MIRS: an imaging spectrometer for the MMX mission

Earth, Planets and Space

Pierre Vernazza¹  Takehiko Arai²  Elisa Baldit³  Yves André³  Gilles Hervet³  Francis Rocard³  Elisabet Canalias³  Matthieu Castelnau³  Eric Sawyer³  Christian Imbert³  Sylvain Trémolières³  Laurie Pistre³  Michel Le Du³  Aurélien Ledot³  Marco Delbo⁴  Takeshi Kuroda⁵  Fuminori Tsuchiya⁵  Hiromu Nakagawa⁵  Takeshi Sakanoi⁵  Tomoki Nakamura⁵  Hidenori Genda⁶  Hiroyuki Kurokawa⁶  Takao M. Sato⁷  Jeremie Lasue⁸  Ryuki Hyodo⁹  Takahiro Iwata⁹  Shohei Aoki⁹  Takahito Osawa^1,10  Kazunori Ogohara^1,11  Sean N. Raymond^1,12  Benjamin Quertier^1,12  Stephane Gauffre^1,12  Laurent Lapaw^1,13  Valerie Ciarletti^1,13  Rafik Hassen-Khodja^1,13  Thomas Gautier^1,13  Napoleon Nguyen Tuong^1,14  Didier Zeganadin^1,14  Jérôme Parisot^1,14  Jean-Tristan Buey^1,14  Cedric Leyrat^1,14  Pernelle Bernardi^1,14  Sonia Fornasier^1,14  Moe Matsuoka^1,14  Frederic Merlin^1,14  Maria Antonietta Barucci^1,14  Alain Doressoundiram^1,14  Jean-Michel Reess^1,14  Fériel Tache^1,14  Bertrand Le Ruyet^1,14  Fréderic Chapron^1,14  Laetitia Le Deit^1,15  Laurent Jorda^1,16  Toru Kouyama^1,17  Driss Kouach^1,18  Bruno Dubois^1,18  Shingo Kameda^1,19  Hideaki Miyamoto^2,20  Takeshi Imamura^2,20  Pierre Beck^2,21  Frederic Moynier^2,22  Marc Chaussidon^2,22  Sebastien Charnoz^2,22 

[1] Aix Marseille Univ. CNRS, CNES, LAM;Ashikaga University;CNES;CNRS, Observatoire Côte d’Azur;Department of Geophysics, Tohoku University;Earth-Life Science Institute, Tokyo Institute of Technology;Hokkaido Information University;IRAP;ISAS JAXA;Japan Atomic Energy Agency;Kyoto Sangyo University;LAB Université de Bordeaux;LATMOS/IPSL, UVSQ Université Paris-Saclay, Sorbonne Université, CNRS;LESIA-Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris;LPG, UMR CNRS 6112, Université de Nantes, Université d’Angers;Laboratoire d’Astrophysique de Marseille;NIAIST;Observatoire Midi-Pyrenées;Rikkyo University;University of Tokyo;Université Grenoble Alpes, CNRS, IPAG;Université de Paris, Institut de Physique du Globe de Paris, CNRS;

关键词: MIRS;    MMX;    Imaging spectrometer;    Phobos;    Deimos;    Mars;   

DOI  :  10.1186/s40623-021-01423-2

来源: DOAJ

【 摘 要 】

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

【 授权许可】

Unknown