Molybdenum speciation tracking hydrocarbon migration in fine-grained sedimentary rocks

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  • Omid H. Ardakani, Natural Resources Canada, University of Calgary
  • ,
  • Stephan R. Hlohowskyj, Central Michigan University
  • ,
  • Anthony Chappaz, Central Michigan University
  • ,
  • Hamed Sanei
  • Mastaneh H. Liseroudi, University of Calgary
  • ,
  • James M. Wood, Calaber1 Resources

Molybdenum (Mo) systematics (i.e., total concentration and isotope ratios) are widely used for the reconstruction of paleo-redox conditions in sedimentary records. However, the geochemical processes affecting the distribution of Mo in carbonaceous fine-grained sedimentary rocks remain unclear. This study investigates how the organic matter type may control Mo concentration and speciation in siltstone/shale strata of the Lower Triassic Montney Formation in the Western Canadian Sedimentary Basin (WCSB) to identify the effects of hydrocarbon expulsion and migration, fluid/rock interactions, and thermal maturity on Mo geochemistry when used as a paleo-redox proxy. The bulk Mo concentration in the studied samples varies from 0.2 to 86 ppm (mean = 13 ± 16.7 ppm), with Mo enrichment factors of 22.7 ± 24.4 suggesting an anoxic paleo-depositional setting. The X-ray Absorption Near Edge Spectroscopy (XANES) results show the presence of two separate Mo species within distinct geographic locations: (1) a group with a higher average Mo oxidation state where Mo is mostly surrounded by oxygen (O) atoms in an octahedral configuration, and (2) a group showing a lower average Mo oxidation state where Mo is mostly surrounded by sulfur (S) atoms in a tetrahedral configuration. The reduced Mo species are distributed in the vicinity of fault-related hydrothermal diagenesis/dolomitization zones. In contrast, the oxidized Mo species are found associated with samples enriched with solid bitumen/pyrobitumen. The results of our study show Mo speciation can significantly help to elucidate complex paleo-redox histories.

OriginalsprogEngelsk
TidsskriftGeochimica et Cosmochimica Acta
Vol/bind283
Sider (fra-til)136-148
ISSN0016-7037
DOI
StatusUdgivet - aug. 2020

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