Following the latest Permian extinction ∼252 million years ago, normal marine and terrestrial ecosystems did not recover for another 5-9 million years. The driver(s) for the Early Triassic biotic crisis, marked by high atmospheric CO2 concentration, extreme ocean warming, and marine anoxia, remains unclear. Here we constrain the timing of authigenic K-bearing mineral formation extracted from supergene weathering profiles of NW-Pangea by Argon geochronology, to demonstrate that an accelerated hydrological cycle causing intense chemical alteration of the continents occurred between ∼254 and 248 Ma, and continued throughout the Triassic period. We show that enhanced ocean nutrient supply from this intense continental weathering did not trigger increased ocean productivity during the Early Triassic biotic crisis, due to strong thermal ocean stratification off NW Pangea. Nitrogen isotope constraints suggest, instead, that full recovery from ocean nutrient stress, despite some brief amelioration ∼1.5 million years after the latest Permian extinction, did not commence until climate cooling revitalized the global upwelling systems and ocean mixing ∼10 million years after the mass extinction.
The causes of delayed recovery of devastated marine and terrestrial ecosystems following the latest Permian Extinction (LPE, ∼252 Ma) are still debated1,2,3. Possible events triggering the biotic crisis and prolonged recovery during the Early Triassic4 might have been episodic pulses of volcanisms and/or a CO2-induced “hothouse” climate state with significant ocean redox perturbations that ultimately delayed the recovery of life1,3,4,5. The Early Triassic biotic crisis (ETBC, ∼252–247 Ma) corresponds to a relative palaeotemperature maximum albeit with short recovery episodes6 that was accompanied by an accelerated hydrological cycle and increased global weathering rates. Elevated continental weathering has been generally inferred from increased 87Sr/86Sr of marine carbonate7,8,9, and anomalously high sediment fluxes during the Early Triassic10,11. These inferences, however, are only derived from marine deposits and are thus indirect. The only direct evidence of enhanced continental weathering, although it stems from the direct aftermath of the LPE on terrestrial ecosystems, is from high-latitude paleosols (65°−85°S)12, massive soil erosion at low-latitudes (equator)13, and specific lithium and magnesium isotope signatures derived from Paleo-Tethys marine deposits1,14,15 (Fig. 1). From these studies, enhanced continental weathering during the Early Triassic has been proposed as an effective mechanism for excessive nutrient supply to the oceans, thereby leading to marine eutrophication, anoxia, and ecological perturbations. Onshore NW Pangea, direct evidence for enhanced continental weathering is absent (Fig. 1) and knowledge of the relationship between chemical weathering intensity, ocean response, and climate and ecosystem recovery during the Early to Middle Triassic is effectively not available. Hence, a better understanding of the timing and spatial distribution of continental weathering during the ETBC is of importance for Earth system models to single out the role of CO2 drawdown and marine anoxia during final climatic stabilization16,17.
Remnants of continental basement weathering on NW Pangea in a warm and humid climate are reported beneath Pleistocene glacial deposits at a few localities in Fennoscandia18,19,20,21,22,23. These terrestrial successions are significantly enriched in mature weathering products (i.e., kaolinite, gibbsite)18,20,21. The exact timing of this kaolinitization, however, remains elusive except in southern Sweden and Denmark where overlying Jurassic-Cretaceous cover rocks provide minimum age contraints for basement weathering22,23. Recently, Fredin et al.20 showed that large regions of southwestern Fennoscandia have potentially been subjected to intense continental weathering in Late Triassic time (ca. 220–200 Ma). Thus, evidence of enhanced continental weathering following the LPE is currently missing in Fennoscandia and elsewhere in NW Pangea (Fig. 1) implying that ocean response to continental weathering intensity and thus excessive nutrient supply can not be tested with the currently available data.
In this study, we characterize and directly date paleoweathering soils (saprolites) formed at the expense of crystalline basement rocks in northern Norway, along with two drill cores from offshore central Norway (Fig. 2). We report new data from chemically weathered rocks in crystalline granitoid basement occurring conformably below a 30 m (well 6408/12-U-01) to 170 m thick (well 6814/4-U-01; hereafter 6408 and 6814) Lower to Upper Jurassic sedimentary cover rocks offshore (Fig. 2)24. Onshore, we studied Archean granitoids in a drill core (BH3) from Andøya, northern Norway, that are intensively kaolinitized and occur conformably below a 212 m thick Middle to Upper Jurassic (Bajocian–Kimmeridgian) sedimentary cover25,26,27,28. We determined the age of weathering by K-Ar geochronology of authigenically formed K-bearing clay minerals separated from weathered basement rocks at all three investigated sites. We follow recent conceptual advances using K-Ar dating of clay as a valuable tool to date brittle fault rocks29,30,31,32,33 and weathering episodes20. Conventional K-Ar dating was used instead of 40Ar/39Ar dating, since the latter is affected by 39Ar recoil during sample irradiation34 and requires non-standardized corrections, making it less suitable for dating fine-grained clay minerals. We couple this geochronologically constrained evidence for continental weathering with evidence for elevated marine productivity and ocean stratification by examining a continuous Lower to Middle Triassic deep water section off NW Pangea with the aim to constrain changes in nutrient utilization at mid-paleolatitudes (∼40°N; Fig. 1). New nitrogen stable isotope (δ15N) data from Middle Triassic sections of Otto Creek, Sverdrup Basin, Canadian Arctic, are integrated with published Upper Permian to Lower Triassic bulk organic proxy data (TOC, δ13Corg, C/S ratio, δ15N) from Buchanan Lake35 and Smith and Otto creeks, Sverdrup Basin5,36. This new dataset helps to advance knowledge on the ocean response to enhanced continental weathering rates and ocean nutrient supply during “hothouse” climate conditions off NW Pangea. Analytical details are provided in the method section and supplementary online material.
Results and discussion
Evidence for continental weathering in central and northern Norway
The degree of weathering of crystalline bedrock from the studied off- and onshore wells was determined on unoriented powdered samples by X-ray diffraction (XRD) analysis, through major element composition using X-ray fluorescence (XRF) analysis and calculation of the chemical index of alteration (CIA)37 and other weathering indices (CIW: Chemical Index of Weathering38, PIA: Plagioclase Index of Alteration39, and WIP: Weathering Index of Parker40), in addition to mass-balance trends for major oxide depletion41 using Ti as an immobile index element42. XRD analysis of offshore wells 6408 and 6814 reveals a well-developed ∼5–10 m thick saprolite layer beneath Mesozoic sediments etching into the Paleo- to Neoproterozoic granitoid and gneissic crystalline basement with kaolinite content approaching 70% in the bulk fraction (Fig. 3 and Table S1). Less than 30 wt% of the bulk fraction consists of primary minerals (K-feldspar, plagioclase) (Table S1). The kaolinite is well-ordered as shown by the sharply developed peak triplet at 4.0–4.5 Å43 and may represent early diagenetic authigenesis44,45 (Fig. 3). Similarly, in situ kaolinitization of weathered Archean granitoids in Andøya BH3 is confirmed by the abundance of 32–36 wt% kaolinite in the bulk fraction with quartz being the dominant primary mineral (>50%) (Table S1). Mica clay minerals (i.e., illite) are a minor component (<11 wt%) in the bulk fractions. The Chemical Index of Alteration (CIA) in the weathered zone of all studied basement rocks increases upward from ∼70 to ∼96 (Table S2), thus constraining a gradual upward intensification of basement weathering as illustrated along an idealized SW-NE geological profile (Fig. 4a). Other weathering proxies (CIW, PIA, WIP) and the kaolinite content in the same samples corroborate this trend (Table S2). Furthermore, an A-CN-K plot (Al2O3, CaO + Na2O, K2O) suited for granitoid basement rocks37,46,47 (Fig. 4b) confirms this advanced weathering trend for both offshore and onshore wells, with a gradual enrichment of relatively immobile Al and distinct kaolinitization towards the top of the weathering zone (Figs. 3, 4b)48. Mass-balance trends in well 6814 support this interpretation of intense weathering by documenting distinct K- and Mg- (and moderate Fe-) depletion while Al remains largely constant48 except it becomes progressively concentrated towards the altered zone at the top of the section (Fig. 4c).
Age of weathering
Dating weathering processes by absolute isotopic methods remains challenging and is mainly focused on dating supergene K-Mn oxides by K-Ar and 40Ar/39Ar methods49. Due to the fact that weathering can indeed be part of a very long-lasting geological process, mostly integrated ages are reported49. Weathering processes can result in rock alteration from the surface down and may be documented by inverted age profiles, with the oldest ages at the top surface and more recently weathered rocks in deeper parts of the weathering column yielding younger ages. K-Ar age dating of authigenically formed illite applied to constrain weathering processes is a new approach, originally introduced by Fredin et al.20, and further discussed in the present study. This dating process relies upon different concepts than those of the classical mineral cooling models and Ar closure temperature50. Instead of a simple cooling model, authigenic clays in weathering zones can, after their initial formation, reflect additional weathering and recrystallization episodes. Each subsequent weathering event might then partially or fully reset the previously attained isotopic equilibrium between 40K and radiogenic 40Ar, resulting in a new “integrated K-Ar age”. Based on these complexities, the reported ages and errors of weathering events in the present study are larger than classical cooling isotopic ages and in the 2% range for authigenic illites (Table S3), but lower than the 7 to 18% errors for K-Ar ages of supergene K-Mn oxides49.
Our new K-Ar ages in all three sites on- and offshore Norway range from 374.3 ± 7.6 Ma to 221.5 ± 5.9 Ma (Table S3). “Age vs. grain size” plots of the dated samples define inclined curves (Fig. 5), where the finest grain size fractions (<0.1, 0.1–0.4 µm) invariably yield the youngest ages, and the coarsest fractions (2–6, 6–10 μm) the oldest. All the eight ages of the 2–6 µm and 6–10 μm fractions define a cluster with a weighted mean age of 353.0 ± 2.3 Ma. The ages of the finest fractions (<0.1, 0.1–0.4 µm) range between 310 ± 6.8 and 221.5 ± 5.9 Ma. In Andøya BH3, not enough material could be separated from the limited core material to date the <0.1 µm fraction (Table S3).
Following recent conceptual advances in the K-Ar dating of clays in saprolitic material and brittle faults20,29,30,31, we interpret the inclined curves of K-Ar ages in various grain size fractions as reflecting mixing between coarser protolithic or detrital illite/muscovite and the fine-grained authigenic K-bearing clay minerals that (neo)crystallized during deep weathering. Arguments in support of this interpretation, and thus of the reliability of the obtained geochronological results, derived from the characterization of the dated grain size fractions by XRD and TEM analysis.
XRD patterns display a dominance of characteristic triplets of kaolinite in the coarsest fractions (0.4–10 µm) at all sites (Figs. S1–4). This well-ordered nature of kaolinite is supported by its crystallinity index which was determined after both Hinckley (HI)51,52 and Liétard (R2)53,54. For both approaches, the two coarsest, quartz- and feldspar-free fractions have an index of 0.9 (HI) and 1.0–1.1 (R2), which is characteristic of a high degree of ordering. This leads to the assumption that kaolinite may have crystallized at an early diagenetic stage, possibly under acidic conditions44,45. In the coarsest fractions (2–6, 6–10 µm) at all sites, illite/muscovite is well-crystallized; its 10 Å peak is sharply defined with a CIS-standardized FWHM of <0.3 °2θ. Along with the presence of K-feldspar in the coarsest fractions, an enrichment in protolithic (inherited) minerals is indicated in Andøya BH3 and well 6814 (Table S1 and Figs. S1, S3). In support of this interpretation for Andøya BH3 comes the illite polytype analysis. It confirms the presence of the well-crystallized 2M1 polytype at 2.8 Å, interpreted as input from detrital muscovite, in both fractions with the oldest K-Ar ages55, but its absence in the 0.4–2 µm fraction, which yielded an intermediate K-Ar age (Fig. 5 and Figs. S3, S4). The 2M1 illite polytype is absent in the finer fractions in well 6408 as well (Fig. S2). The broadening of the smectite peak at 14Å towards the finer fractions (0.4–2 µm) may suggest intercalation of minor amounts of illite in well 640856 (Fig. S2).
As to the finest fractions (<0.1 µm, 0.1–0.4 µm), due to the lack of material, only material from well 6814 provided reliable XRD patterns, which indicate that kaolinite is the only clay mineral therein (Table. S1 and Fig. S1). Indeed, TEM analysis of the finest fractions confirms the presence of kaolinite with largely subhedral to euhedral sheet morphologies (Fig. 6). Still, the presence of finely dispersed K-bearing particles is evident from the TEM EDS spectra in well 6814 (Fig. 6). Analogous to what was reported from kaolinite-rich Brazilian soils57, these K-bearing phases may be interleaved in kaolinite crystals. Similarly, the finest fractions in well 6408 are largely composed of euhedral kaolinite minerals (Fig. 6). However, distinct K- and Mg-signals in the EDS spectra (Fig. 6) suggest that illite-intercalations within smectite contribute to the K-Ar ages of the finest fraction in well 6408. The finest fractions in Andøya BH3 contain authigenic illite with elongated euhedral particle edges (Fig. 6), which is also supported by the K signal in the EDS spectra.
The presence of K-bearing minerals within a matrix of largely subhedral to euhedral kaolinite minerals in the finest grain size fractions may suggest an authigenic crystallization during a more advanced stage of basement saprolitization. The uneqivocal identification of authigenic illite in Andøya BH3 supports this inference. Still, the finest fractions may include inherited protolithic minerals or different generations of authigenic phases reworked during multiple stages of the weathering process. K-Ar ages from the finest grain size fractions (<0.1 µm, 0.1–0.4 µm) should thus be considered as maximum ages, as studies from synkinematic brittle faults have shown29,30,31,58. Hence, we follow the conceptual approach outlined by Fredin et al.20 that the age of the finest fraction is taken as the best approximation of the (maximum) age of the weathering episode. This is because the finest fractions contain the highest amount of authigenic K-bearing minerals and the least of potential contaminating mineral phases derived from the protolithic weathered rock20,29,30.
A ca. 375–337 Ma age cluster (1) defined by seven ages of the coarsest fractions (2–10 µm) and one age in intermediate fraction (0.4–2 µm) (Fig. 7) corroborates the presence of well-crystallized illite (10 Å) and K-feldspar as well as the 2M1 illite polytype (Figs. S1–S4), implying that this age cluster reflects a significant protolithic or detrital component from the respective source rocks. A second cluster (2) between 310 and 292 Ma is constrained by three ages by the intermediate (0.4–2 µm) fraction and one single age by the fine-grained (0.1–0.4 µm) fraction (Fig. 7). While the 2M1 illite polytype was not identified in the intermediate grain fractions of well 6408 and Andøya BH3, well-crystallized illite peaks at 10 Å indicate a significant contribution from detrital components in this cluster (Figs. S2–S4) The ∼310 Ma age in the kaolinite-rich matrix of the fine fraction (0.1–0.4 µm) in well 6814 is enigmatic and we interpret the K-Ar age as the result of mixed assemblages of authigenic and protholitic detrital K-bearing minerals interleaved within the kaolinite crystals. A third cluster (3) between 264 and 248 Ma is defined by 3 ages in the 0.1–0.4 µm fraction and one age in the finest fraction (<0.1 µm), permitting the calculation of a weighted mean age of 254.1 ± 2.6 Ma (Fig. 7). The presence of authigenic illite with elongated euhedral particle edges in an otherwise dominated matrix of kaolinite in this cluster (Fig. 6) may suggest a significant proportion of authigenically derived K-bearing minerals. The youngest age in the dataset (221.5 Ma) occurs in the finest fraction (<0.1 µm) of well 6814. This fraction is solely composed of kaolinite without clear evidence of the origin of the interleaved K-bearing particles and represents the most mature weathering stage of all studied samples.
Despite these remaining uncertainties on the origin of the K-bearing minerals, the verified presence of K-bearing authigenic minerals within a matrix largely dominated by highly mature weathering products suggests that the range of K-Ar ages in the third cluster (Fig. 7) provides the maximum age of saprolitization at all sites. The majority of ages for enhanced saprolitization of exposed crystalline basement between the Late Permian and Early Triassic (∼254–248 Ma) is supported by inferences on a worldwide increase in sedimentation rates after the LPE10 that is attributed to a climate-driven increase in continental weathering1,14,15. Increased sediment supply likely as a consequence of intense weathering as shown by the present study is recognized from northern Fennoscandia59, Greenland and Spitsbergen60 and Ural mountains61 during the Permian-Triassic transition. The single Late Triassic age (221.5 ± 5.9 Ma) in the finest fraction (<0.1 µm) in well 6814 corroborate findings from southern Scandinavia (Ivö) where the weathered basement directly overlain by Upper Cretaceous sedimentary rocks yielded a maximum age of saprolitization of 221.3 ± 7.0 Ma20 (Fig. 7). Late Triassic ages (210–206 Ma) of saprolitization of a crystalline basement are also reported from Utsira High (North Sea), and from the island of Bømlo (SW Norway) (Fig. 7)20. It remains debatable whether continental weathering intensified both in southern and northern Scandinavia already during Norian times (∼227–209 Ma)62. Kaolinitic saprolites are inferred to have formed during warm and wet climatic conditions, preferably during Latest Triassic (Rhaetian) to Early Jurassic20,21,63. However, increased humidity of the Boreal realm has already been reported during Norian times64,65. The single Middle Permain age (∼264 Ma) in well 6814 remains enigmatic. A strong decline in seawater 87Sr/86Sr implies reduced continental weathering in central and northern Pangea, potentially fostered by dry climate and the absence of large orogens66. Indeed, the widely developed Middle Permian evaporites and calcretes indicate a semi-arid to arid climate in the tropical regions of Pangea implying the reduced potential of weathering of the granitic continental crust67,68. Whether the formation of weathering products can be linked to Emeishan flood volcanism during the Middle-Late Permian (∼262 ± 3 to 259 ± 3 Ma)69,70 remains uncertain.
Continental weathering and recovery from ocean nutrient stress
The new K-Ar geochronological data provide—within the given 1σ uncertainties (Table S3)—strong evidence for saprolitization and intense chemical weathering of NW Pangea during the Late Permian to Early Triassic (Fig. 8). Moreover, the near-complete transformation of the granitoid source rocks into authigenic kaolinite in two wells (Andøya BH3, 6408/12-U-01) with K-Ar ages between 249.5 to 248.1 Ma in the finest fraction (<0.1 µm), suggests intense weathering connected with a strong hydrological cycle under warm and humid climatic conditions during the ETBC (Fig. 8). The new evidence expands recent proxy (magnesium isotope) reconstruction for intensified chemical weathering of continental bedrock in the circum-Paleo-Tethys14 towards NW Pangea during the Early Triassic. To further test the ocean response to enhanced continental weathering and associated nutrient supply, we studied a complete Late Permian to Middle Triassic deep water record from Sverdrup Basin, Arctic Canada (Fig. 1), where a shale-dominated sediment sequence deposited in slope to distal shelf settings along the northwest margin of Pangea71. We examined new nitrogen isotope (δ15N) data, along with key bioproductivity (TOC), redox-sensitive (C/S ratio), and nutrient (P) proxies (Fig. 8)5,35,36 to study the impact of chemical weathering intensity onshore on nutrient availability and, thus, to produce new constraints on primary productivity offshore NW Pangea.
Generally, the oceanic δ15N signal depends on the isotopic composition of nitrate and the degree to which this inorganic nitrogen pool is utlized72. It records the combined isotopic signals of the inputs (mainly N2 fixation) and outputs (mainly denitrification) of fixed nitrogen to and from the ocean72,73. Previous studies have shown that records of δ15N in sedimentary organic matter are useful to examine changes in the oceanic nitrogen cycle off NW Pangea across the Late Permian to Early Triassic crisis5,35,36,74. The inference builds on the arguments that (1) there is little difference between the δ15N of the original OM and diagenetically produced NH4+ 75 (see methods for details) and (2) that postdepositional temperature changes exert negligible effects on sedimentary δ15N76.
Knies et al.35 reported that Late Permian high δ15N values (>9‰) off NW Pangea (Fig. 8) are consistent with water-column denitrification in continental margin upwelling zones. These changes in oxygenation are largely controlled by the recycling of nutrients delivered from enhanced continental weathering and high organic productivity as documented by our dated weathering profiles onshore and elevated TOC values offshore (Fig. 8). The progressive δ15N decline in the aftermath of the LPE has been interpreted as a decrease in nitrate availability in anoxic waters with a C/S ratio ≤1 (Fig. 8), shrinking the oceanic nutrient-N inventory that culminated in low ocean productivity (low TOC values) during the ETBC (Fig. 8)5. The related reduced nutrient supply to the surface caused significant nutrient stress in the photic zone with a prevalence of atmospheric N2-fixation as the major source for oceanic fixed nitrogen77,78. The latter is documented by δ15N values between ∼0‰ and −1‰ during the Early Triassic (Fig. 8). The inferred ocean stagnation off NW Pangea is paralleled by a rising nutrient inventory in the deep sea. This pool of inorganic nutrients in the deep ocean during periods of anoxia/euxinia during the Early Triassic79 was sustained by enhanced continental weathering as evidenced by our K-Ar ages of authigenically formed K-bearing minerals (Fig. 8) and elsewhere80. Indeed, the finding of identical quartz grains in both lower Triassic saprolites and overlying Mesozoic marine sediments in wells 6408 and 6814 (Fig. 9) argues for the continous ocean supply of nutrients from an exposed and chemically weathered crystalline basement front either by marine or fluvial erosion during the ETBC. Regional tectonic uplift and denudation of basement rocks on NW Pangea during the Early-Middle Triassic81 provided sufficient (sub)aerial exposure to sustain basement weathering under “hothouse” climate conditions. Our observations agree with an inferred lower pole-to-equator temperature gradient of 2 °C and higher global temperatures of 3–4 °C during the Early Triassic from climate system modeling3,82. This timing of enhanced continental weathering also agrees with the proposed intensification of global weathering rates, and increased warming-driven river runoff inferred from rising 87Sr/86Sr isotopic variations8 (Fig. 10).
However, unlike the Paleo-Tethys, where direct evidence for reduced ocean redox conditions were likely caused by increased continental weathering, high productivity and ultimately marine eutrophication1,14,83, the weathering on NW Pangea did not boost marine productivity in the adjacent Panthalassa Ocean as low TOC values indicate (Fig. 8)5,36. Instead, the rapid rise in ocean surface temperatures (Fig. 10) and eventually thermal stratification6 counteracted the potential eutrophication, and thus fully anoxic conditions. Meyer et al.84 suggested that the modeled estuarine-like circulation of the Paleo-Tethys acted as a nutrient trap implying a constant import of nutrient-rich deep waters with ongoing export of surface waters. The basinwide increase in nutrient levels with this nutrient-trapping ocean circulation may have caused widespread oceanic euxinia and hydrogen sulfide release to the atmosphere. In contrast, simulation results for the Panthalassa Ocean indicate a decline of Ekman-induced upwelling and thus reduced supply of nutrient-rich waters to the surface ocean during “hothouse” climate states3. Together with reduced cloud albedo and CO2-induced radiative forcing, the modeling results suggest that enhanced freshwater supply and warming of the polar sea surface led to a distinct thermo- and halocline, enhanced vertical stratification, and limited meridional overturning circulation3,82, in agreement with preferred atmospheric N2 fixation in surface water inferred from the nitrogen isotope data during the early Triassic (Fig. 10)5,35,36.
Our new δ15N data from Sverdrup Basin suggest that the predominance of diazotrophs as principle source for organic matter production offshore NW Pangea ended during the latest Anisian (∼242 Ma). While organic-rich phosphatic black shales during Anisian times are still characterized by a 15N content typical of newly fixed atmospheric N2 (∼0‰) due to replenished surface nutrients with low N:P ratio5 (Fig. 8), the progressive rise of N-isotopes from −1‰ to +3‰ during the Ladinian (∼242–237 Ma) (Fig. 8) suggests increasing upwelling of a partially denitrified water mass into the photic zone and subsequent utilization of various plankton groups. It marked the end of ocean stagnation with high nutrient inventories, as simulated for the LPE85, however, not yet tested for the Early to Middle Triassic. Our data of gradual recovery from ocean nutrient stress since the latest Anisian corroborate a period of atmospheric CO2 drawdown, reduced radiative forcing, and associated ocean cooling (Fig. 10) and reflect improved ocean mixing. With the upwelling of a partially denitrified, and thus δ15N-enriched, water mass into the photic zone, residual nitrate gradually replaced N2-fixing cyanobacteria as the primary N-source utilized by marine phytoplankton that fueled the biological activity. This allowed the full recovery of marine ecosystems with common reptile- and fish-dominated communities from the end of the Anisian4 (Fig. 10).
In conclusion, our direct evidence of chemical weathering intensity of basement rocks onshore NW Pangea in the aftermath of the LPE supports modeling experiments suggesting that volcanic-induced warming and high pCO2 stimulated continental weathering, and thus high nutrient supply to the ocean17,82. The widespread anoxia79, however, was not controlled by the surplus of nutrients and thus higher oxygen demand in the deep ocean due to higher export productivity, but rather by the stability of the thermal stratification of the ocean. The pool of additional nutrients from weathering continents was made available to massive organic matter production only when ocean mixing commenced again. Pre-LPE continental margin upwelling zones, however, were not established before the Early-Middle Ladinian, ca. 10 million years after the mass extinction, when deep water nutrients fuelled open-ocean marine productivity again.
Offshore and onshore material
Offshore well 6408/12-U-01 (64°10′13.3″N, 08°44′53.5″E) recovered in total 33.3 m of Lower Jurassic (Late Toarcian) sedimentary rocks and weathered crystalline granitoid basement on the Trøndelag Platform, central Norway24. The Jurassic sediments mainly consist of carbonaceous mudstone reflecting a transgressional development from non-marine to lower shoreface conditions. The underlying (unconstrained) granitoid basement is K-feldspar poor and intensively kaolinitized and indicates exposure under warm and humid climate conditons24. Well, 6814/04-U-01 (68°39′10.9″N, 14°11′08.9″E) off the Lofoten/Vesterålen islands recovered in total 168.6 m of Middle to Upper Jurassic (Early/Middle Bathonian – Kimmeridgian) sediments and weathered crystalline gneiss basement24. The gneiss in the basal part of the borehole (178.6–170.5 m) has been subjected to intensive kaolinite weathering and its parent composition is completely transformed into kaolinite at the boundary directly below the Jurassic sedimentary cover (Fig. 3). Unweathered gneiss at the base of the core is homogenous, foliated, gray-colored with small (<5 mm) augen of microperthitic feldspar and resembles Proterozoic mangeritic gneiss on the Lofoten-Vesterålen islands86. Onshore, Andøya Borehole 3 (BH3) (69°10′32.7″N, 16°0′38.9″E), recovered 225 m of Middle to Upper Jurassic (Bajocian–Kimmeridgian) sediments and weathered crystalline Archean granitoides28. The Middle to Upper Jurassic unconformity is located at 176.4 m. The granitoides below 212 m of sedimentary cover have been subjected to intensive kaolinite weathering and are generally clay-rich (40%)27.
X-ray diffractometry (XRD)
Bulk mineral assemblages of dried, homogenized powder (<20 µm particle size) and individual grain size fractions of wells 6408/12-U-01 and 6814/4-U-01 as well as Andøya BH3 (Tab. S1) were measured via X-ray diffraction (XRD) using a Bruker D8 Advance diffractometer with Cu Kα radiation and a Lynxeye XE detector at the Geological Survey of Norway, Trondheim. XRD scans were carried out for 3–75° 2θ and a step size of 0.02°. Signal acquisition time was 1 s per step. The optical system was equipped with soller slits (2.5°) and fixed divergence and anti-scatter slits (0.6 mm). Full quantification of the mineral assemblage of the bulk fraction was conducted via the QUAX full pattern method at the University of Bremen87. At NGU, mineral identification for different grain size fractions was carried out with Bruker’s Diffrac.EVA 3.1 using ICDD’s PDF4 Minerals as well as the Crystallographic Open Database. Quantification was performed with TOPAS and refined parameters included unit cell dimensions, sample displacement, preferred orientation as well as background coefficients. Limit of quantification and uncertainty is mineral-dependent, but commonly 1–2 wt% and 2–3 wt%, respectively. Illite crystallinity (Kübler Index) was determined from the full-width at half maximum (FWHM) of the 10 Å peak and standardized according to Warr88,89.
X-ray fluorescence (XRF)
Single samples (5cc) were analysed for major elements by using a PANalytical Axios sequential wavelength-dispersive XRF-spectrometer equipped with a 4 kW Rh X-ray tube at the Geological Survey of Norway, Trondheim. Loss on ignition (LOI) was determined after igniting 2–3 g finely-ground sample material for 1 h at 1000 °C. 4.200 ± 0.005 g Li2B4O7 was mixed with 0.600 ± 0.005 g pre-ignited sample and fused to glass beads at 1200 °C in Pt95/Au5-crucibles. Accuracy was tested with certified reference materials (CRM). The analytical uncertainty is an element- and concentration-dependent, but usually better than 5% rel. (2 σ). Please refer to the raw data in Table S2.
Scanning electron microscopy (SEM) and catholuminescence
SEM investigations were carried out on carbon-coated thin sections of wells 6408/12-U-01 and 6814/4-U-01 using an LEO 1450VP analytical SEM at the Geological Survey of Norway in Trondheim. SEM was applied to document kaolinite in a weathered basement (Fig. 3) and the microstructure of quartz in basement samples by backscattered electron (BSE) imaging (Fig. 9). SEM-catholuminescence (SEM-CL) images of quartz were obtained with a Centaurus BS Bialkali CL detector attached to the LEO 1450VP analytical SEM. The applied voltage and current were the same as for the SEM investigations (20 kV, ∼2 nA). The Bialkali tube has a CL response range from 300 (violet) to 650 nm (red). The detector sensitivity peaks in the violet spectrum range around 400 nm. SEM-CL images were collected from one scan of 43 s photo speed and a processing resolution of 1024 × 768 pixels and 256 gray levels.
Transmission electron microscopy (TEM)
Transmission electron microscopy (TEM) studies were conducted on all three studied wells at NTNU (Fig. 6). The sample powders were dispersed in isopropanol, ultrasonicated for 5–10 min, before a droplet was transferred to a holey, carbon-coated Cu TEM grid. TEM was performed with a double Cs aberration-corrected cold FEG JEOL ARM 200FC, operated at 200 kV. This TEM is equipped with a 100 mm2 (covering 0.98 sr solid angle) Centurio detector for energy-dispersive X-ray spectroscopy (EDS). EDS was performed by the acquisition of two-dimensional maps in scanning transmission electron microscopy (STEM) mode. The Cliff-Lorimer equation, by employing theoretical k-factors, was used for quantification of the chemical composition. Error estimates for the EDS quantifications are not included since the error bars due to counting statistics are negligible, while the systematic errors due to X-ray re-absorption are sample thickness and element dependent and vary from one location to another.
Laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS)
Trace element concentrations in quartz were determined by LA-ICP-MS (Fig. 9). The samples were prepared as surface-polished, 300-µm-thick sections mounted on standard glass slides. The analyses were undertaken with a double-focusing high mass-resolution sector-field (HR-SF) ICP-MS, model ELEMENT XR from Thermo Scientific, located at the Geological Survey of Norway in Trondheim. The instrument is linked to a 193 nm New Wave UP193FX ESI excimer laser probe. The laser parameters are provided in Table S4. A continuous raster or line ablation was applied. The carrier gas for transport of the ablated material to the ICP-MS was He mixed with Ar. The isotope 29Si was used as the internal standard, applying the stoichiometric concentration of Si in quartz. External standards applied for calibration are given in Table S4. Certified, recommended, and proposed values for these reference materials were taken from ref. 90. Each measurement comprised 15 scans of each isotope. An Ar blank was run before each reference material and sample measurement to determine the background signal. The background was subtracted from the instrumental response of the reference material/sample before normalization against the internal standard in order to avoid the effects of instrumental drift and memory between sample measurements. A weighted least squares regression model, including several measurements of the reference materials, was used to define the calibration curve for each element. Ten sequential measurements of the BAM No.1 SiO2 quartz glass were used to estimate the limits of detection (LOD) which were based on 3× standard deviation (3σ) of the ten measurements.
K-Ar dating of saprolite illite
All analytical details for the present study have been described by refs. 20,30. K-Ar dating was optimally performed on five clay size fractions (<0.1, <0.4, <2, 2-6, and 6–10 µm). For samples of wells 6408/12-U-01 (all fractions) and 6814/4-U-01 (<2 µm), K-Ar-analysis were conducted at CSIRO, Australia. K-analysis was done by atomic absorption spectrometry (AAS, Varian Spectra AA 50). For Ar analysis by noble gas spectrometry, sample splits were loaded into clean Mo foil, weighed and subsequently pre-heated to 80 °C overnight to remove moisture, and reweighted using a Mettler AT20 balance. The measured dry weight was used in the K-Ar age calculation. Once loaded into the gas purification line, the samples were pre-heated under vacuum at 80 °C for several hours to reduce the amount of atmospheric Ar adsorbed onto the mineral surfaces during sample handling. Argon was extracted from the separated clay mineral fractions by fusing samples within a vacuum line with an online 38Ar spike pipette. The isotopic composition of the spiked Ar was measured with a high sensitivity online VG3600 mass spectrometer. The 38Ar spike was calibrated against standard biotite GA155091. Blanks for the extraction line and mass spectrometer were systematically determined and the mass discrimination factor was determined periodically by air shots (Table S5).
K-Ar analysis of all fractions of Andøya BH3 and fractions 2–6, <0.4, and <0.1 µm of well 6814/4-U-01 was conducted at the Geological Survey of Norway following protocols outlined in ref. 31. Potassium was determined by fluxing clay samples in Li-tetraborate and digesting the resulting glass in HNO3 prior to analysis on a Perkin Elmer 5110DV ICP-OES. Argon concentrations were determined by weighing samples on a Mettler-Toledo XP26DR microbalance, and fusing in a Pond Engineering furnace at 1400 °C. The evolved gas was spiked with pure 38Ar, calibrated using HD-B192,93 and purified using a combination of SAES-GP50 (ST101) getters and a Titanium Sublimation Pump. Argon isotope intensities were measured using an IsotopX NGX multicollector noble gas mass spectrometer. Although the calibration standards used at NGU (HD-B1) are different from CSIRO (GA1550), 22 analyses of GA1550 at NGU yield a weighted mean age of 98.55 ± 0.07 Ma (MSWD = 1.18), which compares favorably to the published age of 98.5 ± 0.5 Ma94. The calibrations between both laboratories are thus comparable.
All K-Ar ages were calculated using 40K abundance and decay constants recommended by Steiger and Jäger95. The pooled error of duplicate K determination on all samples and standards is better than 2%, whereas the error for Ar analyses is below 1%. The age uncertainties take into account the errors during sample weighing, 38Ar/36Ar and 40Ar/38Ar measurements, and K-analysis. K-Ar age errors are within 1σ uncertainties.
Stable nitrogen isotopes
For the stable nitrogen isotope analyses, we studied a composite section of (1) Late Permian from Buchanan Lake35, (2) Early Triassic from Smith Creek (Smithian stratotype)5, and (3) Middle Triassic from Otto Creek (this study). The three locations from Sverdrup Basin, Arctic Canada have similar shale-dominated sedimentation in slope to distal shelf settings at mid-paleolatitudes (∼40°N)71. Total N and δ15Ntot were analysed on homogenized sub-samples by elemental analyser isotope ratio mass spectrometry (EA-IRMS) on an ANCA-GSL/20-20 system (Europa Scientific, Crewe, UK). Approximately 20% of the samples were analyzed in duplicate with a mean standard deviation of 0.16‰. δ15Ntot data are reported as standard δ-values per mil (‰ vs. air). A KOBr-KOH treated aliquot in pre-selected samples measures the amount of inorganic nitrogen (IN) and its isotopic signature (δ15Ninorg)35 representing the amount of NH4+ fixed within the clay lattice96 (Table S6 and Supplementary Data 1). We observe nearly identical δ15Ninorg (mean 3.07‰) and δ15Ntot (mean 2.79‰) values with a covariance of 0.95 and a significant covariation between TOC and TOC/IN ratio (R2 = 0.8) suggesting an organic origin for the IN. All geochemical proxy data for the middle Triassic Otto Creek profile are reported in Table S7 (Supplementary Data 2).
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We thank the Norwegian Petroleum Directorate for accessing the offshore borehole material. We are grateful to Atle Mørk for supporting the sample party. We acknowledge Andrew Todd (CSIRO) and Ruikai Xie (NGU) for the K-Ar geochronological work. The research is funded by the Research Council of Norway (grants #319849 and #223259).
Open access funding provided by UiT The Arctic University of Norway (incl University Hospital of North Norway).
The authors declare no competing interests.
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Knies, J., Schönenberger, J., Zwingmann, H. et al. Continental weathering and recovery from ocean nutrient stress during the Early Triassic Biotic Crisis. Commun Earth Environ 3, 161 (2022). https://doi.org/10.1038/s43247-022-00480-z
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