MIRS: an imaging spectrometer for the MMX mission

Abstract 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, co...

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Main Authors: Maria Antonietta Barucci, Jean-Michel Reess, Pernelle Bernardi, Alain Doressoundiram, Sonia Fornasier, Michel Le Du, Takahiro Iwata, Hiromu Nakagawa, Tomoki Nakamura, Yves André, Shohei Aoki, Takehiko Arai, Elisa Baldit, Pierre Beck, Jean-Tristan Buey, Elisabet Canalias, Matthieu Castelnau, Sebastien Charnoz, Marc Chaussidon, Fréderic Chapron, Valerie Ciarletti, Marco Delbo, Bruno Dubois, Stephane Gauffre, Thomas Gautier, Hidenori Genda, Rafik Hassen-Khodja, Gilles Hervet, Ryuki Hyodo, Christian Imbert, Takeshi Imamura, Laurent Jorda, Shingo Kameda, Driss Kouach, Toru Kouyama, Takeshi Kuroda, Hiroyuki Kurokawa, Laurent Lapaw, Jeremie Lasue, Laetitia Le Deit, Aurélien Ledot, Cedric Leyrat, Bertrand Le Ruyet, Moe Matsuoka, Frederic Merlin, Hideaki Miyamoto, Frederic Moynier, Napoleon Nguyen Tuong, Kazunori Ogohara, Takahito Osawa, Jérôme Parisot, Laurie Pistre, Benjamin Quertier, Sean N. Raymond, Francis Rocard, Takeshi Sakanoi, Takao M. Sato, Eric Sawyer, Fériel Tache, Sylvain Trémolières, Fuminori Tsuchiya, Pierre Vernazza, Didier Zeganadin
Format: Article
Language:English
Published: SpringerOpen 2021-12-01
Series:Earth, Planets and Space
Subjects:
Online Access:https://doi.org/10.1186/s40623-021-01423-2
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author Maria Antonietta Barucci
Jean-Michel Reess
Pernelle Bernardi
Alain Doressoundiram
Sonia Fornasier
Michel Le Du
Takahiro Iwata
Hiromu Nakagawa
Tomoki Nakamura
Yves André
Shohei Aoki
Takehiko Arai
Elisa Baldit
Pierre Beck
Jean-Tristan Buey
Elisabet Canalias
Matthieu Castelnau
Sebastien Charnoz
Marc Chaussidon
Fréderic Chapron
Valerie Ciarletti
Marco Delbo
Bruno Dubois
Stephane Gauffre
Thomas Gautier
Hidenori Genda
Rafik Hassen-Khodja
Gilles Hervet
Ryuki Hyodo
Christian Imbert
Takeshi Imamura
Laurent Jorda
Shingo Kameda
Driss Kouach
Toru Kouyama
Takeshi Kuroda
Hiroyuki Kurokawa
Laurent Lapaw
Jeremie Lasue
Laetitia Le Deit
Aurélien Ledot
Cedric Leyrat
Bertrand Le Ruyet
Moe Matsuoka
Frederic Merlin
Hideaki Miyamoto
Frederic Moynier
Napoleon Nguyen Tuong
Kazunori Ogohara
Takahito Osawa
Jérôme Parisot
Laurie Pistre
Benjamin Quertier
Sean N. Raymond
Francis Rocard
Takeshi Sakanoi
Takao M. Sato
Eric Sawyer
Fériel Tache
Sylvain Trémolières
Fuminori Tsuchiya
Pierre Vernazza
Didier Zeganadin
author_facet Maria Antonietta Barucci
Jean-Michel Reess
Pernelle Bernardi
Alain Doressoundiram
Sonia Fornasier
Michel Le Du
Takahiro Iwata
Hiromu Nakagawa
Tomoki Nakamura
Yves André
Shohei Aoki
Takehiko Arai
Elisa Baldit
Pierre Beck
Jean-Tristan Buey
Elisabet Canalias
Matthieu Castelnau
Sebastien Charnoz
Marc Chaussidon
Fréderic Chapron
Valerie Ciarletti
Marco Delbo
Bruno Dubois
Stephane Gauffre
Thomas Gautier
Hidenori Genda
Rafik Hassen-Khodja
Gilles Hervet
Ryuki Hyodo
Christian Imbert
Takeshi Imamura
Laurent Jorda
Shingo Kameda
Driss Kouach
Toru Kouyama
Takeshi Kuroda
Hiroyuki Kurokawa
Laurent Lapaw
Jeremie Lasue
Laetitia Le Deit
Aurélien Ledot
Cedric Leyrat
Bertrand Le Ruyet
Moe Matsuoka
Frederic Merlin
Hideaki Miyamoto
Frederic Moynier
Napoleon Nguyen Tuong
Kazunori Ogohara
Takahito Osawa
Jérôme Parisot
Laurie Pistre
Benjamin Quertier
Sean N. Raymond
Francis Rocard
Takeshi Sakanoi
Takao M. Sato
Eric Sawyer
Fériel Tache
Sylvain Trémolières
Fuminori Tsuchiya
Pierre Vernazza
Didier Zeganadin
author_sort Maria Antonietta Barucci
collection DOAJ
description Abstract 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. Graphical Abstract
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spelling doaj.art-bf7c689b50b5415e8289eb0dbaf7e0092022-12-21T21:32:28ZengSpringerOpenEarth, Planets and Space1880-59812021-12-0173112810.1186/s40623-021-01423-2MIRS: an imaging spectrometer for the MMX missionMaria Antonietta Barucci0Jean-Michel Reess1Pernelle Bernardi2Alain Doressoundiram3Sonia Fornasier4Michel Le Du5Takahiro Iwata6Hiromu Nakagawa7Tomoki Nakamura8Yves André9Shohei Aoki10Takehiko Arai11Elisa Baldit12Pierre Beck13Jean-Tristan Buey14Elisabet Canalias15Matthieu Castelnau16Sebastien Charnoz17Marc Chaussidon18Fréderic Chapron19Valerie Ciarletti20Marco Delbo21Bruno Dubois22Stephane Gauffre23Thomas Gautier24Hidenori Genda25Rafik Hassen-Khodja26Gilles Hervet27Ryuki Hyodo28Christian Imbert29Takeshi Imamura30Laurent Jorda31Shingo Kameda32Driss Kouach33Toru Kouyama34Takeshi Kuroda35Hiroyuki Kurokawa36Laurent Lapaw37Jeremie Lasue38Laetitia Le Deit39Aurélien Ledot40Cedric Leyrat41Bertrand Le Ruyet42Moe Matsuoka43Frederic Merlin44Hideaki Miyamoto45Frederic Moynier46Napoleon Nguyen Tuong47Kazunori Ogohara48Takahito Osawa49Jérôme Parisot50Laurie Pistre51Benjamin Quertier52Sean N. Raymond53Francis Rocard54Takeshi Sakanoi55Takao M. Sato56Eric Sawyer57Fériel Tache58Sylvain Trémolières59Fuminori Tsuchiya60Pierre Vernazza61Didier Zeganadin62LESIA-Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de ParisLESIA-Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de ParisLESIA-Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de ParisLESIA-Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de ParisLESIA-Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de ParisCNESISAS JAXADepartment of Geophysics, Tohoku UniversityDepartment of Geophysics, Tohoku UniversityCNESISAS JAXAAshikaga UniversityCNESUniversité Grenoble Alpes, CNRS, IPAGLESIA-Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de ParisCNESCNESUniversité de Paris, Institut de Physique du Globe de Paris, CNRSUniversité de Paris, Institut de Physique du Globe de Paris, CNRSLESIA-Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de ParisLATMOS/IPSL, UVSQ Université Paris-Saclay, Sorbonne Université, CNRSCNRS, Observatoire Côte d’AzurObservatoire Midi-PyrenéesLAB Université de BordeauxLATMOS/IPSL, UVSQ Université Paris-Saclay, Sorbonne Université, CNRSEarth-Life Science Institute, Tokyo Institute of TechnologyLATMOS/IPSL, UVSQ Université Paris-Saclay, Sorbonne Université, CNRSCNESISAS JAXACNESUniversity of TokyoLaboratoire d’Astrophysique de MarseilleRikkyo UniversityObservatoire Midi-PyrenéesNIAISTDepartment of Geophysics, Tohoku UniversityEarth-Life Science Institute, Tokyo Institute of TechnologyLATMOS/IPSL, UVSQ Université Paris-Saclay, Sorbonne Université, CNRSIRAPLPG, UMR CNRS 6112, Université de Nantes, Université d’AngersCNESLESIA-Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de ParisLESIA-Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de ParisLESIA-Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de ParisLESIA-Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de ParisUniversity of TokyoUniversité de Paris, Institut de Physique du Globe de Paris, CNRSLESIA-Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de ParisKyoto Sangyo UniversityJapan Atomic Energy AgencyLESIA-Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de ParisCNESLAB Université de BordeauxLAB Université de BordeauxCNESDepartment of Geophysics, Tohoku UniversityHokkaido Information UniversityCNESLESIA-Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de ParisCNESDepartment of Geophysics, Tohoku UniversityAix Marseille Univ. CNRS, CNES, LAMLESIA-Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de ParisAbstract 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. Graphical Abstracthttps://doi.org/10.1186/s40623-021-01423-2MIRSMMXImaging spectrometerPhobosDeimosMars
spellingShingle Maria Antonietta Barucci
Jean-Michel Reess
Pernelle Bernardi
Alain Doressoundiram
Sonia Fornasier
Michel Le Du
Takahiro Iwata
Hiromu Nakagawa
Tomoki Nakamura
Yves André
Shohei Aoki
Takehiko Arai
Elisa Baldit
Pierre Beck
Jean-Tristan Buey
Elisabet Canalias
Matthieu Castelnau
Sebastien Charnoz
Marc Chaussidon
Fréderic Chapron
Valerie Ciarletti
Marco Delbo
Bruno Dubois
Stephane Gauffre
Thomas Gautier
Hidenori Genda
Rafik Hassen-Khodja
Gilles Hervet
Ryuki Hyodo
Christian Imbert
Takeshi Imamura
Laurent Jorda
Shingo Kameda
Driss Kouach
Toru Kouyama
Takeshi Kuroda
Hiroyuki Kurokawa
Laurent Lapaw
Jeremie Lasue
Laetitia Le Deit
Aurélien Ledot
Cedric Leyrat
Bertrand Le Ruyet
Moe Matsuoka
Frederic Merlin
Hideaki Miyamoto
Frederic Moynier
Napoleon Nguyen Tuong
Kazunori Ogohara
Takahito Osawa
Jérôme Parisot
Laurie Pistre
Benjamin Quertier
Sean N. Raymond
Francis Rocard
Takeshi Sakanoi
Takao M. Sato
Eric Sawyer
Fériel Tache
Sylvain Trémolières
Fuminori Tsuchiya
Pierre Vernazza
Didier Zeganadin
MIRS: an imaging spectrometer for the MMX mission
Earth, Planets and Space
MIRS
MMX
Imaging spectrometer
Phobos
Deimos
Mars
title MIRS: an imaging spectrometer for the MMX mission
title_full MIRS: an imaging spectrometer for the MMX mission
title_fullStr MIRS: an imaging spectrometer for the MMX mission
title_full_unstemmed MIRS: an imaging spectrometer for the MMX mission
title_short MIRS: an imaging spectrometer for the MMX mission
title_sort mirs an imaging spectrometer for the mmx mission
topic MIRS
MMX
Imaging spectrometer
Phobos
Deimos
Mars
url https://doi.org/10.1186/s40623-021-01423-2
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