Volume 35, Issue 10 e2019PA003838
Research Article
Free Access

The Brachiopod δ11B Record Across the Carboniferous-Permian Climate Transition

S. A. Legett

Corresponding Author

S. A. Legett

Department of Geosciences, State University of New York at Stony Brook, Stony Brook, NY, USA

Now at Los Alamos National Laboratory, Los Alamos, NM, USA

Correspondence to:

S. A. Legett,

[email protected]

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E. T. Rasbury

E. T. Rasbury

Department of Geosciences, State University of New York at Stony Brook, Stony Brook, NY, USA

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E. L. Grossman

E. L. Grossman

Department of Geology and Geophysics, Texas A&M University, College Station, TX, USA

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N. G. Hemming

N. G. Hemming

Department of Geosciences, State University of New York at Stony Brook, Stony Brook, NY, USA

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D. E. Penman

D. E. Penman

Department of Geology and Geophysics, Yale University, New Haven, CT, USA

Department of Geosciences, Utah State University, Logan, UT, USA

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First published: 12 September 2020

Abstract

We present the δ11B of well-preserved brachiopod fossils coupled with geochemical modeling to examine how seawater boron responded to abrupt and dynamic climate changes in the Late Paleozoic. The Late Carboniferous, a time of major coal formation and glacioeustatic sea level changes, is characterized by relatively stable brachiopod δ11B of 15–17‰, similar to values seen in modern brachiopods. Brachiopod δ11B dropped by ~5‰ in the early Permian and then restabilized at a new value of 10‰ within a few million years. Mass balance models of seawater δ11B reproduced the overall trends in our brachiopod data but failed to capture the large drop in δ11B in the early Permian. Published seawater 87Sr/86Sr and δ44/40Ca data based on brachiopod shells also shift to lower values in the early Permian, suggesting a common control on all three seawater isotope systems. The Permian terrestrial record of evaporites and eolian deposits suggests a prolonged reduced delivery of dissolved weathering products to the ocean, accounting for the change in seawater 87Sr/86Sr. This reduced weathering, in turn, led to increased atmospheric CO2 and lowered seawater pH, which may have significantly decreased major removal mechanisms for seawater calcium and boron leading to declines in both isotope systems. We propose that boron removal via coprecipitation in carbonates and adsorption onto clay minerals was significantly diminished due to a reduction in the availability of the borate aqueous species caused by lowered seawater pH.

Key Points

  • Seawater δ11B changed from high values in the Carboniferous to 5‰ lower values in the Permian with a steep decrease in the early Permian
  • Seawater δ11B, 87Sr/86Sr, and δ44/40Ca all drop in early Permian suggesting reduced weathering/higher atmospheric CO2 as common control
  • Lower seawater pH in Permian ➔ reduction in borate concentration ➔ reduction in light B removed from seawater ➔ decreased seawater δ11B

Plain Language Summary

A great way to understand the effects of climate changes happening today is to look at how climate changes affected Earth systems in the past. One of the most extreme climate changes happened roughly 290 million years ago during the early Permian period. Prior to this time, all of the continents on Earth had come together to form the supercontinent Pangea, which caused major changes in ocean circulation and climate patterns around the equator. In the Carboniferous, the low-latitude environment was very wet, but in the Permian it became very arid, meaning there was less rainwater to dissolve rocks on the continents and deliver their dissolved salts to the oceans. To see how the oceans responded to these changes, we measured boron isotope ratios (11B/10B) in shell fossils. Boron isotopes usually change because of differences in ocean inputs/outputs or because of changes in ocean pH. The boron isotopes, along with strontium and calcium isotopes, changed significantly during the Carboniferous-Permian transition. This suggests that all of the isotopes changed because of the same processes. We argue that a reduction of dissolved salts delivered to the ocean by rivers caused the pH in the ocean to become more acidic.

1 Introduction

The Late Paleozoic was a time of dramatic climate change, with the formation of some of the largest glaciers in Earth history in the Pennsylvanian and earliest Permian, followed by glacial retreat in the early Permian (e.g., Fielding et al., 2008; Goddéris et al., 2017; Tabor & Montañez, 2002) and a transition from wet to arid conditions in low-latitude regions (Poulsen et al., 2007; Tabor et al., 2013). This reduction in rainfall was likely the result of the final amalgamation of Pangea changing ocean circulation and leading to increased continentality. Models indicate arid interiors in the low-latitude regions of the supercontinent beginning in the early Permian (Blakey, 2003; Goddéris et al., 2017; Parrish, 1993; Poulsen et al., 2007; Tabor et al., 2013). Along with the aridity, current models based on the δ13C of terrestrial pedogenic carbonates and the stomatal index of fossil leaves also suggest a switch from one of the lowest atmospheric pCO2 values on Earth during the Carboniferous to a much higher pCO2 by the end of the Sakmarian (Foster et al., 2017; Montañez et al., 2007, 2016; Witkowski et al., 2018).

As the continents combined to form Pangaea in the Late Paleozoic, key ocean gateways closed (Ziegler, 1990), and the normal westward flowing ocean-air circulation switched to a more monsoonal circulation (Blakey, 2003; Parrish, 1993). Mountains created by the amalgamation of continents intensified low pressure in the equatorial continental interior leaving it very arid. Furthermore, warming in the Permian increased evapotranspiration throughout Pangaea, driving the interior aridity further poleward (Parrish, 1993). Stratigraphic units from the early Permian express this aridity in the form of calcretes and aridisols (Tabor et al., 2013; Tabor & Montañez, 2002; Tabor & Poulsen, 2008), evaporites (Mack, 2003; McCahon & Miller, 1997; Tabor & Poulsen, 2008), and large eolian sediment deposits (Soreghan et al., 2002; Tabor & Poulsen, 2008). These deposits began to appear in low-latitude regions of Pangea at the end of the Pennsylvanian and expanded to include all but high latitudes by the early-to-middle Permian (Tabor et al., 2013; Tabor & Montañez, 2002; Tabor & Poulsen, 2008). This transition toward extreme aridity along with reported changes in atmospheric pCO2 (Foster et al., 2017; Goddéris et al., 2017; Montañez et al., 2007, 2016; Witkowski et al., 2018) provides a unique opportunity to better understand the controls on the boron isotopic composition of seawater.

2 Materials and Methods

2.1 Brachiopod Sample Selection

The δ11B of well-preserved, carefully sampled brachiopods has been shown to reflect the δ11B of seawater and ambient pH, similar to other marine calcifiers (Jurikova et al., 2019; Lemarchand et al., 2002; Penman et al., 2013). For this study, we used well-characterized brachiopods from Ethan Grossman's collection at Texas A&M University (TAMU) and from the Yale Peabody Museum (YPM) collection. These brachiopods (Spirifer, Composita, and Dictyoclostus) were collected from low-latitude Carboniferous and Permian deposits in the U.S. Mid-continent (USM), Ural Mountains (UM), and West Spitsbergen (WSP; Grossman et al., 1991, 2008; Mii et al., 1997, 2001). USM brachiopods represent Carboniferous-Permian epicontinental seas and interior basin environments. They were collected from shales, limestones, and calcareous sandstones in the Kincaid, Fayetteville, Hale, Bloyd, and Tradewater Formations in Nebraska, Oklahoma, Arkansas, and Illinois, as well as the Admire, Council Grove, Chase, Cisco, and Wichita Groups in Nebraska, Kansas, Oklahoma, and Texas. UM brachiopods are predominantly Carboniferous (mid-Serpukhovian through early Permian). Finally, WSP brachiopods represent early Permian epicontinental seas and were collected from the Kapp Starostin formation in the westernmost island of the Norwegian Svalbard archipelago.

The samples used for this study all passed initial screening tests based on petrographic and cathodoluminescence (CL) microscopy (Figure 1; Grossman & Mii, 1996; Grossman et al., 1991, 1993, 2008; Mii et al., 2001). More recently, samples from the TAMU collection underwent clumped isotope analyses, and some of them (specifically UM samples) recorded anomalously high temperatures (Henkes et al., 2018), suggesting reordering at temperatures greater than 100°C. Additional work by electron backscatter diffraction demonstrated a range of preservation quality even in samples that appear well preserved (Pérez-Huerta & Laiginhas, 2018). Thus, there is clear evidence for solid-state alteration even if shells appear chemically and texturally preserved. This is important because boron is very sensitive to diagenesis and is typically lost with fluid-rock interactions, generally becoming isotopically lighter (Gaillardet & Allègre, 1995; Stewart et al., 2015). To screen for these potentially altered samples, elemental analyses (Li, Mg, Mn, Fe, and Sr) of solid brachiopods via laser ablation as well as dissolved sample solutions were performed using an Agilent 7500cx quadrupole inductively-coupled plasma mass spectrometry (ICP-MS). The elemental analysis results as well as δ18O values for samples previously analyzed by Grossman et al. (1991, 1993, 2008); Grossman and Mii (1996) and Mii et al. (2001) are listed in the supporting information (SI) associated with this article.

Details are in the caption following the image
Plane light (left) and cathodoluminescent (right) images of brachiopod sample TXP074 from the Permian of north central Texas showing fibrous texture and lack of luminescence in the shell.

2.2 Boron Separation and Analysis via ICP-MS

Powdered samples were collected from nonluminescent areas (low Mn/Fe) in the secondary layers of brachiopod shells and dissolved in 2% nitric acid. Once samples were fully dissolved, the carbonate solution was increased to an alkaline pH by adding high-purity ammonia to ensure retention on the ion exchange resin. Columns were created by fitting a 1,000 μl pipet tip with a polyurethane frit and filling the tip with ~50 μl Amberlite 743 boron-specific ion exchange resin that was crushed and sieved to 63–120 μm. The flow rate for the columns was controlled by connecting the pipet tips to clean peripump tubing attached to a peristaltic pump. Before loading samples, the resin was cleaned with 3 ml 2% nitric acid and equilibrated to the sample pH (pH = 9–10) with a solution of Milli-Q water and high-purity ammonia at a flow rate of 5 rpm. Samples were then loaded onto the columns at a rate of 0.5–3 rpm. Columns were washed with 1.5 ml Milli-Q water and high-purity ammonia solution at 0.5–3 rpm before eluting the boron in 1.2 ml 2% nitric acid at 0.5–3 rpm. The load and wash steps were collected as boron-free sample solutions for trace-element analysis and archived for additional isotope work in the future.

Most boron isotopic compositions and concentrations were determined using a Nu Plasma II MC-ICPMS at the FIRST@StonyBrook isotope lab. We used a Glass Expansion Tracey PFA44 spray chamber with helix, a Glass Expansion 100 microliter/minute nebulizer with a flow rate of 30–35 psi, Nu Instruments light element sampling cones, and collectors H7 (11B) and L6 (10B) in low-resolution mode. Each sample was bracketed with 50 ppb or 25 ppb (matching concentrations of diluted samples) NIST SRM 951 boric acid standard with a 2% nitric acid background run between all standards and samples. Washes with Milli-Q deionized water were completed before and after every analysis (90 s after standard and sample measurement; 60 s after background nitric measurements). Background was subtracted from samples and standards by taking the average signal of the bracketing nitric backgrounds and subtracting from the signal of the sample or standard, and the δ11B was calculated based on the average of the bracketing standards after background correction. All samples were run multiple times with an in-house coral standard (SB Coral; δ11B = 23.6 ± 0.3‰, [B] = 51.8 ppm, n = 35; comparison with international coral standard JCp-1 shown in Table 1), and the reported results (SI) were separated into two categories: reliable data with 2σ better than 1.5‰, a sample/blank ratio of 30 or more, and SB Coral δ11B = 23.6 ± 0.5‰; and less reliable data with 2σ better than 3‰, a sample/blank ratio of 10 or more, and SB Coral δ11B = 23.6 ± 1.5‰. Overall, we completed >200 analyses on Carboniferous and Permian brachiopods, though only 58 analyses met our data selection criteria. The reliable data are the only data shown in the figures within this article, but the results of all analyses are shown in the SI. All sample δ11B values obtained via MC-ICPMS were corrected by the offset (±0.5‰) of SB Coral from 23.6‰ in each batch of analyses.

Table 1. Comparison of SB Coral and JCp-1 Standards
SB coral JCp-1
δ11B (‰) 23.6 ± 0.3 23.8 ± 0.5
B concentration (ppm) 51.8 47.6
  • Note. For each standard, n = 35.

For samples analyzed by NTIMS at LDEO, all samples were bleached overnight in NaOCl to remove organic material and subsequently rinsed and ultrasonicated 10 times in quartz-distilled water then dissolved in quartz-distilled 2N hydrochloric acid. The 1 μl aliquots of sample solution (~1 ng of B) were loaded on degassed zone refined rhenium filaments with 1 μl of boron free seawater. Boron isotope ratios were measured in oxide form, acquiring masses 43 (11B16O2) and 42 (10B16O2) using the NTIMS techniques of Hemming and Hanson (1992). To avoid possible biases resulting from in-run instrumental fractionation, analyses were accepted only if the signal was stable or rising, the measured ratio (43/42) varied less than 1‰ throughout the course of the run, and at least three replicates gave concordant 43/42 ratios to within <1‰. To test the consistency of δ11B values between MC-ICPMS and NTIMS analyses, we ran some samples on both instruments (Table 2). When samples were taken from the same areas of the brachiopod shell, the variation in δ11B values from NTIMS and MC-ICPMS was very small (±0.2‰). However, when samples were taken from different areas of the brachiopod shell, δ11B values differed by up to 2‰, confirming the findings of Penman et al. (2013), which showed an intrashell δ11B variability in modern brachiopods of up to 3‰.

Table 2. Comparison of NTIMS and MC-ICPMS δ11B Results for Brachiopods Used in This Study
Sample name NTIMS δ11B (‰) MC-ICPMS δ11B (‰)
217434 15.6 15.4
223474 16.2 16.3
228942a 15.7 15.1
229932a 14.9 16.9
  • a For these analyses, samples run by NTIMS and samples run by MC-ICPMS were taken from different areas of the same brachiopod shell.

2.3 Principle Component Analysis of Brachiopods

In addition to the abovementioned screening techniques, we also performed principle component analysis (PCA) for all brachiopods used in this study to check for any variables that may bias the δ11B results (i.e., to determine if the δ11B values of our samples are due to sample locations or genera rather than seawater chemistry). To be sure that these analyses were complete, we also included the samples from Joachimski et al. (2005), which are plotted in Figure 4 along with samples from this study. Along with their δ11B, boron concentrations, and ages, each sample was assigned numbers from 1 to 13 to represent the sample's genus and numbers from 1 to 4 to represent the location from which the sample came. The results of these analyses are shown below (Figure 2).

Details are in the caption following the image
Biplot of principle components affecting δ11B of brachiopods used in this study. (a) Biplot of first and second principle components. (b) Biplot of second and third principle components.

Based on the results of the PCA, we see that there is no correlation between the location of a brachiopod sample and any other variable. Unsurprisingly, there is a significant correlation between the geologic age of the brachiopods and the boron concentration (Figure 2a). Additionally, there seems to be a slight correlation between brachiopod genus and δ11B, though when looking at the second and third principle components, genus is also correlated with the geologic age and boron concentration of the brachiopod (Figure 2b). This correlation is likely the result of different brachiopod genera occurring at different times in the geologic record.

3 Results and Discussion

3.1 Results

Based on the δ11B of the samples that passed screening tests (58 of 173), we can group brachiopods into two categories: the Pennsylvanian to earliest Permian (320–295 Ma) and the early-to-middle Permian (295–270 Ma). The older brachiopod δ11B values average ~15‰, while the younger brachiopods average much lower δ11B values around 10‰ (Figure 3 and Table 3). Based on the average δ11B of brachiopods from this study and Joachimski et al. (2005), we can calculate possible Carboniferous-Permian seawater δ11B values using the following equation (Equation 1; Foster & Rae, 2016):
urn:x-wiley:25724517:media:palo20924:palo20924-math-0001(1)
where δ11BSW is the δ11B of seawater δ11BCarb is the δ11B of carbonates (in this case, brachiopods), αB is the boron isotopic fractionation factor, KB is the dissociation constant, pH is the pH of seawater, and εB = (αB − 1) × 1,000. For the seawater δ11B reconstructions in this study, we used the mean surface seawater pH values of a “Neritan” ocean modeled by Ridgwell (2005) as well as constant modern-day values (pH = 8.2), a pKB of 8.6 (Dickson, 1990; T = 25°C; salinity = 35 psu), and boron isotopic fractionation factors from Lecuyer et al. (2002); αB = 1.020023) and Klochko et al. (2006); αB = 1.019368; Figure 3).
Details are in the caption following the image
Brachiopod δ11B values and estimated seawater δ11B across the Carboniferous-Permian boundary. Error bars represent 2σ standard deviation on ≥3 analyses. Unfilled (white) symbols represent samples analyzed by NTIMS rather than ICP-MS. Solid black line through data represents a 1 Myr moving average of 1–13 data points depending on the number of data points available per Myr interval. Black vertical line represents the Carboniferous-Permian boundary. Dashed lines represent seawater δ11B calculated using the boron fractionation factor of Lecuyer et al. (2002); dotted lines represent seawater δ11B calculated using the boron fractionation factor of Klochko et al. (2006). Blue lines were calculated using the mean surface seawater pH values of Ridgwell (2005); gray lines were calculated using a constant seawater pH of 8.2. Ages and stage information are from GTS2012.
Details are in the caption following the image
Estimated changes in Carboniferous-Permian processes controlling the boron isotopic budget of seawater and modeled Carboniferous-Permian seawater δ11B. (a) Clastic sediment flux (Wold & Hay, 1990). (b) Oceanic crust production (Gaffin, 1987). (c) Marine carbonate accretion rate (Walker et al., 2002). (d) Modeled Carboniferous-Permian seawater δ11B and LOESS regression of brachiopod-based seawater δ11B versus age; light gray shaded areas surrounding LOESS curve represent 95% confidence interval. Black vertical line represents the Carboniferous-Permian boundary. Ages and stage information from GTS2012.
Table 3. Brachiopod Ages (GTS 2012), δ11B, Boron Concentration, and Analysis Methods Used
Sample name Age (Ma) δ11B (‰) B (ppm) Analysis method
WSP370T 270.2 10.71 ± 0.85 35.4 MC-ICPMS
SS6-96-12 274.2 9.32 50.11 MC-ICPMS
TXP001 274.3 12.45 21.24 MC-ICPMS
TXP003 274.3 10.36 8.06 MC-ICPMS
TXP005 274.3 11.41 8.13 MC-ICPMS
RST27 293.6 11.09 ± 1.10 34.1 MC-ICPMS
RST27T 293.6 10.55 4.12 MC-ICPMS
RST29 293.6 11.88 ± 0.84 40.9 MC-ICPMS
TXP053 295.5 17.36 8.45 MC-ICPMS
TXP074A 295.9 15.68 ± 2.20 98.3 MC-ICPMS
TXP074B 295.9 17.02 MC-ICPMS
RAK15 296.2 16.59 62 MC-ICPMS
228987 297.2 18.30 NTIMS
TXP020 297.4 18.88 ± 0.88 26.5 MC-ICPMS
217434-2 297.48 14.44 ± 0.70 MC-ICPMS
217434 297.48 16.37 ± 0.80 MC-ICPMS
217434 297.48 15.59 NTIMS
223474 299.25 16.25 ± 0.43 MC-ICPMS
223474 299.25 16.23 NTIMS
223474-2A 299.25 13.95 ± 0.30 MC-ICPMS
223474-2B 299.25 15.97 ± 1.28 MC-ICPMS
228952 299.25 14.41 ± 0.80 MC-ICPMS
228954 299.25 15.95 ± 0.20 MC-ICPMS
228942 299.32 15.15 ± 0.41 MC-ICPMS
228942 299.32 15.74 NTIMS
228942-2 299.32 16.94 ± 0.40 MC-ICPMS
228949 299.32 14.54 ± 0.43 MC-ICPMS
228958 299.35 15.18 ± 1.15 MC-ICPMS
228961 299.35 14.64 ± 0.44 MC-ICPMS
TXP037 299.4 13.98 35.63 MC-ICPMS
TXP009 300 16.70 21.55 MC-ICPMS
TXP017 300 16.44 6.99 MC-ICPMS
228768h-1 300.5 16.29 ± 0.25 MC-ICPMS
228768h-2 300.5 16.01 ± 0.28 MC-ICPMS
228768s-1 300.5 15.65 ± 0.79 MC-ICPMS
228768s-2 300.5 14.56 ± 0.42 MC-ICPMS
229762 302.33 16.77 ± 1.98 MC-ICPMS
229819 303.47 16.26 ± 1.12 MC-ICPMS
229332 303.7 16.98 ± 0.48 MC-ICPMS
229025 303.87 14.32 ± 0.80 MC-ICPMS
K042C 304.17 15.23 ± 0.43 18.2 MC-ICPMS
229895 304.39 16.25 ± 0.64 MC-ICPMS
229903A 304.64 15.42 ± 0.64 MC-ICPMS
229903B 304.64 14.93 ± 0.67 MC-ICPMS
229884 305.35 14.30 ± 0.41 MC-ICPMS
229814 305.5 14.72 ± 0.11 MC-ICPMS
319341 307 13.63 NTIMS
229964 307.38 14.49 ± 0.67 MC-ICPMS
229964 307.38 16.00 NTIMS
502292 307.38 14.12 ± 0.66 MC-ICPMS
502292 307.38 15.15 NTIMS
Y86 307.4 20.40 ± 0.98 13.3 MC-ICPMS
Ru181 307.7 14.89 1.16 MC-ICPMS
TXD002 308.3 15.10 ± 0.76 27.2 MC-ICPMS
TXD033 312.8 15.42 ± 0.88 27.9 MC-ICPMS
229932 314 16.88 ± 1.07 23.26 MC-ICPMS
229932 314 14.88 NTIMS
847 320.2 14.30 24.35 MC-ICPMS

3.2 Modeled Boron Isotopic Budget of Seawater

Boron isotopes have been shown to have great utility in the Cenozoic for estimating changes in atmospheric pCO2 due to a pH-controlled isotope fractionation. A major hurdle to taking this further into the geologic past is the need to know the δ11B of ancient seawater to calculate its pH. For the Cenozoic, foraminifera that inhabit known depths in the ocean can be used to consider gradients, allowing the estimation of seawater δ11B (Greenop et al., 2017; Pearson, 1999). However, beyond the time when these taxa are recognized, there are few ways to definitively determine the δ11B of past seawater. Several studies have addressed this issue by modeling the boron isotopic ratio of seawater through time based on estimates of past boron fluxes (i.e., Joachimski et al., 2005; Lemarchand et al., 2002; Simon et al., 2006). These estimates are based on modern boron fluxes and their isotopic ratios as well as assumptions about the controlling mechanisms behind those fluxes throughout geologic time (Table 4).

Table 4. Modern Seawater Boron Fluxes and δ11B
Boron flux (Tg/yr) δ11B (‰) Source
Ocean inputs
Rivers/continental weathering 0.38 ± 0.04 10 a
Hydrothermal 0.04 6.5 ± 8 b
Fluid expelled from accretionary prisms 0.02 25 ± 5 c
Ocean outputs
Low-temperature oceanic crust alteration 0.27 3.7 b
Adsorption onto clays 0.13 15 ± 1 d
Coprecipitation in carbonates 0.06 20 ± 5 e
  • Note. Sources: (a) Lemarchand et al. (2002), (b) Smith et al. (1995), (c) You et al. (1993), (d) Spivack and Edmond (1987), and (e) Vengosh et al. (1991).
Using two mass-balance equations for the boron content and boron isotopic composition of seawater (Equations 2 and 3; Lemarchand et al., 2002), we modeled Carboniferous-Permian seawater δ11B in an attempt to fit our data-based seawater δ11B curve (Figure 4d). For this model, we used scaled versions of the flux rates and the boron isotopic compositions seen in Table 4 along with the following equations from Lemarchand et al. (2002; Equations 2 and 3):
urn:x-wiley:25724517:media:palo20924:palo20924-math-0002(2)
urn:x-wiley:25724517:media:palo20924:palo20924-math-0003(3)
where BSW is the boron content of seawater, t is time in years, φin is total boron flux into the ocean, φout is total boron flux out of the ocean, RSW is the 11B/10B of seawater, and Rin and Rout are the weighted averages of the 11B/10B for the fluxes into and out of the ocean. We initialized our model at 320 Ma with modern-day boron flux rates and isotopic compositions. The data-based seawater curve seen in Figure 4 is a locally weighted scatterplot smoothing (LOESS) regression and 95% confidence interval of seawater δ11B calculated from our brachiopod data using the Lecuyer et al. (2002) brachiopod boron fractionation factor and seawater pH from Ridgwell (2005); for comparison, the seawater δ11B calculated using the inorganic calcite boron fractionation factor of Klochko et al. (2006) can be seen in Figure 3. While there may be unknown vital effects affecting the relationship between the δ11B of Paleozoic brachiopods and the δ11B of Paleozoic seawater, we have chosen to use the modern brachiopod-based boron fractionation factor of Lecuyer et al. (2002) for our seawater δ11B reconstruction. We then used scaling factors for the boron fluxes throughout the Carboniferous and Permian based on Wold and Hay (1990; riverine/weathering flux; Figure 4a), Gaffin (1987; hydrothermal, accretionary prisms, and low-temperature alteration fluxes; Figure 4b), and Walker et al. (2002; carbonate flux; Figure 4c). The δ11B of the fluxes were kept constant at their modern values with the exception of flux out from carbonates, which was based on the average δ11B values of the brachiopods used in this study.

3.3 Comparison to Other Seawater Isotopes

While the modeled seawater δ11B mirrors the general trend seen in the seawater δ11B estimated from our brachiopod data, it fails to capture the ~4‰ drop across the Asselian-Sakmarian transition. To better understand what the seawater δ11B model may be missing and why it does not match the δ11B curve suggested by our brachiopod data, we compared our δ11B record to trends in other seawater isotope systems during this time (Figure 5). The strontium isotopic composition of seawater (87Sr/86Sr) based on brachiopod measurements shows a trend that is similar to our δ11B curve, with a high plateau during the Pennsylvanian followed by a steep decline across the boundary and into the Permian (Figure 5b; McArthur et al., 2012; Veizer et al., 1999). The brachiopod-based calcium isotopic composition (δ44/40Ca) of seawater appears to show an overall decrease across the Carboniferous-Permian transition and continuing further into the Permian (Figure 5; Blättler et al., 2012). Unfortunately, because of the gap in δ44/40Ca data from ~283 to ~265 Ma, we do not know if this decrease was gradual or steep. Overall, all three seawater isotope proxies decrease as the Carboniferous transitions into the early Permian, suggesting a common controlling mechanism.

Details are in the caption following the image
Comparison of Carboniferous-Permian seawater δ11B, 87Sr/86Sr, and δ44/40Ca. (a) estimated seawater δ11B from LOESS regression and 95% confidence interval (shaded areas) of brachiopod δ11B presented in this study, (b) brachiopod-based seawater 87Sr/86Sr from Veizer et al. (1999), (c) brachiopod-based seawater δ44/40Ca from Blättler et al. (2012); black arrow represents average seawater δ44/40Ca for the Roadian and Wordian from Blättler et al. (2012).

The most significant source of boron to the oceans is riverine discharge (86% of boron input), while seawater boron outflux is dominated by low-temperature oceanic crust alteration (59% of boron output) and, to a lesser extent, adsorption onto clay minerals (28% of boron output; Table 4; Lemarchand et al., 2002). The strontium isotopic composition of seawater is controlled by the balance between riverine (granitic) and hydrothermal (basaltic) inputs to the oceans (Antonelli et al., 2017). Similarly, the major controls on the calcium isotopic composition of seawater are the balance between riverine and hydrothermal inputs and outflux via carbonate precipitation and oceanic crust alteration (Table 5; Fantle & Tipper, 2014; Farkaš et al., 2007; Griffith et al., 2008). The dominant mineralogy of seawater (i.e., calcite vs. aragonite seas) is also thought to play a significant role in the calcium isotopic composition of seawater (Blättler et al., 2012), but there is no such switch during the period of interest in this study. Based on these, the major factors likely controlling all three seawater isotope systems during the early Permian climate transition are riverine and/or hydrothermal fluxes.

Table 5. Modern Seawater Calcium Fluxes and δ44/40Casw
Ca flux (Tmol/yr)a δ44/40Casw (‰)b
Ocean Inputs
Weathering/rivers 10.8 −0.87 to −1.30
Hydrothermal 3.2 −0.96 ± 0.2
Ocean Outputs
Coprecipitation in carbonates 14.7 −0.7 to −1.6
Oceanic crust alteration 0.7 −0.7 to −1.7
  • a From Farkaš et al. (2007).
  • b From Griffith et al. (2008).

The Carboniferous-Permian decline in seawater 87Sr/86Sr has traditionally been interpreted as the result of two major environmental changes: (1) an initial decrease in continental weathering due to the extreme aridity associated with the assembly of Pangaea and (2) a continued decrease caused by increased hydrothermal activity associated with the opening of the Neotethys and heightened volcanism (Korte et al., 2006; Martin & Macdougall, 1995). With a decrease in continental weathering at the Carboniferous-Permian boundary, we would expect an increase in seawater δ11B and δ44/40Ca as the major source of “lighter” (relative to seawater) isotopes are removed (Tables 4 and 5; Farkaš et al., 2007; Griffith et al., 2008; Lemarchand et al., 2002). Because both the boron and calcium seawater isotopic compositions show decreases in the Permian, decreased continental weathering does not appear to be a common direct controlling factor for all three isotopic systems examined here. Similarly, an increase in hydrothermal activity in the early Permian is also unlikely to be directly controlling all three isotope systems as this would also result in an increase in seawater δ11B and δ44/40Ca by intensifying a major removal mechanism for light isotopes of boron and calcium (Tables 4 and 5; Farkaš et al., 2007; Griffith et al., 2008; Lemarchand et al., 2002).

Another possible interpretation of the changes in seawater isotopic composition in the early Permian is a change in the isotopic composition of riverine discharge. Traditionally, continental weathering materials transported by rivers are assumed to have an overall granitic composition (Taylor & McLennan, 1985). However, this may not have been the case throughout the entire Phanerozoic. In fact, a significant amount of weathering material delivered to the oceans may come from “basaltic rivers” and volcanic islands causing the weathering flux to have a more mafic composition (Allègre et al., 2010; Antonelli et al., 2017; Godderis et al., 2009; Kump et al., 2000). A more mafic riverine input due to increased weathering of basalts would certainly fit the decline seen in seawater 87Sr/86Sr across the Carboniferous-Permian boundary; however, it cannot explain the decrease in seawater δ11B and δ44/40Ca during the early Permian as the isotopic composition of the source rocks weathered and transported by rivers has been found to have little effect on the boron and calcium isotopic compositions of the riverine input to seawater (Rose et al., 2000; Tipper et al., 2006).

3.4 Permian Weathering and the Carbon Cycle

Overall, there seems to be no singular mechanism controlling the boron, strontium, and calcium isotopic compositions of seawater during the Carboniferous-Permian transition. Instead, there were likely multiple connected controls in effect. One such scenario would be the carbon cycle changes resulting from a decrease in continental weathering. Goddéris et al. (2017) suggest that the assembly of Pangaea combined with the lowering of the Hercynian Mountains in the early Permian led to a significant decrease in continental weathering due to extreme aridity and the creation of a thick, weather-resistant soil layer on the continent. Along with this reduction in continental weathering, there was also subsequent rise in atmospheric CO2. Diminished continental weathering explains the drop we see in seawater strontium isotopes, while the decreases in boron and calcium isotopes fit with a drop in seawater pH resulting from the increased atmospheric CO2. As the pH of seawater declines, we would see an increase in the dissolution of marine carbonates. These dissolved carbonates would, in turn, release light boron and calcium isotopes back into seawater as well as diminish one of their removal mechanisms. Both of these consequences would lead to a decrease in seawater δ11B and δ44/40Ca. However, though carbonates are the largest remover of calcium from seawater (Table 5; Farkaš et al., 2007; Griffith et al., 2008), they only make up 13% of the seawater boron outflux (Smith et al., 1995; Spivack & Edmond, 1987; Vengosh et al., 1991), meaning there must be an additional boron removal mechanism affected by the decrease in seawater pH.

To better constrain the extent to which boron removal from seawater would need to decrease in the early Permian to reproduce the seawater δ11B curve suggested by our data, we modeled the boron outflux fraction values needed to fit the seawater δ11B curve based on our brachiopod data (Figure 6). The results of this calculation imply that boron outflux from seawater began to decrease at the beginning of the Sakmarian before reaching its lowest value (a 29.2% reduction) by the early Artinskian. The dissolution of marine carbonates alone would only result in a maximum boron removal reduction of 13%, so we need to examine the chemistry behind how boron is removed from the seawater system.

Details are in the caption following the image
Modeled changes in boron outflux. (a) LOESS regression of seawater δ11B based on our brachiopod data (blue curve and shaded area) and the modeled fit produced by varying the fraction of boron outflux from seawater (black curve) and (b) modeled fraction of boron outflux needed to produce fit in (a).

All known boron fluxes out of the ocean are isotopically light compared to seawater (Joachimski et al., 2005; Lemarchand et al., 2002; Simon et al., 2006). This is due to the preferential removal of 10B in the form of borate sorption onto clays and coprecipitation in carbonates. Since the availability of borate in seawater is pH dependent (Hemming & Hanson, 1992), the decrease in seawater pH caused by reduced weathering in the early Permian would lead not only to the dissolution of carbonates releasing light boron back into the system but also to a depletion of borate in solution throughout the ocean. At the modern seawater pH of 8.2, the proportion of aqueous boron species is approximately 70% boric acid (B (OH)3) and 30% borate (B (OH)4; Figure 7). Based on the modeling study of Ridgwell (2005), the seawater pH was 8.05 during the Bashkirian at 320 Ma and dropped to 7.85 by the Roadian at 270 Ma. According to the seawater boron speciation graph (Figure 7; Hemming & Hanson, 1992), the availability of borate drops by 23% from modern seawater pH to Bashkirian seawater pH, while the change from Bashkirian to Rodian seawater pH shows a borate availability decrease of 31%. Because boron removal from seawater via coprecipitation in carbonates and adsorption onto clays relies almost exclusively on the availability of borate, a decrease in the borate composition of seawater due to lowered pH would directly and significantly impact the amount of boron outflux from seawater.

Details are in the caption following the image
Fraction of boron species versus pH (pKa = 8.6). The solid black line represents the pH of modern seawater at 8.2; the dashed black line represents the pH of seawater at 320 Ma (pH = 8.05) based on Ridgwell (2005); the dotted black line represents the pH of seawater at 270 Ma (pH = 7.85) based on Ridgwell (2005).

4 Summary and Conclusions

We measured the δ11B of Carboniferous-Permian brachiopods, encompassing the transition from the Late Paleozoic Ice Age to a greenhouse climate, to investigate the effects of a major climate shift on the boron isotopic composition of seawater. The results show high brachiopod δ11B throughout the Pennsylvanian, followed by a steep drop in the early Permian roughly coincident with glacial collapse, and ending in a restabilization of δ11B averaging ~10–11‰ in the early-to-middle Permian (Figure 3). We converted our brachiopod δ11B to seawater δ11B by applying the boron fractionation factor of Lecuyer et al. (2002) and using the estimated seawater pH values of Ridgwell (2005). When we modeled the secular variation of seawater δ11B and compared the results to our brachiopod-based seawater curve, we found that the model was able to reproduce the overall trends seen in our data, but it failed to capture the large drop in δ11B in the early Permian (Figure 4). To understand what the model may be missing, we compared our δ11B curve to brachiopod-based 87Sr/86Sr (Veizer et al., 1999) and δ44/40Ca (Blättler et al., 2012) seawater trends, which also showed decreasing isotopic values in the early Permian suggesting a common control on all three systems (Figure 5). We concluded that a decrease in continental weathering at the Carboniferous-Permian boundary and the subsequent rise in atmospheric CO2 and drop in seawater pH in the early Permian could explain the trends in seawater δ11B, 87Sr/86Sr, and δ44/40Ca through a decrease in radiogenic strontium delivered to the oceans and a reduction in the removal of seawater calcium and boron. Along with the dissolution of marine carbonates, we concluded that boron removal from seawater (though coprecipitation in carbonates and adsorption onto clay minerals) was further reduced by a diminution in the availability of the borate aqueous species caused by the drop in seawater pH in the early Permian.

Acknowledgments

The authors would like to thank the Editors and reviewers for their constructive comments, Chip Legett for his help with the modeling, Katie Wooton for her help with the analyses of the brachiopod samples, Bärbel Hönisch for the use of her lab for the NTIMS analyses, and Susan Butts for her help with finding and selecting brachiopod samples at the Yale Peabody Museum. This work was supported by National Science Foundation project EAR 1327425. The instrumentation used for the boron isotope analyses was part of an EAR MRI Grant 0959524.

    Data Availability Statement

    Sample information and data from this study are available through the Pangaea online database (https://issues.pangaea.de/browse/PDI-22644).