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Towards Martian Moons Exploration: micro-Raman and VIS-MIR reflection spectroscopy of the Phobos surface simulants

Pavlov, Sergey and Böttger, Ute and Weber, I. and Stoijc, A.N. and Säuberlich, Thomas and Pohl, Andreas and Rodd-Routley, Selene and Cho, Y. and Rull, Fernando and Hübers, Heinz-Wilhelm and Belenguer, Tomas and Börner, Anko and Buder, Maximilian and Bunduki, Y. and Dietz, Enrico and Hagelschuer, Till and Kameda, S. and Kopp, Emanuel and Moral Inza, A. G. and Mori, S. and Perez Canora, C. and Pertenais, Martin and Peter, Gisbert and Prieto-Ballesteros, O. and Rockstein, Steve and Rodriguez Perez, P. and Ryan, Conor and Santamaria, P. and Schrandt, Friedrich and Schröder, Susanne and Ulamec, Stephan and Usui, Tomohiro and Westerdorff, Karsten (2021) Towards Martian Moons Exploration: micro-Raman and VIS-MIR reflection spectroscopy of the Phobos surface simulants. THE TWELFTH MOSCOW SOLAR SYSTEM SYMPOSIUM 2021, 2021-10-11 - 2021-10-15, Moskau, Russland. doi: 10.21046/12M-S3. ISBN 978-5-00015-015-3.

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Official URL: https://ms2021.cosmos.ru/docs/2021/12ms3_book_5.pdf

Abstract

The Japan Aerospace Exploration Agency (JAXA)’ Martian Moons eXploration (MMX) remote sensing, robotic and sample return mission, scheduled to be launched in 2024 and to return in 2029, will have a strong focus on studying Phobos, including close-up surface analysis and collecting samples for Earth return. A rover, provided by CNES and DLR, will be deployed to Phobos. Its payload includes the Raman spectrometer (RAX) for in-situ characterization of the surface composition. Characterization of payload instrumentation by measurements of planetary simulants is a crucial test for performance and prediction of scientific yield. Controversial conclusions on similarity of infrared reflection and imaging of Phobos to those of low-albedo asteroids imply that combined optical spectroscopy studies will prepare a set of possible clues shortly before the MMX mission. Different Phobos simulants were selected and have been used for Raman and broad range (visible-to-mid-infrared) reflection spectroscopy in order to provide critical parameters on detectivity of mineral phases in the sample matrix as well as to compare the close-up spectroscopy with the known remote sensing of Phobos surface by previous Earth-based observatories and planetary missions.

Item URL in elib:https://elib.dlr.de/144551/
Document Type:Conference or Workshop Item (Poster)
Title:Towards Martian Moons Exploration: micro-Raman and VIS-MIR reflection spectroscopy of the Phobos surface simulants
Authors:
AuthorsInstitution or Email of AuthorsAuthor's ORCID iDORCID Put Code
Pavlov, SergeyUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Böttger, UteUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Weber, I.Institut für Planetologie, WWU Münster, GermanyUNSPECIFIEDUNSPECIFIED
Stoijc, A.N.Westfälische Wilhelms-Universität MünsterUNSPECIFIEDUNSPECIFIED
Säuberlich, ThomasUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Pohl, AndreasUNSPECIFIEDhttps://orcid.org/0009-0005-5091-6476UNSPECIFIED
Rodd-Routley, SeleneUNSPECIFIEDhttps://orcid.org/0000-0002-8864-0891UNSPECIFIED
Cho, Y.The University of Tokyo, Tokyo 113-0033, JapanUNSPECIFIEDUNSPECIFIED
Rull, FernandoDepartment of Condensed Matter Physics, Crystallography and Mineralogy, Valladolid University, Valladolid, Spain.UNSPECIFIEDUNSPECIFIED
Hübers, Heinz-WilhelmUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Belenguer, TomasInstituto National de Técnica Aerospacial (INTA)UNSPECIFIEDUNSPECIFIED
Börner, AnkoUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Buder, MaximilianUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Bunduki, Y.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Dietz, EnricoUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Hagelschuer, TillUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Kameda, S.Rikkyo University, Tokyo 171-8501, JapanUNSPECIFIEDUNSPECIFIED
Kopp, EmanuelUNSPECIFIEDhttps://orcid.org/0000-0003-3450-906XUNSPECIFIED
Moral Inza, A. G.Instituto National de Técnica Aerospacial (INTA)UNSPECIFIEDUNSPECIFIED
Mori, S.The University of Tokyo, Tokyo, JapanUNSPECIFIEDUNSPECIFIED
Perez Canora, C.Instituto National de Técnica Aerospacial (INTA)UNSPECIFIEDUNSPECIFIED
Pertenais, MartinUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Peter, GisbertUNSPECIFIEDhttps://orcid.org/0000-0001-6101-2513UNSPECIFIED
Prieto-Ballesteros, O.Laboratorio de Geologia Planetaria, Centro de Astrobiologia-INTA-CSIC, Ctra. Ajalvir km.4, Torrejon de Ardoz, Madrid, SpainUNSPECIFIEDUNSPECIFIED
Rockstein, SteveDLR, Institut für Optische SensorsystemeUNSPECIFIEDUNSPECIFIED
Rodriguez Perez, P.Instituto National de Técnica Aerospacial (INTA)UNSPECIFIEDUNSPECIFIED
Ryan, ConorDLR, Institut für Optische SensorsystemeUNSPECIFIEDUNSPECIFIED
Santamaria, P.Instituto National de Técnica Aerospacial (INTA)UNSPECIFIEDUNSPECIFIED
Schrandt, FriedrichUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Schröder, SusanneUNSPECIFIEDhttps://orcid.org/0000-0003-1870-3663UNSPECIFIED
Ulamec, StephanUNSPECIFIEDhttps://orcid.org/0000-0002-8856-4622UNSPECIFIED
Usui, TomohiroJapan Aerospace Exploration Agency (JAXA), Institute of Space and Astronautical ScienceUNSPECIFIEDUNSPECIFIED
Westerdorff, KarstenUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Date:2021
Refereed publication:Yes
Open Access:Yes
Gold Open Access:No
In SCOPUS:No
In ISI Web of Science:No
DOI:10.21046/12M-S3
Page Range:pp. 78-80
ISBN:978-5-00015-015-3
Status:Published
Keywords:RAX, MMX, Phobos, Raman spectroscopy, infrared spectroscopy, planetary simulants
Event Title:THE TWELFTH MOSCOW SOLAR SYSTEM SYMPOSIUM 2021
Event Location:Moskau, Russland
Event Type:international Conference
Event Start Date:11 October 2021
Event End Date:15 October 2021
HGF - Research field:Aeronautics, Space and Transport
HGF - Program:Space
HGF - Program Themes:Space System Technology
DLR - Research area:Raumfahrt
DLR - Program:R SY - Space System Technology
DLR - Research theme (Project):R - Detectors for optical instruments
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Optical Sensor Systems > Terahertz and Laser Spectroscopy
Deposited By: Pavlov, Dr. Sergey
Deposited On:19 Oct 2021 10:04
Last Modified:24 Apr 2024 20:43

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