論文

査読有り 本文へのリンクあり
2021年12月

MIRS: an imaging spectrometer for the MMX mission

Earth, Planets and Space
  • 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

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記述言語
掲載種別
研究論文(学術雑誌)
DOI
10.1186/s40623-021-01423-2

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: [Figure not available: see fulltext.].

リンク情報
DOI
https://doi.org/10.1186/s40623-021-01423-2
Scopus
https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85120824686&origin=inward 本文へのリンクあり
Scopus Citedby
https://www.scopus.com/inward/citedby.uri?partnerID=HzOxMe3b&scp=85120824686&origin=inward
ID情報
  • DOI : 10.1186/s40623-021-01423-2
  • ISSN : 1343-8832
  • eISSN : 1880-5981
  • SCOPUS ID : 85120824686

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