• Medientyp: E-Artikel
  • Titel: MIRS: an imaging spectrometer for the MMX mission
  • Beteiligte: Barucci, Maria Antonietta; Reess, Jean-Michel; Bernardi, Pernelle; Doressoundiram, Alain; Fornasier, Sonia; Le Du, Michel; Iwata, Takahiro; Nakagawa, Hiromu; Nakamura, Tomoki; André, Yves; Aoki, Shohei; Arai, Takehiko; Baldit, Elisa; Beck, Pierre; Buey, Jean-Tristan; Canalias, Elisabet; Castelnau, Matthieu; Charnoz, Sebastien; Chaussidon, Marc; Chapron, Fréderic; Ciarletti, Valerie; Delbo, Marco; Dubois, Bruno; Gauffre, Stephane; [...]
  • Erschienen: Springer Science and Business Media LLC, 2021
  • Erschienen in: Earth, Planets and Space
  • Umfang:
  • Sprache: Englisch
  • DOI: 10.1186/s40623-021-01423-2
  • ISSN: 1880-5981
  • Schlagwörter: Space and Planetary Science ; Geology
  • Zusammenfassung: <jats:title>Abstract</jats:title><jats:p>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.</jats:p> <jats:p><jats:bold>Graphical Abstract</jats:bold></jats:p>
  • Beschreibung: <jats:title>Abstract</jats:title><jats:p>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.</jats:p>
    <jats:p><jats:bold>Graphical Abstract</jats:bold></jats:p>
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  • Zugangsstatus: Freier Zugang