MIRS: an imaging spectrometer for the MMX mission

被引：19

作者：

Barucci, Maria Antonietta ^{[1
]}

Reess, Jean-Michel ^{[1
]}

Bernardi, Pernelle ^{[1
]}

Doressoundiram, Alain ^{[1
]}

Fornasier, Sonia ^{[1
]}

Le Du, Michel ^{[2
]}

Iwata, Takahiro ^{[3
]}

Nakagawa, Hiromu ^{[4
]}

Nakamura, Tomoki ^{[4
]}

Andre, Yves ^{[2
]}

Aoki, Shohei ^{[3
]}

Arai, Takehiko ^{[6
]}

Baldit, Elisa ^{[2
]}

Beck, Pierre ^{[7
]}

Buey, Jean-Tristan ^{[1
]}

Canalias, Elisabet ^{[2
]}

Castelnau, Matthieu ^{[2
]}

Charnoz, Sebastien ^{[8
]}

Chaussidon, Marc ^{[8
]}

Chapron, Frederic ^{[1
]}

Ciarletti, Valerie ^{[9
]}

Delbo, Marco ^{[10
]}

Dubois, Bruno ^{[11
]}

Gauffre, Stephane ^{[12
]}

Gautier, Thomas ^{[9
]}

Genda, Hidenori ^{[13
]}

Hassen-Khodja, Rafik ^{[9
]}

Hervet, Gilles ^{[2
]}

Hyodo, Ryuki ^{[3
]}

Imbert, Christian ^{[2
]}

Imamura, Takeshi ^{[14
]}

Jorda, Laurent ^{[15
]}

Kameda, Shingo ^{[16
]}

Kouach, Driss ^{[11
]}

Kouyama, Toru ^{[17
]}

Kuroda, Takeshi ^{[4
]}

Kurokawa, Hiroyuki ^{[13
]}

Lapaw, Laurent ^{[9
]}

Lasue, Jeremie ^{[18
]}

Le Deit, Laetitia ^{[19
]}

Ledot, Aurelien ^{[2
]}

Leyrat, Cedric ^{[1
]}

Le Ruyet, Bertrand ^{[1
]}

Matsuoka, Moe ^{[1
]}

Merlin, Frederic ^{[1
]}

Miyamoto, Hideaki ^{[14
]}

Moynier, Frederic ^{[8
]}

Napoleon Nguyen Tuong ^{[1
]}

Ogohara, Kazunori ^{[20
]}

Osawa, Takahito ^{[21
]}

机构：

[1] Univ Paris, LESIA Observ Paris, Univ PSL, CNRS,Sorbonne Univ, 5 Pl Jules Janssen, F-92195 Meudon, France

[2] CNES, Toulouse, France

[3] ISAS JAXA, Sagamihara, Kanagawa, Japan

[4] Tohoku Univ, Dept Geophys, Sendai, Miyagi 9808578, Japan

[5] CNES, Paris, France

[6] Ashikaga Univ, Ashikaga, Japan

[7] Univ Grenoble Alpes, IPAG, CNRS, Grenoble, France

[8] Univ Paris, Inst Phys Globe Paris, CNRS, Paris, France

[9] Sorbonne Univ, UVSQ Univ Paris Saclay, LATMOS IPSL, CNRS, Guyancourt, France

[10] CNRS, Observ Cote dAzur, Nice, France

[11] Observatoire Midi Pyrenees, Toulouse, France

[12] LAB Univ Bordeaux, Bordeaux, France

[13] Tokyo Inst Technol, Earth Life Sci Inst, Tokyo, Japan

[14] Univ Tokyo, Tokyo, Japan

[15] Lab Astrophys Marseille, Marseille, France

[16] Rikkyo Univ, Tokyo, Japan

[17] NIAIST, Tokyo, Japan

[18] IRAP, Toulouse, France

[19] Univ Angers, Univ Nantes, LPG, UMR CNRS 6112, Nantes, France

[20] Kyoto Sangyo Univ, Kyoto, Japan

[21] Japan Atom Energy Agcy, Tokai, Ibaraki, Japan

[22] Hokkaido Informat Univ, Ebetsu, Hokkaido, Japan

[23] Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France

来源：

EARTH PLANETS AND SPACE | 2021年 / 73卷 / 01期

关键词：

MIRS; MMX; Imaging spectrometer; Phobos; Deimos; Mars; CO2 ICE CLOUDS; WATER-VAPOR; MARTIAN ATMOSPHERE; PHOTOMETRIC PROPERTIES; INFRARED OBSERVATIONS; SURFACE REFLECTANCE; SPECTRAL PROPERTIES; SEASONAL-VARIATIONS; CHAOTIC OBLIQUITY; MARS EXPRESS;

D O I：

10.1186/s40623-021-01423-2

中图分类号：

P [天文学、地球科学];

学科分类号：

07 ;

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.

引用

页数：28

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