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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Earth Sci.</journal-id>
<journal-title>Frontiers in Earth Science</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Earth Sci.</abbrev-journal-title>
<issn pub-type="epub">2296-6463</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.3389/feart.2021.652501</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Earth Science</subject>
<subj-group>
<subject>Original Research</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>Neodymium Isotopes in Glauconite for Palaeoceanographic Reconstructions at Continental Margins: A Preliminary Investigation From Demerara Rise</article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author" corresp="yes">
<name><surname>Giresse</surname> <given-names>Pierre</given-names></name>
<xref ref-type="aff" rid="aff1"><sup>1</sup></xref>
<xref ref-type="corresp" rid="c001"><sup>&#x002A;</sup></xref>
</contrib>
<contrib contrib-type="author" corresp="yes">
<name><surname>Bayon</surname> <given-names>Germain</given-names></name>
<xref ref-type="aff" rid="aff2"><sup>2</sup></xref>
<xref ref-type="corresp" rid="c002"><sup>&#x002A;</sup></xref>
<uri xlink:href="http://loop.frontiersin.org/people/751040/overview"/>
</contrib>
<contrib contrib-type="author">
<name><surname>Tallobre</surname> <given-names>Cedric</given-names></name>
<xref ref-type="aff" rid="aff1"><sup>1</sup></xref>
</contrib>
<contrib contrib-type="author">
<name><surname>Loncke</surname> <given-names>Lies</given-names></name>
<xref ref-type="aff" rid="aff1"><sup>1</sup></xref>
<uri xlink:href="http://loop.frontiersin.org/people/1271776/overview"/>
</contrib>
</contrib-group>
<aff id="aff1"><sup>1</sup><institution>Centre de Formation et de Recherche sur les Environnements M&#x00E9;diterran&#x00E9;ens (CEFREM), UMR 5110 CNRS, Universit&#x00E9; de Perpignan Via Domitia</institution>, <addr-line>Perpignan</addr-line>, <country>France</country></aff>
<aff id="aff2"><sup>2</sup><institution>Centre de Bretagne, Institut Fran&#x00E7;ais de Recherche pour l&#x2019;Exploitation de la Mer, Marine Geosciences Unit</institution>, <addr-line>Plouzan&#x00E9;</addr-line>, <country>France</country></aff>
<author-notes>
<fn fn-type="edited-by"><p>Edited by: Christian M&#x00E4;rz, University of Leeds, United Kingdom</p></fn>
<fn fn-type="edited-by"><p>Reviewed by: Patrick Blaser, University of Lausanne, Switzerland; Philipp B&#x00F6;ning, University of Oldenburg, Germany</p></fn>
<corresp id="c001">&#x002A;Correspondence: Pierre Giresse, <email>giresse@univ-perp.fr</email></corresp>
<corresp id="c002">Germain Bayon, <email>gbayon@ifremer.fr</email></corresp>
<fn fn-type="other" id="fn004"><p>This article was submitted to Geochemistry, a section of the journal Frontiers in Earth Science</p></fn>
</author-notes>
<pub-date pub-type="epub">
<day>15</day>
<month>04</month>
<year>2021</year>
</pub-date>
<pub-date pub-type="collection">
<year>2021</year>
</pub-date>
<volume>9</volume>
<elocation-id>652501</elocation-id>
<history>
<date date-type="received">
<day>12</day>
<month>01</month>
<year>2021</year>
</date>
<date date-type="accepted">
<day>17</day>
<month>03</month>
<year>2021</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#x00A9; 2021 Giresse, Bayon, Tallobre and Loncke.</copyright-statement>
<copyright-year>2021</copyright-year>
<copyright-holder>Giresse, Bayon, Tallobre and Loncke</copyright-holder>
<license xlink:href="http://creativecommons.org/licenses/by/4.0/"><p>This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.</p></license>
</permissions>
<abstract>
<p>Contourite sediment accumulations at continental margins are related to strong bottom water circulation, where intense winnowing can result in neoformation of authigenic grains of glauconite at the seafloor. In this study, we investigated whether such glauconite grains could faithfully record ambient bottom-water neodymium (Nd) isotopic compositions, and hence be used as paleoceanographic archives. To this purpose, we measured Nd isotopic compositions (&#x03B5;<sub><italic>Nd</italic></sub>) in a series of glauconitic grains, foraminiferal assemblages, leached Fe-Mn oxyhydroxide phases, and detrital clays separated from a contourite sediment record at the Demerara slope off French Guiana (IG-KSF-11; 2370 m water depth), at a location where the present-day &#x03B5;<sub><italic>Nd</italic></sub> distribution along the water column is well characterised. We show that the &#x03B5;<sub><italic>Nd</italic></sub> composition of core-top glauconite grains (&#x2212;12.0 &#x00B1; 0.5) agrees with the expected NADW-like seawater signature at the same location and water depth (&#x2212;11.6 &#x00B1; 0.3), while departing from measured &#x03B5;<sub><italic>Nd</italic></sub> values for corresponding detrital clays (&#x2212;11.3 &#x00B1; 0.2), foraminiferal (&#x2212;10.9 &#x00B1; 0.2), and Fe-Mn oxyhydroxide fractions (&#x2212;9.2 &#x00B1; 0.2). This finding indicates that glauconitic grains at this particular location are probably best suited for paleoceanographic reconstructions than foraminifera and leached Fe-oxyhydroxide fractions, which appear to be influenced by sediment redistribution and the presence of terrestrial continental Fe-oxides, respectively. Using rare earth elements (REE), we tentatively propose that the acquisition of seawater Nd isotopic signatures by glauconite is controlled by the presence of authigenic REE-bearing phosphate-rich phases intertwined within clay mineral sheets, while confirming previous findings that the process of glauconitisation results in the progressive loss of REE within glauconitic grains. Preliminary paleoceanographic implications suggest strengthened bottom-water circulation of the glacial analogue of NADW at this particular location and water depth, with a &#x03B5;<sub><italic>Nd</italic></sub> signature (between &#x2212;10.8 and &#x2212;11.5) similar to that of modern NADW.</p>
</abstract>
<kwd-group>
<kwd>rare earth elements</kwd>
<kwd>neodymium isotopes</kwd>
<kwd>glauconitisation</kwd>
<kwd>Demerara</kwd>
<kwd>contourite</kwd>
</kwd-group>
<counts>
<fig-count count="7"/>
<table-count count="2"/>
<equation-count count="0"/>
<ref-count count="60"/>
<page-count count="14"/>
<word-count count="0"/>
</counts>
</article-meta>
</front>
<body>
<sec id="S1">
<title>Introduction</title>
<p>Since at least the beginning of the Neogene, the sedimentation at the Guianese margin of the Demerara Plateau has been controlled by large contour currents (<xref ref-type="bibr" rid="B32">Loncke et al., 2016</xref>; <xref ref-type="bibr" rid="B51">Tallobre et al., 2016</xref>; <xref ref-type="bibr" rid="B13">Fanget et al., 2020</xref>). At this location, slope bottom deposits are subject to recurrent winnowing that favours the appearance and mineralogical maturation of green glauconitic grains at the seawater&#x2013;sediment interface (<xref ref-type="bibr" rid="B50">Tallobre et al., 2019</xref>). Each contourite sequence is characterised by high abundance of glauconitic grains (especially in the moat area), but also in a moderately to strongly discontinuous sediment accumulation associated with relatively low sedimentation rates. In contrast with nearby shallower settings along the French Guiana margin that have experienced continuous fine-grained hemipelagic sedimentation during the Late Quaternary (<xref ref-type="bibr" rid="B22">H&#x00E4;ggi et al., 2017</xref>; <xref ref-type="bibr" rid="B59">Zhang et al., 2017</xref>; <xref ref-type="bibr" rid="B11">Crivellari et al., 2018</xref>), the Demerara contourite system, as other contourite deposits (e.g., <xref ref-type="bibr" rid="B19">Giresse and Wiewi&#x00F3;ra, 2001</xref>; <xref ref-type="bibr" rid="B17">Giresse, 2008</xref>), is characterised by deposition of discontinuous sediment records, which prevents their use for paleoceanographic reconstructions. Additionally, intense bottom current activity at Demerara and other contourite settings at continental margins can also result in substantial sediment redistribution, with potential effect on the reliability of commonly used paleoceanographic archives in marine sediment records.</p>
<p>The purpose of this study is to show the potential interest of using glauconitic grains in such discontinuous sedimentary records for paleoceanographic reconstructions based on radiogenic neodymium isotopes. Neodymium (Nd) isotopic ratios are commonly measured in biogenic material, such as fish teeth or foraminifer shells, or in the associated Fe-Mn oxyhydroxide fractions of the sediment, as tracers of bottom water circulation (e.g., <xref ref-type="bibr" rid="B15">Frank, 2002</xref>; <xref ref-type="bibr" rid="B20">Goldstein and Hemming, 2003</xref>). In the ocean, each water mass is tagged with a distinctive Nd isotopic composition (typically expressed using the epsilon notation &#x03B5;<sub>Nd</sub>), which reflects, to a large extent, that of the continental masses surrounding their source region (e.g., <xref ref-type="bibr" rid="B47">Tachikawa et al., 2017</xref>; <xref ref-type="bibr" rid="B42">Robinson et al., 2021</xref>). While Nd isotopes have proven particularly helpful for reconstructing past ocean circulation patterns over various geological timescales, their application to contourite sediment accumulations at ocean margins, such as the Demerara Rise, can be skewed by sedimentary processes related to strong bottom current activity, such as winnowing and reworking.</p>
<p>In oceanic environments, glauconitic grains are the result of transformation and neoformation processes taking place at the water&#x2013;sediment interface. Various granular supports (mudclasts, faecal pellets, and foraminifera infillings) include inherited 1:1 interstratified clays (or Te-Oc; i.e., clay minerals consisting of one tetrahedral sheet and one octahedral sheet, such as kaolinite) that become gradually replaced by 2:1 clays (Te-Oc-Te) dominated first by smectite, and then glauconite. These processes are accompanied by aluminium and silicium depletion in inherited minerals, together with significant enrichment of iron and potassium in neoformed minerals (e.g., <xref ref-type="bibr" rid="B37">Odin and Matter, 1981</xref>). While K in neoformed clays is supplied by ambient seawater, the source of Fe is most likely derived from reactive phases of the terrigenous sediment, such as Fe-oxide and oxyhydroxide phases (<xref ref-type="bibr" rid="B37">Odin and Matter, 1981</xref>; <xref ref-type="bibr" rid="B36">Odin and Fullagar, 1988</xref>; <xref ref-type="bibr" rid="B19">Giresse and Wiewi&#x00F3;ra, 2001</xref>; <xref ref-type="bibr" rid="B56">Wiewi&#x00F3;ra et al., 2001</xref>; <xref ref-type="bibr" rid="B17">Giresse, 2008</xref>; <xref ref-type="bibr" rid="B1">Banerjee et al., 2016</xref>). In all cases, these thermodynamic reactions operate at slow kinetic rates, especially regarding the acquisition of seawater-derived K, thereby requiring prolonged residence time at the water&#x2013;sediment interface, presumably over thousands of years (e.g., <xref ref-type="bibr" rid="B16">Giresse, 1975</xref>), and thus reduced sedimentation rates. Earlier studies suggested that such conditions were mostly met at continental platforms, in particular at their outer edges, far from any continental source of terrigenous material. More recently, however, several investigations of contouritic deposits along continental margins revealed important glauconitic accumulations at water depths between &#x223C;2000 and 3000 m (<xref ref-type="bibr" rid="B18">Giresse et al., 1998</xref>; <xref ref-type="bibr" rid="B19">Giresse and Wiewi&#x00F3;ra, 2001</xref>; <xref ref-type="bibr" rid="B17">Giresse, 2008</xref>; <xref ref-type="bibr" rid="B46">Stow and Faug&#x00E8;res, 2008</xref>; <xref ref-type="bibr" rid="B14">Faug&#x00E8;res and Mulder, 2011</xref>). Similar to continental shelf analogues, the occurrence of abundant glauconitic grains in contouritic systems indicates prolonged exposure at the water&#x2013;sediment interface, reflecting here recurring sediment reworking related to the winnowing action of contouritic currents. Due to Fe incorporation, glauconite grains typically display higher specific gravity (between &#x223C;2.4 and 2.9 g/cm<sup>3</sup>; <xref ref-type="bibr" rid="B58">Yadav and Sharma, 1992</xref>) than the average surrounding sediment (&#x223C;1.7 g/cm<sup>3</sup>; <xref ref-type="bibr" rid="B53">Tenzer and Gladkikh, 2014</xref>). As a consequence, authigenic grains of glauconite are less likely to be remobilised and dispersed by currents, compared to empty foraminiferal tests. Additionally, because glauconite formation occurs over relatively long timescales at the seawater&#x2013;sediment interface, unlike other archives of bottom water chemistry (e.g., fish teeth and sedimentary Fe-Mn oxyhydroxide phases), glauconite grains could possibly integrate the signature of bottom water masses over prolonged periods of time (<xref ref-type="bibr" rid="B19">Giresse and Wiewi&#x00F3;ra, 2001</xref>; <xref ref-type="bibr" rid="B17">Giresse, 2008</xref>), which, while preventing their use in high-resolution studies, would provide an effective means for yielding reliable average estimates on past &#x03B5;<sub><italic>Nd</italic></sub> signatures of bottom water masses. To date, however, this hypothesis has never been tested.</p>
<p>To address this issue, we have investigated the Nd isotopic composition of glauconite grains recovered from contourite sediment deposits at Demerara Rise; at a location where &#x03B5;<sub><italic>Nd</italic></sub> signatures of modern water masses are already well characterised (<xref ref-type="bibr" rid="B25">Huang et al., 2014</xref>). This &#x03B5;<sub><italic>Nd</italic></sub> comparison extends to more conventional paleoceanographic archives (uncleaned foraminifers and leached sedimentary Fe-oxyhydroxide phases), being also complemented by the additional use of rare earth elements (REE) and major element ratios, such as K<sub>2</sub>O/Al<sub>2</sub>O<sub>3</sub> and Fe<sub>2</sub>O/Al<sub>2</sub>O<sub>3</sub>. Since the different phases of glauconitisation include the transformation and neoformation of phyllosilicate minerals, a careful investigation is also required to assess the degree to which Nd isotopes in glauconite grains may reflect the detrital &#x03B5;<sub><italic>Nd</italic></sub> signature of inherited clay minerals within the sediment. Following proxy calibration using core-top sediments, preliminary interpretations will be made of a set of Nd isotopic data for buried glauconitic grains, in the light of the changing paleoceanographic context since the last glacial period.</p>
</sec>
<sec id="S2">
<title>Modern and Past Oceanographic Setting</title>
<p>This study focuses on an area of contourite accumulation located at Demerara Rise, along a regional slope failure headscarp, where the bottom current influence is the strongest, with flow velocity up to &#x223C;30 cm/s (<xref ref-type="bibr" rid="B51">Tallobre et al., 2016</xref>; <xref ref-type="fig" rid="F1">Figure 1</xref>). At this location (&#x223C;2400 m water depth), sedimentary dynamics is controlled by uneven accelerations of contour currents that define condensed intervals of deposits, or even lead to significant stratigraphic gaps in the sediment record (<xref ref-type="bibr" rid="B32">Loncke et al., 2016</xref>; <xref ref-type="bibr" rid="B51">Tallobre et al., 2016</xref>, <xref ref-type="bibr" rid="B50">2019</xref>). Under such conditions, the application of both oxygen isotopes and radiocarbon chronostratigraphic methods has proven generally unreliable (<xref ref-type="bibr" rid="B50">Tallobre et al., 2019</xref>), yielding &#x03B4;<sup>18</sup>O depth profiles that cannot be directly tuned to nearby continuous records of hemipelagic sediments (<xref ref-type="bibr" rid="B25">Huang et al., 2014</xref>; <xref ref-type="bibr" rid="B22">H&#x00E4;ggi et al., 2017</xref>).</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption><p>Bathymetric map of the Demerara Plateau and location of studied core IG-KSF-11. The arrows represent surface (red), intermediate (blue), and deep (black) ocean circulation patterns. Also shown for comparison are the location of reference core 46CDH (<xref ref-type="bibr" rid="B25">Huang et al., 2014</xref>) and hydrocast station 3CTD (<xref ref-type="bibr" rid="B25">Huang et al., 2014</xref>).</p></caption>
<graphic xlink:href="feart-09-652501-g001.tif"/>
</fig>
<p>The present-day distribution of radiogenic Nd isotopes along the water column at Demerara Rise identifies the presence of distinct water masses (<xref ref-type="fig" rid="F2">Figure 2</xref>), including the West North Atlantic Central waters (WNACW; &#x03B5;<sub>Nd</sub> &#x223C;&#x2212;13), from surface to &#x223C;500 m water depth, the Antarctic Intermediate Water (AAIW; &#x03B5;<sub>Nd</sub> &#x223C;&#x2212;10.5), between &#x223C; 500 and 1200 m depth, the North Atlantic Deep Water (NADW; &#x03B5;<sub>Nd</sub> from &#x223C;&#x2212;12 to &#x2212;11.5), from &#x223C; 1200 and 4000 m depth, and finally, the Antarctic Bottom Water (AABW; &#x03B5;<sub>Nd</sub> &#x223C;&#x2212;10.5) below 4000 m depth (<xref ref-type="bibr" rid="B25">Huang et al., 2014</xref>). In previous investigations, the application of Nd isotope measurements to various paleoceanographic archives retrieved from Demerara Rise (<xref ref-type="bibr" rid="B25">Huang et al., 2014</xref>) and other locations in the Atlantic have proven particularly useful to reconstruct past ocean circulation patterns, indicating prominent changes in the Atlantic Meridional Overturning Circulation (AMOC) over glacial&#x2013;interglacial timescales, with impact on heat transport and carbon storage in the surface and deep ocean, respectively (e.g., <xref ref-type="bibr" rid="B44">Rutberg et al., 2000</xref>; <xref ref-type="bibr" rid="B39">Piotrowski et al., 2004</xref>, <xref ref-type="bibr" rid="B40">2005</xref>; <xref ref-type="bibr" rid="B38">Pahnke et al., 2008</xref>; <xref ref-type="bibr" rid="B10">B&#x00F6;hm et al., 2015</xref>; <xref ref-type="bibr" rid="B24">Howe et al., 2016</xref>; <xref ref-type="bibr" rid="B31">Lippold et al., 2016</xref>; <xref ref-type="bibr" rid="B41">P&#x00F6;ppelmeier et al., 2020</xref>). A survey of the spatial distribution of Nd isotopes in the Atlantic during both the recent Holocene and the last glacial periods indicated relatively unradiogenic NADW-like &#x03B5;<sub>Nd</sub> values (&#x223C;&#x2212;13) below 1500 m water depth at Demerara Rise (<xref ref-type="bibr" rid="B24">Howe et al., 2016</xref>). Further south in the Atlantic Ocean, the Nd isotopic composition of NADW becomes progressively more radiogenic, reflecting gradual dilution of northern-sourced waters with overlying and underlying Antarctic water masses (<xref ref-type="bibr" rid="B24">Howe et al., 2016</xref>). As a consequence, the unradiogenic &#x201C;tongue&#x201D; of NADW can be traced as the water mass flows southward in the South Atlantic at water depths between &#x223C;2000 and 4000 m (e.g., <xref ref-type="bibr" rid="B55">von Blanckenburg, 1999</xref>; <xref ref-type="bibr" rid="B24">Howe et al., 2016</xref>). During the Last Glacial Maximum (LGM), the deep Atlantic water column displayed a greater influence of southern-sourced waters consistent with a reduced flux of NADW to the Southern Atlantic (<xref ref-type="bibr" rid="B44">Rutberg et al., 2000</xref>; <xref ref-type="bibr" rid="B24">Howe et al., 2016</xref>; <xref ref-type="bibr" rid="B41">P&#x00F6;ppelmeier et al., 2020</xref>). At the Demerara margin, Nd isotopic measurements were previously acquired on uncleaned foraminifera from a nearby sediment core collected at 947 m depth, bathed at present-day by AAIW (<xref ref-type="bibr" rid="B25">Huang et al., 2014</xref>; see core 46CDH on <xref ref-type="fig" rid="F1">Figure 1</xref>). The obtained &#x03B5;<sub>Nd</sub> record for the past 25,000 years indicated similar Nd isotopic compositions during the Holocene and the LGM (&#x03B5;<sub>Nd</sub> &#x223C;&#x2212;10), while revealing pronounced &#x03B5;<sub>Nd</sub> excursions towards unradiogenic values (between &#x2212;11 and &#x2212;12) during the short-lived North Atlantic cold periods of the Heinrich Stadial 1 (HS1) and the Younger Dryas (YD), interpreted as reflecting strong reduction of the AMOC leading to reduced influence of northward flowing AAIW in the equatorial Atlantic (<xref ref-type="bibr" rid="B25">Huang et al., 2014</xref>).</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption><p>The distribution of water masses and associated Nd isotope profile (&#x03B5;<sub><italic>Nd</italic></sub>) along the water column at the Demerara Rise (after <xref ref-type="bibr" rid="B25">Huang et al., 2014</xref>). Comparative &#x03B5;<sub><italic>Nd</italic></sub> values for core-top foraminifers, glauconitic grains, terrigenous clays, and Fe-Mn oxyhydroxide phases in core IG-KSF-11 are shown for comparison.</p></caption>
<graphic xlink:href="feart-09-652501-g002.tif"/>
</fig>
</sec>
<sec id="S3" sec-type="materials|methods">
<title>Materials and Methods</title>
<p>This study was conducted on sediment core IG-KSF-11 (07&#x00B0;51.85N, 052&#x00B0;29.25W; 2370 m water depth), recovered off French Guiana during the IGUANES cruise (R/V <italic>L&#x2019;Atalante;</italic> Loncke L., 2013<sup><xref ref-type="fn" rid="footnote1">1</xref></sup>). The sedimentary records retrieved from this dynamic sedimentary environment are characterised by the occurrence of abundant glauconite grains (<xref ref-type="bibr" rid="B50">Tallobre et al., 2019</xref>). The sediment is dominated by homogeneous grey-green silty mud with alternation of discrete sand layers (<xref ref-type="bibr" rid="B51">Tallobre et al., 2016</xref>, <xref ref-type="bibr" rid="B50">2019</xref>). Core IG-KSF-11 was specifically chosen for this study because foraminifera &#x03B4;<sup>18</sup>O measurements suggest a continuous and coherent stratigraphy for the upper 0&#x2013;80 cm sediment interval that is considered in this study (<xref ref-type="fig" rid="F3">Figure 3A</xref>), which covers approximately the last 60,000 years BP (<xref ref-type="bibr" rid="B50">Tallobre et al., 2019</xref>). However, similar to the other sediment records retrieved from the Demerara contourite system, IG-KSF-11 suffers from inherent chronostratigraphic uncertainties due to the presence of recurrent winnowing and other erosional processes, resulting in hiatuses and frequent radiocarbon age inversions in the lower part of the core (from &#x223C;2.5 to 6 m depth; <xref ref-type="bibr" rid="B50">Tallobre et al., 2019</xref>). As a consequence, in this study, the analysed sediment layers were only assigned a period of deposition (i.e., marine isotope stage 1, MIS 2&#x2026;), rather than a precise stratigraphic age (<xref ref-type="table" rid="T1">Tables 1</xref>, <xref ref-type="table" rid="T2">2</xref>).</p>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption><p><bold>(A)</bold> Planktonic foraminifer &#x03B4;<sup>18</sup>O depth profile (<xref ref-type="bibr" rid="B50">Tallobre et al., 2019</xref>) and <bold>(B)</bold> relative abundance distribution of glauconitic grains in core IG-KSF-11 (<xref ref-type="bibr" rid="B50">Tallobre et al., 2019</xref>). The beige, light green, and dark green boxes correspond to increasing degrees of glauconitic maturity based on visual colour and number of cracks. <bold>(C)</bold> Bulk Fe<sub>2</sub>O<sub>3</sub>/Al<sub>2</sub>O<sub>3</sub> and K<sub>2</sub>O/Al<sub>2</sub>O<sub>3</sub> ratios of studied glauconite grains (this study), reflecting the degree of glauconitisation. <bold>(D)</bold> Nd isotopic composition (&#x03B5;<sub>Nd</sub>) of bulk glauconite grains. The dotted line and associated grey band indicates the present-day &#x03B5;<sub>Nd</sub> value of ambient bottom-waters at the same water depth (<xref ref-type="bibr" rid="B25">Huang et al., 2014</xref>). Note that the uncertainty on measured &#x03B5;<sub>Nd</sub> values (&#x00B1;0.15; 2 SD) is smaller than symbol size, unless reported (sample 0_1 cm).</p></caption>
<graphic xlink:href="feart-09-652501-g003.tif"/>
</fig>
<table-wrap position="float" id="T1">
<label>TABLE 1</label>
<caption><p>Major (wt %), rare earth elements (&#x03BC;g/g), and Nd isotopic composition of glauconitic grains.</p></caption>
<table cellspacing="5" cellpadding="5" frame="hsides" rules="groups">
<thead>
<tr>
<td valign="top" align="left">Sample depth</td>
<td valign="top" align="center">Age</td>
<td valign="top" align="center">Fe<sub>2</sub>O<sub>3</sub></td>
<td valign="top" align="center">MgO</td>
<td valign="top" align="center">Al<sub>2</sub>O<sub>3</sub></td>
<td valign="top" align="center">K<sub>2</sub>O</td>
<td valign="top" align="center">CaO</td>
<td valign="top" align="center">P<sub>2</sub>O<sub>5</sub></td>
<td valign="top" align="center">MnO</td>
<td valign="top" align="center">Y</td>
<td valign="top" align="center">La</td>
<td valign="top" align="center">Ce</td>
<td valign="top" align="center">Pr</td>
<td valign="top" align="center">Nd</td>
<td valign="top" align="center">Sm</td>
<td valign="top" align="center">Eu</td>
<td valign="top" align="center">Gd</td>
<td valign="top" align="center">Tb</td>
<td valign="top" align="center">Dy</td>
<td valign="top" align="center">Ho</td>
<td valign="top" align="center">Er</td>
<td valign="top" align="center">Yb</td>
<td valign="top" align="center">Lu</td>
<td valign="top" align="center">Y/Ho</td>
<td valign="top" align="center"><sup>143</sup>Nd/<sup>144</sup>Nd</td>
<td valign="top" align="left">2 se (10<sup>&#x2013;6</sup>)</td>
<td valign="top" align="center" colspan="2">&#x03B5;<sub>Nd &#x00B1; 2 sd</sub></td>
</tr>
</thead>
<tbody>
<tr>
<td valign="top" align="left">0&#x2013;1 cm</td>
<td valign="top" align="center">MIS 1</td>
<td valign="top" align="center">23.48</td>
<td valign="top" align="center">3.38</td>
<td valign="top" align="center">6.96</td>
<td valign="top" align="center">1.82</td>
<td valign="top" align="center">9.09</td>
<td valign="top" align="center">0.91</td>
<td valign="top" align="center">0.04</td>
<td valign="top" align="center">5.06</td>
<td valign="top" align="center">11.87</td>
<td valign="top" align="center">11.87</td>
<td valign="top" align="center">2.74</td>
<td valign="top" align="center">10.20</td>
<td valign="top" align="center">1.96</td>
<td valign="top" align="center">0.42</td>
<td valign="top" align="center">1.72</td>
<td valign="top" align="center">0.18</td>
<td valign="top" align="center">1.03</td>
<td valign="top" align="center">0.18</td>
<td valign="top" align="center">0.48</td>
<td valign="top" align="center">n.d.</td>
<td valign="top" align="center">0.08</td>
<td valign="top" align="center">28.8</td>
<td valign="top" align="center">0.512021</td>
<td valign="top" align="left">&#x00B1; 24</td>
<td valign="top" align="center">&#x2212;12.0</td>
<td valign="top" align="center">&#x00B1; 0.5</td>
</tr>
<tr>
<td valign="top" align="left">8&#x2013;9 cm</td>
<td valign="top" align="center">MIS 1</td>
<td valign="top" align="center">18.41</td>
<td valign="top" align="center">2.62</td>
<td valign="top" align="center">11.37</td>
<td valign="top" align="center">1.72</td>
<td valign="top" align="center">1.91</td>
<td valign="top" align="center">0.12</td>
<td valign="top" align="center">0.04</td>
<td valign="top" align="center">5.04</td>
<td valign="top" align="center">19.21</td>
<td valign="top" align="center">33.52</td>
<td valign="top" align="center">3.87</td>
<td valign="top" align="center">13.48</td>
<td valign="top" align="center">2.30</td>
<td valign="top" align="center">0.41</td>
<td valign="top" align="center">1.62</td>
<td valign="top" align="center">0.19</td>
<td valign="top" align="center">1.05</td>
<td valign="top" align="center">0.18</td>
<td valign="top" align="center">0.46</td>
<td valign="top" align="center">0.42</td>
<td valign="top" align="center">0.06</td>
<td valign="top" align="center">27.5</td>
<td valign="top" align="center">0.512040</td>
<td valign="top" align="left">&#x00B1; 7</td>
<td valign="top" align="center">&#x2212;11.7</td>
<td valign="top" align="center">&#x00B1; 0.2</td>
</tr>
<tr>
<td valign="top" align="left">20&#x2013;21 cm</td>
<td valign="top" align="center">MIS 2</td>
<td valign="top" align="center">26.95</td>
<td valign="top" align="center">3.51</td>
<td valign="top" align="center">5.89</td>
<td valign="top" align="center">3.24</td>
<td valign="top" align="center">3.79</td>
<td valign="top" align="center">0.15</td>
<td valign="top" align="center">0.04</td>
<td valign="top" align="center">3.45</td>
<td valign="top" align="center">8.33</td>
<td valign="top" align="center">15.72</td>
<td valign="top" align="center">1.96</td>
<td valign="top" align="center">7.29</td>
<td valign="top" align="center">1.38</td>
<td valign="top" align="center">0.27</td>
<td valign="top" align="center">1.09</td>
<td valign="top" align="center">0.13</td>
<td valign="top" align="center">0.71</td>
<td valign="top" align="center">0.13</td>
<td valign="top" align="center">0.30</td>
<td valign="top" align="center">0.30</td>
<td valign="top" align="center">0.04</td>
<td valign="top" align="center">27.5</td>
<td valign="top" align="center">0.512075</td>
<td valign="top" align="left">&#x00B1; 9</td>
<td valign="top" align="center">&#x2212;11.0</td>
<td valign="top" align="center">&#x00B1; 0.2</td>
</tr>
<tr>
<td valign="top" align="left">29&#x2013;30 cm</td>
<td valign="top" align="center">MIS 2</td>
<td valign="top" align="center">24.99</td>
<td valign="top" align="center">3.05</td>
<td valign="top" align="center">6.32</td>
<td valign="top" align="center">2.57</td>
<td valign="top" align="center">2.44</td>
<td valign="top" align="center">0.15</td>
<td valign="top" align="center">0.03</td>
<td valign="top" align="center">2.71</td>
<td valign="top" align="center">8.39</td>
<td valign="top" align="center">15.12</td>
<td valign="top" align="center">1.82</td>
<td valign="top" align="center">6.59</td>
<td valign="top" align="center">1.21</td>
<td valign="top" align="center">0.23</td>
<td valign="top" align="center">0.83</td>
<td valign="top" align="center">0.10</td>
<td valign="top" align="center">0.56</td>
<td valign="top" align="center">0.10</td>
<td valign="top" align="center">0.26</td>
<td valign="top" align="center">0.25</td>
<td valign="top" align="center">0.03</td>
<td valign="top" align="center">28.2</td>
<td valign="top" align="center">0.512041</td>
<td valign="top" align="left">&#x00B1; 8</td>
<td valign="top" align="center">&#x2212;11.7</td>
<td valign="top" align="center">&#x00B1; 0.2</td>
</tr>
<tr>
<td valign="top" align="left">40&#x2013;41 cm</td>
<td valign="top" align="center">MIS 2/3</td>
<td valign="top" align="center">16.12</td>
<td valign="top" align="center">2.68</td>
<td valign="top" align="center">13.23</td>
<td valign="top" align="center">1.87</td>
<td valign="top" align="center">1.60</td>
<td valign="top" align="center">0.13</td>
<td valign="top" align="center">0.03</td>
<td valign="top" align="center">5.51</td>
<td valign="top" align="center">21.80</td>
<td valign="top" align="center">37.89</td>
<td valign="top" align="center">4.40</td>
<td valign="top" align="center">15.08</td>
<td valign="top" align="center">2.63</td>
<td valign="top" align="center">0.49</td>
<td valign="top" align="center">1.89</td>
<td valign="top" align="center">0.21</td>
<td valign="top" align="center">1.16</td>
<td valign="top" align="center">0.20</td>
<td valign="top" align="center">0.51</td>
<td valign="top" align="center">0.42</td>
<td valign="top" align="center">0.06</td>
<td valign="top" align="center">27.5</td>
<td valign="top" align="center">0.512021</td>
<td valign="top" align="left">&#x00B1; 6</td>
<td valign="top" align="center">&#x2212;12.0</td>
<td valign="top" align="center">&#x00B1; 0.2</td>
</tr>
<tr>
<td valign="top" align="left">70&#x2013;71 cm</td>
<td valign="top" align="center">MIS 3</td>
<td valign="top" align="center">17.28</td>
<td valign="top" align="center">2.67</td>
<td valign="top" align="center">13.15</td>
<td valign="top" align="center">2.24</td>
<td valign="top" align="center">1.50</td>
<td valign="top" align="center">0.13</td>
<td valign="top" align="center">0.03</td>
<td valign="top" align="center">5.30</td>
<td valign="top" align="center">22.36</td>
<td valign="top" align="center">22.36</td>
<td valign="top" align="center">4.45</td>
<td valign="top" align="center">15.24</td>
<td valign="top" align="center">2.62</td>
<td valign="top" align="center">0.45</td>
<td valign="top" align="center">1.71</td>
<td valign="top" align="center">0.19</td>
<td valign="top" align="center">1.06</td>
<td valign="top" align="center">0.19</td>
<td valign="top" align="center">0.48</td>
<td valign="top" align="center">0.40</td>
<td valign="top" align="center">0.05</td>
<td valign="top" align="center">28.0</td>
<td valign="top" align="center">0.512025</td>
<td valign="top" align="left">&#x00B1; 7</td>
<td valign="top" align="center">&#x2212;12.0</td>
<td valign="top" align="center">&#x00B1; 0.2</td>
</tr>
<tr>
<td valign="top" align="left"><bold>WRAS<sup><italic>a</italic></sup></bold></td>
<td/>
<td valign="top" align="center">5.71</td>
<td valign="top" align="center">1.66</td>
<td valign="top" align="center">13.8</td>
<td valign="top" align="center">2.26</td>
<td valign="top" align="center">0.94</td>
<td valign="top" align="center">0.84</td>
<td valign="top" align="center">0.03</td>
<td valign="top" align="center">29.40</td>
<td valign="top" align="center">37.80</td>
<td valign="top" align="center">77.69</td>
<td valign="top" align="center">8.77</td>
<td valign="top" align="center">32.69</td>
<td valign="top" align="center">6.15</td>
<td valign="top" align="center">1.19</td>
<td valign="top" align="center">5.19</td>
<td valign="top" align="center">0.82</td>
<td valign="top" align="center">4.95</td>
<td valign="top" align="center">1.02</td>
<td valign="top" align="center">2.97</td>
<td valign="top" align="center">3.01</td>
<td valign="top" align="center">0.46</td>
<td valign="top" align="center">29</td>
<td/>
<td/>
<td/>
<td/>
</tr>
</tbody>
</table>
<table-wrap-foot>
<attrib><italic><sup><italic>a</italic></sup>World River Average Silt (WRAS; <xref ref-type="bibr" rid="B9">Bayon et al., 2015</xref>).</italic></attrib>
</table-wrap-foot>
</table-wrap>
<table-wrap position="float" id="T2">
<label>TABLE 2</label>
<caption><p>Nd isotopic composition of unclean foraminifers, leached Fe-Mn oxyhydroxide phases, and detrital clays.</p></caption>
<table cellspacing="5" cellpadding="5" frame="hsides" rules="groups">
<thead>
<tr>
<td valign="top" align="left">Sample depth</td>
<td valign="top" align="center">Age</td>
<td valign="top" align="center"><sup>143</sup>Nd/<sup>144</sup>Nd</td>
<td/>
<td valign="top" align="center">2 se (10<sup>&#x2013;6</sup>)</td>
<td valign="top" align="center" colspan="3">&#x03B5;<sub>Nd &#x00B1; 2 sd</sub></td>
</tr>
</thead>
<tbody>
<tr>
<td valign="top" align="left" colspan="3"><bold>Unclean foraminifers</bold></td>
<td/>
<td/>
<td/>
<td/>
<td/>
</tr>
<tr>
<td valign="top" align="left">0&#x2013;1 cm</td>
<td valign="top" align="center">MIS 1</td>
<td valign="top" align="center">0.512079</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">8</td>
<td valign="top" align="center">&#x2212;10.9</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0.2</td>
</tr>
<tr>
<td valign="top" align="left">8&#x2013;9 cm</td>
<td valign="top" align="center">MIS 1</td>
<td valign="top" align="center">0.512087</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">8</td>
<td valign="top" align="center">&#x2212;10.7</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0.2</td>
</tr>
<tr>
<td valign="top" align="left">20&#x2013;21 cm</td>
<td valign="top" align="center">MIS 2</td>
<td valign="top" align="center">0.512116</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">5</td>
<td valign="top" align="center">&#x2212;10.2</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0.2</td>
</tr>
<tr>
<td valign="top" align="left">29&#x2013;30 cm</td>
<td valign="top" align="center">MIS 2</td>
<td valign="top" align="center">0.512103</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">12</td>
<td valign="top" align="center">&#x2212;10.4</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0.2</td>
</tr>
<tr>
<td valign="top" align="left">40&#x2013;41 cm</td>
<td valign="top" align="center">MIS 2/3</td>
<td valign="top" align="center">0.512095</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">9</td>
<td valign="top" align="center">&#x2212;10.6</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0.2</td>
</tr>
<tr>
<td valign="top" align="left">70&#x2013;71 cm</td>
<td valign="top" align="center">MIS 3</td>
<td valign="top" align="center">0.512083</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">8</td>
<td valign="top" align="center">&#x2212;10.8</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0.2</td>
</tr>
<tr>
<td valign="top" align="left" colspan="4"><bold>Leached Fe-Mn oxyhydroxides</bold></td>
<td/>
<td/>
<td/>
<td/>
</tr>
<tr>
<td valign="top" align="left">4&#x2013;5 cm</td>
<td valign="top" align="center">MIS 1</td>
<td valign="top" align="center">0.512165</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">9</td>
<td valign="top" align="center">&#x2212;9.2</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0.2</td>
</tr>
<tr>
<td valign="top" align="left">9&#x2013;10 cm</td>
<td valign="top" align="center">MIS 1</td>
<td valign="top" align="center">0.512160</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">6</td>
<td valign="top" align="center">&#x2212;9.3</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0.2</td>
</tr>
<tr>
<td valign="top" align="left">20&#x2013;21 cm</td>
<td valign="top" align="center">MIS 2</td>
<td valign="top" align="center">0.512173</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">4</td>
<td valign="top" align="center">&#x2212;9.1</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0.2</td>
</tr>
<tr>
<td valign="top" align="left">28&#x2013;29 cm</td>
<td valign="top" align="center">MIS 2</td>
<td valign="top" align="center">0.512160</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">8</td>
<td valign="top" align="center">&#x2212;9.3</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0.2</td>
</tr>
<tr>
<td valign="top" align="left">40&#x2013;41 cm</td>
<td valign="top" align="center">MIS 2/3</td>
<td valign="top" align="center">0.512168</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">5</td>
<td valign="top" align="center">&#x2212;9.2</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0.2</td>
</tr>
<tr>
<td valign="top" align="left">50&#x2013;51 cm</td>
<td valign="top" align="center">MIS 3</td>
<td valign="top" align="center">0.512173</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">6</td>
<td valign="top" align="center">&#x2212;9.1</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0.2</td>
</tr>
<tr>
<td valign="top" align="left">60&#x2013;61 cm</td>
<td valign="top" align="center">MIS 3</td>
<td valign="top" align="center">0.512163</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">5</td>
<td valign="top" align="center">&#x2212;9.3</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0</td>
</tr>
<tr>
<td valign="top" align="left">70&#x2013;71 cm</td>
<td valign="top" align="center">MIS 3</td>
<td valign="top" align="center">0.512165</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">8</td>
<td valign="top" align="center">&#x2212;9.2</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0</td>
</tr>
<tr>
<td valign="top" align="left">80&#x2013;81 cm</td>
<td valign="top" align="center">MIS 4</td>
<td valign="top" align="center">0.512197</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">8</td>
<td valign="top" align="center">&#x2212;8.6</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0</td>
</tr>
<tr>
<td valign="top" align="left" colspan="5"><bold>Detrital clay-rich fractions (&#x003C;4 &#x03BC;m)</bold></td>
<td/>
<td/>
<td/>
</tr>
<tr>
<td valign="top" align="left">4&#x2013;5 cm</td>
<td valign="top" align="center">MIS 1</td>
<td valign="top" align="center">0.512060</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">8</td>
<td valign="top" align="center">&#x2212;11.3</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0.2</td>
</tr>
<tr>
<td valign="top" align="left">9&#x2013;10 cm</td>
<td valign="top" align="center">MIS 1</td>
<td valign="top" align="center">0.512046</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">5</td>
<td valign="top" align="center">&#x2212;11.6</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0.2</td>
</tr>
<tr>
<td valign="top" align="left">20&#x2013;21 cm</td>
<td valign="top" align="center">MIS 2</td>
<td valign="top" align="center">0.512051</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">6</td>
<td valign="top" align="center">&#x2212;11.5</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0.2</td>
</tr>
<tr>
<td valign="top" align="left">28&#x2013;29 cm</td>
<td valign="top" align="center">MIS 2</td>
<td valign="top" align="center">0.512050</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">7</td>
<td valign="top" align="center">&#x2212;11.5</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0.2</td>
</tr>
<tr>
<td valign="top" align="left">40&#x2013;41 cm</td>
<td valign="top" align="center">MIS 2/3</td>
<td valign="top" align="center">0.512055</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">6</td>
<td valign="top" align="center">&#x2212;11.4</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0.2</td>
</tr>
<tr>
<td valign="top" align="left">50&#x2013;51 cm</td>
<td valign="top" align="center">MIS 3</td>
<td valign="top" align="center">0.512065</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">5</td>
<td valign="top" align="center">&#x2212;11.2</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0.2</td>
</tr>
<tr>
<td valign="top" align="left">60&#x2013;61 cm</td>
<td valign="top" align="center">MIS 3</td>
<td valign="top" align="center">0.512073</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">7</td>
<td valign="top" align="center">&#x2212;11.0</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0</td>
</tr>
<tr>
<td valign="top" align="left">70&#x2013;71 cm</td>
<td valign="top" align="center">MIS 3</td>
<td valign="top" align="center">0.512043</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">7</td>
<td valign="top" align="center">&#x2212;11.6</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0</td>
</tr>
<tr>
<td valign="top" align="left">80&#x2013;81 cm</td>
<td valign="top" align="center">MIS 4</td>
<td valign="top" align="center">0.512062</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">6</td>
<td valign="top" align="center">&#x2212;11.2</td>
<td valign="top" align="center">&#x00B1;</td>
<td valign="top" align="center">0</td>
</tr>
</tbody>
</table></table-wrap>
<p>For this study, a series of glauconite grains and planktonic foraminifers were collected from six distinct sediment layers (0, 8, 20, 29, 40, and 70 cm) representative of specific time intervals (Holocene, MIS 2, MIS 3) in core IG-KSF-11. Evidence for continuous stratigraphy in this section of core IG-KSF-11 suggests that collected glauconite grains were formed <italic>in situ</italic>. There is no evidence for gravity-induced sediment deposition in this part of the margin. At the Demerara margin, glauconite grains mostly occur as internal fillings of foraminifera. The grains were isolated under the microscope and were then classified into three main colour categories: (1) beige/grey, (2) light green/green, and (3) dark green (<xref ref-type="fig" rid="F4">Figure 4</xref>). Representative samples of each category were selected for SEM observation, using a SEM HITACHI S-4500 (University of Perpignan). Microprobe chemical microanalyses were performed on hemispherical sections obtained after grains were broken. Scanning was performed on both 100 and 2 &#x03BC;m<sup>2</sup> areas in order to obtain representative semi-quantitative analyses of bulk grains and newly formed nano-crystallites.</p>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption><p>Photograph showing the various degrees of glauconitic maturity inferred from colour and characteristic cracks. (1) Beige grains; (2) light green grains; (3) light green grains with cracks; and (4) dark green grains with cracks.</p></caption>
<graphic xlink:href="feart-09-652501-g004.tif"/>
</fig>
<p>For geochemical and Nd isotope analyses of glauconite grains, a few grains of &#x223C;300&#x2013;400 &#x03BC;m size were used. Between 30 and 90 mg of powdered sample were digested on hotplate (120&#x00B0;C; 1 day) with distilled 6 M HCl, following a procedure adapted from <xref ref-type="bibr" rid="B58">Yadav and Sharma (1992)</xref>. This method achieves efficient preferential dissolution of glauconite, yielding almost quantitative recovery of K, while leaving behind more resistant Al- and Si-rich silicate minerals. This implies that major element abundances and ratios (e.g., K<sub>2</sub>O/Al<sub>2</sub>O<sub>3</sub> and Fe<sub>2</sub>O<sub>3</sub>/Al<sub>2</sub>O<sub>3</sub>; see section &#x201C;Discussion&#x201D;) reported here for glauconitic grains may slightly differ from values that would otherwise be obtained for bulk glauconite digested using HF-based mineralisation methods. For the analyses of foraminiferal tests, about 10&#x2013;15 mg of mixed planktonic foraminifera assemblages was prepared using the methodology described in <xref ref-type="bibr" rid="B49">Tachikawa et al. (2014)</xref>, being dissolved using dropwise addition of ultrapure 1 M acetic acid in order to reduce any potential leaching of associated silicate detritus.</p>
<p>In addition, a total of nine bulk sediment samples from the same core interval were processed for isolating Fe-Mn oxyhydroxide phases and detrital clays. Bulk sediments were first treated using a sequential leaching procedure (<xref ref-type="bibr" rid="B6">Bayon et al., 2002</xref>) that successively removes biogenic carbonates (with 5% v/v acetic acid), Fe-Mn oxyhydroxide phases (with a mixed 15% acetic acid&#x2014;0.5 M hydroxylamine hydrochloride solution) and organic matter (with 15% v/v hydrogen peroxide). For Fe-Mn oxyhydroxide phases, the resulting leachates were filtered through 0.45 &#x03BC;m PTFE Nalgene filters, evaporated to dryness, and finally redissolved using ultrapure HNO<sub>3</sub> prior to subsequent elemental analyses. Clay-rich detrital fractions (&#x003C;4 &#x03BC;m) were separated from the residual detrital material using low-speed centrifugation (<xref ref-type="bibr" rid="B9">Bayon et al., 2015</xref>) and further digested by alkaline fusion (<xref ref-type="bibr" rid="B5">Bayon et al., 2009</xref>).</p>
<p>Major and trace element analyses for 6 M HCl digests of glauconite grains were determined at the P&#x00F4;le Spectrom&#x00E9;trie Oc&#x00E9;an (PSO, Brest) with a Thermo Scientific Element XR sector field ICP-MS, using the following masses (<sup>24</sup>Mg, <sup>27</sup>Al, <sup>31</sup>P, <sup>39</sup>K, <sup>44</sup>Ca, <sup>55</sup>Mn, and <sup>57</sup>Fe) acquired in medium mass resolution. Yttrium and REE concentrations were also measured in low resolution mode. Elemental abundances were calculated using the Tm addition method, following the procedures described in <xref ref-type="bibr" rid="B2">Barrat et al. (1996</xref>, <xref ref-type="bibr" rid="B3">2012)</xref>. The internal precision for all measurements was better than 2%. The precision and accuracy of our data were assessed by analysing a series of silicate rock certified reference materials (CRM) having various chemical compositions (AN-G, AGV-1, BCR-1, DNC-1, DR-N, G-2, and WS-E), digested using conventional HF-HCl-HNO<sub>3</sub> method. The results obtained for these reference materials were in full agreement with reference values from the literature (typically &#x003C; 8%), with precisions generally better than 10% (RSD; <italic>n</italic> = 3 for all of the CRMs). Neodymium was isolated using conventional ion chromatography, and isotopic measurements were performed at the PSO-Brest, using a Thermo Scientific Neptune multi-collector ICPMS. Nd isotopic compositions were determined using sample-standard bracketing, by analysing an in-house standard solution (SPEX-Nd) every two samples, yielding a mean value of 0.511687 &#x00B1; 0.000007 (2 SD, <italic>n</italic> = 14). Mass bias corrections were made with the exponential law, using <sup>146</sup>Nd/<sup>144</sup>Nd = 0.7219. Analyses of the JNdi-1 standard solution during the course of this study gave <sup>143</sup>Nd/<sup>144</sup>Nd of 0.512114 &#x00B1; 0.000010 (2 SD, <italic>n</italic> = 8), in full agreement with the reference value of 0.512115 (<xref ref-type="bibr" rid="B52">Tanaka et al., 2000</xref>), and corresponding to an external reproducibility of &#x223C; &#x00B1; 0.2 &#x03B5; (2 SD). Note that epsilon Nd values [&#x03B5;<sub>Nd</sub> = (<sup>143</sup>Nd/<sup>144</sup>Nd<sub>SAMPLE</sub>/<sup>143</sup>Nd/<sup>144</sup>Nd<sub><italic>CHUR</italic></sub> &#x2212; 1) &#x00D7; 10<sup>4</sup>] were calculated using the chondritic (CHUR) <sup>143</sup>Nd/<sup>144</sup>Nd value of 0.512638 (<xref ref-type="bibr" rid="B27">Jacobsen and Wasserburg, 1980</xref>).</p>
</sec>
<sec id="S4">
<title>Results</title>
<sec id="S4.SS1">
<title>Microscopic Observations and SEM Microanalyses</title>
<p>As a general rule, the maturity process of glauconitisation is indicated by darker colour and deeper cracks at the grain surface (<xref ref-type="bibr" rid="B19">Giresse and Wiewi&#x00F3;ra, 2001</xref>; <xref ref-type="bibr" rid="B17">Giresse, 2008</xref>). Therefore, to a first approximation, both the grain colour and its facies can be used to infer the successive stages of glauconitisation in sedimentary records (<xref ref-type="fig" rid="F4">Figure 4</xref>). This descriptive approach was already used by <xref ref-type="bibr" rid="B50">Tallobre et al. (2019)</xref>, indicating that maximum abundance of mature dark green grains in core IG-KSF-11 generally occurred during MIS 2 (between <italic>ca</italic>. 19&#x2013;29 kyr BP) and in MIS 4 (&#x223C;60&#x2013;70 kyr BP), in sediment layers also characterised by high contents of glauconitic grains indicative of enhanced winnowing conditions (<xref ref-type="fig" rid="F3">Figure 3B</xref>). Another layer containing relatively high abundance of dark green mature grains is also encountered near the top of the core of Early Holocene age, where the series is extremely condensed (<xref ref-type="fig" rid="F3">Figure 3B</xref>). The geochemical results obtained from newly acquired SEM/EDS microanalyses of glauconite grains are listed in <xref ref-type="supplementary-material" rid="SM1">Supplementary Table 1</xref> (Al<sub>2</sub>O<sub>3</sub>, K<sub>2</sub>O, Fe<sub>2</sub>O<sub>3</sub>, and MgO) and illustrated in <xref ref-type="fig" rid="F5">Figures 5</xref>, <xref ref-type="fig" rid="F6">6</xref>. These data indicate that at the microscopic scale neoformed microcrystals of dark green grains can yield K<sub>2</sub>O and Fe<sub>2</sub>O<sub>3</sub> concentrations of up to 8 and 42%, respectively (<xref ref-type="fig" rid="F5">Figure 5</xref> and <xref ref-type="supplementary-material" rid="SM1">Supplementary Table 1</xref>). The average Al<sub>2</sub>O<sub>3</sub> concentrations in studied glauconitic grains progressively decrease with the degree of maturity of the grains, from 10.1 &#x00B1; 2.4% (light-coloured grains; <italic>n</italic> = 17), 6.4 &#x00B1; 1.6% (green grains; <italic>n</italic> = 39), and 5.1 &#x00B1; 2.3% (dark green grains; <italic>n</italic> = 11). By contrast, both K<sub>2</sub>O abundances increase from 2.7 &#x00B1; 0.7% (light-coloured) to 3.7 &#x00B1; 0.8% (green) and 5.7 &#x00B1; 1.1%, similar to Fe<sub>2</sub>O<sub>3</sub>: 29.1 &#x00B1; 4.0% (light-coloured) to 32.1 &#x00B1; 3.7% (green) and 35.9 &#x00B1; 4.2% (<xref ref-type="supplementary-material" rid="SM1">Supplementary Table 1</xref>). Finally, measured MgO contents remain near constant in beige and light green grains (2.4&#x2013;4.3%), but decrease in dark green grains (1.1&#x2013;2.6%; <xref ref-type="supplementary-material" rid="SM1">Supplementary Table 1</xref>) due to progressive replacement of 2:1 (Te-Oc-Te) layers of montmorillonite by glauconite.</p>
<fig id="F5" position="float">
<label>FIGURE 5</label>
<caption><p>Structural, microstructural, and chemical compositions of the successive glauconitic sequence in core IG-KSF-11. <bold>(A)</bold> Beige grain exhibiting high porosity (left side), showing microstructural evidence of neoformed glauconitic microcrystals (right side). <bold>(B)</bold> Light green grain with minor cracks (left side), exhibiting honeycomb development of newly formed microcrystals (right side). <bold>(C)</bold> Hummocky dark green grain with marked cracks (left side), showing high density of newly formed microcrystals (right side). Note that the white squares indicate microscanned SEM/EDS areas, with corresponding chemical compositions.</p></caption>
<graphic xlink:href="feart-09-652501-g005.tif"/>
</fig>
<fig id="F6" position="float">
<label>FIGURE 6</label>
<caption><p>Relationship between Fe<sub>2</sub>O<sub>3</sub>/Al<sub>2</sub>O<sub>3</sub> and K<sub>2</sub>O/Al<sub>2</sub>O<sub>3</sub> in glauconitic grains of core IG-KSF-11, based on SEM/EDS microanalyses. Values for Amazon detrital clay are from <xref ref-type="bibr" rid="B9">Bayon et al. (2015)</xref>.</p></caption>
<graphic xlink:href="feart-09-652501-g006.tif"/>
</fig>
</sec>
<sec id="S4.SS2">
<title>Major and Trace Elements and Nd Isotopic Compositions of Glauconitic Grains</title>
<p>The major and trace element concentrations obtained for HCl digests of glauconitic grains are listed in <xref ref-type="table" rid="T1">Table 1</xref>, together with corresponding Nd isotopic compositions. Measured concentrations are reported relative to the initial mass of bulk glauconite grain prior to 6 M HCl digestion. The HCl digests display Fe<sub>2</sub>O<sub>3</sub> and Al<sub>2</sub>O<sub>3</sub> concentrations ranging from 16.1 to 15.0% and 5.9 to 13.2 wt%, respectively. Potassium (K<sub>2</sub>O) concentrations vary from 1.7 to 3.2 wt%, while CaO and P<sub>2</sub>O<sub>5</sub> range from 1.5 to 9.1% and 0.1 to 0.9 wt%, respectively. The major element data are also expressed using K<sub>2</sub>O/Al<sub>2</sub>O<sub>3</sub> and Fe<sub>2</sub>O<sub>3</sub>/Al<sub>2</sub>O<sub>3</sub> ratios (<xref ref-type="fig" rid="F3">Figure 3C</xref>). The REE display abundances significantly lower than those for typical detrital sediments, with Nd ranging between &#x223C;6 and 15 &#x03BC;g/g. Measured REE concentrations are also reported as shale-normalised patterns using values for World River Average Silt (WRAS; <xref ref-type="bibr" rid="B9">Bayon et al., 2015</xref>), displaying marked light-REE enrichments relative to mid- and heavy-REE (<xref ref-type="fig" rid="F7">Figure 7</xref>). The Nd isotopic compositions vary from &#x03B5;<sub>Nd</sub> &#x2212;12.0 (at 0&#x2013;1 and 40&#x2013;41 cm depth) to &#x2212;11.0 (at 20&#x2013;21 cm) (<xref ref-type="fig" rid="F3">Figure 3D</xref>). In comparison, the &#x03B5;<sub>Nd</sub> values determined in corresponding uncleaned foraminifers (between &#x2212;10.9 and &#x2212;10.2) and leached sedimentary Fe-Mn oxyhydroxide phases (between &#x2212;9.3 and &#x2212;8.6) are significantly more radiogenic (<xref ref-type="table" rid="T2">Table 2</xref>). Finally, the Nd isotopic composition of the detrital clay-rich fraction is relatively homogenous along core IG-KSF-11 (between &#x2212;11.6 and &#x2212;11.0), with a mean &#x03B5;<sub>Nd</sub> signature of &#x2212;11.4 &#x00B1; 0.2 (1SD).</p>
<fig id="F7" position="float">
<label>FIGURE 7</label>
<caption><p><bold>(A)</bold> Relationship between Fe<sub>2</sub>O<sub>3</sub>/Al<sub>2</sub>O<sub>3</sub> and K<sub>2</sub>O/Al<sub>2</sub>O<sub>3</sub> for bulk glauconitic grains from core IG-KSF-11 (diamonds), compared to microscale results obtained by SEM/EDS analyses (crosses). <bold>(B)</bold> Shale-normalised REE patterns of bulk glauconitic grains. WRAS refers to World River Average Silt (<xref ref-type="bibr" rid="B9">Bayon et al., 2015</xref>). Note that # refers the sample depth (cm). Values for Amazon detrital clay are from <xref ref-type="bibr" rid="B9">Bayon et al. (2015)</xref>.</p></caption>
<graphic xlink:href="feart-09-652501-g007.tif"/>
</fig>
</sec>
</sec>
<sec id="S5">
<title>Discussion</title>
<sec id="S5.SS1">
<title>Glauconitisation at the Demerara Margin</title>
<p>As already shown in <xref ref-type="bibr" rid="B50">Tallobre et al. (2019)</xref>, the new SEM-EDS data reported in this study indicate that the glauconitic grains formed at site IG-KSF-11 progressively evolve towards darker green shades as they incorporate higher amounts of Fe and K (<xref ref-type="fig" rid="F5">Figures 5</xref>, <xref ref-type="fig" rid="F6">6</xref>). Successive glauconite neoformation steps are also accompanied by a gradual decrease in Al contents, generally reflecting the gradual disappearance of inherited terrigenous 1:1 minerals, such as kaolinite. By contrast, the corresponding increase in K<sub>2</sub>O and Fe<sub>2</sub>O<sub>3</sub> is largely independent of the presence of inherited minerals. The source of K in glauconite is directly derived from ambient bottom water, being sequestered between newly formed and/or transformed micaceous sheets. The abundance of K<sub>2</sub>O thus directly reflects the process of glauconitogenesis (<xref ref-type="bibr" rid="B36">Odin and Fullagar, 1988</xref>; <xref ref-type="bibr" rid="B56">Wiewi&#x00F3;ra et al., 2001</xref>). In the case of core IG-KSF-11, the increase in K<sub>2</sub>O contents, and by inference K<sub>2</sub>O/Al<sub>2</sub>O<sub>3</sub> ratios (<xref ref-type="fig" rid="F5">Figure 5</xref>), most likely corresponds to the presence of neoformed sheets of 2:1 clay minerals, such as K-bearing montmorillonite and illite.</p>
<p>In core IG-KSF-11, the abundance of the different types of glauconite grains displays clear correlation with corresponding &#x03B4;<sup>18</sup>O records for both planktonic and benthic foraminifers over the last three isotopic stages (<xref ref-type="fig" rid="F3">Figure 3</xref>; <xref ref-type="bibr" rid="B50">Tallobre et al., 2019</xref>). The maximum abundance of glauconite grains in the 15&#x2013;60 and 90&#x2013;100 cm core intervals of IG-KSF-11 (expressed by the relative weight glauconitic green grains within the sandy fraction; <xref ref-type="bibr" rid="B50">Tallobre et al., 2019</xref>) coincides with the glacial periods of MIS 2 and MIS 4, respectively (<xref ref-type="fig" rid="F3">Figure 3</xref>). These enriched glauconitic layers were interpreted as reflecting periods characterised by intense winnowing effect, which prevented the burial of the glauconitic grains at that time, favouring their mineralogical evolution at the water&#x2013;sediment interface. Overall, the occurrence of both higher concentrations of glauconitic grains, higher relative abundances of dark green grains, and higher K<sub>2</sub>O/Al<sub>2</sub>O<sub>3</sub> and Fe<sub>2</sub>O<sub>3</sub>/Al<sub>2</sub>O<sub>3</sub> ratios (<xref ref-type="fig" rid="F3">Figure 3</xref>) collectively point towards a higher dynamics of contouritic currents during MIS 2 and MIS 4, in agreement with what had been proposed by <xref ref-type="bibr" rid="B50">Tallobre et al. (2019)</xref>.</p>
</sec>
<sec id="S5.SS2">
<title>Core-Top Evidence for a Seawater-Derived Nd Isotopic Signature in Glauconite</title>
<p>A striking feature is the evidence that core-top glauconitic grains at site IG-KSF-11 display a similar Nd isotopic composition (&#x2212;12.0 &#x00B1; 0.5) than that of the corresponding water mass at the Demerara margin (&#x2212;11.6 &#x00B1; 0.3; <xref ref-type="bibr" rid="B25">Huang et al., 2014</xref>; <xref ref-type="fig" rid="F2">Figure 2</xref>). This finding suggests that in highly dynamic depositional environments, characterised by high bottom current velocity, glauconite grains may capture the Nd isotopic composition of ambient bottom water masses. While radiocarbon dating of planktonic foraminifera assemblages suggested possible loss of the surficial sediment layer upon core recovery, the upper 10 cm of core IG-KSF-11 is still assumed to correspond to the Holocene period, hence covering a period of time during which bottom water &#x03B5;<sub>Nd</sub> signatures are expected to have remained near present-day values. In marked contrast, both uncleaned foraminifera (&#x2212;10.9 &#x00B1; 0.1; 0&#x2013;1 cm depth) and leached sedimentary Fe-Mn oxyhydroxide (&#x2212;9.2 &#x00B1; 0.2; 4&#x2013;5 cm depth) fractions from the same upper sediment layer depart significantly from the expected NADW-like Holocene seawater signature. Neodymium isotopic measurements on uncleaned foraminifera are usually assumed to reflect the signature of associated Fe-Mn oxyhydroxide coatings that precipitate onto and within the foraminifera tests at the seawater&#x2013;sediment interface (e.g., <xref ref-type="bibr" rid="B12">Elmore et al., 2011</xref>; <xref ref-type="bibr" rid="B49">Tachikawa et al., 2014</xref>), hence acquiring the &#x03B5;<sub>Nd</sub> composition of ambient bottom waters. The fact that core-top foraminifera at site IG-KSF-11 do not match similar Nd isotopic composition than the overlying water mass suggests that they were initially derived from another depositional environment, before being transported to site IG-KSF-11 by erosion and subsequent bottom current transport. Considering the &#x03B5;<sub>Nd</sub> distribution along the water column at the Demerara Rise (<xref ref-type="bibr" rid="B25">Huang et al., 2014</xref>; <xref ref-type="fig" rid="F2">Figure 2</xref>), we infer that the foraminifera assemblages encountered in the contourite moat at site IG-KSF-11 may be possibly derived from shallower depositional environments, at water depths between 600 m and 800 m bathed by AAIW.</p>
<p>While Fe-Mn oxyhydroxide phases leached from bulk marine sediments are commonly used as paleoceanographic archives (e.g., <xref ref-type="bibr" rid="B44">Rutberg et al., 2000</xref>; <xref ref-type="bibr" rid="B40">Piotrowski et al., 2005</xref>; <xref ref-type="bibr" rid="B21">Gutjahr et al., 2008</xref>), the Fe-oxide fractions extracted from continental margin sediment records can also include pre-formed continental oxides associated with terrigenous material (e.g., <xref ref-type="bibr" rid="B7">Bayon et al., 2004</xref>; <xref ref-type="bibr" rid="B30">Kraft et al., 2013</xref>; <xref ref-type="bibr" rid="B28">Jang et al., 2020</xref>), hence complicating their use for reconstructing past ocean circulation. In this study, the evidence that leached Fe-oxyhydroxide phases significantly depart from NADW-like &#x03B5;<sub>Nd</sub> values clearly point towards the presence of such pre-formed continental oxides. In fact, recent investigations have shown that river-borne Fe oxides are almost systematically characterised by more radiogenic Nd isotopic compositions relative to the associated detrital material (<xref ref-type="bibr" rid="B23">Hindshaw et al., 2018</xref>; <xref ref-type="bibr" rid="B8">Bayon et al., 2020</xref>; <xref ref-type="bibr" rid="B28">Jang et al., 2020</xref>). This Nd isotope decoupling between paired Fe oxide and detrital silicate fractions has been attributed to the preferential erosion and/or weathering of sedimentary rocks on continents (e.g., <xref ref-type="bibr" rid="B8">Bayon et al., 2020</xref>). For instance, recent sediments deposited near the mouth of the Amazon River display &#x03B5;<sub>Nd</sub> values of &#x2212;8 and &#x2212;10.7 for leached Fe oxides and detrital fractions, respectively (<xref ref-type="bibr" rid="B8">Bayon et al., 2020</xref>). At the Demerara Rise, the main potential sources of sediment include suspended particulate material from the large South American tropical rivers (Amazon, Orinoco, and Maroni) that are subsequently transported by ocean currents. These different sources display pronounced &#x03B5;<sub>Nd</sub> compositional variability, which can be used to trace the origin of the lithogenic material deposited on adjacent ocean margins (<xref ref-type="bibr" rid="B43">Rousseau et al., 2019</xref>). For instance, over the hydrological year, the Amazon River exhibits particulate &#x03B5;<sub>Nd</sub> values ranging from &#x2212;9.8 to &#x2212;11.4 (mean &#x2212;10.6 &#x00B1; 0.6) while the suspended loads of the Orinoco and the Maroni yield &#x2212;14.1 &#x00B1; 0.3 and &#x2212;23.7 &#x00B1; 1.2, respectively. By analogy and in agreement with previous studies (<xref ref-type="bibr" rid="B22">H&#x00E4;ggi et al., 2017</xref>; <xref ref-type="bibr" rid="B59">Zhang et al., 2017</xref>; <xref ref-type="bibr" rid="B11">Crivellari et al., 2018</xref>), we infer that measured Nd isotopic compositions for both detrital (&#x2212;11.4 &#x00B1; 0.2) and Fe-oxide (&#x2212;9.1 &#x00B1; 0.2) fractions in core IG-KSF-11 possibly reflect the dominant presence of Amazon sediments at the studied site.</p>
<p>Taken together, the above findings hence suggest that in highly dynamic environments at continental margins, such as the Demerara Rise, glauconitic grains may be best suited than foraminifera and leached sedimentary Fe-oxides for reconstructing the Nd isotopic composition of ambient bottom water masses.</p>
</sec>
<sec id="S5.SS3">
<title>Mode of Acquisition of Ambient Seawater &#x03B5;<sub>Nd</sub> Signatures by Glauconitic Grains</title>
<p>In contrast with Nd isotopes, which suggest a seawater origin for the core-top glauconitic grains at site IG-KSF-11, the distribution of REE in studied grains is far more equivocal, suggesting a complex mode of acquisition of ambient bottom water &#x03B5;<sub>Nd</sub> signatures. For instance, Y/Ho, i.e., a proxy for the relative contribution of seawater versus terrestrial signatures in marine sediments (<xref ref-type="bibr" rid="B35">Nozaki et al., 1997</xref>) displays values (27.9 &#x00B1; 0.5; <xref ref-type="table" rid="T1">Table 1</xref>) indistinguishable from detrital river sediments worldwide (WRAS; 28.7 &#x00B1; 1.3; <xref ref-type="bibr" rid="B9">Bayon et al., 2015</xref>), far from the range of seawater values (Y/Ho &#x003E; &#x223C;40&#x2013;70; <xref ref-type="bibr" rid="B4">Bau, 1996</xref>). To some extent, this finding could indicate that the initial acquisition of REE by glauconitic grains is set by the dissolution of clay minerals, being modified subsequently by sustained isotopic exchange with seawater. Albeit different, such a process would echo with previous investigations that already suggested that fine-grained particles settling in the ocean could interact with seawater through intense dissolved-particle exchange, resulting in no significant Nd enrichment but overall leading to the acquisition of seawater Nd isotopic signatures (e.g., <xref ref-type="bibr" rid="B29">Jeandel et al., 1995</xref>; <xref ref-type="bibr" rid="B48">Tachikawa et al., 1997</xref>). In marine environments, glauconitisation involves successive dissolutions of dominant 1:1 and subsequent 2:1 clay minerals (smectite), followed by neoformation of other 2:1 micaceous sheets of glauconite. As mentioned above, the process of glauconitisation is accompanied by the loss of several cations (Al and even Si) and the enrichment of other major elements such as Fe and K. Dissolution can also occur when the starting clay phase is mainly composed of 1:1 clay minerals, such as kaolinite. For example, in the case of Fe-bearing montmorillonite green grains from the Ivory Coast-Ghana marginal ridge (ODP Site 359), kaolinite was shown to dissolve slowly with remnants of d (001) and d (060) peaks of kaolinite being still present in the pristine light coloured grains (<xref ref-type="bibr" rid="B56">Wiewi&#x00F3;ra et al., 2001</xref>). At the Demerara Rise, this process can also be illustrated using Fe<sub>2</sub>O<sub>3</sub>/Al<sub>2</sub>O<sub>3</sub> versus K<sub>2</sub>O/Al<sub>2</sub>O<sub>3</sub> ratios determined in bulk glauconite grains (<xref ref-type="fig" rid="F7">Figure 7</xref>), where the observed positive relationship (which perfectly matches with the correlation defined by SEM/EDS data; <xref ref-type="fig" rid="F6">Figure 6</xref>) indicates increasing glauconitisation and seawater influence as both Fe<sub>2</sub>O<sub>3</sub>/Al<sub>2</sub>O<sub>3</sub> and K<sub>2</sub>O/Al<sub>2</sub>O<sub>3</sub> ratios increase. In core IG-KSF-11, the highest Fe and K concentrations are encountered in grains formed during MIS 2 (at 20 and 28 cm depth), in full agreement with the preferential abundance of dark green grains in the corresponding sediment interval, indicative of greater degree of glauconitisation and a longer residence time due to strengthened bottom current activity.</p>
<p>Interestingly, the shale-normalised REE patterns of the green glauconite grains extracted from our Demerara contourite sediments indicate that increasing degrees of glauconitisation is accompanied by a net loss in REE (<xref ref-type="fig" rid="F7">Figure 7</xref>). This finding echoes with previous works conducted on glauconitic grains of both Recent (<xref ref-type="bibr" rid="B45">Stille and Clauer, 1994</xref>) and Cenozoic (<xref ref-type="bibr" rid="B54">T&#x00F3;th et al., 2010</xref>) ages, which reported similar observations that the REE contents of glauconite grains gradually decrease during glauconitisation. These latter authors proposed that the progressive REE loss during glauconitisation directly resulted from the crystallographic transformation of the phyllosilicate layers, leading to the combined depletion of both Ca and REE (<xref ref-type="bibr" rid="B54">T&#x00F3;th et al., 2010</xref>). Additionally, one striking feature of the studied glauconitic grains from core IG-KSF-11 is that they display apparent LREE enrichment relative to MREE and HREE, resulting in shale-normalised patterns that depart significantly from both the typical seawater and detrital distribution patterns (<xref ref-type="fig" rid="F7">Figure 7</xref>). As previously proposed, this particular REE signature could possibly relate to the presence of discrete authigenic REE-rich phosphate phases, such as cryptocrystalline apatite, which are typically found in close association with green glauconite grains in the sedimentary record (<xref ref-type="bibr" rid="B45">Stille and Clauer, 1994</xref>; <xref ref-type="bibr" rid="B57">Wigley and Compton, 2007</xref>; <xref ref-type="bibr" rid="B54">T&#x00F3;th et al., 2010</xref>; <xref ref-type="bibr" rid="B26">Huggett et al., 2017</xref>). Present as inclusions within glauconitic grains, these authigenic REE-rich phosphate phases are thought to play an important role in controlling the REE budget of glauconitic grains (<xref ref-type="bibr" rid="B45">Stille and Clauer, 1994</xref>; <xref ref-type="bibr" rid="B54">T&#x00F3;th et al., 2010</xref>). At the Demerara margin, studied grains display no direct correlation between both P<sub>2</sub>O<sub>5</sub> and REE contents (<xref ref-type="table" rid="T2">Table 2</xref>), possibly suggesting that the REE composition of accessory phosphate phases may vary substantially amongst glauconitic grains. Nevertheless, based on the above consideration, we propose that the presence of such discrete authigenic phosphate minerals most likely explain why glauconitic grains at the Demerara margin can faithfully record the Nd isotopic composition of ambient bottom waters. In any case, our results suggest that increasing glauconite maturity results in progressive loss of the &#x03B5;<sub>Nd</sub> signature of inherited clay minerals, most likely accompanied by a gradual shift towards seawater Nd isotope composition. To some extent, this finding would also be in agreement with the evidence that other authigenic phosphate mineral phases (hydroxyfluorapatite), which control the REE budget of fish teeth following their deposition at seafloor, also act as reliable recorders of the Nd isotopic composition of bottom waters (e.g., <xref ref-type="bibr" rid="B33">Martin and Haley, 2000</xref>; <xref ref-type="bibr" rid="B34">Martin and Scher, 2004</xref>).</p>
</sec>
<sec id="S5.SS4">
<title>Preliminary Paleoceanographic Implications</title>
<p>As mentioned above, the occurrence of both higher concentrations of glauconitic grains and increasing relative abundances of more evolved dark green grains during MIS 2 has been interpreted as reflecting a strengthening of bottom water circulation along the Demerara margin during glacial times (<xref ref-type="bibr" rid="B50">Tallobre et al., 2019</xref>). Since the studied site is located in the core interval of the modern NADW, at a water depth of &#x223C;2400 m, this finding was taken as evidence for an intensification of the glacial AMOC. This hypothesis was in agreement with recent &#x03B5;<sub>Nd</sub>-based paleoceanographic reconstructions, which suggested sustained production of glacial NADW during the last glacial period (<xref ref-type="bibr" rid="B24">Howe et al., 2016</xref>; <xref ref-type="bibr" rid="B41">P&#x00F6;ppelmeier et al., 2020</xref>). Our newly acquired data also provide additional support for a vigorous flow of the glacial analogue of NADW at the Demerara margin. First, our major element data for bulk glauconite grains further indicate that glauconitisation was enhanced at that time as inferred from significant enrichments in Fe and K in neoformed glauconitic minerals, hence also pointing towards intensifying winnowing during glacial periods (<xref ref-type="fig" rid="F3">Figure 3C</xref>). Second, our Nd isotope data for the glauconitic grains formed during MIS 2 (<xref ref-type="fig" rid="F3">Figure 3D</xref>) indicate no major change in the &#x03B5;<sub>Nd</sub> signature of ambient bottom water masses during glacials (between &#x2212;11.0 and &#x2212;11.7) relative to their present-day composition (&#x2212;11.6 &#x00B1; 0.3; <xref ref-type="bibr" rid="B25">Huang et al., 2014</xref>). The evidence that the glacial NADW flowing along the Demerara margin was slightly more radiogenic compared to the modern NADW &#x03B5;<sub>Nd</sub> signature could be explained by the fact that northern-sourced waters may have acquired a distinctive Nd isotopic composition at that time (&#x2212;10.4 &#x00B1; 1.0), reflecting the impact of ice sheets on nearby continents on the release of dissolved Nd to the North Atlantic (<xref ref-type="bibr" rid="B60">Zhao et al., 2019</xref>). This finding is in agreement with the results obtained by <xref ref-type="bibr" rid="B25">Huang et al. (2014)</xref> on uncleaned foraminifera extracted from a nearby shallower sediment core (&#x223C;950 m), which also indicated similar &#x03B5;<sub>Nd</sub> composition for the overlying AAIW during the Holocene and the LGM. Taken together, these two &#x03B5;<sub>Nd</sub> records hence collectively suggest that the structure of the water column at the Demerara margin during glacial times was probably similar to its modern oceanographic configuration.</p>
</sec>
</sec>
<sec id="S6">
<title>Conclusion and Perspectives</title>
<p>Our geochemical investigation of glauconitic grains recovered from a contourite sediment sequence at the Demerara margin suggests that authigenic glauconite can faithfully record the Nd isotopic composition of ambient bottom water masses. The acquisition of &#x03B5;<sub>Nd</sub> seawater signatures in glauconitic grains appears to be controlled by the presence of LREE-enriched phases, possibly corresponding to dispersed authigenic phosphate phases intertwined within the neoformed clay mineral sheets. The absence of a strong detrital control on measured Nd isotopic compositions in glauconite grains is further inferred from the evidence for a progressive loss of REE with increasing degrees of glauconitisation; a process that also results in gradual enrichments in Fe and K. Overall, our new results suggest that the application of Nd isotopes to glauconite grains could serve as useful proxies for paleoceanographic reconstructions at continental margins, wherever intense winnowing and/or erosional processes may prevent the use of other more conventional archives of past seawater &#x03B5;<sub>Nd</sub> compositions, such as uncleaned foraminifera or leached Fe-Mn oxyhydroxide fractions. In particular, the combined use of Nd isotopes (as tracers of water mass) and various elemental ratios, such as Fe<sub>2</sub>O<sub>3</sub>/Al<sub>2</sub>O<sub>3</sub> and K<sub>2</sub>O/Al<sub>2</sub>O<sub>3</sub> (as tracers for the degree of glauconitisation), could provide complementary information of both the source and strength of past bottom water circulation. An important requisite prior to establishing Nd isotopes in glauconite grains as robust paleoceanographic archives will be to further demonstrate the preliminary findings reported in this study, by investigating additional sites from the Demerara Rise or from any other contourite systems where bottom water masses and local detrital sediment may display contrasted Nd isotopic compositions.</p>
</sec>
<sec id="S7">
<title>Data Availability Statement</title>
<p>The original contributions presented in the study are included in the article/<xref ref-type="supplementary-material" rid="SM1">Supplementary Material</xref>. Further inquiries can be directed to the corresponding author/s.</p>
</sec>
<sec id="S8">
<title>Author Contributions</title>
<p>PG and GB contributed to the conception and design of the study and wrote the manuscript with contributions from all authors. CT contributed to the first visual analysis and counting of glauconitic grains in core IKSF11. PG and CT prepared the glauconitic grains and conducted SEM observations and analyses. GB performed all REE and Nd isotopic compositions. LL was the head scientist of the IGUANES cruise allowing the acquisition of IKSF11 core and contributed to the regional understanding of the study area. All authors contributed to the article and approved the submitted version.</p>
</sec>
<sec sec-type="COI-statement" id="conf1">
<title>Conflict of Interest</title>
<p>The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.</p>
</sec>
</body>
<back>
<fn-group>
<fn fn-type="financial-disclosure">
<p><bold>Funding.</bold> The geochemical analyses were performed through internal funding at IFREMER.</p>
</fn>
</fn-group>
<ack>
<p>We thank the crews of R/V <italic>L&#x2019;Atalante</italic> and all participants of the IGUANES cruise (2013; Chief scientist: Lies Loncke, <ext-link ext-link-type="uri" xlink:href="https://doi.org/10.17600/13010030">https://doi.org/10.17600/13010030</ext-link>) for their assistance at sea. We are most grateful to Alexis De Prunel&#x00E9; for assistance during MC-ICPMS measurements. We also greatly thank two reviewers for providing insightful and constructive comments, together with CM for editorial handling.</p>
</ack>
<sec id="S11" sec-type="supplementary material"><title>Supplementary Material</title>
<p>The Supplementary Material for this article can be found online at: <ext-link ext-link-type="uri" xlink:href="https://www.frontiersin.org/articles/10.3389/feart.2021.652501/full#supplementary-material">https://www.frontiersin.org/articles/10.3389/feart.2021.652501/full#supplementary-material</ext-link></p>
<supplementary-material xlink:href="Table_1.xlsx" id="SM1" mimetype="application/vnd.openxmlformats-officedocument.spreadsheetml.sheet" xmlns:xlink="http://www.w3.org/1999/xlink"/>
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