2017
DOI: 10.1186/s40645-017-0132-y
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Structural context and variation of ocean plate stratigraphy, Franciscan Complex, California: insight into mélange origins and subduction-accretion processes

Abstract: The transfer (accretion) of materials from a subducting oceanic plate to a subduction-accretionary complex has produced rock assemblages recording the history of the subducted oceanic plate from formation to arrival at the trench. These rock assemblages, comprising oceanic igneous rocks progressively overlain by pelagic sedimentary rocks (chert and/or limestone) and trench-fill clastic sedimentary rocks (mostly sandstone, shale/mudstone), have been called ocean plate stratigraphy (OPS). During accretion of OPS… Show more

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Cited by 62 publications
(45 citation statements)
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References 78 publications
(146 reference statements)
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“…In this paper, we present the results of new detailed field mapping, geochronology data, and geochemistry analysis of the mélange complex (Figure ). The mélange rocks here are generally dominated by chaotic mixtures of metapelites, metapsammites, mica schist, paragneisses, and amphibolite as metapelite matrices, and exotic mafic, metagabbroic rocks, and metabasalts as blocks (Silver & Beutner, ; Wakabayashi, , ). Our field observations indicate that the Bayan Obo mélange contains a structurally complex mixture of metapelites (Figures e, f, and j), metapsammites (Figure j), mica‐quartz schist matrix (Figures k–m) mixed with exotic blocks of ultramafic (Figures a and g–k) and metagabbroic rocks (Figures a and f), metabasalts (Figures e–g and i) that locally include possible relict pillow structures (Figure e), plagiogranite (Figures f and i), amphibolite (Figures c–f and i), metacarbonate rocks (Figures l and m), alkaline granulite (Figure m) and tonalite‐trondhjemite (TT) gneisses (Figures b–e, i, and k).…”
Section: Bayan Obo Mélangementioning
confidence: 99%
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“…In this paper, we present the results of new detailed field mapping, geochronology data, and geochemistry analysis of the mélange complex (Figure ). The mélange rocks here are generally dominated by chaotic mixtures of metapelites, metapsammites, mica schist, paragneisses, and amphibolite as metapelite matrices, and exotic mafic, metagabbroic rocks, and metabasalts as blocks (Silver & Beutner, ; Wakabayashi, , ). Our field observations indicate that the Bayan Obo mélange contains a structurally complex mixture of metapelites (Figures e, f, and j), metapsammites (Figure j), mica‐quartz schist matrix (Figures k–m) mixed with exotic blocks of ultramafic (Figures a and g–k) and metagabbroic rocks (Figures a and f), metabasalts (Figures e–g and i) that locally include possible relict pillow structures (Figure e), plagiogranite (Figures f and i), amphibolite (Figures c–f and i), metacarbonate rocks (Figures l and m), alkaline granulite (Figure m) and tonalite‐trondhjemite (TT) gneisses (Figures b–e, i, and k).…”
Section: Bayan Obo Mélangementioning
confidence: 99%
“…In general, a subduction system is required to consume an intervening oceanic plate separating two cratons/blocks prior to the collisional orogeny that ultimately joins the two continents. The mélange associated with oceanic subduction, accretion, and eventual continental collision is thus significant in documenting the tectonic process of orogen (e.g., Festa et al, ; Ghatak et al, ; Greenly, ; Wakabayashi, , ; Wakabayashi & Medley, ; Wang et al, ). In this contribution, we report for the first time a new Paleoproterozoic mélange located in the Bayan Obo region on the northernmost margin of the North China craton (present‐day coordinates).…”
Section: Introductionmentioning
confidence: 99%
“…Mid‐ocean ridge basalt (MORB) and oceanic island basalt (OIB) are the main protoliths of metabasite in accretionary complexes and high‐pressure metamorphic complexes (e.g. Isozaki, Maruyama, & Fukuoka, ; Safonova et al, ; Wakabayashi, ). The MORB oceanic crust generally lies beneath a thick sedimentary cover at the trench.…”
Section: Introductionmentioning
confidence: 99%
“…Accretionary complex related sedimentation is probably responsible for the Halatumiao Formation as well since high aquatic productivity is common in olistostromes deposition under an accretionary wedge environment. However, the accretionary complex is dominated by turbidite and clastic rocks with a percentage of ~90% (Wakabayashi, , ). This differs from the Halatumiao Formation which is mainly composed of fine‐grained carbonaceous and sandy slate (Figure 11a), making it difficult to stand for an accretionary wedge or fore‐arc setting.…”
Section: Discussionmentioning
confidence: 99%