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Early Triassic paleogeography (ca. 250 Ma) of (A) the world (adapted from Ron Blakey, http://jan.ucc.nau.edu/∼rcb7/) and (B) the South China craton (Yin et al., 2014). Red rectangle in A shows location of inset map B. Black triangles (outlined in white) in B represent present study sections (SS-Shangsi; GX-Ganxi; CH-Chaohu). Number of ash beds from conodont Clarkina changxingensis to Isarcicella isarcica zones is shown by red (8), yellow (5-7), purple (3-4), black (1-2), and open (0) symbols (note: Site numbers are given in the Supplemental Material [see footnote 1]). In panel A, red numbers represent previous mercury studies, as shown in Figure 2, including 43 (Zal; Sial et al., 2020), 66 (Buchanan Lake [BL]; Sanei et al., 2012), 67 (Festningen [F]; Grasby et al., 2015), and 70 (Gujo-Hachiman [GH]; Shen et al., 2019a). C-Cathaysia Oldland; K-Kangdian uplift; PTO-Paleo-Tethys Ocean; NTO-Neo-Tethys Ocean; NPJ-Nanpanjiang.

Early Triassic paleogeography (ca. 250 Ma) of (A) the world (adapted from Ron Blakey, http://jan.ucc.nau.edu/∼rcb7/) and (B) the South China craton (Yin et al., 2014). Red rectangle in A shows location of inset map B. Black triangles (outlined in white) in B represent present study sections (SS-Shangsi; GX-Ganxi; CH-Chaohu). Number of ash beds from conodont Clarkina changxingensis to Isarcicella isarcica zones is shown by red (8), yellow (5-7), purple (3-4), black (1-2), and open (0) symbols (note: Site numbers are given in the Supplemental Material [see footnote 1]). In panel A, red numbers represent previous mercury studies, as shown in Figure 2, including 43 (Zal; Sial et al., 2020), 66 (Buchanan Lake [BL]; Sanei et al., 2012), 67 (Festningen [F]; Grasby et al., 2015), and 70 (Gujo-Hachiman [GH]; Shen et al., 2019a). C-Cathaysia Oldland; K-Kangdian uplift; PTO-Paleo-Tethys Ocean; NTO-Neo-Tethys Ocean; NPJ-Nanpanjiang.

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Enhanced regional subduction-related volcanism in the South China craton concurrent with Siberian Traps large igneous province magmatism was a likely contributor to major biotic and environmental stresses associated with the Permian-Triassic boundary (ca. 252 Ma) mass extinction. However, the timing, intensity, and duration of this regional volcani...

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... the Permian-Triassic transition, the South China craton was a small (∼3 × 10 6 km 2 ) near-equatorial microcontinent in the eastern part of the Paleo-Tethys Ocean (Fig. 1A). The three study sections were located on its northwestern margin (an upwelling zone; Fig. 1B) and represent shallow shelf (Ganxi) to deep shelf/ basin (Shangsi and Chaohu) environments. The study sections accumulated sediment throughout the PTB transition despite a eustatic regression at the end of the Permian (e.g., as recorded by ...
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... the Permian-Triassic transition, the South China craton was a small (∼3 × 10 6 km 2 ) near-equatorial microcontinent in the eastern part of the Paleo-Tethys Ocean (Fig. 1A). The three study sections were located on its northwestern margin (an upwelling zone; Fig. 1B) and represent shallow shelf (Ganxi) to deep shelf/ basin (Shangsi and Chaohu) environments. The study sections accumulated sediment throughout the PTB transition despite a eustatic regression at the end of the Permian (e.g., as recorded by absence of the conodont Clarkina meishanensis zone in shallow-water sections; Yin et al., 2014). ...
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... and (3) similar patterns of Hg/ TOC variation were observed in all three study sections, despite differences in environmental setting (i.e., Ganxi = shallow shelf, Shangsi and Chaohu = deep shelf/basin) and geographic location (>1000 km separation). These considerations support a regional control on Hg inputs to the sediment during ME1 to ME3 (Fig. ...
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... First, these events are not documented in any section outside of the Tethys region (Fig. 2). Second, the Upper Permian across the South China craton contains many ash beds, demonstrating frequent volcanic activity at a regional scale ( Yin et al., 1992). These ash beds increase in number and thickness to the south and southwest (paleocoordinates; Fig. 1; Yin et al., 1992), favoring a subduction-zone volcanic arc along the South China craton-Indochina plate boundary as their source. Third, the chemical compositions (i.e., trace elements and hafnium isotopes) of syndepositional magmatic zircons from these ash beds demonstrate a felsic to intermediate source, consistent with ...
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... hafnium isotopes) of syndepositional magmatic zircons from these ash beds demonstrate a felsic to intermediate source, consistent with subduction-zone rather than flood-basalt volcanism ( Gao et al., 2013;He et al., 2014). Regional volcanism may have also contributed Hg to ME4, although this spike is found in almost all PTB sections globally ( Fig. 2; Shen et al., 2019a), demonstrating that it was not primarily related to plate-margin volcanism in the PaleoTethys region. Rather, ME4 records the second stage of STLIP eruptions, which has been linked to combustion of organic-rich sediments in the West Siberian Coal Field (Burgess et al., 2017), ...
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... volcanism may have also contributed Hg to ME4, although this spike is found in almost all PTB sections globally ( Fig. 2; Shen et al., 2019a), demonstrating that it was not primarily related to plate-margin volcanism in the PaleoTethys region. Rather, ME4 records the second stage of STLIP eruptions, which has been linked to combustion of organic-rich sediments in the West Siberian Coal Field (Burgess et al., 2017), ...

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... Latitudinal diachroneity of the terrestrial EPME Previous work has shown that the marine ecosystem collapse was brief and globally synchronous and was embedded in a long-term interval of global environmental degradation. The onset of the main marine extinction has been constrained to the Clarkina meishanensis and equivalent conodont zones (40)(41)(42)(43), which was calibrated to 251.945 ± 0.033 Ma ago at the Meishan GSSP (3) (table S4), 251.984 ± 0.031 (44) or 251.939 ± 0.031 Ma ago (4) at the extended Penglaitan section, and 251.939 ± 0.031 Ma ago at the Dongpan section (44) in South China. ...
... The emplacement of the SLIP has been the most widely hypothesized trigger of the terrestrial and marine EPME since the early 1990s due to their temporal coincidence (3,5). However, sediments related to felsic volcanism developed extensively along the convergent margins of southern Pangea and around the Tethyan Ocean during the Permian-Triassic transition (21,43,(75)(76)(77) (Fig. 1), introducing another possible stressor for the EPME. Mercury spikes during this interval have been reported globally and are thought to be derived from the SLIP (6), but they are not correlative between different sections based on the high-resolution geochronologic framework presented here, which could be generated from different stages of the SLIP or affected by local sedimentological processes (Fig. 5). ...
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... Given the common use of Hg as a proxy for volcanism within Mesozoic sediments (Sanei et al., 2012;Sial et al., 2013;Thibodeau et al., 2016;Grasby et al., 2019;Keller et al., 2020;Shen et al., 2020a), it has been heavily used as a tool to understand the triggering mechanism for the perturbation in the carbon cycle during the TOAE (Percival et al., 2015;Fantasia et al., 2018aFantasia et al., , 2019Font et al., 2022). The KF-LIP is commonly invoked as the primary source of Hg and trigger for the onset of the TOAE ). ...
... Based on this Δ 199 Hg trend, they interpreted their Griesbachian Hg/TOC excursion as having resulted from terrestrial Hg input due to elevated Early Triassic continental weathering. Recently, J. Shen et al. (2021) reported several Hg enrichment intervals predating the PTBME (named ME1-ME3), as well as one interval coeval with the PTBME (ME4), from three marine sections in South China. These authors reported the same pattern of decreasing Δ 199 Hg values from the Changhsingian to Griesbachian. ...
... Owing to the paucity of U-Pb zircon ages for deep-water sections from which Hg anomalies have been reported in South China, it is difficult to confidently correlate our recorded Hg anomalies with those reported for other localities in the Tethys region. However, the E1 anomaly recorded from the studied successions together with ME2 and ME3 episodes of J. Shen et al. (2021), indicate that Hg anomalies preceding the PTB extinction are recorded in both shallow and deep-marine settings in South China. In contrast, the E2 Griesbachian Hg anomaly is not recorded from any shallow-water marine section nor deep-water sections in South China, except for deep-water sections in the Nanpanjiang Basin (e.g., Xinmin, Kejiao; Figure 9). ...
... This is evident from the older and well-known Emeishan LIP , the occurrence of P-T volcanic rocks especially in southwest South China (Gao et al., 2013), the abundant volcanic ash layers within P-T marine sedimentary successions, shown to be genetically distinct from STLIP rocks (Gao et al., 2013;He et al., 2014;Yang et al., 2012), as well as Changhsingian Hg/TOC anomalies restricted to the Tethys region (J. Shen et al., 2021;this study). In addition, regional arc volcanism has been linked to notably decreased carbonate and biogenic silica production, as well as decreased water column oxygenation in South China (J. ...
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... Our results suggest that several different types of regional volcanic activities could have been responsible for the basal middle Tournaisian biotic turnover. In recent years, many authors emphasized the influence of enhanced regional subduction-related arc-volcanism as a potential trigger of biotic crises during the end-Ordovician (Yang et al., 2019), Frasnian-Famennian (Racki et al., 2018b;Racki, 2020;Zhao et al., 2022a), end-Devonian (Kalvoda et al., 2019;Rakociński et al., 2021b), and end-Permian (Shen et al., 2021). However, to better constrain the influence of volcanic activity during the LASE, additional Hg isotopic data are needed. ...
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... Previous studies often assumed the enhanced Hg enrichment and the negative shift of Δ 199 Hg were synchronous across the EPME and interpreted them as the result of increased atmospheric Hg deposition from volcanic emission, and/or of massive terrestrial Hg input to oceans from biomass burning and soil erosion, which are often also linked to volcanism [24][25][26][29][30][31][32][33] . Such interpretations follow because mantle-sourced volcanic Hg typically has circum-zero Δ 199 Hg values 34,35 , and modern terrestrial vegetation and soil typically have negative Δ 199 Hg values 23 , both of which are lower than background values of pre-EPME marine sediments (0.1-0.2‰) (Supplementary Table 1). ...
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... Mercury is hosted in sediments in multiple phases, including organic matter, sulfides, and clay minerals Shen et al., 2020). Recent studies suggest that anomalously high Hg to total organic carbon (Hg/TOC) ratios can be a useful proxy for tracing large volcanism in geological history Shen et al., 2020), although studies also suggest that the depositional environments may play a critical role in Hg accumulation in sediments rather than input sources (Shen et al., 2022;Xue et al., 2022). Besides, caution must be paid to weathered rocks because Hg may be lost during silicate weathering (Charbonnier et al., 2020;Park et al., 2022). ...
... Possible host phases of Hg in sediments include organic matter, sulfides, and clay minerals (Krupp, 1988;Grasby et al., 2019;Shen et al., 2019Shen et al., , 2020. Mercury has a strong affinity to the organic matter in normal sediments Shen et al., 2020), however recent studies have suggested that sulfides (e.g., pyrite) can be another important host of Hg in sulfidic water conditions (Shen et al., 2019(Shen et al., , 2022. ...
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... Mercury contents and isotope ratios in sediments have been widely used to trace and evaluate the record of volcanism in geological history, and to determine Hg source(s) and evaluate Hg's transport mechanisms in the Earth system (e.g., Sanei et al., 2012;Grasby et al., 2019;Shen et al., 2020a;Percival et al., 2021;Yager et al., 2021;Shen et al., 2022a). Volcanism and wildfires are the main causes of abnormal mercury enrichment anomalies in strata (Shen et al., 2020a(Shen et al., , 2020bShen et al., 2022). Volcanism can not only release Hg directly into the atmosphere, but can also lead to abnormal Hg accumulation in sediments through magma heating of organic-rich sediments (e.g., Shen et al., 2020b;Shen et al., 2022). ...
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... McKenzie et al. 2016;Lu et al. 2021) and other biotic crises, such as the Ordovician-Silurian(Yang et al. 2019), end-Frasnian(Racki, 2020), end-Devonian(Rakociński et al. 2021b) and end-Permian(Shen et al. 2021). ...
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