Geology - All Los - G11 - S2
Geology - All Los - G11 - S2
Geology - All Los - G11 - S2
• The heat in this young Earth was 3 times of the internal heat of Earth now . The
very young Earth is called Hadean . Named for Hades the god of the underworld
in the Greek mythology .
• After while , the hit of meteorites and eruption of volcanos were slowed down .
That resulted in the cooling down of OUTSIDE of Earth .
• In that time , A few minerals begun to crystalize and something like scum
patches begun to form in the molten surface and they were able to move around
a lot which resulted in the destruction of the unstable surface of the Hadean by
melting .
• Also this melting was an impact of meteorites . Some of the
melted material was recycled into the mantle .
• Because of the high temperatures in the upper mantle , most of
the oceanic and continental crust was in the form of BASALT
which had the ability to stay stable in high temperatures like
those who crystalize in the mid-ocean ridges ( explained in the
upcoming slide ) .
• Due to the melting and remelting of basalt rock , GRANITE was
formed as recycled rocks .
The oldest material on Earth
• Zircon is the oldest continental material in Earth’s surface , its
chemical name is zirconium silicate . It is hard and durable .
• It was originally formed as igneous rock which means that it was
formed due to cooling of magma but due to the weathering
process it was recycled to younger sedimentary rocks .
• Its age is nearly 4.4 billion years old .
• Its image :
Mid-ocean Ridges
• It is something related to plate tectonics but here is a quick hint
for what is it helpful for and why does it happen :
https://youtu.be/3ZpDjdFzQUM
Recapping
• The plate tectonics happened due to the conventual currents that
happened due to the transmission of the heat restored in the
core after it the mantle
• Plate tectonics got 3 different types :
1-CONVERGENT plate boundary
2-TRANSFORM plate boundary
3-DIVERGENT plate boundary
Convergent Plate Boundary
• Continental crust and Continental crust , this forms high
mountains like Himalaya Mountains which happened due to the
Collison of 2 continental plates ( Eurasian and Indian plates )
• Continental crust and Oceanic crust , this forms subduction zones
where these zone happens due to Collison of a continental crust
with an oceanic crust making the oceanic crust bulks under the
continental crust because oceanic crust got high density , this
results in volcanos in the sides of the continental crusts .
• Oceanic crust and Oceanic crust , this forms island arcs where this
formed due to the Collison of 2 oceanic crusts , one of them will
buckle under the other forming these arcs ( orogeny )
Divergent Plate Boundary
• Continental crust and Continental crust , this forms the rifts we
see in the deserts where this happens due to the diverges of both
of 2 continental crusts .
• Oceanic crust and Oceanic crust , this forms the rifts in the sea
where this happens due to the diverges of both 2 oceanic crust .
https://youtu.be/6LkmD6B2ncs
LO 10 :
The release of gases from earth’s interior
Gases and liquids in Mantle rocks
• Everyone of us must observed that when you open a carbonated
beverage (Coca-Cola) which contains dissolved gas in it , the gas flow
away this is the reason for the reduction of pressure .
• The reason you do not see bubbles in an unopened bottle is
because the pressure of the outside of the bottle restricts
the movement of the gas in the liquid. This prevents the gas
from escaping .
• Heating the opened bottle increases the rate at which the gas
escapes.
• There are some gases dissolved in earth’s hot mantle which are:
carbon dioxide, nitrogen, and water vapor.
• Mantle is subjected to very high pressures , this pressure could range
between 250,000 to 1.7 million times of the atmospheric pressure .
• This high pressure make the dissolved gases (carbon dioxide , nitrogen
, water vapor) remain in equilibrium in their environment . Remember
the example of the carbonated beverage
• During volcanic activity, molten rock rises through the crust. The
environmental conditions change. As the depth below the surface
decreases, the mass of the overlying crust decreases. Therefore, the
pressure on the rising magma also decreases . With a decrease in
pressure, gases dissolved within the magma are released.
• Earth’s rocky lithospheric plates contain special minerals.
These minerals can hold water within their crystals. Mineral
matter in Earth’s mantle also contains water.
• According to several experiments done by scientists in Japan
in order to know about the relation between the pressure
and the ability for crystals to carry water in it , They found
that at this great pressure the rocks in the mantle are able to
contain huge volumes of dissolved water vapor.
• There is debate that the mantle contains volume of water
greater than all the water in Earth’s ocean .
• Many crystals in Earth’s crust begin to form in some kind of
fluid. As these crystals grow, they often trap tiny bubbles of
the fluid. This provides important information about the
conditions under which the crystals formed. By heating the
bubbles, scientists can find the temperature and pressure at
which the crystals formed. One instrument used for this was
designed by the USGS. It is extremely sensitive. It is capable
of detecting amounts as low as 8 parts per billion in samples
as small as 0.01 mm in diameter.
A microscopic fluid inclusion within a quartz
grain
• Gases dissolved in Earth’s mantle are released into the atmosphere during
volcanic eruptions. These can occur when a plate descends downward
into the mantle. The plate can get so hot that any water or gas it contains
rises into the overlying mantle. The overlying mantle melts into magma.
The magma is less dense than the solid rock that surrounds it. It then rises
through the mantle to the overlying crust. As it nears Earth’s surface,
there is less overlying rock. The pressure on the magma decreases. At the
surface, the magma is under atmospheric pressure. Gases such as carbon
dioxide, nitrogen, sulphur dioxide, and water vapor dissolved in the magma
are released into the atmosphere .
• Various volcanic processes release dissolved gases from Earth’s mantle.
These include continental and oceanic volcanic eruptions, outpouring of
lava flows, and rifting. Also included are rising plumes at hot spots and at
mid-ocean ridges. During these processes, hot material from the deep
mantle reaches Earth’s surface. As this takes place, any dissolved gases it
contains are released.
Plate which
descends down
The Evolution of Earth’s Fluid spheres
• Earth’s interior has been releasing gases since its formation 4.6 billion
years ago. These gases were trapped within the solid rock particles that
came together under the influence of gravity to form Earth. Over time,
Earth mas increased by more and more rocky debris was pulled in from
the solar system. As Earth’s mass increased, its gravity grew. The
pressure increased on its interior , then its interior heated and melted.
• Meteorites bombarded the surface of the young Earth. This caused its
primitive crust to melt and rift. As this occurred, large amounts of gases
were released through fissures in Earth’s surface. As this occurred, large
amounts of gases were released through fissures in Earth’s surface.
• Earth’s gravity kept these gases from being stripped away by the
solar wind and blowing off into space. The process by which huge
volcanic eruptions transfer matter from the mantle to the
atmosphere is called outgassing.
Outgassing
• The release of gases from Earth’s interior that formed the
primordial
atmosphere and continues today.
• Outgassing early in Earth’s history produced primoradial atmosphere
(largely water vapor and carbon dioxide). There were also lesser
amounts of carbon monoxide, hydrogen, and hydrogen chloride.
• In contrast to the atmosphere today, oxygen was mostly absent.
• During the early Hadean, Earth’s surface temperature was extremely
hot. It was too hot for water to exist as a liquid at the surface. As a
result, there were no oceans, lakes, rivers, or groundwater.
• As the young Earth cooled, outgassing formed a new atmosphere. It is
consists of (methane, hydrogen, nitrogen, and water vapor, with
smaller amounts of noble gases and carbon dioxide). Noble gases like
helium.
• Earth’s cooler surface radiated less heat into the atmosphere. Further
cooling enabled water vapor to condense. It fell to the surface as rain.
Much of the first rains would have fallen on hot volcanic rock and
evaporated. As the crust cooled more, rain began to collect in low-
lying areas. This formed bodies of water on the surface. Eventually,
enough water was released from Earth and condensed to form the
world’s oceans .
• On the primitive continents, Earth’s first river networks formed. The
rivers flowed and transported rock particles worn from the
continents. These sediments built up in the oceans. They formed early
marine sedimentary rocks .
• The outgassing of carbon dioxide produced rainfall and oceans that
were more acidic than today: Because carbon dioxide, when
combined with water, forms carbonic
` acid. For instance the pH of
early Haden ocean 5.8 and the pH of the ocean now nearly 7.
• Some of the dissolved chemicals would later become limestone and
the shells of marine organisms. Today, the oldest organic marine
limestones are found in western Australia. They are in rocks 3.5 billion
years old.
Formation of oceans and atmosphere
• Some scientists believe that the process of outgassing did not form
the atmosphere and oceans. They argue that the young Earth’s gravity
pulled in chemicals released by the Sun.
• Other scientists think that Earth’s water came from gigantic comets
several kilometers long, passing by Earth. They suggest that Earth’s
gravity pulled in ice and rocky material from these comets.
Interaction between Fluid Sphere and Young
Earth
• Many scientists believe that Earth’s young atmosphere was richer in
greenhouse gases. This kept the planet from freezing over. As the Sun
became brighter, the concentration of greenhouse gases declined.
They eventually reached modern levels. This is known as the faint
young Sun paradox.
• The interaction between the geosphere and the fluid spheres was
very important to the development of the granite rocks that now
make up the continents.
• Earth’s young crust was largely made of basalt weathered from the
crust had more silica. Silica is resistant to chemical and physical
attack. Silica-rich sedimentary rocks built up in the oceans. They later
melted in subduction zones. As a result, the melted basaltic oceanic
crust became richer in silica from the added melted sedimentary
rocks.
Fluid Spheres on Other planets and Moons
• Earth is not the only planetary body in the solar system with fluid
spheres. Venus and Mars both have atmospheres. Like Earth. The
mass of Earth’s atmosphere is about 100 times greater than Mars. It is
100 times less than that of Venus.
• One of Jupiter’s moons, Io, has an atmosphere that is strongly
affected by the Jupiter’s gravitational field. Europa, another of
Jupiter’s moons, has a thin oxygen-rich atmosphere.
• Titan, Saturn’s largest moon, is icy and rocky. It has an atmosphere
rich in nitrogen with clouds of methane.
• Earth’s fluid spheres are unique among the other planets. Earth is the
only planet with abundant free oxygen.
• Venus and Mars also have oxygen, but it is tied up in carbon dioxide
molecules.
• Earth also has abundant water in all three states
Questions
LO.11:
The Biosphere and The Evolution of The
Atmosphere
How scientists detected the Early Atmosphere ?
Chert
• a sedimentary rock made of tiny quartz crystals formed from watery
solutions rich in silica , often grey in colour.
Example for Example for
Branded Iron Formation Chert
• Branded Iron Formations are commonly associated with greenstone
belts. They were moved onto the continents by accretion.
• Accretion is the process by which the cores of ancestral continents
grew by the subduction of adjacent oceanic crust and the welding of
crust to the continental margin which means that accretion happens
when there is island arc in the oceanic crust and at the same time the
oceanic crust is being subducted by the continental crust so that island
arc resist the oceanic crust to be subducted resulting in the accretion
of the both of the plates .
• Scientists think that during the late Hadean the oceans contained vast
amounts of iron and silica. One source of the iron seems to have been
underwater volcanoes. The iron was released in fluids from
hydrothermal vents. There, the material from the upper mantle mixed
with seawater
• Another source for the iron and silica in the oceans was Earth’s
crust.
Earth’s young basaltic crust was rich in minerals that contain iron
and
silica. Earth’s new crust was exposed to the warm primitive
atmosphere. This caused rocks to weather. The weathering process
released iron and silica from the crust. They found their way into
rivers in solution and in mineral fragments. The rivers eventually
deposited the iron and silica into the oceans.
• Iron was being added to seawater for several hundred million years.
However, it was not being removed. Also, at that time, there were no
organisms that required silica to form shells. As a result, the ocean
water became saturated with silica as well. Iron and silica are the
chemicals found in the iron-rich and chert layers that form banded
iron formations
How banded iron formed ?
• Between about 3.5 and 2 billion years ago, the iron and silica
began to
react with oxygen dissolved in Earth’s ancient ocean. Iron
reacted to form iron-oxide minerals. They built up in layers on
the ocean bottom. Silica in the water also reacted with the
oxygen. As a result, layers of silica-rich chert were formed.
• Some scientists think that the layering of banded iron
formations reflects the competing influences of hydrothermal
processes and continental fluxes of material where volcanism
released iron and silica
From where did oxygen come from ?
• Scientists thought that the oxygen must have come from ancient
cyanobacteria. Recall that cyanobacteria are phototrophs. They use
photosynthesis to convert energy from the Sun into food. Oxygen is a
by-product of photosynthesis. The population of cyanobacteria on
Earth increased. As a result, 3.5 to 2.5 billion years ago, more and
more oxygen was released into Earth’s atmosphere.
• Cyanobacteria is considered the first prokaryotic cell to be formed
• The atmosphere and oceans readily exchange gases. As the oxygen
content of the atmosphere increased, the dissolved oxygen content
of
the surface waters in the oceans also increased. Oxygen reacted
with the dissolved iron and silica in the ocean. This resulted in the
layers of the banded iron formations. Until 2.3 billion years ago,
oxygen was drawn down into the oceans. It replaced oxygen used
up in forming the banded iron formations. This kept the
concentration of oxygen in the atmosphere to low levels. The levels
were 1–2 percent of what they are today.
• the deposition of banded iron formations began to slow down.
There was less and less dissolved iron in the oceans. The rate at
which iron was resupplied to the oceans had decreased. By 1.8
billion years ago, there was very little dissolved iron in ocean water.
The banded iron formations stopped forming altogether.
• The cyanobacteria flourished. They continued to produce oxygen.
However, the iron was no longer there to act as a sink for oxygen in the
oceans. Less oxygen was drawn from the atmosphere into the oceans. As
a result, oxygen began to build up in the atmosphere.
• The soils indicate that atmospheric oxygen at the time was 15 percent
that of the modern level. Current levels of oxygen were reached probably
about 600 million years ago .
• Along with a buildup of oxygen, came an increase in ozone levels (O ). The
3
• The longest unit of time and division of geologic time that contains
two or more eras. So far, there have been four eons. Each has its own
unique story.
• The Hadean Eon is the first part of Earth’s history. This part of
Earth’s history lasted 800 million years. During this time, the Moon
formed , and meteorites bombarded the geosphere.
• Toward the end of the Hadean, simple life had gained a foothold on
Earth.
Scientific Notation for Geological time
Archean
Proterozoic
Phanerozoic
Eras
• Eons are divided into shorter units of time called eras which is a major
division of geologic time that contains two or more periods.
• The Phanerozoic Eon is divided into three eras.
The Paleozoic Era is the era of ancient life. It lasted about
290 million years.
The Mesozoic Era is the era of middle life. It lasted about
185 million years.
The Cenozoic Era is the current era of modern life. It has lasted
about 65 million years so far.
• Changes in the mix of animals and plants in the biosphere define the
beginning and end of each era.
• For example, the Mesozoic Era is called the Age of Dinosaurs. It
ended when most of life on Earth became extinct.
• The next is called the Cenozoic Era . It included the evolution of
mammals. Many of these mammals live on Earth today.
Periods
• Eras are divided into shorter units of time called periods. Each period is
named by the scientists who discovered it.
• Sometimes the names are from a particular region like the Cambrian,
Ordovician, and Silurian are names of three periods . They are named after
Welsh tribes.
• Each period lasts tens of millions of years. They subdivide geologic time in a
way similar to how hours divide a day.
• Each one also tells a unique part of Earth’s history. For example, the
Cretaceous Period was when large dinosaurs were abundant. It lasted about
80 million years. After the Cretaceous Period ended, the number of
dinosaurs decreased.
• A new period began. This was called the Paleogene Period. Scientists have
defined this period according to the appearance of a large number of
mammal fossils.
Epoch
• It is part of the geologic time scale. That help define time even more
precisely. This is much like minutes within an hour. Epochs are often
determined by special events in other parts of the Earth system.
Dating Rocks by using Radioactive decay
• Scientists use geologic evidence for many events in Earth’s history.
• Mountains provide evidence of plate collisions or volcanic activity. The
shields that form each continent tell about how Earth’s crust evolved.
• Special iron-rich rocks formed in the oceans tell about how the
atmosphere was formed. Changes in fossil groups indicate changes in
past climates.
• Younger layers of sediments are deposited on top of older layers. This
gives a relative age of a layer of rock. You can identify a rock layer as
being younger or older than the layers next to it.
• Relative age: a date given for a sample expressed as younger than or
older than another rock or fossil.
• Knowing the exact ages of rocks helps them to unravel further some of
the secrets of Earth’s history.
• It can help them to answer questions like: -
1-How old is Earth?
2- When did the first continents form?
3-How long does it take for ocean crust to be recycled in the mantle?
• To determine the absolute age of a rock, scientists look for radioactive
minerals.
• Absolute age: a date given for a sample expressed in years.
• These minerals contain radioactive elements. The nuclei of these
elements are unstable. As a result, they break apart over time. This
process is known as radioactive decay.
• Radioactive decay: the process by which an atomic nucleus of an
unstable atom loses particles
• As particles are released, the original element changes into a different
one. The new element has slightly lighter properties. The atom that
undergoes decay is called the parent atom. The product is called the
daughter atom.
• Parent atom is the atom that undergoes radioactive decay in a
nuclear reaction.
• Daughter atom is the product atom from the radioactive decay of a
parent atom.
• Scientists look at the rate at which a radioactive element in a mineral
decays to determine the age of the rock in which it is contained. The
time it takes for half of the parent atoms to decay into daughter
atoms of a different element is called a half-life.
• Half-life : the length of time it takes for half of a radioactive
substance to decay
• Knowing the half-life of an element and the fraction of parent atoms
left, a decay graph is used to determine when the parent atoms were
fully intact. The date when the rock was formed can then be
determined.
• Example for decay graph :
• The radioactive isotope of rubidium has a very long half-life. It takes
about 48.8 billion years for half of it to change to strontium. Elements
such as this, with very slow rates of decay, are good for finding the
ages of very old rocks.
• Using radioactive decay, scientists have found Earth’s oldest mineral
to be zircon
• Zircon contains small traces of the radioactive element uranium.
(Uranium decays to form lead.)
• Zircon samples have been found that date as far back as 4 billion
years.
• Zircon is highly resistant to weathering and erosion.
Zircon
Radioactive Dating
• Radioactive dating is done mostly on igneous rocks.
• Radioactive elements are trapped in certain minerals when magma
cools and hardens to form rock.
• There are a few types of sedimentary rocks that contain radioactive
elements.
• The radioactive “clock” is reset in new minerals that form when rocks
are deformed. These minerals give a younger age for the rock than
when it originally formed.
Radiocarbon Dating
• Radiocarbon dating is used to find the age of once-living materials between
100 and 50,000 years old. This range is especially useful for determining
ages of human fossils and habitation sites. The atmosphere contains three
isotopes of carbon: carbon-12, carbon-13 and carbon-14. Only carbon-14 is
radioactive , it has a half-life of 5,730 years. The amount of carbon-14 in the
atmosphere is tiny and has been relatively stable through time. Plants
remove all three isotopes of carbon from the atmosphere during
photosynthesis. Animals consume this carbon when they eat plants or other
animals that have eaten plants. After the organism’s death, the carbon-14
decays to stable nitrogen-14 by releasing a beta particle.
• The nitrogen atoms are lost to the atmosphere, but the amount of carbon-
14 that has decayed can be estimated by measuring the proportion of
radioactive carbon-14 to stable carbon- 12. As time passes, the amount of
carbon-14 decreases relative to the amount of carbon-12.
Potassium-Argon dating
• Potassium-40 decays to argon-40 with a half-life of 1.26 billion years.
Argon is a gas so it can escape from molten magma, meaning that any
argon that is found in an igneous crystal probably formed as a result
of the decay of potassium-40. Measuring the ratio of potassium-40 to
argon-40 yields a good estimate of the age of that crystal. Potassium
is common in many minerals, such as feldspar, mica, and amphibole .
With its half-life, the technique is used to date rocks from 100,000
years to over a billion years old. The technique has been useful for
dating fairly young geological materials and deposits containing the
bones of human ancestors.
Uranium-lead dating
• Two uranium isotopes are used for radiometric dating.
Uranium-238 decays to lead-206 with a half-life of 4.47 billion years.
Uranium-235 decays to form lead-207 with a half-life of 704 million years.
• Uranium-lead dating is usually performed on zircon crystals When zircon
forms in an igneous rock, the crystals readily accept atoms of uranium but
reject atoms of lead. If any lead is found in a zircon crystal, it can be
assumed that it was produced from the decay of uranium. Uranium-lead
dating is useful for dating igneous rocks from 1 million years to around 4.6
billion years old. Zircon crystals from Australia are 4.4 billion years old,
among the oldest rocks on the planet.
Questions:
(these slides are animated make sure to
get in the Fullscreen mode)
LO 14:
The fossil record
Food Chains and Food Webs:
• Plants use energy from the Sun to make food through the photosynthesis
process.
• Producers are the organisms that make their own food.
• Consumers are the organisms that rely on plants for food to obtain energy.
• The food chain is a kind of flowchart to show how organisms are connected
to each other by the food they eat. It shows how energy and matter are
transferred from producers to the next levels of consumers.
• The relationships between organisms are
shown in the form of a food web. (as
shown in the figures)
• Decomposers are a special group of
consumers who obtain the matter and
energy they need from wastes and dead
plants and animals.
Fossils:
• Fossils are any evidence of past life preserved in sediments or rocks.
• There are two types of fossils:
1- Body fossil 2- Trace fossils
1-Body fossils:
• They are any remains or imprints of actual organic
material from a creature or plant that has been
preserved in the geologic record (Bones, teeth, shells,
and other hard body parts).
Dinosaur bones
• They may become broken, worn, or even dissolved before they might be
buried by sediment.
• Soft bodies organisms are hard to preserve unless under specific conditions
(such organisms fall into a muddy sea bottom in quiet water and are fossilized)
• For the specific conditions, the fossil record of soft-
bodied organisms is far less well known
• There is a strong bias in the fossil record. Some
organisms rarely have the chance of becoming
fossilized. Under very specific circumstances, however,
even these can become part of the fossil record.
• Bias is a purposeful or accidental distortion of observations,
data, or calculations in a systematic or nonrandom manner
Jellyfish fossil
2-Trace fossil:
• It is a fossilized track, trail, burrow, tube, boring, tunnel or other remnant
resulting from the life activities of an animal.
• In older rocks, the body parts are usually dissolved away, recrystallized or
replaced by another kind of mineral but the imprints are still preserved
which can be studied if the rock splits apart in the right place and the right
orientation .
• Scientest collect rocks and put them on special mechanical splitting devices
to try to find at least a few fossils.
Fossilization:
• only a very small part of what once lived is spared being a meal for some
other organism.
• Decay affects soft body parts and some of the harder, more resistant body
parts.
• Each plant and animal that lives in the forest eventually ends up on the
forest floor in some form.
• Soft tissues of animals, leaves, and
flowers are used by decomposers as they
decay within several weeks or are used by
some other organism as a food source.
• all organisms will decay but there must be other factors at work during or
right after burial to slow or stop decay.
• The conditions necessary for fossilization do not exist everywhere all of the
time but only in a few places and for only a tiny bit of the time.
• huge numbers of organisms have
become fossilized because of the extent
of geologic time.
• It is difficult to imagine how long a
million years is. Yet physical, chemical,
and biological processes have been
operating on Earth not just for millions
of years, but for billions of years.
Fossiliferous limestone
• Some shales are fossiliferous as well because certain organisms like to
live on muddy seafloors.
• Sandstones usually contain much fewer fossils than limestones.
• Fewer kinds of organisms can tolerate the strong currents and shifting
sand beds that are found in areas where sand is being deposited.
• For the same reason, conglomerates are the least fossiliferous of
sedimentary rocks.
LO 15:
Mass Extinction
Textbook:
EarthComm chapter 8 section 9
The Extinction of Species
• It is impossible to predict the success or failure of one species . Many
physical and biological factors interact in complicated ways , all these
factors determine the success or failure of a species.
• Also, the data from the fossil record seem to indicate that different kinds
of organisms have different rates of success.
• It is found that there are species that lasted for tens of millions of years ,
others lasted for hundreds of million of years . Other life spans for
species only lasted for a few million years.
• The 2 main reasons for Extinction are loss of habitat and loss of genetic
variation
The Extinction of Species at the end of Mesozoic
• There was big difference in the landscapes of the Mesozoic Era and
the Cenozoic Era. (The terms come from the Greek meso-, meaning
middle and kainos-, meaning new.)
• The group of animals that dominated the Earth for nearly 130 million
years during Mesozoic suddenly became extinct , the extinction
process mostly took place almost overnight. This sudden extinction
affected some plants and many groups of animals that lived on land. It
affected much of the food web in the oceans as well.
• Groups from phytoplankton to top carnivorous disappeared from
fossil record , they were never be seen again except as a fossil
material.
• Phytoplankton are small photosynthetic organisms, mostly algae and
bacteria, found inhabiting aquatic ecosystem.
• Carnivorous are an organism that eats mostly meat, or the flesh of
animals, sometimes carnivores are called predators.
• The post boundary biosphere was very different in nature. It was
established early in the Paleogene. It took several million years for the
plant and animal groups known to exist now to evolve. It took a long
time to fill all the ecological spaces opened by this extinction event.
• The Paleogene is one of periods in tertiary period of Cenozoic Era.
• The post-boundary fossil record shows that changes in the kinds of
animals now extinct are linked to food source(s). They are related to
the appearance and disappearance of these food sources.
• The fossil record shows that when evolution comes and changes the make up of
plants in a community, dependent organisms must find a new food source. They
must change how they process food for nutrition as well. If they are not able to do
so, they face extinction.
• Until the Mid-Cenozoic, there was no evidence in the fossil record for grazing
animals. About this time grasslands appeared . Following this, many new groups of
animals are found for the first time in the fossil record. The diets of these animals
include the plants of the grasslands like grazing animals .
• In North America, such animals include camels, rhinoceroses, and horses. Also
included are many other mammals that are now known to be extinct. The extinction
of a few species now and then appears to be a normal phenomenon. Scientists refer
to the appearance and disappearance of a few species at any time as background
extinction.
• Background extinction is normal extinction of species that occurs as a result of
changes in local environmental conditions.
Biodiversity & Mass Extinction
• It is the diversity of different biologic species and/or the genetic
variability among individuals within each species.
• Fossil record sometimes show a change in the biodiversity
• A mass extinction event is when species vanish much faster than they
are replaced. This is usually defined as about 75% of the world's
species being lost in a 'short' amount of geological time - less than 2.8
million years.
• The major types of diversities in the biodiversity are genetic diversity,
species diversity, ecological diversity and functional diversity
• There have been five major ones throughout the history of life. During
these, up to 90 percent of the known biodiversity was lost. One such event
took place at the end of the Palaeozoic Era. This was between the Permian
and the Triassic Periods.
• it was more devastating to life on Earth than extinction at the end of
Mesozoic.
• Geologic time is divided into the Palaeozoic, Mesozoic, and Cenozoic
Eras. The specific places the time is divided and the time each era last
has a reason. The reason is the size and abruptness of the extinctions.
Causes of Mass Extinction
• A scientist named Luis Alvarez and his colleagues proposed a hypothesis. It
stated that the extinction was caused by the collision of a huge asteroid
with Earth. They based this on studies of sections through sedimentary
rocks. These rocks were found at the Mesozoic– Cenozoic boundary. In
several sections, they found geochemical evidence. Where amounts of
element iridium in this time was many times greater than normal amounts
of the element iridium. The evidence pointed toward a catastrophic
collision.
• Iridium is very rare on Earth’s crust. Large amounts of iridium are
found on meteorites and comets. Therefore, the iridium was
introduced into the Earth system during certain impacts.
Another Evidence of the collison
• Another important piece of evidence was found in the Yucatán
Peninsula of Mexico. It was the remnants of a colossal impact
structure. This structure is called the Chicxulub crater. The collision
placed so much dust and ash into the atmosphere that the climate
became much cooler. It is thought that light could not reach Earth’s
surface. Earth’s ecosystems were stressed for a long time after the
collision. This led to widespread extinction of many species. Evidence
of sediment movement and deposition by a gigantic sea wave could
be seen in the Gulf of Mexico. This evidence, likely caused by the
impact, has strengthened the hypothesis.
Another Evidence
• There is also good evidence for increased volcanic activity
around this time.
• A few scientists like an alternative hypothesis for the great
extinction. It has to do with climate change induced by the eruption
of the volcanoes. Evidence is still being gathered. There are still details
to resolve about the extinction and its causes.