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Sources and input mechanisms of hafnium and neodymium in surface waters of the Atlantic sector of the Southern Ocean

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  • Radiogenic isotopes of hafnium (Hf) and neodymium (Nd) are powerful tracers for water mass transport and trace metal cycling in the present and past oceans. However, due to the scarcity of available data the processes governing their distribution are not well understood. Here we present the first combined dissolved Hf and Nd isotope and concentration data from surface waters of the Atlantic sector of the Southern Ocean. The samples were collected along the Zero Meridian, in the Weddell Sea and in the Drake Passage during RV Polarstern expeditions ANTXXIV/3 and ANTXXIII/3 in the frame of the International Polar Year (IPY) and the GEOTRACES program. The general distribution of Hf and Nd concentrations in the region is similar. However, at the northernmost station located 200 km southwest of Cape Town a pronounced increase of the Nd concentration is observed, whereas the Hf concentration is minimal, suggesting much less Hf than Nd is released by the weathering of the South African Archean cratonic rocks. From the southern part of the Subtropical Front (STF) to the Polar Front (PF) Hf and Nd show the lowest concentrations (<0.12 pmol/kg and 10 pmol/kg, respectively), most probably due to the low terrigenous flux in this area and efficient scavenging of Hf and Nd by biogenic opal. In the vicinity of landmasses the dissolved Hf and Nd isotope compositions are clearly labeled by terrigenous inputs. Near South Africa Nd isotope values as low as ε[subscript Nd] = −18.9 indicate unradiogenic inputs supplied via the Agulhas Current. Further south the isotopic data show significant increases to ε[subscript Hf] = 6.1 and ε[subscript Nd] = −4.0 documenting exchange of seawater Nd and Hf with the Antarctic Peninsula. In the open Southern Ocean the Nd isotope compositions are relatively homogeneous (ε[subscript Nd] ∼ −8 to −8.5) towards the STF, within the Antarctic Circumpolar Current, in the Weddell Gyre, and the Drake Passage. The Hf isotope compositions in the entire study area only show a small range between ε[subscript Hf] = + 6.1 and +2.8 support Hf to be more readily released from young mafic rocks compared to old continental ones. The Nd isotope composition ranges from ε[subscript Nd] = −18.9 to −4.0 showing Nd isotopes to be a sensitive tracer for the provenance of weathering inputs into surface waters of the Southern Ocean.
  • This is the publisher’s final pdf. The article is sponsored by the Geochemical Society and the Meteoritical Society and published by Elsevier. It can be found at: http://www.journals.elsevier.com/geochimica-et-cosmochimica-acta.
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  • Stichel, T., Frank, M., Rickli, J., Hathorne, E. C., Haley, B. A., Jeandel, C., & Pradoux, C. (2012). Sources and input mechanisms of hafnium and neodymium in surface waters of the atlantic sector of the southern ocean. Geochimica Et Cosmochimica Acta, 94, 22-37. doi: 10.1016/j.gca.2012.07.005
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  • 94
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  • This study was funded by a Grant of the Deutsche Forschungsgemeinschaft (DFG) to M.F. (Project FR1198/2) within the priority program “Antarctic Research” (SPP 1158).
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