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Physics

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Speed of Light

11-12
⚡ Quick Summary
The speed of light in a vacuum is a fundamental constant. Its measurement has evolved over time, from early attempts like Galileo's to precise modern definitions. Historical methods include astronomical observations (Roemer, Bradley) and terrestrial experiments (Fizeau, Foucault, Michelson).
None explicitly mentioned in the extracted text, but the concept implies: Speed = Distance / Time
  • The speed of light in vacuum is a fundamental constant.
  • The speed of light is the same in all frames of reference.
  • In 1983, the speed of light was defined as exactly 299,792,458 m/s.
  • Early attempt to measure the speed of light: Galileo (failed due to human reaction time limitations).
  • First recorded speed of light in modern era: Olaf Roemer (astronomical observations).
  • Bradley measured the speed of light from astronomical observations. The value was quite close to the correct one.
  • First measurement of the speed of light from terrestrial experiments: Fizeau.

Foucault's Method for Measuring the Speed of Light

XII
⚡ Quick Summary
Foucault's method uses a rotating mirror to measure the speed of light within a laboratory setting. By measuring the shift in the image position due to the rotating mirror and knowing the distances between the components, the speed of light can be calculated.
["OO' = R(2Δθ)", "s = II' = SS'", 'Δθ = ωΔt = ω(2R/c)', 'c = (4R²ωa) / (s(R+b))']
The experiment involves a concave mirror (M2), a rotating plane mirror (M1), a lens (L), a glass plate (G), and a light source (S). 1. **Setup:** * A beam of light from source S is reflected by the glass plate G and converges due to the lens L onto the rotating mirror M1. * When M1 is in a specific position, the light reflected from it converges at the concave mirror M2. * The light retraces its path back to L, and a portion is reflected by G to form an image at I. * When M1 rotates by a small angle Δθ to M'1, the reflected light now converges at a slightly different point on M2, and after retracing its path, forms a new image at I'. 2. **Measurements:** * `R`: Radius of the concave mirror M2 and distance from B to O (BO = BC = R). * `b`: Distance from M1 to L. * `a`: Distance from L to S. * `ω`: Angular speed of the plane mirror M1. * `s`: Shift in the image position (II'). 3. **Derivation:** * The distance OO' is related to the angular displacement by OO' = R(2Δθ). * The shift in the image is SS' = II' = s. * The magnification of the lens L is given by SS'/OO' = a/(R+b). * Combining these relations, s / (R*(2*delta_theta)) = a / (R+b) => s = a*R*2*delta_theta / (R+b) ..... (iii) * The time taken for light to travel from M1 to M2 and back is Δt = 2R/c. * The angle rotated by M1 during this time is Δθ = ωΔt = ω(2R/c). * Substituting Δθ in the earlier expression, we get s = a*R*2*(omega * 2R/c) / (R+b). * Solving for c, we obtain the speed of light: c = (4R²ωa) / (s(R+b)). 4. **Advantages:** * Small space requirement, allowing the experiment to be performed in a laboratory. * Allows for the insertion of a transparent material between the mirrors to measure the speed of light in that medium. * Demonstrates that light travels slower in a medium compared to vacuum, contradicting Newton's corpuscular theory.