A Geochemical Mechanism for >10 m Apparent Downward Offsets of Magnetic Reversals Inferred From Comparison of Two Scotia Sea Drill Sites

Author:

Reilly Brendan T.1ORCID,Tauxe Lisa2ORCID,Brachfeld Stefanie A.3ORCID,Kenlee Bridget4,Gutjahr Marcus5ORCID,Dale Andrew W.5ORCID,Hernández‐Almeida Iván6ORCID,Hemming Sidney1,Bailey Ian7ORCID,Zheng Xufeng8ORCID,Cheu Daven2,Taglienti Reece2,Weber Michael E.9ORCID,Raymo Maureen E.1ORCID,Williams Trevor10

Affiliation:

1. Lamont‐Doherty Earth Observatory Columbia University Palisades NY USA

2. Scripps Institution of Oceanography University of California San Diego La Jolla CA USA

3. Earth and Environmental Studies Montclair State University Upper Montclair NJ USA

4. Crowder College Neosho MO USA

5. GEOMAR Helmholtz Centre for Ocean Research Kiel Kiel Germany

6. Past Global Changes University of Bern Bern Switzerland

7. Camborne School of Mines University of Exeter Cornwall UK

8. South China Sea Institute of Oceanology Chinese Academy of Sciences Guangzhou China

9. Institute for Geosciences University of Bonn Bonn Germany

10. International Ocean Discovery Program Texas AM University College Station TX USA

Abstract

AbstractWe document an apparent downward displacement of the Matuyama‐Brunhes magnetic reversal by ∼20 m at Scotia Sea International Ocean Discovery Program Site U1538 (Pirie Basin) by comparison with the well‐defined paleomagnetic record at nearby Site U1537 (Dove Basin). Detailed stratigraphic correlation between the two sites is possible due to similar lithologic variations. However, the two sites have distinctly different porewater geochemistry. Notably, Site U1538 indicates a greater demand for electron acceptors to oxidize organic carbon and Fe2+ enrichment below the depth of SO42− depletion. Magnetic parameters indicate enrichment of an authigenic magnetic mineral with strong remanence properties around the depth of SO42− depletion (∼46 m at Site U1538) relative to magnetic parameters at correlative depths at Site U1537. Fe2+ enrichment below the depth of SO42− depletion is not predicted based on the energetically favorable order of electron acceptors for microbial respiration but is documented here and in other depositional settings. This indicates Fe2+ production exceeds the production of H2S by SO42− reduction, providing a geochemical environment that favors the production and preservation of ferrimagnetic remanence‐bearing iron sulfides over paramagnetic pyrite and, thus, a mechanism for deep chemical remanent magnetization acquisition at depths of tens of meters. The influence of authigenic ferrimagnetic iron sulfides on paleomagnetic signals can be difficult to demonstrate with magnetic properties alone; therefore, this finding has implications for evaluating the fidelity of magnetostratigraphic records with complementary geochemical data. Such situations should be considered in other depositional environments with similar porewater Fe2+ accumulation below the SO42− reduction depth.

Funder

National Science Foundation

Publisher

American Geophysical Union (AGU)

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