Earth, Planets and Space | |
In situ science on Phobos with the Raman spectrometer for MMX (RAX): preliminary design and feasibility of Raman measurements | |
Olga Prieto-Ballesteros1  Koki Yumoto2  Yuichiro Cho2  Jo Akino Ogura2  Shoki Mori2  Shingo Kameda3  Iris Weber4  Claudia Stangarone5  Ute Böttger6  Emanuel Kopp6  Yuri Bunduki6  Susanne Schröder6  Anko Börner6  Carsten Paproth6  Conor Ryan6  Friedrich Schrandt6  Heinz-Wilhelm Hübers6  Gisbert Peter6  Karsten Westerdorff6  Matthias Lieder6  Till Hagelschuer6  Martin Pertenais6  Maximilian Buder6  Enrico Dietz6  Selene Rodd-Routley6  Thomas Säuberlich6  Steve Rockstein6  Tomohiro Usui7  Andoni Gaizka Moral Inza8  Pablo Rodriguez Perez8  Carlos Perez Canora8  Pilar Santamaria8  Tomàs Belenguer8  Stephan Ulamec9  Guillermo Lopez-Reyes1,10  Fernando Rull1,10  | |
[1] Centro de Astrobiología (CAB-INTA-CSIC), Ctra. Ajalvir, Km 4, 28850, Torrejón de Ardoz, Spain;Department of Earth and Planetary Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo, 113-0033, Tokyo, Japan;Department of Physics, College of Science, Rikkyo University, 3-34-1 Nishiikebukuro, Toshima, 171-8501, Tokyo, Japan;Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodai, Chuo, 252-5210, Sagamihara, Kanagawa, Japan;Institut für Planetologie, WWU Münster, Wilhelm-Klemm-Str. 10, 48149, Münster, Germany;Institute for Planetary Research, Deutsches Zentrum für Luft- und Raumfahrt e.V. (DLR), Rutherfordstr. 2, 12489, Berlin, Germany;Institute of Optical Sensor Systems, Deutsches Zentrum für Luft- und Raumfahrt e.V. (DLR), Rutherfordstr. 2, 12489, Berlin, Germany;Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodai, Chuo, 252-5210, Sagamihara, Kanagawa, Japan;Instituto Nacional de Técnica Aerospacial (INTA), Ctra. Ajalvir, Km 4, 28850, Torrejón de Ardoz, Spain;Space Operations and Astronaut Training, Deutsches Zentrum für Luft- und Raumfahrt e.V. (DLR), Linder Höhe, 51147, Cologne, Germany;Universidad de Valladolid - GIR ERICA, Av. Francisco valles, 8, Parque Tecnólogico de Boecillo, Parcela 203, 47151, Boecillo, Valladolid, Spain; | |
关键词: Raman spectroscopy; Raman spectrometer for MMX (RAX); Phobos; Mineralogy; In situ analysis; Sample return; Martian Moons eXploration (MMX); | |
DOI : 10.1186/s40623-021-01496-z | |
来源: Springer | |
【 摘 要 】
Mineralogy is the key to understanding the origin of Phobos and its position in the evolution of the Solar System. In situ Raman spectroscopy on Phobos is an important tool to achieve the scientific objectives of the Martian Moons eXploration (MMX) mission, and maximize the scientific merit of the sample return by characterizing the mineral composition and heterogeneity of the surface of Phobos. Conducting in situ Raman spectroscopy in the harsh environment of Phobos requires a very sensitive, compact, lightweight, and robust instrument that can be carried by the compact MMX rover. In this context, the Raman spectrometer for MMX (i.e., RAX) is currently under development via international collaboration between teams from Japan, Germany, and Spain. To demonstrate the capability of a compact Raman system such as RAX, we built an instrument that reproduces the optical performance of the flight model using commercial off-the-shelf parts. Using this performance model, we measured mineral samples relevant to Phobos and Mars, such as anhydrous silicates, carbonates, and hydrous minerals. Our measurements indicate that such minerals can be accurately identified using a RAX-like Raman spectrometer. We demonstrated a spectral resolution of approximately 10 cm−1, high enough to resolve the strongest olivine Raman bands at ~ 820 and ~ 850 cm−1, with highly sensitive Raman peak measurements (e.g., signal-to-noise ratios up to 100). These results strongly suggest that the RAX instrument will be capable of determining the minerals expected on the surface of Phobos, adding valuable information to address the question of the moon’s origin, heterogeneity, and circum-Mars material transport.Graphical Abstract
【 授权许可】
CC BY
【 预 览 】
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