
Nguồn ngoài
Big Ideas in Cosmology
The traditional textbook, bound to the physical limits of the printed page, cannot illustrate the full complexity, movement, and beauty of the cosmos.
- Tác giả
- Kim Coble, Kevin McLin, and Lynn Cominsky
- Nhà xuất bản
- San Francisco State University, Chico State University, and Sonoma State University
- Nguồn
- LibreTexts
- Giấy phép
- CC BY-NC-SA
- Ngôn ngữ
- EN
- Danh mục
- Khoa học cơ bản
Mục lục· 218 mục
- 01: Size and Scope
- 1.00: Size and Scope Introduction
- 1.01: Your Model of the Universe
- 1.02: Our Solar System
- 1.03: Our Galaxy - The Milky Way
- 1.04: Other Galaxies and Large-scale Structures in the Universe
- 1.05: The Smallest Stuff- Particles Atoms and Molecules
- 1.06: Hierarchy- How the Objects Are Arranged
- 1.07: Scale the Universe
- 1.08: Wrapping It Up 1 - Size Scope and Units
- 1.09: Mission Report for Wrapping It Up Activity 1 - Size Scope and Units
- 02: Light
- 2.00: Light Introduction
- 2.01: The Wave Nature of Light
- 2.02: The Particle Nature of Light
- 2.03: The Electromagnetic Spectrum
- 2.04: What a Spectrum of Light Can Tell Us About Matter
- 2.05: Continuous Spectra - a Planck Spectrum Tells us the Temperature of Objects
- 2.06: Lines Spectra- Emission and Absorption Lines
- 2.07: Determining the Composition of an Unknown Gas
- 2.08: Mission Report
- 2.09: Wrapping It Up
- 03: Telescopes
- 3.00: Telescope Introduction
- 3.01: Designing Telescopes Across the Spectrum
- 3.02: Location Location Location
- 3.03: Imaging Astronomical Objects
- 3.04: Determining the Brightness of Astronomical Objects
- 3.05: Wrapping It Up
- 3.06: Mission Report
- 04: Moving Through Space
- 4.00: Moving Through Space Introduction
- 4.01: Relationship Between Distance Speed and Time
- 4.02: Measuring Motion - the Doppler Shift
- 4.03: Astronomical Objects in Motion
- 4.04: Wrapping It Up
- 4.05: Mission Report
- 05: Moving Through Time
- 5.00: Moving Through Time Introduction
- 5.01: Measuring the Ages of Objects- Radiometric Dating
- 5.02: Measuring Ages - Lifetimes of Stars
- 5.03: Change Over Time- Evolution of Stars
- 5.04: Evolution of Galaxies and the Universe Itself
- 5.05: Wrapping It Up
- 5.06: Mission Report
- 06: Measuring Cosmic Distances
- 6.00: Measuring Cosmic Distances Introduction
- 6.01: Geometrical Methods
- 6.02: Standard Ruler
- 6.03: Standard Candle
- 6.04: The Cosmic Distance Ladder
- 6.05: Wrapping It Up
- 6.06: Mission Report
- 07: Classical Physics- Gravity and Energy
- 7.00: Classical Physics- Gravity and Energy Introduction
- 7.01: Gravity on Earth
- 7.02: Force Mass and Weight
- 7.03: Gravity Is a Universal Force
- 7.04: Gravity and Orbits
- 7.05: Forms of Energy
- 7.06: Conservation of Energy
- 7.07: Wrapping It Up
- 7.08: Mission Report
- 08: Dark Matter
- 8.00: Dark Matter Introduction
- 8.01: Making Models for Rotation
- 8.02: Velocities Mass and Gravity- the Solar System
- 8.03: Gravity and Models for Different Mass Distributions
- 8.04: Velocity and Mass Distributions in Galaxies
- 8.05: Velocity and Mass Distributions in Galaxy Clusters
- 8.06: Possible Explanations for the Missing Mass in Galaxies and Clusters
- 8.07: Wrapping It Up - What Is the Matter With NGC 3198
- 8.08: Mission Report - What Is the Matter With NGC 3198
- 09: Special Relativity
- 9.00: Special Relativity Introduction
- 9.01: The Principles of Special Relativity
- 9.02: Time Dilation
- 9.03: Length Contraction
- 9.04: The Geometry of Special Relativity- Spacetime
- 9.05: Applications of Spacetime
- 9.06: Mass and Energy
- 9.07: Faster Than Light
- 9.08: Wrapping It Up - A Trip to Alpha Centauri
- 9.09: Mission Report for Wrapping It Up Activity 9 - A Trip to Alpha Centauri
- 10: General Relativity
- 10.00: General Relativity Introduction
- 10.01: Einsteins Equivalence Principle
- 10.02: Gravity and Curvature
- 10.03: What is Curvature
- 10.04: Tests of General Relativity
- 10.05: The Source of Gravity
- 10.06: Wrapping It Up - Curved Spacetime Around Astronomical Objects
- 10.07: Curved Spacetime Around Astronomical Objects
- 10.08: FORMULAE CONSTANTS AND CONVERSION FACTORS
- 11: Black Holes
- 11.00: Black Holes Introduction
- 11.01: What Are Black Holes
- 11.02: Spacetime Near Black Holes
- 11.03: Quantum Effects Near Black Holes
- 11.04: Astrophysical Black Holes
- 11.05: Wrapping It Up - Black Hole Densities
- 11.06: Black Hole Densities
- 12: Gravitational Lenses
- 12.00: Gravitational Lensing Introduction
- 12.01: What Are Gravitational Lenses
- 12.02: Lensing by Point Masses
- 12.03: Lensing by Extended Mass Distributions
- 12.04: Weak Lensing
- 12.05: Wrapping It Up - Measuring Gravitational Lenses
- 12.06: Mission Report - Measuring Gravitational Lenses
- 13: The Expansion of the Universe
- 13.00: The Expansion of the Universe Introduction
- 13.01: Some History
- 13.02: The Hubble Law
- 13.03: The Universe Is Expanding
- 13.04: The Age of the Universe
- 13.05: The Basic Big Bang Model
- 13.06: Wrapping It - Up How Well Do We Know the Expansion Rate and Age of the Universe
- 13.07: How Well Do We Know the Expansion Rate and Age of the Universe
- 14: The Growth of Structure
- 14.00: The Growth of Structure Introduction
- 14.01: Large Scale Structure
- 14.02: The Formation of Galaxy Clusters and Groups
- 14.03: The Formation and Evolution of Galaxies
- 14.04: The First Stars
- 14.05: Wrapping It Up - Map the Universe
- 14.06: Mission Report - Map the Universe
- 15: The Cosmic Microwave Background
- 15.00: The Cosmic Microwave Background Introduction
- 15.01: Observations of the CMB Spectrum
- 15.02: Implications of the CMB Temperature and Spectrum
- 15.03: Observations of Variations in the CMB
- 15.04: Understanding the Variations in the CMB
- 15.05: Comparing Models and Data - The CMB and the Curvature of Space
- 15.06: Wrapping It Up - Using CMB Data to Determine Cosmological Parameters
- 15.07: Using CMB Data to Determine Cosmological Parameters
- 16: The Early Universe
- 16.00: The Early Universe Introduction
- 16.01: The Formation of the Lightest Elements
- 16.02: Particle Soup
- 16.03: Inflation
- 16.04: The Beginning
- 16.05: Wrapping It Up - Timeline of the Early Universe
- 16.06: Timeline of the Early Universe
- 17: Dark Energy and the Fate of the Universe
- 17.00: Dark Energy and the Fate of the Universe Introduction
- 17.01: Evidence for Dark Energy
- 17.02: Candidates for Dark Energy
- 17.03: The Friedmann Equation and the Fate of the Universe
- 17.04: Cosmic Concordance and Cosmological Parameters
- 17.05: Summary - You Will Reflect on What You Have Learned About Cosmology
- 17.06: Wrapping It Up - Cosmological Parameter Estimation
- 17.07: Cosmological Parameter Estimation
- Knowls
- 18: Big Ideas JS code
- 0.5: Meters To Kilometres
- 0.5: Sun Moon Distance
- 18.00: 15 4 how cosmological parameters affect the cmb cold dark matter
- 18.01: 15 4 how cosmological parameters affect the cmb regular matter
- 18.02: 16 2 4 particle creation timeline
- 18.03: bigIdeasActivityOne
- 18.04: ch16 particle classification
- 18.05: ch4pg1lightminute
- 18.06: ch4pg1lightyear
- 18.07: ch4pg1powersoftentimescales
- 18.08: ch4pg2boatwavedemobcmovingsource
- 18.09: 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