Difference between revisions of "Silica burp hypothesis"

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Revision as of 16:26, 31 March 2008

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

By comparing the contents of a large number of cores drilled down through layers of ocean sediments, it is possible to construct an estimate of how the particle rain to the seafloor has changed over geological time. One consistent finding is that there was a period of unusually high flux of solid SiO2 (known as opal or biogenic silica) to the seafloor about 50 million years ago that lasted for about 4 million years. This silicon-rich seam of sediment is known as Horizon AC, and a colourfully named hypothesis, the "silica burp", was developed by McGowran (1989) to explain its origin.

McGowran's "silica burp" hypothesis suggested that a sequence of geological and climatological events conspired to create Horizon AC. Firstly, a period of vulcanism known as the Thulean (56.7 to 53.8 Mya) added a large quantity of dissolved silicon to the ocean. Next, the warming climate of the Early Eocene Climatic Optimum (EECO) acted to decrease ocean circulation and increase stratification, with the result that silicon added by this vulcanism was isolated from the productive surface waters and was able to accumulate within the ocean interior. This build-up of silicon in the ocean was then compounded by the further addition of silicic acid by increased, climate-induced weathering at high latitudes. The warming of the EECO period persisted until approximately 49 to 48 Mya (Boharty & Zachos, 2003), after which major climate cooling occurred. This reinvigorated the circulation of the ocean, and, so McGowran's hypothesis went, released the accumulated silicic acid from the deep to the surface ocean, the "silica burp", where it fuelled increased biogenic silica production which led to the creation of Horizon AC.

Essentially, McGowran's hypothesis proposed that changes to the Earth’s climate around the period that Horizon AC was formed acted to decoupled in time the geophysical processes that supplied silicic acid to the ocean from the biological processes that acted to remove it.

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.

Select the "scenarios" option from the main window
Select the "McGowran" option from the scenarios
Simulate the model to test the "silica burp" hypothesis

Further details about the "silica burp" hypothesis can also be found in McGowran (1989), Yool & Tyrrell (2005) and Muttoni & Kent (2007).

Other related pages


External links