1. Measuring the Speed of EMR
Lesson 2

2. Objectives You will be able to
Describe qualitatively some experiments measuring the speed of light
Quantitatively calculate the speed of light using Michelson’s apparatus.

4. Speed of Sound It was known that the speed of sound was about 330 m/s.
Experiment to measure speed:
Person A and B are on two hills.
Person A fires a cannon and drops flag.
Person at B starts clock when flag dropped.
Person at B hears sound and stops clock.

6. Speed of Light Person A and B are on two hills.
Person A flashes light and starts clock.
Person B sees flash and sends a flash of light back at A.
Person A sees flash and stops clock.
Suppose the distance from one hill to the other is 20.0 km. Using today’s accepted speed of light (3.00 x 108 m/s), calculate the time that it takes the light to go from A to B and back again.

7. Calculation:
Clearly a time too small to measure centuries ago.

9. Roemer and Huygens
Roemer found that the time that Io would appear from behind Jupiter would vary.
He determined that the maximum difference in time would be 22 minutes.
This was due to the movement of the Earth away from Jupiter as it moves around the Sun.

10. Roemer and Huygens
This “late” time was the time it took light to cover the extra distance.

11. Roemer and Huygens
Roemer could not calculate the speed of light because the distance from the Earth to the Sun was not known at this time.
Huygens estimated the diameter of the Earth's orbit around the Sun and used Roemer's data to calculate the speed of light.
His value was about 2.0 x 108 m/s.
The error was due to the error in “late time” observed by Roemer. The actual late time is 16 mins and not the 22 mins that Roemer stated.

14. Michelson’s Apparatus

15. Michelson’s 8 sided mirror – How it works
Line everything up while the 8 sided mirror is stationary.
Start to rotate the mirrors.
The light will be reflected and no longer be seen in the observer’s telescope.
The light will return to the same position (observed in telescope) if the mirror rotates fast enough that side B moves to exactly the same position as side C was initially in the time that it takes the light to go to the far mirror and back. (1/8 of a revolution)

16. Example 1:
The octagonal mirror apparatus turns at RPM and an image is observed through the telescope.
Determine the time required for the mirror to go totally around once.
Calculate the time for side B to get to side C.
Calculate c based on this data.

17. Calculations

18. Value of c

19. Example 2:
Using the currently accepted value for c, calculate how far apart the two mirrors would need to be placed if the octagonal mirror is able to turn at RPM.

20. Calculation

21. Calculation of d

22. Example 3: Calculation:
How fast (in RPM) would a hexagonal mirror need to turn if the stationary mirror is 20.0 km from the rotating mirror?
Calculation:
20.0 km is d between. Light travels 20.0 km • 2 = 40.0 km

23. Mirror t = 1.33… x 10-4 s is time for mirror to turn 1/6 rotation.
t for full rotation = 1.33… x 10-4 s • 6 = s
t in min = 1.33… x 10-6 min

24. Your Turn Read text pages 648-652 Do practice problems p. 650
check and reflect p. 652 #1-6