2017
DOI: 10.2204/iodp.proc.348.203.2017
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Data report: clay mineral assemblages and illite/smectite diagenesis in cuttings from Hole C0002P, IODP Expedition 348, Nankai Trough accretionary prism

Abstract: This report summarizes the results of X-ray diffraction analyses of cuttings samples (1-4 mm diameter) from Integrated Ocean Drilling Program Hole C0002N, which is located offshore southwest Japan. The analyses included 73 specimens (<2 µm size fraction) from the upper to middle levels of the Nankai accretionary prism. The cuttings were collected over a depth interval of 1175 to 2305 meters below seafloor (mbsf). Smectite is generally the most abundant clay mineral. Within lithologic Unit IV, percentages of sm… Show more

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Cited by 14 publications
(13 citation statements)
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“…All of the procedures for sampling, sample processing, X-ray diffraction (XRD) analysis, determination of normalization factors, and computation of relative mineral abundances have been described thoroughly in a series of IODP data reports (Guo & Underwood, 2012;Underwood, 2017aUnderwood, , 2017bUnderwood & Guo, 2013Underwood & Song, 2016a, 2016b. Briefly, those workers isolated the < 2 μm size fraction from core samples and cuttings and scanned glycol-saturated oriented aggregates for smectite, illite, chlorite, kaolinite, and quartz.…”
Section: Methodsmentioning
confidence: 99%
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“…All of the procedures for sampling, sample processing, X-ray diffraction (XRD) analysis, determination of normalization factors, and computation of relative mineral abundances have been described thoroughly in a series of IODP data reports (Guo & Underwood, 2012;Underwood, 2017aUnderwood, , 2017bUnderwood & Guo, 2013Underwood & Song, 2016a, 2016b. Briefly, those workers isolated the < 2 μm size fraction from core samples and cuttings and scanned glycol-saturated oriented aggregates for smectite, illite, chlorite, kaolinite, and quartz.…”
Section: Methodsmentioning
confidence: 99%
“…Above the diagenetic ceiling at 2200 mbsf, the proportion of smectite in bulk mudstones generally ranges from 11 wt% to 35 wt%, with an average of 23 wt% (Underwood, 2017a(Underwood, , 2017bUnderwood & Song, 2016a). Values within the cored interval (Underwood & Song, 2016b) show considerably more variability (e.g.…”
Section: Interpretation Of Facies Relations Within Older and Deeper Pmentioning
confidence: 99%
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“…The sampled part of the accretionary prism consists mainly of silty claystone with interbedded sandstone between~950 and~1,665 mbsf (lithologic Unit IV) and fine silty claystone with small amounts of sandstone between~1,665 and 3,058 mbsf (lithologic Unit V; Figure 2b; Tobin et al, 2015). These sediments are composed of~50-60% clay materials (Underwood, 2017a(Underwood, , 2017bUnderwood & Song, 2016). Steep bedding attitudes (60-90°) have been measured in cores and borehole resistivity image logs (Strasser et al, 2014;Tobin et al, 2015).…”
Section: Geological Settingmentioning
confidence: 99%
“…Due to much effort (Expedition 319 Scientists 2010a; Guo and Underwood 2012;Saffer et al 2017;Strasser et al 2014a;Underwood 2017aUnderwood , 2017bUnderwood , 2017cUnderwood andGuo 2013, 2017;Underwood and Song 2016;Yamaguchi et al 2020), clay mineral assemblages have been determined and used to interpret the evolution of the accretionary prism (Underwood 2018;Underwood and Guo, 2018). However, XRD is limited by the fact that data cannot be acquired when core samples are not recovered.…”
Section: Introductionmentioning
confidence: 99%