100 m wind-mixed surface layer (O2 present) CO2 photoautotrophic Fe(II)-oxidation Fe(OH)3 biomass -2 90.0 mol Fe(III) m -2 22.5 mol C m (Fe:C = 4:1) 2+ CH4 anoxic deep waters H2 -2 methanogenesis 5.9 mol C m sedimentation 400 m Fe 2+ - Fe / HCO3 2+ Fe CH4 1 mm methanotrophy CH4 / Fe(OH)3 mid-ocean ridge (CH3COO- , H2) fermentation annual deposit Fe-rich layers SiO2-rich layers Fe3 O4 Fe(III)reduction 63.8 mol Fe(III) -2m-2 15.9 mol C m (Fe:C = 4:1) 26.2 mol Fe(III) m-2 0.7 mol C m-2 (as Fe3O4) (Fe:C = 36:1) 6.6 mol C m-2 (as FeCO3 ) (Fe:C = 4:1) CH4 + 8Fe(OH)3 Æ 8Fe2+ + CO2 + 16OH- + 6H2O (-ΔGº) 3. Solute Sorbents OH OH Si OH OH OH OH > Fe O O OH OH > Fe OH OH P OH O 100 >FeO>FeOH2+ >FeOH >FeOH2+ >FeOH2+ >FeOH2+ >FeOH2+ >FeOH2+ >FeOH2+ 50 >FeO>FeO>FeO>FeO>FeO>FeO>FeO- >FeOH2+ >FeOH >FeO>FeOH >FeO>FeOH >FeOH2+ 0 0 2 4 6 8 pH 10 12 14 Phosphate Adsorbed (%) Available Surface Sites (%) 100 >FeO- >FeOH2+ 0 2 >FeOH 50 0 4 6 8 pH 10 12 14 The Key Paper Calculated [PO4] concentrations ranging from 0.03 to 0.29 µM, while today’s average [PO4] is 2.3 µM. Such a reduction could have reduced the rate of organic carbon burial by up to 90%. Bjerrum, Bjerrum, C.J., C.J., and and Canfield, Canfield, D.E. D.E. (2002) (2002) Nature Nature 417: 417: 159-162 159-162 BUT, w hat abo ut silica ? today’s oceans average < 0.10 mM Si cristobalite saturation : 0.67 mM Si amorphous SiO2 saturation : 2.20 mM Si 100 0m 75 0. 67 50 2.2 0 25 mM m M M Si Si Si 0 6 7 8 pH 9 10 100 0m 75 0. 67 50 2.2 0 25 mM m M M Si Si Si 0 6 7 8 pH 9 10 Net Negative Charge Net Positive Charge Implications Recall that today’s ocean [PO44] averages 2.3 µM In the absence of silica, we calculate an average [PO44] concentration of 0.14 µM For cristobalite saturation, we calculate an average [PO44] concentration of 0.95 µM For amorphous silica saturation, we calculate an average [PO44] concentration of 5.25 µM Inferred concentrations may be up to 50% low due to diagenetic remobilization Ni in BIF Through Time Konhauser et al. (2009) Komatiites Through Time Preferential Mobilization of Ni Paleo-Seawater Ni Concentrations Methanogens require Ni in their enzymes 1. hydrogenase 2. CO-dehydrogenase 3. methyl-coenzyme M reductase 4. urease Hausrath et al. (2007) A Very Interesting Time… Klein (2005) There are many theories for the timing of the rise of atmospheric O22, the so-called ‘Great Oxidation Event’. (1) a change in styles of volcanism peak mantle plume activity at 3.0-2.9 and 2.7 Ga (H2, CO, CH4, H2S) (H2O, CO2, SO2) (2) increased nutrient availability post glaciation (3) the demise of methanogens Previous explanations for a methane collapse revolve around the outcompetition of methanogens by sulfate-reducing bacteria. We suggest instead that the oceanic Ni famine recorded in BIF would have strongly stifled methanogenesis without the need to invoke increasing sulfate concentrations. How do BIF compare with other marine sediments as proxies, such as black shales? From Scott et al. (2008) The timing of the great oxidation event may have been determined by evolution of the composition of volcanic extrusions and the nutrients it supplied to microbial populations. Unresolved Issues 1. Source of Fe(II) – MOR, seamount, land? 2. Oxidation? – If yes; O2, photosynthesis, UV 3. Primary Fe ppts – how much Fe(II) component? 4. Metabolism used by seafloor microbes? What’s the solution? - isotopes - elemental ratios in BIF - modern analogues
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