RESEARCH
Thomas J. Algeo
Professor of Geology
University of Cincinnati
Biocrisis at the Permian/Triassic Boundary: Causes and Consequences
The mass extinction at the Permian/Triassic boundary (PTB) was the largest biocrisis in Earth history, eliminating ~90% of marine species and ~70% of terrestrial species (right; Sepkoski, 2002). Eruption of the Siberian Traps flood basalts is regarded as the most likely cause of this crisis (Renne et al., 1995; Korte and Kozur, 2010), but the manner in which volcanic outpourings devastated the environment and biosphere is uncertain. I am investigating changes in environmental conditions in marine PTB sections having a global distribution, with the goal of better understanding the causes and consequences of this biocrisis. |
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The PTB mass extinction resulted in major changes in marine ecosystems. At Meishan (upper right), benthic marine faunas were sharply reduced in diversity, abundance, and range of ecological tiering from the Late Permian to the Early Triassic (Benton and Twitchett, 2003). The extinction event was broad, affecting many clades including calcareous algae, foraminifera, radiolarians, and others (lower right). Patterns of post-crisis recovery vary widely: some clades quickly exceeded their pre-crisis diversity levels (e.g., ammonoids), others were permanently reduced (e.g., brachiopods), while yet others went extinct in the aftermath of the crisis (e.g., bellerophontid gastropods). During the Early Triassic, some clades (e.g., bivalves and gastropods) exhibited a pronounced reduction in average size, termed the "Lilliput effect" (Twitchett, 2007). These ecosystem changes were accompanied by large fluctuations in marine carbonate d13C values (right; Payne et al., 2004), indicating major perturbations to the global carbon cycle for several million years during the Early Triassic. The summary figure at lower right is from Algeo et al. (2011a). |
Late Permian Early Triassic
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Despite decades-long study of the Permian- Triassic boundary, there are relatively few integrated, high-resolution chemostratigraphic datasets for marine sections that can address critical questions related to, e.g., the extent, intensity, and timing of deep-ocean anoxia, patterns of oxygen-minimum zone (OMZ) expansion and/or upwelling of toxic deep- ocean waters onto shallow-marine shelves and platforms, marine-terrestrial teleconnections, and the relationships of these events to the delayed recovery of Early Triassic marine biotas. My research program has generated integrated chemostratigraphic datasets for marine sections around the world in order to address these questions (map at right with sections numbered; adapted from Algeo et al., 2012a). | |
Earlier studies inferred that almost the
entire global ocean went anoxic during the PTB crisis (Wignall and Twitchett,
1996, 2002), and that deep-ocean anoxia commenced as early as the early Late
Permian, ~8 million years before the PTB mass extinction (Isozaki,
1997). These inferences are not in accord with the results of my
recent studies.
First, deep-sea sections from Japan show evidence of only limited changes in redox conditions on the deep seafloor (i.e., <2X increases in the concentrations of redox- sensitive elements in the Early Triassic black shale facies relative to the Late Permian gray chert facies; upper right, Algeo et al., 2010 and 2011b). In contrast, there is a huge (>6X) increase in the burial flux of S related to the appearance of pyrite framboids in the black shale facies (lower right). I inferred that the framboids were forming high in the water column, for example within the OMZ, rather than close to or below the seafloor. This inference is in accord with paleoceanographic models for the PTB (Kiehl and Shields, 2005; Winguth and Maier-Reimer, 2005; Winguth and Winguth, 2012). |
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Second, the timing of changes in ocean redox conditions during the Late Permian-Early Traissic has been extensively debated. While small changes may have occurred in advance of the PTB crisis, U isotope analysis of the Dawen (China) section demonstrates that a major shift toward more reducing conditions occurred at the level of the mass extinction horizon (Brennecka et al., 2011). This study showed that d238U shifted rapidly from ca. -0.40‰ to ca. -0.65‰ (upper right). Mass balance calculations indicate that this shift is consistent with expansion of the anoxic sink for U by a factor of ~6X (from 10% to 60%; lower right). A synchronous shift in Th/U ratios from ~0.1 to ~0.6 is also consistent with a ~6X drawdown of U in seawater (upper right). These results demonstrate that the most important changes in ocean redox conditions were concurrent with the mass extinction event. | |
These findings suggest a major expansion of
the oceanic oxygen-minimum zone (OMZ) during the PTB crisis. Expansion
of the OMZ during the latest Permian is supported by recent analyses of
radiolarian faunas in deepwater sections of the Nanpanjiang Basin (South
China). At Dongpan, all families of radiolaria exhibit steep declines
in diversity and abundance about 2 meters below the PTB mass extinction
horizon (upper right; Shen et al., 2012a). This pattern indicates that
deepwater biota were affected by an expanding OMZ about 100kyr prior to the
main extinction event (lower right). That radiolarian were affected by
a rising chemocline rather than by stresses imposed from the ocean surface
is demonstrated by the observation that the albaillellarian family,
representing the deepest dwelling radiolarians, went completely extinct at
this time, whereas the relatively shallower-dwelling families (Latentifistularia,
Spumelaria, and Entactinaria) declined but did not disappear (upper right).
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Expansion of the oceanic OMZ during the Late Permian is implied also by biotic changes in the Sverdrup Basin of Arctic Canada. Sections in this region such as West Blind Fiord exhibit an abrupt extinction of siliceous sponges (the main biota of the Late Permian Sverdrup Basin), termed the "Arctic extinction event" (AEE) (Algeo et al., 2012b). Through detailed conodont correlations, my colleague, Charles Henderson of the University of Calgary, was able to show that the AEE is older than the latest Permian mass extinction (LPME) horizon in Tethyan PTB sections (Yin et al., 2012). The implication of this finding is that marine environmental stresses were felt earlier at high northern paleolatitudes than in the equatorial latitudes of the Tethys Ocean, possibly because of large-scale volcanic ash deposition or moderate pre-crisis climatic warming that disproportionately affected high-latitude regions (Algeo et al., 2011a). | |
These insights regarding expansion of the oceanic OMZ during the latest Permian help to make sense of biotic and geochemical changes at the LPME in shallow-marine sections. PTB sections such as that at Nhi Tao (Vietnam) accumulated on the top of a carbonate platform in the Nanpanjiang Basin at water depths of a few meters to tens of meters (right; Algeo et al., 2007a, 2008). Such sections commonly show an abrupt extinction horizon that coincided with (1) a ca. 3‰ negative excursion in carbonate d13C, (2) appearance of framboidal pyrite (S spikes) that is 34S-depleted, and (3) near- complete loss of TOC (cf. Algeo et al., 2012a). This pattern is consistent with episodic upward movement of sulfidic deepwaters, possibly via the chemocline upward excursion mechanism of Kump et al. (2005), with the first such event resulting in decimation of benthic biotas and near-sterilization of shallow-marine habitats. | |
Another facet of my PTB research focuses on terrestrial-marine "teleconnections", i.e., fluxes of material between terrestrial and marine systems that might have played a role in marine environmental changes during the PTB crisis. An analysis of sediment fluxes revealed a nearly global increase in sediment accumulation rates during the earliest Triassic (right; Algeo and Twitchett, 2010). This increase is observed in both carbonate and siliciclastic facies in shallow-marine areas, owing to a higher flux of dissolved and particulate weathering products from continents, but not in deep-ocean areas that were far from continents and below the paleo-CCD (carbonate compensation depth). Increased continental weathering rates were probably due to a combination of higher surface temperatures, acid rainfall, and generally disturbed terrestrial landscapes (cf. Looy et al., 1999, 2001). | |
The findings above allow development of a revised model of relationships between the Siberian Traps flood basalt eruptions and the terrestrial and marine environmental-biotic crises (upper right, Algeo et al., 2011a; see Wignall, 2001, for original version of flowchart). Massive eruptions triggered strong warming through release of volcanic CO2 and possibly also thermogenic methane following magmatic intrusions into the West Siberian Coal Basin (lower right). A combination of higher surface temperatures, acid rainfall, and generally disturbed terrestrial landscapes led to an increased flux of weathered material to shallow-marine areas. This flux included excess nutrients that locally stimulate marine productivity, which, in combination with warming-induced water-column stratification, resulted in a rapid expansion of the oceanic OMZ during the latest Permian. These conditions persisted, or recurred episodically for ~2 million years during the Early Triassic, resulting in a delayed recovery of terrestrial and marine ecosystems. | |
Work now in progress will address additional
important issues related to the Permian-Triassic boundary crisis, including:
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References
Algeo, T., and Twitchett, R., 2010. Anomalous Early Triassic
sediment fluxes due to due to elevated weathering rates and their biological
consequences. Geology, v. 38, p.
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Last updated 17 Sept 2012