Affiliation:
1. Institute for Geophysics Jackson School of Geosciences The University of Texas at Austin Austin TX USA
2. Department of Earth and Planetary Sciences Jackson School of Geosciences The University of Texas at Austin Austin TX USA
3. Oden Institute for Computational Engineering & Sciences The University of Texas at Austin Austin TX USA
4. Institute for Geosciences Goethe University Frankfurt Germany
Abstract
AbstractEarth's style of planetary heat transport is characterized by plate tectonics which requires rock strength to be reduced plastically in order to break an otherwise stagnant lithospheric lid, and for rocks to have a memory of past deformation to account for strain localization and the hysteresis implied by geological sutures. Here, we explore ∼107 Rayleigh number, visco‐plastic, 3‐D global mantle convection with damage. We show that oceanic lithosphere‐only models generate strong toroidal‐poloidal power ratios and features such as a mix of long‐wavelength tectonic motions and smaller‐scale, back‐arc tectonics driven by downwellings. Undulating divergent plate boundaries can evolve to form overlapping spreading centers and microplates, promoted and perhaps stabilized by the effects of damage with long memory. The inclusion of continental rafts enhances heat flux variability and toroidal flow, including net rotation of the lithosphere, to a level seen in plate reconstructions for the Cenozoic. Both the super‐continental cycle and local rheological descriptions affect heat transport and tectonic deformation across a range of scales, and we showcase both general tectonic dynamics and regionally applied continental breakup scenarios. Our work points toward avenues for renewed analysis of the typical, mean behavior as well as the evolution of fluctuations in geological and model plate boundary evolution scenarios.
Publisher
American Geophysical Union (AGU)
Subject
Geochemistry and Petrology,Geophysics