Quick
Search: 
 
advanced search
 GSW Home    GeoRef Home    My GSW Alerts    Contact GSW    About GSW    Journals List    Help 
Geology Email Content Delivery
JOURNAL HOME HELP CONTACT PUBLISHER SUBSCRIBE ARCHIVE SEARCH TABLE OF CONTENTS

Geology; June 2004; v. 32; no. 6; p. 533-536; DOI: 10.1130/G20323.1
© 2004 Geological Society of America
This Article
Right arrow Figures Only
Right arrow Full Text
Right arrow Full Text (PDF)
Right arrow Alert me when this article is cited
Right arrow Alert me if a correction is posted
Services
Right arrow Email this article to a friend
Right arrow Similar articles in this journal
Right arrow Alert me to new issues of the journal
Right arrow Download to citation manager
Right arrow reprints & permissions
Citing Articles
Right arrow Citing Articles via Google Scholar
Google Scholar
Right arrow Articles by Potter, J.
Right arrow Articles by Tsypukov, M.
Right arrow Search for Related Content
GeoRef
Right arrow GeoRef Citation

Large-scale carbon isotope fractionation in evaporites and the generation of extremely 13C-enriched methane

Joanna Potter*,1, Michael G. Siemann*,1 and Mikhail Tsypukov*,2

1 Institut für Mineralogie und Mineralische Rohstoffe, Technische Universität Clausthal, Adolph-Roemer Strasse 2a, 38678 Clausthal-Zellerfeld, Germany
2 Institut für Mineralogie und Mineralische Rohstoffe, Technische Universität Clausthal, Adolph-Roemer Strasse 2a, 38678 Clausthal-Zellerfeld, Germany, and Institute of Geochemistry, Russian Academy of Science, Irkutsk, Russia

Petrographic, fluid-inclusion, geochemical, and gas stable isotope data are reported here for a Permian Zechstein evaporite sequence. This deposit is a geochemically unaltered sequence. Bromine concentrations show a continuous evaporation profile with little postdepositional alteration in halite chemistry. Bacterial fermentation gases, identified in primary inclusions, change from an N2-H2S composition in the lower-middle halite series to a CH4-H2 composition in the upper halite and potash series. Carbon isotope results for CH4 show a 13C enrichment up-sequence from typical biogenic values of –45{per thousand} to –50{per thousand} to extremely unusual 13C-enriched values as high as +21{per thousand}. The {delta}D values for these 13C-enriched CH4 gases range from –240{per thousand} to –377{per thousand}. A model is proposed for the formation of the CH4 gases whereby the dominant isotopic fractionation process controlling the system was evaporation of the brines. This generated a progressive 13C enrichment in the carbon in the residual brines due to preferential loss of 12CO2 to the atmosphere. The resulting CH4 generated in the sediments, as evaporation and precipitation advanced, recorded this 13C enrichment in the carbon reservoir. Therefore, the isotopic profile observed in this sequence today represents a primary feature with little evidence for postdepositional migration.

Key Words: methane • evaporites • stable isotopes • fluid inclusions







JOURNAL HOME HELP CONTACT PUBLISHER SUBSCRIBE ARCHIVE SEARCH TABLE OF CONTENTS
Copyright © 2009 by Geological Society of America