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Accretionary wedge

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pressure (source terms) and those that limit flow (permeability and drainage path length). Sediment permeability and incoming sediment thickness are the most important factors, whereas fault permeability and the partitioning of sediment have a small effect. In one such study, it was found that as sediment permeability is increased, pore pressure decreases from near-lithostatic to hydrostatic values and allows stable taper angles to increase from ~2.5° to 8°–12.5°. With increased sediment thickness (from 100–8,000 m (330–26,250 ft)), increased pore pressure drives a decrease in stable taper angle from 8.4°–12.5° to <2.5–5°. In general, low-permeability and thick incoming sediment sustain high pore pressures consistent with shallowly tapered geometry, whereas high-permeability and thin incoming sediment should result in steep geometry. Active margins characterized by a significant proportion of fine-grained sediment within the incoming section, such as northern
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overpressured fluid. Dilatant fracturing will create escape routes, so the fluid pressure is likely to be buffered at the value required for the transition between shear and oblique tensile (dilatant) fracture, which is slightly in excess of the load pressure if the maximum compression is nearly horizontal. This in turn buffers the strength of the wedge at the cohesive strength, which is not pressure-dependent, and will not vary greatly throughout the wedge. Near the wedge front the strength is likely to be that of the cohesion on existing thrust faults in the wedge. The shear resistance on the base of the wedge will also be fairly constant and related to the cohesive strength of the weak sediment layer that acts as the basal detachment. These assumptions allow the application of a simple plastic continuum model, which successfully predicts the observed gently convex taper of accretionary wedges.
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margin of North America. This process formed a stacking sequence in which the structurally highest rocks (on the east) are the oldest, and in which each major thrust wedge to the west becomes younger. Within each of the terrane blocks, however, the rocks become younger upsection, but the sequence may be repeated multiple times by thrust faults.
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basement, where imaged, appears to diverge from the sedimentary package, dipping under the wedge while the overlying sediments are often lifted up against it. Backthrusting may be favored where relief is high between the crest of the wedge and the surface of the forearc basin because the relief must be supported by
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of accretionary wedges dip back toward the arc, and that accreted material is emplaced below such backstops, is contradicted by observations from many active forearcs that indicate (1) backthrusting is common, (2) forearc basins are nearly ubiquitous associates of accretionary wedges, and (3) forearc
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in Italy are largely an accretionary wedge formed as a consequence of subduction. This region is tectonically and geologically complex, involving both subduction of the Adria micro-plate beneath the Apennines from east to west, continental collision between the Eurasia and Africa plates building the
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range in age from about 200 million to 80 million years old. The Franciscan Complex is composed of a complex amalgamation of semi-coherent blocks, called tectonostratigraphic terranes, that were episodically scraped from the subducting oceanic plate, thrust eastward, and shingled against the western
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of the South China Sea slope. The existence of the South China Sea slope also leads the strike of impinging folds with NNW-trend to turn more sharply to a NE-strike, parallel to strike of the South China Sea slope. Analysis shows that the pre-orogenic mechanical/crustal heterogeneities and seafloor
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margin, suggesting that pre-orogenic sediment thickness is the major control on the geometry of frontal structures. The preexisting South China Sea slope that lies obliquely in front of the advancing accretionary wedge has impeded the advancing of frontal folds resulting in a successive termination
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is dominated by two major lithologic units, the Valdez Group (Late Cretaceous) and the Orca Group (Paleocene and Eocene). The Valdez Group is part of a 2,200-km-long by 100-km-wide belt of Mesozoic accretionary complex rocks called the Chugach terrane. This terrane extends along the Alaska coastal
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and trench rollback of the Ionian basin under Eurasia, causing the opening of the Liguro-Provençal and Tyrrhenian back-arc basins and the formation of the Calabrian accretionary wedge. The Calabrian accretionary wedge is a partially submerged accretionary complex located in the Ionian offshore and
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as critically tapered wedges of sediment demonstrate that pore pressure controls their taper angle by modifying basal and internal shear strength. Results from some studies show that pore pressure in accretionary wedges can be viewed as a dynamically maintained response to factors which drive pore
177:, are transported toward the subduction zone and accreted to the continental margin. Since the Late Devonian and Early Carboniferous periods, some 360 million years ago, subduction beneath the western margin of North America has resulted in several collisions with terranes, each producing a 377:
Rapid tectonic loading of wet sediment in accretionary wedges is likely to cause the fluid pressure to rise until it is sufficient to cause dilatant fracturing. Dewatering of sediment that has been underthrust and accreted beneath the wedge can produce a large steady supply of such highly
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The topographic expression of the accretionary wedge forms a lip, which may dam basins of accumulated materials that, otherwise, would be transported into the trench from the overriding plate. Accretionary wedges are the home of
318:, are preserved on land. They provide a valuable natural laboratory for studying the composition and character of the oceanic crust and the mechanisms of their emplacement and preservation on land. A classic example is the 1032:
Nemcok, M., Coward, M. P., Sercombe, W. J. and Klecker, R. A., 1999: Structure of the West Carpathian Accretionary Wedge: Insights from Cross Section Construction and Sandbox Validation. Phys. Chem. Earth (A), 24, 8, pp.
374:, have steep taper angles. Observations from active margins also indicate a strong trend of decreasing taper angle (from >15° to <4°) with increased sediment thickness (from <1 to 7 km). 950:
Jones, D.L., Siberling, N.J., Coney, P.J., and Monger, J.W.H., 1987, Lithotectonic terrane map of Alaska (west of the 141st meridian): U.S. Geological Survey Miscellaneous Field Studies Map MF 1847-A.
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Tsang, Man-Yin; Bowden, Stephen A.; Wang, Zhibin; Mohammed, Abdalla; Tonai, Satoshi; Muirhead, David; Yang, Kiho; Yamamoto, Yuzuru; Kamiya, Nana; Okutsu, Natsumi; Hirose, Takehiro (February 1, 2020).
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Saffer, D. M., and B. A. Bekins (2006), An evaluation of factors influencing pore pressure in accretionary complexes: Implications for taper angle and wedge mechanics, J. Geophys. Res., 111, B04101,
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are not equivalent to tectonic plates, but rather are associated with tectonic plates and accrete as a result of tectonic collision. Materials incorporated in accretionary wedges include:
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Schrader, F.C., 1900, A reconnaissance of a part of Prince William Sound and the Copper River District, Alaska, in 1898: U.S. Geological 20th Anniversary Report, pt. 7, p. 341–423.
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Fruehn, J., R. von Huene, and M. Fisher (1999), Accretion in the wake of terrane collision: The Neogene accretionary wedge off Kenai Peninsula, Alaska, Tectonics, 18(2), 263–277.
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Period, roughly 170 million years ago, in an extensional regime within either a back-arc or a forearc basin. It was later accreted to the continental margin of Laurasia.
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Backthrusting of the rear of the accretionary wedge, arcward over the rocks of the forearc basin, is a common aspect of accretionary tectonics. An older assumption that
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Material exposed in the forearc ridge may include fragments of oceanic crust or high pressure metamorphic rocks thrust from deeper in the subduction zone.
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Pelayo, A., and D. Wiens (1992), Tsunami Earthquakes: Slow Thrust-Faulting Events in the Accretionary Wedge, J. Geophys. Res., 97(B11), 15321–15337.
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event. The piecemeal addition of these accreted terranes has added an average of 600 km (370 mi) in width along the western margin of the
1007: 543:. This wedge incorporates sediment eroded from the continental margin and marine sediments carried into the subduction zone on the Pacific plate. 441:. In recent years, this is the site of attention for studying the temperature of subseafloor life and underground hot fluids in subducting zones. 329:
Longitudinal sedimentary tapering of pre-orogenic sediments correlates strongly with curvature of the submarine frontal accretionary belt in the
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A Seismic Sequence from Northern Apennines (Italy) Provides New Insight on the Role of Fluids in the Active Tectonics of Accretionary Wedges.
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of California, which is one of the most extensive ophiolite terranes in North America. This oceanic crust likely formed during the middle
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In accretionary wedges, seismicity activating superimposed thrusts may drive methane and oil upraising from the upper crust.
513:. The Orca Group is part of an accretionary complex of Paleogene age called the Prince William terrane that extends across 1320: 216: 539:. During the Neogene the terrane's western part was subducted after which a sediment wedge accreted along the northeast 455: 238: 787:
Platt, J. (1990), Thrust Mechanics in Highly Overpressured Accretionary Wedges, J. Geophys. Res., 95(B6), 9025–9034.
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is a current (in modern use) or former accretionary wedge. Accretionary complexes are typically made up of a mix of
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have resulted from rupture through the sedimentary rock along the basal decollement of an accretionary wedge.
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are formed with the youngest most outboard structures progressively uplifting the older more inboard thrusts.
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Minelli, L. and C. Faccenna (2010), Evolution of the Calabrian accretionary wedge (central Mediterranean),
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Silver, E., and D. Reed (1988), Backthrusting in Accretionary Wedges, J. Geophys. Res., 93(B4), 3116–3126.
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The internal structure of an accretionary wedge is similar to that found in a thin-skinned foreland
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Piggy-back basins, which are small basins located in surface depression on the accretionary prism.
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Alpine mountain belt further to the north and the opening of the Tyrrhenian basin to the west.
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located in Washington State. The mountains began to form about 35 million years ago when the
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The small sections of oceanic crust that are thrust over the overriding plate are said to be
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The sediments accreted onto the non-subducting tectonic plate at a convergent plate boundary
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Pelagic sediments – typically immediately overlying oceanic crust of the subducting plate
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morphology exert strong controls on the thrust-belt development in the incipient Taiwan
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The shape of the wedge is determined by how readily the wedge will fail along its basal
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Lin, Andrew T.; Liu, Char-Shine; Lin, Che-Chuan; et al. (December 5, 2008).
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Material transported into the trench by gravity sliding and debris flow from the
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Ocean-floor basalts – typically seamounts scraped off the subducting plate
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Davis, George H. Structural Geology of Rocks and Regions. (1996). pp583.
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thin-skinned zone of Carpathian thrustbelt, which is thrust over the
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Calderoni, Giovanna et al. Earth and Planetary Science Letters.
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Calabrian Accretionary Wedge in the Central Mediterranean – The
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Adjacent continental masses located along strike (such as
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laterally bounded by the Apulia and Malta escarpments.
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Volume 281, Issues 1-2, April 30, 2009, pages 99–109.
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Archived from 983:"Geology of the Golden Gate Headlands" 109:Materials within an accretionary wedge 105:is made up of accretionary complexes. 1059: 814: 221:adding citations to reliable sources 192: 1321:List of tectonic plate interactions 13: 14: 1776: 1040: 980: 113:Accretionary wedges and accreted 1739: 1738: 197: 67:formed on the overriding plate. 1049:United States Geological Survey 1026: 1008:"Magnitude 6.3 - CENTRAL ITALY" 1000: 974: 965: 953: 944: 935: 913: 892: 867:10.1016/j.marpetgeo.2019.104080 833: 808: 799: 456:BahĂ­a Mansa Metamorphic Complex 293: 208:needs additional citations for 790: 781: 764: 751: 712: 689: 668:. Britannica. January 22, 2014 658: 632: 165:such as linear island chains, 1: 625: 521:area, underlying much of the 349:Mechanical models that treat 127:Trench sediments – typically 846:Marine and Petroleum Geology 745:10.1016/j.margeo.2008.10.002 620:Subduction zone metamorphism 161:Elevated regions within the 134:Oceanic, volcanic island arc 7: 827:10.14379/iodp.proc.370.2017 613: 431:Nankai accretionary complex 400: 334:of folds against and along 188: 97:. For example, most of the 10: 1781: 437:is subducting beneath the 263:belt. A series of thrusts 1734: 1706: 1673: 1655: 1602: 1530: 1467: 1424: 1406:Thick-skinned deformation 1200: 1159: 1093: 465:tectonics of the central 131:that may be derived from: 78:of terrestrial material, 53:convergent plate boundary 1411:Thin-skinned deformation 1187:Stereographic projection 1177:Orthographic projection 1160:Measurement conventions 1106:LamĂ©'s stress ellipsoid 988:. National Park Service 531:accretionary wedge off 498:Chugach National Forest 454:between 38°S and 43°S ( 406:Currently active wedges 603:East European Platform 567:Carpathian Flysch Belt 446:Exhumed ancient wedges 424:is subducting beneath 397:along the backthrust. 351:accretionary complexes 307: 26: 1688:Paleostress inversion 1381:Strike-slip tectonics 1251:Extensional tectonics 1231:Continental collision 1101:Deformation mechanism 646:on September 16, 2016 517:westward through the 496:– The geology of the 320:Coast Range ophiolite 301: 24: 1266:Fold and thrust belt 908:10.1029/2009TC002562 776:10.1029/2005JB003990 548:Franciscan Formation 515:Prince William Sound 492:Kodiak Shelf in the 487:North American Plate 435:Philippine Sea Plate 422:South American Plate 302:Accretionary wedge ( 217:improve this article 151:ridge (olistostrome) 72:accretionary complex 1698:Section restoration 1574:Rock microstructure 1236:Convergent boundary 1136:Strain partitioning 1121:Overburden pressure 1111:Mohr–Coulomb theory 921:"Olympic Mountains" 858:2020MarPG.11204080T 737:2008MGeol.255..186L 511:southwestern Alaska 469:are related to the 452:Chilean Coast Range 412:Mediterranean Ridge 280:pore fluid pressure 99:geological basement 1675:Kinematic analysis 1331:Mountain formation 1246:Divergent boundary 1211:Accretionary wedge 1087:Structural geology 981:Elder, William P. 483:Juan de Fuca Plate 308: 35:accretionary prism 31:accretionary wedge 27: 1752: 1751: 1683:3D fold evolution 1569:Pressure solution 1564:Oblique foliation 1444:Exfoliation joint 1434:Columnar jointing 1094:Underlying theory 1014:on April 14, 2010 698:"Plate Tectonics" 666:"Deep-sea Trench" 523:continental shelf 479:Olympic Mountains 249: 248: 241: 179:mountain-building 171:crustal fragments 1772: 1742: 1741: 1487:Detachment fault 1482:Cataclastic rock 1416:Thrust tectonics 1386:Structural basin 1361:Pull-apart basin 1301:Horst and graben 1080: 1073: 1066: 1057: 1056: 1034: 1030: 1024: 1023: 1021: 1019: 1004: 998: 997: 995: 993: 987: 978: 972: 969: 963: 957: 951: 948: 942: 939: 933: 932: 930: 928: 917: 911: 896: 890: 889: 879: 869: 837: 831: 830: 812: 806: 803: 797: 794: 788: 785: 779: 768: 762: 755: 749: 748: 731:(3–4): 186–203. 716: 710: 709: 707: 705: 693: 687: 684: 678: 677: 675: 673: 662: 656: 655: 653: 651: 642:. 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1165: 1164: 1162: 1158: 1152: 1149: 1147: 1144: 1142: 1139: 1137: 1134: 1132: 1129: 1127: 1124: 1122: 1119: 1117: 1116:Mohr's circle 1114: 1112: 1109: 1107: 1104: 1102: 1099: 1098: 1096: 1092: 1088: 1081: 1076: 1074: 1069: 1067: 1062: 1061: 1058: 1052: 1050: 1045: 1044: 1029: 1013: 1009: 1003: 984: 977: 968: 961: 956: 947: 938: 922: 916: 909: 905: 901: 895: 887: 883: 878: 873: 868: 863: 859: 855: 851: 847: 843: 836: 828: 824: 820: 819: 811: 802: 793: 784: 777: 773: 767: 760: 754: 746: 742: 738: 734: 730: 726: 722: 715: 699: 692: 683: 667: 661: 645: 641: 635: 631: 621: 618: 617: 608: 607:Penninic Unit 604: 600: 596: 592: 588: 584: 580: 576: 572: 568: 565: 561: 557: 553: 549: 545: 542: 538: 534: 530: 527: 524: 520: 519:Kodiak Island 516: 512: 508: 504: 499: 495: 491: 488: 484: 480: 476: 472: 468: 467:Mediterranean 464: 460: 457: 453: 450: 449: 440: 436: 432: 429: 427: 423: 419: 416: 413: 410: 409: 398: 396: 391: 386: 384: 379: 375: 373: 369: 365: 361: 357: 352: 347: 344: 342: 341:arc-continent 337: 332: 327: 325: 321: 317: 313: 305: 300: 291: 289: 285: 281: 277: 272: 270: 266: 262: 257: 255: 243: 240: 232: 222: 218: 212: 211: 206:This section 204: 200: 195: 194: 186: 184: 180: 176: 172: 168: 164: 156: 153: 150: 146: 143: 139: 136: 133: 130: 126: 123: 120: 119: 118: 116: 106: 104: 100: 96: 93: 89: 85: 81: 77: 73: 68: 66: 62: 61:oceanic crust 58: 54: 50: 47: 44:onto the non- 43: 40: 36: 32: 23: 19: 1512:Thrust fault 1210: 1201:Large-scale 1172:Inclinometer 1146:Stress field 1048: 1028: 1016:. 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Index


sediments
accreted
subducting
tectonic plate
convergent plate boundary
slab
oceanic crust
island arcs
turbidites
basalts
ocean floor
pelagic
hemipelagic
sediments
geological basement
Japan
terranes
turbidites
Barbados
forearc
ocean basins
ocean ridges
crustal fragments
terranes
mountain-building
North American

verification
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