1 Introduction to Science and the Universe
9 The Universe of the Very Small
11 For Further Exploration: The Science and the Universe
13 The Sky Above
14 Ancient Astronomy
17 For Further Exploration: The Birth of Modern Astronomy
20 The Laws of Planetary Motion
21 Newton’s Great Synthesis
24 Motions of Satellites and Spacecraft
29 Earth and Sky
30 The Seasons
39 The Behavior of Light
40 The Electromagnetic Spectrum
41 Spectroscopy in Astronomy
42 The Structure of the Atom
49 Telescopes Today
51 Radio Telescopes
52 Observations outside Earth’s Atmosphere
54 For Further Exploration: Astronomical Instruments
57 Overview of Our Planetary System
61 For Further Exploration: Other Worlds: An Introduction to the Solar System
62 Exercises: Other Worlds: An Introduction to the Solar System
65 Earth’s Crust
66 Earth’s Atmosphere
69 For Further Exploration: Earth as a Planet
72 General Properties of the Moon
73 The Lunar Surface
82 The Massive Atmosphere of Venus
83 The Geology of Mars
84 Water and Life on Mars
89 Exploring the Outer Planets
90 The Giant Planets
95 Ring and Moon Systems Introduced
96 The Galilean Moons of Jupiter
98 Pluto and Charon
100 For Further Exploration: Rings, Moons, and Pluto
103 Asteroids
105 The “Long-Haired” Comets
108 Exercises: Comets and Asteroids: Debris of the Solar System
110 Meteors
112 Formation of the Solar System
118 The Structure and Composition of the Sun
120 Solar Activity above the Photosphere
122 For Further Exploration: The Sun: A Garden-Variety Star
123 Exercises: The Sun: A Garden-Variety Star
124 Introduction to the Sun: A Nuclear Powerhouse
126 Mass, Energy, and the Theory of Relativity
129 For Further Exploration: The Sun: A Nuclear Powerhouse
132 The Brightness of Stars
134 The Spectra of Stars (and Brown Dwarfs)
135 Using Spectra to Measure Stellar Radius, Composition, and Motion
139 A Stellar Census
144 Exercises: The Stars: A Celestial Census
153 The Interstellar Medium
158 Interstellar Matter around the Sun
163 The H–R Diagram and the Study of Stellar Evolution
172 Star Clusters
177 Exercises: Stars from Adolescence to Old Age
180 Evolution of Massive Stars: An Explosive Finish
185 For Further Exploration: The Death of Stars
186 Exercises: The Death of Stars
195 For Further Exploration: Black Holes and Curved Spacetime
196 Exercises: Black Holes and Curved Spacetime
198 The Architecture of the Galaxy
201 The Center of the Galaxy
209 Properties of Galaxies
210 The Extragalactic Distance Scale
212 For Further Exploration: Galaxies
213 Exercises: Galaxies
215 Quasars
216 Supermassive Black Holes: What Quasars Really Are
222 Galaxy Mergers and Active Galactic Nuclei
223 The Distribution of Galaxies in Space
226 For Further Exploration: The Evolution and Distribution of Galaxies
230 A Model of the Universe
236 For Further Exploration: The Big Bang
237 Exercises: The Big Bang
243 For Further Exploration: Life in the Universe
244 Exercises: Life in the Universe
247 Scientific Notation
257 Star Chart and Sky Event Resources
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124 Introduction to the Sun: A Nuclear Powerhouse
124 Introduction to the Sun: A Nuclear Powerhouse
The Sun puts out an incomprehensible amount of energy—so much that its ultraviolet radiation can cause sunburns from 93 million miles away. It is also very old. As you learned earlier, evidence shows that the Sun formed about 4.5 billion years ago and has been shining ever since. How can the Sun produce so much energy for so long?
The Sun’s energy output is about 4 × 1026 watts. This is unimaginably bright: brighter than a trillion cities together each with a trillion 100-watt light bulbs. Most known methods of generating energy fall far short of the capacity of the Sun. The total amount of energy produced over the entire life of the Sun is staggering, since the Sun has been shining for billions of years. Scientists were unable to explain the seemingly unlimited energy of stars like the Sun prior to the twentieth century.