The accretion of foreland basin sediments during early stages of continental collision in the European Alps and similarities to accretionary wedge tectonics

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Original languageEnglish
Pages (from-to)2216-2238
Number of pages23
JournalTectonics
Volume35
Issue number10
Publication statusPublished - 2016
Externally publishedYes

Abstract

We present structural observations from foreland basin sediments that were incorporated into the orogenic wedge of the central European Alps during early stages of continental collision. Our analysis focuses on the prograde evolution and considers the full history of the sediments ranging from their deposition in the basin to deep burial and metamorphism at temperatures of ~320°C. The tectonic evolution is matched with constraints on the diagenetic alteration of the sediments. For this purpose, we calculate the temperatures and depths of sediment compaction and illitization as well as the associated fluid liberation. The data set highlights that the tectonic incorporation of the sediments into the orogenic wedge was strongly controlled by their diagenetic state. Earliest deformation took place during imbrication and frontal accretion of unconsolidated and fluid-saturated sediments. Ductile folding of the sediments occurred already at this stage and was assisted by particulate flow. With the progressive consolidation of the sediments the elastic strength increased, which resulted in an overall embrittlement. This rheological change is recorded by the onset of out-of-sequence thrusting, brittle faulting, and the formation of massive quartz-calcite veins, which took place in the approximate temperature range of the seismogenic zone (i.e., ~150–350°C). Moreover, widespread pressure solution resulted in the formation of a penetrative cleavage and records slow but long-lasting deformation at low background strain rates. In summary, the prograde tectonic evolution of the frontal Alpine wedge exhibits many similarities with the structural and mechanical evolution of accretionary wedges at active subduction zones.

Keywords

    Foreland basin, accretion, clay dehydration, continental subduction, orogeny, out-of-sequence thrusting

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The accretion of foreland basin sediments during early stages of continental collision in the European Alps and similarities to accretionary wedge tectonics. / Dielforder, Armin; Berger, Alfons; Herwegh, Marco.
In: Tectonics, Vol. 35, No. 10, 2016, p. 2216-2238.

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title = "The accretion of foreland basin sediments during early stages of continental collision in the European Alps and similarities to accretionary wedge tectonics",
abstract = "We present structural observations from foreland basin sediments that were incorporated into the orogenic wedge of the central European Alps during early stages of continental collision. Our analysis focuses on the prograde evolution and considers the full history of the sediments ranging from their deposition in the basin to deep burial and metamorphism at temperatures of ~320°C. The tectonic evolution is matched with constraints on the diagenetic alteration of the sediments. For this purpose, we calculate the temperatures and depths of sediment compaction and illitization as well as the associated fluid liberation. The data set highlights that the tectonic incorporation of the sediments into the orogenic wedge was strongly controlled by their diagenetic state. Earliest deformation took place during imbrication and frontal accretion of unconsolidated and fluid-saturated sediments. Ductile folding of the sediments occurred already at this stage and was assisted by particulate flow. With the progressive consolidation of the sediments the elastic strength increased, which resulted in an overall embrittlement. This rheological change is recorded by the onset of out-of-sequence thrusting, brittle faulting, and the formation of massive quartz-calcite veins, which took place in the approximate temperature range of the seismogenic zone (i.e., ~150–350°C). Moreover, widespread pressure solution resulted in the formation of a penetrative cleavage and records slow but long-lasting deformation at low background strain rates. In summary, the prograde tectonic evolution of the frontal Alpine wedge exhibits many similarities with the structural and mechanical evolution of accretionary wedges at active subduction zones.",
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author = "Armin Dielforder and Alfons Berger and Marco Herwegh",
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T1 - The accretion of foreland basin sediments during early stages of continental collision in the European Alps and similarities to accretionary wedge tectonics

AU - Dielforder, Armin

AU - Berger, Alfons

AU - Herwegh, Marco

N1 - Publisher Copyright: ©2016. American Geophysical Union. All Rights Reserved.

PY - 2016

Y1 - 2016

N2 - We present structural observations from foreland basin sediments that were incorporated into the orogenic wedge of the central European Alps during early stages of continental collision. Our analysis focuses on the prograde evolution and considers the full history of the sediments ranging from their deposition in the basin to deep burial and metamorphism at temperatures of ~320°C. The tectonic evolution is matched with constraints on the diagenetic alteration of the sediments. For this purpose, we calculate the temperatures and depths of sediment compaction and illitization as well as the associated fluid liberation. The data set highlights that the tectonic incorporation of the sediments into the orogenic wedge was strongly controlled by their diagenetic state. Earliest deformation took place during imbrication and frontal accretion of unconsolidated and fluid-saturated sediments. Ductile folding of the sediments occurred already at this stage and was assisted by particulate flow. With the progressive consolidation of the sediments the elastic strength increased, which resulted in an overall embrittlement. This rheological change is recorded by the onset of out-of-sequence thrusting, brittle faulting, and the formation of massive quartz-calcite veins, which took place in the approximate temperature range of the seismogenic zone (i.e., ~150–350°C). Moreover, widespread pressure solution resulted in the formation of a penetrative cleavage and records slow but long-lasting deformation at low background strain rates. In summary, the prograde tectonic evolution of the frontal Alpine wedge exhibits many similarities with the structural and mechanical evolution of accretionary wedges at active subduction zones.

AB - We present structural observations from foreland basin sediments that were incorporated into the orogenic wedge of the central European Alps during early stages of continental collision. Our analysis focuses on the prograde evolution and considers the full history of the sediments ranging from their deposition in the basin to deep burial and metamorphism at temperatures of ~320°C. The tectonic evolution is matched with constraints on the diagenetic alteration of the sediments. For this purpose, we calculate the temperatures and depths of sediment compaction and illitization as well as the associated fluid liberation. The data set highlights that the tectonic incorporation of the sediments into the orogenic wedge was strongly controlled by their diagenetic state. Earliest deformation took place during imbrication and frontal accretion of unconsolidated and fluid-saturated sediments. Ductile folding of the sediments occurred already at this stage and was assisted by particulate flow. With the progressive consolidation of the sediments the elastic strength increased, which resulted in an overall embrittlement. This rheological change is recorded by the onset of out-of-sequence thrusting, brittle faulting, and the formation of massive quartz-calcite veins, which took place in the approximate temperature range of the seismogenic zone (i.e., ~150–350°C). Moreover, widespread pressure solution resulted in the formation of a penetrative cleavage and records slow but long-lasting deformation at low background strain rates. In summary, the prograde tectonic evolution of the frontal Alpine wedge exhibits many similarities with the structural and mechanical evolution of accretionary wedges at active subduction zones.

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KW - accretion

KW - clay dehydration

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JO - Tectonics

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