- 1School of Resources and Earth Sciences, China University of Mining and Technology, Xuzhou, Jiangsu, China
- 2School of Management, Xi’an University of Science and Technology, Xi’an, Shaanxi, China
- 3Xuzhou Datun Engineering Consulting Co., Ltd., Xuzhou, Jiangsu, China
- 4Yunnan Vocational Institute of Energy Technology, Qujing, Yunnan, China
Parallel positive excursions of organic carbon (δ13Corg) and pyrite sulfur (δ34Spy) isotopes occurred globally during the Hirnantian glacial period. However, the reasons for these isotope excursions and their relationship with paleoenvironmental dynamics are not fully understood. This study presents a high-resolution geochemical investigation of the Tianlin section of the Upper Yangtze Basin, South China. The total organic carbon (TOC), iron speciation, trace elements, δ13Corg, and δ34Spy were analyzed and compared with published results from the other four sections in the same basin. A negative relationship was observed for the sulfate reduction index (SRI) with TOC and organic carbon accumulation rate. This suggests that the abundance of sedimentary organic matter was not the main factor inhibiting microbial sulfate reduction (MSR). The significant positive correlations of SRI with pyrite and δ34Spy showed that MSR promoted the formation of pyrite and that the availability of sulfate was the main limiting factor for the δ34Spy change. The negative excursions of δ13Corg and δ34Spy during the pre-glacial and post-glacial periods were coupled with dense segments of bentonite, indicating that volcanism was the main driving force for the negative excursions of C and S isotopes. Moreover, the sulfate input of rivers, restored at the post-glacial period, was the main reason for the continued negative excursion of S isotopes. Our results emphasize the key role of MSR and volcanic activity in C and S isotope excursions and their corresponding environmental changes in semi-restricted basins during the Hirnantian glaciation.
1 Introduction
The Hirnantian Stage (Late Ordovician to Early Silurian, O-S, 445.6–443.7 Ma), was one of the three period in Earth’s history with continental glaciers distributed globally (Tumer et al., 2005). With the expansion and dissipation of glaciation, this period also witnessed the first Paleozoic biotic extinction and recovery (Sutcliffe et al., 2000; Sheehan, 2001). At this stage, substantial evidence regarding significant changes in climate and ice cover formation has been found; these changes include the positive excursion of the carbon isotope (δ13C); sea-level fall; the emergence of glacial sedimentary cycles in the Katian Stage; the deposition of carbonate rocks containing flint and phosphate; and an increased global marine δ18O value (Hambrey, 1985; Kump and Arthur, 1999; Pope and Steffen, 2003; Trotter et al., 2008; Kiipli et al., 2010; Munnecke et al., 2010; Finnegan et al., 2011; Elrick et al., 2013; Yang et al., 2021). Because carbon and sulfur isotopes are closely tied to environmental change and biological innovation, disturbances in these isotopes, as they relate to the complex changes that characterized the Hirnantian Stage, have been studied extensively (Brenchley et al., 2003; Jones and Fike, 2013; Wang et al., 2021a; Zhang et al., 2021a; Li Y et al., 2021).
Numerous studies have highlighted positive excursions in both organic (δ13Corg) and carbonate carbon (δ13Ccarb) during the Hirnantian Stage (e.g., Brenchley et al., 2003; Fan et al., 2009; Zhang et al., 2009; Jones and Fike, 2013). This phenomenon is often explained via two mainstream views. According to the first explanation, before Hirnantian glaciation, the burial of large amounts of organic carbon (i.e., due to high productivity) resulted in the positive deviation of carbon isotope (Qing and Veizer, 1994; Brenchley et al., 2003). The extensive burial of organic carbon that characterizes this period is thought to have also caused a significant decrease in the atmospheric CO2, culminating in glaciation (Gibbs et al., 1997; Herrmann et al., 2004; Lv et al., 2022). The other explanation is centered on the idea that the input of terrigenous debris (i.e., via carbonate weathering) rich in carbon isotopes, during the glacial periods, promoted the increase of δ13C in sediments (Kump and Arthur, 1999 (Jones et al., 2011). Additionally, synchronized positive excursions of pyrite sulfur isotopes (δ34Spy) have also been observed in the Hirnantian Stage (Yan et al., 2009a; Zhang et al., 2009; Hammarlund et al., 2012). Interpretations of the positive excursions of δ34Spy can be summarized by two mechanisms. First, the burial mechanism points to the possibility that strong microbial sulfate reduction (MSR), under anoxic conditions, resulted in the consumption of sulfate in the water column. The pyrite generated during this process was then buried in large quantities, resulting in a gradual increase in δ34Spy (Zhang et al., 2009; Gill et al., 2011). The other mechanism suggests that the input of Hirnantian oxygen-containing water forced the chemocline into the sediments, limiting the supply of sulfate in the pore water, and then generating 34S-rich pyrite (Yan et al., 2009a; Jones and Fike, 2013). It is apparent that explanations behind the changes in the carbon and sulfur cycles in the Hirnantian Stage are complex, and that more information is needed to comprehensively characterize their relationship.
Data from different profiles have confirmed the occurrence of carbon and sulfur disturbances in the Upper Yangtze Basin during the O-S period, and the effects of the resultant environmental changes. These data also brought forth insights tried to sulfate availability and volcanic activity during this period (Yan et al., 2009b; Zhang et al., 2009; Gorjan et al., 2012; Li et al., 2017a; Li et al., 2019; Li N et al., 2021; Xi et al., 2021). However, a fine-scale study on the effect of MSR on carbon and sulfur cycles has not been conducted to data, and the dynamic mechanism of δ13Corg and δ34Spy negative excursions and their long-term maintenance after a glacial period have not been explained clearly.
In this study, detailed analyses of δ13Corg and δ34Spy were conducted to determine their prevalence during the O-S period. Combined with iron speciation and trace element analysis, mechanisms driving δ13Corg and δ34Spy changes were discussed and analyzed through the lens of MSR and volcanic activity, providing new insights into carbon and sulfur cycles during the Hirnantian Stage.
2 Geological background
The Upper Yangtze Basin, located in the central part of the Yangtze Plate, was dominated by carbonate deposits in the Early Ordovician and covered by vast epeiric seas (Figure 1A). In the Late Ordovician, influenced by the Kwangsian Orogeny, the Yangtze Plate was subjected to the subduction and compression of the Cathaysian plate in the southeast, and gradually surrounded by several paleo-continents and uplifts (Zhou et al., 2015). At this time, the Qianzhong uplift in the south was connected to the Xuefeng uplift, and the Kangdian paleocontinent and Chuanzhong uplift in the west continued to expand, inducing a low-energy, compensational stacking of sediment within the plate (Figure 1B). Petrographically, carbonate rocks have been replaced by terrigenous clastic deposits–from the Baota Formation and Linxiang Formation limestone to the O-S Wufeng-Longmaxi (WF-LMX) Formation black shale deposits (Chen et al., 2004).
FIGURE 1. Paleogeographic context and geological setting of the Tianlin section. (A) Global paleogeography for the Late Ordovician (∼445 Ma) (Zhou et al., 2015). (B) Paleogeography of the Upper Yangtze Basin from the Late Ordovician to Early Silurian (modified from Liu et al., 2016) (C) Biostratigraphy and bentonite distribution for the Tianlin section (graptolite biozones based on Chen et al. (2004). GYQ, Guanyinqiao Formation; HF, Hirnantia Fauna).
The Tianlin section (27°55′15″N, 105°36′45″E) is in the southern sedimentary center of the Upper Yangtze Basin (Figure 1B). This section reveals complete strata containing the entire Ordovician–Silurian boundary. From bottom to top, it is composed of carbonaceous and siliceous black shale from the WF Formation of the Katian stage, argillaceous limestone from the Guanyinqiao (GYQ) Formation of the Hirnantian Stage, and black silty shale from the LMX Formation of the Rhuddanian Stage (Figure 1C). The graptolite biostratigraphy of the Yangtze Basin is well established (Chen et al., 2000; Chen et al., 2004). In the Tianlin section, five graptolite biozones and their estimated yielding durations have been identified from bottom to top, i.e., D. complexus ∼ 0.6 Myr, P. pacificus ∼ 1.86 Myr, M. extraordinarius ∼ 0.73 Myr, M. persculptus ∼ 0.6 Myr, and A. ascensus ∼ 0.43 Myr zones (Chen et al., 2004; Cooper et al., 2012).
3 Samples and methods
3.1 Samples
To circumvent the influence of surface weathering, 23 representative fresh shale samples were collected from the Tianlin section via drilling. A BC-20S portable drilling rig was used for sampling. The diameter of the borehole was 36 mm and the depth was 0.15 m. All samples were ground to ≤200 mesh size using an agate mortar, and then δ13Corg, δ34Spy, and the major and trace elements were evaluated.
3.2 Methods
First, each powder sample (2 g) was placed in a 5 ml centrifuge tube. Then, 5 ml HCl, with a concentration of 4 mol/L, was added to the tube and then shaken. The powder was allowed to dissolve in the HCl for 12 h; its dissolution was considered complete when there was the formation of bubbles stopped. This step was conducted to remove carbonate from the samples. The treated samples were then repeatedly washed and centrifuged with deionized water until the pH of the supernatant reached 7. Once the pH was neutral, the samples were dried thoroughly. Total organic matter (TOC) and total sulfur (TS) were then determined using the LECO CS-200 carbon-sulfur analyzer. δ13Corg was determined using an isotope ratio mass spectrometer (MAT-253). The organic carbon isotope composition was calibrated using USG (δ13C = −23.39‰) and UREA (δ13C = −37.32‰), and the analysis results were uniformly expressed as δ13C relative to the Vienna Pee Dee Belemnite (VPDB). δ34S was determined via the chromium reduction method (Canfield and Farquhar, 1986), and the sulfur isotope of the generated sulfide was analyzed using by Thermo Fisher Scientific Delta V Plus mass spectrometer and Costech ECS 4010 elemental analyzer. The sulfur isotope composition was calibrated using IAEA-S1 (−3.0‰), IAEA-S2 (22.65‰), and IAEA-S3 (−32.5‰), and the analysis results were uniformly expressed as δ34S relative to the Vienna-Canyon Diablo Troilite (V-CDT). The accuracy of carbon and sulfur isotope analyses was 0.2‰. All experimental tests were conducted at the State Key Laboratory of Biogeology and Environmental Geology, China.
Major and trace elements were tested at the Jiangsu Geological and Mineral Resources Design and Research Institute using the Bruker S8 Tiger X-ray fluorescence spectrometer (XRF) and the PE Elan600 standard inductively coupled plasma mass spectrometer (ICP-MS), respectively. The specific steps and standards involved in this step can be found in a previous study (Wang et al., 2021a; Zhang et al., 2021b).
The content of mercury (Hg) was determined using the DMA-80 automatic mercury analyzer at the School of Resources and Earth Sciences, China University of Mining and Technology. Specifically, 100 mg dried shale powder samples were weighed and put into a cracking furnace. Mercury vapor was released under the action of a high temperature catalyst, and the carrier gas was moved into an optical cell for determination at a wavelength of 253.7 nm.
Additionally, we used the organic carbon accumulation rate (OCAR) to evaluate the characters of primary productivity (Schoepfer et al., 2015). The following formula was used OCAR = TOC × LSR × ρ, where ρ = 2.5g/cm−3, represents the density of bulk rock (Shen et al., 2015). LSR is the linear sedimentation rate.
4 Results
All geochemical data, δ13Corg, and δ34Spy results of the Tianlin section are presented in Table 1 and Figure 2. The test data for the Shuanghe section, YY1 well, Wangjiawan section and Nanbazi section can be found in previous studies (Yan et al., 2009b, 2012; Liu et al., 2016; Li et al., 2017b; Li Y et al., 2021).
FIGURE 2. Chemo-stratigraphic profiles of (A) TOC and OCAR, (B) FeT and TS, (C) FeHR/FeT and Fepy/FeHR, (D) MoEF and UEF, (E) δ13Corg and δ34Spy, and a redox summary for the Tianlin section. Vertical dotted lines represent the threshold for each proxy.
4.1 TOC content and organic carbon isotope
Results of the TOC content for the Tianlin section ranged from 0.59 to 7.17% (average=3.01%). For the WF Formation (including the Late Katian stage and Early Hirnantian Stage), the TOC content ranged from 0.79 to 4.99% (average = 2.85%). In the GYQ Formation, it ranged from 0.59 to 1.54% (average = 1.18%). Comparatively, for the LMX Formation, the TOC value increased sharply from 3.11 to 7.17% (average = 4.60%) (Table 1 and Figure 2A). The distribution of OCAR showed a trend similar to that of TOC (Figure 2A). From the Late Katian Stage to Early Rhuddanian Stage, OCAR first decreased and then increased.
Results of the δ13Corg for the Tianlin section ranged from −30.8‰ to −29.6‰ (average = −30.3‰). From the WF Formation to GYQ Formation, and then to the LMX Formation, the δ13Corg values first increased from −30.41‰ to −29.73‰, and then decreased to −30.48‰ (Table 1 and Figure 2E). Although the values of δ13Corg were generally low in organic-rich layers and high in organic-poor layers, there was no significant correlation between TOC and δ13Corg (Figure 3A), suggesting that the δ13Corg was less affected by the original productivity of OM, and recorded important information about the global carbon reservoir changes during the O-S period (Kump and Arthur, 1999).
FIGURE 3. Crossplots of TOC vs. (A) δ13Corg and (B) Fepy, crossplots of (C) δ13Corg and (D) Fepy vs. δ34Spy. All fitting curves are linear.
4.2 TS content and pyrite sulfur isotope
Results of the TS content for the Tianlin section ranged from 0.03 to 2.16% (average = 1.20%) (Figure 2B). Additionally, there was a significant positive correlation between Fepy and TOC (r = 0.67, p < 0.01, n = 23) (Figure 3B), indicating that the abundance of organic matter (OM) could be a factor that controlled the formation of pyrite.
δ34Spy varied across a large range, from −9.60 to 11.7‰ (average = −1.38‰) (Figure 2E). The change in δ34Spy was similar to that in δ13Corg, with the highest value observed for the Hirnantian Stage, particularly in the GYQ Formation (11.7‰ for sample TL-18; Table 1 and Figure 3C). Additionally, there was a negative correlation between δ34Spy and Fepy (r = −0.48, p < 0.05, Figure 3D), indicating that the availability of sulfate may control pyrite formation (Li et al., 2019).
4.3 Major and trace element contents
Iron speciation and its proportional relationship have been widely used to determine the redox conditions of paleowater columns (Poulton and Canfield, 2011; Li et al., 2015). The FeT values of all samples were >0.5% (ranging from 1.37 to 3.58%, average = 2.22%; Table 1 and Figure 2B). FeHR/FeT and Fepy/FeHR showed similar trends from the WF Formation to GYQ Formation, and then to the LMX Formation; these trends are characterized by an initial decrease followed by an increased (Figure 2C). Particularly, the FeHR/FeT and Fepy/FeHR values of the GYQ Formation samples were the lowest, at 0.25 and 0.44 (average values), respectively (Table 1).
Results of the Al content for the Tianlin section ranged from 3.81 to 8.17% (average = 5.75%) (Table 1). Hg concentrations in the samples ranged from 41.6 to 210.4 ppb (average = 108.8 ppb) (Table 1). The highest average content was 166.8 ppb, at the late Katian Stage, whereas the lowest value was 55.5 ppb, at the Hirnantian Stage. The MoEF and UEF contents showed similar trends to that of iron speciation (Figure 2D), which first decreased and then increased. In this study, UEF and MoEF were calculated using the following equation XEF = (X/Al) sample/(X/Al)PAAS, where PAAS represents the values of corresponding elements for post Archean average shale (Taylor and McClcnnan, 1985). Additionally, the MoEF and UEF values of the GYQ Formation samples reached lowest average values of 18.33 and 8.20, respectively (Table 1).
5 Discussion
The variation in δ13Corg and δ34Spy values in the Tianlin section of the Yangtze Basin from the late Katian to early Rhuddanian stages was consistent with that of the other four sections in the same basin (Figure 4); additionally, it was also consistent with the data for other basins (e.g., Scotland and Denmark) (Kump and Arthur, 1999; Hammarlund et al., 2012). Both isotopes showed positive excursions during the late Hirnantian Stage (i.e., GYQ Formation), further showing that this is a global phenomenon. To further constrain the evolution of carbon and sulfur during the Hirnantian glaciation period, graptolite biostratigraphy was used to discuss the duration and control mechanism of δ13Corg and δ34Spy excursions.
FIGURE 4. Stratigraphic correlation ofδ13Corg and δ34Spy sections during the O-S period. Data of the Shuanghe section, YY1 well, Nanbazi section, and Wangjiawan section can be found in previous studies (Yan et al., 2009b, 2012; Liu et al., 2016; Li et al., 2017a; Li N et al., 2021; Li Y et al., 2021).
5.1 Water restriction and redox conditions
5.1.1 Water restriction
The enrichment of sedimentary OM and biogeochemical cycles of elements are controlled by the degree of water restriction (Rowe et al., 2008; Algeo and Rowe, 2012). Geochemical characteristics and the enrichment of Mo and U are often used to determine the degree of water restriction (Algeo and Tribovillard, 2009; Wang et al., 2021a). Specifically, Mo and U show different adsorption rates and degrees of enrichment in restricted and non-restricted water columns under suboxic-to-anoxic conditions, and the covariant relationship between UEF and MoEF is often used to determine the degree of water restriction (Tribovillard et al., 2012).
In the Tianlin section, from the Late Katian to Early Hirnantian stage (i.e., M. extraordinarius), the contents of U and Mo in the samples showed a gradually increase, increasing the value of UEF-MoEF from 0.1×SW to 1×SW (SW, represents sea water; the value of 1×SW is 7.9), but remained less than 1×SW, representing a restricted environment (Tribovillard et al., 2012) (Figure 5A). From the Hirnantian to early Rhuddanian stages, the contents of U and Mo first decreased and then increased, but the value of UEF-MoEF was close to 1×SW, representing a semi-restricted environment (Figure 5A). Combining these results with the YY1 well and Shuanghe section, it is clear that the Upper Yangtze Basin was always in a semi-restricted state during the O-S period (Figure 5B).
FIGURE 5. Covariant relationship between UEF and MoEF for the (A)Tianlin section and (B) Tianlin, YY1 well and Shuanghe sections. The solid line represents the molar concentration ratio of Mo/U in seawater (SW=7.9).
5.1.2 Redox conditions
The redox conditions of water not only play an important role in controlling the preservation of sedimentary OM and the formation of black shale, but also restrict the spatial distribution of microorganisms, especially anaerobic ones (Hammarlund et al., 2012; Jones and Fike, 2013; Gomes and Hurtgen, 2015). Iron speciation and its ratios are reliable indicators for determining redox conditions in water columns (Poulton and Canfield, 2011; Li et al., 2015). For samples with FeT > 0.5%, FeHR/FeT < 0.38 represents oxic conditions; otherwise, its represents anoxic conditions. Additionally, under anoxic conditions, Fepy/FeHR < 0.7–0.8 represents ferruginous conditions, otherwise, it represents euxinic conditions (Poulton and Canfield, 2011). All FeT values of the samples were >0.5%, which can be used to determine the redox condition.
From the late Katian to early Hirnantian stages, the value of FeHR/FeT ranged from 0.31 to 0.71 (average = 0.56), representing suboxic to anoxic conditions (Figure 2C). Additionally, the value of Fepy/FeHR ranged from 0.41 to 0.67 (average = 0.58), suggesting a ferruginous environment. For the GYQ Formation, the value of FeHR/FeT decreased to 0.19, representing oxic conditions. Then, for the early Rhuddanian Stage, the value of FeHR/FeT increased to 0.71, and the Fepy/FeHR values increased to 0.64 (on average), suggesting that the water conditions returned to being ferruginous conditions (Figure 2). Comparing these data with those of the other three sections, we found that the Upper Yangtze Basin was dominated by anoxic ferruginous conditions before and after the Hirnantian glacial period, and that transient oxic-suboxic conditions occurred in the early late Katian Stage and GYQ Formation period (Figure 6).
FIGURE 6. Redox condition correlations for the study sections. Data of the Shuanghe section, Nanbazi section, and Wangjiawan section can be found in previous studies (Yan et al., 2009b, 2012; Liu et al., 2016; Li et al., 2017b; Li N et al., 2021; Li Y et al., 2021).
Additionally, the degree of water anoxic varied in different sections, especially in the early stage of the Hirnantian glaciation (i.e., M. extraordinarius): when other sections were dominated by ferruginous conditions, while, Shuanghe section located in the southwestern sedimentary center of the Upper Yangtze Basin presented euxinic condition (Figure 6). The reasons for the difference in redox conditions are complex, which may be related to the input of terrigenous debris, the effectiveness of sulfate, the changes of sea level and paleoproductivity (Zou et al., 2018; Li et al., 2019; Wang et al., 2021a; Li N et al., 2021; Dong et al., 2022).
5.2 Microbial sulfate reduction effects in marine sediments
In the early diagenesis stage, Fe2+ combined with the H2S generated by the MSR in the water column. This combination formed pyrite, which is an important part of the sulfur cycle (Hurtgen, 2012). This process not only consumes sulfate but it also consumes OM in water, thereby controlling the formation of black shale (Gomes and Hurtgen, 2015). Existing research shows that the abundance of OM, availability of sulfate and the input of active iron jointly controls the strength of MSR (Berner and Raiswell, 1984; Johnston et al., 2005; Raiswell and Canfield, 2012). To effectively evaluate the strength of MSR, the sulfate reduction index (SRI) was introduced (Lallier-Verges et al., 1993). SRI can be calculated using the following equation:
Where TOCOR represents the original carbon content, which was calculated according to previous studies (Berner and Raiswell, 1984; Lallier-Verges et al., 1993; VETO et al., 1994), as
Thus, the equation for SRI can be rewritten as:
This equation does not take into account the organic carbon loss and related hydrocarbon generation and loss (i.e., via expulsion) during the thermal maturation of OM; the obtained SRI value is thus the minimum OM consumed by the MSR. The greater the value of SRI, the higher the strength of MSR.
It should be noted that the above equations were only applicable to anoxic conditions, without biological disturbance (Ekpo et al., 2012). This is because under anoxic conditions, most of the metabolizable organic carbon can be assumed to be consumed by sulfate reduction, and the generated H2S is not likely to oxidize and escape from the sediments owing to the protection of large amounts of active iron. Of course, the actual reaction process is more complex, and is controlled by many factors, such as the availability of organic carbon and sulfate. However, the positive exponential relationship between SRI and TOC observed in different modern aquatic environments can confirm the effectiveness of SRI as an index of MSR (Shen et al., 2011). We noted that the value of SRI decreases, and the value of TOC increases with a decrease in the sulfate content from euxinic water to normal seawater and then to fresh water; this represents a decrease in sulfate reduction strength and the preservation of organic carbon.
For the Tianlin section, from the late Katian to Hirnantian and then to early Rhuddanian stages, the value of SRI first decreased and then increased, reaching its minimum value in the GYQ Formation, with an average of 1.27 (Table 1). Owing to limited sample data, no significant correlation was found between SRI and other elements or indicators in the Tianlin section (Table 1). Therefore, we discuss these data in relation to the four other sections within the same basin to understand the impact of SRI on the sediments.
There was a significant power function negative correlation between SRI and TOC (r = −0.43, p < 0.01, n=117, Figure 7A), indicating that the consumption of active OM increased with increasing MSR intensity. It is worth noting that under different sedimentary environments, TOC values clearly show different trends with a change in SRI (Figure 7A). In euxinic environments (i.e., TS/TOC ≤0.5, SRI ≤1.499) (Berner and Raiswell, 1984; Liu et al., 2021), TOC decreases rapidly with an increase in SRI. Under other environments (SRI >1.499), with the increase in SRI, TOC gradually tends to stabilized (Figure 7A). This indicates that, under anoxic conditions, the availability of active OM was not the main factor limiting MSR in the study area. Additionally, there was a logarithmic negative correlation between SRI and OCAR (r = −0.22, p < 0.05, n = 117, Figure 7B), which further supports the speculation above. For regions with a high TOC content, the value of SRI was low, which may be related to the availability of sulfate in the water column.
The SRI vs. Fepy plot exhibits a significant positive power function relationship (r = 0.33, p < 0.01, n = 117, Figure 7C), indicating that the pyrite in shale was mainly generated by MSR, and that the input of active iron was not the main factor limiting MSR. Additionally, there was a positive logarithmic correlation between SRI and δ34Spy (r = 0.30, p < 0.01, n=117, Figure 7D), indicating that MSR was one of the main driving forces for the positive excursion of δ34Spy in the Upper Yangtze Basin. It is noteworthy that this driving force relationship mainly occurs in sulfate limited environments, such as in a closed system and/or porewater (Bradley et al., 2016). In a semi-restricted environment, the Upper Yangtze Basin conforms to this trend. There was no significant relationship between SRI and δ13Corg (data not shown), suggesting that MSR was not the cause of the δ13Corg excursion.
5.3 Impact of volcanic activity on marine sediments
Large-scale volcanic eruptions can cause a series of changes in the atmospheric composition, climate, and biosphere of the earth; most notably, volcanic activity plays an important role in OM enrichment and biological extinction (Ernst and Youbi, 2017). Volcanic activities promote the enrichment of OM via two main pathways. First, emitted volcanic ash and aerosols provide substantial nutrients for marine organisms (e.g., Fe, P, N, Mn, etc.), which improves primary productivity; second, volcanic activities can create an extremely anoxic water environment, which increase the amount of OM (Ge et al., 2019; Wu et al., 2019). Many bentonite rocks were found in the late Katian Stage (P. pacificus) and early Rhuddanian Stage (A. ascensus) in the Upper Yangtze Basin, confirming the frequent volcanic activity during the O-S transition period (Figure 8). In this study, we used the thickness and layer number of bentonite rocks to discuss their relationship with paleoproductivity and redox conditions.
In the Tianlin section, dense segments of bentonite were mainly concentrated in the early Hirnantian (Met. extraordinarius) and early Rhuddanian stages (A. ascensus), whereas other segments were loosely distributed (Figure 1C). Evidently, the TOC value of black shale in dense segments was generally higher than that in the loose segments, which indirectly proves that volcanic activity could promote the enrichment of black OM. Moreover, similar conclusions have been drawn in other sections of the Upper Yangtze Basin (Wu et al., 2018; Li Y et al., 2021). The same corresponding characteristics were also reflected in the relationship of bentonite with OCAR and Fepy/FeHR (Figure 2), that is, the dense section of bentonite induced an increase marine primary productivity and thereby the lack of oxygen in water columns.
In addition to the thickness of bentonite, the Hg content is one of the most effective proxies indicating the strength of volcanic activity (Sial et al., 2013; Charbonnier et al., 2017; Grasby et al., 2019). In marine systems, Hg can be stored in sediments combined with OM, clay minerals, sulfides and other components (Ravichandran, 2004; Selin, 2009). Organic mercury complexes formed by OM are often the main host of Hg in sediments (Ravichandran, 2004). However, there was no significant correlation between Hg and TOC (r = 0.27, p > 0.1, n=23, Figure 9A) in the Tianlin section, suggesting that organic mercury was not the main occurrence state of Hg. Additionally, there was no significant correlation between Hg and Al (r = −0.23, p > 0.1, n=23, Figure 9B); this indicates that clay minerals were also not the main occurrence state of Hg. There was a weak positive correlation between Hg and TS (r = 0.50, p < 0.05, n=23, Figure 9C) suggested that the occurrence of mercury in sulfide minerals may be a reason for its enrichment. However, there was no significant correlation between Hg and Mo, an indicator that can reflect the redox conditions of water (r = 0.13, p > 0.1, n = 23, Figure 9D). This indicates that the change in redox conditions did not affect the enrichment of Hg (Algeo and Lyons, 2006; Duan et al., 2016). Alternatively, the rapid formation of sulfide under anoxic conditions did not change the content of Hg. Therefore, we believe that the increased input of atmospheric mercury, associated with volcanic eruptions, may be a valid explanation for Hg enrichment.
Additionally, the location of the dense segments of bentonite and the high Hg content were the same as or close to the negative excursions of δ13Corg and δ34Spy, especially in the early Rhuddanian Stage, showing that volcanic activity was the trigger for δ13Corg and δ34Spy disturbances (Figures 1, 2). Li Y et al. (2021) also confirmed this inference using Hg results measured in the same basin.
The CO2 released by volcanic activities is relatively rich in light carbon isotopes, and these carbon isotope values range from 0‰ to −7.5‰ (average = −5.0‰). Volcanic activities are considered to be the main source of carbon isotope excursions (Hesselbo et al., 2000). Volcanic eruptions release a large amount of CO2 that is rich in light C isotopes, which can saturate the atmosphere-ocean system. Many carbon sources rich in 12C enter the atmosphere and are absorbed and fixed by marine planktonic algae, one of the main sources of sedimentary OM, through photosynthesis, resulting in negative excursion of carbon isotope in subsequent sediments (Kemp et al., 2005; Wang et al., 2021b; Hu et al., 2022). In addition, it takes a long time for CO2 from volcanic eruptions to affect the composition of carbon isotopes in seawater, which is consistent with the negative excursion of carbon isotope in the early Rhuddanian Stage, which lasted for nearly 3 Myr. This is in line with the possibility that CO2 released by volcanic activity may be the main driver of negative carbon isotope excursion. Science it is a greenhouse gas, an increase in the CO2 concentration in the atmosphere can induce a prolonged greenhouse effect on earth, translating to increased surface temperatures. This is consistent with glacier melting and sea-level rise events during the Early Silurian.
However, the proportion of sulfate input to the marine environment from volcanic activities is relatively low (<6.0%) (Canfield and Farquhar, 2009), which may cause a significant negative excursion of δ34Spy in a short time. However, there is not certainty that this is the reason for the low value of δ34Spy for a long time. A comprehensive analysis is required to explain the causes of this phenomenon.
5.4 Analysis of δ34Spy variability in hirnantian glaciation
In the MSR process, the lighter 32S is preferentially reduced from sulfate, and the generated sulfide has a lower content δ34S, leaving a residual carbonate reservoir rich in δ34S. Under limited sulfate, and the continuous consumption of MSR, the δ34S increases gradually, and the difference between the δ34S value and the residual carbonate reservoir decreases gradually (Canfield, 2001). It is apparent that the value of δ34Spy mainly depends on the sulfur isotope composition of sulfate (δ34SCAS) in the source region and isotope fractionation between sulfate and sulfide (Δ34S = δ34SCAS − δ34Spy). The magnitude of isotope fractionation (Δ34S) is related to the MSR reaction rate and marine sulfate concentration (Leavitt et al., 2013; Algeo et al., 2015). With sufficiently active OM, an open system featuring a high concentration of sulfate is prone to large isotope fractionation; on the contrary, this increases the reaction rate of MSR, and induces smaller isotope fractionation (Leavitt et al., 2013).
During the O-S transition period, samples from five sections in the Upper Yangtze Basin showed a significant variation in δ34Spy, especially during the Hirnantian Stage (Figure 3). Discussions on the causes of this phenomenon mainly focus on whether the marine sulfate concentration changed during this period, that is, whether sulfate availability changed significantly. (Jones and Fike, 2013). analyzed shale samples from Ellis Bay Formation and found that δ34SCAS did not undergo significant excursions throughout the O-S period. The main reason for the global δ34Spy excursion was the instantaneous decrease in Δ34S in the microbial sulfur cycle under the influence of abrupt climate change. The transition from anoxic conditions to oxic ones caused the chemocline to migrate below the sediment-water interface, where the exchange of sulfate between pore water and overlying water is limited, resulting in a gradual increase in δ34Spy (Yan et al., 2009a; Jones and Fike, 2013). Under these conditions, the framboids generated by MSR should have a large particle size difference, but the pyrite found in the upper Yangtze basin is relatively uniform. It was thus inferred that the framboids were generated in the water column and were the result of synergy (Zou et al., 2018; Li N et al., 2021). Zou et al. (2018), Li N et al. (2021), and Wang et al. (2021a) also found that in the O-S period, the offset of δ34Spy did not appear in a large range like that in a closed system. On the contrary, the positive offset range was small. Therefore, it can be assumed that the reason for the decrease in the Δ34S value in the Upper Yangtze Basin during the O-S period was a decreased difference between the limited sulfate input and MSR fractionation, rather than the influence of sulfate concentration in pore water.
5.5 Potential causes of δ13Corg and δ34Spy variations
For the C cycle, δ13Corg presented a negative excursion for a long time before the Hirnantian glaciation (i.e., late Katian stage), corresponding to a high TOC content, indicating that a large amount of organic carbon was buried (Figures 2, 10A). The burial of organic carbon removes a large amount of 12C from the marine carbon pool, causing the carbon isotopes in the marine system to become heavier, thereby making the carbon isotopes in the sediments accordingly heavier. At the same time, the burial of a large amount of organic carbon consumes the CO2 released by volcanic activity in the atmospheric, resulting in a decrease in atmosphere pCO2 concentrations, leading to a drop in temperature and the cooling of the global climate (Murray, 1994). Additionally, sulfur species (i.e., SO2, H2S, and COS) emitted by volcanic activities also control climate change. These sulfur species can be rapidly oxidized into sulfate in the troposphere and washed out of the atmosphere (McCormick et al., 1995; Mather, 2015; Hu et al., 2020). In the stratosphere, sulfate will backscatter the short-wave solar radiation in the form of aerosols, and absorb the long-wave radiation, making the temperature on the Earth’s surface decreased, resulting in global cooling (McCormick et al., 1995; Mather, 2015). This variability was similar to those of climate and δ13Corg changes in the Hirnantian period, indicating that carbon burial was the direct reason for the positive excursion of δ13Corg (Figure 10B). This, of course, the composition of δ13Corg was not only affected by the atmospheric pCO2 concentrations, but also affected by the secondary productivity, terrestrial OM, and marine dissolved organic carbon (Bekker et al., 2008; Jiang et al., 2010; Jiang et al., 2012). Recent studies on multiple proxies of biomarkers showed that the planktonic algae was the main source of OM during this period (Zhang et al., 2020; Wang et al., 2021b). Meanwhile, the values of ∑steranes/∑hopanes and steranes C27/C29 were used to exclude the contribution of bacteria and terrestrial plants to sedimentary OM (Zhang et al., 2020). Therefore, the convincing explanation for the excursion of δ13C during this period is that planktonic algae can gradually consume CO2 in the water column through photosynthesis, which makes the δ13C is gradually enriched in the newly generated sedimentary OM.
FIGURE 10. Schematic model for the carbon and sulfur cycles in the Upper Yangtze Basin during the O-S period. (A) Pre- and post glaciation for the negative excursions of δ13Corg and δ34Spy, (B) Hirnantian glaciation for the positive excursions ofδ13Corg and δ34Spy. MSR, microbial sulfate reduction.
During the post-glaciation period, with the warming of the climate and the recovery of volcanic activity, the concentration of CO2 in the atmosphere increased, and the 12C input into the marine environment rapidly increased, triggering the negative excursion of 13Corg (Figure 10A). Additionally, TOC and δ13Corg showed no significant correlation, and carbonate sedimentary facies were not found in the Upper Yangtze Basin, indicating that carbonate weathering was not the reason for the positive deviation in δ13Corg (Chen et al., 2004).
For the S cycle, during the pre-glaciation period, hot and humid climatic conditions and strong weathering increased the input of terrestrial sulfates, coupled with frequent volcanic activity, this resulted in the continuous input of 32S-rich sulfates to produce 34S-poor sulfides under the MSR (Figure 10A). During the Hirnantian glaciation period, rivers were frozen, sea levels fell, and the terrestrial input of sulfate was blocked, further reinforcing the limitations experienced by the basin. At this time, different degrees of anoxic conditions occurred in water columns, at different locations, resulting in different level of sulfur isotope fractionation. Nevertheless, the generated sulfide gradually enriched 34S and reached its maximum in the GYQ Formation (Figure 10B).
During the post-glaciation period, as the temperature rose, the ice sheet melted, the sea level rose, the volcanic activity was restored, weathering was enhanced, and rivers recovered. Overall, this resulted in inputs of sulfate to rapidly increase within the basin, and the sulfide rich in 32S deposited under the action of MSR throughout the Rhuddanian Stage (Figure 10A).
6 Conclusion
A high-resolution analysis of δ13Corg, and δ34Spy was conducted for the Tianlin section, and combined with data for four previously published sections, our study provides new insights into the isotopic disturbances and factors underlying the Hirnantian glaciation period in the Upper Yangtze Basin. Under semi-restricted conditions, the influence of warm climatic conditions and terrigenous clastic inputs caused by strong weathering caused the Upper Yangtze Basin to have a high primary productivity. This state was maintained until the early Hirnantian Stage, which promoted carbon burial and led to positive excursions of δ13Corg. During post-glaciation, the temperature and primary productivity gradually recovered under the influence of volcanic activity, resulting in negative excursions of δ13Corg. The excursion of δ34Spy can be explained through the lens of several factors. During pre-and post-glaciation, because of an increase in terrestrial sulfate input and the influence of volcanic activity, the sulfides produced by MSR had lower δ34Spy. Additionally, during Hirnantian glaciation, the availability of sulfate decreased, and under the action of MSR, sulfate in the water gradually enriched δ34S, thereby producing sulfides with high δ34S levels. The low values of δ13Corg and δ34Spy in pre- and post-glaciation sections coincided with the strengthened volcanic activity, indicating that volcanic activity was a major mechanism for the negative excursion of δ13Corg and δ34Spy. This study emphasizes the complex influence of volcanic activity and MSR on carbon and sulfur cycle disturbances and environmental changes in semi-restricted basins.
Data availability statement
The original contributions presented in the study are included in the article/supplementary material, further inquiries can be directed to the corresponding authors.
Author contributions
Investigation, ZD and ZW; Methodology, WZ and FZ; review and editing YD and XF; data curation, ZW and YZ; writing original draft, ZD; funding acquisition, CW.
Funding
This study was funded by the National Natural Science Foundation of China (No. 41772129).
Conflict of interest
Author FZ is employed by Xuzhou Datun Engineering Consulting Co., Ltd.
The remaining 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.
Publisher’s note
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Keywords: sulfur isotopes, carbon isotope, bentonite, sulfate reduction index, Upper Yangtze Basin, Hirnantian
Citation: Dong Z, Wang Z, Zhang W, Zhao F, Du Y, Zhu Y, Fu X and Wang C (2022) Dynamic sulfur and carbon cycles related to microbial sulfate reduction and volcanic activity during the Hirnantian glaciation in the Upper Yangtze Basin, South China. Front. Earth Sci. 10:971031. doi: 10.3389/feart.2022.971031
Received: 16 June 2022; Accepted: 08 August 2022;
Published: 30 August 2022.
Edited by:
Qingtao Meng, Jilin University, ChinaReviewed by:
Yu Song, China University of Geosciences Wuhan, ChinaKun Zhang, Northeast Normal University, China
Copyright © 2022 Dong, Wang, Zhang, Zhao, Du, Zhu, Fu and Wang. 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.
*Correspondence: Zetang Wang, wangzetang@cumt.edu.cn; Wenli Zhang, 649069716@qq.com