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Earth System History Part 6.

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Presentation on theme: "Earth System History Part 6."— Presentation transcript:

1 Earth System History Part 6

2 Precambrian 4.5 to 3.8 billion years ago. Solar system forms

3 Protoplanet: a hypothetical whirling gaseous mass within a giant cloud of gas and dust that rotates around a sun and is believed to give rise to a planet.

4 Precambrian Hadean, Archean, and Proterozoic Eon’s -

5 Precambrian Hadean, Archean, and Proterozoic Eon’s -

6 Precambrian Hadean, Archean, and Proterozoic Eon’s -

7 Precambrian Hadean, Archean, and Proterozoic Eon’s -

8 Earth’s molten layers form (Denser materials go to the middle / core)
Copyright © 2010 Ryan P. Murphy

9 Formation of Earth’s Crust (cooling).
Copyright © 2010 Ryan P. Murphy

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11 Meteorites bombard the planet.
The earth increases in size. Copyright © 2010 Ryan P. Murphy

12 Meteorites bombard the planet.
The earth increases in size. Copyright © 2010 Ryan P. Murphy

13 Meteorites bombard the planet.
The earth increases in size. Copyright © 2010 Ryan P. Murphy

14 How did the moon get here / form?

15 Theories on how moon was formed?
The Fission Theory: The Moon was once part of the Earth and somehow separated from the Earth early in the history of the Solar System. The present Pacific Ocean basin is the most popular site for the part of the Earth from which the Moon came. The Capture Theory: The Moon was formed somewhere else, and was later captured by the gravitational field of the earth. The Condensation Theory: The Moon and the Earth condensed together from the original nebula that formed the Solar System. The Colliding Planetesimals Theory: The interaction of earth-orbiting and Sun-orbiting planetesimals (very large chunks of rocks like asteroids) early in the history of the Solar System led to their breakup. The Moon condensed from this debris. The Ejected Ring Theory: A planetesimal the size of Mars struck the earth, ejecting large volumes of matter. A disk of orbiting material was formed, and this matter eventually condensed to form the Moon in orbit around the earth.

16 Theories on how moon was formed?
The Fission Theory: The Moon was once part of the Earth and somehow separated from the Earth early in the history of the Solar System. The present Pacific Ocean basin is the most popular site for the part of the Earth from which the Moon came. The Capture Theory: The Moon was formed somewhere else, and was later captured by the gravitational field of the earth. The Condensation Theory: The Moon and the Earth condensed together from the original nebula that formed the Solar System. The Colliding Planetesimals Theory: The interaction of earth-orbiting and Sun-orbiting planetesimals (very large chunks of rocks like asteroids) early in the history of the Solar System led to their breakup. The Moon condensed from this debris. The Ejected Ring Theory: A planetesimal the size of Mars struck the earth, ejecting large volumes of matter. A disk of orbiting material was formed, and this matter eventually condensed to form the Moon in orbit around the earth.

17 4.5 Billion Years Ago

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19 Early Earth

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22 Theia

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33 Debris Disk

34 Debris Disk

35 Debris Disk

36 Debris Disk

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38 Earth

39 Earth

40 Moon Earth

41 Kind of like that... Moon Earth

42 Kind of like that... Moon Axial Tilt 23.5 Earth

43 Kind of like that... Moon Axial Tilt 23.5 Spin / Day Length Earth

44 Kind of like that... Moon Axial Tilt 23.5 Spin / Day Length Earth Earth increased in mass.

45 Kind of like that... Moon Axial Tilt 23.5 Spin / Day Length Earth
Theia’s Remains Moon Axial Tilt 23.5 Spin / Day Length Earth Earth increased in mass.

46 Kind of like that... Moon Axial Tilt 23.5 Spin / Day Length Earth
Theia’s Remains Moon Axial Tilt 23.5 Spin / Day Length Earth Earth increased in mass. Theories on moon formation, Learn more:

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50 Atmosphere originates (No oxygen yet).

51 Hydorgen and Helium based
Atmosphere originates (No oxygen yet). Hydorgen and Helium based

52 Hydorgen and Helium based
Atmosphere originates (No oxygen yet). Hydorgen and Helium based You would die breathing it.

53 The first oceans…

54 The tides were a 1000 feet b/c the moon was close.
The first oceans… The tides were a 1000 feet b/c the moon was close.

55 The first continents

56 A long time goes by and then…

57 Earliest life begins (primitive protocells).

58 A long time goes by and then…

59 Microbes helped produce an oxygen rich atmosphere through photosynthesis.
Copyright © 2010 Ryan P. Murphy

60 Microbes helped produce an oxygen rich atmosphere through photosynthesis.
Copyright © 2010 Ryan P. Murphy

61 First Multi-cellular life (many cells).
Copyright © 2010 Ryan P. Murphy

62 First Multi-cellular life (many cells).
Copyright © 2010 Ryan P. Murphy

63 First Multi-cellular life (many cells).
Copyright © 2010 Ryan P. Murphy

64 Picture of earliest fossilized cyanobacteria at 3.4 billion years old.
Copyright © 2010 Ryan P. Murphy

65 Picture of earliest fossilized cyanobacteria at 3.4 billion years old.
Bacteria: Very small single celled organisms. Copyright © 2010 Ryan P. Murphy

66 Picture of earliest fossilized cyanobacteria at 3.4 billion years old.
Bacteria: Very small single celled organisms. -They reproduce by splitting in half. Copyright © 2010 Ryan P. Murphy

67 Picture of earliest fossilized cyanobacteria at 3.4 billion years old.
Bacteria: Very small single celled organisms. -They reproduce by splitting in half. - Very primitive internal structure. No nucleus. Copyright © 2010 Ryan P. Murphy

68

69 Supercontinents form (Rodinia)

70 Explosion of new animals (sea)

71 Paleozoic Era Vendian, Cambrian, Ordovican, Silurian, Devonian, Carboniferous, and Permian Periods. - Copyright © 2010 Ryan P. Murphy

72 Paleozoic Era Vendian, Cambrian, Ordovican, Silurian, Devonian, Carboniferous, and Permian Periods. - Copyright © 2010 Ryan P. Murphy

73 Paleozoic Era Vendian, Cambrian, Ordovican, Silurian, Devonian, Carboniferous, and Permian Periods. - Copyright © 2010 Ryan P. Murphy

74 Paleozoic Era Vendian, Cambrian, Ordovican, Silurian, Devonian, Carboniferous, and Permian Periods. -

75 Paleozoic Era Vendian, Cambrian, Ordovican, Silurian, Devonian, Carboniferous, and Permian Periods. -

76 Paleozoic Era Vendian, Cambrian, Ordovican, Silurian, Devonian, Carboniferous, and Permian Periods. -

77 Paleozoic Era Vendian, Cambrian, Ordovican, Silurian, Devonian, Carboniferous, and Permian Periods. -

78 Paleozoic Era Vendian, Cambrian, Ordovican, Silurian, Devonian, Carboniferous, and Permian Periods. -

79 Marine invertebrates dominate.
Copyright © 2010 Ryan P. Murphy

80 Video Link. Animation of Paleozoic Sea Life at Field Museum in Chicago
Video Link! Animation of Paleozoic Sea Life at Field Museum in Chicago. (Cambrian)

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85 Plants invade land. Copyright © 2010 Ryan P. Murphy

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89 Jawed Fish Evolve. Copyright © 2010 Ryan P. Murphy

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91 First Insects. Copyright © 2010 Ryan P. Murphy

92 Amphibians invade land.
Copyright © 2010 Ryan P. Murphy

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96 First Reptiles

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99 Insects take to the air. Copyright © 2010 Ryan P. Murphy

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102 Mesozoic Era Triassic, Jurassic, Cretaceous Periods -

103 Mesozoic Era Triassic, Jurassic, Cretaceous Periods -

104 Mesozoic Era Triassic, Jurassic, Cretaceous Periods -

105 Mesozoic Era Triassic, Jurassic, Cretaceous Periods -
Copyright © 2010 Ryan P. Murphy

106 Learn more about dinosaurs at… http://dsc.discovery.com/dinosaurs/
Dinosaurs dominate. Learn more about dinosaurs at… Copyright © 2010 Ryan P. Murphy

107 PANGEA 20

108 PANGEA 20

109 The Supercontinent Pangea began to split in the middle / late Jurassic
The Supercontinent Pangea began to split in the middle / late Jurassic. (Plate Tectonics) PANGEA 20

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111 First birds.

112 Archaeopteryx: Earliest ancestor to modern birds (150 million years ago)
Copyright © 2010 Ryan P. Murphy

113 Archaeopteryx: Earliest ancestor to modern birds (150 million years ago)
Copyright © 2010 Ryan P. Murphy

114 Birds came from Theropods.
How are they similar and different?

115 First mammals.

116 First mammals. Early mammals. Learn more at…

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120 First flowers. Copyright © 2010 Ryan P. Murphy

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123 K-T mass extinction event
Copyright © 2010 Ryan P. Murphy

124 K-T mass extinction event
Copyright © 2010 Ryan P. Murphy

125 K-T mass extinction event
Copyright © 2010 Ryan P. Murphy

126 A layer of Iridium can be found across the globe in rock layers around 65 million years ago.

127 A layer of Iridium can be found across the globe in rock layers around 65 million years ago.

128 A layer of Iridium can be found across the globe in rock layers around 65 million years ago.
Iridium is found on Meteorites.

129 A layer of Iridium can be found across the globe in rock layers around 65 million years ago.
Iridium is found on Meteorites. Impact Event

130 Impact Event Dinosaur Fossils
A layer of Iridium can be found across the globe in rock layers around 65 million years ago. Iridium is found on Meteorites. Impact Event Dinosaur Fossils

131 No Dinosaur Fossils Impact Event Dinosaur Fossils
A layer of Iridium can be found across the globe in rock layers around 65 million years ago. Iridium is found on Meteorites. No Dinosaur Fossils Impact Event Dinosaur Fossils

132 No Dinosaur Fossils Impact Event Cretaceous Period Dinosaur Fossils
A layer of Iridium can be found across the globe in rock layers around 65 million years ago. Iridium is found on Meteorites. No Dinosaur Fossils Impact Event Cretaceous Period Dinosaur Fossils

133 No Dinosaur Fossils Tertiary Period Impact Event Cretaceous Period
A layer of Iridium can be found across the globe in rock layers around 65 million years ago. Iridium is found on Meteorites. No Dinosaur Fossils Tertiary Period Impact Event Cretaceous Period Dinosaur Fossils

134 No Dinosaur Fossils Tertiary Period Impact Event Cretaceous Period
A layer of Iridium can be found across the globe in rock layers around 65 million years ago. K-T Mass Extinction Event Iridium is found on Meteorites. No Dinosaur Fossils Tertiary Period Impact Event Cretaceous Period Dinosaur Fossils

135 No Dinosaur Fossils Tertiary Period Impact Event Cretaceous Period
A layer of Iridium can be found across the globe in rock layers around 65 million years ago. K-T Mass Extinction Event Iridium is found on Meteorites. No Dinosaur Fossils Tertiary Period Impact Event Cretaceous Period Dinosaur Fossils

136 No Dinosaur Fossils Tertiary Period Impact Event Cretaceous Period
A layer of Iridium can be found across the globe in rock layers around 65 million years ago. K-T Mass Extinction Event Iridium is found on Meteorites. No Dinosaur Fossils Tertiary Period Impact Event Cretaceous Period Dinosaur Fossils

137 K-T mass extinction event...(Debate Exists)
Combination of Impact event. Volcanism. Disease.

138 K-T mass extinction event...(Debate Exists)
Combination of Impact event. Volcanism. Disease. Learn more about the extinction of the dinosaurs at…

139 Optional PowerPoint. Found in Activities folder
Asteroids, Impact Craters, and Torino Scale

140 Without this extinction event, the odds are…

141 The age of Mammals wouldn’t have happened.

142 Age of Mammals wouldn’t have happened.

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146 “I love a good Mammal.”

147 The age of dinosaur dominance was over.

148 The age of dinosaur dominance was over.

149 The age of dinosaur dominance was over.
99.5%

150 The age of dinosaur dominance was over. The age of mammals begins.

151 The age of dinosaur dominance was over. The age of mammals begins.

152 Video Link! (Optional) Life After Dinosaurs

153 Cenozoic Era Tertiary, and Quaternary Periods -

154 Cenozoic Era Tertiary, and Quaternary Periods -

155 Cenozoic Era Tertiary, and Quaternary Periods -

156 Mammals change. Copyright © 2010 Ryan P. Murphy

157 Mammals continued to radiate but still had to hide from the Terror Birds of the Cenozoic.
Phorusrhacids

158 Mammals continued to radiate but still had to hide from the Terror Birds of the Cenozoic.
Phorusrhacids

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161 Present Day Bird Species
Size Comparison

162 Present Day Bird Species
Size Comparison

163 Present Day Bird Species
Size Comparison

164 Present Day Bird Species
Size Comparison

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168 “Imagine how cool it would be to have these Terror Birds running around today.”

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173 Eventually, Larger mammals evolved that were able to prey upon the Terror Birds and caused their extinction.

174 Eventually, Larger mammals evolved that were able to prey upon the Terror Birds and caused their extinction.

175 Eventually, Larger mammals evolved that were able to prey upon the Terror Birds and caused their extinction.

176 Earliest Monkeys. Copyright © 2010 Ryan P. Murphy

177 47 million year old primate fossil.
“Ida”

178 Climate becomes drier. Copyright © 2010 Ryan P. Murphy

179 Panama attaches South America to North America

180 Panama attaches South America to North America

181 Why would the connection of Panama to South America cause ecological chaos?
Copyright © 2010 Ryan P. Murphy

182 Why would the connection of Panama to South America cause ecological chaos?
Copyright © 2010 Ryan P. Murphy

183 Why would the connection of Panama to South America cause ecological chaos?
Copyright © 2010 Ryan P. Murphy

184 Why would the connection of Panama to South America cause ecological chaos?
Copyright © 2010 Ryan P. Murphy

185 Answer. Many animals species in S. America rush into N
Answer! Many animals species in S. America rush into N. America and vice versa.

186 Answer. Many animals species in S. America rush into N
Answer! Many animals species in S. America rush into N. America and vice versa. Increased competition causes many extinctions.

187 Evolution is the change in the gene pool overtime.
Gene Pools can change when… Populations can shrink Diseases, extinctions, introduction of new better adapted species, predators. Non-random mating Organisms choose strongest mate, ones in similar boundaries, Mutations in the genes Genes can change. Some are good, some are bad. The environment will decide. Movement in and out of the population Immigration, gene flow. Natural selection Adaptations to the environment that do well replace poor ones. Usually an advancement.

188 Study for 1 minute Evolution is the change in the gene pool overtime.
Gene Pools can change when… Populations can shrink Diseases, extinctions, introduction of new better adapted species, predators. Non-random mating Organisms choose strongest mate, ones in similar boundaries, Mutations in the genes Genes can change. Some are good, some are bad. The environment will decide. Movement in and out of the population Immigration, gene flow. Natural selection Adaptations to the environment that do well replace poor ones. Usually an advancement. Study for 1 minute

189 Evolution is the change in the gene pool overtime.
Gene Pools can change when… Populations can shrink Diseases, extinctions, introduction of new better adapted species, predators. Non-random mating Organisms choose strongest mate, ones in similar boundaries, Mutations in the genes Genes can change. Some are good, some are bad. The environment will decide. Movement in and out of the population Immigration, gene flow. Natural selection Adaptations to the environment that do well replace poor ones. Usually an advancement.

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191 Evolution is the change in the gene pool overtime.
Gene Pools can change when… Populations can shrink Diseases, extinctions, introduction of new better adapted species, predators. Non-random mating Organisms choose strongest mate, ones in similar boundaries, Mutations in the genes Genes can change. Some are good, some are bad. The environment will decide. Movement in and out of the population Immigration, gene flow. Natural selection Adaptations to the environment that do well replace poor ones. Usually an advancement.

192 Evolution is the change in the gene pool overtime.
Gene Pools can change when… Populations can shrink Diseases, extinctions, introduction of new better adapted species, predators. Non-random mating Organisms choose strongest mate, ones in similar boundaries, Mutations in the genes Genes can change. Some are good, some are bad. The environment will decide. Movement in and out of the population Immigration, gene flow. Natural selection Adaptations to the environment that do well replace poor ones. Usually an advancement.

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194 Evolution is the change in the gene pool overtime.
Gene Pools can change when… Populations can shrink Diseases, extinctions, introduction of new better adapted species, predators. Non-random mating Organisms choose strongest mate, ones in similar boundaries, Mutations in the genes Genes can change. Some are good, some are bad. The environment will decide. Movement in and out of the population Immigration, gene flow. Natural selection Adaptations to the environment that do well replace poor ones. Usually an advancement.

195 Evolution is the change in the gene pool overtime.
Gene Pools can change when… Populations can shrink Diseases, extinctions, introduction of new better adapted species, predators. Non-random mating Organisms choose strongest mate, ones in similar boundaries, Mutations in the genes Genes can change. Some are good, some are bad. The environment will decide. Movement in and out of the population Immigration, gene flow. Natural selection Adaptations to the environment that do well replace poor ones. Usually an advancement.

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197 Evolution is the change in the gene pool overtime.
Gene Pools can change when… Populations can shrink Diseases, extinctions, introduction of new better adapted species, predators. Non-random mating Organisms choose strongest mate, ones in similar boundaries, Mutations in the genes Genes can change. Some are good, some are bad. The environment will decide. Movement in and out of the population Immigration, gene flow. Natural selection Adaptations to the environment that do well replace poor ones. Usually an advancement.

198 Evolution is the change in the gene pool overtime.
Gene Pools can change when… Populations can shrink Diseases, extinctions, introduction of new better adapted species, predators. Non-random mating Organisms choose strongest mate, ones in similar boundaries, Mutations in the genes Genes can change. Some are good, some are bad. The environment will decide. Movement in and out of the population Immigration, gene flow. Natural selection Adaptations to the environment that do well replace poor ones. Usually an advancement.

199 First human hominids.

200 Modern Man (Whoa)

201 Part I Part II Part III Video Links! (Optional)
Walking with Prehistoric Beasts Part I: Part II: Part III: Part I Part II Part III Caution! Mating

202 Video - Evolution of Everything, 13
Video - Evolution of Everything, 13.7 billion years ago to modern humans in 7 min. Enjoy! Encore Copyright © 2010 Ryan P. Murphy


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