Proceedings of the Ocean Drilling Program, 146 Part 1 Scientific Results 1995
DOI: 10.2973/odp.proc.sr.146-1.224.1995
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Frontal Thrust, Oregon Accretionary Prism: Geometry, Physical Properties, and Fluid Pressure

Abstract: The frontal thrust of the Oregon accretionary prism scrapes off about 2 km of incoming sedimentary section and underlies a fault-bend fold of the first ridge landward of the abyssal plain. Scarps with associated chemosynthetic biological communities at the surface and pore-water anomalies at depth indicate that the frontal thrust is tectonically and hydrologically active. At Site 891, near seismic line OR-5, the thrust splits into at least three splays from 375 to 500 mbsf. The upper splay is defined in the co… Show more

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Cited by 8 publications
(7 citation statements)
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“…The important prerequisite of little sediment input to prevent massive accretion is provided by the Nazca Ridge, with its sedimentary cover not exceeding 400 m. The lack of a thick sedimentary cover contributes to seafloor roughness, which is further intensified by underthrusting of seamounts, volcanic ridges, and fault scarps. Accretive margins for example Makran, Cascadia or Nankai are underthrusted by oceanic crust buried beneath a thick sediment pile [ Moore and Biju‐Duval , 1984; Davis and Hyndman , 1989; Minshull and White , 1989; Moore et al , 1990, 1995; Kukowski et al , 2001a]. As revealed by our Peru seismic reflection data, the complete sequence of sediment on the Nazca Ridge is dragged beneath the toe of the continental slope (Figure 6a).…”
Section: Discussionmentioning
confidence: 91%
“…The important prerequisite of little sediment input to prevent massive accretion is provided by the Nazca Ridge, with its sedimentary cover not exceeding 400 m. The lack of a thick sedimentary cover contributes to seafloor roughness, which is further intensified by underthrusting of seamounts, volcanic ridges, and fault scarps. Accretive margins for example Makran, Cascadia or Nankai are underthrusted by oceanic crust buried beneath a thick sediment pile [ Moore and Biju‐Duval , 1984; Davis and Hyndman , 1989; Minshull and White , 1989; Moore et al , 1990, 1995; Kukowski et al , 2001a]. As revealed by our Peru seismic reflection data, the complete sequence of sediment on the Nazca Ridge is dragged beneath the toe of the continental slope (Figure 6a).…”
Section: Discussionmentioning
confidence: 91%
“…The faults are shear zones that exhibit evidence of large strains and fabric modification. Fabric collapse associated with fault movement and fluid escape may lead to higher density, whereas faulted zones that retain water remain underconsolidated, exhibit anomalously low density, and are overpressured [Moore' et al, 1995b]. Conversion of density determinations from borehole samples and downhole logs to fluid pressure [Moore et al, 1995c] provides indirect evidence that fluids in low-density fault zones may approach lithostatic pressure.…”
Section: Porosity Loss and Overpressuresmentioning
confidence: 99%
“…The role of compaction in deformation of poorly lithified sedimentary rocks has long been considered as a significant and often difficult to quantify shortening mechanism in addition to folding and thrusting (e.g. Cochrane et al ., ; Moore et al ., ; Evans et al ., ; Bangs & Gulick, ; Gonzalez‐Mieres & Suppe, ). In deepwater gravity‐driven systems where ideally up‐dip extension is balanced by down‐dip contraction, mismatches in shortening/extension amounts between the two structural regimes in regional restored sections have been documented (see discussions in Butler & Paton, and Morley et al ., ).…”
Section: Introductionmentioning
confidence: 98%