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The History of Life on Earth
Chapter 25 The History of Life on Earth
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Past organisms were very different from those now alive.
Overview: Lost Worlds Past organisms were very different from those now alive. The fossil record shows macroevolutionary changes over large time scales including. The emergence of terrestrial vertebrates. The origin of photosynthesis. Long-term impacts of mass extinctions.
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Fig. 25-1 Figure 25.1 What does fossil evidence say about where these dinosaurs lived? Figure 25.1 What does fossil evidence say about where these dinosaurs lived?
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Fig 25-UN1 Cryolophosaurus
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Concept 25.1: Conditions on early Earth made the origin of life possible.
Chemical and physical processes on early Earth may have produced very simple cells through a sequence of stages: 1. Abiotic synthesis of small organic molecules. 2. Joining of these small molecules into macromolecules. 3. Packaging of molecules into “protobionts.” 4. Origin of self-replicating molecules.
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Synthesis of Organic Compounds on Early Earth
Earth formed about 4.6 billion years ago, along with the rest of the solar system. Earth’s early atmosphere likely contained water vapor and chemicals released by volcanic eruptions (nitrogen, nitrogen oxides, carbon dioxide, methane, ammonia, hydrogen, hydrogen sulfide).
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A. I. Oparin and J. B. S. Haldane hypothesized that the early atmosphere was a reducing environment.
Stanley Miller and Harold Urey conducted lab experiments that showed that the abiotic synthesis of organic molecules in a reducing atmosphere is possible.
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Video: Hydrothermal Vent
However, the evidence is not yet convincing that the early atmosphere was in fact reducing. Instead of forming in the atmosphere, the first organic compounds may have been synthesized near submerged volcanoes and deep-sea vents. Video: Tubeworms Video: Hydrothermal Vent
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Figure 25.2 A window to early life?
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Amino acids have also been found in meteorites.
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Abiotic Synthesis of Macromolecules
Small organic molecules polymerize when they are concentrated on hot sand, clay, or rock.
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Protobionts Replication and metabolism are key properties of life. Protobionts are aggregates of abiotically produced molecules surrounded by a membrane or membrane-like structure. Protobionts exhibit simple reproduction and metabolism and maintain an internal chemical environment.
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Experiments demonstrate that protobionts could have formed spontaneously from abiotically produced organic compounds. For example, small membrane-bounded droplets called liposomes can form when lipids or other organic molecules are added to water.
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Figure 25.3 Laboratory versions of protobionts
20 µm Glucose-phosphate Glucose-phosphate Phosphatase Starch Amylase Phosphate Maltose Figure 25.3 Laboratory versions of protobionts (a) Simple reproduction by liposomes Maltose (b) Simple metabolism
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(a) Simple reproduction by liposomes
Fig. 25-3a 20 µm Figure 25.3 Laboratory versions of protobionts (a) Simple reproduction by liposomes
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Glucose-phosphate Glucose-phosphate Phosphatase Starch Amylase
Fig. 25-3b Glucose-phosphate Glucose-phosphate Phosphatase Starch Amylase Phosphate Figure 25.3 Laboratory versions of protobionts Maltose Maltose (b) Simple metabolism
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Self-Replicating RNA and the Dawn of Natural Selection
The first genetic material was probably RNA, not DNA. RNA molecules called ribozymes have been found to catalyze many different reactions. For example, ribozymes can make complementary copies of short stretches of their own sequence or other short pieces of RNA.
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Early protobionts with self-replicating, catalytic RNA would have been more effective at using resources and would have increased in number through natural selection. The early genetic material might have formed an “RNA world.”
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Concept 25.2: The fossil record documents the history of life.
The fossil record reveals changes in the history of life on earth.
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The Fossil Record Sedimentary rocks are deposited into layers called strata and are the richest source of fossils. Video: Grand Canyon
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Figure 25.4 Documenting the history of life
Present Rhomaleosaurus victor, a plesiosaur Dimetrodon 100 million years ago Casts of ammonites 175 200 270 300 4.5 cm Hallucigenia 375 Coccosteus cuspidatus 400 1 cm Figure 25.4 Documenting the history of life Dickinsonia costata 500 525 2.5 cm 565 Stromatolites 600 Tappania, a unicellular eukaryote Fossilized stromatolite 3,500 1,500
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Hallucigenia Dickinsonia costata 500 525 565 Stromatolites Tappania, a
Fig Hallucigenia 1 cm Dickinsonia costata 500 525 2.5 cm 4.5 cm 565 Stromatolites Figure 25.4 Documenting the history of life 600 Tappania, a unicellular eukaryote Fossilized stromatolite 3,500 1,500
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Rhomaleosaurus victor, a plesiosaur
Fig. 25-4a-2 Present Rhomaleosaurus victor, a plesiosaur Dimetrodon 100 million years ago Casts of ammonites 175 200 Figure 25.4 Documenting the history of life 270 300 4.5 cm 375 Coccosteus cuspidatus 400
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Rhomaleosaurus victor, a plesiosaur
Fig. 25-4b Figure 25.4 Documenting the history of life Rhomaleosaurus victor, a plesiosaur
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Fig. 25-4c Figure 25.4 Documenting the history of life Dimetrodon
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Casts of ammonites Fig. 25-4d
Figure 25.4 Documenting the history of life Casts of ammonites
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Coccosteus cuspidatus
Fig. 25-4e Figure 25.4 Documenting the history of life 4.5 cm Coccosteus cuspidatus
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Fig. 25-4f Figure 25.4 Documenting the history of life 1 cm Hallucigenia
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2.5 cm Dickinsonia costata Fig. 25-4g
Figure 25.4 Documenting the history of life Dickinsonia costata 2.5 cm
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Tappania, a unicellular eukaryote
Fig. 25-4h Figure 25.4 Documenting the history of life Tappania, a unicellular eukaryote
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Fig. 25-4i Figure 25.4 Documenting the history of life Stromatolites
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Fossilized stromatolite
Fig. 25-4j Figure 25.4 Documenting the history of life Fossilized stromatolite
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Animation: The Geologic Record
Few individuals have fossilized, and even fewer have been discovered. The fossil record is biased in favor of species that: Existed for a long time. Were abundant and widespread. Had hard parts. Animation: The Geologic Record
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How Rocks and Fossils Are Dated
Sedimentary strata reveal the relative ages of fossils. The absolute ages of fossils can be determined by radiometric dating. A “parent” isotope decays to a “daughter” isotope at a constant rate. Each isotope has a known half-life, the time required for half the parent isotope to decay.
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1/2 1/4 1/8 1/16 Accumulating “daughter” isotope
Fig. 25-5 Accumulating “daughter” isotope Fraction of parent isotope remaining 1/2 Remaining “parent” isotope 1/4 Figure 25.5 Radiometric dating 1/8 1/16 1 2 3 4 Time (half-lives)
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Radiocarbon dating can be used to date fossils up to 75,000 years old.
For older fossils, some isotopes can be used to date sedimentary rock layers above and below the fossil.
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The magnetism of rocks can provide dating information.
Reversals of the magnetic poles leave their record on rocks throughout the world.
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The Origin of New Groups of Organisms
Mammals belong to the group of animals called tetrapods. The evolution of unique mammalian features through gradual modifications can be traced from ancestral synapsids through the present.
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Figure 25.6 The origin of mammals
Synapsid (300 mya) Figure 25.6 The origin of mammals Temporal fenestra Key Articular Dentary Quadrate Squamosal Therapsid (280 mya) Reptiles (including dinosaurs and birds) Temporal fenestra EARLY TETRAPODS Dimetrodon Early cynodont (260 mya) Synapsids Temporal fenestra Very late cynodonts Earlier cynodonts Therapsids Figure 25.6 The origin of mammals Later cynodont (220 mya) Mammals Very late cynodont (195 mya)
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Synapsid (300 mya) Temporal fenestra Key Articular Quadrate
Fig Figure 25.6 The origin of mammals Synapsid (300 mya) Temporal fenestra Key Articular Quadrate Therapsid (280 mya) Dentary Squamosal Figure 25.6 The origin of mammals Temporal fenestra
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Very late cynodont (195 mya)
Fig Early cynodont (260 mya) Figure 25.6 The origin of mammals Key Articular Temporal fenestra Quadrate Dentary Squamosal Later cynodont (220 mya) Figure 25.6 The origin of mammals Very late cynodont (195 mya)
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Concept 25.3: Key events in life’s history include the origins of single-celled and multicelled organisms and the colonization of land. The geologic record is divided into the Archaean, the Proterozoic, and the Phanerozoic eons.
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Table 25-1 Table 25.1
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Table 25-1a Table 25.1
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Table 25-1b Table 25.1
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The Phanerozoic encompasses multicellular eukaryotic life.
The Phanerozoic is divided into three eras: the Paleozoic, Mesozoic, and Cenozoic. Major boundaries between geological divisions correspond to extinction events in the fossil record.
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Figure 25.7 Clock analogy for some key events in Earth’s history
Ceno- zoic Meso- zoic Humans Paleozoic Figure 25.7 Clock analogy for some key events in Earth’s history Colonization of land Animals Origin of solar system and Earth 1 4 Proterozoic Archaean Prokaryotes Figure 25.7 Clock analogy for some key events in Earth’s history Billions of years ago 2 3 Multicellular eukaryotes Single-celled eukaryotes Atmospheric oxygen
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The First Single-Celled Organisms
The oldest known fossils are stromatolites, rock-like structures composed of many layers of bacteria and sediment. Stromatolites date back 3.5 billion years ago. Prokaryotes were Earth’s sole inhabitants from 3.5 to about 2.1 billion years ago.
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Fig 25-UN2 1 4 Billions of years ago 2 3 Prokaryotes
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Photosynthesis and the Oxygen Revolution
Most atmospheric oxygen (O2) is of biological origin. O2 produced by oxygenic photosynthesis reacted with dissolved iron and precipitated out to form banded iron formations. The source of O2 was likely bacteria similar to modern cyanobacteria.
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This “oxygen revolution” from 2.7 to 2.2 billion years ago:
By about 2.7 billion years ago, O2 began accumulating in the atmosphere and rusting iron-rich terrestrial rocks. This “oxygen revolution” from 2.7 to 2.2 billion years ago: Posed a challenge for life. Provided opportunity to gain energy from light. Allowed organisms to exploit new ecosystems.
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Fig 25-UN3 1 4 Billions of years ago 2 3 Atmospheric oxygen
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Figure 25.8 Banded iron formations: evidence of oxygenic photosynthesis
For the Discovery Video Early Life, go to Animation and Video Files.
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The First Eukaryotes The oldest fossils of eukaryotic cells date back 2.1 billion years. The hypothesis of endosymbiosis proposes that mitochondria and plastids (chloroplasts and related organelles) were formerly small prokaryotes living within larger host cells. An endosymbiont is a cell that lives within a host cell.
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Fig 25-UN4 1 4 Billions of years ago 2 3 Single- celled eukaryotes
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The prokaryotic ancestors of mitochondria and plastids probably gained entry to the host cell as undigested prey or internal parasites. In the process of becoming more interdependent, the host and endosymbionts would have become a single organism. Serial endosymbiosis supposes that mitochondria evolved before plastids through a sequence of endosymbiotic events.
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Endoplasmic reticulum Nucleus
Fig Figure 25.9 A model of the origin of eukaryotes through serial endosymbiosis Cytoplasm Plasma membrane DNA Ancestral prokaryote Endoplasmic reticulum Nucleus Figure 25.9 A model of the origin of eukaryotes through serial endosymbiosis Nuclear envelope
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Aerobic heterotrophic prokaryote Mitochondrion Ancestral heterotrophic
Fig Figure 25.9 A model of the origin of eukaryotes through serial endosymbiosis Aerobic heterotrophic prokaryote Mitochondrion Ancestral heterotrophic eukaryote Figure 25.9 A model of the origin of eukaryotes through serial endosymbiosis
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Ancestral photosynthetic eukaryote
Fig Figure 25.9 A model of the origin of eukaryotes through serial endosymbiosis Photosynthetic prokaryote Mitochondrion Plastid Figure 25.9 A model of the origin of eukaryotes through serial endosymbiosis Ancestral photosynthetic eukaryote
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Endoplasmic reticulum Nucleus
Fig Cytoplasm Plasma membrane DNA Ancestral prokaryote Endoplasmic reticulum Nucleus Nuclear envelope Aerobic heterotrophic prokaryote Photosynthetic prokaryote Mitochondrion Figure 25.9 A model of the origin of eukaryotes through serial endosymbiosis Mitochondrion Ancestral heterotrophic eukaryote Plastid Ancestral photosynthetic eukaryote
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Key evidence supporting an endosymbiotic origin of mitochondria and plastids:
Similarities in inner membrane structures and functions. Division is similar in these organelles and some prokaryotes. These organelles transcribe and translate their own DNA. Their ribosomes are more similar to prokaryotic than eukaryotic ribosomes.
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The Origin of Multicellularity
The evolution of eukaryotic cells allowed for a greater range of unicellular forms. A second wave of diversification occurred when multicellularity evolved and gave rise to algae, plants, fungi, and animals.
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The Earliest Multicellular Eukaryotes
Comparisons of DNA sequences date the common ancestor of multicellular eukaryotes to 1.5 billion years ago. The oldest known fossils of multicellular eukaryotes are of small algae that lived about 1.2 billion years ago.
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The “snowball Earth” hypothesis suggests that periods of extreme glaciation confined life to the equatorial region or deep-sea vents from 750 to 580 million years ago. The Ediacaran biota were an assemblage of larger and more diverse soft-bodied organisms that lived from 565 to 535 million years ago.
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Fig 25-UN5 1 4 Billions of years ago 2 3 Multicellular eukaryotes
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The Cambrian Explosion
The Cambrian explosion refers to the sudden appearance of fossils resembling modern phyla in the Cambrian period (535 to 525 million years ago). The Cambrian explosion provides the first evidence of predator-prey interactions.
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Fig 25-UN6 Animals 1 4 Billions of years ago 2 3
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Sponges Cnidarians 500 Annelids Molluscs Chordates Arthropods
Fig 500 Sponges Cnidarians Annelids Molluscs Chordates Arthropods Echinoderms Brachiopods Early Paleozoic era (Cambrian period) Millions of years ago 542 Figure Appearance of selected animal phyla Late Proterozoic eon
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DNA analyses suggest that many animal phyla diverged before the Cambrian explosion, perhaps as early as 700 million to 1 billion years ago. Fossils in China provide evidence of modern animal phyla tens of millions of years before the Cambrian explosion. The Chinese fossils suggest that “the Cambrian explosion had a long fuse.”
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(a) Two-cell stage (b) Later stage 150 µm 200 µm
Fig Figure Proterozoic fossils that may be animal embryos (SEM) Figure Proterozoic fossils that may be animal embryos (SEM) (a) Two-cell stage (b) Later stage 150 µm 200 µm
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The Colonization of Land
Fungi, plants, and animals began to colonize land about 500 million years ago. Plants and fungi likely colonized land together by 420 million years ago. Arthropods and tetrapods are the most widespread and diverse land animals. Tetrapods evolved from lobe-finned fishes around 365 million years ago.
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Fig 25-UN7 Colonization of land 1 4 Billions of years ago 2 3
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Video: Volcanic Eruption
Concept 25.4: The rise and fall of dominant groups reflect continental drift, mass extinctions, and adaptive radiations. The history of life on Earth has seen the rise and fall of many groups of organisms. Video: Volcanic Eruption Video: Lava Flow
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Continental Drift At three points in time, the land masses of Earth have formed a supercontinent: 1.1 billion, 600 million, and 250 million years ago. Earth’s continents move slowly over the underlying hot mantle through the process of continental drift. Oceanic and continental plates can collide, separate, or slide past each other. Interactions between plates cause the formation of mountains and islands, and earthquakes.
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Figure 25.12 Earth and its continental plates
North American Plate Eurasian Plate Crust Juan de Fuca Plate Caribbean Plate Philippine Plate Arabian Plate Indian Plate Mantle Cocos Plate Pacific Plate South American Plate Nazca Plate Outer core African Plate Australian Plate Inner core Figure Earth and its continental plates Scotia Plate Antarctic Plate (a) Cutaway view of Earth (b) Major continental plates
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(a) Cutaway view of Earth
Fig a Figure Earth and its continental plates Crust Mantle Outer core Figure Earth and its continental plates Inner core (a) Cutaway view of Earth
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(b) Major continental plates
Fig b Figure Earth and its continental plates North American Plate Eurasian Plate Juan de Fuca Plate Caribbean Plate Philippine Plate Arabian Plate Indian Plate Cocos Plate South American Plate Pacific Plate Nazca Plate African Plate Australian Plate Figure Earth and its continental plates Scotia Plate Antarctic Plate (b) Major continental plates
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Consequences of Continental Drift
Formation of the supercontinent Pangaea about 250 million years ago had many effects. A reduction in shallow water habitat. A colder and drier climate inland. Changes in climate as continents moved toward and away from the poles. Changes in ocean circulation patterns leading to global cooling.
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Present Figure The history of continental drift during the Phanerozoic eon Cenozoic North America Eurasia 65.5 Africa South America India Madagascar Australia Antarctica Laurasia 135 Mesozoic Millions of years ago Gondwana Figure The history of continental drift during the Phanerozoic eon 251 Pangaea Paleozoic
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Present Cenozoic Millions of years ago 65.5
Figure The history of continental drift during the Phanerozoic eon Present Cenozoic North America Eurasia Millions of years ago 65.5 Africa Figure The history of continental drift during the Phanerozoic eon India South America Madagascar Australia Antarctica
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135 Mesozoic Millions of years ago 251 Paleozoic
Laurasia 135 Figure The history of continental drift during the Phanerozoic eon Gondwana Mesozoic Millions of years ago Figure The history of continental drift during the Phanerozoic eon 251 Pangaea Paleozoic
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The break-up of Pangaea lead to allopatric speciation.
The current distribution of fossils reflects the movement of continental drift. For example, the similarity of fossils in parts of South America and Africa is consistent with the idea that these continents were formerly attached.
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Mass Extinctions The fossil record shows that most species that have ever lived are now extinct. At times, the rate of extinction has increased dramatically and caused a mass extinction.
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The “Big Five” Mass Extinction Events
In each of the five mass extinction events, more than 50% of Earth’s species became extinct.
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(families per million years):
Figure Mass extinction and the diversity of life 20 800 700 15 600 500 Number of families: (families per million years): Total extinction rate 10 400 300 5 200 100 Figure Mass extinction and the diversity of life Era Period Paleozoic Mesozoic Cenozoic E O S D C P Tr J C P N 542 488 444 416 359 299 251 200 145 65.5 Time (millions of years ago)
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The Permian extinction defines the boundary between the Paleozoic and Mesozoic eras.
This mass extinction occurred in less than 5 million years and caused the extinction of about 96% of marine animal species. This event might have been caused by volcanism, which lead to global warming, and a decrease in oceanic oxygen.
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The Cretaceous mass extinction 65
The Cretaceous mass extinction 65.5 million years ago separates the Mesozoic from the Cenozoic. Organisms that went extinct include about half of all marine species and many terrestrial plants and animals, including most dinosaurs.
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Figure 25.15 Trauma for Earth and its Cretaceous life
NORTH AMERICA Chicxulub crater Yucatán Peninsula Figure Trauma for Earth and its Cretaceous life For the Discovery Video Mass Extinctions, go to Animation and Video Files.
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The presence of iridium in sedimentary rocks suggests a meteorite impact about 65 million years ago.
The Chicxulub crater off the coast of Mexico is evidence of a meteorite that dates to the same time.
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Is a Sixth Mass Extinction Under Way?
Scientists estimate that the current rate of extinction is 100 to 1,000 times the typical background rate. Data suggest that a sixth human-caused mass extinction is likely to occur unless dramatic action is taken.
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Consequences of Mass Extinctions
Mass extinction can alter ecological communities and the niches available to organisms. It can take from 5 to 100 million years for diversity to recover following a mass extinction. Mass extinction can pave the way for adaptive radiations.
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(percentage of marine genera)
Fig Figure Mass extinctions and ecology 50 40 30 (percentage of marine genera) Predator genera 20 10 Paleozoic Era Period Mesozoic Cenozoic Figure Mass extinctions and ecology E O S D C P Tr J C P N 542 488 444 416 359 299 251 200 145 65.5 Time (millions of years ago)
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Adaptive Radiations Adaptive radiation is the evolution of diversely adapted species from a common ancestor upon introduction to new environmental opportunities.
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Worldwide Adaptive Radiations
Mammals underwent an adaptive radiation after the extinction of terrestrial dinosaurs. The disappearance of dinosaurs (except birds) allowed for the expansion of mammals in diversity and size. Other notable radiations include photosynthetic prokaryotes, large predators in the Cambrian, land plants, insects, and tetrapods.
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Figure 25.17 Adaptive radiation of mammals
Ancestral mammal Monotremes (5 species) ANCESTRAL CYNODONT Marsupials (324 species) Eutherians (placental mammals; 5,010 species) Figure Adaptive radiation of mammals 250 200 150 100 50 Millions of years ago
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Regional Adaptive Radiations
Adaptive radiations can occur when organisms colonize new environments with little competition. The Hawaiian Islands are one of the world’s great showcases of adaptive radiation.
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Figure 25.18 Adaptive radiation on the Hawaiian Islands
Close North American relative, the tarweed Carlquistia muirii KAUAI 5.1 million years MOLOKAI 1.3 million years Dubautia laxa MAUI OAHU 3.7 million years Argyroxiphium sandwicense LANAI HAWAII 0.4 million years Figure Adaptive radiation on the Hawaiian Islands Dubautia waialealae Dubautia scabra Dubautia linearis
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1.3 KAUAI MOLOKAI million 5.1 years million MAUI years OAHU 3.7
Fig a Figure Adaptive radiation on the Hawaiian Islands 1.3 million years KAUAI 5.1 million years MOLOKAI MAUI OAHU 3.7 million years LANAI Figure Adaptive radiation on the Hawaiian Islands HAWAII 0.4 million years
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Close North American relative, the tarweed Carlquistia muirii
Fig b Figure Adaptive radiation on the Hawaiian Islands Figure Adaptive radiation on the Hawaiian Islands Close North American relative, the tarweed Carlquistia muirii
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Fig c Figure Adaptive radiation on the Hawaiian Islands Figure Adaptive radiation on the Hawaiian Islands Dubautia waialealae
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Dubautia laxa Figure 25.18 Adaptive radiation on the Hawaiian Islands
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Figure 25.18 Adaptive radiation on the Hawaiian Islands
Dubautia scabra
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Argyroxiphium sandwicense
Fig f Figure Adaptive radiation on the Hawaiian Islands Figure Adaptive radiation on the Hawaiian Islands Argyroxiphium sandwicense
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Fig g Figure Adaptive radiation on the Hawaiian Islands Figure Adaptive radiation on the Hawaiian Islands Dubautia linearis
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Concept 25.5: Major changes in body form can result from changes in the sequences and regulation of developmental genes. Studying genetic mechanisms of change can provide insight into large-scale evolutionary change.
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Evolutionary Effects of Development Genes
Genes that program development control the rate, timing, and spatial pattern of changes in an organism’s form as it develops into an adult.
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Changes in Rate and Timing
Heterochrony is an evolutionary change in the rate or timing of developmental events. It can have a significant impact on body shape. The contrasting shapes of human and chimpanzee skulls are the result of small changes in relative growth rates. Animation: Allometric Growth
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Figure 25.19 Relative growth rates of body parts
Newborn 2 5 15 Adult Age (years) (a) Differential growth rates in a human Figure Relative growth rates of body parts Chimpanzee fetus Chimpanzee adult Human fetus Human adult (b) Comparison of chimpanzee and human skull growth
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(a) Differential growth rates in a human
Figure Relative growth rates of body parts Figure Relative growth rates of body parts Newborn 2 5 15 Adult Age (years) (a) Differential growth rates in a human
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(b) Comparison of chimpanzee and human skull growth
Figure Relative growth rates of body parts Chimpanzee fetus Chimpanzee adult Figure Relative growth rates of body parts Human fetus Human adult (b) Comparison of chimpanzee and human skull growth
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Heterochrony can alter the timing of reproductive development relative to the development of nonreproductive organs. In paedomorphosis, the rate of reproductive development accelerates compared with somatic development. The sexually mature species may retain body features that were juvenile structures in an ancestral species.
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Gills Figure 25.20 Paedomorphosis Fig. 25-20
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Changes in Spatial Pattern
Substantial evolutionary change can also result from alterations in genes that control the placement and organization of body parts. Homeotic genes determine such basic features as where wings and legs will develop on a bird or how a flower’s parts are arranged.
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Hox genes are a class of homeotic genes that provide positional information during development.
If Hox genes are expressed in the wrong location, body parts can be produced in the wrong location. For example, in crustaceans, a swimming appendage can be produced instead of a feeding appendage.
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Evolution of vertebrates from invertebrate animals was associated with alterations in Hox genes.
Two duplications of Hox genes have occurred in the vertebrate lineage. These duplications may have been important in the evolution of new vertebrate characteristics.
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Hypothetical vertebrate ancestor (invertebrate)
Fig Hypothetical vertebrate ancestor (invertebrate) with a single Hox cluster First Hox duplication Figure Hox mutations and the origin of vertebrates Hypothetical early vertebrates (jawless) with two Hox clusters Second Hox duplication Figure Hox mutations and the origin of vertebrates Vertebrates (with jaws) with four Hox clusters
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The Evolution of Development
The tremendous increase in diversity during the Cambrian explosion is a puzzle. Developmental genes may play an especially important role. Changes in developmental genes can result in new morphological forms.
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Changes in Genes New morphological forms likely come from gene duplication events that produce new developmental genes. A possible mechanism for the evolution of six-legged insects from a many-legged crustacean ancestor has been demonstrated in lab experiments. Specific changes in the Ubx gene have been identified that can “turn off” leg development.
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Hox gene 6 Hox gene 7 Hox gene 8 Ubx About 400 mya Drosophila Artemia
Fig Figure Origin of the insect body plan Hox gene 6 Hox gene 7 Hox gene 8 Ubx About 400 mya Figure Origin of the insect body plan Drosophila Artemia
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Changes in Gene Regulation
Changes in the form of organisms may be caused more often by changes in the regulation of developmental genes instead of changes in their sequence. For example three-spine sticklebacks in lakes have fewer spines than their marine relatives. The gene sequence remains the same, but the regulation of gene expression is different in the two groups of fish.
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Figure 25.23 What causes the loss of spines in lake stickleback fish?
RESULTS Test of Hypothesis A: Differences in the coding sequence of the Pitx1 gene? Result: No The 283 amino acids of the Pitx1 protein are identical. Test of Hypothesis B: Differences in the regulation of expression of Pitx1 ? Pitx1 is expressed in the ventral spine and mouth regions of developing marine sticklebacks but only in the mouth region of developing lake stickbacks. Result: Yes Marine stickleback embryo Lake stickleback embryo Figure What causes the loss of spines in lake stickleback fish? Close-up of mouth Close-up of ventral surface
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Figure 25.23 What causes the loss of spines in lake stickleback fish?
Fig a Figure What causes the loss of spines in lake stickleback fish? Marine stickleback embryo Lake stickleback embryo Close-up of mouth Figure What causes the loss of spines in lake stickleback fish? Close-up of ventral surface
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Concept 25.6: Evolution is not goal oriented
Evolution is like “tinkering”—it is a process in which new forms arise by the slight modification of existing forms.
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Evolutionary Novelties
Most novel biological structures evolve in many stages from previously existing structures. Complex eyes have evolved from simple photosensitive cells independently many times. Exaptations are structures that evolve in one context but become co-opted for a different function. Natural selection can only improve a structure in the context of its current utility.
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Figure 25.24 A range of eye complexity among molluscs
Pigmented cells (photoreceptors) Pigmented cells Figure A range of eye complexity among molluscs Epithelium Nerve fibers Nerve fibers (a) Patch of pigmented cells (b) Eyecup Fluid-filled cavity Cellular mass (lens) Cornea Epithelium Optic nerve Pigmented layer (retina) Optic nerve (c) Pinhole camera-type eye (d) Eye with primitive lens Figure A range of eye complexity among molluscs Cornea Lens Retina Optic nerve (e) Complex camera-type eye
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Evolutionary Trends Extracting a single evolutionary progression from the fossil record can be misleading. Apparent trends should be examined in a broader context.
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Figure 25.25 The branched evolution of horses
Recent (11,500 ya) Equus Hippidion and other genera Pleistocene (1.8 mya) Nannippus Pliohippus Pliocene (5.3 mya) Hipparion Neohipparion Sinohippus Megahippus Callippus Archaeohippus Miocene (23 mya) Merychippus Anchitherium Hypohippus Parahippus Miohippus Oligocene (33.9 mya) Figure The branched evolution of horses Mesohippus Paleotherium Epihippus Propalaeotherium Eocene (55.8 mya) Pachynolophus Orohippus Key Grazers Hyracotherium Browsers
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Figure 25.25 The branched evolution of horses
Miohippus Oligocene (33.9 mya) Mesohippus Paleotherium Epihippus Propalaeotherium Eocene (55.8 mya) Pachynolophus Orohippus Key Figure The branched evolution of horses Grazers Hyracotherium Browsers
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Figure 25.25 The branched evolution of horses
Fig b Recent (11,500 ya) Equus Hippidion and other genera Pleistocene (1.8 mya) Nannippus Pliohippus Pliocene (5.3 mya) Hipparion Neohipparion Sinohippus Megahippus Callippus Archaeohippus Miocene (23 mya) Figure The branched evolution of horses Merychippus Anchitherium Hypohippus Parahippus
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According to the species selection model, trends may result when species with certain characteristics endure longer and speciate more often than those with other characteristics. The appearance of an evolutionary trend does not imply that there is some intrinsic drive toward a particular phenotype.
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Millions of years ago (mya)
Fig 25-UN8 1.2 bya: First multicellular eukaryotes 535–525 mya: Cambrian explosion (great increase in diversity of animal forms) 500 mya: Colonization of land by fungi, plants and animals 2.1 bya: First eukaryotes (single-celled) 3.5 billion years ago (bya): First prokaryotes (single-celled) 500 4,000 3,500 3,000 2,500 2,000 1,500 1,000 Present Millions of years ago (mya)
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Ceno- Meso- zoic zoic Paleozoic Origin of solar system and Earth 1 4 2
Fig 25-UN9 Ceno- zoic Meso- zoic Paleozoic Origin of solar system and Earth 1 4 Proterozoic Archaean Billions of years ago 2 3
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Flies and fleas Caddisflies Moths and butterflies Herbivory
Fig 25-UN10 Flies and fleas Caddisflies Moths and butterflies Herbivory
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Ceno- zoic Meso- zoic Paleozoic Origin of solar system and Earth 1 4
Fig 25-UN11 Ceno- zoic Meso- zoic Paleozoic Origin of solar system and Earth 1 4 Proterozoic Archaean Billions of years ago 2 3
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You should now be able to:
Define radiometric dating, serial endosymbiosis, Pangaea, snowball Earth, exaptation, heterochrony, and paedomorphosis. Describe the contributions made by Oparin, Haldane, Miller, and Urey toward understanding the origin of organic molecules. Explain why RNA, not DNA, was likely the first genetic material.
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Describe and suggest evidence for the major events in the history of life on Earth from Earth’s origin to 2 billion years ago. Briefly describe the Cambrian explosion. Explain how continental drift led to Australia’s unique flora and fauna. Describe the mass extinctions that ended the Permian and Cretaceous periods. Explain the function of Hox genes.
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