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Chapter 12
Deep Time: How Old Is Old?

LECTURE OUTLINE

earth

Portrait of a Planet

Third Edition
©2008 W. W. Norton & Company, Inc.
Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Deep Time: How Old Is Old?

Prepared by

Ronald Parker
Earlham College Department of Geosciences
Richmond, Indiana
Geologic Time
Discovering the magnitude of the Earth’s past was
a momentous discovery in the history of humanity.
 This discovery forever altered our perception of
ourselves within nature and the Universe.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic Time


Understanding time permits assigning an age to…
Rocks.
 Fossils.
 Geologic structures.
 Landscapes.
 Tectonic events.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic Time
Deep time – The immense span of geologic time.
 It is so vast that it is difficult for people to grasp.




We think of time in terms of our lives…
The lives of our parents and grandparents.
The lives of our children or grandchildren.



Human history is tiny compared
to geologic time.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic Time


Prior to the late 17th century, geologic time was
thought to be the same as historical time.


Archbishop James Ussher of Armagh, Ireland, 1654.
He added up generations from the Old Testament.
He determined that Earth formed on October 23, 4004 BCE.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic Time


Scientists began to find clues to an ancient Earth.


Nicolaus Steno (1638–1686) – Danish physician.
Observed marine fossils high in the Apennines.
Deduced that these were ancient animals in loose sediment.
Lithification and uplift suggested long periods of time.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic Time


James Hutton (1726-1797) – Scottish physician.
Called “the Father of Modern Geology.”
 First to articulate the “Principle of Uniformitarianism.”
 Of the abyss of time, Hutton wrote: “we find no vestige of
a beginning; no prospect of an end.”


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic Time


James Hutton’s Principle of Uniformitarianism.


“The present is the key to the past.”
Processes seen today are the same as those of the past.

Ancient mudcracks formed as mudcracks do today.
Geologic change is slow; large changes require large times.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic Time


There are two ways of dating geological materials.


Relative ages – Based upon order of formation.
Qualitative method developed 100s of years ago.
Permit determination of older vs. younger relationships.



Numerical ages – Actual number of years since an event.
Quantitative method developed recently.
Age is given a number.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Relative vs. Absolute
Relative ages
assign order
to events.
 Numerical ages
assign exact
dates to events.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Relative Age


Logical tools are useful for defining relative age.
Principle of uniformitarianism.
 Principle of superposition.
 Principle of original horizontality.
 Principle of original continuity.
 Principle of cross-cutting relationships.
 Principle of inclusions.
 Principle of baked contacts.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic Time


Uniformitarianism – The present is key to the past.
Physical processes that we observe today operated in the
same way in the geological past.
 Modern processes help us understand ancient events.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Defining Relative Age


Superposition.


In an undeformed sequence of layered rocks…
Each bed is older than the one above and…
Younger than the one below.



Younger strata are on top; older strata below.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Relative Age


Horizontality and continuity.
Strata often form laterally extensive horizontal sheets.
 Subsequent erosion dissects once-continuous layers.
 Flat-lying rock layers are unlikely to have been disturbed.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Relative Age


Cross-cutting relations.
Younger features truncate (cut across) older features.
 Faults, dikes, erosion, etc., must be younger than the
material that is faulted, intruded, or eroded.
 A volcano cannot intrude rocks that aren’t there yet.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Relative Age


Inclusions – A rock fragment within another.
Igneous xenoliths – Country rock that fell into magma.
 Weathering rubble – Debris from pre-existing rocks.




The inclusion is older than the material enclosing it.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Relative Age


Baked contacts.
Thermal metamorphism occurs when country rock is
invaded by a plutonic igneous intrusion.
 The baked rock must have been there first (it is older).


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Relative Age


Determining relative ages empowers geologists to
easily unravel complicated geologic histories.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic History


Deposition of horizontal strata below sea level in
order 1, 2, 3, 4, 5, 6, 7, and 8 (oldest to youngest).

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic History


Igneous intrusion of a sill.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic History


Tectonic compression and folding.




Beds had to be present to be folded.

Uplift above sea level and erosion.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic History


Intrusion of a granitic igneous pluton.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic History


Extensional normal faulting.


Faulting cross-cuts the older granitic pluton.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic History


Intrusion of a dike.


Dike cross-cuts the normal fault.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic History


Erosion to present landscape configuration.


Erosion removed the volcano and cross-cuts the dike.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic History
Relative ages help to unravel a complicated history.
 Simple rules permit one to decipher this diagram.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Fossil Succession
Fossil remnants, or traces of once living organisms,
are often preserved in sedimentary rocks.
 Fossil are useful for relative age determination.


Several types of fossils will occur as an assemblage.
 Fossils are time markers.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Fossil Succession
Species evolve, exist for a time, and then go extinct.
 First appearance, range, and extinction dates rocks.
 Fossils succeed one another in a known order.
 A time period is recognized by its fossil content.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Fossil Succession


Fossil range – First and last appearance.
Each fossil has a unique range.
 Overlapping ranges provide
distinctive time markers.




Permit correlation of strata.
Locally.
 Regionally.
 Globally.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Unconformities


An unconformity is a time gap in the rock record.
Nondeposition.
 Erosion.




There are three types of unconformity.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Unconformities


Three unconformity types:


Disconformity – Parallel strata bracketing nondeposition.
Due to an interruption in sedimentation.
May be difficult to recognize.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Disconformities
Unconformities


Three unconformity types:


Nonconformity – Metamorphic or igneous rocks overlain
by sedimentary strata.
Crystalline ig/met rocks
were exposed by erosion.
Sediment was deposited
on this eroded surface.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Nonconformity
Unconformities


Three unconformity types:


Angular unconformity – Represents a huge gulf in time.
Horizontal marine sediments deformed by orogenesis.
High mountains are eroded away to below sea level.
Sediments deposited horizontally on the erosion surface.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Angular Unconformity


James Hutton was the 1st to realize the enormous
time-significance of angular unconformities.
Mountains created.
 Mountains completely erased.
 New sediment deposition.




Incomprehensible time.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Angular Unconformity


“Hutton’s Unconformity” on Siccar Point, Scotland,
is a common destination for geologists.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Unconformities
Earth history is
recorded in strata.
 Missing strata =
missing history.
 The Grand Canyon.


Thick layers of strata.
 Numerous gaps.
 A partial record of
geological history.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Stratigraphic Correlation


Stratigraphic columns depict strata in a region.
Drawn to scale to accurately portray relative thicknesses.
 Rock types are depicted by graphical fill patterns.
 Divided into formations.


Mapable rock units.


Formations are
separated by contacts.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Stratigraphic Correlation


In 1793, William “Strata” Smith was the first to note
that strata could be matched across distances.
Similar rock types in a similar order.
 Rock layers contained the same distinctive fossils.




After years of work, he made the 1st geologic map.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Stratigraphic Correlation


Lithologic correlation is based on rock type.
Sequence – The relative order in which the rocks occur.
 Limited to correlation between nearby regions.




Fossil correlation – Based on fossils within rocks.


Applicable to much broader areas.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Stratigraphic Correlation


National parks of Arizona and Utah.
Formations can be traced long distances.
 Overlap is seen in the sequences of rock types.
 Overlapping rock columns are used to build a composite.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Correlation among rock strata in 3 national parks.
The Geologic Column


A composite stratigraphic column exists.
Constructed from incomplete sections across the globe.
 It brackets almost the entirety of Earth history.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic Time
The composite column is divided into time blocks.
 This is the geologic time scale, Earth’s “calendar.”




The structure of the geologic time scale.
Eons – The largest subdivision of time (100s to 1000s Ma).
Eras – Subdivisions of an eon (65 to 100s Ma).
Periods – Subdivisions of an era (2 to 70 Ma).
Epochs – Subdivisions of a period (0.011 to 22 Ma).

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic Time


Time scale subdivisions are variously named.
The nature of life (“zoic” means life); i.e., Proterozoic.
 A characteristic of the time period; i.e., Carboniferous.
 A specific locality; i.e., Devonian.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
The Geologic Time
Scale
Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic Time and Life









Life first appears on Earth ~ 3.8 Ga.
Early life consisted of anaerobic
single-celled organisms.
Oxygen from cyanobacteria
built up by 2 Ga.
~ 700 Ma, multicellular
life evolved.
~ 542 Ma marks the
1st appearance
of hard shells.




Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Shells increased fossil
preservation.
Life diversified rapidly –
the “Cambrian Explosion.”
Chapter 12: Deep Time: How Old Is Old?
The Geologic Time Scale


Names of the eons.


Phanerozoic – “Visible life” (542 Ma to the present).
Started 542 Ma at the Precambrian – Cambrian boundary.
Marks the 1st appearance of hard shells.
Life diversified rapidly afterward.



Proterozoic – “Before life” (2.5 to 0.542 Ga).
Development of tectonic plates like those of today.
Buildup of atmospheric O2; multicellular life appears.



Archean – “Ancient” (3.8 to 2.5 Ga).
Birth of continents.
Appearance of the earliest life forms.



Hadean – “Hell” (4.6 to 3.8 Ga).
Internal differentiation.
Formation of the oceans and secondary atmosphere.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
The Geologic Time Scale


Names of the eras.


Cenozoic – “Recent life.”
65.5 Ma to present.
The “Age of Mammals.”



Mesozoic – “Middle life.”
251 to 65.5 Ma.
The “Age of Dinosaurs.”



Paleozoic – “Ancient life.”
542 to 251 Ma.
Life diversified rapidly.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Numerical Age
The relative age of geologic events is established.
 Based on radioactive decay of atoms in minerals.


Radioactive decay proceeds at a known, fixed rate.
 Radioactive elements act as internal clocks.




Numerical dating is also called geochronology.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Radioactive Decay
Isotopes – Atoms with the same # of protons,
different # of neutrons.
 Isotopes have similar but different mass numbers.


Stable – Isotopes that never change (i.e., 13C).
 Radioactive – Isotopes that spontaneously decay.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Radioactive Decay


Radioactive decay progresses along a decay chain.
Decay creates new unstable elements that also decay.
 Decay proceeds to a stable element endpoint.


Parent isotope – The isotope that undergoes decay.
 Daughter isotope – The product of this decay.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Radioactive Decay


Half-life (t½) – Time for ½ unstable nuclei to decay.



After one t½ half of the original parent remains.





t½ is a characteristic of each isotope.
After three t½ an eighth of the original parent remains.

As the parent disappears, the daughter “grows in”.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Radiometric Dating


The age of a mineral can be determined by…
Measuring the ratio of parent to daughter isotopes.
 Calculating the amount of time by using the known t½.


Must pick the right mineral and the right isotope.
 Geochronology requires analytical precision.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
What Is a Radiometric Date?


Radiometric dates give the time a mineral began to
preserve all atoms of parent and daughter isotopes.
Requires cooling below a “blocking temperature.”
 If rock is reheated, the radiometric clock can be reset.


Ig / Met rocks are best for geochronologic work.
 Sedimentary rocks cannot be directly dated.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Other Numerical Ages


Numerical ages are possible without isotopes.
Growth rings – Annual layers from trees or shells.
 Rhythmic layering – Annual layers in sediments or ice.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Other Numerical Ages


Magnetostratigraphy – Magnetic signatures in
strata are compared to the global reference
column.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Other Numerical Ages


Fission-track analysis – Measuring decay paths.
Radioactive decay particles scar crystals.
 The number of scars is proportional to age.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Dating the Geologic Column
Geochronology less useful for sediment deposits.
 It can, however, constrain these deposits.
 Sediments can be bracketed by absolute dates.


Yields age ranges that improve as data accumulates.
 Defines major boundaries in the geologic column.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
The Age of the Earth


Before radioactivity-based
dating methods…
20 Ma – From Earth cooling.
 90 Ma –Ocean salinization.


Assumed oceans were
initially freshwater.
Measured the mass of
dissolved material in rivers.


Uniformitarianism and
evolution indicated an Earth
older than ~100 Ma.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
The Age of the Earth
The oldest rocks on Earth’s surface date to 3.96 Ga.
 Zircons in ancient sandstones date to 4.1-4.2 Ga.
 Age of Earth is 4.57 Ga based on correlation with…


Meteorites.
 Moon rocks.


Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic Time
The immensity of time is beyond comprehension.
 Metaphors illustrate the scale of time.


The age of Earth (4.6 Ga) can be compared to pennies.
 Lined up, 4.6 billion pennies would be 87,400 km long.


More than twice around Earth.

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
Geologic Time

Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?
This concludes the
Chapter 12
Deep Time: How Old Is Old?

LECTURE OUTLINE

earth

Portrait of a Planet

Third Edition
©2008 W. W. Norton & Company, Inc.
Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak

Chapter 12: Deep Time: How Old Is Old?

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Op ch12 lecture_earth3, geological time

  • 1. Chapter 12 Deep Time: How Old Is Old? LECTURE OUTLINE earth Portrait of a Planet Third Edition ©2008 W. W. Norton & Company, Inc. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 2. Deep Time: How Old Is Old? Prepared by Ronald Parker Earlham College Department of Geosciences Richmond, Indiana
  • 3. Geologic Time Discovering the magnitude of the Earth’s past was a momentous discovery in the history of humanity.  This discovery forever altered our perception of ourselves within nature and the Universe.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 4. Geologic Time  Understanding time permits assigning an age to… Rocks.  Fossils.  Geologic structures.  Landscapes.  Tectonic events.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 5. Geologic Time Deep time – The immense span of geologic time.  It is so vast that it is difficult for people to grasp.   We think of time in terms of our lives… The lives of our parents and grandparents. The lives of our children or grandchildren.  Human history is tiny compared to geologic time. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 6. Geologic Time  Prior to the late 17th century, geologic time was thought to be the same as historical time.  Archbishop James Ussher of Armagh, Ireland, 1654. He added up generations from the Old Testament. He determined that Earth formed on October 23, 4004 BCE. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 7. Geologic Time  Scientists began to find clues to an ancient Earth.  Nicolaus Steno (1638–1686) – Danish physician. Observed marine fossils high in the Apennines. Deduced that these were ancient animals in loose sediment. Lithification and uplift suggested long periods of time. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 8. Geologic Time  James Hutton (1726-1797) – Scottish physician. Called “the Father of Modern Geology.”  First to articulate the “Principle of Uniformitarianism.”  Of the abyss of time, Hutton wrote: “we find no vestige of a beginning; no prospect of an end.”  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 9. Geologic Time  James Hutton’s Principle of Uniformitarianism.  “The present is the key to the past.” Processes seen today are the same as those of the past. Ancient mudcracks formed as mudcracks do today. Geologic change is slow; large changes require large times. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 10. Geologic Time  There are two ways of dating geological materials.  Relative ages – Based upon order of formation. Qualitative method developed 100s of years ago. Permit determination of older vs. younger relationships.  Numerical ages – Actual number of years since an event. Quantitative method developed recently. Age is given a number. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 11. Relative vs. Absolute Relative ages assign order to events.  Numerical ages assign exact dates to events.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 12. Relative Age  Logical tools are useful for defining relative age. Principle of uniformitarianism.  Principle of superposition.  Principle of original horizontality.  Principle of original continuity.  Principle of cross-cutting relationships.  Principle of inclusions.  Principle of baked contacts.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 13. Geologic Time  Uniformitarianism – The present is key to the past. Physical processes that we observe today operated in the same way in the geological past.  Modern processes help us understand ancient events.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 14. Defining Relative Age  Superposition.  In an undeformed sequence of layered rocks… Each bed is older than the one above and… Younger than the one below.  Younger strata are on top; older strata below. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 15. Relative Age  Horizontality and continuity. Strata often form laterally extensive horizontal sheets.  Subsequent erosion dissects once-continuous layers.  Flat-lying rock layers are unlikely to have been disturbed.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 16. Relative Age  Cross-cutting relations. Younger features truncate (cut across) older features.  Faults, dikes, erosion, etc., must be younger than the material that is faulted, intruded, or eroded.  A volcano cannot intrude rocks that aren’t there yet.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 17. Relative Age  Inclusions – A rock fragment within another. Igneous xenoliths – Country rock that fell into magma.  Weathering rubble – Debris from pre-existing rocks.   The inclusion is older than the material enclosing it. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 18. Relative Age  Baked contacts. Thermal metamorphism occurs when country rock is invaded by a plutonic igneous intrusion.  The baked rock must have been there first (it is older).  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 19. Relative Age  Determining relative ages empowers geologists to easily unravel complicated geologic histories. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 20. Geologic History  Deposition of horizontal strata below sea level in order 1, 2, 3, 4, 5, 6, 7, and 8 (oldest to youngest). Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 21. Geologic History  Igneous intrusion of a sill. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 22. Geologic History  Tectonic compression and folding.   Beds had to be present to be folded. Uplift above sea level and erosion. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 23. Geologic History  Intrusion of a granitic igneous pluton. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 24. Geologic History  Extensional normal faulting.  Faulting cross-cuts the older granitic pluton. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 25. Geologic History  Intrusion of a dike.  Dike cross-cuts the normal fault. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 26. Geologic History  Erosion to present landscape configuration.  Erosion removed the volcano and cross-cuts the dike. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 27. Geologic History Relative ages help to unravel a complicated history.  Simple rules permit one to decipher this diagram.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 28. Fossil Succession Fossil remnants, or traces of once living organisms, are often preserved in sedimentary rocks.  Fossil are useful for relative age determination.  Several types of fossils will occur as an assemblage.  Fossils are time markers.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 29. Fossil Succession Species evolve, exist for a time, and then go extinct.  First appearance, range, and extinction dates rocks.  Fossils succeed one another in a known order.  A time period is recognized by its fossil content.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 30. Fossil Succession  Fossil range – First and last appearance. Each fossil has a unique range.  Overlapping ranges provide distinctive time markers.   Permit correlation of strata. Locally.  Regionally.  Globally.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 31. Unconformities  An unconformity is a time gap in the rock record. Nondeposition.  Erosion.   There are three types of unconformity. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 32. Unconformities  Three unconformity types:  Disconformity – Parallel strata bracketing nondeposition. Due to an interruption in sedimentation. May be difficult to recognize. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 34. Unconformities  Three unconformity types:  Nonconformity – Metamorphic or igneous rocks overlain by sedimentary strata. Crystalline ig/met rocks were exposed by erosion. Sediment was deposited on this eroded surface. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 36. Unconformities  Three unconformity types:  Angular unconformity – Represents a huge gulf in time. Horizontal marine sediments deformed by orogenesis. High mountains are eroded away to below sea level. Sediments deposited horizontally on the erosion surface. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 37. Angular Unconformity  James Hutton was the 1st to realize the enormous time-significance of angular unconformities. Mountains created.  Mountains completely erased.  New sediment deposition.   Incomprehensible time. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 38. Angular Unconformity  “Hutton’s Unconformity” on Siccar Point, Scotland, is a common destination for geologists. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 39. Unconformities Earth history is recorded in strata.  Missing strata = missing history.  The Grand Canyon.  Thick layers of strata.  Numerous gaps.  A partial record of geological history.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 40.
  • 41. Stratigraphic Correlation  Stratigraphic columns depict strata in a region. Drawn to scale to accurately portray relative thicknesses.  Rock types are depicted by graphical fill patterns.  Divided into formations.  Mapable rock units.  Formations are separated by contacts. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 42. Stratigraphic Correlation  In 1793, William “Strata” Smith was the first to note that strata could be matched across distances. Similar rock types in a similar order.  Rock layers contained the same distinctive fossils.   After years of work, he made the 1st geologic map. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 43. Stratigraphic Correlation  Lithologic correlation is based on rock type. Sequence – The relative order in which the rocks occur.  Limited to correlation between nearby regions.   Fossil correlation – Based on fossils within rocks.  Applicable to much broader areas. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 44. Stratigraphic Correlation  National parks of Arizona and Utah. Formations can be traced long distances.  Overlap is seen in the sequences of rock types.  Overlapping rock columns are used to build a composite.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 45. Correlation among rock strata in 3 national parks.
  • 46. The Geologic Column  A composite stratigraphic column exists. Constructed from incomplete sections across the globe.  It brackets almost the entirety of Earth history.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 47. Geologic Time The composite column is divided into time blocks.  This is the geologic time scale, Earth’s “calendar.”   The structure of the geologic time scale. Eons – The largest subdivision of time (100s to 1000s Ma). Eras – Subdivisions of an eon (65 to 100s Ma). Periods – Subdivisions of an era (2 to 70 Ma). Epochs – Subdivisions of a period (0.011 to 22 Ma). Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 48. Geologic Time  Time scale subdivisions are variously named. The nature of life (“zoic” means life); i.e., Proterozoic.  A characteristic of the time period; i.e., Carboniferous.  A specific locality; i.e., Devonian.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 49. The Geologic Time Scale Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 50. Geologic Time and Life      Life first appears on Earth ~ 3.8 Ga. Early life consisted of anaerobic single-celled organisms. Oxygen from cyanobacteria built up by 2 Ga. ~ 700 Ma, multicellular life evolved. ~ 542 Ma marks the 1st appearance of hard shells.   Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Shells increased fossil preservation. Life diversified rapidly – the “Cambrian Explosion.” Chapter 12: Deep Time: How Old Is Old?
  • 51. The Geologic Time Scale  Names of the eons.  Phanerozoic – “Visible life” (542 Ma to the present). Started 542 Ma at the Precambrian – Cambrian boundary. Marks the 1st appearance of hard shells. Life diversified rapidly afterward.  Proterozoic – “Before life” (2.5 to 0.542 Ga). Development of tectonic plates like those of today. Buildup of atmospheric O2; multicellular life appears.  Archean – “Ancient” (3.8 to 2.5 Ga). Birth of continents. Appearance of the earliest life forms.  Hadean – “Hell” (4.6 to 3.8 Ga). Internal differentiation. Formation of the oceans and secondary atmosphere. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 52. The Geologic Time Scale  Names of the eras.  Cenozoic – “Recent life.” 65.5 Ma to present. The “Age of Mammals.”  Mesozoic – “Middle life.” 251 to 65.5 Ma. The “Age of Dinosaurs.”  Paleozoic – “Ancient life.” 542 to 251 Ma. Life diversified rapidly. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 53. Numerical Age The relative age of geologic events is established.  Based on radioactive decay of atoms in minerals.  Radioactive decay proceeds at a known, fixed rate.  Radioactive elements act as internal clocks.   Numerical dating is also called geochronology. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 54. Radioactive Decay Isotopes – Atoms with the same # of protons, different # of neutrons.  Isotopes have similar but different mass numbers.  Stable – Isotopes that never change (i.e., 13C).  Radioactive – Isotopes that spontaneously decay.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 55. Radioactive Decay  Radioactive decay progresses along a decay chain. Decay creates new unstable elements that also decay.  Decay proceeds to a stable element endpoint.  Parent isotope – The isotope that undergoes decay.  Daughter isotope – The product of this decay.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 56. Radioactive Decay  Half-life (t½) – Time for ½ unstable nuclei to decay.   After one t½ half of the original parent remains.   t½ is a characteristic of each isotope. After three t½ an eighth of the original parent remains. As the parent disappears, the daughter “grows in”. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 57. Radiometric Dating  The age of a mineral can be determined by… Measuring the ratio of parent to daughter isotopes.  Calculating the amount of time by using the known t½.  Must pick the right mineral and the right isotope.  Geochronology requires analytical precision.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 58.
  • 59. What Is a Radiometric Date?  Radiometric dates give the time a mineral began to preserve all atoms of parent and daughter isotopes. Requires cooling below a “blocking temperature.”  If rock is reheated, the radiometric clock can be reset.  Ig / Met rocks are best for geochronologic work.  Sedimentary rocks cannot be directly dated.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 60. Other Numerical Ages  Numerical ages are possible without isotopes. Growth rings – Annual layers from trees or shells.  Rhythmic layering – Annual layers in sediments or ice.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 61. Other Numerical Ages  Magnetostratigraphy – Magnetic signatures in strata are compared to the global reference column. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 62. Other Numerical Ages  Fission-track analysis – Measuring decay paths. Radioactive decay particles scar crystals.  The number of scars is proportional to age.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 63. Dating the Geologic Column Geochronology less useful for sediment deposits.  It can, however, constrain these deposits.  Sediments can be bracketed by absolute dates.  Yields age ranges that improve as data accumulates.  Defines major boundaries in the geologic column.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 64. The Age of the Earth  Before radioactivity-based dating methods… 20 Ma – From Earth cooling.  90 Ma –Ocean salinization.  Assumed oceans were initially freshwater. Measured the mass of dissolved material in rivers.  Uniformitarianism and evolution indicated an Earth older than ~100 Ma. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 65. The Age of the Earth The oldest rocks on Earth’s surface date to 3.96 Ga.  Zircons in ancient sandstones date to 4.1-4.2 Ga.  Age of Earth is 4.57 Ga based on correlation with…  Meteorites.  Moon rocks.  Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 66. Geologic Time The immensity of time is beyond comprehension.  Metaphors illustrate the scale of time.  The age of Earth (4.6 Ga) can be compared to pennies.  Lined up, 4.6 billion pennies would be 87,400 km long.  More than twice around Earth. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 67. Geologic Time Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?
  • 68. This concludes the Chapter 12 Deep Time: How Old Is Old? LECTURE OUTLINE earth Portrait of a Planet Third Edition ©2008 W. W. Norton & Company, Inc. Earth: Portrait of a Planet, 3rd edition, by Stephen Marshak Chapter 12: Deep Time: How Old Is Old?