The Physical Universe
17th EditionISBN10: 1260150526
ISBN13: 9781260150520
Copyright: 2020
With the McGraw Hill eBook, students can access their digital textbook on the web or go offline via the ReadAnywhere app for phones or tablets.
McGraw Hill eBook Courses Include:
- Offline reading – study anytime, anywhere
- One interface for all McGraw Hill eBooks
- Highlighting and note-taking
- Syncs across platforms, always up-to-date
- Available for Android and iOS
Rent Monthly
Purchase Options
Students, we’re committed to providing you with high-value course solutions backed by great service and a team that cares about your success. See tabs below to explore options and pricing. Don't forget, we accept financial aid and scholarship funds in the form of credit or debit cards.
McGraw-Hill eBook
- Rent or purchase for a fraction of the printed textbook price
- Easily highlight, take notes and search
- Download the free ReadAnywhere App for offline access and anytime reading
- Watch a quick video to learn more
- Note: the eBook does not include access to Connect. If your instructor assigned Connect, click the "Digital" tab.
Rent Monthly
$9.95/mo
Rent (180 Day)
$50.00
Lifetime
$80.00
Textbook Rental
- Rent for a fraction of the printed textbook price
- Rental transaction occurs through McGraw Hill's authorized rental partner
ISBN10: 1260150526 | ISBN13: 9781260150520
Purchase
$70.00
Loose-Leaf Purchase
- Purchase un-bound 3-ring binder ready textbook
- Flexibility and ease of selecting chapters to take where you want to go
ISBN10: 1260466094 | ISBN13: 9781260466096
Purchase
$130.66
Connect
- Personalize your learning, save time completing homework, and possibly earn a better grade
- Access to eBook, homework and adaptive assignments, videos, and study resources
- Download free ReadAnywhere App for offline access to eBook for anytime reading
- Connect may be assigned as part of your grade. Check with your instructor to see if Connect is used in your course.
ISBN10: 1260466078 | ISBN13: 9781260466072
6 Month
$89.50
Connect + Loose Leaf
- Personalize your learning, save time completing homework, and possibly earn a better grade
- Access to eBook, homework and adaptive assignments, videos, and study resources
- Download free ReadAnywhere App for offline access to eBook for anytime reading
- Purchase un-bound 3-ring binder ready textbook
- Flexibility and ease of selecting chapters to take where you want to go
ISBN10: 1260699285 | ISBN13: 9781260699289
Purchase
$150.65
The estimated amount of time this product will be on the market is based on a number of factors, including faculty input to instructional design and the prior revision cycle and updates to academic research-which typically results in a revision cycle ranging from every two to four years for this product. Pricing subject to change at any time.
The estimated amount of time this product will be on the market is based on a number of factors, including faculty input to instructional design and the prior revision cycle and updates to academic research-which typically results in a revision cycle ranging from every two to four years for this product. Pricing subject to change at any time.
Program Details
1 The Scientific Method
How Scientists Study Nature
1.1 The Scientific Method
1.2 Why Science Is Successful
The Solar System
1.3 A Survey of the Sky
1.4 The Ptolemaic System
1.5 The Copernican System
1.6 Kepler's Laws
1.7 Why Copernicus Was Right
Universal Gravitation
1.8 What Is Gravity?
1.9 Why the Earth Is Round
1.10 The Tides
1.11 The Discovery of Neptune
How Many of What
1.12 The SI System
2 Motion
Describing Motion
2.1 Speed
2.2 Vectors
2.3 Acceleration
2.4 Distance, Time, and Acceleration
Acceleration due to Gravity
2.5 Free Fall
2.6 Air Resistance
Force and Motion
2.7 First law of Motion
2.8 Mass
2.9 Second Law of Motion
2.10 Mass and Weight
2.11 Third Law of Motion
Gravitation
2.12 Circular Motion
2.13 Newton's Law of Gravity
2.14 Artificial Satellites
3 Energy
Work
3.1 The Meaning of Work
3.2 Power
Energy
3.3 Kinetic Energy
3.4 Potential Energy
3.5 Conservation of Energy
3.6 Mechanical Advantage
3.7 The Nature of Heat
Momentum
3.8 Linear Momentum
3.9 Rockets
3.10 Angular Momentum
Relativity
3.11 Special Relativity
3.12 Rest Energy
3.13 General Relativity
4 Energy and the Future
The Energy Problem
4.1 Population and Prosperity
4.2 Energy Supply and Consumption
4.3 Climate Change
4.4 Carbon Dioxide and the Greenhouse Effect
Fossil Fuels
4.5 Liquid Fuels
4.6 Natural Gas
4.7 Coal
Alternative Sources
4.8 A Nuclear World?
4.9 Renewable Energy I
4.10 Renewable Energy II
4.11 Energy Storage
4.12 Biofuels
Strategies for the Future
4.13 Conservation and Geoengineering
4.14 What Governments Must Do
5 Matter and Heat
Temperature and Heat
5.1 Temperature
5.2 Heat
5.3 Metabolic Energy
Fluids
5.4 Density
5.5 Pressure
5.6 Buoyancy
5.7 The Gas Laws
Kinetic Theory of Matter
5.8 Kinetic Theory of Gases
5.9 Molecular Motion and Temperature
5.10 Heat Transfer
Changes of State
5.11 Liquids and Solids
5.12 Evaporation and Boiling
5.13 Melting
Energy Transformations
5.14 Heat Engines
5.15 Thermodynamics
5.16 Fate of the Universe
5.17 Entropy
6 Electricity and Magnetism
Electric Charge
6.1 Positive and Negative Charge
6.2 What Is Charge?
6.3 Coulomb's Law
6.4 Force on an Uncharged Object
Electricity and Matter
6.5 Matter in Bulk
6.6 Conductors and Insulators
6.7 Superconductivity
Electric Current
6.8 The Ampere
6.9 Potential Difference
6.10 Ohm's Law
6.11 Electric Power
Magnetism
6.12 Magnets
6.13 Magnetic Field
6.14 Oersted's Experiment
6.15 Electromagnets
Using Magnetism
6.16 Magnetic Force on a Current
6.17 Electric Motors
6.18 Electromagnetic Induction
6.19 Transformers
7 Waves
Wave Motion
7.1 Water Waves
7.2 Transverse and Longitudinal Waves
7.3 Describing Waves
7.4 Standing Waves
Sound Waves
7.5 Sound
7.6 Doppler Effect
7.7 Musical Sounds
Electromagnetic Waves
7.8 Electromagnetic Waves
7.9 Types of EM Waves
7.10 Light "Rays"
Wave Behavior
7.11 Reflection
7.12 Refraction
7.13 Lenses
7.14 The Eye
7.15 Color
7.16 Interference
7.17 Diffraction
8 The Nucleus
Atom and Nucleus
8.1 Rutherford Model of the Atom
8.2 Nuclear Structure
Radioactivity
8.3 Radioactive Decay
8.4 Half-Life
8.5 Radiation Hazards
Nuclear Energy
8.6 Units of Mass and Energy
8.7 Binding Energy
8.8 Binding Energy per Nucleon
Fission and Fusion
8.9 Nuclear Fission
8.10 How a Reactor Works
8.11 Reactor Accidents
8.12 Plutonium
8.13 Nuclear Fusion
Elementary Particles
8.14 Antiparticles
8.15 Fundamental Interactions
8.16 Leptons and Hadrons
9 The Atom
Quantum Theory of Light
9.1 Photoelectric Effect
9.2 Photons
9.3 What Is Light?
9.4 X-Rays
Matter Waves
9.5 De Broglie Waves
9.6 Waves of What?
9.7 Uncertainty Principle
The Hydrogen Atom
9.8 Atomic Spectra
9.9 The Bohr Model
9.10 Electron Waves and Orbitals
9.11 The Laser
Quantum Theory of the Atom
9.12 Quantum Mechanics
9.13 Quantum Numbers
9.14 Exclusion Principle
10 The Periodic Law
Elements and Compounds
10.1 Chemical Change
10.2 Three Classes of Matter
10.3 The Atomic Theory
The Periodic Law
10.4 Metals and Nonmetals
10.5 Chemical Activity
10.6 Families of Elements
10.7 The Periodic Table
10.8 Groups and Periods
Atomic Structure
10.9 Shells and Subshells
10.10 Explaining the Periodic Table
Chemical Bonds
10.11 Types of Bond
10.12 Covalent Bonding
10.13 Ionic Bonding
10.14 Ionic Compounds
10.15 Naming Compounds
10.16 Chemical Equations
10.17 Types of Chemical Reactions
11 Crystals, Ions, and Solutions
Solids
11.1 Ionic and Covalent Crystals
11.2 The Metallic Bond
11.3 Molecular Crystals
Solutions
11.4 Solubility
11.5 Polar and Nonpolar Liquids
11.6 Ions in Solution
11.7 Evidence for Dissociation
11.8 Water
11.9 Water Pollution
Acids and Bases
11.10 Acids
11.11 Strong and Weak Acids
11.12 Bases
11.13 The pH Scale
11.14 Salts
12 Chemical Reactions
Quantitative Chemistry
12.1 Phlogiston
12.2 Oxygen
12.3 The Mole
12.4 Formula Units
Chemical Energy
12.5 Exothermic and Endothermic Reactions
12.6 Chemical Energy and Stability
12.7 Activation energy
Reaction Rates
12.8 Temperature and Reaction Rates
12.9 Other Factors
12.10 Chemical Equilibrium
12.11 Altering an Equilibrium
Oxidation and Reduction
12.12 Oxidation-Reduction Reactions
12.13 Electrochemical cells
13 Organic Chemistry
Carbon Compounds
13.1 Carbon Bonds
13.2 Alkanes
13.3 Petroleum Products
Structures of Organic Molecules
13.4 Structural Formulas
13.5 Isomers
13.6 Unsaturated Hydrocarbons
13.7 Benzene
Organic Compounds
13.8 Hydrocarbon Groups
13.9 Functional Groups
13.10 Polymers
Chemistry of Life
13.11 Carbohydrates
13.12 Photosynthesis
13.13 Lipids
13.14 Proteins
13.15 Soil Nitrogen
13.16 Nucleic Acids
13.17 Origin of Life
14 Atmosphere and Hydrosphere
The Atmosphere
14.1 Regions of the Atmosphere
14.2 Atmospheric Moisture
14.3 Clouds
Weather
14.4 Atmospheric Energy
14.5 The Seasons
14.6 Winds
14.7 General Circulation of the Atmosphere
14.8 Middle-Latitude Weather Systems
Climate
14.9 Tropical Climates
14.10 Middle- and High-Latitude Climates
14.11 Climatic Change
The Hydrosphere
14.12 Ocean Basins
14.13 Ocean Currents
15 The Rock Cycle
Rocks
15.1 Composition of the Crust
15.2 Minerals
15.3 Igneous Rocks
15.4 Sedimentary Rocks
15.5 Metamorphic Rocks
Within the Earth
15.6 Earthquakes
15.7 Structure of the Earth
15.8 The Earth's Interior
15.9 Geomagnetism
Erosion
15.10 Weathering
15.11 Stream Erosion
15.12 Glaciers
15.13 Groundwater
15.14 Sedimentation
Vulcanism
15.15 Volcanoes
15.16 Intrusive Rocks
15.17 The Rock Cycle
16 The Evolving Earth
Tectonic Movement
16.1 Types of Movement
16.2 Mountain Building
16.3 Continental Drift
Plate Tectonics
16.4 Lithosphere and Asthenosphere
16.5 The Ocean Floors
16.6 Ocean-Floor Spreading
16.7 Plate Tectonics
Methods of Historical Geology
16.8 Principles of Uniform Change
16.9 Rock Formations
16.10 Radiometric Dating
16.11 Fossils
16.12 Geologic Time
Earth History
16.13 Precambrian Time
16.14 The Paleozoic Era
16.15 Coal and Petroleum
16.16 The Mesozoic Era
16.17 The Cenozoic Era
16.18 Human History
17 The Solar System
The Family of the Sun
17.1 The Solar System
17.2 Comets
17.3 Meteors
The Inner Planets
17.4 Mercury
17.5 Venus
17.6 Mars
17.7 Is There Life On Mars?
17.8 Asteroids
The Outer Planets
17.9 Jupiter
17.10 Saturn
17.11 Uranus, Neptune, Pluto, and More
The Moon
17.12 Phases of the Moon
17.13 Eclipses
17.14 Lunar Surface and Interior
17.15 Evolution of the Lunar Landscape
17.16 Origin of the Moon
18 The Stars
Tools of Astronomy
18.1 The Telescope
18.2 The Spectrometer
18.3 Spectrum Analysis
The Sun
18.4 Properties of the Sun
18.5 The Aurora
18.6 Sunspots
18.7 Solar Energy
The Stars
18.8 Stellar Distances
18.9 Variable Stars
18.10 Stellar Motions
18.11 Stellar Properties
Life Histories of the Stars
18.12 H-R Diagrams
18.13 Stellar Evolution
18.14 Supernovas
18.15 Pulsars
18.16 Black Holes
19 The Universe
Galaxies
19.1 The Milky Way
19.2 Stellar Populations
19.3 Radio Astronomy
19.4 Galaxies
19.5 Cosmic Rays
The Expanding Universe
19.6 Red Shifts
19.7 Quasars
Evolution of the Universe
19.8 Dating the Universe
19.9 After the Big Bang
19.10 Origin of the Solar System
Extraterrestrial Life
19.11 Exoplanets
19.12 Interstellar Travel
19.13 Interstellar Communication
Math Refresher
The Elements
Answers to Multiple-Choice Questions and Odd-Numbered Exercises
About the Author
Konrad Krauskopf
Konrad B. Krauskopf was born and raised in Madison, Wisconsin and earned a B.S. in chemistry from University of Wisconsin in 1931. He then earned a Ph.D. in chemistry at the University of California in Berkeley. When the Great Depression made jobs in chemistry scarce, Professor Krauskopf decided to study geology, which had long fascinated him. Through additional graduate work at Stanford University, he earned a second Ph.D. and eventually a position on the Stanford faculty. He remained at Stanford until his retirement in 1976. During his tenure, Professor Krauskopf also worked at various times with the U.S. Geological Survey, served with the U.S. army in occupied Japan, and traveled to Norway, France, and Germany on sabbatical leaves. His research interests included field work on granites and metamorphic rocks and laboratory study on applications of chemistry to geologic problems, especially the formation of ore deposits. In recent years, Professor Krauskopf had spent time working with various government agencies on the problem of radioactive waste disposal. Professor Krauskopf passed away on May 8, 2003.
Arthur Beiser
Arthur Beiser, a native of New York City, received B.S., M.S., and Ph.D. degrees in physics from New York University, where he later served as Associate Professor of Physics. He then was a Senior Research Scientist at the Lamont Geo- logical Observatory of Columbia University. His research interests were chiefly in cosmic rays and in magnetohydrodynamics as applied to geophysics and astrophys- ics. In addition to theoretical work, he participated in a cosmic-ray expedition to an Alaskan peak and directed a search for magnetohydrodynamic waves from space in various Pacific locations. A Fellow of The Explorers Club, Dr. Beiser was the first chairman of its Committee on Space Exploration. He is the author or coauthor of 36 books, mostly college texts on physics and mathematics, 14 of which have been translated into a total of 27 languages. Two of his books are on sailing, The Proper Yacht and The Sailor’s World. Figure 13-21 is a photograph of Dr. Beiser at the helm of his 58-ft sloop; he and his wife Germaine have sailed over 150,000 miles, includ- ing two Atlantic crossings and a rounding of Cape Horn. Germaine Beiser, who has degrees in physics from the Massachusetts Institute of Technology and New York University, is the author or coauthor of seven books on various aspects of physics and has contributed to The Physical Universe. For a number of years she was the editor of a cruising guide to the Adriatic Sea.
Affordability
Find out more about our affordable course material programs.
Reduce course material costs for your students while still providing full access to everything they need to be successful. It isn't too good to be true - it's Inclusive Access.
Learn more about Inclusive Access here.
When your students still want a book but don't want to keep it, McGraw-Hill's Textbook Rental program provides students with our latest editions at our most affordable hardcover prices.
Learn more about our Textbook Rental program.
Want more information?
By prompting students to engage with key concepts, while continually adapting to their individual needs, Connect activates learning and empowers students to take control resulting in better grades and increased retention rates. Proven online content integrates seamlessly with our adaptive technology, and helps build student confidence outside of the classroom.
Learn moreEquip students with adaptive, mobile study resources. They'll be better prepared in less time. They'll thank you.
Learn moreHow to Access Instructor Tools for your Course
- To get started, you'll need to visit connect.mheducation.com to sign in. (If you do not have an account, you'll need to request one from your MH rep. To find your rep – visit the Find Your Rep page).
- Then, under "Find a Title," you'll search by title, author or subject.
- Select your desired title and create a course. (Note – you do not have to create assignments, just a course instance)
- Then go to your Connect course homepage.
- In the top navigation, select library to access the instructor resources that accompany the title.
Accessibility Rubric
Creating accessible products is a priority for McGraw-Hill. We have put in place processes to make accessibility and meeting the WCAG AA guidelines part of our day-to-day development efforts and product roadmaps.
Please review our accessibility information for this specific product.
In future editions, this rubric will be reformatted to increase accessibility and usability.
McGraw-Hill sites may contain links to websites owned and operated by third parties. These links are provided as supplementary materials, and for learners’ information and convenience only. McGraw-Hill has no control over and is not responsible for the content or accessibility of any linked website.
For further information on McGraw‐Hill and Accessibility, please visit our accessibility page or contact us at accessibility@mheducation.com
1 The Scientific Method
How Scientists Study Nature
1.1 The Scientific Method
1.2 Why Science Is Successful
The Solar System
1.3 A Survey of the Sky
1.4 The Ptolemaic System
1.5 The Copernican System
1.6 Kepler's Laws
1.7 Why Copernicus Was Right
Universal Gravitation
1.8 What Is Gravity?
1.9 Why the Earth Is Round
1.10 The Tides
1.11 The Discovery of Neptune
How Many of What
1.12 The SI System
2 Motion
Describing Motion
2.1 Speed
2.2 Vectors
2.3 Acceleration
2.4 Distance, Time, and Acceleration
Acceleration due to Gravity
2.5 Free Fall
2.6 Air Resistance
Force and Motion
2.7 First law of Motion
2.8 Mass
2.9 Second Law of Motion
2.10 Mass and Weight
2.11 Third Law of Motion
Gravitation
2.12 Circular Motion
2.13 Newton's Law of Gravity
2.14 Artificial Satellites
3 Energy
Work
3.1 The Meaning of Work
3.2 Power
Energy
3.3 Kinetic Energy
3.4 Potential Energy
3.5 Conservation of Energy
3.6 Mechanical Advantage
3.7 The Nature of Heat
Momentum
3.8 Linear Momentum
3.9 Rockets
3.10 Angular Momentum
Relativity
3.11 Special Relativity
3.12 Rest Energy
3.13 General Relativity
4 Energy and the Future
The Energy Problem
4.1 Population and Prosperity
4.2 Energy Supply and Consumption
4.3 Climate Change
4.4 Carbon Dioxide and the Greenhouse Effect
Fossil Fuels
4.5 Liquid Fuels
4.6 Natural Gas
4.7 Coal
Alternative Sources
4.8 A Nuclear World?
4.9 Renewable Energy I
4.10 Renewable Energy II
4.11 Energy Storage
4.12 Biofuels
Strategies for the Future
4.13 Conservation and Geoengineering
4.14 What Governments Must Do
5 Matter and Heat
Temperature and Heat
5.1 Temperature
5.2 Heat
5.3 Metabolic Energy
Fluids
5.4 Density
5.5 Pressure
5.6 Buoyancy
5.7 The Gas Laws
Kinetic Theory of Matter
5.8 Kinetic Theory of Gases
5.9 Molecular Motion and Temperature
5.10 Heat Transfer
Changes of State
5.11 Liquids and Solids
5.12 Evaporation and Boiling
5.13 Melting
Energy Transformations
5.14 Heat Engines
5.15 Thermodynamics
5.16 Fate of the Universe
5.17 Entropy
6 Electricity and Magnetism
Electric Charge
6.1 Positive and Negative Charge
6.2 What Is Charge?
6.3 Coulomb's Law
6.4 Force on an Uncharged Object
Electricity and Matter
6.5 Matter in Bulk
6.6 Conductors and Insulators
6.7 Superconductivity
Electric Current
6.8 The Ampere
6.9 Potential Difference
6.10 Ohm's Law
6.11 Electric Power
Magnetism
6.12 Magnets
6.13 Magnetic Field
6.14 Oersted's Experiment
6.15 Electromagnets
Using Magnetism
6.16 Magnetic Force on a Current
6.17 Electric Motors
6.18 Electromagnetic Induction
6.19 Transformers
7 Waves
Wave Motion
7.1 Water Waves
7.2 Transverse and Longitudinal Waves
7.3 Describing Waves
7.4 Standing Waves
Sound Waves
7.5 Sound
7.6 Doppler Effect
7.7 Musical Sounds
Electromagnetic Waves
7.8 Electromagnetic Waves
7.9 Types of EM Waves
7.10 Light "Rays"
Wave Behavior
7.11 Reflection
7.12 Refraction
7.13 Lenses
7.14 The Eye
7.15 Color
7.16 Interference
7.17 Diffraction
8 The Nucleus
Atom and Nucleus
8.1 Rutherford Model of the Atom
8.2 Nuclear Structure
Radioactivity
8.3 Radioactive Decay
8.4 Half-Life
8.5 Radiation Hazards
Nuclear Energy
8.6 Units of Mass and Energy
8.7 Binding Energy
8.8 Binding Energy per Nucleon
Fission and Fusion
8.9 Nuclear Fission
8.10 How a Reactor Works
8.11 Reactor Accidents
8.12 Plutonium
8.13 Nuclear Fusion
Elementary Particles
8.14 Antiparticles
8.15 Fundamental Interactions
8.16 Leptons and Hadrons
9 The Atom
Quantum Theory of Light
9.1 Photoelectric Effect
9.2 Photons
9.3 What Is Light?
9.4 X-Rays
Matter Waves
9.5 De Broglie Waves
9.6 Waves of What?
9.7 Uncertainty Principle
The Hydrogen Atom
9.8 Atomic Spectra
9.9 The Bohr Model
9.10 Electron Waves and Orbitals
9.11 The Laser
Quantum Theory of the Atom
9.12 Quantum Mechanics
9.13 Quantum Numbers
9.14 Exclusion Principle
10 The Periodic Law
Elements and Compounds
10.1 Chemical Change
10.2 Three Classes of Matter
10.3 The Atomic Theory
The Periodic Law
10.4 Metals and Nonmetals
10.5 Chemical Activity
10.6 Families of Elements
10.7 The Periodic Table
10.8 Groups and Periods
Atomic Structure
10.9 Shells and Subshells
10.10 Explaining the Periodic Table
Chemical Bonds
10.11 Types of Bond
10.12 Covalent Bonding
10.13 Ionic Bonding
10.14 Ionic Compounds
10.15 Naming Compounds
10.16 Chemical Equations
10.17 Types of Chemical Reactions
11 Crystals, Ions, and Solutions
Solids
11.1 Ionic and Covalent Crystals
11.2 The Metallic Bond
11.3 Molecular Crystals
Solutions
11.4 Solubility
11.5 Polar and Nonpolar Liquids
11.6 Ions in Solution
11.7 Evidence for Dissociation
11.8 Water
11.9 Water Pollution
Acids and Bases
11.10 Acids
11.11 Strong and Weak Acids
11.12 Bases
11.13 The pH Scale
11.14 Salts
12 Chemical Reactions
Quantitative Chemistry
12.1 Phlogiston
12.2 Oxygen
12.3 The Mole
12.4 Formula Units
Chemical Energy
12.5 Exothermic and Endothermic Reactions
12.6 Chemical Energy and Stability
12.7 Activation energy
Reaction Rates
12.8 Temperature and Reaction Rates
12.9 Other Factors
12.10 Chemical Equilibrium
12.11 Altering an Equilibrium
Oxidation and Reduction
12.12 Oxidation-Reduction Reactions
12.13 Electrochemical cells
13 Organic Chemistry
Carbon Compounds
13.1 Carbon Bonds
13.2 Alkanes
13.3 Petroleum Products
Structures of Organic Molecules
13.4 Structural Formulas
13.5 Isomers
13.6 Unsaturated Hydrocarbons
13.7 Benzene
Organic Compounds
13.8 Hydrocarbon Groups
13.9 Functional Groups
13.10 Polymers
Chemistry of Life
13.11 Carbohydrates
13.12 Photosynthesis
13.13 Lipids
13.14 Proteins
13.15 Soil Nitrogen
13.16 Nucleic Acids
13.17 Origin of Life
14 Atmosphere and Hydrosphere
The Atmosphere
14.1 Regions of the Atmosphere
14.2 Atmospheric Moisture
14.3 Clouds
Weather
14.4 Atmospheric Energy
14.5 The Seasons
14.6 Winds
14.7 General Circulation of the Atmosphere
14.8 Middle-Latitude Weather Systems
Climate
14.9 Tropical Climates
14.10 Middle- and High-Latitude Climates
14.11 Climatic Change
The Hydrosphere
14.12 Ocean Basins
14.13 Ocean Currents
15 The Rock Cycle
Rocks
15.1 Composition of the Crust
15.2 Minerals
15.3 Igneous Rocks
15.4 Sedimentary Rocks
15.5 Metamorphic Rocks
Within the Earth
15.6 Earthquakes
15.7 Structure of the Earth
15.8 The Earth's Interior
15.9 Geomagnetism
Erosion
15.10 Weathering
15.11 Stream Erosion
15.12 Glaciers
15.13 Groundwater
15.14 Sedimentation
Vulcanism
15.15 Volcanoes
15.16 Intrusive Rocks
15.17 The Rock Cycle
16 The Evolving Earth
Tectonic Movement
16.1 Types of Movement
16.2 Mountain Building
16.3 Continental Drift
Plate Tectonics
16.4 Lithosphere and Asthenosphere
16.5 The Ocean Floors
16.6 Ocean-Floor Spreading
16.7 Plate Tectonics
Methods of Historical Geology
16.8 Principles of Uniform Change
16.9 Rock Formations
16.10 Radiometric Dating
16.11 Fossils
16.12 Geologic Time
Earth History
16.13 Precambrian Time
16.14 The Paleozoic Era
16.15 Coal and Petroleum
16.16 The Mesozoic Era
16.17 The Cenozoic Era
16.18 Human History
17 The Solar System
The Family of the Sun
17.1 The Solar System
17.2 Comets
17.3 Meteors
The Inner Planets
17.4 Mercury
17.5 Venus
17.6 Mars
17.7 Is There Life On Mars?
17.8 Asteroids
The Outer Planets
17.9 Jupiter
17.10 Saturn
17.11 Uranus, Neptune, Pluto, and More
The Moon
17.12 Phases of the Moon
17.13 Eclipses
17.14 Lunar Surface and Interior
17.15 Evolution of the Lunar Landscape
17.16 Origin of the Moon
18 The Stars
Tools of Astronomy
18.1 The Telescope
18.2 The Spectrometer
18.3 Spectrum Analysis
The Sun
18.4 Properties of the Sun
18.5 The Aurora
18.6 Sunspots
18.7 Solar Energy
The Stars
18.8 Stellar Distances
18.9 Variable Stars
18.10 Stellar Motions
18.11 Stellar Properties
Life Histories of the Stars
18.12 H-R Diagrams
18.13 Stellar Evolution
18.14 Supernovas
18.15 Pulsars
18.16 Black Holes
19 The Universe
Galaxies
19.1 The Milky Way
19.2 Stellar Populations
19.3 Radio Astronomy
19.4 Galaxies
19.5 Cosmic Rays
The Expanding Universe
19.6 Red Shifts
19.7 Quasars
Evolution of the Universe
19.8 Dating the Universe
19.9 After the Big Bang
19.10 Origin of the Solar System
Extraterrestrial Life
19.11 Exoplanets
19.12 Interstellar Travel
19.13 Interstellar Communication
Math Refresher
The Elements
Answers to Multiple-Choice Questions and Odd-Numbered Exercises
About the Author
Konrad Krauskopf
Konrad B. Krauskopf was born and raised in Madison, Wisconsin and earned a B.S. in chemistry from University of Wisconsin in 1931. He then earned a Ph.D. in chemistry at the University of California in Berkeley. When the Great Depression made jobs in chemistry scarce, Professor Krauskopf decided to study geology, which had long fascinated him. Through additional graduate work at Stanford University, he earned a second Ph.D. and eventually a position on the Stanford faculty. He remained at Stanford until his retirement in 1976. During his tenure, Professor Krauskopf also worked at various times with the U.S. Geological Survey, served with the U.S. army in occupied Japan, and traveled to Norway, France, and Germany on sabbatical leaves. His research interests included field work on granites and metamorphic rocks and laboratory study on applications of chemistry to geologic problems, especially the formation of ore deposits. In recent years, Professor Krauskopf had spent time working with various government agencies on the problem of radioactive waste disposal. Professor Krauskopf passed away on May 8, 2003.
Arthur Beiser
Arthur Beiser, a native of New York City, received B.S., M.S., and Ph.D. degrees in physics from New York University, where he later served as Associate Professor of Physics. He then was a Senior Research Scientist at the Lamont Geo- logical Observatory of Columbia University. His research interests were chiefly in cosmic rays and in magnetohydrodynamics as applied to geophysics and astrophys- ics. In addition to theoretical work, he participated in a cosmic-ray expedition to an Alaskan peak and directed a search for magnetohydrodynamic waves from space in various Pacific locations. A Fellow of The Explorers Club, Dr. Beiser was the first chairman of its Committee on Space Exploration. He is the author or coauthor of 36 books, mostly college texts on physics and mathematics, 14 of which have been translated into a total of 27 languages. Two of his books are on sailing, The Proper Yacht and The Sailor’s World. Figure 13-21 is a photograph of Dr. Beiser at the helm of his 58-ft sloop; he and his wife Germaine have sailed over 150,000 miles, includ- ing two Atlantic crossings and a rounding of Cape Horn. Germaine Beiser, who has degrees in physics from the Massachusetts Institute of Technology and New York University, is the author or coauthor of seven books on various aspects of physics and has contributed to The Physical Universe. For a number of years she was the editor of a cruising guide to the Adriatic Sea.
Affordability
Find out more about our affordable course material programs.
Reduce course material costs for your students while still providing full access to everything they need to be successful. It isn't too good to be true - it's Inclusive Access.
Learn more about Inclusive Access here.
When your students still want a book but don't want to keep it, McGraw-Hill's Textbook Rental program provides students with our latest editions at our most affordable hardcover prices.
Learn more about our Textbook Rental program.
Want more information?
By prompting students to engage with key concepts, while continually adapting to their individual needs, Connect activates learning and empowers students to take control resulting in better grades and increased retention rates. Proven online content integrates seamlessly with our adaptive technology, and helps build student confidence outside of the classroom.
Learn moreEquip students with adaptive, mobile study resources. They'll be better prepared in less time. They'll thank you.
Learn moreHow to Access Instructor Tools for your Course
- To get started, you'll need to visit connect.mheducation.com to sign in. (If you do not have an account, you'll need to request one from your MH rep. To find your rep – visit the Find Your Rep page).
- Then, under "Find a Title," you'll search by title, author or subject.
- Select your desired title and create a course. (Note – you do not have to create assignments, just a course instance)
- Then go to your Connect course homepage.
- In the top navigation, select library to access the instructor resources that accompany the title.
Accessibility Rubric
Creating accessible products is a priority for McGraw-Hill. We have put in place processes to make accessibility and meeting the WCAG AA guidelines part of our day-to-day development efforts and product roadmaps.
Please review our accessibility information for this specific product.
In future editions, this rubric will be reformatted to increase accessibility and usability.
McGraw-Hill sites may contain links to websites owned and operated by third parties. These links are provided as supplementary materials, and for learners’ information and convenience only. McGraw-Hill has no control over and is not responsible for the content or accessibility of any linked website.
For further information on McGraw‐Hill and Accessibility, please visit our accessibility page or contact us at accessibility@mheducation.com
Shipping Options
- Standard
- Next day air
- 2nd day air
- 3rd day air
Rent Now
You will be taken to our partner Chegg.com to complete your transaction.
After completing your transaction, you can access your course using the section url supplied by your instructor.