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Subducted seafloor relief stops rupture in South American great earthquakes: implications for rupture behaviour in the 2010 Maule, Chile earthquake

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posted on 2013-08-23, 10:03 authored by Robert Sparkes, Frederik Tilmann, Niels Hovius, John HillierJohn Hillier
Great subduction earthquakes cause destructive surface deformation and ground shaking over hundreds of kilometres. Their rupture length is limited by the characteristic strength of the subduction plate interface, and by lateral variations in its mechanical properties. It has been proposed that subduction of topographic features such as ridges and seamounts can affect these properties and stop rupture propagation, but the required relief and physical mechanisms of topographic rupture limitation are not well understood. Here, we show that the rupture limits of thirteen historic great earthquakes along the South America–Nazca plate margin are strongly correlated with subducted topography with relief > 1000 m, including the Juan Fernandez Ridge. The northern limit of rupture in the Mw 8.8 Maule, Chile earthquake of 27 February 2010 is located where this ridge subducts. Analysis of intermediate-magnitude earthquakes shows that in most places, the subduction of high seafloor relief creates weak, aseismic zones at the plate interface, which prevent rupture propagation, but that the Juan Fernandez Ridge is associated with a locally strong plate interface. The maximum rupture length, and thus magnitude, of great subduction earthquakes is therefore determined by the size and lateral spacing of topographic features where they are present on the subducting plate.

History

School

  • Social Sciences

Department

  • Geography and Environment

Citation

SPARKES, R. ... et al., 2010. Subducted seafloor relief stops rupture in South American great earthquakes: implications for rupture behaviour in the 2010 Maule, Chile earthquake. Earth and Planetary Science Letters, 298 (1-2), pp. 89 - 94.

Publisher

© Elsevier B.V.

Version

  • AM (Accepted Manuscript)

Publication date

2010

Notes

This article was published in the journal, Earth and Planetary Science Letters [© Elsevier B.V.] and the definitive version is available at: http://dx.doi.org/10.1016/j.epsl.2010.07.029

ISSN

0012-821X

Language

  • en

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