Permian-Triassic Extinction Event Notes

PERMIAN-TRIASSIC

Permo-Triassic Mass Extinction

  • Also known as:
    • Permian-Triassic Extinction Event
    • End-Permian Mass Extinction (EPME)
    • The Great Dying
    • P-T

Extinction

  • Extinction happens continuously (background extinction).
  • Background extinction rate: 0.110.1-1 extinctions per million species per year.
  • Current extinction rate: 1001000+100-1000+ times higher than the background rate (estimates vary).

Causes of Extinction

  • Major causes:
    • Habitat loss
    • Climate change
  • Other contributing causes.
  • Past causes of habitat loss and climate change: geological factors.
  • Modern causes:
    • Overharvesting
    • Pollution
    • Invasive species

Extinction Risk

  • Some species are more at-risk due to specific characteristics.
  • Conversely, some species are normally less at-risk due to opposite characteristics.
  • Mass extinctions disrupt the "rules" of background extinction risk.

Mass Extinction

  • High amount of extinction: 3030% + of species.
  • Affects a broad range of habitats or ecologies.
  • Global in nature.
  • Occurs over a short time period/abrupt change.
  • Rate is considerably higher than background rates.

Mass Extinctions

  • Affects approximately 305030-50% of marine families.
  • Examples:
    • End-Ordovician
    • Late Devonian
    • End-Permian (Permo-Triassic)
    • Late Triassic
    • Cretaceous-Paleogene
  • Smaller extinctions can still have a global signal.

Causes of Mass Extinction

  • Each mass extinction event is unique.
  • Multiple interacting mechanisms.
  • No single common cause for all mass extinctions.

General Causes

  • Sea level drop:
    • Reduces shallow shelf photic zone habitat
  • Cooling or warming:
    • Changes sea level
    • Impacts organisms adapted to climate
    • Affects ocean oxygenation
  • Anoxia

General Causes (Continued)

  • Flood basalts:
    • Disrupt climate (cooling from "volcanic winter" or warming from greenhouse gases).
    • Contribute to anoxia
  • Impact events:
    • "Impact winter" (disrupt photosynthesis).
    • Widespread fires
    • Possibly acid rain

The Big Five Extinctions

  • Includes Ordovician-Silurian (OS), Late Devonian (D), Permian-Triassic (P), Triassic-Jurassic (Tr), and Cretaceous-Paleogene (K-Pg) extinction events.
  • The graph illustrates the extinction rate correlated with extent and rate of temperature change

End-Permian Extinction

  • Largest mass extinction in Earth's history.
  • Approximately 6060% of genera and 8080% of species extinct.
  • Terminal Paleozoic mass extinction.
  • End of the Middle Permian (terminal Guadalupian, ~10 million years before EPME) was a large extinction (~35% of marine genera); likely had land impact too.
  • Terminal Permian: 2 pulses.
  • Affected terrestrial and marine organisms.
  • First of the "Big 5" to include terrestrial organisms.

P-T mass extinction losses

  • Forams: 97% of genera
  • Radiolarians: 99% of genera
  • Cnidarians: 96% of genera
  • Bryozoan: 79% of genera
  • Brachiopod: 96% of genera
  • Bivalve: 59% of genera
  • Gastropod: 98% of genera
  • Ammonoids: 97% of genera
  • Crinoids: 98% of genera
  • Trilobites: 100% of genera
  • Eurypterids: 100% of genera
  • Acanthodians: 100% of genera

Totally Extinct

  • Rugose and tabulate corals (all hard corals at the time).
  • Trilobites.
  • Blastoid echinoderms.
  • Acanthodians.
  • Pelycosaur synapsids, 20 families of therapsid synapsids
  • Reefs and forests disappeared temporarily.

Upper Permian vs. Early Triassic

  • Reefs were destroyed.
  • No burrowing.
  • Corals did not return until the Middle Triassic.

Environmental Changes

  • Forests and plant ecosystems destroyed
  • Coal formation stops
  • Red beds common across boundary

Causes and contributing factors to the Permian Extinction

  • Large continent = dry interiors; increasingly arid climate.
  • Evidence: fossil dunes, extensive evaporite deposits.
  • Low sea level and loss of shallow marine habitat.
  • Poor ocean circulation due to warming and changed currents (no cold water sink at poles).
  • Widespread anoxia.
  • Disrupts nutrient cycling.

Siberian Traps

  • Approximately 2,000,000km32,000,000 km^3 of flood basalts.
  • Global cooling from ash cloud.
  • Global warming from CO2CO_2 release.
  • Possibly burned extensive coal deposits in this area.

Ocean Warming and CO2CO_2 Problems

  • Trap volcanism produced massive amounts of CO2CO_2.
  • CO2CO_2 levels in ocean increased (hypercapnia) and poisoned marine life (ocean less oxygenated, more acidic).
  • Support: heavily calcified organisms suffered huge losses; likely unable to form their shells correctly.

Environmental consequences of the Siberian Traps eruptions

  • SO2 emissions, CO2 emissions, thermogenic methane.
  • Increased continental weathering, soil erosion, global warming, oceanic anoxia.
  • Increased marine productivity, disturbed landscapes.
  • Negative C-isotope excursion, positive C-isotope excursion, increased seawater 87Sr86Sr\frac{^{87}Sr}{^{86}Sr}, faster Sr reaction rates.
  • Abundant microbial growth, acid rain, siltation, eutrophication.

Methane Clathrates

  • Methane is a powerful greenhouse gas.
  • Significant amounts stored frozen in ice crystals on seafloor (gas hydrates).
  • If oceans warm enough, it can release through melting.
  • Global warming catastrophe
  • New estimates of ~500-2500 PgC in gas hydrates

Synthesis of Events

  • Volcanic eruptions.
  • Moderate global warming.
  • Methane release catastrophe.
  • Abrupt global warming.
  • Ocean anoxia.
  • EXTINCTIONS