Chemical weathering consumes atmospheric carbon dioxide through the breakdown of silicate minerals and is thought to stabilize Earth’s long-term climate. However, the potential influence of silicate weathering on atmospheric pCO2 levels on geologically short timescales (103–105 years) remains poorly constrained. Here we focus on the record of a transient interval of severe climatic warming across the Toarcian Oceanic Anoxic Event or T-OAE from an open ocean sedimentary succession from western North America. Paired osmium isotope data and numerical modelling results suggest that weathering rates may have increased by 215% and potentially up to 530% compared to the pre-event baseline, which would have resulted in the sequestration of significant amounts of atmospheric CO2. This process would have also led to increased delivery of nutrients to the oceans and lakes stimulating bioproductivity and leading to the subsequent development of shallow-water anoxia, the hallmark of the T-OAE. This enhanced bioproductivity and anoxia would have resulted in elevated rates of organic matter burial that would have acted as an additional negative feedback on atmospheric pCO2 levels. Therefore, the enhanced weathering modulated by initially increased pCO2 levels would have operated as both a direct and indirect negative feedback to end the T-OAE.
The chemical weathering of rocks constitutes a negative and stabilizing feedback to Earth’s long-term (108–109 yr) climate by consuming atmospheric CO2, modulating the greenhouse effect and, in turn, global temperatures1,2,3. On these timescales, chemical weathering is dominantly regulated by tectonics, atmospheric pCO2, temperature, the lithology of materials being weathered, and the strength of the hydrological cycle3. Although the influence of weathering on long-term climate is well established3, much less is known about how this process potentially operates and influences climate on shorter times scales (<106 yr)4.
The T-OAE of the Early Jurassic Period constituted an ephemeral interval of global warming, perturbations in the global carbon cycle5, widespread oceanic anoxia6, and elevated marine extinction rates7. These environmental and ecological changes have been linked to the emplacement of the Karoo-Ferrar Large Igneous Province (LIP) and subsequent injection of greenhouse gases into the atmosphere8 (Fig. 1). Specifically, the addition of mantle-derived CO2 and thermogenic CH4 derived from the emplacement of the LIP9,10,11 and subsequent releases of CH4 from marine clathrates12, 13 and terrestrial environments14, 15 to the oceans and atmosphere are the proposed drivers of the T-OAE warming and carbon cycle perturbations. These perturbations are now recorded in sedimentary successions as pronounced negative carbon isotope excursions (CIEs), which occurred during a long-term trend to more positive carbon isotope values. This negative excursion is followed by a positive CIE thought to be the result of enhanced organic matter burial under anoxic conditions in marine and lacustrine environments5, 6. Collectively, these two carbon isotope excursions are used to stratigraphically define the T-OAE interval.
Under the enhanced greenhouse effect triggered by elevated levels of atmospheric greenhouse gases during the T-OAE, global temperatures would have increased and the hydrological cycle would have strengthened5. Rising pCO2, global temperatures, and precipitation rates would have led to accelerated weathering rates3. To investigate the proposition of accelerated weathering during the T-OAE, we have utilized osmium isotope (187Os/188Os) stratigraphy to reconstruct the 187Os/188Os composition of seawater over the event (see Supplemental Information).
The 187Os/188Os composition of seawater (187Os/188Ossw) reflects the sources of osmium to the ocean: rivers that drain continents (187Os/188Oscont ≈ 1.4) and aeolian dust (187Os/188Osaeol ≈ 1.04) represent a radiogenic end-member, and alteration of juvenile ocean crust or from the mantle (187Os/188Osm ≈ 0.12) and cosmic dust/bolides (187Os/188Oscos ≈ 0.12) represent an unradiogenic end-member16 (SI Fig. 1 and Supplemental Information). The flux of cosmic and aeolian dust represents a small fraction of the global input of osmium to the oceans and does not readily dissolve in seawater, and therefore does not appreciably affect the ocean’s 187Os/188Ossw composition16, 17. The present-day 187Os/188Ossw (~1.06) reflects the relatively greater input of continental-derived osmium to the ocean as compared to mantle-sourced osmium. Importantly, the short residence time of osmium in the oceans (~103–104 yr)18 permits the osmium isotope system to record ephemeral changes in global weathering patterns on the order of 103 to 105 years in the geological record19.
The 187Os/188Os compositions of organic-rich sediments are known to record the 187Os/188Os composition of contemporaneous seawater19, and serve as an archive of the past marine osmium isotope compositions. A previous osmium isotope study of the T-OAE interval from a sedimentary succession in the Cleveland Basin of Yorkshire, United Kingdom indicates that, during the event, there was a concomitant, transient increase of 187Os/188Ossw values by 0.720 (Fig. 2). This record was originally interpreted to be the result of an increase in continental weathering rates of 400 to 800%20. However, it has been suggested that these data reflect regional climatic changes where enhanced local runoff influenced the 187Os/188Ossw composition of the European epicontinental sea, which the Cleveland Basin was part of (Fig. 1), and therefore the 187Os/188Os record does not reflect a global weathering signal21. Key to this dispute is whether the Cleveland Basin was significantly hydrographically restricted so the local 187Os/188Ossw signal could be modified21, 22. A recently published osmium isotope record across the T-OAE from the Mochras borehole23, located in nearby Wales, displays a much less pronounced excursion of 0.4 during the T-OAE interval (Fig. 2), which further suggests that geochemical changes recorded in the Cleveland Basin were likely influenced by regional climatic and oceanographic dynamics18, 24, 25.
To resolve whether the transient increases in 187Os/188Os observed across the T-OAE were indeed a global signal, we have investigated the osmium isotope record from the Lower Jurassic Fernie Formation of the Western Canada Sedimentary Basin located in present-day western Alberta (Fig. 1). This new location was situated on the eastern margin of the ocean of Panthalassa and therefore was located in a different ocean basin from the previously studied Yorkshire and Mochras sites (Figs 1 and 2). Ammonite biostratigraphy and carbon isotope stratigraphy of the Fernie Formation at East Tributary of Bighorn Creek has identified the upper Pliensbachian to middle Toarcian interval and the T-OAE CIEs15, 26,27,28. Zircon U-Pb dates from two bentonites located near the base of the section also provide temporal constraint and an age model for the section (Fig. 3; see Methods and Supplementary Data). Importantly, the entire interval of the East Tributary succession contains organic-rich strata (2–8% TOC; Figs 1 and 3)15, and thus represents an ideal location to reconstruct the global 187Os/188Ossw over the T-OAE interval (see Supplemental Information).
187Os/188Osi record from North America
The high-resolution initial 187Os/188Os (187Os/188Osi) record of the East Tributary succession (see Supplemental Information) displays extremely unradiogenic values (187Os/188Osi ≈ 0.25) in the Pliensbachian and Lowest Toarcian, followed by a prominent radiogenic excursion (187Os/188Osi ≈ 0.6) during the Toarcian CIEs (Fig. 3). The 187Os/188Osi values decrease after the Toarcian CIE and asymptotically approach ~0.4 (Fig. 3; see Supplemental Information). Locally at East Tributary, aluminum and titanium concentrations increase 3-fold during the 187Os/188Osi excursion and remain high for the rest of the record (see Fig. 3 and SI Dataset 1), which suggests a local increase in the contribution of continentally derived materials during the event. However, their concentrations remain high as 187Os/188Osi values decrease after the Toarcian CIE, which suggests a minimal influence of a detrital component of rhenium and osmium to the osmium isotopic signature (see Fig. 3, Methods, and SI Dataset 1).
Comparison of Early Jurassic 187Os/188Osi records
Other marine 187Os/188Osi records from the Lower Jurassic (Hettangian through Toarcian stages) generally show unradiogenic values20, 23, 29, 30. These are likely related to relatively elevated inputs of unradiogenic osmium from the weathering of the Central Atlantic Magmatic Province (CAMP) and the alteration of juvenile oceanic lithosphere or direct injection of mantle-derived osmium from initial opening of the North Atlantic31. The Upper Pliensbachian portion of our record from northeastern Panthalassa has broadly similar values to those observed in the European epicontinental sea20, 23, 29, which suggests they are representative of the global 187Os/188Ossw values, and indicative of a well-mixed Early Jurassic ocean. Further, the East Tributary 187Os/188Osi record shows a similar pattern to the other available records during the interval that contains the T-OAE20, 23. All the sites record an excursion to higher 187Os/188Osi values that follow the falling limb of the Toarcian negative CIE. This trend is followed by a return to lower 187Os/188Osi values after the rising limb of the negative CIE. However, in all cases 187Os/188Osi declines to values slightly higher than those observed before the excursion.
While all the 187Os/188Osi records display a similar overall pattern, their 187Os/188Osi values differ. The Yorkshire and East Tributary datasets have similar 187Os/188Osi values before and after the T-OAE (~0.3 and ~0.4, respectively); however, the Yorkshire dataset shows an excursion to significantly more radiogenic values (187Os/188Osi ≈ 1) during the T-OAE20 (Fig. 2). The Mochras data show higher 187Os/188Osi values just before the T-OAE CIE (~0.4), which increase to an acme of 0.8 during the T-OAE, and decrease to ~0.3 after the event23 (Fig. 2). While the absolute 187Os/188Osi values differ between the sites, the magnitude of the excursions at East Tributary and Mochras are similar at 0.4, and are almost half the magnitude observed at Yorkshire (0.7).
The differences observed between the 187Os/188Osi records at East Tributary, Mochras, and Yorkshire suggest there were regional differences in 187Os/188Ossw during the studied interval. These differences likely represent local processes such as differing degrees of hydrographic restriction from the open ocean and the amounts of local runoff and its 187Os/188Os composition. However, the similarity in the magnitude of the excursions recorded at East Tributary and Mochras suggest this likely represents the global record of change during the T-OAE. This observation, coupled with the more extreme 187Os/188Osi excursion record at Yorkshire, supports the suggestion that the Yorkshire 187Os/188Ossw record was influenced by a local riverine input of radiogenic osmium during the T-OAE21, and the East Tributary and Mochras records are more representative of global osmium seawater chemistry
With these observations in mind, we advocate, when possible, analyzing osmium isotope records from coeval stratigraphic successions deposited in different sedimentary and ocean basins18, 24,25,26 before attempting to interpret them as a global signal. This methodology is especially important regarding palaeoceanographic studies on intervals older than the Cretaceous since the preserved records are predominantly from continental margin and epicontinental successions, where geochemical signatures have a greater potential to be modified by local processes.
Quantifying the Early Jurassic marine osmium cycle
To gain a more quantitative measure of the changes in the marine osmium cycle during the Toarcian we employed a numerical box model that simulates the osmium inventory of the ocean and its isotopic composition (see Supplemental Information). Specifically, we test whether the osmium isotope excursion associated with the T-OAE (~300–500 kyr in duration)31, 32 can be reproduced by a transient increase in the weathering input of radiogenic osmium to the ocean. We also explored other situations that may have potentially driven the observed T-OAE osmium isotope record, but are likely implausible, such as decreasing the input flux of mantle-derived osmium to zero (see Table 1 for values explored and Supplemental Information for a discussion of these cases). Overall, the numerical model results show that the osmium isotope excursion can be reproduced by a transient three- to six-fold increase in the input of continental-derived osmium to the oceans over 100 to 200 kyr31, 32 (Fig. 4; more details of the modelling results including sensitivity tests can be found in the Supplemental Information).
Changes in the 187Os/188Oscont to more radiogenic values through the differential weathering of lithologies such as shales and cratonic rocks33,34,35 could have played a role in the T-OAE osmium isotope record. We investigated the potential effect this change would have on the osmium budget during the event by running simulations where we elevated 187Os/188Oscont from 1.4 to 2 (see Supplemental Information for a discussion of the choice of the maximum 187Os/188Oscont value). In these simulations, a nearly three-fold increase of the input of continental-derived osmium to the oceans was still necessary to reproduce the excursion (Fig. 4), regardless of timescale used, and solely increasing 187Os/188Oscont to reasonable values cannot reproduce the observed excursion (see Supplemental Information). Given the plausible proposition of the changing composition of the continental weathering flux, we conservatively suggest that T-OAE weathering rates increased by as much as three-fold.
A potential source of radiogenic, continentally derived osmium was the remnants of the Central Pangaean Mountains, a Himalayan-scale mountain belt in eastern North America and northwestern Africa. This mountain belt was positioned at tropical and subtropical latitudes in the Early Jurassic (Fig. 1). The rifting of Pangaea during the Late Triassic and Early Jurassic would have exposed the core of the mountain range leaving this material open to weathering or erosion. General circulation models predict large increases in the air temperature and runoff during the T-OAE in the geographic region that contained these mountains36. These regional climatic changes would have facilitated enhanced chemical weathering, and makes this mountain belt a plausible source of the enhanced input of osmium to the oceans advocated here.
The weathering of organic-rich rocks and sediments would be another plausible way to raise the isotopic composition of the continental weathering flux, but also results in a net release of CO2 to the atmosphere37. However, enhanced continental runoff would also have increased nutrient delivery and stimulated primary productivity in aquatic environments leading to increased hypoxia, anoxia, and potentially euxinia5. Elevated burial of organic matter in these environments would have sequestered much more atmospheric CO2 than that associated with any black shale weathering, which we suggest represent only a fraction of the continental materials that were predominantly weathered during the event.
Differences in the osmium isotope response between OAE events
A striking feature of the 187Os/188Os records during the Mesozoic OAEs is the directionality of their excursions. The T-OAE records show a positive 187Os/188Os excursion, whereas the onset of the Cretaceous OAE 1a and OAE 2 both display negative excursions. The difference in the 187Os/188Os response to these events most likely lies in the environment where the LIPs were emplaced. The Cretaceous events are associated with subaqueous emplacements of the Ontong Java Plateau (OAE 1a) and the Caribbean and High Arctic LIPs (OAE 2). Emplacement of these LIPs would have supplied large amounts of unradiogenic, mantle-derived osmium directly into the oceans from weathering of basalts on the seafloor, resulting in osmium isotope excursions to nonradiogenic values25, 38,39,40.
The T-OAE, on the other hand, is associated with a subaerial emplacement of the Karoo-Ferrar LIP at high latitudes (Fig. 1), where the semi-arid climate would have made the relative weathering potential of this material low. In contrast to the younger OAEs, the Toarcian 187Os/188Osi records reflect enhancement of the weathering of continental materials facilitated by the injection of greenhouse gases into the atmosphere and subsequent climate changes. Notably, delivery of osmium from the Karoo-Ferrar LIP would have also been delayed, as compared to the Cretaceous LIPs. However, if weathering of the Karoo-Ferrar LIP was a significant source of osmium to the oceans during the T-OAE, then its lower 187Os/188Os compositions41,42,43,44,45 would necessitate an even greater contribution of continental material to generate the observed 187Os/188Osi excursion.
Implications and Conclusions
Based on the osmium isotope records and our modelling results, the transient increase in continental weathering rates during the T-OAE may be one of the largest observed during the Phanerozoic. Chemical weathering rates are also suggested to have significantly increased across the Permian-Triassic boundary46, Triassic-Jurassic boundary47, 48, and the Paleocene-Eocene Thermal Maximum49, all of which are associated with intervals of global warming, environmental deterioration, and extinction events50. The rapid response of the osmium isotope system during the T-OAE, as well as during other OAEs38,39,40, indicates that chemical weathering feedbacks may respond to episodes of rapid climatic warming on short timescales (103–106 years) and lead to a net drawdown of atmospheric CO2 5. Enhanced continental runoff would also have increased nutrient delivery and stimulated primary productivity in nearshore environments, leading to increased marine hypoxia, anoxia, and potentially euxinia5. CO2 would also have been sequestered through the deposition of organic-rich sediments in marine and lacustrine settings5, 6, 51.
In the case of the Toarcian OAE, increased weathering likely played a critical role in reversing the enhanced greenhouse state induced by Karoo-Ferrar magmatism. As atmospheric CO2 was consumed through these mechanisms, global temperatures would have declined5, 20. As modern atmospheric CO2 levels continue to increase at rates much higher than any point during the Cenozoic52, increased weathering, through the chemical and physical weathering feedbacks and stimulation of primary production and subsequent organic matter burial, may eventually act as a negative feedback to global warming, although on timescales much longer than what is necessary to mitigate the immediate environmental and ecological deterioration due to this warming53.
δ13C and total organic carbon analysis
δ13C and total organic carbon (TOC) were measured from each sample for rhenium, osmium, and trace metals (see below). The samples were prepared and analysed using the same methods from ref 15.
Rhenium and osmium isotopic analysis
In order to isolate primarily the hydrogenous rhenium and osmium from our samples, and minimize the removal of detrital rhenium and osmium, we followed the procedures of ref. 54. Between ~0.25 and 1 g of sample powder (dependent upon previously measured rhenium abundances via inductively-coupled plasma mass spectrometry) were digested with a known amount of 185Re and 190Os tracer (spike) solutions in 8 mL of a CrO3-H2SO4 solution; this reaction occurred in sealed Carius tubes, which were heated incrementally to 220 °C for 48 hours. The tubes were allowed to cool before opening. The osmium was immediately isolated and purified from the acid medium by solvent extraction using chloroform. This step was followed by the back reduction of Os from the chloroform into HBr. The Os fraction was further purified by micro-distillation. Rhenium was purified from the remaining CrO3-H2SO4 solution by a NaOH-Acetone solvent extraction55 and further purified using anion exchange chromatography. The purified Re and Os fractions were then loaded onto Ni and Pt filaments, respectively, and analysed for their isotopic composition using negative thermal-ionization mass spectrometry (NTIMS)56, 57 using a Thermo Scientific TRITON mass spectrometer with static Faraday collection for Re and ion-counting using a secondary electron multiplier in peak-hopping mode for Os. In-house Re and Os solutions were continuously analysed during the course of this study to ensure and monitor long-term mass spectrometry reproducibility. A 125 pg aliquot of the Re std solution and a 50 pg aliquot of DROsS yield 185Re/187Re values of 0.5983 ± 0.002 (1 SD, n = 6) and 187Os/188Os values of 0.16089 ± 0.0005 (1 SD, n = 8), respectively; both are identical to previously reported values57. The measured difference in 185Re/187Re values for the Re std solution and the accepted 185Re/187Re value (0.5974)58 is used for mass fractionation correction of the Re sample data. All Re and Os data are oxide and blank corrected. Procedural blanks for Re and Os in this study were 12 ± 3 pg/g and 0.07 ± 0.05 pg/g, respectively, with an 187Os/188Os value of 0.25 ± 0.15 (n = 4). The 187Re/188Os and 187Os/188Os uncertainties are determined through full propagation of uncertainties, including those in weighing, mass spectrometer measurements, spike calibrations, blank abundances and reproducibility of standard values.
Trace metal analysis
In order to compare the changes in [Re] and [Os] to sedimentation patterns across the T-OAE, we also analysed the concentrations of aluminum and titanium in each sample, which are used to estimate the contribution of terrigenous input to a sedimentary basin59, 60 (see Fig. 3 and SI dataset). Approximately 0.05 g of powder was added to a teflon beaker, followed by the addition of 4 mL of a 50:50 mixture of concentrated HCl and concentrated HNO3. This solution was placed inside a (CEM MARS 5) microwave assisted digestion system and run until all organic material had broken down at a temperature of 150 °C. The samples were then dried down and the silicates were dissolved using 4:1 HNO3 to HF, dried down, and re-dissolved in 5% HNO3 solution. A 100 μL solution split was spiked with an internal standard to measure elemental abundances using an Agilent 7500cs inductively-coupled plasma mass spectrometer in He and H mode. Internal standard was used to correct the samples for machine drift. International standards USGS SCO-1 and SDO-1 were also measured and had a reproducibility of ± 5%.
U-Pb analysis of zircons
CA-TIMS procedures described here are modified from refs 61,62,63. After rock samples have undergone standard mineral separation procedures zircons are handpicked in alcohol. The clearest, crack- and inclusion-free grains are selected, photographed, and then annealed in quartz glass crucibles at 900 °C for 60 hours. Annealed grains are transferred into 3.5 mL PFA screwtop beakers, ultrapure HF (up to 50% strength, 500 μL) and HNO3 (up to 14 N, 50 μL) are added and caps are closed finger tight. The beakers are placed in 125 mL PTFE liners (up to four per liner) and about 2 mL HF and 0.2 mL HNO3 of the same strength as acid within beakers containing samples are added to the liners. The liners are then slid into stainless steel Parr™ high pressure dissolution devices, which are sealed and brought up to a maximum of 200 °C for 8–16 hours (typically 175 °C for 12 hours). Beakers are removed from liners and zircon is separated from leachate. Zircons are rinsed with > 18 MΩ.cm water and subboiled acetone. Then 2 mL of subboiled 6 N HCl is added and beakers are set on a hotplate at 80°–130 °C for 30 minutes and again rinsed with water and acetone. Masses are estimated from the dimensions (volumes) of grains. Single grains are transferred into clean 300 μL PFA microcapsules (crucibles), and 50 μL 50% HF and 5 μL 14 N HNO3 are added. Each is spiked with a 233–235U-205Pb tracer solution (EARTHTIME ET535), capped, and again placed in a Parr liner (8–15 microcapsules per liner). HF and nitric acids in a 10:1 ratio, respectively, are added to the liner, which is then placed in a Parr high pressure device and dissolution is achieved at 220 °C for 40 hours. The resulting solutions are dried on a hotplate at 130 °C, 50 μL 6 N HCl is added to microcapsules and fluorides are dissolved in high-pressure Parr devices for 12 hours at 180 °C. HCl solutions are transferred into clean 7 mL PFA beakers and dried with 2 μL of 0.5 N H3PO4. Samples are loaded onto degassed, zone-refined Re filaments in 2 μL of silicic acid emitter64.
Isotopic ratios are measured with a modified single collector 354S (with Sector 54 electronics) thermal ionization mass spectrometer equipped with analogue Daly photomultipliers. Analytical blanks are 0.2 pg for U and up to 1.9 pg for Pb. U fractionation was determined directly on individual runs using the EARTHTIME ET535 mixed 233–235U-205Pb isotopic tracer and Pb isotopic ratios were corrected for fractionation of 0.25 ± 0.03%/amu, based on replicate analyses of NBS-982 reference material and the values recommended by ref. 65. Data reduction employed the excel-based program of ref. 66. Standard concordia diagrams were constructed and regression intercepts, weighted averages calculated with Isoplot67. Unless otherwise noted all errors are quoted at the 2-sigma or 95% level of confidence. Isotopic dates are calculated with the decay constants λ238 = 1.55125E-10 and λ235 = 9.8485E-10 (ref. 68) and a 238U/235U ratio of 137.88. EARTHTIME U-Pb synthetic solutions are analysed on an on-going basis to monitor the accuracy of results.
Five single zircon grains from the bentonite at −1.9 meters in the East Tributary section (see Fig. 3) were analysed by the uranium-lead chemical abrasion isotope dilution thermal ionization mass spectrometry technique (U-Pb CA-ID-TIMS). A weighted mean 206Pb/238U age of 188.58 ± 0.17 (0.25) [0.32] Ma, (MSWD = 0.89) is based on concordant and overlapping results for three of the analysed grains (see SI Dataset 2). Older results for the other two grains suggest that they are xenocrysts and/or contain inherited cores. It is important to note that this bentonite has a previously published multigrain U-Pb ID-TIMS age of 188.3 + 1.5/−1 Ma69.
Five single zircon grains from the bentonite at 2.35 meters in the East Tributary section (see Fig. 3) were analysed by the U-Pb CA-ID-TIMS technique. A weighted mean 206Pb/238U age of 185.49 ± 0.16 (0.25) [0.32] Ma, (MSWD = 1.17) is based on concordant and overlapping results for three of the analysed grains (see SI Dataset 2). Older results for the other two grains, one of which is discordant, suggest that they are xenocrysts and/or contain inherited cores.
Age model and calculation of 187Os/188Osi
The age model (see below) is constructed using a single grain U-Pb CA-ID-TIMS age of 188.58 ± 0.17 (0.25) [0.32] Ma from approximately two meters below the lowest interval with carbon isotope data in the East Tributary section15 and a single grain U-Pb CA-ID-TIMS age of 185.49 ± 0.16 (0.25) [0.32] Ma (see above) located at 2.35 meters in the section (see Fig. 3). Linear interpolation was used to calculate ages between the bentonites layers and between the age assigned for the Toarcian CIE. The onset of the CIE is placed at 183.1 Ma, with a total duration of 300 kyr31. Sedimentation rates are also assumed to remain constant after the Toarcian CIE. The initial osmium isotopic composition of the oceans (187Os/188Osi) was calculated using the following equation and the 187Re decay constant from ref. 70:
This equation accounts for the 187Os produced after deposition by the decay of 187Re. As stated above, the age component was derived from U-Pb ages from this succession (this study) and previously published dates for the age and estimated duration of the Toarcian CIE31. Furthermore, if a longer 500-kyr duration32 is assigned to the T-OAE CIE, the calculated 187Os/188Osi values do not change significantly and our interpretations do not change (see Supplemental Information).
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TRT would like to thank the Virginia Tech College of Science Roundtable grant committee for the Make-a-Difference Scholarship and the ExxonMobil/Geological Society of America, American Association of Petroleum Geologists, and International Association of Sedimentologists graduate student grant programs for funding (IAS grant funded the pilot study). A grant to BCG (EAR-1324752) and JDO (OCE-1624895) from the National Science Foundation also funded this work. DS acknowledges the Total Endowment Fund. Thanks to Dr. Joanna Hesselink, H. Lin, C. Wall, N. Moerhius, and T. Ockerman for laboratory assistance, and to Angela Gerhardt, Emma Tulsky, and Selva Marroquín for their help in collecting samples. Sample collections were authorized by the following permits: Parks Canada, Permit No: YHTR-2014-16156; RTMP, Permit No: 13-058, 14-009, 15-019. Finally, we would like to thank two anonymous reviewers whose comments greatly improved the manuscript.