Hongliang Wang
Making Archean cratonic roots by lateral compression: A two-stage thickening and stabilization model
Wang, Hongliang; van Hunen, Jeroen; Pearson, D. Graham
Abstract
Archean tectonics was capable of producing virtually indestructible cratonic mantle lithosphere, but the dominant mechanism of this process remains a topic of considerable discussion. Recent geophysical and petrological studies have refuelled the debate by suggesting that thickening and associated vertical movement of the cratonic mantle lithosphere after its formation are essential ingredients of the cratonization process. Here we present a geodynamical study that focuses on how the thick stable cratonic lithospheric roots can be made in a thermally evolving mantle. Our numerical experiments explore the viability of a cratonization process in which depleted mantle lithosphere grows via lateral compression into a > 200-km thick, stable cratonic root and on what timescales this may happen. Successful scenarios for craton formation, within the bounds of our models, are found to be composed of two stages: an initial phase of tectonic shortening and a later phase of gravitational self-thickening. The initial tectonic shortening of previously depleted mantle material is essential to initiate the cratonization process, while the subsequent gravitational self-thickening contributes to a second thickening phase that is comparable in magnitude to the initial tectonic phase. Our results show that a combination of intrinsic compositional buoyancy of the cratonic root, rapid cooling of the root after shortening, and the long-term secular cooling of the mantle prevents a Rayleigh-Taylor type collapse, and will stabilize the thick cratonic root for future preservation. This two-stage thickening model provides a geodynamically viable cratonization scenario that is consistent with petrological and geophysical constraints.
Citation
Wang, H., van Hunen, J., & Pearson, D. G. (2018). Making Archean cratonic roots by lateral compression: A two-stage thickening and stabilization model. Tectonophysics, 746, 562-571. https://doi.org/10.1016/j.tecto.2016.12.001
Journal Article Type | Article |
---|---|
Acceptance Date | Dec 1, 2016 |
Online Publication Date | Dec 6, 2016 |
Publication Date | Oct 30, 2018 |
Deposit Date | Jan 3, 2017 |
Publicly Available Date | Mar 13, 2017 |
Journal | Tectonophysics |
Print ISSN | 0040-1951 |
Electronic ISSN | 1879-3266 |
Publisher | Elsevier |
Peer Reviewed | Peer Reviewed |
Volume | 746 |
Pages | 562-571 |
DOI | https://doi.org/10.1016/j.tecto.2016.12.001 |
Public URL | https://durham-repository.worktribe.com/output/1389430 |
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Copyright Statement
Crown Copyright © 2016 Published by Elsevier B.V. This is an open access article under the CC BY-NC-ND license
(http://creativecommons.org/licenses/by-nc-nd/4.0/).
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