Transcript Slide 1

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Geological History & Extinctions
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FOSSIL
The trace of an organism buried
naturally and subsequently preserved
permanently
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Fossilisation
• Original soft parts (rare)
• Original hard parts (unaltered)
• Original hard parts (altered)
• carbonization
• Petrification
• Replacement or mineralisation
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Taphonomy
-The study of the postmortem history of an
organism
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Illustration of Principle of Faunal Succession
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Climate
Proxies
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Speleothem growth as a climate proxy:
Glacial
Interglacial
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Spelothem growth as a climate proxy:
Glacial
Interglacial
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The Ipswichian - 125000 years ago in
Leeds
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86000 years ago in Leeds
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Body Fossils
Alum Bluff
Mystery Fossils
Leaves from Miocene of Alum Bluff, Florida
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Body Fossils?
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Microfossils
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Trace Fossils
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“Living Fossils”
Ginkgo biloba
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Metasequuoia gyptostroboides
Geologic time (millions of years)
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Geologic Time & Biology
Geologic time (millions of years)
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Geologic Time & Biology
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Geologic time (millions of years)
Geologic Time & Biology
Fig. 4-1a, p.74
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Geologic Time
• MAJOR DIVISIONS
• Cenozoic: 66 - 2.5 m.y.a
• Mesozoic: 245 - 66 m.y.a.
• Paleozoic: 544 - 245 m.y.a.
• Precambrian: pre-544 m.y.a.
(Proterozoic)
Geologic Time
• Eon/Era/Period - relative
ages (fossils, stratigraphy )
• Dates: absolute ages
(radiometric dating)
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Precambrian (4.6 Ga – 570 Ma)
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Comprises 88% of Earth History
First continents, plate tectonics
Rock record poorly preserved
Life evolves, but rarely preserved as fossils
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Paleozoic Era (570 Ma - 245 Ma)
 Continents are widely separated
 Continents collide - Pangea
 Reptiles & amphibians
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Mesozoic Era (245 Ma – 66 Ma)
• Breakup of Pangea
• Opening of Atlantic Ocean
• Dinosaurs, mammals,
flowering plants
Cenozoic Era (66 Ma - present)
 Mammals & grasses
 India-Asia collide
 Australia moves N.
 Rocky Mts. form
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Mass Extinctions
Def.: catastrophic events
• that abruptly killed most
• life on Earth & allowed
• new life forms to emerge
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• Scientists debated origin
• Evidence for at least 5
• mass extinctions
• Causes?
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A Bad Day…. 65 Million Years Ago
• The Asteroid: ~10 km
• dinosaur extinction?
• The Impact
• Chicxulub Crater (Yucatan)
• 300 km underwater crater
• The Result
• Cretaceous Extinction
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Mass Extinctions:
Extraterrestrial Impacts
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• Meteoric impact - explosion
• Thick cloud of dust, blocks sunlight
• Ocean?
Fig. 4-2, p.75
Mass Extinctions:
Volcanic Eruptions
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• Eruptions of gas & volcanic ash - contaminate
atmosphere
• SO2 reflects sunlight = cooling
• CO2 blocks radiated energy = warming
Fig. 4-2, p.75
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Example Eruptions:
• Historic “regular” big eruptions:
up to 50,000 fatalities
• “ Siberian Traps”:
250 Ma, massive
eruption: almost
area of USA
Fig. 4-2, p.75
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Mass Extinctions:
Atmosphere-Ocean-Continent Interactions
• Ocean-Atmosphere: Ocean currents mix heat & gases
from oceans to atm.
• Ocean-Continent: Ocean currents partly controlled by
positions of continents
Fig. 4-2, p.75
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Evolution of Earth Atmosphere
• Initially: thick atmosphere of CO2 & H2O
• H2O condense to oceans
• CO2 dissolved in oceans: carbonate rocks, little for atm.
• Additional O2 from photosynthesis
• Today: N2, O2
All Others
Oxygen
Nitrogen
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Mass Extinctions:
Atmosphere-Ocean Interaction (1)
 CO2 transferred from atmosphere to ocean
 Atmosphere cools
Fig. 4-2, p.75
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Mass Extinctions:
Atmosphere-Ocean Interaction (2)
 Cooling water sinks: stirs up deep ocean
 CO2 sent back to surface, kills organisms
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Mass Extinctions:
Atmosphere-Ocean-Continent Interactions
• Ocean-Atmosphere: Ocean currents mix heat & gases from
oceans to atm.
• Ocean-Continent: Ocean currents partly controlled by
positions of continents
Fig. 4-2, p.75
Mass Extinctions:
Ocean-Continent Interaction
 Supercontinent “Pangea”
 Single land mass prevented mixing of ocean
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What is wrong?
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