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© 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

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Page 1: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

© 2006 Pearson Prentice Hall

Lecture Outlines PowerPoint

Chapter 1

Earth Science 11e

Tarbuck/Lutgens

Page 2: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Earth Science, 11e

Introduction to Earth Science

Chapter 1

Page 3: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Earth Science

Encompasses all sciences that seek to understand • Earth • Earth's neighbors in space

Earth Science includes• Geology - literally the “study of Earth” • Oceanography – a study of the ocean

Page 4: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Earth Science

Earth Science includes• Meteorology - the study of the atmosphere

and the processes that produce weather • Astronomy - the study of the universe

Page 5: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

People and the environment

Environment • Surrounds and influences organisms • Physical environment encompasses water,

air, soil, and rock• Term “environmental” is usually reserved

for those aspects that focus on the relationships between people and the natural environment

Page 6: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

People and the environment

Resources • An important focus of the Earth sciences • Includes water, soil, minerals, and energy• Two broad categories

• Renewable – can be replenished (examples include plants and energy from water and wind)

• Nonrenewable – metals (examples include metals and fuels)

Page 7: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

People and the environment

Population • Population of the planet is growing rapidly • Rate of mineral and energy usage has

climbed more rapidly than the overall growth of population

Environmental problems• Local, regional, and global

Page 8: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

People and the environment

Environmental problems• Human-induced and accentuated

• Urban air pollution• Acid rain• Ozone depletion• Global warming

• Natural hazards • Earthquakes • Landslides

Page 9: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

People and the environment

Environmental problems• Natural hazards continued

• Floods• Hurricanes

• World population pressures

Page 10: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Quiz Break Section 1

Page 11: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Scientific inquiry

Science assumes the natural world is • Consistent• Predictable

Goal of science • To discover patterns in nature• To use the knowledge to predict

Page 12: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Scientific inquiry An idea can become a

• Hypothesis (tentative or untested explanation) • Theory (tested and confirmed hypothesis) • Paradigm (a theory that explains a large number

of interrelated aspects of the natural world)

Scientific method • Gather facts through observation • Formulate hypotheses and theories

Page 13: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Scientific inquiry

Scientific knowledge is gained through • Following systematic steps

• Collecting facts• Developing a hypothesis • Conduct experiments • Re-examine the hypothesis and accept, modify,

or reject

• Theories that withstand examination • Totally unexpected occurrences

Page 14: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Early evolution of Earth

Origin of Earth • Most researchers believe that Earth and the

other planets formed at essentially the same time

• Nebular hypothesis • Solar system evolved from an enormous rotating

cloud called the solar nebula • Nebula was composed mostly of hydrogen and

helium

Page 15: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Early evolution of Earth

Origin of Earth • Nebular hypothesis continued

• About 5 billion years ago the nebula began to contract

• Assumes a flat, disk shape with the protosun (pre-Sun) at the center

• Inner planets begin to form from metallic and rocky clumps

• Larger outer planets began forming from fragments with a high percentage of ices

Page 16: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

The Nebular hypothesis

Figure 1.7

Page 17: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Early evolution of Earth Formation of Earth’s layered structure

• As Earth formed, the decay of radioactive elements and heat from high-velocity impacts caused the temperature to increase

• Iron and nickel began to melt and sink toward the center

• Lighter rocky components floated outward, toward the surface

• Gaseous material escaped from Earth’s interior to produce the primitive atmosphere

Page 18: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Earth's “Spheres"

Hydrosphere • Ocean – the most prominent feature of the

hydrosphere • Nearly 71% of Earth's surface • About 97% of Earth's water

• Also includes fresh water found in streams, lakes, and glaciers, as well as that found underground

Page 19: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Earth's “Spheres"

Atmosphere • Thin, tenuous blanket of air • One half lies below 5.6 kilometers (3.5 miles)

Biosphere• Includes all life • Concentrated near the surface in a zone that

extends from the ocean floor upward for several kilometers into the atmosphere

Page 20: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Earth's “Spheres"

Solid Earth • Based on compositional differences, it

consists of the crust, mantle, and core• Divisions of the outer portion are based on

how materials behave • Lithosphere - rigid outer layer • Divisions of Earth’s surface - continents and

ocean basins

Page 21: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Quiz Break Section 2

Page 22: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Earth’s layered structureUsing the following:

V = 4/3 π r3

Ave. Crust thickness = ~30 Km

Upper mantle = 670 Km

What makes up the greatest volume of Earth?

a) Crustb) Upper mantlec) Lower mantled) Outer coree) Inner Core

Page 23: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Earth system science

Earth is a dynamic body with many separate but highly interacting parts or spheres

Earth system science studies Earth as a system composed of numerous parts, or subsystems

System - any size group of interacting parts that form a complex whole

Page 24: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Earth system science

System • Closed systems are self-contained (e.g. an

automobile cooling system) • Open systems - both energy and matter

flow into and out of the system (e.g. a river system)

Page 25: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Earth system science

Feedback mechanisms • Negative-feedback mechanisms resist

change and stabilize the system • Positive-feedback mechanisms enhance

the system

Earth as a system • Consists of a nearly endless array of

subsystems (e.g. hydrologic cycle, rock cycle)

Page 26: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Earth system cycles

Figure 1.17

Page 27: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Earth system science

Earth as a system • Sources of energy

• Sun – drives external processes such as weather, ocean circulation and erosional processes

• Earth’s interior – drives internal processes including volcanoes, earthquakes and mountain building

• Humans are part of the Earth system

Page 28: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

Quiz Break Section 3

Page 29: © 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 1 Earth Science 11e Tarbuck/Lutgens

End of Chapter 1