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Understanding Our Universe Third Edition [Multiple-component retail product]

3.70/5 (64 ratings by Goodreads)
(Barnard College), (University of California, Santa Cruz), (Weber State University)
  • Formatas: Multiple-component retail product, 576 pages, aukštis x plotis x storis: 274x246x18 mm, weight: 1193 g, Contains 1 Paperback / softback and 1 Digital product license key
  • Išleidimo metai: 04-Sep-2018
  • Leidėjas: WW Norton & Co
  • ISBN-10: 0393631710
  • ISBN-13: 9780393631715
Kitos knygos pagal šią temą:
  • Formatas: Multiple-component retail product, 576 pages, aukštis x plotis x storis: 274x246x18 mm, weight: 1193 g, Contains 1 Paperback / softback and 1 Digital product license key
  • Išleidimo metai: 04-Sep-2018
  • Leidėjas: WW Norton & Co
  • ISBN-10: 0393631710
  • ISBN-13: 9780393631715
Kitos knygos pagal šią temą:
Research shows that active learning supports deeper, long-term understanding. The Third Edition text and media package gives students more opportunities to interact with astronomy—both in real life and online. The new edition provides all the resources you need to make it easy to incorporate active learning into the classroom.

Students learn best by doing

Daugiau informacijos

with Ebook and Smartwork5
AstroTours xvi
Interactive Simulations xvi
Astronomy in Action Videos xvi
Preface xvii
About the Authors xxviii
PART I INTRODUCTION TO ASTRONOMY
1 Our Place in the Universe
2(20)
1.1 Astronomy Gives Us a Universal Context
4(4)
1.2 Science Is a Way of Viewing the World
8(3)
1.3 Astronomers Use Mathematics to Find Patterns
11(11)
Working it Out 1.1 Units and Scientific Notation
14(2)
Reading Astronomy News: "Breakthrough: Scientists Detect Einstein's Gravity Ripples"
16(2)
Summary
18(1)
Questions and Problems
18(3)
Exploration: Logical Fallacies
21(1)
2 Patterns in the Sky---Motions of Earth and the Moon
22(26)
2.1 Earth Spins on Its Axis
24(6)
2.2 Revolution Around the Sun Leads to Changes during the Year
30(7)
Working it Out 2.1 Manipulating Equations
31(6)
2.3 The Moon's Appearance Changes as It Orbits Earth
37(2)
2.4 Shadows Cause Eclipses
39(9)
Reading Astronomy News: "Eclipse 2017: `I Need Like Two More Hours of That'"
42(2)
Summary
44(1)
Questions and Problems
44(3)
Exploration: Phases of the Moon
47(1)
3 Laws of Motion
48(26)
3.1 Astronomers Have Studied the Motions of the Planets Since Ancient Times
50(5)
Working it Out 3.1 Kepler's Third Law
54(1)
3.2 Galileo Was the First Modern Scientist
55(1)
3.3 Newton's Laws Govern Motion
56(4)
Working it Out 3.2 Finding the Acceleration
58(2)
3.4 Gravity Is a Force between Any Two Massive Objects
60(4)
Working it Out 3.3 Newton's Law of Gravity: Playing with Proportionality
62(2)
3.5 Orbits Are One Body "Falling Around" Another
64(10)
Reading Astronomy News: "Curiosity, Interrupted: Sun Makes Mars Go Dark"
68(2)
Summary
70(1)
Questions and Problems
70(3)
Exploration: Newtonian Features
73(1)
4 Light and Telescopes
74(24)
4.1 What Is Light?
76(7)
Working it Out 4.1 Wavelength and Frequency
79(4)
4.2 Cameras and Spectrographs Record Astronomical Data
83(3)
4.3 Telescopes Collect Light
86(12)
Working it Out 4.2 Diffraction Limit
91(2)
Reading Astronomy News: "NASA's James Webb Space Telescope Could Study Planet 9"
93(1)
Summary
94(1)
Questions and Problems
95(2)
Exploration: Light as a Wave
97(1)
PART II THE SOLAR SYSTEM
5 The Formation of Stars and Planets
98(30)
5.1 Molecular Clouds Are the Cradles of Star Formation
100(2)
5.2 The Protostar Becomes a Star
102(5)
Working it Out 5.1 The Stefan-Boltzmann Law and Wien's Law
103(4)
5.3 Planets Form in a Disk around the Protostar
107(6)
5.4 The Inner and Outer Disk Have Different Compositions
113(1)
5.5 A Case Study: The Solar System
114(3)
5.6 Planetary Systems Are Common
117(11)
Working it Out 5.2 Making Use of the Doppler Shift
119(4)
Reading Astronomy News: "Kepler Provides More Information About Trappist-1"
123(1)
Summary
124(1)
Questions and Problems
124(3)
Exploration: Exploring Extrasolar Planets
127(1)
6 Terrestrial Worlds in the Inner Solar System
128(32)
6.1 Impacts Help Shape the Terrestrial Planets
130(6)
Working it Out 6.1 How to Read Cosmic Clocks
135(1)
6.2 The Surfaces of Terrestrial Planets Are Affected by Processes in the Interior
136(6)
Working it Out 6.2 The Density of Earth
137(5)
6.3 Planetary Surfaces Evolve through Tectonism
142(5)
6.4 Volcanism Reveals a Geologically Active Planet
147(3)
6.5 Wind and Water Modify Surfaces
150(10)
Reading Astronomy News: "Mars Canyon Study Adds Clues about Possible Water"
154(2)
Summary
156(1)
Questions and Problems
156(3)
Exploration: Earth's Tides
159(1)
7 Atmospheres of Venus, Earth, and Mars
160(28)
7.1 Atmospheres Change over Time
162(2)
7.2 Secondary Atmospheres Evolve
164(5)
Working it Out 7.1 How Can We Find the Temperature of a Planet?
166(3)
7.3 Earth's Atmosphere Has Detailed Structure
169(7)
7.4 The Atmospheres of Venus and Mars Differ from Earth's
176(3)
7.5 Earth's Climate Is Changing
179(9)
Reading Astronomy News: "Curiosity Rover Sees Signs of Vanishing Martian Atmosphere"
183(1)
Summary
184(1)
Questions and Problems
184(3)
Exploration: Climate Change
187(1)
8 The Giant Planets
188(30)
8.1 Giant Planets Are Large, Cold, and Massive
190(5)
Working it Out 8.1 Finding the Diameter of a Giant Planet
193(2)
8.2 The Giant Planets Have Clouds and Weather
195(7)
Working it Out 8.2 Measuring Wind Speeds on Distant Planets
200(2)
8.3 The Interiors of the Giant Planets Are Hot and Dense
202(3)
Working it Out 8.3 Internal Thermal Energy Heats the Giant Planets
204(1)
8.4 The Giant Planets Are Magnetic Powerhouses
205(3)
8.5 Rings Surround the Giant Planets
208(10)
Reading Astronomy News: "Giant Propeller Structures Seen in Saturn's Rings"
212(2)
Summary
214(1)
Questions and Problems
214(3)
Exploration: Estimating Rotation Periods of Giant Planets
217(1)
9 Small Bodies of the Solar System
218(32)
9.1 Dwarf Planets May Outnumber Planets
220(2)
9.2 Moons as Small Worlds
222(7)
9.3 Asteroids Are Pieces of the Past
229(3)
9.4 Comets Are Clumps of Ice
232(6)
9.5 Comet and Asteroid Collisions Still Happen Today
238(3)
Working it Out 9.1 Finding the Radius of a Meteoroid
240(1)
9.6 Meteorites Are Remnants of the Early Solar System
241(9)
Reading Astronomy News: "The Rosetta Probe Has Officially Stopped Listening for Philae, Its Little Lost Comet Lander"
245(1)
Summary
246(1)
Questions and Problems
246(3)
Exploration: Comparative Dwarf Planetology
249(1)
PART III STARS AND STELLAR EVOLUTION
10 Measuring the Stars
250(30)
10.1 The Luminosity of a Star Can Be Found from the Brightness and the Distance
252(6)
Working it Out 10.1 Parallax and Distance
256(2)
10.2 Radiation Tells Us the Temperature, Size, and Composition of Stars
258(10)
10.3 The Mass of a Star Can Be Determined in Some Binary Systems
268(3)
10.4 The H-R Diagram Is the Key to Understanding Stars
271(9)
Reading Astronomy News: "Mystery of Nearby SS Cygni Star System Finally Resolved"
275(1)
Summary
276(1)
Questions and Problems
276(3)
Exploration: The H-R Diagram
279(1)
11 Our Star: The Sun
280(28)
11.1 The Structure of the Sun Is a Matter of Balance
282(5)
Working it Out 11.1 How Much Longer Will the Sun "Live"?
284(3)
11.2 Energy in the Sun's Core Moves through Radiation and Convection
287(4)
11.3 The Atmosphere of the Sun
291(3)
11.4 The Atmosphere of the Sun Is Very Active
294(14)
Working it Out 11.2 Sunspots and Temperature
296(6)
Reading Astronomy News: "Weather Forecast in Space: Not Sunny, with Solar Flares"
302(1)
Summary
303(1)
Questions and Problems
304(3)
Exploration: The Proton-Proton Chain
307(1)
12 Evolution of Low-Mass Stars
308(28)
12.1 The Life of a Main-Sequence Star Follows a Predictable Path
310(3)
Working it Out 12.1 Estimating Main-Sequence Lifetimes
312(1)
12.2 A Star Runs Out of Hydrogen and Leaves the Main Sequence
313(3)
12.3 Helium Begins to Burn in the Degenerate Core
316(3)
12.4 The Low-Mass Star Enters the Last Stages of Its Evolution
319(6)
12.5 Binary Stars Sometimes Share Mass, Resulting in Novae and Supernovae
325(3)
12.6 Star Clusters Are Snapshots of Stellar Evolution
328(8)
Reading Astronomy News: "Scientists May Be Missing Many Star Explosions"
331(1)
Summary
332(1)
Questions and Problems
332(3)
Exploration: Evolution of Low-Mass Stars
335(1)
13 Evolution of High-Mass Stars
336(34)
13.1 High-Mass Stars Follow Their Own Path
338(4)
13.2 High-Mass Stars Go Out with a Bang
342(3)
13.3 Supernovae Change the Galaxy
345(5)
13.4 Einstein Moved Beyond Newtonian Physics
350(5)
Working it Out 13.1 The Boxcar Experiment
353(2)
13.5 Gravity Is a Distortion of Spacetime
355(6)
13.6 Black Holes Are a Natural Limit
361(9)
Working it Out 13.2 Finding the Schwarzschild Radius
362(3)
Reading Astronomy News: "LIGO Is Back and It's on the Hunt for Gravitational Waves Again"
365(1)
Summary
366(1)
Questions and Problems
366(3)
Exploration: The CNO Cycle
369(1)
PART IV GALAXIES, THE UNIVERSE, AND COSMOLOGY
14 Measuring Galaxies
370(26)
14.1 Galaxies Come in Many Sizes and Shapes
372(5)
14.2 There Are Many Ways to Measure Distance
377(4)
14.3 We Live in an Expanding Universe
381(3)
Working it Out 14.1 Redshift: Calculating the Recession Velocities and Distances of Galaxies
383(1)
14.4 A Supermassive Black Hole Exists at the Heart of Most Galaxies
384(12)
Reading Astronomy News: "Colliding Galaxies Swirl in Dazzling New Photo"
391(1)
Summary
392(1)
Questions and Problems
393(2)
Exploration: Galaxy Classification
395(1)
15 Our Galaxy: The Milky Way
396(26)
15.1 Galaxies Are Mostly Dark Matter
398(6)
Working it Out 15.1 Finding the Mass of a Galaxy
402(2)
15.2 Stars Form in the Spiral Arms of a Galaxy's Disk
404(4)
15.3 Components of the Milky Way Reveal Its Evolution
408(6)
15.4 The Milky Way Offers Clues about How Galaxies Form
414(8)
Reading Astronomy News: "Hyperfast Star Kicked Out of Milky Way"
416(2)
Summary
418(1)
Questions and Problems
418(3)
Exploration: Dark Matter in a Galaxy
421(1)
16 The Evolution of the Universe
422(28)
16.1 Hubble's Law Implies a Hot, Dense Beginning
424(4)
Working it Out 16.1 Expansion and the Age of the Universe
425(3)
16.2 The Cosmic Microwave Background Confirms the Big Bang
428(4)
16.3 The Expansion of the Universe Is Speeding Up
432(3)
16.4 The Earliest Moments of the Universe Connect the Very Largest Size Scales to the Very Smallest
435(5)
16.5 Inflation Solves Several Problems in Cosmology
440(2)
16.6 Other Universes?
442(8)
Reading Astronomy News: "Gravity May Have Chased Light in the Early Universe"
444(1)
Summary
445(1)
Questions and Problems
445(3)
Exploration: Hubble's Law for Balloons
448(2)
17 Formation of Structure
450(24)
17.1 Galaxies Form Groups, Clusters, and Larger Structures
452(3)
Working it Out 17.1 Mass of a Cluster of Galaxies
455(1)
17.2 Gravity Forms Large-Scale Structure
455(5)
17.3 The First Stars and Galaxies Form
460(3)
17.4 Galaxies Evolve
463(4)
17.5 Astronomers Think about the Far Future
467(7)
Reading Astronomy News: "Massive Black Holes Sidle Up to Other Galaxies"
469(1)
Summary
470(1)
Questions and Problems
470(3)
Exploration: The Story of a Proton
473(1)
18 Life in the Universe
474(2)
18.1 Life on Earth Began Early and Evolved over Time
476(7)
Working it Out 18.1 Exponential Growth
482(1)
18.2 Life beyond Earth Is Possible
483(7)
18.3 Scientists Search for Signs of Intelligent Life
490(4)
18.4 The Fate of Life on Earth
494(2)
Reading Astronomy News: "Scientists Find Signs That Saturn's Moon Enceladus Might Be Hospitable to Life"
496(2)
Summary
498(1)
Questions and Problems
498(3)
Exploration: Fermi Problems and the Drake Equation
501
Appendix 1 Periodic Table of the Elements 1(1)
Appendix 2 Properties of Planets, Dwarf Planets, and Moons 2(3)
Appendix 3 Nearest and Brightest Stars 5(2)
Appendix 4 Star Maps 7
Glossary 1(1)
Selected Answers 1(1)
Credits 1(1)
Index 1
Stacy Palen is an award-winning professor in the physics department at Weber State University. She received her BS in physics from Rutgers University and her PhD in physics from the University of Iowa. As a lecturer and postdoc at the University of Washington, she taught Introductory Astronomy more than 20 times over 4 years. Since joining Weber State, she has been very active in science outreach activities ranging from star parties to running the state Science Olympiad. Stacy does research in formal and informal astronomy education and the death of Sun-like stars. She spends much of her time thinking, teaching, and writing about the applications of science in everyday life. She then puts that science to use on her small farm in Ogden, Utah. Laura Kay is Ann Whitney Olin professor and Chair of the Department of Physics and Astronomy at Barnard College, where she has taught since 1991. She received a BS degree in physics and an AB degree in feminist studies from Stanford University, and MS and PhD degrees in astronomy and astrophysics from the University of CaliforniaSanta Cruz. As a graduate student she spent 13 months at the Amundsen Scott station at the South Pole in Antarctica, and has had fellowships in Chile and Brazil. She studies active galactic nuclei using optical and X-ray telescopes. At Barnard she teaches courses on astronomy, astrobiology, women and science, and polar exploration. George Blumenthal is the director of the Center for Studies in Higher Education at the University of California, Berkeley. From 2006 to 2019 he was chancellor at the University of California, Santa Cruz. He joined the UC Santa Cruz faculty as a professor of astronomy and astrophysics in 1972. Chancellor Blumenthal received his BS degree from the University of WisconsinMilwaukee and his PhD in physics from the University of California, San Diego. As a theoretical astrophysicist, Blumenthal's research encompasses several broad areas, including the nature of the dark matter that constitutes most of the mass in the universe, the origin of galaxies and other large structures in the universe, the earliest moments in the universe, astrophysical radiation processes, and the structure of active galactic nuclei such as quasars.