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Shells of oysters (Ostreidae) are predominantly composed of foliated and chalky calcite microstructures. The formation process of the more porous chalky structure is subject to debate, with some studies suggesting that it is not formed directly by the oyster but rather through microbial mineralization within the shell. Here, this hypothesis is tested in modern shells of the Pacific oyster (Crassostrea gigas) from coastal regions in France and the Netherlands. We combine measurements of stable carbon, oxygen, nitrogen, sulfur, and clumped isotope ratios with high-resolution spatially resolved element (Na, Mg, Cl, S, Mn and Sr) data and microscopic observations of chalky and foliated microstructures in the oyster shells. Our results show no isotopic differences between the different microstructures, arguing against formation of the chalky calcite by microorganisms. However, we observe a small difference in the oxygen isotope ratio (0.32‰) and clumped isotope composition (0.017‰) between the microstructures, which is likely caused by sampling biases due to seasonal differences in growth rate and the short timespan over which the chalky microstructure forms. We therefore recommend sampling profiles through the foliated microstructure to control for strong seasonal variability recorded in the shell which can bias environmental reconstructions. High-resolution (25–50 µm) Na, Mg, Cl, S, Mn and Sr profiles yield empirical distribution coefficients between seawater and shell calcite for these elements. Significant differences in element concentrations and distribution coefficients were confirmed between the two microstructures, likely reflecting differences in mineralization rates or inclusion of non-lattice-bound elements. Only Mg/Ca ratios in the foliated microstructure vary predictably with growth seasonality, and we show that these can be used to establish accurate oyster shell chronologies. The observed effect of mineralization rate on element incorporation into oyster shells should be considered while developing potential element proxies for paleoclimate reconstructions. Trace element proxies in oyster shells should be interpreted with caution, especially when element chemical properties were measured in different microstructures.
Originele taal-2 | English |
---|---|
Pagina's (van-tot) | 326-352 |
Aantal pagina's | 27 |
Tijdschrift | Geochimica et Cosmochimica Acta |
Volume | 308 |
DOI's | |
Status | Published - 1 sep 2021 |
Bibliografische nota
Funding Information:NdW is funded by a Marie Skłodowska Curie Individual Fellowship by the European Commission (843011-UNBIAS) and a Junior Postdoc Fellowship by the Flemish Research Council (FWO; 12ZB220N). GJR and LKD acknowledge funding from the Netherlands Earth System Science Center (NESSC; grant no. 024.002.001) from the Dutch Ministry for Education, Culture and Science (gravitation grant no. NWO 024.002.001). BRS gratefully acknowledges funding by the Deutsche Forschungsgemeinschaft (DFG; SCHO793/20+23). SG acknowledges support by the Belgian Science Policy (BELSPO) and Research Foundation - Flanders (FWO - Vlaanderen). FV, SG and KR thank FWO for financial support through the EOS-Excellence of Science program (ET-HoME - ID 30442502) and for providing the funding for the acquisition of the MC-ICP-MS instrumentation (ZW15-02 – G0H6216N). AMG and SM acknowledge support for nitrogen isotope analyses by the Max Planck Society. MZ acknowledges funding through the NWO VIDI project 016.161.365, which is financed by the Netherlands Organization for Scientific Research (NWO). XRF instrumentation at the VUB was funded by Hercules infrastructure grants. The authors would like to thank Bart Lippens for help with sample preparation, Arnold van Dijk for laboratory assistance, Wim Boer and Piet van Gaever for vital technical support, Eric Wagemaakers for maintaining the NIOZ jetty continuous measurements, the participants of the 2017 and 2018 edition of the NIOZ Marine Masters Summer School for their contribution to this research and Prof. Philippe Claeys for providing access to the X-Ray Fluorescence platform of the AMGC research group of the Vrije Universiteit Brussel for elemental analyses.
Funding Information:
NdW is funded by a Marie Skłodowska Curie Individual Fellowship by the European Commission (843011-UNBIAS) and a Junior Postdoc Fellowship by the Flemish Research Council (FWO; 12ZB220N). GJR and LKD acknowledge funding from the Netherlands Earth System Science Center (NESSC; grant no. 024.002.001) from the Dutch Ministry for Education, Culture and Science (gravitation grant no. NWO 024.002.001). BRS gratefully acknowledges funding by the Deutsche Forschungsgemeinschaft (DFG; SCHO793/20+23). SG acknowledges support by the Belgian Science Policy (BELSPO) and Research Foundation - Flanders (FWO - Vlaanderen). FV, SG and KR thank FWO for financial support through the EOS-Excellence of Science program (ET-HoME - ID 30442502) and for providing the funding for the acquisition of the MC-ICP-MS instrumentation (ZW15-02 – G0H6216N). AMG and SM acknowledge support for nitrogen isotope analyses by the Max Planck Society. MZ acknowledges funding through the NWO VIDI project 016.161.365, which is financed by the Netherlands Organization for Scientific Research (NWO). XRF instrumentation at the VUB was funded by Hercules infrastructure grants. The authors would like to thank Bart Lippens for help with sample preparation, Arnold van Dijk for laboratory assistance, Wim Boer and Piet van Gaever for vital technical support, Eric Wagemaakers for maintaining the NIOZ jetty continuous measurements, the participants of the 2017 and 2018 edition of the NIOZ Marine Masters Summer School for their contribution to this research and Prof. Philippe Claeys for providing access to the X-Ray Fluorescence platform of the AMGC research group of the Vrije Universiteit Brussel for elemental analyses.
Publisher Copyright:
© 2021 The Author(s)
Copyright:
Copyright 2021 Elsevier B.V., All rights reserved.
Vingerafdruk
Duik in de onderzoeksthema's van 'Multi-isotopic and trace element evidence against different formation pathways for oyster microstructures'. Samen vormen ze een unieke vingerafdruk.-
OZRSRF33: Planetaire archieven om de oorsprong en voortdurende evolutie van de aarde te bestuderen - SRF-mandaat
1/11/19 → 31/10/24
Project: Fundamenteel
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SRP2: Tracers van verleden en heden global changes
Claeys, P., Elskens, M., Huybrechts, P., Gao, Y., Kervyn De Meerendre, M., Claeys, P., Baeyens, W. & Dehairs, F.
1/11/12 → 31/10/24
Project: Fundamenteel
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FWOEOS4: Evolutie en tracers van bewoonbaarheid op Mars en de Aarde
Goderis, S., Claeys, P., Debaille, V., Mattielli, N., Vanhaecke, F., Dehant, V., Javaux, E., Karatekin, O., Vandaele, A. C. & Robert, S.
1/01/18 → 31/12/21
Project: Fundamenteel
Datasets
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Supplementary data to: "Multi-isotopic and trace element evidence against different formation pathways for oyster microstructures"
De Winter, N. (Creator), Dämmer, L. K. (Creator), Falkenroth, M. (Creator), Reichart, G. (Creator), Moretti, S. (Creator), Martínez-García, A. (Creator), Höche, N. (Creator), Schöne, B. R. (Creator), Rodiouchkina, K. (Creator), Goderis, S. (Creator), Vanhaecke, F. (Creator), van Leeuwen, S. M. (Creator) & Ziegler, M. (Creator), Zenodo, 3 mei 2021
Dataset
Uitrusting
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AMGC - Inductively Coupled Plasma Mass Spectrometry Lab.
Philippe Claeys (Scientific coordinator), Christophe Snoeck (Scientific coordinator), Steven Goderis (Scientific coordinator) & Martyna Kopec (Infrastructure coordinator)
Uitrusting/faciliteit: e-resource/single sited
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AMGC - Isotope Ratio Mass Spectrometry Laboratory (IRMS)
Philippe Claeys (Manager) & David Verstraeten (Infrastructure coordinator)
Uitrusting/faciliteit: no e-resource/single sited