Published May 2010 | Version public
Journal Article

The role of oceanic plateau subduction in the Laramide orogeny

  • 1. ROR icon California Institute of Technology
  • 2. ROR icon University of Sydney

Abstract

The cause of the Laramide phase of mountain building remains uncertain. Conceptual models implicate the subduction of either ocean ridges or conjugates of the buoyant Hess or Shatsky oceanic plateaux. Independent verification of these models has remained elusive, because the putative ridges or plateaux are no longer at the Earth's surface. Inverse convection models have identified two prominent seismic anomalies on the recovered Farallon plate. Here we combine inverse convection models with reconstructions of plate motions, to show that these seismic anomalies coincide palaeogeographically with the restored positions of the Shatsky and Hess conjugate plateaux as they subducted beneath North America. Specifically, the distribution of Laramide crustal shortening events tracked the passage of the Shatsky conjugate beneath North America, whereas the effects of the Hess conjugate subduction were restricted to the northern Mexico foreland belt. We propose that continued subduction caused the oceanic crust to undergo the basalt–eclogite phase transformation, during which the Shatsky conjugate lost its extra buoyancy and was effectively removed. Increases in slab density and coupling between the overriding and subducting plates initially dragged the surface downward, followed by regional-scale surface rebound. We conclude that Laramide uplift resulted from the removal, rather than emplacement, of the Shatsky conjugate.

Additional Information

© 2010 Macmillan Publishers Limited. Received 25 August 2009; accepted 26 February 2010; published online 28 March 2010. We thank D. Helmberger, D. Anderson, P. DeCelles and K. Karlstrom for helpful discussions and P. DeCelles for a helpful review. This represents Contribution number 10026 of the Division of Geological and Planetary Sciences and 102 of the Tectonics Observatory, Caltech. At Caltech this work has been supported by the National Science Foundation (EAR-0739071 and EAR-0810303) and through the Tectonics Observatory by the Gordon and Betty Moore Foundation. Author contributions: L.L. and M.G. designed the whole workflow and carried out the inverse convection model, M.S. and R.D.M. carried out the plate reconstruction, J.S. worked on the geological interpretation and J.M.J. provided mineral physics analysis. All authors participated in preparing the paper.

Additional details

Identifiers

Eprint ID
18451
Resolver ID
CaltechAUTHORS:20100526-100500524

Funding

NSF
EAR-0739071
NSF
EAR-0810303
Gordon and Betty Moore Foundation

Dates

Created
2010-06-20
Created from EPrint's datestamp field
Updated
2021-11-08
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
Caltech Tectonics Observatory, Seismological Laboratory, Division of Geological and Planetary Sciences (GPS)
Other Numbering System Name
Caltech Tectonics Observatory
Other Numbering System Identifier
102