1. Supernova in images of Greg Thorne and Nick McCaw
Image of spiral galaxy NGC 3938 taken on April 7 for 29:050 lab partners Thorne and McCaw.
Discovery was reported only ten days earlier on March 27 of SN2005ay.

2. Black Holes Observed properties of black holes Gravitational energy
Rotating black holes
Eddington luminosity
Accretion disks
Jets

3. Black Holes Fundamental properties of black holes Mass Spin
Charge = zero for astrophysical black holes

4. Observed properties of black holes
Luminosity
Orientation
Jets

5. Gravitational energy
The Hoover dam generates 4 billion kilowatt hours of power per year.
Where does the energy come from?

6. Gravitational energy
Water falling down to the generators at the base of the dam accelerates to 80 mph.
The same water leaving the turbines moves at only 10 mph.
The gravitational energy of the water at the top of the dam is converted to kinetic energy by falling. The turbines convert kinetic energy to electricity.

7. Gravitational energy
Black holes generate energy from matter falling into them.

9. Compared to a non-rotating black hole of the same mass, the event horizon for a rotating black is
smaller
larger
the same
blue

10. Rotating black holes For non-rotating black holes:
- event horizon is at the Schwarzschild radius
- inner edge of the disk is at 3 Schwarzschild radii
For maximally rotating black holes:
- event horizon is at ½ Schwarzschild radius
- inner edge of the disk is at ½ Schwarzschild radius
Schwarzschild radius = 3 km (M/MSun)

11. Luminosity
Gravitational energy is converted to kinetic energy as particles fall towards BH
Efficiency of generators:
Chemical burning < %
Nuclear burning < 1%
Non-rotating black hole = 6%
Rotating black hole = 42%

12. Accretion disk

13. In Active Galaxies the disk is surrounded by a dusty torus

14. Accretion disks

15. The light from a quasar is emitted from a region 10 light-days across
The light from a quasar is emitted from a region 10 light-days across. What does this tell us about the quasar?
The brightness will change every day.
The brightness will change every 20 days.
The brightness will not change in less than 10 days.
The brightness will not change in less than 100 days.

16. Varieties of Active Galaxies
Radio Galaxies – big jets, no obvious BH
Quasars – jets and BH
Blazars – mainly see the jet

17. Orientation

18. Eddington Luminosity
Limit on the brightness of a black hole

19. Eddington Luminosity

20. Accretion disks
Disks form because infalling matter has angular momentum.
Accretion leads to release of gravitational energy.
Inner regions of disks rotate very rapidly – near the speed of light.
The luminosity of a black hole is limited by its mass.
Accretion disks of solar-mass and supermassive BHs are similar.

21. Review Questions
What are fundamental versus observed properties of black holes?
What is the efficiency of a BH for conversion of matter to energy?
What is the maximum luminosity for a BH of a given mass?
Are the different types of Active Galaxies fundamentally different?