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MIRS: an imaging spectrometer for the MMX mission

dc.contributor.authorBarucci, M.A.
dc.contributor.authorReess, J.-M.
dc.contributor.authorBernardi, P.
dc.contributor.authorDoressoundiram, A.
dc.contributor.authorFornasier, S.
dc.contributor.authorLe Du, M.
dc.contributor.authorIwata, T.
dc.contributor.authorNakagawa, H.
dc.contributor.authorNakamura, T.
dc.contributor.authorAndré, Y.
dc.contributor.authorAoki, S.
dc.contributor.authorArai, T.
dc.contributor.authorBaldit, E.
dc.contributor.authorBeck, P.
dc.contributor.authorBuey, J.-T.
dc.contributor.authorCanalias, E.
dc.contributor.authorCastelnau, M.
dc.contributor.authorCharnoz, S.
dc.contributor.authorChaussidon, M.
dc.contributor.authorChapron, F.
dc.contributor.authorCiarletti, V.
dc.contributor.authorDelbo, M.
dc.contributor.authorDubois, B.
dc.contributor.authorGauffre, S.
dc.contributor.authorGautier, T.
dc.contributor.authorGenda, H.
dc.contributor.authorHassen-Khodja, R.
dc.contributor.authorHervet, G.
dc.contributor.authorHyodo, R.
dc.contributor.authorImbert, C.
dc.contributor.authorImamura, T.
dc.contributor.authorJorda, L.
dc.contributor.authorKameda, S.
dc.contributor.authorKouach, D.
dc.contributor.authorKouyama, T.
dc.contributor.authorKuroda, T.
dc.contributor.authorKurokawa, H.
dc.contributor.authorLapaw, L.
dc.contributor.authorLasue, J.
dc.contributor.authorLe Deit, L.
dc.contributor.authorLedot, A.
dc.contributor.authorLeyrat, C.
dc.contributor.authorLe Ruyet, B.
dc.contributor.authorMatsuoka, M.
dc.contributor.authorMerlin, F.
dc.contributor.authorMiyamoto, H.
dc.contributor.authorMoynier, F.
dc.contributor.authorNguyen Tuong, N.
dc.contributor.authorOgohara, K.
dc.contributor.authorOsawa, T.
dc.contributor.authorParisot, J.
dc.contributor.authorPistre, L.
dc.contributor.authorQuertier, B.
dc.contributor.authorRaymond, S.N.
dc.contributor.authorRocard, F.
dc.contributor.authorSakanoi, T.
dc.contributor.authorSato, T.M.
dc.contributor.authorSawyer, E.
dc.contributor.authorTache, F.
dc.contributor.authorTrémolières, S.
dc.contributor.authorTsuchiya, F.
dc.contributor.authorVernazza, P.
dc.contributor.authorZeganadin, D.
dc.date2021
dc.date.accessioned2022-01-06T12:45:49Z
dc.date.available2022-01-06T12:45:49Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/9674
dc.descriptionThe 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.
dc.languageeng
dc.titleMIRS: an imaging spectrometer for the MMX mission
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeMIRS
dc.subject.freeMMX
dc.subject.freeImaging spectrometer
dc.subject.freePhobos
dc.subject.freeDeimos
dc.subject.freeMars
dc.source.titleEarth, Planets and Space
dc.source.volume73
dc.source.pageA211
Orfeo.peerreviewedYes
dc.identifier.doi10.1186/s40623-021-01423-2
dc.identifier.scopus


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