Abstract
Correlation of stratigraphic sections from different continents suggests a worldwide interruption of carbonate sedimentation at the Triassic–Jurassic boundary, which coincided with one of the most catastrophic mass extinctions in the Phanerozoic. Both events are linked by a vulcanogenic maximum of carbon dioxide, which led to a temporary undersaturation of sea water with respect to aragonite and calcite and a corresponding suppression of carbonate sedimentation including non-preservation of calcareous skeletons. Besides the frequently cited climatic effect of enhanced carbon dioxide, lowering the saturation state of sea water with respect to calcium carbonate was an additional driving force of the end-Triassic mass extinction, which chiefly affected organisms with thick aragonitic or high-magnesium calcitic skeletons. Replacement of aragonite by calcite, as found in the shells of epifaunal bivalves, was an evolutionary response to this condition.
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Introduction
Various extrinsic factors such as volcanism (Stothers 1993; Pálfy et al. 2002; Pálfy 2003), asteroid impact (Olsen et al. 1987; Ward et al. 2001) and sea level changes (Hallam and Wignall 1999) have been proposed as potential causes of the end-Triassic mass extinction, one of the five major extinction events in the Phanerozoic. However, sea-level changes fail to explain the terrestrial biotic crisis (Beerling 2002; Pálfy 2003), and potential impact craters and ejecta deposits predate the extinction event by several million years (Walkden et al. 2002). By contrast, recent radiometric data corroborate that the eruptions in the Central Atlantic Magmatic Province (CAMP) were synchronous with the end-Triassic mass extinction (Pálfy 2003). The most frequently suggested link between CAMP-volcanism and mass extinction are rapid climate changes caused by volcanic outgassing of sulphur dioxide (SO2) and carbon dioxide (CO2; McHone 2003; Pálfy 2003). Total CO2 emission by CAMP-volcanism has been estimated at 5.19×1012 metric tons (McHone 2003), i.e. about twice the total of Recent (pre-industrial) atmospheric CO2. Additionally, a synchronous release of CO2 from dissociated gas hydrates has been postulated to explain a carbon isotope excursion toward light values at the Triassic–Jurassic (T–J) boundary (Pálfy et al. 2001; Hesselbo et al. 2002). Evidence for enhanced atmospheric CO2 has been found in reduced stomatal densities of land plants, which indicate that CO2 increased from 600 ppm to 2100–2400 ppm across the T–J boundary (McElwain et al. 1999). Even higher CO2 concentrations have been proposed on the basis of carbon isotope compositions of the Fe(CO3)OH component in pedogenic oolithic goethites, which suggest a rise up to 18 times of the modern partial pressure of CO2 (pCO2), i.e. up to 5,990 ppmv (Yapp and Poths 1996). Calculation of the influence of high p CO2 on the solubility of CaCO3 in T–J sea water is complicated by uncertainties about palaeo-temperatures and ancient concentrations of the various dissolved ions (in particular Mg2+/Ca2+ ratio). However, present-day sea water at a temperature of 25 °C would become undersaturated with respect to aragonite at p CO2=10−2.73 atm (1,860 ppmv) and with respect to calcite at p CO2=10−2.53 atm (2,950 ppmv; Stanley and Hardie 1998), thus within the same order of magnitude that has been suggested for CO2 concentrations at the T–J boundary. Temporary suppression of marine carbonate production was therefore a potential consequence of the CAMP-volcanism.
Stratigraphy of the T–J boundary
Few continuous marine sections allow a more or less precise biostratigraphic determination of the T–J boundary. That of Queen Charlotte Islands (Canada) shows a shift from calcareous to siliciclastic sedimentation earlier than the T–J boundary defined by radiolarians, but the lithological change is accompanied by the disappearance of monotid bivalves and by a preservation change from body fossils to shell impressions (Ward et al. 2001). Similarly, there is a shift from carbonate to siliciclastic dominated sedimentation immediately above the highest occurrence of Monotis in northeastern British Columbia, starting with a hiatus at the upper surface of the top Monotis -bed (McRoberts et al. 2001; Orchard et al. 2001). In the section of St. Audrie’s Bay, southwest England, the exact position of the T–J boundary is uncertain, but δ13C excursions toward light values are invariably correlated with decreasing carbonate content (Hesselbo et al. 2002).
More precise biostratigraphic data are available in the classical sections of the Alps and in the candidate global stratotype sections of Nevada and Peru. In the Kendelbach Gorge (Austria) of the Alps (Fig. 1A), the base of the Jurassic is formed by an “unusual thick shale” overlying the calcareous beds of the Late Triassic Kössen Formation (Hallam 1981). This unit, also known as “Grenzmergel” (boundary marl), is actually free of carbonate (Hallam and Goodfellow 1990). It extends over more than 800 km from the western border of Austria, here known as the “boundary beds” (McRoberts et al. 1997), to the Tatra mountains (Carpathians) in Slovakia, where the non-calcareous “boundary clay” forms the base of the Jurassic (Soták 2003). The carbonates that underlay this widespread horizon locally show fissures and cavities that were originally interpreted as the effect of faulting and subsequent dissolution of aragonite under influence of freshwater (Furrer 1993), but submarine dissolution as a consequence of high p CO2 may be an alternative interpretation. In the New York Canyon section (Fig. 1B), Nevada, USA, both biostratigraphy and geochemistry (negative δ13C excursion) place the T–J boundary at the base of a siliciclastic intercalation between calcareous units (Guex et al. 2003), which probably is the equivalent of the clay horizon of the Alps and Carpathians. The Chambara Formation near Chilingote, Peru, is presently the only fully calcareous succession where ammonoid finds allow a relatively precise determination of the T–J boundary (Hillebrandt 1994). The first Psiloceras is found in a horizon originally interpreted as a tempestite (Hillebrandt 1994), but a highly irregular base, a chaotic distribution of the fossils and the find of a reworked fragment of Choristoceras suggest that it is more likely a condensation horizon (Fig. 1C, D). The irregularity of the base resembles karstification but was obviously formed below sea level, because marine sedimentation continued in the siliciclastic Aramachay Formation, which is the landward equivalent of the Chambara Formation (Hillebrandt 1994). The discontinuity is therefore interpreted as a submarine dissolution surface that corresponds with the non-calcareous clay horizon that was simultaneously deposited in other regions.
In summary, the T–J transition is either found within a siliciclastic layer, which frequently marks an abrupt end of long-term carbonate sedimentation, or is represented by a hiatus in otherwise continuously calcareous sections. The concurrence of a worldwide interruption of carbonate deposition with a maximum in atmospheric CO2 that was potentially high enough to dissolve calcium carbonate minerals is strong evidence for a causal linkage. Recent estimates of the duration of the T–J CO2 maximum vary between >600,000 years (Hesselbo et al. 2002) and <100,000 years (Pálfy 2003). Taking standard sedimentation rates as starting point, a value near the lower extreme may be a good estimation of the time of duration, during which p CO2 was high enough to suppress carbonate sedimentation. The inability to find a global stratotype section that provides a continuous record of calcareous fossils, in particular ammonoids, is probably an inevitable consequence of this non-actualistic condition.
CaCO3 undersaturation of sea water and marine mass extinction
The effect of increased p CO2 on the carbonate saturation state of sea water and correlative consequences for carbonate secreting animals, in particular reef-forming corals, is of great interest for predictions of ecological and environmental changes associated with industrial CO2 release. Smith and Buddemeier (1992) suggested that even in supersaturated conditions, lowering of the carbonate saturation state could cause a decrease in calcification, a shift towards calcite secretors, and/or a competitive advantage for non-calcifying reef organisms. Kleypas et al. (2001) calculated that doubling the pre-industrial CO2 concentration in the atmosphere would decrease reef calcification by 14–30%, and they predicted that this drop would shift many reefs from net carbonate accumulation to net carbonate loss. Studies of extinction patterns of marine biocalcifiers during the time of the end-Triassic CO2 maximum may provide clues to test such assumptions, which can not be verified by direct observations because they deal with non-actualistic conditions.
Assessing the relevance of CaCO3 undersaturation of sea water for the T–J mass extinction requires a comparison between theoretically expected and actually observed effects. In sea water that is undersaturated with respect to calcium carbonate minerals, secretion of the least soluble polymorph would be a selective advantage because it requires the relatively lowest metabolic costs and provides the relatively highest resistance against dissolution. By contrast, organisms with aragonitic and high-magnesium calcitic skeletons are predicted to have suffered particularly high extinction rates, especially if their skeletons were thick. Replacement of aragonite by calcite is expected as an evolutionary response of animals that are pre-adapted to secrete both polymorphs, and size-reduction of the skeleton is a potential adaptation to the increased energetic costs for carbonate secretion.
Although it is not claimed that CaCO3 undersaturation was the only mechanism that promoted the T–J marine mass extinction, extinction of aragonite- or high-magnesium calcite-secreting organisms clearly stands out from more random extinction of other groups. Most striking is the sudden disappearance of previously flourishing reef communities (Stanley 1988) that were nearly exclusively composed of organisms with thick aragonitic and high-magnesium calcitic skeletons. Accordingly, all major groups of reef organisms suffered high extinction rates, in particular aragonite-secreting spongiomorphs, inozoid and sphinctozoid sponges, tabulozoans, disjectoporids, scleractinian corals and involutinid foraminifers as well as high-magnesium calcite-secreting solenopores and Tubiphytes (Stanley 1988; Stanley and Hardie 1998). The severity of the end-Triassic extinction event for reef organisms is also expressed by an unusual long lag phase and a very slow recovery that did not start before the Pliensbachian (Stanley 1988).
Apart from reef organisms, extinction took the heaviest toll on aragonite-shelled mollusks. Most adversely affected were the ammonites, with no fewer than six superfamilies becoming extinct and possibly no more than one genus surviving the boundary (Hallam and Wignall 1997). The progressive decline through the Rhaetian that preceded the final extinction of many families (Hallam 2002) might have made them particularly vulnerable for an end-of-period coup de grâce caused by CaCO3 undersaturation of sea water. The faunal turnover of gastropods is less well studied, but it has been proposed that it was even more pronounced than that at the end of the Permian (Batten 1973). Bivalves are worth a closer look because they are able to secrete both aragonite and low-magnesium calcite. Infaunal bivalves, which are invariably aragonite-shelled, were slightly more affected by the end-Triassic extinction event than epifaunal bivalves (McRoberts 2001), which frequently had partly calcitic shells. This pattern contrasts with higher extinction rates of epifaunal bivalves during the Triassic (McRoberts 2001), but any comparison between in- and epifauna might be inadequate because of the different chemical composition of pore and ocean water. However, epifaunal bivalve families that were particularly lightly affected by the end-Triassic extinction such as Ostreidae, Gryphaeidae, Plicatulidae, and Pectinidae, significantly enhanced the portion of calcite in their shell synchronous with the T–J CO2 maximum (Fig. 2A). The Megalodontoidea, which were the largest and most thick-shelled bivalves of the Late Triassic, retained their aragonitic shell but distinctly reduced their shell size (Fig. 2B). Yet, a strong decrease in their species diversity across the T–J boundary indicates that this strategy was less successful (Fig. 2B).
Replacement of shell aragonite by calcite at the T–J boundary was previously (Hautmann 2001a, 2001b) attributed to the shift from aragonite- to calcite-facilitating conditions in the oceans (Sandberg 1983). However, co-occurrence of calcitic and aragonitic ooides in the Rhaetian (Lakew 1990) and Liassic (Blomeier and Reijmer 1999) indicates that this transition was rather gradual, which is in contrast to the precise concurrence of shell mineralogical changes and the T–J boundary. Nonetheless, both phenomena may be linked: The end-Triassic CO2 maximum obviously suppressed precipitation of both aragonite and calcite but exerted the strongest influence on organisms that built their skeletons by the more soluble polymorph. The apparently undirected pattern of ooid mineralogy at the T–J boundary interval might have been caused similarly by pulses of lower CO2 emissions that preceded and followed the boundary maximum and solely inhibited aragonite precipitation. By contrast, long-term oscillations between aragonite and calcite sea were probably triggered by gradual shifts in the Mg2+/Ca2+ ratio, which led to the establishment of a stable “calcite sea” from the Middle Jurassic onwards (Stanley and Hardie 1998).
Conclusions
The lack of continuous fossiliferous sections across the T–J boundary has always been a major obstruction in analyses of the end-Triassic extinction event (e.g. Morante and Hallam 1996). Correlation of stratigraphic sections from Europe and North and South America demonstrates that this lack is attributed to a worldwide interruption of carbonate sedimentation at the T–J boundary, which includes the non-preservation of calcareous fossils. Its concurrence with the major volcanic activity of the Central Atlantic Magmatic Province and the corresponding atmospheric CO2 peak suggests a causal linkage between volcanism, suppression of carbonate sedimentation and the end-Triassic mass extinction event. The mediating factor of enhanced atmospheric CO2, which has repeatedly been suspected to have caused the end-Triassic mass extinction chiefly by extreme global warming (McElwain et al. 1999; Beerling 2002; Pálfy 2003), caused undersaturation of sea water with respect to aragonite and calcite and thereby suppressed carbonate deposition. Additionally, calcium carbonate undersaturation of sea water posed serious problems for marine carbonate secreting organisms that had to cope with raised energy expenditure for skeletal biomineralisation. This factor became critical for taxa with thick aragonitic and high-magnesium calcitic skeletons, which frequently failed to survive the T–J boundary. Size reduction and replacement of skeletal aragonite by calcite, as observed in several clades of epifaunal bivalves, were evolutionary responses to the non-actualistic chemical condition of sea water during the T–J transition.
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Acknowledgements
The manuscript benefited from comments by A. Freiwald, F.T. Fürsich, A. Hallam and J. Pálfy. A. von Hillebrandt kindly provided the photo of the T–J boundary in Peru (Fig. 1D). This paper is a contribution to the IGCP Project 458: Triassic–Jurassic boundary events.
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Hautmann, M. Effect of end-Triassic CO2 maximum on carbonate sedimentation and marine mass extinction. Facies 50, 257–261 (2004). https://doi.org/10.1007/s10347-004-0020-y
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DOI: https://doi.org/10.1007/s10347-004-0020-y