Silica burp hypothesis
The Eocene (55.8 ± 0.2 to 33.9 ± 0.1 Mya; Luterbacher et al., 2005) was a period of Earth history with enhanced crustal activity and a markedly warmer climate. Additionally, the Eocene saw prolonged periods of silica accumulation on the ocean floor. The peak of this accumulation occurred at approximately 50 Mya, creating Horizon AC, a layer of silica-rich sediments spanning approximately 4 My. Significantly, Horizon AC is comparatively isolated in time from known silicic acid addition processes, and this led McGowran (1989) to propose a novel mechanism, the "silica burp" hypothesis, that centres on the temporal decoupling of silicic acid supply and burial by climatic variation.
The "silica burp" hypothesis
The "silica burp" hypothesis suggests that following a period of vulcanism (Thulean; 56.7 to 53.8 Mya), the warm climate of the Early Eocene Climatic Optimum (EECO) decreased ocean circulation and increased stratification with the result that silica added by this vulcanism was isolated from the productive surface waters and was able to accumulate within the ocean interior. According to the hypothesis, this was then compounded by the addition of silicic acid by increased, climate-induced weathering at high latitudes. This warming period persisted until approximately 49 to 48 Ma (Boharty & Zachos, 2003), after which major climate cooling occurred, reinvigorating ocean circulation, and, so the hypothesis goes, releasing the accumulated silicic acid to the surface ocean (the "silica burp") where it fuelled increased biogenic silica production which led to the creation of Horizon AC. Essentially, the hypothesis proposed that changes to the Earth’s climate during this period temporally decoupled the (geophysical) supply of silicic acid to the ocean from its (biological) removal.
Testing the hypothesis in JModels
The silicon-phosphorus model in the JModels suite includes a representation of the "silica burp" as one of its scenarios. This allows users to test whether the hypothesis is able to explain the formation of Horizon AC. The pictures below illustrate the steps to run this scenario using this model.
Further details about the "silica burp" hypothesis can also be found in McGowran (1989), Yool & Tyrrell (2005) and Muttoni & Kent (2007).
- Silicon-phosphorus model overview
- Silicon-phosphorus model details
- Silicon-phosphorus model pros
- Silicon-phosphorus model cons
- Boharty, S.M. and Zachos, J.C. (2003). Significant Southern ocean warming event in the late middle Eocene. Geology 31, 1017–1020.
- Luterbacher, H.P., Ali, J.R., Brinkhuis, H., Gradstein, F.M., Hooker, J.J., Monechi, S., Ogg, J.G., Powell, J., Rfhl, U., Sanfilippo, A. and Schmitz, B. (2005). The Paleogene period. In: Gradstein, F., Ogg, J., Smith, A. (Eds.), A geologic time scale 2004. Cambridge University Press, Cambridge, UK.
- McGowran, B. (1989). Silica burp in the Eocene ocean. Geology 17, 857–860.
- Muttoni, G. and Kent, D.V. (2007). Widespread formation of cherts during the early Eocene climate optimum. Palaeogeography, Palaeoclimatology, Palaeoecology 253, 348-362.
- Yool, A. and Tyrrell, T. (2003). Role of diatoms in regulating the ocean's silicon cycle. Global Biogeochemical Cycles 17, 1103, doi:10.1029/2002GB002018.
- Yool, A. and Tyrrell, T. (2005). Implications for the history of Cenozoic opal deposition from a quantitative model. Palaeogeography, Palaeoclimatology, Palaeoecology 218, 239-255.