2018
DOI: 10.1130/ges01537.1
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Structure of oceanic crust and serpentinization at subduction trenches

Abstract: This paper is published under the terms of the CC-BY-NC license.

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Cited by 185 publications
(296 citation statements)
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References 105 publications
(227 reference statements)
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“…Blue‐shaded area represents the velocity envelope from mature Atlantic‐type oceanic crust (144–170 Ma, White et al, ). Pink‐shaped area corresponds to the velocity envelope of oceanic crust found at slow‐spreading ridges as compiled by Grevemeyer et al (). Green‐shaded area corresponds to the velocity envelope of serpentinized mantle presented by Dean et al ().…”
Section: Discussionmentioning
confidence: 99%
“…Blue‐shaded area represents the velocity envelope from mature Atlantic‐type oceanic crust (144–170 Ma, White et al, ). Pink‐shaped area corresponds to the velocity envelope of oceanic crust found at slow‐spreading ridges as compiled by Grevemeyer et al (). Green‐shaded area corresponds to the velocity envelope of serpentinized mantle presented by Dean et al ().…”
Section: Discussionmentioning
confidence: 99%
“…The velocities from 6.8-7.2 km/s to 8.0 km/s are too low for unaltered mantle and may result from serpentinization of the upper mantle (e.g., in fracture zones, Detrick et al, 1993, the COT of nonvolcanic rifted margins, Davy et al, 2016, and slow or ultraslow spreading oceanic basins; e.g., the Labrador Sea; Delescluse et al, 2015;Osler & Louden, 1992 or magma intrusion (e.g., in NW Indian Ocean; Gupta et al, 2010). In our final model (Figure 3b), velocities at depths >3 km below the top basement sit outside the envelopes for Pacific and magmatic oceanic crust newly compiled by Grevemeyer et al (2018;Figure 9a well with the velocity profiles in the models of thin oceanic crust overlying serpentinized mantle in the North Atlantic Ocean (Figure 9b; Davy et al, 2016;Funck et al, 2003;Hopper et al, 2004;Whitmarsh et al, 1996) and the exhumed mantle zone in West Iberia (Figure 9b; Dean et al, 2000;Sallarès et al, 2013) and the Central Tyrrhenian Basin (Figure 9c; Prada et al, 2014). Serpentinization of the upper mantle is facilitated when the crust is thin and fractured to allow seawater to flow in (Minshull et al, 1998;Sauter et al, 2013;Shillington et al, 2006).…”
Section: Reflection Moho Hypothesismentioning
confidence: 94%
“…Fluids enter the shallow seismogenic system either within the pore space of the subducting igneous crust and sediment, or bound in hydrous minerals. Normal faulting associated with bending of the subducting plate is likely to produce enhanced hydration of the crust and upper mantle seaward of the subduction zone (e.g., Ranero et al, 2003;Naliboff et al, 2013;Korenaga, 2017;Grevemeyer et al, 2018). These fluids are released either through compaction in the shallowest 5-7 km or in dehydration reactions at higher pressures and temperatures (e.g., Saffer and Tobin, 2011).…”
Section: Role Of Megathrust Fluidsmentioning
confidence: 99%