MIRS: an imaging spectrometer for the MMX mission

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

Earth, Planets and Space（2021）

引用 10|浏览4

暂无评分

摘要

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

查看译文

关键词

MIRS,MMX,Imaging spectrometer,Phobos,Deimos,Mars

AI 理解论文

溯源树

样例

生成溯源树，研究论文发展脉络

Chat Paper

正在生成论文摘要