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Understanding Our Universe (Fourth Edition)

✍ Scribed by Stacy Palen, George Blumenthal


Publisher
W. W. Norton & Company
Year
2021
Tongue
English
Leaves
1598
Edition
4
Category
Library

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✦ Synopsis


The most innovative resources for the most important course


Stacy Palen knows that introductory astronomy may be the only science course some students take in their college careers, so it’s their best chance to develop scientific literacy. Education research shows that the best way to attain scientific literacy is through active learning. Understanding Our Universe, Fourth Edition makes it easier for instructors to help students understand the concepts and learn to value science by providing activities that can be used before, during, and after class. By expanding her pedagogy to include What If scenarios and What an Astronomer Sees figure captions, Stacy helps students build scientific literacy and to think critically about science in the media. This purchase offers access to the digital ebook only.

✦ Table of Contents


Cover
Publisher’s Notice
Half-title Page
Title Page
Copyright
Dedication
Brief Table of Contents
Contents
AstroTours
Interactive Simulations
Astronomy in Action Videos
Preface
About the Authors
Half-title Page
1: Our Place in the Universe
1.1: Astronomy Creates a Universal Context
1.2: Science Is a Way of Viewing the World
1.3: Astronomers Use Mathematics to Find Patterns
Reading Astronomy News
Summary
Exploration: Scaling the Solar System
2: Patterns in the Sky—Motions of Earth and the Moon
2.1: Earth Spins on Its Axis
2.2: Revolution around the Sun Leads to Changes during the Year
2.3: The Moon’s Appearance Changes As It Orbits Earth
2.4: Shadows Cause Eclipses
Reading Astronomy News
Summary
Exploration: Phases of the Moon
3: Laws of Motion
3.1: Astronomers Have Studied the Motions of the Planets since Ancient Times
3.2: Galileo Was the First Modern Scientist
3.3: Newton’s Laws Govern Motion
3.4: Gravity Is a Force between Any Two Massive Objects
3.5: Orbits Are One Body “Falling around” Another
Reading Astronomy News
Summary
Exploration: Newtonian Orbits
4: Light and Telescopes
4.1: What Is Light?
4.2: Cameras and Spectrographs Record Astronomical Data
4.3: Telescopes Collect Light
Reading Astronomy News
Summary
Exploration: Light as a Wave
5: The Formation of Stars and Planets
5.1: Molecular Clouds Are the Cradles of Star Formation
5.2: The Protostar Becomes a Star
5.3: Planets Form in a Disk around the Protostar
5.4: The Inner and Outer Disk Have Different Compositions
5.5: A Case Study: The Solar System
5.6: Planetary Systems Are Common
Reading Astronomy News
Summary
Exploration: Exploring Exoplanets
6: Terrestrial Worlds in the Inner Solar System
6.1: Impacts Help Shape the Terrestrial Planets
6.2: The Surfaces of Terrestrial Planets Are Affected by Processes in the Interior
6.3: Planetary Surfaces Evolve through Tectonism
6.4: Volcanism Reveals a Geologically Active Planet
6.5: Wind and Water Modify Surfaces
Reading Astronomy News
Summary
Exploration: Earth’s Tides
7: Atmospheres of Venus, Earth, and Mars
7.1: Atmospheres Change over Time
7.2: Secondary Atmospheres Evolve
7.3: Earth’s Atmosphere Has Detailed Structure
7.4: The Atmospheres of Venus and Mars Differ from Earth’s
7.5: Earth’s Climate Is Changing
Reading Astronomy News
Summary
Exploration: Climate Change
8: The Giant Planets
8.1: Giant Planets Are Large, Cold, and Massive
8.2: The Giant Planets Have Clouds and Weather
8.3: The Interiors of the Giant Planets Are Hot and Dense
8.4: The Giant Planets Are Magnetic Powerhouses
8.5: Rings Surround the Giant Planets
Reading Astronomy News
Summary
Exploration: Estimating Rotation Periods of Giant Planets
9: Small Bodies of the Solar System
9.1: Dwarf Planets May Outnumber Planets
9.2: Moons as Small Worlds
9.3: Asteroids Are Pieces of the Past
9.4: Comets Are Clumps of Ice
9.5: Comet and Asteroid Collisions Still Happen Today
9.6: Meteorites Are Remnants of the Early Solar System
Reading Astronomy News
Summary
Exploration: Comparative Dwarf Planetology
10: Measuring the Stars
10.1: The Luminosity of a Star Can Be Found from Its Brightness and Distance
10.2: Radiation Tells Us the Temperature, Size, and Composition of Stars
10.3: The Mass of a Star Can Be Determined in Some Binary Systems
10.4: The Hertzsprung-Russell Diagram Is the Key to Understanding Stars
Reading Astronomy News
Summary
Exploration: The Hertzsprung-Russell Diagram
11: Our Star: The Sun
11.1: The Structure of the Sun Is a Matter of Balance
11.2: Energy in the Sun’s Core Moves through Radiation and Convection
11.3: The Atmosphere of the Sun
11.4: The Atmosphere of the Sun Is Very Active
Reading Astronomy News
Summary
Exploration: The Proton-Proton Chain
12: Evolution of Low-Mass Stars
12.1: The Life of a Main-Sequence Star Follows a Predictable Path
12.2: A Star Runs Out of Hydrogen and Leaves the Main Sequence
12.3: Helium Begins to Burn in the Degenerate Core
12.4: The Low-Mass Star Enters the Last Stages of Its Evolution
12.5: Binary Stars Sometimes Share Mass, Resulting in Novae and Supernovae
12.6: Star Clusters Are Snapshots of Stellar Evolution
Reading Astronomy News
Summary
Exploration: Evolution of Low-Mass Stars
13: Evolution of High-Mass Stars
13.1: High-Mass Stars Follow Their Own Path
13.2: High-Mass Stars Go Out with a Bang
13.3: Supernovae Change the Galaxy
13.4: Einstein Moved beyond Newtonian Physics
13.5: Gravity Is a Distortion of Spacetime
13.6: Black Holes Are a Natural Limit
Reading Astronomy News
Summary
Exploration: The CNO Cycle
14: Measuring Galaxies
14.1: Galaxies Come in Many Sizes and Shapes
14.2: There Are Many Ways to Measure Astronomical Distances
14.3: We Live in an Expanding Universe
14.4: A Supermassive Black Hole Exists at the Heart of Most Galaxies
Reading Astronomy News
Summary
Exploration: Galaxy Classification
15: Dark Matter and the Milky Way
15.1: Galaxies Are Mostly Dark Matter
15.2: Stars Form in the Spiral Arms of a Galaxy’s Disk
15.3: Components of the Milky Way Reveal Its Evolution
15.4: The Milky Way Offers Clues about How Galaxies Form
Reading Astronomy News
Summary
Exploration: Dark Matter in a Galaxy
16: The Evolution of the Universe
16.1: Hubble’s Law Implies a Hot, Dense Beginning
16.2: The Cosmic Microwave Background Confirms the Big Bang
16.3: The Expansion of the Universe Is Speeding Up
16.4: The Earliest Moments of the Universe Connect the Very Largest Size Scales to the Very Smallest
16.5: Inflation Solves Several Problems in Cosmology
16.6: Are There Other Universes?
Reading Astronomy News
Summary
Exploration: Hubble’s Law for Balloons
17: Formation of Structure
17.1: Galaxies Form Groups, Clusters, and Larger Structures
17.2: Gravity Drives the Formation of Large-Scale Structure
17.3: The First Stars and Galaxies Form
17.4: Galaxies Evolve
17.5: Astronomers Think about the Far Future
Reading Astronomy News
Summary
Exploration: The Story of a Proton
18: Life in the Universe
18.1: Life on Earth Began Early and Evolved over Time
18.2: Life beyond Earth Is Possible
18.3: Scientists Search for Signs of Intelligent Life
18.4: The Fate of Life on Earth
Reading Astronomy News
Summary
Exploration: Fermi Problems and the Drake Equation
Appendix 1: Periodic Table of the Elements
Appendix 2: Properties of Planets, Dwarf Planets, and Moons
Appendix 3: Nearest and Brightest Stars
Appendix 4: Star Maps
Glossary
Selected Answers
Credits
Index


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