Download presentation
Presentation is loading. Please wait.
1
Copyright Pearson Prentice Hall
Biology Copyright Pearson Prentice Hall
2
Copyright Pearson Prentice Hall
17-1 The Fossil Record Photo credit: Jackie Beckett/American Museum of Natural History Copyright Pearson Prentice Hall
3
Fossils and Ancient Life
What is the fossil record? Copyright Pearson Prentice Hall
4
Fossils and Ancient Life
The fossil record provides evidence about the history of life on Earth. It also shows how different groups of organisms, including species, have changed over time. Could be eggs, footprints, body parts etc Fossils and Ancient Life Copyright Pearson Prentice Hall
5
Fossils and Ancient Life
The fossil record provides incomplete information about the history of life. Over 99% of all species that have lived on Earth have become extinct, which means that the species has died out. Those species that still exist are referred to as being extant. Copyright Pearson Prentice Hall
6
Copyright Pearson Prentice Hall
How Fossils Form How Fossils Form Most fossils form in sedimentary rock. Sedimentary rock forms when exposure to the elements breaks down existing rock into small particles of sand, silt, and clay. Copyright Pearson Prentice Hall
7
Copyright Pearson Prentice Hall
How Fossils Form Fossil Formation Water carries small rock particles to lakes and seas. The fossil record provides evidence about the history of life on Earth. Most fossils are formed in sedimentary rock. Copyright Pearson Prentice Hall
8
Copyright Pearson Prentice Hall
How Fossils Form Dead organisms are buried by layers of sediment, which forms new rock. The fossil record provides evidence about the history of life on Earth. Most fossils are formed in sedimentary rock. Copyright Pearson Prentice Hall
9
Copyright Pearson Prentice Hall
How Fossils Form The preserved remains may be later discovered and studied. The fossil record provides evidence about the history of life on Earth. Most fossil formed in sedimentary rock. Copyright Pearson Prentice Hall
10
Interpreting Fossil Evidence
Paleontologists determine the age of fossils using relative dating or radioactive dating. Copyright Pearson Prentice Hall
11
Interpreting Fossil Evidence
Relative Dating In relative dating, the age of a fossil is determined by comparing its placement with that of fossils in other layers of rock. Rock layers form in order by age—the oldest on the bottom, with more recent layers on top. Copyright Pearson Prentice Hall
12
Interpreting Fossil Evidence
Relative Dating In relative dating, a paleontologist estimates a fossil’s age in comparison with that of other fossils. Each of these fossils is an index fossil. It enables scientists to date the rock layer in which it is found. Scientists can also use index fossils to date rocks from different locations. Photo credit: l. ©David Hanson/Stone; r. ©CORBIS Copyright Pearson Prentice Hall
13
Interpreting Fossil Evidence
Index fossils are used to compare the relative ages of fossils. An index fossil is a species that is recognizable and that existed for a short period but had a wide geographic range. Copyright Pearson Prentice Hall
14
Interpreting Fossil Evidence
Radioactive Dating Scientists use radioactive decay to assign an absolute age to rocks. Radioactive dating is the use of half-lives to determine the age of a sample. A half-life is the length of time required for half of the radioactive atoms in a sample to decay. Copyright Pearson Prentice Hall
15
Interpreting Fossil Evidence
Radioactive dating involves measuring the amounts of radioactive isotopes in a sample to determine its actual age. Such measurements enable scientists to determine the absolute age of rocks and the fossils they contain. Copyright Pearson Prentice Hall
16
Copyright Pearson Prentice Hall
The basic divisions of the geologic time scale are eras and periods. Geologic Time Scale Copyright Pearson Prentice Hall
17
Copyright Pearson Prentice Hall
18
Copyright Pearson Prentice Hall
Extinction Rate Millions of years ago 600 500 400 300 200 100 Permian mass extinction 80 60 40 20 Extinction rate Cretaceous mass extinction 2,500 2,000 1,500 1,000 Neogene Proterozoic eon Cambrian Ordovician Silurian Devonian Carboniferous Permian Triassic Jurassic Paleogene Paleozoic Mesozoic Ceno- zoic Number of families ( ) Extinction rate ( Number of taxonomic families Copyright Pearson Prentice Hall
19
Copyright Pearson Prentice Hall
Geologic Time Scale Geologic time begins with Precambrian Time, which covers about 88% of Earth’s history. The basic units of the geologic time scale after Precambrian Time are eras and periods. Each era is divided into periods. Vendian 650–544 Copyright Pearson Prentice Hall
20
Copyright Pearson Prentice Hall
Geologic Time Scale Eras Geologists divide the time between Precambrian time and the present into three eras: Paleozoic Era Mesozoic Era Cenozoic Era Copyright Pearson Prentice Hall
21
Copyright Pearson Prentice Hall
Geologic Time Scale Permian 290–245 Carboniferous 360–290 Devonian 410–360 Silurian 440–410 The basic units of the geologic time scale after Precambrian Time are eras and periods. Each era is divided into periods. Ordovician 505–440 Cambrian 544–505 Copyright Pearson Prentice Hall
22
Copyright Pearson Prentice Hall
Geologic Time Scale Cretaceous 145–65 Jurassic 208–145 The basic units of the geologic time scale after Precambrian Time are eras and periods. Each era is divided into periods. Triassic 245–208 Copyright Pearson Prentice Hall
23
Copyright Pearson Prentice Hall
Geologic Time Scale The basic units of the geologic time scale after Precambrian Time are eras and periods. Each era is divided into periods. Copyright Pearson Prentice Hall
24
Copyright Pearson Prentice Hall
Geologic Time Scale Clock Model of Earth’s History First humans Radiation of mammals First land plants First prokaryotes First multicellular organisms Cenozoic Era Mesozoic Era Paleozoic Era Precambrian Time Earth’s history is often compared to a familiar measurement, such as the twelve hours between noon and midnight. In such a comparison, notice that Precambrian Time lasts from noon until after 10:30 pm. First eukaryotes Accumulation of atmospheric oxygen Copyright Pearson Prentice Hall
25
Copyright Pearson Prentice Hall
17-2 Earth's Early History Photo credit: Jackie Beckett/American Museum of Natural History Copyright Pearson Prentice Hall
26
Copyright Pearson Prentice Hall
17-2 Earth's Early History What prevents organic molecules from forming on their own and remaining intact today? (424) What are the characteristics of earth before oceans formed? (423) The first organisms on Earth were most like todays? (426) Why did the development of sexual reproduction speed up the process of evolution? (428) Two gasses that probably existed in Earths early atmosphere are? (423) Photo credit: Jackie Beckett/American Museum of Natural History Copyright Pearson Prentice Hall
27
Copyright Pearson Prentice Hall
17-2 Earth's Early History What prevents organic molecules from forming on their own and remaining intact today? (424) Atmospheric oxygen is too reactive What are the characteristics of earth before oceans formed? (423) volcanic activity, atmosphere of poisonous gas The first organisms on Earth were most like todays? (426) bacteria Why did the development of sexual reproduction speed up the process of evolution? (428) it increases genetic variety Two gasses that probably existed in Earths early atmosphere are? (423) hydrogen cyanide and carbon monoxide Photo credit: Jackie Beckett/American Museum of Natural History Copyright Pearson Prentice Hall
Similar presentations
© 2025 SlidePlayer.com. Inc.
All rights reserved.