Geology Study Guide #2
Sections 9 and 10 - Plate Tectonics
Continental Drift
The potential to fit the continents together like puzzle pieces had been noted before (as early as 1596!), but…
Alfred Wegener (1912, 1915) marshaled many lines of evidence that the continents had moved
Many Permian-Triassic aged fossils are found across the southern continents
Easy to explain if they were once joined (Gondwana)
Distribution of Carboniferous-Permian Glacial Deposits
~ glaciers will be in cold areas where it will be ice all year round
~ continents were located closer together and centered around the South Pole
Distribution of older rocks matches up too
Boundary Types
Divergent: pulling apart
Continental rift: faulting forms a rift valley and parallel valleys along it
Faulting/rift forming leads to volcanic and earthquake activity
Transform: sliding past
Can be ocean-ocean or continental
Plates slide past on strike-slip faults
Lithosphere isn’t created or destroyed
Earthquakes common
Convergent: one plate pushed under another at subduction zone
Ocean-ocean: colder and denser plate subducts, oceanic trench forms
Volcanic arc/orogeny on plate that isn’t subducted
Continent-ocean: oceanic plate subducts
Volcanic arc/orogeny on continental plate
Continent-continent: neither plate wants to subduct
Lithosphere shortens via crumpling and thickening
Leads to faulting and folding
Wegener’s “Continental Drift”
Wegener had no plausible explanation for how the continents moved – he proposed that they plowed across the ocean floor
Most geologists rejected his theory for this reason
Crust and Upper Mantle
Continental crust – low density, felsic (feldspar-rich)
~ underlies continental shelves as well as land
Oceanic crust – high density, mafic (iron-rich)
Mantle – very high density, ultramafic (very iron-rich)
Crust and Upper Mantle
Crust-mantle boundary = Moho (Mohorovicic discontinuity)
~ Marks an increase in rock density
Lithosphere = crust + upper mantle
~ firmly attached, forming a rigid layer
Asthenosphere = slushy, partially molten layer below the lithosphere
Most earthquakes and volcanoes occur at plate boundaries
Sinking blocks of crust
Earthquakes are going to happen when there is pressure, variety of depths
Strike and Dip
Sed rocks = most likely to have layers
Strike line = horizontal line
Tick mark records that it is going downhill
Number = magnitude of dip
Geologic Subsurface Structures
Syncline:
Concave up
Layers dip toward each other
Youngest rock in the middle
Anticline
Concave down
Layers dip away from each other
Oldest rock in the middle
Strike and Dip? Why should we care?
Landslide risk
Oil exploration
Mineral resources
Groundwater resources
Overturned folds
Axial plane – boundary between two plates
Syncline and anticline
Section 11 - Biogeochemical Cycles
Relative Size of Different Water Reservoirs
(saltwater) Oceans ~ 97.5%
(freshwater)
Ice caps and glaciers ~79%
Groundwater ~20%
Water in lakes ~52%
Water in rivers
Water in living organisms
Water vapor in atmosphere
Water in soil ~38%
Water Cycle
Evaporation, precipitation, groundwater, pools (reservoirs) and fluxes, evapotranspiration
Evaporation and Evapotranspiration
Water enters the atmosphere (air) by:
Evaporation: conversion to water vapor from bodies of surface water (lakes, oceans, etc.)
Evapotranspiration:
Water vapor is lost to the air by plants
Delivers groundwater into the atmosphere
Evapotranspiration
Water enters plants through roots
Flows up vascular (tubelike) tissues
Leafe Stomata:
Openings for gas exchange
Water loss through these openings
Draws additional water up the vascular tissues
This process delivers water from soil (groundwater) to atmosphere (air)
Desertification: drying up of an area due to lack of plants
deforestation → no mechanism (plants) to get groundwater into atmosphere → area dries up
Carbon Cycle
Earth’s “Thermostat”
Determines Earth’s climate over very long timescales
Volcanism releases carbon dioxide
Rock weathering absorbs (fixes) carbon dioxide
Volcanic Outgassing
Hydrogen Sulfide
Methane (carbon gas - greenhouse gas)
Carbon Dioxide (carbon gas - greenhouse gas)
Water Vapor
Biological Carbon
Atmospheric carbon enters biological systems via photosynthesis
CO2+H2O => C6H12)6(sugar)+O2
Carbon is then repurposed into a wide variety of organic molecules
fats/oils (lipids)
Proteins
Nucleic acids (DNA & RNA)
ex.) “Blue-Green Algae” (photosynthesizing bacteria)
ex.) Tree photosynthesizing
Fossil Fuels
Ancient Organic Material
Generally the result of photosynthesis
Contain many high-energy bonds → burn readily
Major contributor to climate change
Include:
Coal
Oil
Natural gas
Future Coal
Coal:
Accumulated plant matter
Start as peat bogs
Anoxic conditions prevent decay
Future Oil
Oil:
Accumulation of algal biomass
Accumulate at bottoms of oceans and large lakes
Fossil Fuel Formation
Organisms live and die
Organic material is buried
Heat and pressure alter molecule structure (not unlike metamorphic rock formation)
Wildfires: Another Source of Atmospheric Carbon
Why Continental Weathering Draws Down CO2
Rocks exposed to air and water are susceptible to chemical weathering
Produces:
Clastic sediments
Dissolved ions (including Ca+)
Ca+ & CO2 can combine to form CaCO3 → limestone
Eutrophication
Can be caused by an excess of nitrogenous nutrients
Results in anoxia
Healthy Water living organisms: fresh water and natural balance between water organisms, oxygen, algae and nutrients: enough sunlight for water plants
Eutrophication dead zone: explosive algal bloom due to excess nutrients coming from nitrogen (N) and phosphorus (P) rich pollutants; oxygen (O2) consumption by algae, reduced by sunlight, breakdown of natural chemical cycles
Human Causes of Eutrophication
Nitrate and Phosphate fertilizers
Concentrated animal feeding operations
Direct sewage and industrial waste discharge into water
Improperly managed aquaculture
Natural events
Stream discharge
Flood events
Section 12 - Paleoclimate
Rules for air flow:
Flows from high pressure to low pressure
Hot air rises, cold air sinks
Locations that produce hot air, produce low pressure zones
Global air circulation & precipitation
Warms air rises
Dry air descends, warms, and becomes even drier
Warm air rises, cools and loses moisture
Dry belts at ~30º N/S and at the poles
Can be altered by local geography
Greenhouse Gases
Gases like O2 and O3 absorb Ultraviolet radiations
Blocked from Earth’s Energy Budget
O2 and O3 let through visible and some shortwave radiation
Greenhouse gases also let through visible and shortwave radiation
Earth absorbs visible and shortwave radiation
Earth re-radiates near-and IR radiation
Greenhouse gases absorb and re-radiate and near-and IR radiation
Consider Also: Albedo
Albedo:
Reflectiveness of a surface
Controls how much energy is absorbed (as heat) vs reflected
Different Surfaces with different albedos:
Land vs water
Forest
Deserts
Glacial ice
Continental Position Influences Albedo
Availability of ice
Bare rock vs foliage cover
Proxy Data
Information accessible in the present that indirectly indicates conditions in the past
Climate Proxy Data: Recent Past
How do we get temperature info from the distant past? → PROXY DATA:
Tree ring thickness and density
Coral reef annual layers
Lake sediment – snowmelt and pollen
δ18O in mollusk shells and ice cores
Various metrics agree that current average temperatures are higher than they have ever been in the past 1000 years.
Proxies for Conditions of the More Distant Past
Rocks specific to climate:
E.g. Glacial deposits
E.g. Bauxite, only forms in tropical climates
Fossil organisms present
Geochemical data
Stable isotopes
Chemically equivalent, but have different masses
Proxy Data
Fossils – some organisms live in specific environments. Their fossils indicate climate
Cycads and crocodilians prefer tropical climates today but lived closer to the poles in the past – therefore, mid-to-high latitudes must have had warmer climates than today
Proxy Data
Lead Margin Analysis – cold-adapted floras have more jagged leaves; warm-adapted ones have more smooth leaves.
The percentage of smooth leaves in a fossil flora can be used to determine temperature.
Proxy Data
Stomatal density – plants respire through openings called stomata
In woody plants, the number of stomata increases as CO2 decreases
Low CO2 correlates with low temperatures, so more stomata suggest low temperatures too
Proxy Data
Oxygen isotope ratios – at low temperatures, heavy isotopes move slower. This is terms fractionation.
Section 13 - Geochronology
What are Isotopes?
Forms of an element that have a different number of neutrons than usual
Atomic mass is different but chemical properties are the same
Each radioisotope has a characteristic Half Life: the time it takes for half the atoms to decay
On a linear scale, decay follows a hollow curve
On a logarithmic scale, decay follows a straight line
When is a particular isotope useful?
Short half-life good for young samples
Long half-life good for old samples
Why?
Must have enough parent isotope left to measure accurately
Enough time must have past for some daughter isotope to accumulate
Blocking or Closure Temperature
In radiometric dating, we measure the ratio between parent and daughter isotope
There is no daughter isotope to begin with
Above the blocking temperature, the daughter isotope diffuses out of a mineral
Below the blocking tem, the daughter isotope collects
Thus, a radiometric age is the age since the mineral last cooled below the blocking temp.
Can represent time since cooling from a magma or cooling after metamorphism
Blocking temp. depends on the mineral and isotope
Radiometric dating only puts upper and lower boundaries on dates of sedimentary rocks
Procedure: date igneous rocks and determine relative age of associated sedimentary rocks using:
Principle of Superposition
Principle of Cross-Cutting Relationships
Principle of Inclusions
Radiometric dating does not tell you when a sedimentary rock was deposited
Section 14 - Paleogeography
Reconstructing Paleogeography
Methods
Linear Magnetic Anomalies: can reverse time by “deleting” stripes of opposite polarity from oceanic ridges
Paleomagnetism: magnetic grains are vertical at poles and horizontal at equator (measures paleolatitude)
Paleobiogeography: can indicate paleolatitude (based on climate) and proximity of continents
Paleoclimatology
Regional Geologic and Tectonic History: matching up geologic features to find paleolongitude
Paleoclimatology: Some rocks are only deposited in certain climatic conditions
Evaporite = Arid
Coal = Swamp = High Precipitation
Most Carbonates = Warm Water
Our knowledge of paleogeography
Cenozoic & Mesozoic – Excellent
Magnetic seafloor anomalies allow precise reconstructions
Paleozoic – Good
Lots of paleomagnetic and geologic data
Neoproterzoic – topic of current research
Data are more sparse, but they are being collected
There are competing interpretations
Earlier in the Precambrian – much less known
Much less rock on which to work
Section 15 - Precambrian Geology ** need oldest regions of crust (where are they?)
Precambrian Geology
Cratons
Large under-formed portions of continents
Primarily Precambrian
Precambrian shield
Craton exposed at surface
Canadian Shield exposed by glaciation
Oldest Region of Crust: the Canadian Shield (northeastern Canada)
Land bodies colliding with continents
More continental crust through volcanic rocks – more felsic materials/minerals, lower melting point
Precambrian Geology
Continental crust formed during Archean
High heat flow early in Earth’s history required small continents
Thinner sections of crust
Origin of the Universe
Fragments of larger rocky bodies that have undergone collision and broken into pieces
Provide important information concerning age of Earth
Origin of the Universe
Stony meteorites
Rocky composition
Iron meteorites
Metallic composition
Stony-iron meteorites
Mixture of rocky and metallic
Proxy for core composition
Most date around 4.6 billion years ago
Origin of the Universe
Stars cluster in galaxies
Organized in disks
Milky Way
Our galaxy of stars
Expanding universe
Galaxies move apart
Redshift
Originally concentrated into a single point
Big Bang
~13.7 billion years ago (age of universe)
Galactic matter in concentrated
Stars form
Our sun
Supernova
Exploding star
Solar nebula
Dense rotational cloud
Origin of Earth and Moon
4.6 Ba
Earth materials differentiated
Dense at center
Less dense silicates rose to surface
Magma ocean
Cooled to form crust
Meteorite impacts increased concentrations of some elements in upper Earth
Origin of Earth and Moon
Early Atmosphere
Degassing from volcanic emission
CH4 and NH3 abundant
Little O2
No photosynthesis
Earth’s oceans
Volcanic emissions cooled, condensed
Salts
Carried to sea by rivers and introduced at ridges
Approximately constant through time
Origin of Continents
Small Archean fragments
High heat flow limited continental thickness
Zircon crystals
4.1-4.2 B years old
Weathered from felsic rocks
Canadian Shield
3.8-4.0 B years old
Origin of Continents
Greenstone belts
Weakly metamorphosed
Previously ancient sedimentary rocks
Abundant chlorite
Green color
Nested in high-grade felsic metamorphic rocks
Greenstone belts contain igneous rocks
Volcanics contain pillow basalts
Underwater extrusion
Formation of sediments in deep water
Greywackes, mudstones, iron formations, volcanic sediments
Origin of Continents
Continental accretion
Deep water sediments accreted to continent
Marine sediments form wedge between continental masses
Section 16 - Precambrian Life
Prokaryote
Smaller and simpler
No organelles
Many different metabolisms, including anaerobic
Bacteria and Archaea
Eukaryote
Larger, more complex
Organelles, incl. nucleus
Generally require oxygen
Some lineages evolved multicellularity
Where did life begin?
Some think on the ocean floor, where hot, nutrient-rich waters are expelled
Mid-ocean ridges, hydrothermal vents
When did life begin?
Not many sedimentary rocks older than ~3.5 Ga (=billions of years ago)
Pretty good evidence there was life by at least 3.5-3.2 Ga, although people argue about the fossils and the exact date
Hematite tubes: Possible microbial sheathes from 3.77-4.28 Ga, Quebec. Would have lived in a hydrothermal setting
Other scientists dispute both the age of the rocks and the biological nature of the structures.
Multicellular Algae
~580 Ma
Fossils of non-mineralized “seaweeds” are relatively rare
Section 17 - Cambrian Period
Ediacaran Biota
There were animals, but most of them…
Did not belong to modern phyla (e.g., echinoderms, arthropods)
Did not have legs, fins, etc.
Did not have obvious sense organs
Did not have obvious body openings (probably fed by absorption)
Did not have mineralized skeletons
Did not burrow into the sediment, at least deeply
In the Cambrian
Almost all modern phyla with skeletons appeared
Animals with legs, fins, body openings, sense organs, and skeletons were abundant
Marine ecosystems are relatively modern: herbivory, predation, suspension feedings, etc. were present
Burrowing and bioturbation increased
Cambrian World – Geologic Environments and Events
Laurentia (N. America) rifts from Gondwana
Laurentia coastlines become passive margins all the way around
Sedimentation accommodated by:
Sea level rise
Thermal subsidence
Sediment Sources:
Silicate weathering from continent
Carbonates precipitating from water
Biogenic carbonates
Sea Level in the Cambrian Period
Sea level low at beginning of Cambrian
Rises over course of the period
Laurentia (N. America) is almost entirely drowned by the end of the period
Marine Sedimentation Around Laurentia
Dominated by terrigenous sands
Mature silicates
Almost solely quartz
Rounded, well-sorted grains
Evidence for aeolian (wind-based) weathering
Carbonates on shelf edges, far from terrestrial sources
Toward end of Cambrian period, continent flooded
Way less terrigenous sediment
Widespread carbonate deposition
Tropical temperatures
Agitated water → carbonate precipitation
Rise of skeletal carbonate
Why was there so much highly-processed terrigenous sediment?
Continents above sea level
NO PLANTS
ex.) Still from the opening sequence of the movie Prometheus. This sequence depicts erosion and transportation of sediment on a landscape without plants.
Mineralized skeletons, what are they?
Minerals for structure and protections
calcite/Aragonite
Apatite
Silica
Ediacaran trace fossils: simple horizontal burrows
Cambrian trace fossils: some are more complex, branching an/or probing vertically into the sediment
ex.) Treptichnus pedum: defined the base of the Cambrian
Ediacaran/Cambrian boundary type section
Fortune Head, SE Newfoundland
Increase in sediment disturbance during the early Paleozoic
Ediacaran
Microbial mats cover seafloor
Only shallow horizontal burrows
Animals can attach to mat
Later Cambrian
Bioturbated “mixed layer” replaces mats
More burrowing, some vertical burrowing
Sediment surface less stable
Section 18 - Ordovician Period
Tectonic Changes to Laurentia
Started at high sea level with extensive epicontinental seas
Subduction zone forms on east coast of Laurentia
Taconic orogeny at the end of the Ordovician
Island arc accreted to Laurentia
Prominent Ordovician Fauna
Graptolites: colonial filter feeders
Good index fossils, wide geographic range b/c some floated closer to surface
Corals: functioned as reef-builders
Rugose Corals
Tabulate Corals
Ecosystem engineers
Extinct now
Cephalopods: nautiloids (curved walls) and ammonoids (zigzag walls)
Sections 9 and 10 - Plate Tectonics
Continental Drift
The potential to fit the continents together like puzzle pieces had been noted before (as early as 1596!), but…
Alfred Wegener (1912, 1915) marshaled many lines of evidence that the continents had moved
Many Permian-Triassic aged fossils are found across the southern continents
Easy to explain if they were once joined (Gondwana)
Distribution of Carboniferous-Permian Glacial Deposits
~ glaciers will be in cold areas where it will be ice all year round
~ continents were located closer together and centered around the South Pole
Distribution of older rocks matches up too
Boundary Types
Divergent: pulling apart
Continental rift: faulting forms a rift valley and parallel valleys along it
Faulting/rift forming leads to volcanic and earthquake activity
Transform: sliding past
Can be ocean-ocean or continental
Plates slide past on strike-slip faults
Lithosphere isn’t created or destroyed
Earthquakes common
Convergent: one plate pushed under another at subduction zone
Ocean-ocean: colder and denser plate subducts, oceanic trench forms
Volcanic arc/orogeny on plate that isn’t subducted
Continent-ocean: oceanic plate subducts
Volcanic arc/orogeny on continental plate
Continent-continent: neither plate wants to subduct
Lithosphere shortens via crumpling and thickening
Leads to faulting and folding
Wegener’s “Continental Drift”
Wegener had no plausible explanation for how the continents moved – he proposed that they plowed across the ocean floor
Most geologists rejected his theory for this reason
Crust and Upper Mantle
Continental crust – low density, felsic (feldspar-rich)
~ underlies continental shelves as well as land
Oceanic crust – high density, mafic (iron-rich)
Mantle – very high density, ultramafic (very iron-rich)
Crust and Upper Mantle
Crust-mantle boundary = Moho (Mohorovicic discontinuity)
~ Marks an increase in rock density
Lithosphere = crust + upper mantle
~ firmly attached, forming a rigid layer
Asthenosphere = slushy, partially molten layer below the lithosphere
Most earthquakes and volcanoes occur at plate boundaries
Sinking blocks of crust
Earthquakes are going to happen when there is pressure, variety of depths
Strike and Dip
Sed rocks = most likely to have layers
Strike line = horizontal line
Tick mark records that it is going downhill
Number = magnitude of dip
Geologic Subsurface Structures
Syncline:
Concave up
Layers dip toward each other
Youngest rock in the middle
Anticline
Concave down
Layers dip away from each other
Oldest rock in the middle
Strike and Dip? Why should we care?
Landslide risk
Oil exploration
Mineral resources
Groundwater resources
Overturned folds
Axial plane – boundary between two plates
Syncline and anticline
Section 11 - Biogeochemical Cycles
Relative Size of Different Water Reservoirs
(saltwater) Oceans ~ 97.5%
(freshwater)
Ice caps and glaciers ~79%
Groundwater ~20%
Water in lakes ~52%
Water in rivers
Water in living organisms
Water vapor in atmosphere
Water in soil ~38%
Water Cycle
Evaporation, precipitation, groundwater, pools (reservoirs) and fluxes, evapotranspiration
Evaporation and Evapotranspiration
Water enters the atmosphere (air) by:
Evaporation: conversion to water vapor from bodies of surface water (lakes, oceans, etc.)
Evapotranspiration:
Water vapor is lost to the air by plants
Delivers groundwater into the atmosphere
Evapotranspiration
Water enters plants through roots
Flows up vascular (tubelike) tissues
Leafe Stomata:
Openings for gas exchange
Water loss through these openings
Draws additional water up the vascular tissues
This process delivers water from soil (groundwater) to atmosphere (air)
Desertification: drying up of an area due to lack of plants
deforestation → no mechanism (plants) to get groundwater into atmosphere → area dries up
Carbon Cycle
Earth’s “Thermostat”
Determines Earth’s climate over very long timescales
Volcanism releases carbon dioxide
Rock weathering absorbs (fixes) carbon dioxide
Volcanic Outgassing
Hydrogen Sulfide
Methane (carbon gas - greenhouse gas)
Carbon Dioxide (carbon gas - greenhouse gas)
Water Vapor
Biological Carbon
Atmospheric carbon enters biological systems via photosynthesis
CO2+H2O => C6H12)6(sugar)+O2
Carbon is then repurposed into a wide variety of organic molecules
fats/oils (lipids)
Proteins
Nucleic acids (DNA & RNA)
ex.) “Blue-Green Algae” (photosynthesizing bacteria)
ex.) Tree photosynthesizing
Fossil Fuels
Ancient Organic Material
Generally the result of photosynthesis
Contain many high-energy bonds → burn readily
Major contributor to climate change
Include:
Coal
Oil
Natural gas
Future Coal
Coal:
Accumulated plant matter
Start as peat bogs
Anoxic conditions prevent decay
Future Oil
Oil:
Accumulation of algal biomass
Accumulate at bottoms of oceans and large lakes
Fossil Fuel Formation
Organisms live and die
Organic material is buried
Heat and pressure alter molecule structure (not unlike metamorphic rock formation)
Wildfires: Another Source of Atmospheric Carbon
Why Continental Weathering Draws Down CO2
Rocks exposed to air and water are susceptible to chemical weathering
Produces:
Clastic sediments
Dissolved ions (including Ca+)
Ca+ & CO2 can combine to form CaCO3 → limestone
Eutrophication
Can be caused by an excess of nitrogenous nutrients
Results in anoxia
Healthy Water living organisms: fresh water and natural balance between water organisms, oxygen, algae and nutrients: enough sunlight for water plants
Eutrophication dead zone: explosive algal bloom due to excess nutrients coming from nitrogen (N) and phosphorus (P) rich pollutants; oxygen (O2) consumption by algae, reduced by sunlight, breakdown of natural chemical cycles
Human Causes of Eutrophication
Nitrate and Phosphate fertilizers
Concentrated animal feeding operations
Direct sewage and industrial waste discharge into water
Improperly managed aquaculture
Natural events
Stream discharge
Flood events
Section 12 - Paleoclimate
Rules for air flow:
Flows from high pressure to low pressure
Hot air rises, cold air sinks
Locations that produce hot air, produce low pressure zones
Global air circulation & precipitation
Warms air rises
Dry air descends, warms, and becomes even drier
Warm air rises, cools and loses moisture
Dry belts at ~30º N/S and at the poles
Can be altered by local geography
Greenhouse Gases
Gases like O2 and O3 absorb Ultraviolet radiations
Blocked from Earth’s Energy Budget
O2 and O3 let through visible and some shortwave radiation
Greenhouse gases also let through visible and shortwave radiation
Earth absorbs visible and shortwave radiation
Earth re-radiates near-and IR radiation
Greenhouse gases absorb and re-radiate and near-and IR radiation
Consider Also: Albedo
Albedo:
Reflectiveness of a surface
Controls how much energy is absorbed (as heat) vs reflected
Different Surfaces with different albedos:
Land vs water
Forest
Deserts
Glacial ice
Continental Position Influences Albedo
Availability of ice
Bare rock vs foliage cover
Proxy Data
Information accessible in the present that indirectly indicates conditions in the past
Climate Proxy Data: Recent Past
How do we get temperature info from the distant past? → PROXY DATA:
Tree ring thickness and density
Coral reef annual layers
Lake sediment – snowmelt and pollen
δ18O in mollusk shells and ice cores
Various metrics agree that current average temperatures are higher than they have ever been in the past 1000 years.
Proxies for Conditions of the More Distant Past
Rocks specific to climate:
E.g. Glacial deposits
E.g. Bauxite, only forms in tropical climates
Fossil organisms present
Geochemical data
Stable isotopes
Chemically equivalent, but have different masses
Proxy Data
Fossils – some organisms live in specific environments. Their fossils indicate climate
Cycads and crocodilians prefer tropical climates today but lived closer to the poles in the past – therefore, mid-to-high latitudes must have had warmer climates than today
Proxy Data
Lead Margin Analysis – cold-adapted floras have more jagged leaves; warm-adapted ones have more smooth leaves.
The percentage of smooth leaves in a fossil flora can be used to determine temperature.
Proxy Data
Stomatal density – plants respire through openings called stomata
In woody plants, the number of stomata increases as CO2 decreases
Low CO2 correlates with low temperatures, so more stomata suggest low temperatures too
Proxy Data
Oxygen isotope ratios – at low temperatures, heavy isotopes move slower. This is terms fractionation.
Section 13 - Geochronology
What are Isotopes?
Forms of an element that have a different number of neutrons than usual
Atomic mass is different but chemical properties are the same
Each radioisotope has a characteristic Half Life: the time it takes for half the atoms to decay
On a linear scale, decay follows a hollow curve
On a logarithmic scale, decay follows a straight line
When is a particular isotope useful?
Short half-life good for young samples
Long half-life good for old samples
Why?
Must have enough parent isotope left to measure accurately
Enough time must have past for some daughter isotope to accumulate
Blocking or Closure Temperature
In radiometric dating, we measure the ratio between parent and daughter isotope
There is no daughter isotope to begin with
Above the blocking temperature, the daughter isotope diffuses out of a mineral
Below the blocking tem, the daughter isotope collects
Thus, a radiometric age is the age since the mineral last cooled below the blocking temp.
Can represent time since cooling from a magma or cooling after metamorphism
Blocking temp. depends on the mineral and isotope
Radiometric dating only puts upper and lower boundaries on dates of sedimentary rocks
Procedure: date igneous rocks and determine relative age of associated sedimentary rocks using:
Principle of Superposition
Principle of Cross-Cutting Relationships
Principle of Inclusions
Radiometric dating does not tell you when a sedimentary rock was deposited
Section 14 - Paleogeography
Reconstructing Paleogeography
Methods
Linear Magnetic Anomalies: can reverse time by “deleting” stripes of opposite polarity from oceanic ridges
Paleomagnetism: magnetic grains are vertical at poles and horizontal at equator (measures paleolatitude)
Paleobiogeography: can indicate paleolatitude (based on climate) and proximity of continents
Paleoclimatology
Regional Geologic and Tectonic History: matching up geologic features to find paleolongitude
Paleoclimatology: Some rocks are only deposited in certain climatic conditions
Evaporite = Arid
Coal = Swamp = High Precipitation
Most Carbonates = Warm Water
Our knowledge of paleogeography
Cenozoic & Mesozoic – Excellent
Magnetic seafloor anomalies allow precise reconstructions
Paleozoic – Good
Lots of paleomagnetic and geologic data
Neoproterzoic – topic of current research
Data are more sparse, but they are being collected
There are competing interpretations
Earlier in the Precambrian – much less known
Much less rock on which to work
Section 15 - Precambrian Geology ** need oldest regions of crust (where are they?)
Precambrian Geology
Cratons
Large under-formed portions of continents
Primarily Precambrian
Precambrian shield
Craton exposed at surface
Canadian Shield exposed by glaciation
Oldest Region of Crust: the Canadian Shield (northeastern Canada)
Land bodies colliding with continents
More continental crust through volcanic rocks – more felsic materials/minerals, lower melting point
Precambrian Geology
Continental crust formed during Archean
High heat flow early in Earth’s history required small continents
Thinner sections of crust
Origin of the Universe
Fragments of larger rocky bodies that have undergone collision and broken into pieces
Provide important information concerning age of Earth
Origin of the Universe
Stony meteorites
Rocky composition
Iron meteorites
Metallic composition
Stony-iron meteorites
Mixture of rocky and metallic
Proxy for core composition
Most date around 4.6 billion years ago
Origin of the Universe
Stars cluster in galaxies
Organized in disks
Milky Way
Our galaxy of stars
Expanding universe
Galaxies move apart
Redshift
Originally concentrated into a single point
Big Bang
~13.7 billion years ago (age of universe)
Galactic matter in concentrated
Stars form
Our sun
Supernova
Exploding star
Solar nebula
Dense rotational cloud
Origin of Earth and Moon
4.6 Ba
Earth materials differentiated
Dense at center
Less dense silicates rose to surface
Magma ocean
Cooled to form crust
Meteorite impacts increased concentrations of some elements in upper Earth
Origin of Earth and Moon
Early Atmosphere
Degassing from volcanic emission
CH4 and NH3 abundant
Little O2
No photosynthesis
Earth’s oceans
Volcanic emissions cooled, condensed
Salts
Carried to sea by rivers and introduced at ridges
Approximately constant through time
Origin of Continents
Small Archean fragments
High heat flow limited continental thickness
Zircon crystals
4.1-4.2 B years old
Weathered from felsic rocks
Canadian Shield
3.8-4.0 B years old
Origin of Continents
Greenstone belts
Weakly metamorphosed
Previously ancient sedimentary rocks
Abundant chlorite
Green color
Nested in high-grade felsic metamorphic rocks
Greenstone belts contain igneous rocks
Volcanics contain pillow basalts
Underwater extrusion
Formation of sediments in deep water
Greywackes, mudstones, iron formations, volcanic sediments
Origin of Continents
Continental accretion
Deep water sediments accreted to continent
Marine sediments form wedge between continental masses
Section 16 - Precambrian Life
Prokaryote
Smaller and simpler
No organelles
Many different metabolisms, including anaerobic
Bacteria and Archaea
Eukaryote
Larger, more complex
Organelles, incl. nucleus
Generally require oxygen
Some lineages evolved multicellularity
Where did life begin?
Some think on the ocean floor, where hot, nutrient-rich waters are expelled
Mid-ocean ridges, hydrothermal vents
When did life begin?
Not many sedimentary rocks older than ~3.5 Ga (=billions of years ago)
Pretty good evidence there was life by at least 3.5-3.2 Ga, although people argue about the fossils and the exact date
Hematite tubes: Possible microbial sheathes from 3.77-4.28 Ga, Quebec. Would have lived in a hydrothermal setting
Other scientists dispute both the age of the rocks and the biological nature of the structures.
Multicellular Algae
~580 Ma
Fossils of non-mineralized “seaweeds” are relatively rare
Section 17 - Cambrian Period
Ediacaran Biota
There were animals, but most of them…
Did not belong to modern phyla (e.g., echinoderms, arthropods)
Did not have legs, fins, etc.
Did not have obvious sense organs
Did not have obvious body openings (probably fed by absorption)
Did not have mineralized skeletons
Did not burrow into the sediment, at least deeply
In the Cambrian
Almost all modern phyla with skeletons appeared
Animals with legs, fins, body openings, sense organs, and skeletons were abundant
Marine ecosystems are relatively modern: herbivory, predation, suspension feedings, etc. were present
Burrowing and bioturbation increased
Cambrian World – Geologic Environments and Events
Laurentia (N. America) rifts from Gondwana
Laurentia coastlines become passive margins all the way around
Sedimentation accommodated by:
Sea level rise
Thermal subsidence
Sediment Sources:
Silicate weathering from continent
Carbonates precipitating from water
Biogenic carbonates
Sea Level in the Cambrian Period
Sea level low at beginning of Cambrian
Rises over course of the period
Laurentia (N. America) is almost entirely drowned by the end of the period
Marine Sedimentation Around Laurentia
Dominated by terrigenous sands
Mature silicates
Almost solely quartz
Rounded, well-sorted grains
Evidence for aeolian (wind-based) weathering
Carbonates on shelf edges, far from terrestrial sources
Toward end of Cambrian period, continent flooded
Way less terrigenous sediment
Widespread carbonate deposition
Tropical temperatures
Agitated water → carbonate precipitation
Rise of skeletal carbonate
Why was there so much highly-processed terrigenous sediment?
Continents above sea level
NO PLANTS
ex.) Still from the opening sequence of the movie Prometheus. This sequence depicts erosion and transportation of sediment on a landscape without plants.
Mineralized skeletons, what are they?
Minerals for structure and protections
calcite/Aragonite
Apatite
Silica
Ediacaran trace fossils: simple horizontal burrows
Cambrian trace fossils: some are more complex, branching an/or probing vertically into the sediment
ex.) Treptichnus pedum: defined the base of the Cambrian
Ediacaran/Cambrian boundary type section
Fortune Head, SE Newfoundland
Increase in sediment disturbance during the early Paleozoic
Ediacaran
Microbial mats cover seafloor
Only shallow horizontal burrows
Animals can attach to mat
Later Cambrian
Bioturbated “mixed layer” replaces mats
More burrowing, some vertical burrowing
Sediment surface less stable
Section 18 - Ordovician Period
Tectonic Changes to Laurentia
Started at high sea level with extensive epicontinental seas
Subduction zone forms on east coast of Laurentia
Taconic orogeny at the end of the Ordovician
Island arc accreted to Laurentia
Prominent Ordovician Fauna
Graptolites: colonial filter feeders
Good index fossils, wide geographic range b/c some floated closer to surface
Corals: functioned as reef-builders
Rugose Corals
Tabulate Corals
Ecosystem engineers
Extinct now
Cephalopods: nautiloids (curved walls) and ammonoids (zigzag walls)