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Section Days abstract book 2010.indd - RUB Research School ...

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NSE_04<br />

COOLING AND ACCRETION OF THE LOWER<br />

OCEANIC CRUST AT FAST SPREADING<br />

MID-OCEAN RIDGES<br />

Kathrin Faak,<br />

Sumit Chakraborty and Laurence Coogan<br />

Faculty of Geoscience, Institute for Geology, Mineralogy and Geophysics<br />

Ruhr-Universität Bochum, 44780 Bochum, Germany<br />

email: Kathrin.Faak@rub.de<br />

The formation and cooling of new oceanic lithosphere continually resurfaces the surface of<br />

two-thirds of Earth and is the principal mechanism of cooling of Earth's interior. The<br />

formation of new ocean crust along the global mid-ocean ridge system involves the<br />

emplacement of ~20 km 3 of magma per year. An intimately linked process is the circulation of<br />

seawater through newly formed crust that extracts magmatic heat and produces hydrothermal<br />

fluids enriched in base metals and nutrients that form massive sulfide deposits and feed<br />

chemosynthetic ecosystems on the seafloor. Additionally these hydrothermal systems have a<br />

profound influence on the composition of the oceans.<br />

However the processes involved in crystallizing and cooling this magma to form the oceanic<br />

crust are still poorly understood. At the moment two different models are discussed in the<br />

literature to explain the formation of oceanic crust – the “Gabbro glacier” and the “Sheeted<br />

sill” model, which predict different thermal evolution of the oceanic crust and different depth<br />

of hydrothermal circulation.<br />

We apply methods of geospeedometry to samples directly from the ocean floor to determine<br />

cooling rates of the oceanic crust as a function of depth. This allows to check, which of the<br />

models is in better conformity with the observations made in nature.

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