423-2

scopus:

Type

Article

Peer-Review

Yes

Language

eng