Mantle Convection and Plate Tectonics: Toward an Integrated Physical and Chemical Theory

Author:

Tackley Paul J.1

Affiliation:

1. Department of Earth and Space Sciences, University of California, Los Angeles, CA 90095, USA.

Abstract

Plate tectonics and convection of the solid, rocky mantle are responsible for transporting heat out of Earth. However, the physics of plate tectonics is poorly understood; other planets do not exhibit it. Recent seismic evidence for convection and mixing throughout the mantle seems at odds with the chemical composition of erupted magmas requiring the presence of several chemically distinct reservoirs within the mantle. There has been rapid progress on these two problems, with the emergence of the first self-consistent models of plate tectonics and mantle convection, along with new geochemical models that may be consistent with seismic and dynamical constraints on mantle structure.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference91 articles.

1. The mantle is solid except for some shallow (<100 km depth) regions where small percentages of partial melting may take place.

2. Mantle rocks deform like a fluid over long time scales with viscosity ∼10 21 Pa·s by the movement of vacancies or dislocations through the crystal lattice.

3. G. Schubert D. L. Turcotte P. Olson Mantle Convection in the Earth and Planets (Cambridge Univ. Press New York in press).

4. Convective velocities are on the order of centimeters per year so one “transit” across the mantle takes ∼100 million years and one “overturn” takes ∼400 to 500 million years. Surface heat flux is 80 mW/m 2 and the cooling rate is ∼100 K per million years.

5. Strength of the lithosphere: Constraints imposed by laboratory experiments

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