Chapter 12: History of Life on Earth - …teacher.cgs.k12.va.us/bwebster/RHS...
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Chapter 12:
History of Life on Earth
Biology II
Radiometric Dating Scientists estimate that Earth formed
~4.5 bya using a technique called
radiometric dating
Estimation of the age of an object by
measuring its content of certain radioactive
isotopes
Radioisotopes An isotope is a form of an element
whose atomic mass differs from that of
other atoms of the same element
Radioisotope – unstable isotope that
breaks down and gives off energy in the
form of charged particles (radiation)
This radioactive decay
results in isotopes that
are smaller and more
stable
Half-Lives By measuring the proportions of certain
radioactive isotopes and their products of decay, scientists can compute how many half-lives have passed since a rock was formed
Half-life – time it takes for one-half of a given amount of radioisotope to decay
Formation of Life Though present hypotheses differ on
the origin of life on Earth, most scientists agree that it developed through natural chemical and physical processes
Thought to have began when molecules of nonliving matter reacted chemically during the 1st billion years of Earth’s history These chemical reactions produced many
different simple organic molecules that, energized by sun and volcanic heat, eventually formed more complex molecules that became building blocks of the 1st cells
Primordial Soup Model In 1920s, Oparin and Haldane suggested that
Earth’s early oceans contained large amounts
of organic molecules
Oceans believed to have formed when the Earth’s
surface cooled and water vapor in atmosphere
condensed
Became known as primordial soup model,
since oceans were thought to be filled with
many different organic molecules, like a soup
filled with many different vegetables and meat
Formation of Organic
Molecules
Oparin and Haldane hypothesized that
these organic molecules formed
spontaneously in chemical reactions
activated by energy from solar radiation,
volcanic eruptions, and lightning
Formation of Organic
Molecules It is believed that Earth’s early atmosphere
lacked O2, and was instead rich in nitrogen
gas (N2), hydrogen gas (H2), and hydrogen-
containing gases like water vapor, ammonia
(NH3), and methane (CH4)
It was reasoned that electrons in these gases
would have been frequently pushed to higher
energy levels by light particles from sun or
electrical energy in lightning
Without O2, these electrons would be free to react with
hydrogen-rich molecules, forming variety of organic
compounds
The Miller-Urey Experiment Primordial soup model was firs tested
by Miller and Urey in 1953
Placed gases proposed to have existed on early Earth into a device like the one below Provided electrical sparks to simulate lightning
After a few days, they found complex collection of organic molecules in apparatus, including some of life’s basic building blocks
– Amino acids, fatty acids, and other hydrocarbons
Results support hypothesis that some basic chemicals of life could have formed spontaneously under these conditions
The Miller-Urey Experiment
Reevaluating the Miller-Urey
Model Recent discoveries have shown that
molecules used in Miller’s experiment could
not have existed in abundance on early Earth
Ozone layer did not exist, meaning that UV
radiation would have destroyed any ammonia and
methane present in atmosphere
In absence of these gases, key biological
molecules are not made in experiment
If these chemicals needed to form life were not
in atmosphere, where did they come from???
The Bubble Model In 1986, Louis Lerman suggested that
key processes that formed the chemicals needed for life took place within bubbles on ocean’s surface
Step 1: Ammonia, methane, and other gases resulting from numerous eruptions of undersea volcanoes were trapped in underwater bubbles
Step 2: Bubbles protected gases from UV radiation Chemical reactions would also take place much
faster in bubbles, where reactants would be more concentrated
The Bubble Model
Step 3: Bubbles rose to surface and burst,
releasing simple organic molecules into air
Step 4: Organic molecules were carried
upward by winds and exposed to UV
radiation and lightning, providing energy for
further reactions
Step 5: More complex organic molecules that
formed by further reactions fell into ocean
with rain, starting another cycle
Lerman’s Bubble Model
RNA as the Precursor to
Macromolecules Scientists have not been able to make
proteins or DNA spontaneously under
laboratory conditions
Short chains of RNA,
however, have been made to
form on their own in water
It is hypothesized that RNA was
the 1st self-replicating
information-storage molecule,
and it catalyzed the assembly
of the 1st proteins
Such a molecule would have been
able to change from one generation
to the next
Microspheres and
Coacervates Lab experiments have shown that, in water,
short chains of amino acids can gather
together in tiny drops called microspheres
Scientists think that microspheres
might have been 1st step toward
cellular organization, though they
could not be considered true cells
without heredity
Another type of droplet, called a coacervate,
is composed of molecules of different types,
including linked amino acids and sugars
Origin of Heredity
Most scientist agree that DNA evolved
after RNA, and that RNA “enzymes”
catalyzed the assembly of the earliest
proteins
Some scientists also think that
microspheres that contained RNA
developed a means of transferring their
characteristics to offspring
Not yet understood how DNA, RNA, and
hereditary mechanisms first developed
The First Prokaryotes Fossil – preserved or
mineralized remains or imprint of organism that lived long ago
Oldest known fossils are microscopic fossils of prokaryotes that come from a 2.5 by old rock Marine cyanobacteria, or photosynthetic
prokaryotic organisms, were one of first prokaryotes to evolve
– After 100s of millions of years, the oxygen gas produced by cyanobacteria began to escape into the air
2 Groups of Prokaryotes 2 different groups of prokaryotes
evolved early in Earth’s history
Eubacteria – prokaryotes that contain a chemical called peptidoglycan in their cell walls Include many bacteria that cause disease and
decay, including E.coli
Commonly called bacteria
Archaebacteria – prokaryotes that lack peptidoglycan in their cell walls and have unique lipids in their cell membranes Chemical evidence shows that archaebacteria
and eubacteria diverged very early
The 1st Eukaryotes
1st eukaryotes appeared 1.5 bya
Much larger than prokaryotic cell
Contain nucleus and
other membrane-
bound organelles,
including
mitochondria and
sometimes
chloroplasts, both which contain their own
DNA
Endosymbiosis Most scientists think that mitochondria
and chloroplasts originated through endosymbiosis
Theory proposed in 1966 by Lynn Margulis stating that mitochondria are the descendents of symbiotic, aerobic eubacteria and chloroplasts are the descendents of symbiotic photosynthetic eubacteria
Endosymbiosis
According to the theory, bacteria
entered large cells either as parasites or
undigested prey
Rather than being digested, bacteria began
to live inside host cell, where they
performed either cellular respiration
(mitochondria) or photosynthesis
(chloroplasts)
Support for Endosymbiosis Both mitochondria and chloroplasts have
characteristics similar to those of bacteria Size and structure: mitochondria are about same
size as most eubacteria and chloroplasts are same size as some cyanobacteria Both have 2 membranes
Both chloroplasts and cyanobacteria contain thylakoids
Genetic material: both have unique and circular DNA similar to chromosomes found in bacteria
Ribosomes: both have ribosomes similar in size and structure to bacterial ribosomes
Reproduction: both reproduce by simple fission, which takes place independently of cell cycle of host cell
Multicellularity Unicellular body plan has been very
successful, with unicellular organisms today
making about half of Earth’s biomass
Single cell must carry out all activities of organisms,
unlike in multicellular organisms, where distinct
types of cells have specialized function
1st multicellular fossils found in 700 my old rock
The 1st eukaryotic kingdom was kingdom
Protista
Protists - make up large, varied group that includes
both multicellular and unicellular organisms
Other 3 kingdoms evolved later and also consist of
eukaryotes
Origin of Modern Organisms Most animal phyla that exist today probably
originated during late Precambrian and
Cambrian periods (10-100 mya)
Rapid diversification of animals is sometimes known
as “Cambrian explosion”
Very rich collection of Cambrian fossils uncovered in
1909 in geological formation in Canada called
Burgess Shale
Ordovician period (505-438 mya) followed
Cambrian, and many different animals,
including trilobites, marine arthropods that went
extinct 250 mya, continued to inhabit the seas
Mass Extinctions Fossil record indicates that sudden change
occurred at end of Ordivician, ~440 mya
Large percentage of organisms on Earth suddenly
became extinct
Extinction – death of all members of a species
This was 1st of 5 major mass extinctions that have
occurred on Earth
Mass extinction – episode during which large numbers
of species become extinct
Another mass extinction of about same size
occurred 360 mya, followed by the 3rd, most
devastating mass extinction ~245 mya, at end of
Permian (96% of all species went extinct)
Mass Extinctions 4th mass extinction took place 35 my later,
followed by 5th mass extinction, ~65 mya, when 2/3 of land species, including dinosaurs, went extinct
Some scientists think that another mass extinction is occurring today Earth’s ecosystems, including rainforests, are
being destroyed by human activity
½ of all tropical rain forests have already been destroyed
At this rate, 22-47% of Earth’s plant species will be lost, along with 2,000 of 9,000 species of birds, and countless insect species
The Ozone Layer About 2.5 bya, photosynthesis by
cyanobacteria began adding oxygen to Earth’s atmosphere
As oxygen reached upper atmosphere, it reacted chemically with sunlight, forming molecules of ozone, which blocks the sun’s harmful UV rays After
millions of years, enough ozone layer had accumulated to make Earth’s land a safe place to live
Plants and Fungi on Land 1st multicellular organisms to live on
land may have been fungi living
together with plants or algae, about 430
mya
Early plants and fungi formed biological
partnerships called mycorrhizae, which
enabled them to live on harsh habitat of
bare rock
Fungus provides minerals to plant, and plant
provides nutrients to fungus
– Mutualism – relationship between 2 species in
which both species benefit
Arthropods 1st animals to successfully invade land were
arthropods
Arthropod – kind of animal with a hard outer
skeleton, segmented body, and paired, jointed
limbs
Include lobsters, crabs, insects, and spiders
The insect evolved from the 1st land dwellers
and were the first animals to have wings
Allowed insects to efficiently search
for food, mates, and nesting sites
Also led to partnership between
insects and flowering plants
Vertebrates
Vertebrate – animal with a backbone
1st vertebrates were jawless fish that
evolved in oceans ~530 mya
Jawed fish 1st appeared ~430 mya
– Jaws enabled fish to bite and chew food,
making them more efficient predators
Fish are most successful
living vertebrate, making
up more than half of all
modern vertebrate
species
Amphibians 1st land vertebrates were early
amphibians that evolved 370 mya
Amphibians are smooth-skinned, 4-legged animals that include frogs, toads, and salamanders
Several structural changes occurred as adaptations to life on land Lungs to absorb oxygen
from air
Strong, flexible internal skeleton
Limbs derived from bones of fish fins
Reptiles
Reptiles evolved from amphibian
ancestors ~340 mya
Include snakes, lizards, turtles, and
crocodiles
Better suited to
dry land than
amphibians
Watertight skin
Watertight eggs
Mammals and Birds Birds are thought to have evolved from
feathered dinosaurs during or after Jurassic
Therapsids, reptiles with complex teeth and legs positioned beneath their body, gave rise to mammals about the same time that dinosaurs evolved, during the Triassic After 5th mass extinction 65 mya, birds and
mammals became dominant vertebrates on land, since dinosaurs went extinct
Continental drift – movement of Earth’s land masses over Earth’s surface through geological time Both extinction and continental drift played large
role in evolution