Big Ideas in Cosmology
by Kim Coble, Kevin McLin, and Lynn Cominsky
The traditional textbook, bound to the physical limits of the printed page, cannot illustrate the full complexity, movement, and beauty of the cosmos.
Description from LibreTexts.
- Publisher
- San Francisco State University, Chico State University, and Sonoma State University
- Subjects
- Physics, Astronomy Cosmology
- Licence
- CC BY-NC-SA 4.0, as LibreTexts states it. Non-commercial use only.
- Who can read
- Tweens profiles and older, judged from its title and subjects
Contents
LibreTexts writes equations in TeX, and here they show as TeX; the PDF has them typeset.
- Front Matter
- TitlePage
- InfoPage
- Table of Contents
- About the Book
- Licensing
- About the Authors
- 0: Review of Mathematics
- 0.0: Scientific Notation
- 0.1: Manipulating Numbers in Scientific Notation
- 0.2: The Metric System
- 0.3: Special Units Used in Astronomy
- 0.4: Comparing Sizes and Converting Units
- 0.5: Problem Solving and Thinking About Your Answers
- 0.6: Measurement Accuracy and Uncertainty
- 0.7: Wrapping It Up
- 1: Size and Scope
- 1.0: Size and Scope Introduction
- 1.1: Your Model of the Universe
- 1.2: Our Solar System
- 1.3: Our Galaxy - The Milky Way
- 1.4: Other Galaxies and Large-scale Structures in the Universe
- 1.5: The Smallest Stuff- Particles, Atoms, and Molecules
- 1.6: Hierarchy- How the Objects Are Arranged
- 1.7: Scale the Universe
- 1.8: Wrapping It Up 1 - Size, Scope, and Units
- 1.9: Mission Report 1 - Size, Scope, and Units
- 2: Light
- 2.0: Light Introduction
- 2.1: The Wave Nature of Light
- 2.2: The Particle Nature of Light
- 2.3: The Electromagnetic Spectrum
- 2.4: What a Spectrum of Light Can Tell Us About Matter
- 2.5: Continuous Spectra - a Planck Spectrum Tells us the Temperature of Objects
- 2.6: Lines Spectra- Emission and Absorption Lines
- 2.7: Determining the Composition of an Unknown Gas
- 2.8: Wrapping It Up 2 - The Properties of Light
- 2.9: Mission Report 2 - The Properties of Light
- 3: Telescopes
- 3.0: Telescope Introduction
- 3.1: Designing Telescopes Across the Spectrum
- 3.2: Location, Location, Location
- 3.3: Imaging Astronomical Objects
- 3.4: Determining the Brightness of Astronomical Objects
- 3.5: Wrapping It Up 3 - Light, Telescopes, and Astronomical Images
- 3.6: Mission Report 3 - Light, Telescopes, and Astronomical Images
- 4: Moving Through Space
- 4.0: Moving Through Space Introduction
- 4.1: Relationship Between Distance, Speed, and Time
- 4.2: Measuring Motion - the Doppler Shift
- 4.3: Astronomical Objects in Motion
- 4.4: Wrapping It Up 4 - The Andromeda Shift
- 4.5: Mission Report 4 - The Andromeda Shift
- 5: Moving Through Time
- 5.0: Moving Through Time Introduction
- 5.1: Measuring the Ages of Objects - Radiometric Dating
- 5.2: Measuring Ages - Lifetimes of Stars
- 5.3: Change Over Time - Evolution of Stars
- 5.4: Evolution of Galaxies and the Universe Itself
- 5.5: Wrapping It Up 5 - Cosmic Timeline
- 5.6: Mission Report 5 - Cosmic Timeline
- 6: Measuring Cosmic Distances
- 6.0: Measuring Cosmic Distances Introduction
- 6.1: Geometrical Methods
- 6.2: Standard Ruler
- 6.3: Standard Candle
- 6.4: The Cosmic Distance Ladder
- 6.5: Wrapping It Up 6 - The Supernova of 1885
- 6.6: Mission Report 6 - Distance Measurement
- 7: Classical Physics- Gravity and Energy
- 7.0: Classical Physics - Gravity and Energy Introduction
- 7.1: Gravity on Earth
- 7.2: Force, Mass, and Weight
- 7.3: Gravity Is a Universal Force
- 7.4: Gravity and Orbits
- 7.5: Forms of Energy
- 7.6: Conservation of Energy
- 7.7: Wrapping It Up 7 - The Galilean Moons of Jupiter
- 7.8: Mission Report 7 - The Galilean Moons of Jupiter
- 8: Dark Matter
- 8.0: Dark Matter Introduction
- 8.1: Making Models for Rotation
- 8.2: Velocities, Mass, and Gravity - The Solar System
- 8.3: Gravity and Models for Different Mass Distributions
- 8.4: Velocity and Mass Distributions in Galaxies
- 8.5: Velocity and Mass Distributions in Galaxy Clusters
- 8.6: Possible Explanations for the Missing Mass in Galaxies and Clusters
- 8.7: Wrapping It Up 8 - What Is the Matter With NGC 3198?
- 8.8: Mission Report 8 - What Is the Matter With NGC 3198?
- 9: Special Relativity
- 9.0: Special Relativity Introduction
- 9.1: The Principles of Special Relativity
- 9.2: Time Dilation
- 9.3: Length Contraction
- 9.4: The Geometry of Special Relativity - Spacetime
- 9.5: Applications of Spacetime
- 9.6: Mass and Energy
- 9.7: Faster Than Light?
- 9.8: Wrapping It Up 9 - A Trip to Alpha Centauri
- 9.9: Mission Report 9 - A Trip to Alpha Centauri
- 10: General Relativity
- 10.0: General Relativity Introduction
- 10.1: Einstein’s Equivalence Principle
- 10.2: Gravity and Curvature
- 10.3: What is Curvature?
- 10.4: Tests of General Relativity
- 10.5: The Source of Gravity
- 10.6: Wrapping It Up 10 - Curved Spacetime Around Astronomical Objects
- 10.7: Mission Report 10: Curved Spacetime Around Astronomical Objects
- 10.8: Formulae, Constants, and Conversion Factors for Chapter 10
- 11: Black Holes
- 11.0: Black Holes Introduction
- 11.1: What Are Black Holes?
- 11.2: Spacetime Near Black Holes
- 11.3: Quantum Effects Near Black Holes
- 11.4: Astrophysical Black Holes
- 11.5: Wrapping It Up 11 - Black Hole Densities
- 11.6: Mission Report 11 - Black Hole Densities
- 12: Gravitational Lenses
- 12.0: Gravitational Lensing Introduction
- 12.1: What Are Gravitational Lenses?
- 12.2: Lensing by Point Masses
- 12.3: Lensing by Extended Mass Distributions
- 12.4: Weak Lensing
- 12.5: Wrapping It Up 12 - Measuring Gravitational Lenses
- 12.6: Mission Report 12 - Measuring Gravitational Lenses
- 13: The Expansion of the Universe
- 13.0: The Expansion of the Universe Introduction
- 13.1: Some History
- 13.2: The Hubble Law
- 13.3: The Universe is Expanding
- 13.4: The Age of the Universe
- 13.5: The Basic Big Bang Model
- 13.6: Wrapping It Up 13 - How Well Do We Know the Expansion Rate and Age of the Universe?
- 13.7: Mission Report 13 - How Well Do We Know the Expansion Rate and Age of the Universe?
- 14: The Growth of Structure
- 14.0: The Growth of Structure Introduction
- 14.1: Large Scale Structure
- 14.2: The Formation of Galaxy Clusters and Groups
- 14.3: The Formation and Evolution of Galaxies
- 14.4: The First Stars
- 14.5: Wrapping It Up 14 - Map the Universe
- 14.6: Mission Report 14 - Map the Universe
- 15: The Cosmic Microwave Background
- 15.0: The Cosmic Microwave Background Introduction
- 15.1: Observations of the CMB Spectrum
- 15.2: Implications of the CMB Temperature and Spectrum
- 15.3: Observations of Variations in the CMB
- 15.4: Understanding the Variations in the CMB
- 15.5: Comparing Models and Data - The CMB and the Curvature of Space
- 15.6: Wrapping It Up 15 - Using CMB Data to Determine Cosmological Parameters
- 15.7: Mission Report 15: Using CMB Data to Determine Cosmological Parameters
- 16: The Early Universe
- 16.0: The Early Universe Introduction
- 16.1: The Formation of the Lightest Elements
- 16.2: Particle Soup
- 16.3: Inflation
- 16.4: The Beginning
- 16.5: Wrapping It Up 16 - Timeline of the Early Universe
- 16.6: Mission Report 16 - Timeline of the Early Universe
- 17: Dark Energy and the Fate of the Universe
- 17.0: Dark Energy and the Fate of the Universe Introduction
- 17.1: Evidence for Dark Energy
- 17.2: Candidates for Dark Energy
- 17.3: The Friedmann Equation and the Fate of the Universe
- 17.4: Cosmic Concordance and Cosmological Parameters
- 17.5: Summary
- 17.6: Wrapping It Up 17 - Cosmological Parameter Estimation
- 17.7: Mission Report 17 - Cosmological Parameter Estimation
- Knowls
- 18: Big Ideas JS code
- 0.5: Meters To Kilometres
- 0.5: Sun Moon Distance
- 18.0: 15_4_how_cosmological_parameters_affect_the_cmb_cold_dark_matter
- 18.1: 15_4_how_cosmological_parameters_affect_the_cmb_regular_matter
- 18.2: 16_2_4_particle_creation_timeline
- 18.3: bigIdeasActivityOne
- 18.4: ch16_particle_classification
- 18.5: ch4pg1lightminute
- 18.6: ch4pg1lightyear
- 18.7: ch4pg1powersoftentimescales
- 18.8: ch4pg2boatwavedemobcmovingsource
- 18.9: ch4pg2boatwavedemosourceofwavesstationary
- 18.10: ch4pg2dopplershiftofhydrogen
- 18.11: ch4pg2quantitativedopplershift
- 18.12: ch4pg2twowaysofrepresentingaspectrum
- 18.13: ch4pg3relativemotion
- 18.14: ch4wiu4theandromedashift
- 18.15: ch6pg2standardruler
- 18.16: ch6pg3animatedfigure612
- 18.17: ch6pg3fluxvsdistance
- 18.18: ch6pg3mainsequencematchingforclustersofdifferentdistances
- 18.19: ch6pg3standardcandle
- 18.20: ch6pg3supernovaetypelaanddistances
- 18.21: ch6pg3tullyfisher
- 18.22: ch6pg4matchthetechniquetothedistance
- 18.23: ch7pg2accelerationandmass
- 18.24: ch7pg2netforceofanobject
- 18.25: ch7pg3animatedfigure75
- 18.26: ch7pg3howdoestheforceofgravitydependondistance
- 18.27: ch7pg3howdoestheforceofgravitydependonmass
- 18.28: ch7wiu7thegalileanmoonsofjupiter
- 18.29: chapter2pg1photonraceroundone
- 18.30: chapter2pg5planckspectrum
- 18.31: chapter2pg6viewingorientation
- 18.32: chapter2pg7determiningthecomposition
- 18.33: chapter3pt1lightcollectingarea
- 18.34: chapter3pt4afindingthesourceandsubtractingthebackground
- 18.35: chapter3pt4bcolorizingccdimages
- 18.36: chapter_11_2_falling_into_a_black_hole_tidalforces
- 18.37: chapter_11_2_time_dilation_spacetime_dialation
- 18.38: chapter_12_2_lensing_by_a_point_mass_gravitationallensing_simple
- 18.39: chapter_12_2_macho_light_curve
- 18.40: chapter_12_2_the_einstein_radius_einsteinring
- 18.41: chapter_12_3_different_types_of_lenses_glbinning
- 18.42: chap_2_1_wave_generator_NEW
- 18.43: comovingcoords
- 18.44: expandinguniverse1
- 18.45: explodinguniverse
- 18.46: explosionvsexpansiondensity
- 18.47: orbitsimulator
- 18.48: testjQueryUI
- 18.49: var1
- 18.50: wiu15_a_curvature
- 18.51: wiu15_b_amount_of_baryonic_matter
- 18.52: wiu15_c_amount_of_cold_dark_matter
- 18.53: wiu6thesupernovaof1885
- 18.54: wiu_12_1_determining_masses_of_lenses_grav_len_mass_measurement
- 18.55: wiu_12_1_determining_masses_of_lenses_mass_calculator
- 18.56: wiu_16_cosmic_timeline
- Kilometres To Miles
- Pop ups
- Math Exploration 13.1
- Math Exploration 13.2
- Back Matter
- Index
- Glossary
- Detailed Licensing
- Resources: Formulae, Constants, and Conversions