Abstract
One of the most severe extinctions of complex marine life in Earth’s history occurred at the end of the Triassic period (~201.4 million years ago). The marine extinction was initiated by large igneous province volcanism and has tentatively been linked to the spread of anoxic conditions. However, the global-scale pattern of anoxic conditions across the end-Triassic event is not well constrained. Here we use the sedimentary enrichment and isotopic composition of the redox-sensitive element molybdenum to reconstruct global–local marine redox conditions through the extinction interval. Peak δ98Mo values indicate that the global distribution of sulfidic marine conditions was similar to the modern ocean during the extinction interval. Meanwhile, Tethyan shelf sediments record pulsed, positive δ98Mo excursions indicative of locally oxygen-poor, sulfidic conditions. We suggest that pulses of severe marine de-oxygenation were restricted largely to marginal marine environments during the latest Triassic and played a substantial role in shallow-marine extinction phases at that time. Importantly, these results show that global marine biodiversity, and possibly ecosystem stability, were vulnerable to geographically localized anoxic conditions. Expanding present-day marine anoxia in response to anthropogenic marine nutrient supply and climate forcing may therefore have substantial consequences for global biodiversity and wider ecosystem stability.
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Main
The Triassic/Jurassic boundary interval (TJB, ~201 million years ago) is marked by one of the largest extinctions of complex marine life in Earth’s history: the end-Triassic mass extinction event (ETME)1. The ETME has been closely associated with supraregional volcanism from the Central Atlantic Magmatic Province, which has been linked to atmospheric carbon injection as evidenced through Triassic–Jurassic negative carbon isotope excursions2. Central Atlantic Magmatic Province activity is also thought to have caused Triassic–Jurassic marine acidification and marine de-oxygenation2,3. Studies of Triassic–Jurassic marine biomarkers and δ34S (where the delta notation (δ) is defined as the difference in isotopic ratio between a sample and a reference standard) indicate that locally sulfidic conditions were prominent within marginal marine surface waters of the Tethys and Panthalassa oceans around the TJB3,4,5,6,7,8. Oxygen-poor conditions have been further identified from blooms of prasinophycean algae3,9, a negative excursion in carbonate uranium isotopes10,11, widespread Early Jurassic black-shale deposition9,12, elemental redox proxies3,13 and iron speciation data14. Therefore, recent studies suggest that marine redox change may have played an important role in end-Triassic marine extinction phases. However, most existing Late Triassic redox studies are at a local, basinal or sub-regional scale and do not provide information about the global-scale distribution of marine redox conditions. The unconstrained areal extent of globally sulfidic conditions during the ETME limits understanding of the spatial complexity of redox change as a driver of Late Triassic marine extinctions.
The isotopic composition of molybdenum (Mo) in organic-rich sediments has been widely used to reconstruct the oxygenation of both local and global ancient marine environments15,16. Under oxic depositional conditions, Mo typically exhibits low sedimentary enrichments and isotopically light compositions, due principally to (Mn)oxyhydroxide adsorption, with compositions ~3‰ lighter than coeval seawater16,17,18. Under reducing conditions, Mo exhibits higher sedimentary enrichments due to the formation of thiolated (poly)molybdate species that have smaller isotopic offsets from seawater than Mo adsorbed onto oxyhydroxides19,20. Generally well-oxygenated global marine conditions are therefore reflected by isotopically heavy δ98Mo seawater values due to oxyhydroxide adsorption acting as the primary vector of Mo burial21. However, isotopically light Mo burial can also occur due to intermediate thiomolybdate formation22. High sulfidic global marine conditions, by contrast, are represented by isotopically light δ98Mo seawater values as global oxyhydroxide burial declines21, but no observations of δ98Mo evolution exist from across the TJB and ETME.
In this Article, we use the sedimentary enrichment (MoEF) and isotopic composition of Mo to examine the link between marine de-oxygenation and extinction during the ETME. We obtained material from the Carnduff-2 core (Northern Ireland), Hebelermeer-2 core (west Germany) and Schandelah-1 core (north Germany), which preserve lithological records of marine marls, sandstones and organic-rich shales deposited on the Tethyan shelf before, during and after the ETME (Fig. 1). All three sites have undergone previous stratigraphic study and include detailed biotic records for correlation6,23,24,25. The samples analysed in this study are therefore ideally suited to explore the relationship between marine extinction and de-oxygenation on the Tethyan shelf across the TJB. We identify little correlation between proxies for detrital sediment input and δ98Mo or MoEF and therefore interpret stratigraphic variations in Mo concentrations mainly as a function of local redox conditions (Supplementary Fig. 4).
Limited euxinia during Triassic–Jurassic transition
The δ98Mo of coeval seawater (δ98MoSW) must be resolved to determine global redox conditions. However, to determine δ98MoSW, sedimentary δ98Mo values must be corrected for isotopic fractionation, with the isotopic fractionation and sedimentary enrichment of Mo being dependent on local redox conditions21. The maximum δ98Mo compositions of Upper Triassic mudstones in the studied cores are ~1.6‰ (Carnduff-2: 1.56‰; Hebelermeer-2: 1.63‰; Fig. 2). These δ98Mo values are obtained from sampling levels where trace-metal distributions are indicative of suboxic depositional conditions (Supplementary Figs. 1–3)13. Suboxic conditions coinciding with upper-bound Carnduff-2 δ98Mo values are further supported by oxic–ferruginous iron speciation values from a correlative horizon within the Larne Basin14. Molybdenum sulfides forming in sedimentary porewaters underlying a non-euxinic water column are fractionated by a minimum of ~0.7‰ relative to coeval seawater26,27, with fractionation probably exceeding 0.7‰ within the Larne Basin because of local redox conditions13,14. Burial of Mo under ferruginous conditions would lead to sediment compositions with similar isotopic offsets from δ98MoSW and so would not alter this conclusion28. Therefore, Late Triassic δ98MoSW was probably >2.3‰, similar to or greater than modern-day seawater29. A Late Triassic δ98MoSW equal to or greater than the modern ocean is consistent with sulfidic conditions covering no more than ~0.05–0.10% of the Late Triassic seafloor, similar to or even less than in the modern day16,29.
The average upper-bound δ98Mo throughout the basal Jurassic of the Carnduff-2 core is 1.47 ± 0.58‰ (n = 3) and characterizes horizons with trace-metal distributions that are indicative of localized suboxia13. Predominantly non-euxinic conditions from the basal Jurassic of the Larne Basin are further supported by iron speciation data14. Therefore, basal Jurassic δ98MoSW was probably >2.2‰, also similar to the Late Triassic and modern global ocean. The persistence of a similar δ98MoSW from the Late Triassic to the basal Jurassic suggests that, unlike uranium isotope records10,11, there was no substantial change in the global Mo cycle across the TJB and that sulfidic anoxia in the Early Jurassic global open ocean remained spatially limited. Our conclusion is further supported by pyrite framboid data from an open ocean Panthalassa site30.
Regional de-oxygenation during the ETME
Oxygen-poor conditions were present across Tethyan and Panthalassa marginal marine environments during the main extinction interval5,7,13,14. Such conditions have been further identified here on the basis of δ98Mo and MoEF data with redox conditions varying according to both site and stratigraphy. The Schandelah-1 and Carnduff-2 cores both exhibit positive δ98Mo shifts that directly coincide with the main extinction interval, as denoted by the ‘initial’ negative carbon isotope excursion (CIE)2,31,32 (Fig. 2). The increase in δ98Mo (and MoEF) during the main extinction interval indicates an increased availability of reduced sulfur [HS−], probably due to the shoaling of the sulfate reduction zone within sedimentary porewaters up to the sediment–water interface26,27,33. Relatively high MoEF alongside low δ98Mo values around the base of the main extinction interval within the Hebelermeer-2 core also indicates increased [HS−] prevalence, probably due to the expansion of the sulfate reduction zone into the water column, with the burial of intermediate thiomolybdate species at H2S concentrations <11 µM (refs. 20,22) (Supplementary Information section 1.4). Isotopically light values are inconsistent with oxide adsorption given the elevated total sulfur (%) at this horizon6. Sulfidic conditions around the base of the initial CIE at St Audrie’s Bay (Somerset, UK) have been interpreted through a positive δ34S excursion4.
Low sulfate within Late Triassic seawater of the Tethyan shelf has been interpreted through δ34S data7. Low marine sulfate concentrations7 are unlikely to have affected broad trends in δ98Mo observed here given the inter-site consistency in data and the argument that calculated sulfate concentrations in Late Triassic oceans (0.2–1.1 mM) were still in excess of those required for thiomolybdate formation up to and exceeding ~11 µM (refs. 7,16) (Supplementary Information section 1.5).
Pulsed marginal marine euxinia during ETME
Multiple pulses of marine sulfidic anoxia were prevalent on the Tethyan shelf during the latest Triassic and earliest Jurassic. Low to moderate MoEF as well as isotopically heavy δ98Mo in all three cores during deposition of the basal Westbury Formation and stratigraphically equivalent units are suggestive of shoaling of the sulfate reduction zone towards the sediment–water interface26,27,33. Similar shoaling of the sulfate reduction zone is also inferred from the Carnduff-2 and Hebelermeer-2 cores during the deposition of the uppermost Westbury Formation and equivalent units. Both phases of porewater de-oxygenation coincided with photic-zone euxinia on the Tethyan shelf during the middle Rhaetian6 (Fig. 3); the upper pulse also coincided with episodic photic-zone euxinia within the Bristol Channel Basin8 and de-nitrification within the Central European Basin at the Mingolsheim and Mariental-1 sites3,34 (Fig. 3). δ98Mo then decreases during the deposition of the lower Cotham Member and stratigraphically equivalent units, as seen within both the Carnduff-2 and Schandelah-1 cores, with MoEF decreasing or remaining low. Despite previous studies interpreting broadly oxygenated depositional conditions during the basal Cotham Member, isotopically light δ98Mo within the Larne Basin may be associated with intermediate thiomolybdates and organic matter preservation, suggesting weakly oxygen-poor conditions22,35.
Multiple further positive shifts in δ98Mo and MoEF are observed within the basal Jurassic of the Carnduff-2 core, suggestive of pulsed increases of [HS−] caused through periodic shoaling of the sulfate reduction zone. Correlative horizons within the Schandelah-1 core contain δ98Mo and MoEF shifts also indicative of variable shoaling of the sulfate reduction zone. Pulsed oxygen-poor conditions within the basal Jurassic of the Carnduff-2 and Schandelah-1 cores coincided with photic-zone euxinia within the Bristol Channel Basin4,8 (Fig. 3).
Periodically pulsed anoxia during the Late Triassic and Early Jurassic has previously been noted on the basis of eccentricity modulated precession timescales in the Bristol Channel Basin (St Audrie’s Bay), with laminated organic-rich black shales forming every precession cycle36. Pulses of marine redox change have also been reported from the Larne Basin, coinciding largely with the disappearance of infaunal bivalve taxa13. We similarly note a close relationship between redox pulses and Late Triassic extinction phases (Fig. 3).
Localized marine euxinia as driver of extinction during ETME
The coincidental pulsed nature of sulfidic marine de-oxygenation and end-Triassic marine extinction phases strongly suggests a causal relationship (Figs. 3 and 4). However, the limited extent of marine sulfidic anoxia through the TJB inferred from our new Mo isotope datasets suggests that these pulses of marine de-oxygenation were limited largely to marginal marine environments. More persistent and widespread oxygen-poor conditions towards the end of the ETME have been suggested from carbonate δ238U data that have been modelled to suggest uranium reduction across ~8–20% of the global seafloor10,11. However, such anoxic conditions probably manifested within marginal marine and intermediate-depth Tethyan and Panthalassa environments3,4,5,7, with little evidence for open marine de-oxygenation30, and provide limited information on the extent of sulfidic conditions. Our new Mo isotope data add to these observations by showing that even if moderate de-oxygenation (enough to perturb the uranium cycle) took place near the ETME, there was little increase in the volume of waters containing dissolved sulfide. We suggest that geographically localized sulfidic marine de-oxygenation within Late Triassic marginal marine environments therefore had major implications for Late Triassic biodiversity and ecosystem stability.
Our inference of geographically localized marine de-oxygenation is consistent with recent studies indicating elevated weathering and erosion rates in Tethyan shelf localities during the Late Triassic37,38. Localized marine de-oxygenation may have been driven by high run-off from the Late Triassic continents triggering eutrophication and stratification, with increased run-off driven by a warming climate, enhanced hydrological cycle and the collapse of forest ecosystems leading to enhanced soil erosion39. Marine de-oxygenation within Tethyan and Panthalassa marginal marine environments may also have been associated with the expansion of oxygen minimum zones5,7. Open marine environments would have been substantially less affected by weathering perturbations, with oxygen minimum zone expansion potentially being focused around intermediate-depth, marginal marine environments, and consequently the open oceans may have remained refugia for marine life.
Modern marginal marine environments are probably also particularly sensitive to changes in marine redox while also being some of the most biodiverse oceanic environments on Earth40,41,42,43. Therefore, anthropogenically driven environmental change, including the local expansion of marine anoxia and enhanced marine nutrient supply, may result in geographically localized marine de-oxygenation, which could have major consequences for future marine biodiversity and ecosystem stability44, with particularly severe consequences for marginal marine corals, mangroves and coastal fishes1,42,43.
Methods
Bulk inorganic geochemistry
From each sample, 50 mg was digested using inverse aqua regia (3/1 HNO3/HCl) followed by digestion of silicates in 1/2 HF/HNO3. Major elemental concentration data were measured using Perkin Elmer Optima 3300RL inductively coupled plasma atomic emission spectroscopy, and minor elemental concentration data were measured using Perkin Elmer NexION 350D inductively coupled plasma mass spectrometry. Accuracy was determined using full procedural digests of MAG-1 (n = 7) and was ±2.5% with Mo within uncertainty of the certified value. Precision was calculated using the 2 s.d. of the MAG-1 digests as ±17% (Cr, Cu, Zn, Al ±<10%), as well as five digests of an in-house mudrock standard (PERN-1) as ±21%. The MoEF was determined using ((Mosample/Alsample)/(Moucc/Alucc)). Upper continental crust concentrations were taken from ref. 48.
Molybdenum concentrations and isotopes
Samples were processed and measured under trace-metal-clean laboratory conditions. Before molybdenum-isotope analysis, each sample was weighed and mixed with a 97Mo–100Mo double-spike solution and digested in 3/1 HNO3/HCl. The Mo samples were separated from matrix elements and interferences using an anion exchange column procedure detailed within refs. 49,50. The δ98/95Mo compositions were measured using Thermo Scientific Neptune Plus multicollector inductively coupled plasma mass spectrometry. Procedural blanks for Mo were between 0.5 and 5.0 ng. All δ98/95Mo data were calculated relative to NIST SRM 3,134 + 0.25% (ref. 51). Accuracy and precision were assessed using the Open University Mo solution standard (compare ref. 52) (−0.35 ± 0.15‰, n = 12, 2 s.d.) and multiple separate digests of USGS SDO-1 shale, which yielded an average δ98/95Mo of 1.04 ± 0.08‰ (2 s.d., n = 6) within uncertainty of published values (1.05 ± 0.1‰) (ref. 52).
Data Availability
All data generated or analysed during this study are deposited in the Zenodo online repository and can be accessed via the following link: https://doi.org/10.5281/zenodo.8319867.
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Acknowledgements
We thank the Geological Survey of Northern Ireland (GSNI), particularly R. Raine, for providing access to the Carnduff-2 core. We also thank M. Blumenberg for generously providing the Hebelermeer-2 core material. We appreciate the help of J. Brakeley (RHUL) and P. Holdship (Oxford) for their assistance with ICP-MS and ICP-AES measurements. This work was funded through a NERC DTP PhD Studentship awarded to A.D.B. (NE/L002485/1). M.R. acknowledges financial support from the National Natural Science Foundation of China (grant no. 41888101).
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A.J.D., A.D.B. and M.R. designed the research. M.R. sampled the Carnduff-2 core at the GSNI core repository. B.v.d.S. and R.B. provided access to material from the Schandelah-1 core. A.D.B. carried out elemental and isotopic geochemical analyses with assistance from A.J.D. A.D.B. and A.J.D. interpreted the data with assistance from M.R., R.B. and B.v.d.S. A.D.B. wrote the paper and designed the figures. All authors contributed to the text and figure amendments.
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Bond, A.D., Dickson, A.J., Ruhl, M. et al. Globally limited but severe shallow-shelf euxinia during the end-Triassic extinction. Nat. Geosci. 16, 1181–1187 (2023). https://doi.org/10.1038/s41561-023-01303-2
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DOI: https://doi.org/10.1038/s41561-023-01303-2
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