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Optimization of the TMAH Thermochemolysis Technique for the Detection of Trace Organic Matter on Mars by the SAM and MOMA-Pyr-GC-MS Experiment

Authors :
Buch, A.
Morisson, M.
Szopa, Cyril
Millan, Maeva
Freissinet, Caroline
He, Y.
Glavin, Daniel
Bonnet, Jean-Yves
Coscia, David
Williams, A.
Stalport, F.
Raulin, François
Stambouli, M.
Teinturier, Samuel
Navarro-González, Rafael
Malespin, C.
Mahaffy, Paul
CentraleSupélec
Laboratoire de Génie des Procédés et Matériaux - EA 4038 (LGPM)
PLANETO - LATMOS
Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS)
Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)
Georgetown University [Washington] (GU)
NASA Goddard Space Flight Center (GSFC)
Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)
Towson University [Towson, MD, United States]
University of Maryland System
Laboratoire Interuniversitaire des Systèmes Atmosphériques (LISA (UMR_7583))
Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12)-Centre National de la Recherche Scientifique (CNRS)
Universidad Nacional Autónoma de México (UNAM)
IMPEC - LATMOS
Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Universidad Nacional Autónoma de México = National Autonomous University of Mexico (UNAM)
Buch, Arnaud
Source :
49th LPSC Lunar and Planetary Science Conference 2018, 49th LPSC Lunar and Planetary Science Conference 2018, Mar 2018, Houston, United States
Publication Year :
2018
Publisher :
HAL CCSD, 2018.

Abstract

International audience; Boththe Sample Analysis at Mars (SAM) and Mars Organic Molecule Analyzer (MOMA)instrumentsare able to identify organic material at the Martian surface and subsurface. Both experiments are equipped with pyrolysis-Gas Chromatography-Mass Spectrometry (Pyr-GC-MS)and derivatization reagents (MTBSTFA)that will allowthe analyzerefractory com-pounds,making them more volatile and protecting the labile chemical groups. In order to improve the Pyr-GC-MS analysis, TMAH (tetramethylammonium hydrox-ide) will be used on MOMA and SAM to extract refrac-tory compounds (macromolecules, kerogen, etc.) and protect polar compounds released from the pyrolysis ex-periment.We performed pyrolysis and TMAH-thermochemolysis of a Martian regolith simulant (JSC-Mars-1) to optimizeanalytical parameters, especially the thermochemolysis temperature, to ensure the success of the near future in situthermochemolysis analyses on Mars.

Details

Language :
English
Database :
OpenAIRE
Journal :
49th LPSC Lunar and Planetary Science Conference 2018, 49th LPSC Lunar and Planetary Science Conference 2018, Mar 2018, Houston, United States
Accession number :
edsair.dedup.wf.001..c922c0277549ed0b27d72b22ed289ee3