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Hafnium and neodymium isotopes in seawater and in ferromanganese crusts: The “element perspective”
Institution:1. Aix Marseille Univ, CNRS, IRD, Coll France, CEREGE, Aix-en-Provence, France;2. Laboratoire de Météorologie Dynamique, École Polytechnique, Palaiseau, France;3. ENSTA ParisTech, Université Paris-Saclay, 828 bd des Maréchaux, 91762 Palaiseau cedex, France;4. IFREMER, Unité de Recherche Géosciences Marines, F-29280 Plouzané, France;5. Université de Lille, CNRS, Université du Littoral Côte d''Opale, UMR8187, LOG, Laboratoire d''Océanologie et de Geéosciences, F-59000 Lille, France;6. Laboratoire Geosciences Paris-Sud (GEOPS), Université de Paris Sud, Université Paris-Saclay, 91405 Orsay, France;7. Laboratoire des Sciences du Climat et de l''Environnement LSCE/IPSL, CEA-CNRS-UVSQ, Université Paris-Saclay, 91191 Gif-sur-Yvette, France;8. Institute of Environmental Physics, University of Heidelberg, 69120 Heidelberg, Germany;9. Université Grenoble Alpes, ISTerre, CS 40700, 38058 Grenoble Cedex 9, France;10. LEGOS (Université de Toulouse/CNRS/CNES/IRD/UPS), Observatoire Midi-Pyrénées, Toulouse, France;11. Equipe de Géochimie-Cosmochimie, Institut de Physique du Globe de Paris – Sorbonne Paris Cité, Université Paris Diderot, UMR CNRS 7154, 1 rue Jussieu, 75005 Paris, France;12. ISMAR-CNR, via Gobetti 101, 40129 Bologna, Italy;13. Department of Earth Sciences, University of Cambridge, Cambridge, UK;14. Department of Earth Sciences, University of Oxford, Oxford OX1 3AN, UK;15. UMR CNRS 6282 Biogéosciences, 6 Bd. Gabriel, 21000 Dijon, France;1. Geological Survey of Japan, AIST, Tsukuba, Ibaraki 305-8567, Japan;2. School of Earth & Space Exploration, Arizona State University, Tempe, AZ 85287, USA;3. Department of Chemistry and Biochemistry, Arizona State University, Tempe, AZ 85287, USA;4. Department of Solid Earth Geochemistry, Japan Agency for Marine-Earth Science and Technology, Yokosuka, Kanagawa 237-0061, Japan;5. Research & Development Center for Submarine Resources, Japan Agency for Marine-Earth Science and Technology, Yokosuka, Kanagawa 237-0061, Japan
Abstract:Hafnium and Nd isotopes are increasingly used as paleoceanographic proxies. Comparing the “mantle–crust array” and the “seawater array” in plots of εHf vs. εNd, it has been observed that for a given εNd value the corresponding εHf value is higher for seawater than it is for terrestrial rocks. While this difference had initially been explained by significant hydrothermal input of mantle Hf into seawater, the currently favoured explanation is incongruent weathering of continental rocks producing radiogenic riverine Hf input.We here address this topic from the perspective of the behaviour of these two elements in seawater and in ferromanganese (Fe–Mn) crusts. We distinguish between a “truly dissolved” and a “dissolved” Hf and Nd pool, the latter being comprised of truly dissolved and colloid-bound (“colloidal”) Hf and Nd. While there exists a hydrothermal pathway for colloid-bound dissolved mantle Hf into the oceans, there is, in marked contrast to Nd, no important riverine pathway for colloidal or truly dissolved continental Hf. Owing to their respective chemical speciation in seawater, there exists truly dissolved Nd in the ocean, while the amount of truly dissolved Hf is insignificant.Neodymium is in exchange equilibrium between local seawater and both, the hydrous Fe and Mn oxides hydrogenetic Fe–Mn crusts are composed of. Due to continuous ad- and desorption there is continuous isotopic re-equilibration and the isotopic composition of Nd in a Fe–Mn crust reflects that of truly dissolved Nd in local ambient seawater. In contrast, Hf is only associated with the hydrous Fe oxides on which it forms surface precipitates that do not exchange with seawater. Due to this lack of isotopic re-equilibration, the isotopic composition of Hf in a Fe–Mn crust is the average of that of all the Hf scavenged during the lifetime of the hydrous Fe oxide particles. Since the Hf-bearing hydrous Fe oxides in a Fe–Mn crust do not form from local ambient seawater at the crust's growth site but are advected as colloids or fine particles, their Hf isotopic composition depends on the origin and migration pathway of these colloids. Hence, while Nd isotopes in Fe–Mn crusts provide reliable information on truly dissolved Nd in local ambient seawater, Hf isotopes rather indicate the origin and pathway of hydrous Fe oxide colloids, and might differ from truly dissolved Hf in local ambient seawater. This may explain the occasional decoupling of Nd and Hf isotopes in Fe–Mn crusts and supports the notion of a significant hydrothermal mantle signal of Hf in seawater.
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