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Evidence for perchlorates and the origin of chlorinated hydrocarbons detected by SAM at the Rocknest aeolian deposit in Gale Crater

Authors :
Glavin, Daniel P.
Freissinet, Caroline
Miller, Kristen E.
Eigenbrode, Jennifer L.
Brunner, Anna E.
Buch, Arnaud
Sutter, Brad
Douglas Archer Jr., P.
Atreya, Sushil K.
Brinckerhoff, William B.
Cabane, Michel
Coll, Patrice
Conrad, Pamela G.
Coscia, David
Dworkin, Jason P.
Franz, Heather B.
Grotzinger, John P.
Leshin, Laurie A.
Martin, Mildred G.
Mckay, Christopher
Ming, Douglas W.
Navarro-González, Rafael
Pavlov, Alexander
Steele, Andrew
Summons, Roger E.
Szopa, Cyril
Teinturier, Samuel
Mahaffy, Paul R.
NASA Goddard Space Flight Center (GSFC)
Department of Earth, Atmospheric and Planetary Sciences [MIT, Cambridge] (EAPS)
Massachusetts Institute of Technology (MIT)
Center for Research and Exploration in Space Science and Technology [GSFC] (CRESST)
Laboratoire de Génie des Procédés et Matériaux - EA 4038 (LGPM)
CentraleSupélec
NASA Johnson Space Center (JSC)
NASA
Department of Atmospheric, Oceanic, and Space Sciences [Ann Arbor] (AOSS)
University of Michigan [Ann Arbor]
University of Michigan System-University of Michigan System
PLANETO - LATMOS
Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS)
Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
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)
California Institute of Technology (CALTECH)
Rensselaer Polytechnic Institute (RPI)
Catholic University of America
NASA Ames Research Center (ARC)
Laboratorio de Química de Plasmas y Estudios Planetarios [Mexico]
Instituto de Ciencias Nucleares [Mexico]
Universidad Nacional Autónoma de México = National Autonomous University of Mexico (UNAM)-Universidad Nacional Autónoma de México = National Autonomous University of Mexico (UNAM)
Geophysical Laboratory [Carnegie Institution]
Carnegie Institution for Science
Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Universidad Nacional Autónoma de México (UNAM)-Universidad Nacional Autónoma de México (UNAM)
Carnegie Institution for Science [Washington]
IMPEC - LATMOS
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)
Source :
Journal of Geophysical Research. Planets, Journal of Geophysical Research. Planets, 2013, 118 (10), pp.1955-1973. ⟨10.1002/jgre.20144⟩, Journal of Geophysical Research. Planets, Wiley-Blackwell, 2013, 118 (10), pp.1955-1973. ⟨10.1002/jgre.20144⟩
Publication Year :
2013
Publisher :
HAL CCSD, 2013.

Abstract

International audience; A single scoop of the Rocknest aeolian deposit was sieved (2 released from the Rocknest sample and the decomposition of a product of N-methyl-N-(tert-butyldimethylsilyl)-trifluoroacetamide (MTBSTFA), a chemical whose vapors were released from a derivatization cup inside SAM. The best candidate for the oxychlorine compounds in Rocknest is a hydrated calcium perchlorate (Ca(ClO4)2*nH2O), based on the temperature release of O2 that correlates with the release of the chlorinated hydrocarbons measured by SAM, although other chlorine-bearing phases are being considered. Laboratory analog experiments suggest that the reaction of Martian chlorine from perchlorate decomposition with terrestrial organic carbon from MTBSTFA during pyrolysis can explain the presence of three chloromethanes and a chloromethylpropene detected by SAM. Chlorobenzene may be attributed to reactions of Martian chlorine released during pyrolysis with terrestrial benzene or toluene derived from 2,6-diphenylphenylene oxide (Tenax) on the SAM hydrocarbon trap. At this time we do not have definitive evidence to support a nonterrestrial carbon source for these chlorinated hydrocarbons, nor do we exclude the possibility that future SAM analyses will reveal the presence of organic compounds native to the Martian regolith.

Details

Language :
English
ISSN :
21699097 and 21699100
Database :
OpenAIRE
Journal :
Journal of Geophysical Research. Planets, Journal of Geophysical Research. Planets, 2013, 118 (10), pp.1955-1973. ⟨10.1002/jgre.20144⟩, Journal of Geophysical Research. Planets, Wiley-Blackwell, 2013, 118 (10), pp.1955-1973. ⟨10.1002/jgre.20144⟩
Accession number :
edsair.dedup.wf.001..e7927ed3518aa45d1b524d3d89e8322a
Full Text :
https://doi.org/10.1002/jgre.20144⟩