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Published February 2022 | public
Journal Article

Geochemical insights into formation of enigmatic ironstones from Rio Grande rise, South Atlantic Ocean

Abstract

Rio Grande Rise (RGR) is an intraplate oceanic elevation in the South Atlantic Ocean that formed at a hotspot on the Mid-Atlantic Ridge during the Cretaceous. In spreading center and hotspot environments, ironstones form mainly by biomineralization of reduced Fe from hydrothermal fluids or oxidation of sulfide deposits. However, RGR has been considered aseismic and volcanically inactive for the past 46 Ma. Here, we investigate the origin of ironstones collected from the summit of RGR using multiple techniques: petrographic observations, X-ray diffraction, U-Th/He geochronology, and chemical composition. The ironstones from RGR consist of finely laminated goethite containing igneous rock fragments, carbonate fluorapatite, and calcite. Our results suggest that Fe oxyhydroxides were precipitated by Fe-oxidizing bacteria forming bacterial mats. The bacterial Fe mats underwent compaction, dewatering, goethite crystallization, and cementation that created the ironstone deposits. U-Th/He geochronology reveals protracted goethite minimum ages extending from the late Miocene to the Quaternary, probably due to multiple generations of mats, slow mineralization rates, and Fe-oxide dissolution-reprecipitation cycles. Flame-like goethite structures underneath FeMn crusts and a chimney-shaped goethite sample with a central channel indicate that the dewatering fluid flowed upward through the deposits, or a thermal fluid source may have been introduced from below the ironstone deposits. High Fe/Mn ratios, low trace metals contents (Ni + Co + Cu), and very low Fe/REY ratios suggest ironstone precipitation from a hydrothermal fluid; however, REY_(SN) plots and bivariate Ce_(SN) /Ce_(SN⁎) versus Y_(SN)/Ho_(SN) and Ce_(SN) /Ce_(SN⁎) versus Nd plots are inconclusive, and a proximal source of magma was unlikely during the period of mat formation. Given this evidence, we hypothesize that a geothermal circulation system may have facilitated ironstone mineralization at RGR.

Additional Information

© 2021 Elsevier B.V. Received 19 October 2021, Revised 15 December 2021, Accepted 21 December 2021, Available online 25 December 2021. MB acknowledges the São Paulo State Research Foundation (FAPESP) for PhD scholarship grant 2018/05114-8 and internship abroad scholarship grant 2019/15587-3. The FAPESP thematic project "Marine E-tech" is acknowledged (grant 2014/50820-7) for financing cruises RGR1 and DY094. LJ is supported by FAPESP projects 16/24946-9 and 18/17061-6. The USGS Pacific Coastal and Marine Science Center is acknowledged for hosting MB for her internship abroad. The authors thank the crew of the RV Alpha Crucis and RRS Discovery for support during sample collection. The authors thank the Brazilian Synchrotron Light Laboratory (LNLS-CNPEM) for providing beamline time, especially Dr. Douglas Galante for support with the micro-XRF analyses. Any use of trade, firm, or product names is for descriptive purposes only and does not imply endorsement by the U.S. Government. The dataset of this research is made public through the repository DOI https://doi.org/10.6084/m9.figshare.16832056 (figshare.com/articles/dataset/Geochemistry-dataset-Ironstones/16832056). The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.

Additional details

Created:
August 22, 2023
Modified:
October 23, 2023