Antiphased dust deposition and productivity in the Antarctic Zone over 1.5 million years.
Michael E WeberIan BaileySidney R HemmingYasmina M MartosBrendan T ReillyThomas A RongeStefanie BrachfeldTrevor WilliamsMaureen RaymoSimon T BeltLukas SmikHendrik VogelVictoria L PeckLinda ArmbrechtAlix CageFabricio G CardilloZhiheng DuGerson FauthChristopher J FogwillMarga GarciaMarlo GarnsworthyAnna GlüderMichelle GuitardMarcus GutjahrIván Hernández-AlmeidaFrida S HoemJi-Hwan HwangMutsumi IizukaYuji KatoBridget KenleeSuzanne OConnellLara F PérezOsamu SekiLee StevensLisa TauxeShubham TripathiJonathan P WarnockXufeng ZhengPublished in: Nature communications (2022)
The Southern Ocean paleoceanography provides key insights into how iron fertilization and oceanic productivity developed through Pleistocene ice-ages and their role in influencing the carbon cycle. We report a high-resolution record of dust deposition and ocean productivity for the Antarctic Zone, close to the main dust source, Patagonia. Our deep-ocean records cover the last 1.5 Ma, thus doubling that from Antarctic ice-cores. We find a 5 to 15-fold increase in dust deposition during glacials and a 2 to 5-fold increase in biogenic silica deposition, reflecting higher ocean productivity during interglacials. This antiphasing persisted throughout the last 25 glacial cycles. Dust deposition became more pronounced across the Mid-Pleistocene Transition (MPT) in the Southern Hemisphere, with an abrupt shift suggesting more severe glaciations since ~0.9 Ma. Productivity was intermediate pre-MPT, lowest during the MPT and highest since 0.4 Ma. Generally, glacials experienced extended sea-ice cover, reduced bottom-water export and Weddell Gyre dynamics, which helped lower atmospheric CO 2 levels.