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Mass Extinctions




  I.G. Kenyon
Mass Extinction - Definition
A significant proportion of
 species become extinct
 (between 30% and 95%)

  The extinctions operate
   across a wide range of
environments and lifestyles

  The extinctions occurred
 rapidly (over a few million
years) and were due to one
  or more physical factors
5 Major Mass Extinctions
  identified since the Cambrian
  Extinction Event     Date of Extinction

End of Ordovician    443 Million years ago
Late Devonian        375 Million years ago
End of Permian       251 Million years ago

End of Triassic      200 Million years ago

End of Cretaceous     65 Million years ago
The 5 Major Mass Extinctions

    Gaps between extinctions vary from 51 Ma
    to 135 Ma with an average gap of 94.5 Ma
Extinctions During the Phanerozoic




The Phanerozoic is from 542 Ma (Cambrian) to the present
Diversity Curves through the Phanerozoic




                          End Triassic Mass Extinction
                         possibly caused by submarine
                         volcanism associated with the
                              break up of Pangea
End of Ordovician Mass Extinction – 443 Ma
      70% of marine species became extinct
Tropical faunas badly affected especially coral reefs




         Main groups affected Trilobites,
        Graptolites, Echinoids, Brachiopods
Late Devonian Mass Extinction – 375 Ma
A series of events that lasted around 10 Ma




Cephalopods, Fish and Corals most affected
End Permian Mass Extinction – 251 Ma
The largest mass extinction event removing 95% of
    marine species and 50% of marine families

       Trilobites, Cephalopods, Bryozoans,
           Corals, Crinoids badly affected




    Major faunal and floral overturn on land
    Marks the boundary between dominance
     by the Palaeozoic and Modern Fauna
End Triassic Mass Extinction – 200 Ma
     Multiple event mostly affected the land
     where over 95% floral species eliminated




Around 30% marine species became extinct – mainly
 reef dwellers, Ceratites, Brachiopods and Bivalves
End Cretaceous Mass Extinction – 65 Ma

    Around 70% of all species wiped out
Dinosaurs, Reptiles, Ammonites, Belemnites,
    Brachiopods, Bivalves, Foraminifera
Causes of Mass Extinctions
     Supercontinent Formation
      Extra-Terrestrial Impacts
       Flood Basalt Eruptions
Methane Hydrates and Global Warming
 Rapid and Major Glaciation Events
Supercontinent Formation
                   Pangea formed at the
                    end of the Permian

              Resulted in fewer continental
              shelves and lack of habitat for
                shallow marine organisms

               Coincided with huge decline
                in the numbers of shallow
                      marine species

               Caused rapid fluctuations in
                climate, unstable weather
              patterns and extreme aridity in
               the interior of the land mass
Supercontinent Formation
             A single continent reduces the
              input of nutrients to oceans
                from rivers and estuaries

             This decreases the amount of
             nutrients available for shallow
               water marine life and may
              have also altered the salinity
Supercontinent Formation
  A supercontinent positioned
  close to one of the poles can
    initiate major glaciations

   Glaciation causes sea levels
 to fall and there is a significant
   reduction in shallow water
      marine environments

 A supercontinent located over a
pole can also lead to the coverage
  of the Earth in ice, a condition
    known as ‘Snowball Earth’
Extra-Terrestrial Impacts
   Asteroids 1 km diameter strike the Earth every 500,000 years




 Large collisions with 5 km diameter
asteroids occur approximately about
     once every 10 million years       The last known impact of an object of
                                        10km diameter or larger was 65Ma
Extra-Terrestrial Impacts

 Local destruction of habitats – impact
 blast, shockwave, ignition of wildfires




Billions of tonnes of debris injected into the
atmosphere resulting in rapid global cooling
Extra-Terrestrial Impacts

Impact in the sea – billions of tonnes
  of water vapour injected into the
atmosphere resulting in a greenhouse
   effect and rapid global warming
Flood Basalt Eruptions

   Eruptions last between 0.5 and 2.0 million
  years and can erupt enough basalt to cover
the whole of the USA to a depth of a kilometre

         Local destruction of habitats
          and initiation of wildfires
Flood Basalt Eruptions
                             Billions of tonnes of
                             carbon dioxide and
                          sulphur dioxide released
                            into the atmosphere
                              during eruptions

  Both are powerful
greenhouse gases and
will contribute to very
rapid global warming
Flood Basalt Eruptions
  When it rains the sulphur dioxide will come
 back down to Earth dissolved in rainwater and
the acid rain will kill vegetation on a large scale




  With vegetation dying, all food chains will
be affected and also the oceans may become
acidified with disastrous effects on marine life
Methane Hydrates in Ocean Floor Sediments
Large volumes currently locked into ocean floor sediments
      Stable under low temperatures of deep ocean
Methane Hydrates in Ocean Floor Sediments
         Global warming may result
        in deep ocean temperatures
          rising and the release of
         large volumes of methane
           from ocean sediments

          The rapid release of large
          amounts of methane into
         the atmosphere will result
            in highly accelerated
               global warming
Methane Hydrates in Permafrost
Glaciations-Possible Causes




    Supercontinents positioned
in high latitudes/close to the poles

 Milankovitch cycles: Precession,
    Obliquity and Eccentricity
Glaciations-Effects on Ecosystems




             Loss of habitat as ice masses grow
    Could eventually lead to ‘Snowball Earth’ scenario
     Contraction of climatic belts towards the equator
Global cooling, decreased productivity of primary producers
End Cretaceous Mass Extinction – 65 Ma




A large asteroid or meteorite (10km in diameter)
   collided with the Earth 65 million years ago
Evidence - Asteroid Impact Location




Location of possible impact site discovered on
 the Yucatan Peninsula in Mexico at Chixulub
       The impact structure is a circular
    depression about 180 km in diameter
Evidence for Asteroid Impact Location
A




                                     B

A. Gravity survey onshore and offshore of the Yucatan Peninsula
  B. 3D map of gravity and magnetic field variations reveals the
Chicxulub crater, now buried beneath tons of sediment. This view
   is looking down at the surface, from an angle of about 60°.
Evidence – The K-T Boundary Layer
                   The presence of a thin 2cm
                    layer of iridium-rich clay
                    found all over the world
                    within sedimentary rocks

                     The K-T Boundary Layer
                   dates the same everywhere
                      at 65.5 Ma +/- 0.3 Ma

                      Iridium is a transition
                   element, rare on Earth but
                       found in meteorites.

                     First proposed by Luis
                         Alvarez in 1980
Evidence – Shocked Quartz

               Shocked quartz is found
              worldwide, in a thin layer
              at the boundary between
            Cretaceous and Tertiary rocks.


           It was first discovered at nuclear
            testing sites and later in craters
            caused by meteorite impacts as
              at the Barringer Crater near
              Flagstaff, Arizona in the USA
Evidence – Shocked Quartz
     Shocked quartz has a
     microscopic structure
different from normal quartz.

Under intense pressure, but
relatively low temperature,
 the crystalline structure of
  quartz is deformed along
  planes inside the crystal.

    These planes, which
  show up as lines under a
   microscope, are called
planar deformation features
 (PDFs), or shock lamellae.
Evidence – Tektites (Glass Spherules)
                                 Tektites (from Greek
                              tektos, molten) are natural
                                glass rocks up to a few
                                  centimetres in size.

                              Most scientists agree they
                              are formed by the impact
                                of large meteorites on
                                    Earth’s surface.
 Tektites (Glass Spherules)
from 1 to 8 mm in diameter
                              Tektites are black or olive-
  are found within a radius
                               green in colour and their
  of 600 to 1,000km of the
                              shape varies from rounded
 Chixulub Crater in Mexico
                                  to quite irregular.
Evidence – Soot from Wildfires




 The K-T Layer has high concentrations of carbon in many locations,
 suggesting that the asteroid impact may have generated wildfires.

Large areas of vegetation would have been destroyed in a short time,
   soot fell to Earth and was incorporated into sedimentary rocks
Evidence – Tsunami Deposits
               It is thought that the asteroid
              impact occurred in the sea and
               initially produced a crater 100
                  km wide and 30 km deep

                This would have displaced
              vast volumes of seawater and
                 generated a series of very
               large tsunamis possibly over
                   100 metres in height

                 The tsunamis would have
              travelled great distances inland,
               and in Texas at Waco there are
             large-scale sedimentary deposits
              thought to be of tsunami origin.
Evidence – Tsunami Deposits
                The tsunami deposits in
            Waco, Texas are thought to be
             from the waves generated by
            the        K-T asteroid impact.

            The sediments are estimated to
             have been deposited at least
            300km inland by the tsunamis!
Animation to show Impact of a large asteroid with the Earth




The impactor's estimated size was about 10 km in diameter
 and is estimated to have released 4×1023 joules of energy,
  equivalent to 100,000,000 megatons of TNT on impact.
Origin of the K-T Asteroid




  Results published in 2007 suggest that the impactor that
  wiped out the dinosaurs and other life forms on Earth 65
 million years ago can been traced back to a break-up event
in the main asteroid belt more than 100 million years earlier.
Flood Basalt Eruptions 66 Ma – The Deccan Traps
    Erupted mainly over a period of 30,000 years
   Over 2000 metres thick and cover 500,000 km²
     May have originally covered 1,500,000 km²
     Caused a global drop in temperature of 2°C




  The term Trap is derived from the Dutch for stairs
   and refers to the step-like landscape of the area
That’s All Folks!

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Massextinctions

  • 1. Mass Extinctions I.G. Kenyon
  • 2. Mass Extinction - Definition A significant proportion of species become extinct (between 30% and 95%) The extinctions operate across a wide range of environments and lifestyles The extinctions occurred rapidly (over a few million years) and were due to one or more physical factors
  • 3. 5 Major Mass Extinctions identified since the Cambrian Extinction Event Date of Extinction End of Ordovician 443 Million years ago Late Devonian 375 Million years ago End of Permian 251 Million years ago End of Triassic 200 Million years ago End of Cretaceous 65 Million years ago
  • 4. The 5 Major Mass Extinctions Gaps between extinctions vary from 51 Ma to 135 Ma with an average gap of 94.5 Ma
  • 5. Extinctions During the Phanerozoic The Phanerozoic is from 542 Ma (Cambrian) to the present
  • 6. Diversity Curves through the Phanerozoic End Triassic Mass Extinction possibly caused by submarine volcanism associated with the break up of Pangea
  • 7. End of Ordovician Mass Extinction – 443 Ma 70% of marine species became extinct Tropical faunas badly affected especially coral reefs Main groups affected Trilobites, Graptolites, Echinoids, Brachiopods
  • 8. Late Devonian Mass Extinction – 375 Ma A series of events that lasted around 10 Ma Cephalopods, Fish and Corals most affected
  • 9. End Permian Mass Extinction – 251 Ma The largest mass extinction event removing 95% of marine species and 50% of marine families Trilobites, Cephalopods, Bryozoans, Corals, Crinoids badly affected Major faunal and floral overturn on land Marks the boundary between dominance by the Palaeozoic and Modern Fauna
  • 10. End Triassic Mass Extinction – 200 Ma Multiple event mostly affected the land where over 95% floral species eliminated Around 30% marine species became extinct – mainly reef dwellers, Ceratites, Brachiopods and Bivalves
  • 11. End Cretaceous Mass Extinction – 65 Ma Around 70% of all species wiped out Dinosaurs, Reptiles, Ammonites, Belemnites, Brachiopods, Bivalves, Foraminifera
  • 12. Causes of Mass Extinctions Supercontinent Formation Extra-Terrestrial Impacts Flood Basalt Eruptions Methane Hydrates and Global Warming Rapid and Major Glaciation Events
  • 13. Supercontinent Formation Pangea formed at the end of the Permian Resulted in fewer continental shelves and lack of habitat for shallow marine organisms Coincided with huge decline in the numbers of shallow marine species Caused rapid fluctuations in climate, unstable weather patterns and extreme aridity in the interior of the land mass
  • 14. Supercontinent Formation A single continent reduces the input of nutrients to oceans from rivers and estuaries This decreases the amount of nutrients available for shallow water marine life and may have also altered the salinity
  • 15. Supercontinent Formation A supercontinent positioned close to one of the poles can initiate major glaciations Glaciation causes sea levels to fall and there is a significant reduction in shallow water marine environments A supercontinent located over a pole can also lead to the coverage of the Earth in ice, a condition known as ‘Snowball Earth’
  • 16. Extra-Terrestrial Impacts Asteroids 1 km diameter strike the Earth every 500,000 years Large collisions with 5 km diameter asteroids occur approximately about once every 10 million years The last known impact of an object of 10km diameter or larger was 65Ma
  • 17. Extra-Terrestrial Impacts Local destruction of habitats – impact blast, shockwave, ignition of wildfires Billions of tonnes of debris injected into the atmosphere resulting in rapid global cooling
  • 18. Extra-Terrestrial Impacts Impact in the sea – billions of tonnes of water vapour injected into the atmosphere resulting in a greenhouse effect and rapid global warming
  • 19. Flood Basalt Eruptions Eruptions last between 0.5 and 2.0 million years and can erupt enough basalt to cover the whole of the USA to a depth of a kilometre Local destruction of habitats and initiation of wildfires
  • 20. Flood Basalt Eruptions Billions of tonnes of carbon dioxide and sulphur dioxide released into the atmosphere during eruptions Both are powerful greenhouse gases and will contribute to very rapid global warming
  • 21. Flood Basalt Eruptions When it rains the sulphur dioxide will come back down to Earth dissolved in rainwater and the acid rain will kill vegetation on a large scale With vegetation dying, all food chains will be affected and also the oceans may become acidified with disastrous effects on marine life
  • 22. Methane Hydrates in Ocean Floor Sediments Large volumes currently locked into ocean floor sediments Stable under low temperatures of deep ocean
  • 23. Methane Hydrates in Ocean Floor Sediments Global warming may result in deep ocean temperatures rising and the release of large volumes of methane from ocean sediments The rapid release of large amounts of methane into the atmosphere will result in highly accelerated global warming
  • 24. Methane Hydrates in Permafrost
  • 25. Glaciations-Possible Causes Supercontinents positioned in high latitudes/close to the poles Milankovitch cycles: Precession, Obliquity and Eccentricity
  • 26. Glaciations-Effects on Ecosystems Loss of habitat as ice masses grow Could eventually lead to ‘Snowball Earth’ scenario Contraction of climatic belts towards the equator Global cooling, decreased productivity of primary producers
  • 27. End Cretaceous Mass Extinction – 65 Ma A large asteroid or meteorite (10km in diameter) collided with the Earth 65 million years ago
  • 28. Evidence - Asteroid Impact Location Location of possible impact site discovered on the Yucatan Peninsula in Mexico at Chixulub The impact structure is a circular depression about 180 km in diameter
  • 29. Evidence for Asteroid Impact Location A B A. Gravity survey onshore and offshore of the Yucatan Peninsula B. 3D map of gravity and magnetic field variations reveals the Chicxulub crater, now buried beneath tons of sediment. This view is looking down at the surface, from an angle of about 60°.
  • 30. Evidence – The K-T Boundary Layer The presence of a thin 2cm layer of iridium-rich clay found all over the world within sedimentary rocks The K-T Boundary Layer dates the same everywhere at 65.5 Ma +/- 0.3 Ma Iridium is a transition element, rare on Earth but found in meteorites. First proposed by Luis Alvarez in 1980
  • 31. Evidence – Shocked Quartz Shocked quartz is found worldwide, in a thin layer at the boundary between Cretaceous and Tertiary rocks. It was first discovered at nuclear testing sites and later in craters caused by meteorite impacts as at the Barringer Crater near Flagstaff, Arizona in the USA
  • 32. Evidence – Shocked Quartz Shocked quartz has a microscopic structure different from normal quartz. Under intense pressure, but relatively low temperature, the crystalline structure of quartz is deformed along planes inside the crystal. These planes, which show up as lines under a microscope, are called planar deformation features (PDFs), or shock lamellae.
  • 33. Evidence – Tektites (Glass Spherules) Tektites (from Greek tektos, molten) are natural glass rocks up to a few centimetres in size. Most scientists agree they are formed by the impact of large meteorites on Earth’s surface. Tektites (Glass Spherules) from 1 to 8 mm in diameter Tektites are black or olive- are found within a radius green in colour and their of 600 to 1,000km of the shape varies from rounded Chixulub Crater in Mexico to quite irregular.
  • 34. Evidence – Soot from Wildfires The K-T Layer has high concentrations of carbon in many locations, suggesting that the asteroid impact may have generated wildfires. Large areas of vegetation would have been destroyed in a short time, soot fell to Earth and was incorporated into sedimentary rocks
  • 35. Evidence – Tsunami Deposits It is thought that the asteroid impact occurred in the sea and initially produced a crater 100 km wide and 30 km deep This would have displaced vast volumes of seawater and generated a series of very large tsunamis possibly over 100 metres in height The tsunamis would have travelled great distances inland, and in Texas at Waco there are large-scale sedimentary deposits thought to be of tsunami origin.
  • 36. Evidence – Tsunami Deposits The tsunami deposits in Waco, Texas are thought to be from the waves generated by the K-T asteroid impact. The sediments are estimated to have been deposited at least 300km inland by the tsunamis!
  • 37. Animation to show Impact of a large asteroid with the Earth The impactor's estimated size was about 10 km in diameter and is estimated to have released 4×1023 joules of energy, equivalent to 100,000,000 megatons of TNT on impact.
  • 38. Origin of the K-T Asteroid Results published in 2007 suggest that the impactor that wiped out the dinosaurs and other life forms on Earth 65 million years ago can been traced back to a break-up event in the main asteroid belt more than 100 million years earlier.
  • 39. Flood Basalt Eruptions 66 Ma – The Deccan Traps Erupted mainly over a period of 30,000 years Over 2000 metres thick and cover 500,000 km² May have originally covered 1,500,000 km² Caused a global drop in temperature of 2°C The term Trap is derived from the Dutch for stairs and refers to the step-like landscape of the area