Ch15

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Ch15

  1. 1. Cosmology Chapter 15 Great Idea: The universe began billions of years ago in the big bang and it has been expanding ever since.
  2. 2. Chapter Outline <ul><li>Galaxies </li></ul><ul><li>The Redshift and Hubble’s Law </li></ul><ul><li>The Big Bang </li></ul><ul><li>The Evolution of the Universe </li></ul><ul><li>Dark Matter and Ripples at the Beginning of Time </li></ul><ul><li>The End of the Universe </li></ul>
  3. 3. Galaxies
  4. 4. The Nebula Debate <ul><li>Nebulae </li></ul><ul><ul><li>Cloud-like objects </li></ul></ul><ul><li>Shapley vs. Curtis </li></ul><ul><ul><li>Debate over distance of nebulae </li></ul></ul>
  5. 5. Edwin Hubble and the Discovery of Galaxies <ul><li>Hubble </li></ul><ul><ul><li>Largest telescope </li></ul></ul><ul><ul><li>Used Cepheid variable stars to measure distance to nebula </li></ul></ul><ul><li>Galaxies </li></ul><ul><ul><li>Hubble discovered universe is billions of galaxies </li></ul></ul><ul><li>Cosmology </li></ul>
  6. 6. Edwin Hubble
  7. 7. Kinds of Galaxies <ul><li>Spiral </li></ul><ul><li>Elliptical </li></ul><ul><li>Irregular and dwarf </li></ul><ul><li>Active galaxies </li></ul><ul><ul><li>Quasars </li></ul></ul>
  8. 8. A Map of the Milky Way
  9. 9. A Typical Spiral Galaxy
  10. 10. A Typical Elliptical Galaxy
  11. 11. Deep-Field Image of Galaxies
  12. 12. The Redshift and Hubble’s Law
  13. 13. The Redshift and Hubble’s Law <ul><li>Redshift </li></ul><ul><li>Hubble’s Law </li></ul><ul><ul><li>The more distant a galaxy, the faster it recedes </li></ul></ul><ul><ul><li>V = H x d </li></ul></ul>
  14. 14. Photographs of Galaxies and Their Spectra
  15. 15. Illustration of Hubble Expansion
  16. 16. Science by the Numbers <ul><li>Analyzing Hubble data </li></ul>
  17. 17. Distance versus Velocity Relationship
  18. 18. The Big Bang
  19. 19. The Big Bang <ul><li>Big Bang </li></ul><ul><ul><li>The universe began at a specific time in the past, and it has been expanding ever since </li></ul></ul>
  20. 20. The Large-Scale Structure of the Universe <ul><li>The Local Group </li></ul><ul><ul><li>Milky Way, Andromeda Galaxy, and others </li></ul></ul><ul><li>Groups, clusters, superclusters </li></ul><ul><li>Voids </li></ul>
  21. 21. Distribution of Galaxies in Space
  22. 22. Apache Point Observatory – New Mexico, U.S.
  23. 23. Useful Analogies <ul><li>Raisin-Bread Dough Analogy </li></ul>Expanding Balloon Analogy
  24. 24. Evidence for the Big Bang <ul><li>The universal expansion </li></ul><ul><ul><li>Steady-state universe </li></ul></ul><ul><li>The cosmic microwave background </li></ul><ul><ul><li>Penzias and Wilson </li></ul></ul><ul><ul><ul><li>End of steady-state theory </li></ul></ul></ul><ul><li>The abundance of light elements </li></ul><ul><ul><li>Hydrogen, helium, and lithium </li></ul></ul>
  25. 25. Cosmic Background Explorer
  26. 26. Map of Microwave Radiation
  27. 27. The Evolution of the Universe
  28. 28. Some General Characteristics of an Expanding Universe <ul><li>All matter heats when compressed </li></ul><ul><ul><li>Hot big bang </li></ul></ul><ul><li>Freezings </li></ul><ul><ul><li>Changes in universe </li></ul></ul>
  29. 29. The Sequence of “Freezings”
  30. 30. 10 –43 Second: The Freezing of All Forces <ul><li>Two fundamental forces </li></ul><ul><ul><li>Gravity </li></ul></ul><ul><ul><li>Strong-electroweak force </li></ul></ul><ul><li>Limit of our knowledge of universe </li></ul>
  31. 31. 10 –35 Second: The Freezing of the Electroweak and Strong Forces <ul><li>Three fundamental forces </li></ul><ul><li>The elimination of antimatter </li></ul><ul><ul><li>Galaxy is ordinary matter </li></ul></ul><ul><ul><li>Why? </li></ul></ul><ul><ul><ul><li>Leftover protons </li></ul></ul></ul><ul><li>Inflation </li></ul><ul><ul><li>Short rapid expansion </li></ul></ul><ul><ul><ul><li>Common temperature </li></ul></ul></ul>
  32. 32. Evolution of the Universe through the Succession of Freezings
  33. 33. 10 –10 Second: The Freezing of the Weak and Electromagnetic Forces <ul><li>Four fundamental forces </li></ul><ul><li>Particle accelerators </li></ul><ul><ul><li>Reproduce from here forward </li></ul></ul><ul><ul><li>Experimental evidence for evolution of universe </li></ul></ul>
  34. 34. 10 –5 Second: The Freezing of Elementary Particles <ul><li>Elementary particles formed </li></ul><ul><li>Prior </li></ul><ul><ul><li>Quarks and leptons </li></ul></ul><ul><li>After </li></ul><ul><ul><li>Hadrons and leptons </li></ul></ul><ul><ul><ul><li>Electrons, protons and neutrons </li></ul></ul></ul>
  35. 35. Three Minutes: The Freezing of Nuclei <ul><li>Nuclei become stable </li></ul><ul><li>Only nuclei of H, He and Li </li></ul><ul><li>Plasma </li></ul>
  36. 36. Before One Million Years: The Freezing of Atoms <ul><li>Formation of atoms </li></ul><ul><li>Radiation released </li></ul><ul><ul><li>Cosmic microwave background </li></ul></ul><ul><li>Galaxy problem </li></ul>
  37. 37. Dark Matter and Ripples at the Beginning of Time <ul><li>Dark Matter </li></ul><ul><ul><li>Measure gravitational effects </li></ul></ul><ul><li>Hydrogen atoms </li></ul><ul><li>Formation of dark matter (questions to be answered) </li></ul><ul><ul><li>Before atoms formed? </li></ul></ul><ul><ul><li>Formed clumps? </li></ul></ul><ul><li>Ripples at the beginning of time </li></ul><ul><ul><li>Collection of luminous matter </li></ul></ul>
  38. 38. Discovery of Dark Matter
  39. 39. The End of the Universe <ul><li>Open, closed or flat universe </li></ul><ul><li>Current data </li></ul><ul><ul><li>Mass of universe </li></ul></ul><ul><ul><ul><li>Open universe </li></ul></ul></ul><ul><ul><li>Type Ia supernova </li></ul></ul><ul><li>Dark Energy </li></ul><ul><ul><li>74% of universe’s mass </li></ul></ul>
  40. 40. Dark Energy
  41. 41. Future <ul><li>Depends on dark energy </li></ul><ul><li>“ Big Rip” </li></ul>

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