1. Where do we come from, where are we going?
The Big Bang
Where do we come from, where are we going?

2. Goals Where did the Universe come from? Where is it going?
How can we see the past?
How can we learn about the future from seeing the past?

3. Hubble’s Law Recall: All galaxies are moving away from us.
The farther away the faster they go.
V = Ho x D

4. Expanding Universe
If galaxies are all moving away, then at some point they were all much closer.
Hubble’s Law implies the Universe is expanding.

5. The Big Bang
Big Bang: the event from which the Universe began expanding.
Into what did the Universe expand?
Where was the Big Bang?
Where is the center of the Universe?

6. Age of the Universe
Since all galaxies are moving away from us, how long has it been since all galaxies were together?
time = distance / velocity
velocity = Ho x distance
time = distance / (Ho x distance)
time = 1/Ho
“An expanding universe does not preclude a creator, but it does place limits on when he might have carried out his job.”
-Steven Hawking, A Brief History of Time

7. Age Disagreements
Until recently, much disagreement on the value of Ho and therefore, the age of the Universe.
Need to know the distance to some galaxies in order to know the slope of velocity versus distance.
Different methods yielded different distances.
Some values of Ho yielded an Universe younger than some of its stars.
HST helped solve the problem: Cepheids.

8. Hubble Space Telescope
Use HST to find Cepheids in other galaxies.

9. Hubble’s Constant In recent decades, Ho = 50 – 100 km/s/Mpc.
Difference in distances by factor of 2.
Difference in age of Universe by factor of 2.
Recent HST results: Ho = 70 +/- 7 km/s/Mpc
Recall: T = 1/ Ho
T = 15 billion years
Is this older than the oldest stars?
Recent HST result says the oldest white dwarfs are 13 billion years old!

10. The End of the Universe Will the universe expand forever?
Depends on the density of the Universe.
Too big: Big Crunch
Closed Universe
Bound Universe
Too small: Big Freeze
Open Universe
Unbound Universe

11. Critical Density Dividing line is the critical density.
Wo is the ratio of measured density to the critical density.
If Wo > 1 then closed, Wo < 1 then open.

12. Density of the Universe
Add up all the mass we see and Wo = 0.01
Result: Open Universe  Big Freeze!

13. The Future from the Past
Is the Universe:
Slowing down?
Speeding up?
Staying the same velocity?
In the past, was the Universe:
Going faster?
Going slower?
Going the same velocity?
The Universe is a time machine.

14. Lookback Time
We see everything as it once was.
Old
Young

15. Baby Boomer Universe 90s 80s 70s 60s 50s 40s
Farther away we look, further back in time we see!

16. What We See

17. Nearby Galaxies

18. Hubble Deep Field

19. Homework #21
No Homework for Wednesday