1 / 19

Announcements

Announcements. Test solutions are posted Pick up graded work Homework 13 is due a week from today. A spreadsheet of the data is posted on the web. No class this Friday (Happy Thanksgiving) Project 2 is due a week from Friday, December 1 No planetarium shows or star party tonight

penningtonj
Download Presentation

Announcements

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. Announcements • Test solutions are posted • Pick up graded work • Homework 13 is due a week from today. A spreadsheet of the data is posted on the web. • No class this Friday (Happy Thanksgiving) • Project 2 is due a week from Friday, December 1 • No planetarium shows or star party tonight • If you filled out the survey for Brian Day, please leave it with me on your way out.

  2. Quasars and Active Galaxies 22 November 2006

  3. Today: • The discovery of quasars • What are quasars? • Alternative cosmologies

  4. Quasars: Quasi-stellar radio sources

  5. Quasars: Quasi-stellar radio sources

  6. Quasars become famous!

  7. Quasars live(d) at centers of galaxies 3C 273 and host galaxy Normal galaxy and “active” galaxy (false color)

  8. Virgo Cluster, M87 M87

  9. Clues to the nature of quasars • A quasar can be up to 1000 times brighter than its host galaxy. • Though quasars are rare today, they were relatively common in the past (several billion years ago). • Statistics indicate that quasars must shine for hundreds of millions of years. • Quasars vary in brightness over time periods as short as weeks; this implies that they are quite small.

  10. Where could all this energy come from? Motion (“kinetic”) Gravitational Elastic Thermal Chemical Nuclear Electrical Radiant (light)

  11. Where could all this energy come from? Motion (“kinetic”) Gravitational Elastic Thermal Chemical Nuclear Electrical Radiant (light)

  12. Theoretical Model of a Quasar Matter falls toward a black hole, gathers into a spinning disk of hot gas, converting gravitational energy to thermal energy. Just outside the horizon, pressures are so high that some material is forced out into a jet at near light speed.

  13. Testing the Theory

  14. Testing the Theory Stars near centers of all large galaxies (including our own) are orbiting VERY fast. Central masses vary from about 1 million to 1 billion solar masses.

  15. Why are quasars rare today? • Eventually they suck up all the nearby gas and run out of fuel. • Stars slightly farther out are in stable orbits; they rarely collide to send material toward the black hole. • But if another galaxy should happen to stray through, its material could reignite the quasar!

  16. Competing Cosmologies • “Big Bang”: 10 - 20 billion years ago the universe was much more dense than today (and therefore hot and unpleasant). • “Steady State”: As galaxies move apart from each other, new atoms are spontaneously created in empty space. These atoms coalesce to form new galaxies. The average density of the universe doesn’t change over time. There was no hot early universe.

  17. Competing Cosmologies • “Big Bang”: 10 - 20 billion years ago the universe was much more dense than today (and therefore hot and unpleasant). • “Steady State”: As galaxies move apart from each other, new atoms are spontaneously created in empty space. These atoms coalesce to form new galaxies. The average density of the universe doesn’t change over time. There was no hot early universe. Quasars were the first evidence that the universe was much different in the past than it is today.

  18. Hubble Deep Field

  19. Competing Cosmologies • Young universe: The “Hubble time” (since everything would have been in the same place, moving at current speeds) is only about 10 billion years. • Old universe: The “Hubble time” is about 20 billion years. Thanks to more accurate distance measurements, this dispute has been settled. The Hubble time is 13 - 14 billion years, in agreement with globular cluster ages.

More Related