A ray coming from an object which is situated at zero distance in the air and falls on a spherical glass surface (\( n = 1.5 \)). Then the distance of the image will be ………. \( R \) is the radius of curvature of a spherical glass.}
Step 1: Using the Refraction Formula for a Spherical Surface
The refraction formula for a spherical surface is given by: \[ \frac{n_2}{v} - \frac{n_1}{u} = \frac{n_2 - n_1}{R} \] where:
- \( n_1 \) is the refractive index of the first medium (air, \( n_1 = 1 \)),
- \( n_2 \) is the refractive index of the second medium (glass, \( n_2 = 1.5 \)),
- \( u \) is the object distance,
- \( v \) is the image distance,
- \( R \) is the radius of curvature.
Step 2: Substituting the Given Values
Since the object is at \( u = 0 \), the equation simplifies to: \[ \frac{n_2}{v} - \frac{1}{0} = \frac{1.5 - 1}{R} \] Since \( \frac{1}{0} \) tends to infinity, the equation reduces to: \[ \frac{n_2}{v} = \frac{0.5}{R} \]
Step 3: Solving for \( v \)
Rearranging the equation: \[ v = \frac{1.5 R}{0.5} = 3R \] Thus, the image distance is \( 3R \).
For a plane mirror, the focal length is ……..
For a thin prism, if the angle of the prism is \( A \) with a refractive index of 1.6, then the angle of minimum deviation will be …….
Consider a refracting telescope whose objective has a focal length of 1m and the eyepiece a focal length of 1cm, then the magnifying power of this telescope will be ……..
The refractive index of glass is 1.6 and the speed of light in glass will be ……… . The speed of light in vacuum is \( 3.0 \times 10^8 \) ms\(^{-1}\).