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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="publisher-id">876913</article-id>
<article-id pub-id-type="doi">10.3389/feart.2022.876913</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>Gas Hydrate Dissociation Events During LGM and Their Potential Trigger of Submarine Landslides: Foraminifera and Geochemical Records From Two Cores in the Northern South China Sea</article-title>
<alt-title alt-title-type="left-running-head">Huang et al.</alt-title>
<alt-title alt-title-type="right-running-head">Gas Hydrate Submarine Landslides Foraminifera</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname>Huang</surname>
<given-names>Yi</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Cheng</surname>
<given-names>Jun</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Wang</surname>
<given-names>Mingmin</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Wang</surname>
<given-names>Shuhong</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<uri xlink:href="https://loop.frontiersin.org/people/865486/overview"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Yan</surname>
<given-names>Wen</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
</contrib-group>
<aff id="aff1">
<sup>1</sup>
<institution>Southern Marine Science and Engineering Guangdong Laboratory (Guangzhou)</institution>, <addr-line>Guangzhou</addr-line>, <country>China</country>
</aff>
<aff id="aff2">
<sup>2</sup>
<institution>Key Laboratory of Ocean and Marginal Sea Geology</institution>, <institution>South China Sea Institute of Oceanology, Chinese Academy of Sciences</institution>, <addr-line>Guangzhou</addr-line>, <country>China</country>
</aff>
<aff id="aff3">
<sup>3</sup>
<institution>University of Chinese Academic of Sciences</institution>, <addr-line>Beijing</addr-line>, <country>China</country>
</aff>
<author-notes>
<fn fn-type="edited-by">
<p>
<bold>Edited by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1420576/overview">Lihua Zuo</ext-link>, Texas A&#x26;M University Kingsville, United States</p>
</fn>
<fn fn-type="edited-by">
<p>
<bold>Reviewed by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/110958/overview">Luigi Jovane</ext-link>, University of S&#xe3;o Paulo, Brazil</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/934554/overview">Xianrong Zhang</ext-link>, Qingdao Institute of Marine Geology (QIMG), China</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: Shuhong Wang, <email>wshds@scsio.ac.cn</email>
</corresp>
<fn fn-type="other">
<p>This article was submitted to Marine Geoscience, a section of the journal Frontiers in Earth Science</p>
</fn>
</author-notes>
<pub-date pub-type="epub">
<day>16</day>
<month>05</month>
<year>2022</year>
</pub-date>
<pub-date pub-type="collection">
<year>2022</year>
</pub-date>
<volume>10</volume>
<elocation-id>876913</elocation-id>
<history>
<date date-type="received">
<day>16</day>
<month>02</month>
<year>2022</year>
</date>
<date date-type="accepted">
<day>28</day>
<month>04</month>
<year>2022</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2022 Huang, Cheng, Wang, Wang and Yan.</copyright-statement>
<copyright-year>2022</copyright-year>
<copyright-holder>Huang, Cheng, Wang, Wang and Yan</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>Although submarine slope failures and occurrence of gas hydrates are well known in the Dongsha area of the South China Sea the potential relationship between the aforementioned phenomena has not been clearly understood yet. Herein, we present carbon and oxygen isotope compositions of benthic foraminifera and sulfur isotopic composition of chromium reducible sulfur (CRS; &#x3b4;<sup>34</sup>S<sub>CRS</sub>) from two cores from the Dongsha slope, aiming at identifying gas hydrate dissociation events in geological history. The geochemical data indicated that a large amount of gas hydrate dissociated at the beginning of the Last Glacial Maximum (LGM). Meanwhile, disturbances in the sedimentary strata revealed that a submarine landslide occurred at the end of the Last Glacial Maximum. Moreover, the associated abrupt increase of benthic foraminifera abundance implies that the submarine landslide was probably caused by an intense methane releasing from gas hydrate dissociation. A smaller scale submarine landslide related to gas hydrate dissociation was also recorded in core 973-5, retrieved from the flat area at the base of the slope.</p>
</abstract>
<kwd-group>
<kwd>gas hydrate</kwd>
<kwd>submarine landslide</kwd>
<kwd>benthic foraminifera</kwd>
<kwd>Dongsha area</kwd>
<kwd>South China Sea</kwd>
</kwd-group>
</article-meta>
</front>
<body>
<sec id="s1">
<title>Introduction</title>
<p>It is known that methane-rich fluids due to subsurface gas hydrate dissociation leak to the seafloor at specific sites on continental slopes the world over (<xref ref-type="bibr" rid="B6">Boetius and Wenzhoefer, 2013</xref>). In these systems, usually most of the methane and higher hydrocarbons are consumed by anaerobic oxidation of methane (AOM) coupled with sulfate reduction in the uppermost sedimentary layers (<xref ref-type="bibr" rid="B5">Boetius et al., 2000</xref>; <xref ref-type="bibr" rid="B6">Boetius and Wenzhoefer, 2013</xref>). This process leads to geochemical anomalies in the shallow surface sediment and porewater, favoring the precipitation of authigenic carbonates in the sulfate-methane transition zone (SMTZ) (<xref ref-type="bibr" rid="B6">Boetius and Wenzhoefer, 2013</xref>). Thus, AOM signals can be recorded by geochemical anomalies in authigenic carbonates, such as extremely negative &#x3b4;<sup>13</sup>C values (<xref ref-type="bibr" rid="B53">Roberts and Aharon, 1994</xref>; <xref ref-type="bibr" rid="B47">Peckmann and Thiel, 2004</xref>; <xref ref-type="bibr" rid="B49">Pierre et al., 2016</xref>). Authigenic carbonates are good archives to study methane seepage, but because of it is not continuous when precipating and sometimes difficult to get proper samples, it is hard to reveal the evolution of the whole process of methane seepage. In contrast, sediment cores can serve as a potential archive to reconstruct the evolution of past methane seepage, especially when combined with age data (<xref ref-type="bibr" rid="B3">Bayon et al., 2015</xref>; <xref ref-type="bibr" rid="B36">Li et al., 2018</xref>). Specifically, &#x3b4;<sup>34</sup>S<sub>CRS</sub> of sediments and &#x3b4;<sup>13</sup>C of foraminifera are the most commonly used research object in sediment cores. The &#x3b4;<sup>34</sup>S<sub>CRS</sub> in the sediments is confirmed to be heavier in the SMTZ where the sulfate concentrations in the pore water has a rapid decrease, and consequently this value can be used to recognize paleo-SMTZs in the geological record (<xref ref-type="bibr" rid="B48">Peketi et al., 2012</xref>; <xref ref-type="bibr" rid="B7">Borowski et al., 2013</xref>; <xref ref-type="bibr" rid="B22">Gong et al., 2018</xref>). Benthic foraminifera near cold seep areas generally occur in large quantities, with wide areal distributions, short life cycles and stable shell preservation in the sediments after death. Thus, they are excellent for recording the effects of gas hydrate dissociation (<xref ref-type="bibr" rid="B51">Rathburn et al., 2000</xref>; <xref ref-type="bibr" rid="B50">Portilho-Ramos et al., 2018</xref>). Benthic foraminifera associations (<xref ref-type="bibr" rid="B42">Panieri, 2005</xref>) and the stable isotope composition of specific benthic foraminifera can therefore be used to record methane seepage activity in the geological record (<xref ref-type="bibr" rid="B67">Wefer et al., 1994</xref>; <xref ref-type="bibr" rid="B61">Stott et al., 2002</xref>; <xref ref-type="bibr" rid="B25">Herguera et al., 2014</xref>; <xref ref-type="bibr" rid="B57">Schneider et al., 2018</xref>). Although the fact that epigenetic carbonate precipitation plays a dominant role in the distinctly negative &#x3b4;<sup>13</sup>C record of benthic foraminifera is still controversial (<xref ref-type="bibr" rid="B17">Consolaro et al., 2015</xref>; <xref ref-type="bibr" rid="B45">Panieri et al., 2017</xref>), it is opportune to mention that the microstructure and geochemical characteristics of foraminifera influenced by post diagenesis can also trace the methane emissions in a geological period (<xref ref-type="bibr" rid="B56">Schneider et al., 2017</xref>). So AOM signals in cold seep environments are recorded in the foraminifera shells. It is well known that hydrate dissociation are likely to trigger intensive methane seepage (<xref ref-type="bibr" rid="B12">Chen et al., 2016</xref>), resulting in an abnormally high pore pressure and a reduction in the effective stress of continental slope sediments. When the amount of gas emission is massive enough or the continental slope with gas hydrate is steep, the fluidized decomposition zone will form a downward sliding surface. In this situation, any small perturbation of the stress, such as an earthquake, or the self-gravity of the sediments, may lead to slope failure (<xref ref-type="bibr" rid="B31">Kayen and Lee, 1991</xref>). Many submarine landslides are proved to be related to gas hydrate dissociation in the world, including the Storegga slide, off the coast of Norway, and Cape Fear, on the Atlantic continental slope (<xref ref-type="bibr" rid="B33">Leynaud et al., 2004</xref>; <xref ref-type="bibr" rid="B60">Solheim et al., 2005</xref>; <xref ref-type="bibr" rid="B10">Chaytor et al., 2009</xref>; <xref ref-type="bibr" rid="B26">Horozal et al., 2017</xref>). In the geological history, there are also some numerical simulation and sedimentary records that demonstrate the rapid changes of sedimentation affect the gas seepage activity, which also indicates the spatial and temporal charateristics of methane seepage (<xref ref-type="bibr" rid="B30">Karstens et al., 2018</xref>; <xref ref-type="bibr" rid="B59">Screaton et al., 2019</xref>). However, other researches argue that the destabilization of a hydrate system is a slow process and could be largely delayed by overpressure accumulation (<xref ref-type="bibr" rid="B16">Colin et al., 2020</xref>). Recently, climate-driven increase in temperature, especially during last deglacial (MIS5e), is proved to be a trigger factor of gas hydrate dissociation in SCS (<xref ref-type="bibr" rid="B13">Chen et al., 2019</xref>). Thus, the questions concerning the main cause of gas hydrate dissociation are still under debate, the subsequently methane seepage and its potential link to the submarine landslides are poorly documented. Many studies have identified the occurrence of fluidized decomposition zone by geophysical methods, such as seisetic reflection data (<xref ref-type="bibr" rid="B18">Eiger et al., 2017</xref>; <xref ref-type="bibr" rid="B24">Handwerger et al., 2017</xref>), little attention has been paid to the geochemical characteristics of gas hydrate and landslide deposits. The Dongsha area, which is located on the continental slope of the northeastern South China Sea (SCS), is an excellent area for such a study. The extensive development of gas chimneys, submarine landslides, mud diapirs, carbonate mounds and active cold seeps in this area (<xref ref-type="bibr" rid="B11">Chen et al., 2005</xref>; <xref ref-type="bibr" rid="B70">Yan et al., 2006</xref>; <xref ref-type="bibr" rid="B71">Yu et al., 2013</xref>; <xref ref-type="bibr" rid="B19">Feng and Chen, 2015</xref>; <xref ref-type="bibr" rid="B69">Wu et al., 2018</xref>), strongly suggests the occurrence of gas hydrate reservoirs (<xref ref-type="bibr" rid="B11">Chen et al., 2005</xref>; <xref ref-type="bibr" rid="B34">Li et al., 2011</xref>; <xref ref-type="bibr" rid="B62">Su et al., 2012</xref>). Here, by using the carbon-sulfate-benthic foraminifera system, two sediment cores in Dongsha slope are used to identify gas hydrate dissociation events and discuss the causal relationship between gas emissions and submarine landslides.</p>
</sec>
<sec sec-type="materials|methods" id="s2">
<title>Materials and Methods</title>
<p>Sediment cores 973-4 and 973-5 were collected from the middle of the slope and the flat area at the base of the Dongsha area, in the northern SCS, respectively, using a piston corer during the 973 cruise by the ship &#x201c;R/V OceanVI&#x201d; in 2011 (<xref ref-type="table" rid="T1">Table 1</xref>; <xref ref-type="fig" rid="F1">Figure 1</xref>).</p>
<table-wrap id="T1" position="float">
<label>TABLE 1</label>
<caption>
<p>The location and length of the sample cores.</p>
</caption>
<table>
<thead valign="top">
<tr>
<th align="left">Core name</th>
<th align="center">Longitude (E)</th>
<th align="center">Latitude(N)</th>
<th align="center">Water depth(m)</th>
<th align="center">Length(m)</th>
</tr>
</thead>
<tbody valign="top">
<tr>
<td align="left">973-4</td>
<td align="center">118&#xb0;49.0818&#x2032;</td>
<td align="center">21&#xb0;54.3247&#x2032;</td>
<td align="char" char=".">1,666</td>
<td align="char" char=".">13.75</td>
</tr>
<tr>
<td align="left">973-5</td>
<td align="center">119&#xb0;11.0066&#x2032;</td>
<td align="center">21&#xb0;18.5586&#x2032;</td>
<td align="char" char=".">2,998</td>
<td align="char" char=".">9.25</td>
</tr>
</tbody>
</table>
</table-wrap>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>Sampling stations in the Dongsha area of the northern SCS. Red stars represent the two sampling cores 973-4 and 973-5, and the yellow star represents the core 973-3 (<xref ref-type="bibr" rid="B15">Chen et al., 2014</xref>).</p>
</caption>
<graphic xlink:href="feart-10-876913-g001.tif"/>
</fig>
<p>The core 973-4 is mostly made of grey and grey-green clay, with coarser-grain-size silt at the depth of 450&#x2013;600&#xa0;cm, in which foraminifera is abundant. Below 600&#xa0;cm, there are black hydrogen sulfide disseminated plaque deposits with a distinct smell of rotten eggs. For the core 973-5, it is also mostly made of grey to grey-dark clay, the obvious foraminifera enriched silt layer occurred at around 250 &#x223c;300&#xa0;cm there is an angular unconformity at around 460&#xa0;cm. Sediment samples were collected every 2&#xa0;cm from 15&#xa0;cm bsf (below the seafloor) to the core bottom, except in the top 15&#xa0;cm of each core, where only one sample was collected. Grain size measurements were carried out at the South China Sea Institution of Oceanology, Chinese Academic of Sciences, using a Mastersizer2000 Laser Particle Size Analyzer. The particle classification was 1&#x3a6; [&#x424; &#x3d; &#x2212;log<sub>2</sub>d; d means particle diameter (mm)]. The detection limit was between 0.5 and 2000&#xa0;&#x3bc;m, and the relative error was less than 3%. The benthic foraminifera <italic>Uvigerina</italic> spp. and <italic>Bulimina</italic> spp. were picked from the &#x3e;200&#xa0;&#x3bc;m-size fractions to calculate the assemblage density (number of individuals per gram of dry sediment) and perform the isotopic analysis (<italic>Uvigerina</italic> spp.). The &#x3b4;<sup>13</sup>C and &#x3b4;<sup>18</sup>O isotopes of foraminifera tests were measured on aMAT253 Stable Isotope Gas Mass Spectrometer in the South China Sea Institution of Oceanology, Chinese Academic of Sciences and calibrated to the VPDB standard. Analytical precision was estimated to be better than 0.03&#x2030; for &#x3b4;<sup>13</sup>C and 0.08&#x2030; for &#x3b4;<sup>18</sup>O. CRS (chromium reducible sulfur, mainly FeS, FeS<sub>2</sub>) in the bulk sediments were extracted following the method of Canfield (<xref ref-type="bibr" rid="B8">Canfield et al., 1986</xref>). two to five gcarbonate powder was digested in 6&#xa0;mol/L HCl at 50&#xb0;C for 6&#xa0;h to release acid volatile sulfur under a continuous flow of N2 (g) and the residue (remain mainly as FeS and FeS<sub>2</sub>) was analyzed for bulk carbonate CRS. CRS was extracted using 6&#xa0;N HCl and 1M CrCl<sub>2</sub> for 3&#xa0;h in 100% N2 atmosphere. The H2S evolved was driven via N2 carrier into 0.1&#xa0;N AgNO<sub>3</sub> and trapped as Ag<sub>2</sub>S for gravimetric and then isotopic measurements (<xref ref-type="bibr" rid="B22">Gong et al., 2018</xref>). The sulfur isotope analysis was performed at the Louisiana State University, using an Elemental Analyzer (EA) at 980&#xb0;C, and subsequently with a Thermo-Electron Delta V Plus Advantage mass spectrometer. The standard deviation associated with &#x3b4;<sup>34</sup>S analysis was &#xb1;0.3&#x2030;, and reported relative to the VCDT (Vienna Canyon Diablo Troilite) standard.</p>
</sec>
<sec sec-type="results" id="s3">
<title>Results</title>
<sec id="s3-1">
<title>Median Particle Size</title>
<p>Median particle size is commonly used to represent the average particle size of sediments (<xref ref-type="bibr" rid="B27">Hu et al., 2017</xref>; <xref ref-type="bibr" rid="B36">Li et al., 2018</xref>). The sediments in core 973-4 were fine-grained in most layers, but the grain size in the 4.3&#x2013;6.0&#xa0;m layer was significantly coarser (<xref ref-type="fig" rid="F2">Figure 2</xref>). Core 973-5 contained fine-grained sediment in most layers, without any significant differences in the particle size being observed throughout the core; only a minor increase in coarser content was found in several layers (e.g., 1.3&#x2013;2.7&#xa0;m, 3.9&#x2013;4.0&#xa0;m, 5.9&#x2013;6.0&#xa0;m, 8.2&#x2013;8.4&#xa0;m, <xref ref-type="fig" rid="F3">Figure 3</xref>).</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>Sediment particle size and geochemical records of core 973-4, lithostratigraphic picture (left) <bold>(A)</bold> Medium size, <bold>(B)</bold> quantity of <italic>Uvigerina</italic> spp., <bold>(C)</bold> quantity of <italic>Bulimina</italic> spp., <bold>(D)</bold> oxygen isotopes of <italic>Uvigerina</italic> spp., <bold>(E)</bold> carbon isotopes of <italic>Uvigerina</italic> spp., <bold>(F)</bold> CRS, <bold>(G)</bold> sulfur isotopic compositions. The triangles indicate the AMS<sup>14</sup>C dating results (<xref ref-type="bibr" rid="B72">Zhang et al., 2018</xref>); the dashed lines indicate the demarcation lines of MIS1/MIS2 and MIS2/MIS3; and the shadowed horizon indicates horizons influenced by submarine landslides.</p>
</caption>
<graphic xlink:href="feart-10-876913-g002.tif"/>
</fig>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption>
<p>Sediment particle size and geochemical records of core 973-5,lithostratigraphic picture (left) <bold>(A)</bold> Medium size, <bold>(B)</bold> quantity of <italic>Uvigerina</italic> spp., <bold>(C)</bold> quantity of <italic>Bulimina</italic> spp., <bold>(D)</bold> oxygen isotopes of <italic>Uvigerina</italic> spp., <bold>(E)</bold> carbon isotopes of <italic>Uvigerina</italic> spp., <bold>(F)</bold> CRS, <bold>(G)</bold> sulfur isotopic compositions, triangles indicate the AMS <sup>14</sup>C dating results (<xref ref-type="bibr" rid="B66">Wang, 2013</xref>); the dashed lines indicate the demarcation lines of MIS1/MIS2 and MIS2/MIS3; and the shadowed horizon indicates horizons influenced by submarine landslides.</p>
</caption>
<graphic xlink:href="feart-10-876913-g003.tif"/>
</fig>
</sec>
<sec id="s3-2">
<title>Foraminifera Content</title>
<p>The foraminifera-rich layer (4.3&#x2013;6.0&#xa0;m) in core 973-4 is consistent with the high content of the sediment coarse fraction (<xref ref-type="fig" rid="F2">Figures 2B,C</xref>). The numbers of the two species were almost always less than five per gram below 6&#xa0;m bsf. This number increases abruptly to more than 10 per gram at about 6&#xa0;m bsf and then gradually decreases upward until 4.3&#xa0;mbsf. Low values are observed in the uppermost 4.3&#xa0;m bsf of the core (<xref ref-type="fig" rid="F2">Figures 2B,C</xref>). In core 973-5, the numbers of benthic foraminifera were far less than core in 973-4 and few foraminifera were seen in the whole core, except in a few layers (e.g., at depths of about 2.5&#xa0;m, 4.0&#x2013;5.5, and 6&#xa0;m; <xref ref-type="fig" rid="F3">Figures 3B,C</xref>).</p>
</sec>
<sec id="s3-3">
<title>Carbon and Oxygen Isotope Compositions of Uvigerina</title>
<p>The &#x3b4;<sup>18</sup>O composition of Uvigerina spp. in the core 973-4 varied from 2.57 to 5.26&#x2030;, with lighter &#x3b4;<sup>18</sup>O values in the upper part of the core (<xref ref-type="fig" rid="F2">Figure 2D</xref>). The &#x3b4;18O depletion fits well with the Deglaciation transition layer at about 4.3&#xa0;m bsf and shows stable values in the uppermost core. In core 973-5, &#x3b4;<sup>18</sup>O values show a broad range of variation below 5.5&#xa0;m bsf (<xref ref-type="fig" rid="F3">Figure 3D</xref>), and values between 2.93 and 4.49&#x2030; at the 3.3&#x2013;3.6&#xa0;m bsf layer, corresponding to the deglaciation transition. The &#x3b4;<sup>13</sup>C values for Uvigerina spp. in core 973-4 ranged from &#x2212;1.97 to 0.25&#x2030; with an average value of &#x2212;1.15&#x2030; (<xref ref-type="fig" rid="F2">Figure 2E</xref>). The &#x3b4;<sup>13</sup>C values below 4.3&#xa0;m bsf are obviously negative, with only small fluctuations; above this depth they become heavier until the surface. In core 973-5, the &#x3b4;13C values were consistently negative below the depth of 3.3&#xa0;m bsf and showed heavier trend from -2.9 to 0.18&#x2030; in the upper part of the core (<xref ref-type="fig" rid="F3">Figure 3E</xref>).</p>
</sec>
<sec id="s3-4">
<title>CRS and &#x3b4;<sup>34</sup>SCRS Values</title>
<p>In core 973-4, the CRS contents vary between 0.01 wt&#x2030; and 0.95 wt&#x2030;. A high CRS content was observed in the interval 6.8&#x2013;9.0&#xa0;m (<xref ref-type="fig" rid="F2">Figure 2G</xref>). The &#x3b4;<sup>34</sup>SCRS values show a wide variation, ranging from &#x2212;43.8 to 32.6&#x2030;. The sulfate isotope compositions show extremely positive values at the CRS enrichment depth (6.8&#x2013;9.0&#xa0;m), and then are lower elsewhere, with a minimum value of &#x2212;43.8&#x2030; in the interval 2.8&#x2013;5.6&#xa0;m (<xref ref-type="fig" rid="F2">Figure 2F</xref>). In core 973-5, high CRS contents and positive &#x3b4;<sup>34</sup>S<sub>CRS</sub> values are observed below 4&#xa0;m bsf (<xref ref-type="fig" rid="F3">Figure 3G</xref>), and the &#x3b4;<sup>34</sup>S<sub>CRS</sub> values above this depth become lighter, ranging from -46&#x2030; to -15.7&#x2030; (<xref ref-type="fig" rid="F3">Figure 3F</xref>).</p>
</sec>
</sec>
<sec sec-type="discussion" id="s4">
<title>Discussion</title>
<p>Radiocarbon- and &#x3b4;<sup>18</sup>O-derived age models (<xref ref-type="bibr" rid="B72">Zhang et al., 2018</xref>) suggested that two studied cores, 973-4 and 973-5, recorded sediment deposition since MIS3. Combined with the oxygen isotope change curve and previous research (<xref ref-type="bibr" rid="B40">Liu et al., 2018</xref>), we found that the 4.0&#x2013;9.0&#xa0;m bsf layer in core 973-4 records the sediment of MIS2, and the layer above 4.0&#xa0;m corresponds to the sediment deposited since the Holocene. Interestingly, there was an age inversion around 5.8&#xa0;m (40.35ka). The strata of MIS3 may be disturbed and MIS3 sediments have been reversed to MIS2. The age inversion intervals coincide with the foraminifera-rich and sand content-rich layers (4.4&#x2013;6.0&#xa0;m), and possibly resulted from landslides or physical disturbance by intense seepage (<xref ref-type="bibr" rid="B39">Lin et al., 2016</xref>). In core 973-5, the demarcation lines of MIS1/2 and MIS2/3 are at the depths of 2.2 and 4.8&#xa0;m bsf respectively; the age absence in 4.8&#xa0;m bsf may also have been caused by a landslide.</p>
<sec id="s4-1">
<title>Geochemical Records of Gas Hydrate Dissociation Events</title>
<p>In the typically anoxic subseafloor marine sediments, the consumption of porewater sulfate is controlled by two microbially mediated processes: 1) organo clastic sulfate reduction (OSR) (<xref ref-type="bibr" rid="B4">Berner, 1982</xref>); and 2) anaerobic oxidation of methane (AOM) (<xref ref-type="bibr" rid="B5">Boetius et al., 2000</xref>). The two net reactions are expressed stoichiometrically as follows: 2CH<sub>2</sub>O &#x2b; SO<sub>4</sub>
<sup>2-</sup>&#x2192;2HCO<sub>3</sub>
<sup>&#x2212;</sup> &#x2b; H<sub>2</sub>S 1) CH<sub>4</sub>&#x2b;SO<sub>4</sub>
<sup>2-</sup>&#x2192;HCO<sub>3</sub>
<sup>&#x2212;</sup> &#x2b; HS<sup>&#x2212;</sup> &#x2b; H<sub>2</sub>O 2) However, these two different processes always result in different average S/C ratio in sediments. In oxic and suboxic marine sediments (OSR dominate), the reduced sulfur and total organic carbon (TOC) contents typically show a positive correlation with an average S/C ratio of 0.36 (<xref ref-type="bibr" rid="B4">Berner, 1982</xref>). In our studied cores, the TOC content was typically low (<xref ref-type="bibr" rid="B72">Zhang et al., 2018</xref>), and the S/C ratios at 6.0&#x2013;9.0&#xa0;m bsf (973-4) and below 4.0&#xa0;m bsf (973-5) were higher than 0.36 (<xref ref-type="fig" rid="F4">Figure 4</xref>). These situations were referred to an organically-limited and methane-rich environment, in which AOM was the dominant process, contributed to a significant fraction of sulfides (<xref ref-type="bibr" rid="B29">Kaneko et al., 2010</xref>; <xref ref-type="bibr" rid="B38">Lim et al., 2011</xref>; <xref ref-type="bibr" rid="B54">Sato et al., 2012</xref>) and may have significantly increased the S/C ratios of sediments. This AOM origin for sulfides explains why there was no correlations between the CRS and TOC contents in the sediments of both cores (<xref ref-type="fig" rid="F5">Figure 5</xref>).</p>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption>
<p>TS/TOC ratios in the cores 973-4 and 973-5 (TS and TOC data cited from (<xref ref-type="bibr" rid="B72">Zhang et al., 2018</xref>); the blue dashed lines indicate the S/C ratio in normal marine sediment).</p>
</caption>
<graphic xlink:href="feart-10-876913-g004.tif"/>
</fig>
<fig id="F5" position="float">
<label>FIGURE 5</label>
<caption>
<p>The correlations between TOC and CRS in cores 973-4 and 973-5 (<xref ref-type="bibr" rid="B72">Zhang et al., 2018</xref>).</p>
</caption>
<graphic xlink:href="feart-10-876913-g005.tif"/>
</fig>
<p>Positive &#x3b4;<sup>34</sup>S (up to 32.6&#x2030;) values of sulfide minerals could represent a present- or paleo-SMTZ (sulfate-methane transition zone) where AOM process occurred strongly (<xref ref-type="bibr" rid="B2">Aharon and Fu, 2003</xref>; <xref ref-type="bibr" rid="B28">Jorgensen et al., 2004</xref>; <xref ref-type="bibr" rid="B7">Borowski et al., 2013</xref>; <xref ref-type="bibr" rid="B74">Zhu et al., 2013</xref>). In the studied cores, the &#x3b4;<sup>34</sup>S<sub>CRS</sub> values below 6.0&#xa0;m bsf in core 973-4 and below 4.0&#xa0;m bsf in the core 973-5 are positive. Especially in the 6.0&#x2013;9.0&#xa0;m bsf layer of core 973-4, a wide SMTZ with positive sulfur isotope compositions up to 20&#x2030; represents a sustained and stable methane flux. As shown in the <xref ref-type="fig" rid="F2">Figure 2G</xref>, at the end of the LGM period (4.0&#x2013;6.0&#xa0;m) with a low sea-level stage, the &#x3b4;<sup>34</sup>S<sub>CRS</sub> became highly negative (&#x2212;43.8&#x2030; to &#x2212;39.4&#x2030;). The low &#x3b4;<sup>34</sup>S values in seep-impacted sediments may be attributed to iron limitation caused by low sedimentation rates (<xref ref-type="bibr" rid="B21">Formolo and Lyons, 2013</xref>) or disproportionation of microbial sulfur occurring close to the sediment-water interface (<xref ref-type="bibr" rid="B9">Canfield and Thamdrup, 1994</xref>; <xref ref-type="bibr" rid="B7">Borowski et al., 2013</xref>). Because the sedimentation rate of our study area is typically high at low sea level stands (<xref ref-type="bibr" rid="B72">Zhang et al., 2018</xref>), disproportionation of microbial sulfur instead of iron limitation might be the reason for the low &#x3b4;<sup>34</sup>S<sub>CRS</sub> values. Generally, disproportionation of microbial sulfur happen in an open system, which can be caused by intense methane flux (<xref ref-type="bibr" rid="B36">Li et al., 2018</xref>). Herein, we suppose the low &#x3b4;<sup>34</sup>S values might be also caused by this phenomenon in this period.</p>
</sec>
<sec id="s4-2">
<title>Response of Specific Benthic Foraminifera to Gas Hydrate Dissociation Events</title>
<p>According to previous research, the &#x3b4;<sup>13</sup>C values of <italic>Uvigerina</italic> spp. in normal seawater range from &#x2212;0.1 to 1.0&#x2030; (<xref ref-type="bibr" rid="B52">Rathburn et al., 2003</xref>; <xref ref-type="bibr" rid="B55">Schmiedl et al., 2004</xref>; <xref ref-type="bibr" rid="B20">Fontanier et al., 2006</xref>). However, in our studied cores, the &#x3b4;<sup>13</sup>C values of benthic foraminifera below 3.9&#xa0;m bsf in core 973-4 and 2.5&#xa0;m bsf in core 973-5 (corresponding to the end of the Last Glacial period) were almost all lower than -1.0&#x2030;, showing an obvious negative carbon bias. Although some researchers considered that the &#x3b4;<sup>13</sup>C values in the Glacial period were more negative than that in Deglacial period (<xref ref-type="bibr" rid="B68">Wei et al., 2006</xref>), the &#x3b4;<sup>13</sup>C values of benthic foraminifera in the northern SCS always vary from about -0.6 to 0.2&#x2030; (range variation of approximately 0.8&#x2030; in the past 90&#xa0;ka) under the influence of climate change (<xref ref-type="bibr" rid="B68">Wei et al., 2006</xref>). These indicate that such wide range of the carbon negative bias (e.g.,1.9&#x2030; in core 973-4) in our study area was not caused by climate change and seem to be caused by AOM reaction. In addition, when recording methane seepage activity, a wide range of &#x3b4;<sup>13</sup>C values of benthic foraminifera are more appropriate than absolute negative values (<xref ref-type="bibr" rid="B52">Rathburn et al., 2003</xref>). Thus, the carbon negative bias can be attributed to methane seepage in the studied cores. Because <sup>18</sup>O is higher in cold seep fluids, and the heavier &#x3b4;<sup>18</sup>O values were thought to be another evident of gas hydrate dissociation or cold seep activity (<xref ref-type="bibr" rid="B65">Uchida et al., 2004</xref>). In core 973-4 and 973-5, the &#x3b4;<sup>18</sup>O values were obviously heavier during the Glacial period in both cores, which is consistent with the &#x3b4;<sup>13</sup>C results. Thus we can tentatively deduce the methane seepage activities in the core 973-4 by analyzing the &#x3b4;<sup>13</sup>C and &#x3b4;<sup>18</sup>O values change. <xref ref-type="fig" rid="F2">Figure 2E</xref> shows negative carbon isotope compositions in MIS2 (4.0&#x2013;9.0&#xa0;m), indicating a sustained methane seepage during this period. Furthermore, other reports have suggested that cold seeps were particularly active at low sea-level stands due to a hydrostatic pressure reduction in the SCS (<xref ref-type="bibr" rid="B64">Tong et al., 2013</xref>; <xref ref-type="bibr" rid="B23">Han et al., 2014</xref>), hence it supports our hypothesis that an intense methane seepage happened during LGM (4.0&#x2013;6.0&#xa0;m). Since the end of the LGM (above 4.0&#xa0;m), the &#x3b4;<sup>13</sup>C values in core 973-4 were quite stable and comparable to normal sea-water values typical of non-seep environments. This implies that the gas hydrate dissociation events gradually weakened in this core since the Holocene. As the temperature rose gradually in the Deglaciation periods, the changes in global ice volume and bottom water temperature were not the dominant factors for hydrate decomposition. Instead, as the sea level and the hydrostatic pressure on the sediment have gradually increased since the Last Glacial, the gas hydrate stability zone has thickened, thus causing a weakening of gas hydrate dissociation and methane seepage. <italic>Uvigerina</italic> spp. and <italic>Bulimina</italic> spp. are considered as specific endophytic benthic foraminifera that can adapt to the modern cold seep environments with high TOC and low oxygen content (<xref ref-type="bibr" rid="B1">Abu-Zied et al., 2008</xref>), and they were the two dominant species of benthic foraminifera in cores 973-4 and 973-5. Moreover, as shown in <xref ref-type="fig" rid="F2">Figures 2B,C</xref>, their numbers increased to different extents during the Last Glacial period (4.0&#x2013;9.0&#xa0;m of core 973-4), which may be under the influence of the methane flux related to the gas hydrate dissociation during that time (<xref ref-type="bibr" rid="B14">Chen et al., 2007</xref>). However, previous research indicated that normal cold seep activity cannot significantly change the total abundance of benthic foraminifera (<xref ref-type="bibr" rid="B43">Panieri et al., 2009</xref>). Therefore, the large increases in the number of benthic foraminifera at the end of the LGM period (4.0&#x2013;6.0&#xa0;m of core 973-4), especially the abrupt increase in the layer at about 6&#xa0;m bsf in core 973-4, is more likely associated with geological events rather than to large quantities of methane fluid. Sustained methane seepage can provide a rich food source for benthic foraminifera (<xref ref-type="bibr" rid="B58">Schonfeld, 2001</xref>), and <italic>Bulimina</italic> spp. can adapt well to a low oxygen and high sulfide cold seep environment, even in shallow waters (<xref ref-type="bibr" rid="B44">Panieri, 2006</xref>). The high density of this species related to methane seepage lead to another increase above the layer in which gas hydrate dissociated.</p>
</sec>
<sec id="s4-3">
<title>Triggering Mechanism for the Submarine Landslides in the Dongsha Area</title>
<p>Gravity flows such as submarine landslides and turbidity currents are ubiquitous in Dongsha area (<xref ref-type="bibr" rid="B37">Li et al., 2020</xref>). And these gravity flows are proved to be able to drive erosion and deposition in Taiwan submarine canyons. As shown on the bathymetric and seismic profiles close to the research areas. Recurrent MTDs are identified in the slope, which indicate Dongsha slope might be eroded by slope failures. And <xref ref-type="bibr" rid="B37">Li et al. (2020)</xref> concluded that a combined action of recurrent slope instability and turbidity currents drive the erosion and deposition of submarine asymmetry in our studying area. But from the C-M plot (<xref ref-type="fig" rid="F6">Figure 6</xref>) (<xref ref-type="bibr" rid="B46">Passega, 1964</xref>), a common method to identify the force of deposition using the sediment size. The grain size distribution in the 4.4&#x2013;6.0&#xa0;m bsf layer in core 973-4 is not parallel to the RQ line in the, which indicated that sedimentation was not impacted by turbidity currents. Thus we contribute the gravity flows recorded in our sediment cores to submarine landslides.</p>
<fig id="F6" position="float">
<label>FIGURE 6</label>
<caption>
<p>The seismic profile of the D2 survey line (from Li, 2020, left) and Passega C-M diagram (Passega, 1964, right). C &#x3d; maximum (D99; first percentile) grain size of 973-4, M &#x3d; median grain size. The dots represent the interval (4&#x2013;6 m) with coarser grain content. <bold>(A)</bold> Two-dimensional (2D) seismic profile of the Taiwan Canyon highlighting the morphological differences in canyon banks. <bold>(B)</bold> The mass transport deposits (MTDs) are characterized by chaotic amplitude reflections. <bold>(C)</bold> Line drawn interpretation of <bold>(B)</bold> illustrating the presence of widespread MTDs in the north-east of Taiwan Canyon.</p>
</caption>
<graphic xlink:href="feart-10-876913-g006.tif"/>
</fig>
<p>The sediment particle size results in the three cores, 973-3 (<xref ref-type="bibr" rid="B15">Chen et al., 2014</xref>), 973-4 and 973-5, which were located at the top, middle and bottom of the Dongsha area continental slope, were comprehensively investigated. The submarine landslides in this study area mainly developed at the top of the continental slope, with lower intensity in the middle slope, and only landslide deposits were present at the bottom of the slope. Furthermore, the age reversal interval (<xref ref-type="fig" rid="F2">Figure 2</xref>) coincided with the high foraminifera and sand content in layer 4.4&#x2013;6.0&#xa0;m bsf in core 973-4, which is consistent with frequent submarine landslides influencing this area (<xref ref-type="bibr" rid="B73">Zhong et al., 2015</xref>; <xref ref-type="bibr" rid="B39">Lin et al., 2016</xref>; <xref ref-type="bibr" rid="B69">Wu et al., 2018</xref>).</p>
<p>Based on a comprehensive analysis of geochemical and sediment records, gas hydrate dissociation events and submarine landslides were recognized in two cores. We take 973-4 for analyzing (<xref ref-type="fig" rid="F7">Figure 7</xref>). There was sustained and stable methane seepage during the beginning of MIS2 (6.0&#x2013;9.0&#xa0;m, <xref ref-type="fig" rid="F7">Figure 7A</xref>) and the methane flux was relatively low. Therefore, iron sulfides with high &#x3b4;<sup>34</sup>S<sub>CRS</sub> and benthic foraminifera with negative &#x3b4;<sup>13</sup>C were found in the sediment layer (<xref ref-type="fig" rid="F7">Figure 7A</xref>). At the end of MIS2, responding to the LGM period (4.0&#x2013;6.0&#xa0;m), the methane flux was very high and the SMTZ was near the seafloor (<xref ref-type="fig" rid="F7">Figure 7B</xref>). In this case, the enrichment of TOC might be due to the lower rates of AOM and higher methane flux into the water column (<xref ref-type="bibr" rid="B17">Consolaro et al., 2015</xref>). More importantly, the massive decomposition of gas hydrate during the low-stand sea level period reduced slope stability (<xref ref-type="bibr" rid="B63">Sultan et al., 2010</xref>; <xref ref-type="bibr" rid="B32">Kwon et al., 2011</xref>), and herein led to the formation of the submarine landslides and sediment transportation from the top to the flat area of the slope (<xref ref-type="fig" rid="F7">Figure 7B</xref>). The abrupt increase in benthic foraminifera quantity also verify this geological activity. Because methane diffused into the atmosphere before it had completely reacted, the &#x3b4;<sup>34</sup>S<sub>CRS</sub> values of iron sulfides were low but the &#x3b4;<sup>13</sup>C values of benthic foraminifera showed negative anomalies (<xref ref-type="fig" rid="F7">Figure 7B</xref>). Since the Last Glacial period (above 4.0&#xa0;m), rising sea level has prevented the decomposition of gas hydrates and gradually weakened cold seep activity. Thus, the geochemical and benthic foraminifera records showed no further anomalies (<xref ref-type="fig" rid="F7">Figure 7C</xref>).</p>
<fig id="F7" position="float">
<label>FIGURE 7</label>
<caption>
<p>Relationship between gas hydrate decomposition and submarine landslides (SWI: sea water interface).</p>
</caption>
<graphic xlink:href="feart-10-876913-g007.tif"/>
</fig>
</sec>
</sec>
<sec sec-type="conclusion" id="s5">
<title>Conclusion</title>
<p>Two sediment cores from the Dongsha slope in the SCS were used to identify gas hydrate dissociation events and subsequently the potential trigger of submarine landslides. The distinctly negative &#x3b4;<sup>13</sup>C values and positive &#x3b4;<sup>18</sup>O values along with extremely positive &#x3b4;<sup>34</sup>S<sub>CRS</sub> values in both cores at the end of the LGM period suggested that there were persistent gas hydrate dissociation events in the Dongsha area during this period. In core 973-4, obvious submarine landslide deposits only occurred at the 4.4&#x2013;6.0&#xa0;m interval (end of LGM), and the numbers of <italic>Uvigerina</italic> spp. and <italic>Bulimina</italic> spp. sharply increased in this horizon. These results implied that the submarine landslides were probably caused by intense methane release events during this period. More importantly, as shown here, a novel strategy with geochemical methods were used to investigate the relationship between submarine landslides and gas hydrate dissociation events. Further studies of numerical methods are needed to quantitatively illustrate the casual relationship between them.</p>
</sec>
</body>
<back>
<sec id="s6">
<title>Data Availability Statement</title>
<p>The raw data supporting the conclusion of this article will be made available by the authors, without undue reservation.</p>
</sec>
<sec id="s7">
<title>Author Contributions</title>
<p>Formal analysis and writing&#x2014;original draft preparation, YH; writing&#x2014;review and editing, JC, MW, SW, and WY; All authors have read and agreed to the published version of the manuscript.</p>
</sec>
<sec id="s8">
<title>Funding</title>
<p>Our work is supported by Key Special Project for Introduced Talents Team of Southern Marine Science and Engineering Guangdong Laboratory (Guangzhou) (GML2019ZD0104), the Innovation Development Fund of South China Sea Eco-Environmental Engineering Innovation Institute of the Chinese Academy of Sciences (ISEE2018PY02), the National Natural Science Foundation of China (41576035).</p>
</sec>
<sec sec-type="COI-statement" id="s9">
<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>
<sec sec-type="disclaimer" id="s10">
<title>Publisher&#x2019;s Note</title>
<p>All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.</p>
</sec>
<ack>
<p>We would like to thank all the crew members of the R/V Ocean VI of the 2011 Guangzhou Marine Geological Survey cruise. We acknowledge Dr. Peng for measuring sulfur isotopic compositions.</p>
</ack>
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