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Field relationships and stable isotope geochemistry of concretions from James Ross Island, Antarctica

Pirrie, Duncan; Marshall, James D.. 1991 Field relationships and stable isotope geochemistry of concretions from James Ross Island, Antarctica. Sedimentary Geology, 71 (3-4). 137-150. https://doi.org/10.1016/0037-0738(91)90098-X

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Abstract/Summary

Early diagenetic (precompactional) concretions are abundant throughout the Cretaceous-Tertiary Marambio Group Larsen Basin, Antarctica. Four distinct concretion types are recognised: (1) spherical-subspherical concretions: (2) sheet concretions; (3) fossil-nucleated concretions; and (4) concretionary burrow networks. All concretion types have a micritic to microsparry variably non-ferroan to ferroan calcite cement. Stable isotope analyses show a wide spread in both δ18O and δ13C. δ13C values are typically negative, ranging between –3.38 and –39.15%o (PDB) (usually –16 to 230%). δ18O ranges between –1.28 and –13.81% (PDB) with most of the values between –5 and –10%. The δ13C signature is interpreted to represent carbon sourced from sulphate reduction and/or methane oxidation, with minor input from shell dissolution, and is consistent with a shallow burial, early diagenetic origin. A single mudstone hosted concretion has a δ18O composition indicative of precipitation of carbonate from seawater. The low δ18O signatures in the sandstone- and siltstone-hosted concretions are possibly due to early diagenetic modification of the pore water composition through volcaniclastic mineral dissolution/reprecipitation reactions and perhaps through input of meteoric water. Concretion distribution is related to (a) changes in sedimentation rate and (b) the dominance of diffusion on concretion cementation.

Item Type: Publication - Article
Digital Object Identifier (DOI): https://doi.org/10.1016/0037-0738(91)90098-X
ISSN: 00370738
NORA Subject Terms: Earth Sciences
Date made live: 23 May 2018 08:28 +0 (UTC)
URI: https://nora.nerc.ac.uk/id/eprint/520143

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