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IUGG XXIV General Assembly July 2-13, 2007 Perugia, Italy<br />

(S) - <strong>IASPEI</strong> - International Association of Seismology and Physics of the Earth's<br />

Interior<br />

JSS011 Oral Presentation 2093<br />

Continental growth and preservation of geochemical mantle heterogeneity<br />

in spite of whole-mantle convection<br />

Prof. Uwe Walzer<br />

Institut f. Geowissenschaften Friedrich-Schiller-Universitaet Jena <strong>IASPEI</strong><br />

Roland Hendel, John. Baumgardner<br />

The focus of this paper is the numerical simulation of the chemical differentiation of the Earth's mantle.<br />

This differentiation induces the generation and growth of the continents and, as a complement, the<br />

formation and augmentation of the depleted MORB mantle. Here, we present a solution of this problem<br />

by an integrated theory in common with the problem of thermal convection in a 3-D compressible<br />

spherical-shell mantle. The conservation of mass, momentum, energy, angular momentum, and of four<br />

sums of the number of atoms of the pairs 238U-206Pb, 235U-207Pb,232Th-208Pb, 40K-40Ar is<br />

guaranteed by the used equations. The whole coupled thermal and chemical evolution of mantle plus<br />

crust was calculated starting with the formation of the solid-state primordial silicate mantle. No<br />

restricting assumptions have been made regarding number, size, form, and distribution of the<br />

continents. It was, however, implemented that moving oceanic plateaus touching a continent are to be<br />

accreted to this continent at the corresponding place. The model contains a mantle-viscosity profile with<br />

a usual asthenosphere beneath a lithosphere, a highly viscous transition zone and a second lowviscosity<br />

layer below the 660-km mineral phase boundary. The central part of the lower mantle is highly<br />

viscous. This explains the fact that there are, regarding the incompatible elements, chemically different<br />

mantle reservoirs in spite of perpetual stirring during more than 4.49 billion years. The highly viscous<br />

central part of the lower mantle also explains the relatively slow lateral movements of CMB-based<br />

plumes, slow in comparison with the lateral movements of the lithospheric plates. The temperature- and<br />

pressure-dependent viscosity of the model is complemented by a viscoplastic yield stress, Sy. The paper<br />

includes a comprehensive variation of parameters, especially the variation of the viscosity-level<br />

parameter, rn, the yield stress, Sy, and the temporal average of the Rayleigh number. In the rn-Sy plot,<br />

a central area shows runs with realistic distributions and sizes of continents. This area is partly<br />

overlapping with the rn-Sy areas of piecewise plate-like movements of the lithosphere and of realistic<br />

values of the surface heat flow and Urey number.<br />

Keywords: mantle convection, continental growth, chemical heterogeneity

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