Abstract
A growing body of evidence suggests that the deep oceans during the early Paleozoic Era were widely oxygen deficient, despite evidence for increased marine oxygenation during the Neoproterozoic. However, the temporal and geographic extents and dynamics of reducing marine conditions within these oceans are not well understood. Here, we investigate marine redox history during the Drumian through the earliest Jiangshanian International Stages of the Cambrian Period, using concentrations of redox-sensitive metals (vanadium, uranium, and molybdenum), iron speciation, and Mo isotope stratigraphy of the Alum Shale Formation of Scandinavia. These data suggest a major perturbation occurred in trace metal cycling during the later Cambrian Period that was linked to a transient change in marine redox conditions coincident with the well-known Steptoean Positive Isotope Excursion or SPICE. The δ98Mo measurements of the Alum shale show systematic variations during the interval that contains the SPICE which are broadly consistent with a transient expansion of sulfidic, reducing marine environments — indicating a significant exacerbation of an already-common condition during the Cambrian Period. Additionally, iron speciation data record a local transition from predominantly anoxic, ferruginous (Fe+2 containing) to anoxic, euxinic (sulfide containing) water column conditions near the initiation of the SPICE. Trace metal abundances, however, appear to decline well before the start of the SPICE, suggesting an earlier initiation of the global expansion of reducing environments. More broadly, our data and modeling support the notion that significant portions of the oceans remained oxygen deficient throughout the later portion of the Cambrian, and that these oceans were also prone to transient intervals of more reducing conditions similar to the Oceanic Anoxic Events of the Mesozoic.
Originalsprog | Engelsk |
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Artikelnummer | 110623 |
Tidsskrift | Palaeogeography, Palaeoclimatology, Palaeoecology |
Vol/bind | 581 |
Antal sider | 15 |
ISSN | 0031-0182 |
DOI | |
Status | Udgivet - 2021 |
Bibliografisk note
Funding Information:We appreciate the editorial guidance of Junpeng Zhang and Thomas Algeo and the constructive reviews by three anonymous reviewers that all helped improve our manuscript. Our thanks go to Per Ahlberg, Mats Eriksson, and Fredrik Terfelt assisting with access and sampling of the Andrarum-3 core at the Department of Geology at Lund University. We also thank Christopher Reinhard, Jeremy Owens, Robert Raiswell, Arne T. Nielsen, and Niels Schovsbo for discussions of the data from the Alum. We would also like to acknowledge Laura Wasylenki for assistance with Mo isotopes analyses. BCG, TWL, and ADA wish to thank the National Science Foundation for financial support of this study (UCR: EAR-0719911 and ASU: EAR- 0720210). TWD thanks NASA Planetary Biology Internship, Nordic Center for Earth Evolution (DNRF-53), and the Villum Foundation (ID: 1168439 and VKR023127) and the Carlsberg Foundation (CF16?0876). EUH thanks the Nordic Center for Earth Evolution (DNRF-53), the Villum Foundation (16518), and the Swedish Research Council (2019-05254). MAL was supported by the National Science Foundation Graduate Research Fellowship Program (NSF-GRFP). The NASA Astrobiology Institute under Cooperative Agreement No. NNA15BB03A issued through the Science Mission Directorate also provided funds (TWL). Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation
Funding Information:
We appreciate the editorial guidance of Junpeng Zhang and Thomas Algeo and the constructive reviews by three anonymous reviewers that all helped improve our manuscript. Our thanks go to Per Ahlberg, Mats Eriksson, and Fredrik Terfelt assisting with access and sampling of the Andrarum-3 core at the Department of Geology at Lund University. We also thank Christopher Reinhard, Jeremy Owens, Robert Raiswell, Arne T. Nielsen, and Niels Schovsbo for discussions of the data from the Alum. We would also like to acknowledge Laura Wasylenki for assistance with Mo isotopes analyses. BCG, TWL, and ADA wish to thank the National Science Foundation for financial support of this study ( UCR: EAR-0719911 and ASU: EAR- 0720210 ). TWD thanks NASA Planetary Biology Internship, Nordic Center for Earth Evolution ( DNRF-53 ), and the Villum Foundation (ID: 1168439 and VKR023127 ) and the Carlsberg Foundation ( CF16–0876 ). EUH thanks the Nordic Center for Earth Evolution ( DNRF-53 ), the Villum Foundation ( 16518 ), and the Swedish Research Council ( 2019-05254 ). MAL was supported by the National Science Foundation Graduate Research Fellowship Program ( NSF-GRFP ). The NASA Astrobiology Institute under Cooperative Agreement No. NNA15BB03A issued through the Science Mission Directorate also provided funds (TWL). Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation
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© 2021 Elsevier B.V.