METHOD 1: FIZEAU METHOD
METHOD 2: FOUCAULT METHOD
In 1857, the French physicist Léon Foucault enhanced Fizeau method to measure the speed of light using a rotating mirror and a fixed mirror, as illustrated in the picture below.
Foucault's measurement is based on the following idea:
- Light coming from the source hits a rotating mirror.
- The rotating mirror reflects the light to a fixed mirror at a far distance (like 8,000 m).
- Then fixed mirror the light back to rotating mirror.
- This backward light will be bounded off the rotating mirror towards the light source with a small angle caused by the rotation. This angle can be used calculate the speed of light.
Using this idea, Foucault was able to measure the speed of light as 299,796,000 m/s. This is very close to today's definition of the speed of light: 299,792,458 m/s.
METHOD 3: MICHELSON METHOD
Michelson's method was devised in 1931 and is the most accurate out of all of the ones we have looked at yet.
Light from an intense source S is incident on a polygon mirror M. Through further reflections this light is sent to a concave mirror M3. The geometry is set such that light from M3 is parallel. This parallel beam is allowed to travel a large distance after which it is converged at the focus of M4, and hits M5.
M5 reflects the beam back to M4, this time on its upper portion which again makes the beam parallel as it travels back to M3, after several reflections it returns to the polygon mirror and a telescope T is ready to receive the light from here.
Now if we rotate the polygon mirror such that while going the beam hits ab and while returning the polygon has rotated enough such that fg is now in the position of ab and reflects the light to T seamlessly.
Therefore we must keep increasing the rotational speed till the beam becomes visible at T. If, N = no. of faces of the mirror, ω = angular speed at which light visible, D = total distance travelled by the light. Time taken by light to travel D=Δt=D/c ,and angle rotates= Δθ=2π/Νa .Therefore,
These are the methods of calculating the speed of light.
CONCLUSION:-
d and
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