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Influence of Oxychlorine Phases During the Pyrolysis of Organic Molecules: Implications for the Quest of Organics on Mars with the SAM Experiment Onboard the Curiosity RoverOne among the main objectives of the Sample Analysis at Mars (SAM) experiment is the in situ molecular analysis of gases evolving from solid samples heated up to approximately 850 degrees Centigrade, and collected by Curiosity on Mars surface/sub-surface in Gale crater. With this aim, SAM uses a gas-chromatograph coupled to a quadrupole mass spectrometer (GC-QMS) devoted to separate, detect and identify both volatile inorganic and organic compounds. SAM detected chlorinated organic molecules produced in evolved gas analysis (EGA) experiments. Several of these were also detected by the Viking experiments in 1976. SAM also detected oxychlorine compounds that were present at the Phoenix landing site. The oxychlorines may be prevelant over much of the martian surface. The C1 to C3 aliphatic chlorohydrocarbons (chloromethane and di- and trichloromethane) detected by SAM were attributed to reaction products occurring between the oxychlorines phases and the organic compounds coming from SAM instrument background. But SAM also showed the presence of a large excess of chlorobenzene and C2 to C4 dichloroalkanes among the volatile species released by the Cumberland sample of the Sheepbed mudstone. For the first time in the history of the Mars exploration, this proved the presence of Mars indigenous organic material at the Mars' surface. However, the identification of the precursor organic compounds of these chlorohydrocarbons is difficult due to the complexity of the reactions occurring during the sample pyrolysis. Laboratory pyrolysis experiments have demonstrated that oxychlorines phases such as perchlorates and chlorates, decomposed into dioxygen and volatile chlorine bearing molecules (HCl and/or Cl2) during the pyrolysis. These chemical species can then react with the organic molecules present in the martian solid samples through oxidation, chlorination and oxychlorination processes.
Document ID
20170002283
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Millan, M.
(Universite de Versailles Saint-Quentin-en-Yvelines Versailles, France)
Szopa, C.
(Universite de Versailles Saint-Quentin-en-Yvelines Versailles, France)
Buch, A.
(Ecole Centrale de Paris France)
Belmahdi, I.
(Ecole Centrale de Paris France)
Glavin, D. P.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Freissinet, C.
(Science Collaborator - Postdoc Greenbelt, MD, United States)
Eigenbrode, J. L.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Archer, P. D., Jr,
(Jacobs Technology, Inc. Houston, TX, United States)
Sutter, B.
(Jacobs Technology, Inc. Houston, TX, United States)
Mahaffy, P.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
March 15, 2017
Publication Date
March 20, 2017
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
LPS Paper-2124
JSC-CN-39019
Report Number: LPS Paper-2124
Report Number: JSC-CN-39019
Meeting Information
Meeting: Lunar and Planetary Science Conference (LPSC 2017)
Location: The Woodlands, TX
Country: United States
Start Date: March 20, 2017
End Date: March 24, 2017
Sponsors: Universities Space Research Association, NASA Johnson Space Center, Lunar and Planetary Inst.
Distribution Limits
Public
Copyright
Public Use Permitted.
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