NUMERICAL STUDY OF MECHANISMS AND TIMESCALES OF OXYGENATION AND INTERPRETATION OF GEOLOGICAL RECORDS IN THE SNOWBALL EARTH AFTERMATH
In this study, we aim to assess the hypothesized oxygenation scenario, as well as to understand mechanisms and timescales of the formation of these characteristic sediments. We developed an atmosphere-ocean biogeochemical cycle model coupled with a redox balance model, and investigated changes in climate, biogeochemical cycles (C, O, P, Ca, Mn, and Fe), and a redox state in the Snowball Earth aftermath.
The results show that, after the Paleoproterozoic Snowball Earth, long-term enhancement of productivity (~5-30 times as high as that of present level) for ~105 years causes a rise of oxygen up to ~0.01PAL in ~102-103 years, and even up to 1PAL in ~106 years. In the surface ocean, Fe and Mn delivered by upwelling of deep water are oxidized and deposit on the timescale of ocean circulation, usually on the order of thousands of years. Fe and Mn oxides deposition precede the carbonate precipitation, because high atmospheric pCO2 and low pH in the ocean prevent the carbonate precipitation just after the deglaciation. We estimate that the carbonates start to precipitate ~105 years after the deglaciation, and a rapid precipitation lasts for ~2-5 x 106 years. Under the Neoproterozoic conditions, i.e., a larger solar constant and lower pCO2 required to escape from the snowball Earth, carbonate precipitation starts relatively earlier (on the order of 104 years). These results may explain the delay in the timing of carbonate deposition in Paleoproterozoic snowball Earth compared to that of cap-carbonates in Neoproterozoic.