The University of Southampton
University of Southampton Institutional Repository

Comparison of fold-thrust belts driven by plate convergence and gravitational failure

Comparison of fold-thrust belts driven by plate convergence and gravitational failure
Comparison of fold-thrust belts driven by plate convergence and gravitational failure
Deepwater fold-thrust belts (FTBs) are predominantly formed by the deformation of sedimentary sequences as a result of subduction of oceanic plates at active margins, gravitational failure at passive margins, or a combination of these two driving mechanisms at both types of margin. A key question is: Is the FTB driven by gravitational failure basically the same as the FTB driven by plate convergence or are there fundamental differences? To address this, we reviewed FTB examples from different tectonic settings (end members and hybrid systems) in terms of geometry, structure, deformation, shortening rate, and tectonic process. The energy source in gravity-driven systems lies within the sedimentary material itself that is being deformed by updip extension and downdip contraction, whereas in the plate convergence-driven systems, it lies outside the local sediment pile and within the broader undeformed crust and lithosphere. The energy in gravity-driven systems is resupplied by sediment input from large river deltas and therefore deformation tends to be episodic, linked to episodes of major sediment input; whereas in a system driven by plate motions, the energy is resupplied by movement of a boundary upon which force is acting, and tends to be stable and less episodic. Therefore the sedimentation plays an important role in the gravity-driven deformation, but a less important role in the plate convergence-driven deformation. In gravity-driven systems, it promotes upward propagation of normal faulting at upslope by increasing maximum principal stress but hinders upward propagation of thrusting (i.e. mostly buried structures) by increasing minimum principal stress at downslope; while in plate convergence systems, thrusts and folds tend to deform sea floor as a result of large compression, with less effect from sedimentation. Despite the varying basal strength, the observed thrust faults in both systems are mostly basinward-verging, in slight contrast to the theoretical model predication (with homogeneous material), implicating the control of likely variability of stratigraphic strength on thrust vergence. The shortening rate across plate convergence-driven systems is high (several tens mm/yr), and continuous on a long timescale; whereas across the gravity-driven fold-thrust belts, it is generally slow (several mm/yr) and more variable or even catastrophic through time. Despite overall seaward younging of thrusting, fault activity differs slightly among different systems. Focused activity at the frontal structures of FTBs is more common at the plate convergence system while activity focused in the rear to middle of FTBs is more common in the gravity-driven system. Plate convergence-driven system is primarily limited by rate of plate motion, i.e. the rate at which the plate is fed into the FTB, whereas in gravity-driven system, the movement is limited (resisted) by the strength of sediments and detachment.
Distribution of deformation, Fold-thrust belt, Gravitational failure, Plate convergence, Shortening rates, Structural propagation, Thrust faults
0012-8252
Yang, Xiaodong
0c44aab1-3c52-4e2a-925e-565a34967c57
Peel, Frank J.
ccbb86f8-56a0-4b59-b664-e772a9c4015f
Mcneill, Lisa
1fe6a1e0-ca1a-4b6f-8469-309d0f9de0cf
Sanderson, David
5653bc11-b905-4985-8c16-c655b2170ba9
Yang, Xiaodong
0c44aab1-3c52-4e2a-925e-565a34967c57
Peel, Frank J.
ccbb86f8-56a0-4b59-b664-e772a9c4015f
Mcneill, Lisa
1fe6a1e0-ca1a-4b6f-8469-309d0f9de0cf
Sanderson, David
5653bc11-b905-4985-8c16-c655b2170ba9

Yang, Xiaodong, Peel, Frank J., Mcneill, Lisa and Sanderson, David (2020) Comparison of fold-thrust belts driven by plate convergence and gravitational failure. Earth-Science Reviews, 203, [103136]. (doi:10.1016/j.earscirev.2020.103136).

Record type: Article

Abstract

Deepwater fold-thrust belts (FTBs) are predominantly formed by the deformation of sedimentary sequences as a result of subduction of oceanic plates at active margins, gravitational failure at passive margins, or a combination of these two driving mechanisms at both types of margin. A key question is: Is the FTB driven by gravitational failure basically the same as the FTB driven by plate convergence or are there fundamental differences? To address this, we reviewed FTB examples from different tectonic settings (end members and hybrid systems) in terms of geometry, structure, deformation, shortening rate, and tectonic process. The energy source in gravity-driven systems lies within the sedimentary material itself that is being deformed by updip extension and downdip contraction, whereas in the plate convergence-driven systems, it lies outside the local sediment pile and within the broader undeformed crust and lithosphere. The energy in gravity-driven systems is resupplied by sediment input from large river deltas and therefore deformation tends to be episodic, linked to episodes of major sediment input; whereas in a system driven by plate motions, the energy is resupplied by movement of a boundary upon which force is acting, and tends to be stable and less episodic. Therefore the sedimentation plays an important role in the gravity-driven deformation, but a less important role in the plate convergence-driven deformation. In gravity-driven systems, it promotes upward propagation of normal faulting at upslope by increasing maximum principal stress but hinders upward propagation of thrusting (i.e. mostly buried structures) by increasing minimum principal stress at downslope; while in plate convergence systems, thrusts and folds tend to deform sea floor as a result of large compression, with less effect from sedimentation. Despite the varying basal strength, the observed thrust faults in both systems are mostly basinward-verging, in slight contrast to the theoretical model predication (with homogeneous material), implicating the control of likely variability of stratigraphic strength on thrust vergence. The shortening rate across plate convergence-driven systems is high (several tens mm/yr), and continuous on a long timescale; whereas across the gravity-driven fold-thrust belts, it is generally slow (several mm/yr) and more variable or even catastrophic through time. Despite overall seaward younging of thrusting, fault activity differs slightly among different systems. Focused activity at the frontal structures of FTBs is more common at the plate convergence system while activity focused in the rear to middle of FTBs is more common in the gravity-driven system. Plate convergence-driven system is primarily limited by rate of plate motion, i.e. the rate at which the plate is fed into the FTB, whereas in gravity-driven system, the movement is limited (resisted) by the strength of sediments and detachment.

Text
Comparison of Fold-Thrust Belts - Proof
Download (27MB)

More information

Accepted/In Press date: 14 February 2020
e-pub ahead of print date: 19 February 2020
Published date: April 2020
Additional Information: Funding Information: We acknowledge the funding to X. Yang from the UK Natural Environment Research Council ( NERC ) Centre for Doctoral Training (CDT) in Oil and Gas and the National Oceanography Centre , Southampton and University of Southampton . We thank the reviewers Jonas Ruh, Chris Morley, and an anonymous reviewer for their robust reviews and constructive comments that significantly improved the manuscript. We thank editor Carlo Doglioni for handling this paper. Publisher Copyright: © 2020 Elsevier B.V.
Keywords: Distribution of deformation, Fold-thrust belt, Gravitational failure, Plate convergence, Shortening rates, Structural propagation, Thrust faults

Identifiers

Local EPrints ID: 439223
URI: http://eprints.soton.ac.uk/id/eprint/439223
ISSN: 0012-8252
PURE UUID: e29d8751-7b55-4ea9-bb6a-632ba6344054
ORCID for Lisa Mcneill: ORCID iD orcid.org/0000-0002-8689-5882
ORCID for David Sanderson: ORCID iD orcid.org/0000-0002-2144-3527

Catalogue record

Date deposited: 07 Apr 2020 16:30
Last modified: 17 Mar 2024 05:28

Export record

Altmetrics

Contributors

Author: Xiaodong Yang
Author: Frank J. Peel
Author: Lisa Mcneill ORCID iD
Author: David Sanderson ORCID iD

Download statistics

Downloads from ePrints over the past year. Other digital versions may also be available to download e.g. from the publisher's website.

View more statistics

Atom RSS 1.0 RSS 2.0

Contact ePrints Soton: eprints@soton.ac.uk

ePrints Soton supports OAI 2.0 with a base URL of http://eprints.soton.ac.uk/cgi/oai2

This repository has been built using EPrints software, developed at the University of Southampton, but available to everyone to use.

We use cookies to ensure that we give you the best experience on our website. If you continue without changing your settings, we will assume that you are happy to receive cookies on the University of Southampton website.

×