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Summary
Summary
Discover the undiscovered with this jargon-free introduction to astrophysics
Astronomy is the study of what you see in the sky. Physics is the study of how things work. Astrophysics is the study of how things in the sky work, from large objects to tiny particles. Astrophysics For Dummies breaks it all down for you, making this difficult but fascinating topic accessible to anyone. Tracking the topics covered in a typical undergraduate astrophysics class, this book will teach you the essential pieces to understanding our universe. Get ready to launch into outer space with this ever-changing branch of science.
Discover the latest advances in the world of astrophysics Understand how and why galaxies form and evolve Find out the origins of cosmic rays Get a standalone primer on the science or supplement your astrophysics courseStudents in introductory astrophysics courses and would-be astronomy buffs who want to better understand the mechanics of the universe will love Astrophysics For Dummies .
Author Notes
Cynthia Phillips, PhD, is a scientist at the NASA Jet Propulsion Laboratory. Previously, she worked at the SETI Institute for 15 years.
Table of Contents
Introduction | 1 |
About This Book | 2 |
Foolish Assumptions | 3 |
Icons Used in This Book | 3 |
Beyond the Book | 4 |
Where to Go from Here | 4 |
Part 1 Getting Started with Astrophysics | 7 |
Chapter 1 Welcome to the Universe | 9 |
The Science of Astrophysics | 10 |
The start of astronomy | 10 |
A beautiful connection: Physics, astronomy, and astrophysics | 11 |
Let there be light! The electromagnetic spectrum | 11 |
Making waves | 13 |
Tools of the Trade | 15 |
The nitty-gritty of telescopes and astronomical instruments | 15 |
Viewing from above: Space-based telescopes | 17 |
Stars, Galaxies, and Their Cosmological Friends | 18 |
Chapter 2 The A to Z of Physics | 21 |
Building Blocks of the Universe: Particles | 22 |
The big three: Protons, neutrons, and electrons | 22 |
Elements and molecules | 24 |
(It's) elementary, particles | 26 |
Light it up with photons | 26 |
What Matters About Matter? | 27 |
The water we drink and the air we breathe, or elements and molecules | 28 |
It's all a state of mind with states of matter | 29 |
But sometimes it just doesn't (anti) matter | 30 |
Let the Force(s) Be With You | 30 |
Getting heavy with gravity | 31 |
Thank Maxwell for the electromagnetic force | 33 |
Strong and weak nuclear forces | 34 |
Store It or Use it, But Don't Waste Energy | 35 |
Fall faster into kinetic and potential energy | 35 |
Transferring thermal energy with conduction, convection, and radiation | 36 |
More than the eye can see: The electromagnetic spectrum | 37 |
Light's unending flexibility as both wave and particle | 37 |
It's the Law! (of Physics) | 38 |
Newton's laws of motion | 39 |
Step it up with velocity, acceleration, and momentum | 40 |
Having a conversation about conservation | 40 |
Einstein and the mass energy equivalence | 42 |
Heat and Energy Unite with Thermodynamics and Statistical Mechanics | 42 |
Learn the laws of thermodynamics | 43 |
Truly being one with the environment: Blackbody radiation | 45 |
Electromagnetic waves do the heavy lifting with radiative transfer | 46 |
When the details matter, zoom in to quantum mechanics | 47 |
Chapter 3 Astronomy in a Nutshell | 49 |
Where to Begin … Or, How It All Began | 50 |
Mapping our Solar System, Galaxy, and the Universe | 53 |
A question of scale | 53 |
A planetary survey | 55 |
Experience nature's light show with meteors, asteroids, and comets | 58 |
Galaxies and beyond | 58 |
Observational Astronomy: What are Those Dots in the Sky? | 59 |
Constellations: Mapping the stars | 60 |
The ecliptic, a year-long journey of the Sun | 61 |
How astronomical objects are named | 62 |
Chapter 4 Bridging the Gap Between Astronomy and Physics | 65 |
More Than the Sum of Its Parts: The Unique Study of Astrophysics | 66 |
One shift, two shift, redshift, blueshift | 67 |
Don't be late to the party when time matters | 68 |
Celestial mechanics and orbits | 70 |
Diving into the Details of Astrophysics | 72 |
Theoretical astrophysics | 72 |
Observational astrophysics | 72 |
Laboratory astrophysics | 72 |
High-energy astrophysics | 73 |
Running the gamut of the universe with cosmology | 73 |
The Nitty-Gritty of Telescopes and Astronomical Instruments | 73 |
Optical telescopes | 74 |
The night life at optical observatories | 76 |
Other types of telescopes | 76 |
Viewing from above; Space-based telescopes | 78 |
The Sun, the Star of Our Solar System | 79 |
Solar flares, solar wind, and other solar activity | 80 |
Hot or cold? The ins and outs of weather in space | 81 |
Studying the Sun | 82 |
Eclipses, or Throwing Shade in a Scientific Way | 83 |
Red Moon: Lunar eclipses | 83 |
Don't look! Solar eclipses | 85 |
Science of eclipses | 88 |
Part 2 When You Wish Upon A | 89 |
Chapter 5 Star Power: Hydrogen, Helium with a Twist of Nuclear Fusion | 91 |
Happy Birthday! A Star Is Born | 92 |
How do we define stars? | 92 |
Two is better than one: Fusion | 92 |
Protostars, star formation regions, and accretion disks | 95 |
Getting to Know Your Stars: Properties, Types, and Characteristics | 98 |
Don't rely on wishing: Understand the brightness, mass, and more about stars | 98 |
Plotting magnitude with the Hertzsprung-Russell diagram | 100 |
Dwarfs and giants | 102 |
The only constant is change with variable stars | 103 |
All Good Things Must Come to an End | 104 |
From flare ups to full-blown explosions: Novae and supernovae | 105 |
Nucleosynthesis and the creation of new elements | 106 |
The life cycle of a star: Heating, cooling, and everything in between | 107 |
Star reincarnation and the next phase of stellar existence | 109 |
Chapter 6 Friends for Life: Star Systems and Dust Clouds | 111 |
The More the Merrier: Binary and Multiple Star Systems | 112 |
The ties that bind: What it means to be gravitationally bound | 112 |
Orbits and the science behind them | 114 |
Formation and evolution of multiple star systems | 114 |
Step into the light; Eclipses in a double star system | 116 |
Binary star orbits and radial velocity | 118 |
Three's not a crowd: Multi-star systems | 119 |
Huddle Up There, Star Clusters | 121 |
Getting sticky with cluster formation | 121 |
Shut the door! Learn about open clusters | 121 |
Get even stickier with globular clusters | 122 |
Pedal to the Metal with Interstellar Gas and Dust | 123 |
The Interstellar medium | 123 |
Dreaming with your head in the (molecular) clouds | 124 |
IR spectroscopy and laboratory astrophysics | 124 |
Adding Structure to That Gas and Dust: Nebulae | 125 |
Diffuse and dark nebulae | 126 |
Who made who? Planetary nebulae and supernova remnants | 127 |
Chapter 7 Exoplanets: The Search for Earth 2.0 | 129 |
Beyond beyond Earth | 130 |
Exoplanets explained | 131 |
Key to understanding planet formation | 132 |
Exoplanets Come in Many Shapes and Sizes | 132 |
Exoplanet properties (mileage may vary) | 133 |
What's in a name? | 134 |
(Non) Flaming giant balls of gas and Neptunian exoplanets | 134 |
They really are super! Super-Earth exoplanets | 135 |
Look no further than Mother Earth for terrestrial exoplanets | 135 |
Looking Under (or Around) Hidden Rocks: Exoplanet Detection | 136 |
Observational techniques and biases | 137 |
Finding the distance between two points with radial velocity | 137 |
Transiting, TTV, and gravitational lensing | 138 |
Ignore the garbage, but know your debris disk | 140 |
Take a picture! The future of exoplanet detection | 140 |
The Nitty-Gritty of Exoplanet Formation | 141 |
Planetary birthrights: Protoplanetary disks | 142 |
Get moving! The dynamics of exoplanet systems | 143 |
What the Hail … Exoplanet Atmospheres | 145 |
Can Life Be Found on Exoplanets? | 146 |
Goldilocks had it right: The "habitable zone," or conditions for life as we know it | 147 |
Twinning: Why haven't we found Earth 2.0? | 148 |
Smells like life: Searching for biosignatures in exoplanet atmospheres | 150 |
The Drake Equation and the search for intelligent life | 150 |
Chapter 8 White Dwarfs, Black Holes, and Neutrinos, Oh My! | 153 |
Snow White and the Seven | 154 |
Pure as the driven snow, but without the snow: White dwarfs | 155 |
So cool and red hot: Red dwarfs | 156 |
Giant stars | 157 |
Evolved Giant Stars | 158 |
There Is No Escape: Black Holes | 158 |
What goes in never comes out: How black holes work | 159 |
The event horizon: The line light cannot cross | 160 |
Seeing the invisible, or the art of detecting black holes | 161 |
Surf's Up! Gravitational Waves | 163 |
A ripple in space-time | 163 |
How to be a wave detective | 164 |
Neutron Stars, or Total Core Collapse | 164 |
Science of the collapse of stars | 165 |
Pulsing radiation from pulsars | 165 |
Quasars, Bursters, and Blazars | 166 |
The XYZ of AGN: Quasars | 167 |
Blazars keep black holes in business | 168 |
Explosions from afar: Burst it out | 169 |
Part 3 Galaxies: Teamwork Makes the Dream Work | 171 |
Chapter 9 From Fuzzy Blobs to Majestic Spirals: The Milky Way and Other Galaxies | 173 |
Where in the World Are We? | 174 |
Galaxy quest | 175 |
Traveling the Milky Way | 175 |
Unraveling the Mystery | 177 |
Galaxies and other fuzzy objects get messier | 177 |
Hubble's puzzle | 178 |
Standard candles and redshifts | 178 |
Galaxy Classification | 181 |
Stars and gas with uncommon beauty: Spiral galaxies | 182 |
Never lose foci: Elliptical galaxies | 184 |
Lenticular galaxies are shaped like … guess what? | 185 |
Last night's leftovers on a universal scale: Irregular galaxies | 187 |
Chapter 10 Quantifying the Unknown, or How Galaxies Work | 189 |
Galaxy Formation Helps Unravel the Cosmos | 190 |
Source matter: No EM radiation for you! | 190 |
The trinity: Gravity dominance, instability, collapse | 191 |
Final push: Gravitational torque with a side of angular momentum | 192 |
Mechanics of a Star System | 193 |
Galactic Structure | 194 |
An inventory of the parts | 196 |
Stellar content of galaxies | 197 |
Excuse you! Emissions of active and inactive galaxies | 199 |
Both large and active: Seyfert and radio galaxies | 199 |
Black Holes and Their Role in Galaxies | 201 |
Black holes, the doughnut holes of the galaxy | 201 |
Dynamics and observation | 203 |
The Hubble Deep Field | 204 |
Chapter 11 Bigger Than Huge: Galaxy Clusters | 207 |
Making Friends: The Basics of Galaxy Clusters | 203 |
The ins and outs of a galaxy cluster | 209 |
Mass estimation: Virial, Sunyaev-Zel'dovich, and more | 210 |
Galaxy distribution throughout space | 212 |
A Galaxy Cluster of Our Very Own: The Local Group | 213 |
Location, location, location | 213 |
Constituent galaxies | 214 |
Galaxy Cluster Structure and Formation | 215 |
The ever-important role of gravity | 216 |
X-rays and the ICM (Intracluster medium) | 216 |
Physics of Galaxy Clusters | 218 |
The unique interactions of dark matter with baryons | 219 |
Shake it up: Gravitational perturbations and shock waves | 220 |
Always under pressure: Radiative gas physics | 221 |
Galaxy and cluster mergers | 222 |
An involuntary story of acquisition: LMC and SMC | 223 |
Prediction via computer modeling | 224 |
Galaxy cluster collisions | 225 |
What Galaxy Clusters Tell You About the Universe | 226 |
Bigger may be better | 226 |
Chemical emissions as prognosticators | 227 |
Change is hard: Slow rates of change in galaxy clusters | 228 |
Chapter 12 Weird and Wacky Galactic Phenomena | 231 |
Not Quite Dinosaurs: Galactic Archaeology | 232 |
What little stars are made of | 233 |
Stellar ages and astroseismology | 233 |
Tracing galactic mergers | 234 |
High Energy Astrophysics | 235 |
Triple E: Extreme energetic events | 236 |
How do we know? ALMA, Hubble, JWST, Chandra, and others | 237 |
Prime examples: Active galactic nuclei, gamma-ray bursts, supernovae | 239 |
Gravitational Lensing | 240 |
The bending of light | 241 |
Strong, weak, and microlensing | 244 |
Heading Down the Wormhole | 245 |
A wormhole by any other name … Einstein-Rosen bridges | 246 |
Making connections between wormholes and string theory | 247 |
Part 4 Cosmology: The Beginning and the End of Everything | 249 |
Chapter 13 The Big Bang: How It All Began | 251 |
What's the Point? A Primer on Cosmology | 252 |
Let's get right to it: The Big Bang | 252 |
Expansion of space, not your grocery bill: Cosmic inflation | 254 |
Creation of fundamental particles | 254 |
Too early to shine or twinkle | 255 |
Scientific Evidence: Why Do We Think There Was a Big Bang? | 255 |
Hubble's Law and the expansion of the universe | 256 |
Not for popcorn: Cosmic microwave background radiation | 257 |
The Big Bang Nucleosynthesis (BBN) era | 258 |
Disproving the steady-state mode! | 259 |
Making Sense of the Unimaginable with the Theory of Inflation | 260 |
The flatness problem | 260 |
CMB and uniform temperature | 261 |
Where galaxy clusters fit in | 262 |
Radiation Dominance in the Radiation Era | 262 |
Nothing Matters More Than Matter in the Matter Era | 266 |
Metric Expansion of Space: The Cosmological Principle | 268 |
We're really not all that special: The Copernican Principle | 269 |
Multi-directional spreading with Hubble universal expansion | 269 |
Big Bang radiation and temperature fluctuation | 270 |
Constant expansion, but of an inconsistent rate | 271 |
The future of direct measurement | 272 |
Chapter 14 First Light in the Universe, or How a Star is Born | 273 |
The Cosmic Dark Age | 274 |
The Big Bang cooled the heat | 274 |
Formation of neutral hydrogen atoms and cosmic background radiation | 275 |
A ripple in the universe led to galaxies | 276 |
End of an era: The cosmic dawn | 276 |
Early Star Formation | 277 |
Origins in primordial gas | 277 |
Nuclear fusion to the rescue | 278 |
Star Classification; Population III | 278 |
No room for diets: Very early stars = massive, low metal content | 279 |
Supernova explosions created heavier elements | 280 |
More metal: Next-gen stars had carbon, oxygen, iron, and heavier elements | 281 |
Star Classification: Population II and I | 281 |
Population II: Oldest observed stars formed 1 to 15 billion years ago | 282 |
Population I: Young stars formed 1 million to 10 billion years ago | 283 |
The Epoch of Reionization | 284 |
Energy bubbles and the leaching of ionized radiation | 285 |
Let there be light | 286 |
Formation of the First Galaxies | 287 |
Opposites (or not) attract! | 287 |
Continued evolution and creation of new galaxies | 288 |
Chapter 15 And Then St Gets Weirder: Dark Matter, Dark Energy, and Relativity | 289 |
General Facts about General Relativity | 290 |
Keeping it special | 290 |
Einstein's explanation of gravity's interaction with space-time | 291 |
Space-time curvature and total forces | 293 |
The three tests for general relativity | 294 |
Advancing Theories Require Advancing Models | 296 |
Holes and waves | 296 |
First general relativity models: A stable universe and its challengers | 297 |
Einstein's "greatest mistake" and its reinterpretation | 298 |
Galactic Glue: Dark Matter | 299 |
Detecting the darkness | 300 |
Don't be a WiMP(s): Weakly interacting massive particles | 302 |
Some like it hot, some like it cold | 302 |
Dark Energy in Review | 304 |
Why do we need dark energy? | 304 |
A story of accelerating expansion | 305 |
Where Did Dark Energy Come From? | 306 |
Origins of dark energy 1: Einstein (again!) and the Cosmoiogical Constant | 307 |
Origins of dark energy 2: Quantum theory | 308 |
Origins of dark energy 3: Quintessence | 308 |
Origins of dark energy 4: Tachyons moving faster than light | 309 |
Origins of dark energy 5: Questioning Einstein and gravity | 310 |
The standard of cosmology: The Lambda-Cold Dark Matter (ACDM) model | 310 |
Chapter 16 The End of It All | 313 |
No Refunds: What Happens When the Sun Explodes | 314 |
Running out of (hydrogen) gas | 314 |
Goodbye, life on Earth | 315 |
Omega Value of the Universe | 316 |
It's critical: The critical density parameter | 318 |
How do we calculate Omega? | 319 |
WMAP and Planck missions | 320 |
Future work on critical density | 321 |
The Big Freeze: An End of the Universe Theory | 323 |
The last stars burn out | 323 |
Over the horizon: Galaxies beyond view | 325 |
Such a degenerate era | 326 |
Heat death of the universe | 326 |
The Big Rip: Another End of the Universe Theory | 327 |
Dynamics: Dark energy changing over time | 328 |
Phantom dark energy | 328 |
The Big Crunch: Yet Another End of the Universe Theory | 329 |
Expanding, then shrinking | 329 |
Spoilers: Dark energy could get in the way | 330 |
Something Before Nothing: Did Anything Come before the Big Bang? | 331 |
Anthropic principle: Why do the laws of physics even allow matter and life? | 331 |
Before and after: The cyclic universe theory | 332 |
Now That We're at the End - How Will It End? | 333 |
Getting Higgy with it: Vacuum decay and the Higgs boson and field | 334 |
Future observations of cosmic microwave background radiation and dark energy | 335 |
Clues from JWST and the earliest galaxies | 336 |
Part 5 The Part of Tens | 337 |
Chapter 17 Ten Scientists Who Paved the Way for Astrophysics | 339 |
Albert Einstein: 1879-1955 | 339 |
Edwin Hubble: 1889-1953 | 340 |
Cecelia Payne-Gaposchkin: 1900-1979 | 340 |
Karl Jansky: 1905-1950 | 340 |
Subrahmanyan Chandrasekhar: 1910-1995 | 341 |
Vera Rubin: 1928-2016 | 341 |
Kip Thorne: 1940- | 342 |
Stephen Hawking: 1942-2018 | 342 |
Jocelyn Bell Bunnell: 1943 | 342 |
Alan Guth: 1947- | 343 |
Chapter 18 Ten Important Space Missions for Astrophysics | 345 |
Hubble Space Telescope (1990-present) | 345 |
James Webb Space Telescope (2021-present) | 346 |
Kepler and TESS (2009-2018 and 2018-present) | 347 |
SOFIA (2010-2022) | 348 |
Chandra X-Ray Observatory (1999-present) | 349 |
Spitzer Space Telescope (2003-2020) | 349 |
Compton Gamma-Ray Observatory (1991-2000) | 350 |
Fermi Gamma-Ray Space Telescope (2008-present) | 351 |
Herschet Space Observatory (2009-2013) | 351 |
Nancy Grace Roman Space Telescope (planned 2027 launch) | 352 |
Glossary | 353 |
Index | 359 |