Preservation of organic matter in the STONE 6 artificial meteorite experiment

International audience The exposure of a carbonaceous siltstone sample to atmospheric entry, as part of the STONE 6 artificial meteorite experiment, has allowed a controlled investigation of the effect of heat shock during atmospheric entry on organic matter in carbonaceous meteorites and, potential...

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Bibliographic Details
Published in:Icarus
Main Authors: Parnell, John, Bowden, Stephen A., Muirhead, David, Blamey, Nigel, Westall, Frances, Demets, René, Verchovsky, Sasha, Brandstaetter, Franz, Brack, André
Other Authors: School of Geosciences, University of Aberdeen, Centre de biophysique moléculaire (CBM), Université d'Orléans (UO)-Université de Tours (UT)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Institut de Chimie - CNRS Chimie (INC-CNRS)-Centre National de la Recherche Scientifique (CNRS), European Space Research and Technology Centre (ESTEC), Agence Spatiale Européenne = European Space Agency (ESA)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2011
Subjects:
ORCADIAN BASIN
PARENT BODY
MARS
EARTH
LIFE
TAGISH LAKE METEORITE
CARBONACEOUS CHONDRITES
ATMOSPHERIC ENTRY
STRUCTURAL-CHARACTERIZATION
NORTHERN SCOTLAND
Tagish
Tagish Lake
Online Access:https://hal.science/hal-00614953
https://doi.org/10.1016/j.icarus.2010.11.029
Description
Summary:International audience The exposure of a carbonaceous siltstone sample to atmospheric entry, as part of the STONE 6 artificial meteorite experiment, has allowed a controlled investigation of the effect of heat shock during atmospheric entry on organic matter in carbonaceous meteorites and, potentially, sedimentary martian meteorites containing carbonaceous biomolecules. Thermal alteration is evident in an increase in structural order of the carbon (i.e. degree of graphitisation), preferential loss of thermally unstable compounds and substantial loss of extractable organic matter. There is a gradient of increasing alteration towards the outer, exposed margin of the rock, and also an increase in hydrocarbons that suggests outward migration following thermally-induced generation. The carbon has not been completely graphitised, and sufficient biomarker compounds survive to prove the biological origin of the organic matter. The experiment implies that meteorites of appropriate size could preserve evidence of biological activity on their parent body.

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