Density-depth model of the continental wedge at the maximum slip segment of the Maule Mw8.8 megathrust earthquake
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2015Metadata
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Maksymowicz Jeria, Andrei
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Density-depth model of the continental wedge at the maximum slip segment of the Maule Mw8.8 megathrust earthquake
Abstract
Complexities in the rupture process during a megathrust earthquake can be attributed to the combined effect of inhomogeneous distribution of stress accumulated during the interseismic period and inho-mogeneous rheology of the seismogenic contact. We modeled the free-air gravity field of the southern Central Chile convergent margin along five 2-D profiles that cross the patch of highest slip during the Chilean 2010 megathrust earthquake in order to analyze variability in the density and shape of the con-tinental wedge and its relationship withseismotectonics. We also analyzed the bathymetry to derive the long-term interplate friction coefficient. The results show that the high slip patch during the Maule earthquake corresponds to a segment of the margin characterized by (1) low densities in the continen-tal wedge, (2)low vertical loading over the inter-plate contact, (3) a well-developed shelf basin and, (4)low taper angles consistent with a low effective basal friction coefficient. We interpret the correla-tion between these parameters in terms of the total potential energy change during the earthquake and conclude that if the normal stress or frictional coefficient are low, then a large slip does not necessar-ily imply a large amount of coseismicwork. Heterogeneities in density of the continental basement can therefore be related to complexities in the pattern of coseismic slip and in the aftershock distribution. Locally, a subducted seamount or seaward spur of high-density continental crust may be present near the high slip patch.
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This work was funded by CONICYT (Comisión Nacional de Ciencia y Tecnología) under the program Development of Re-search Projects between Chile and the United Sates CONICYT grant #USA2012-001. Andrei Maksymowicz gratefully acknowl-edges a scholarship granted by the Chilean National Science Co-operation (CONICYT). Anne Tréhu thanks the U.S. National Sci-ence Foundation Marine Geology and Geophysics program for sup-port for ChilePEPPER data acquisition and analysis through grant OCE1130013 to Oregon State University. Finally, we thanks the de-tailed comments formulated by the anonymous reviewers.
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URI: https://repositorio.uchile.cl/handle/2250/133008
DOI: DOI: 10.1016/j.epsl.2014.11.005
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Earth and Planetary Science Letters 409 (2015) 265-277
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