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 ……..
Step 1: Understanding the Magnifying Power of a Telescope
- A refracting telescope consists of two lenses:
- The objective lens, which collects light and forms an image.
- The eyepiece lens, which magnifies the image formed by the objective. - The magnifying power (\( M \)) of a telescope in normal adjustment (final image at infinity) is given by: \[ M = \frac{f_o}{f_e} \] where:
- \( f_o \) = focal length of the objective lens,
- \( f_e \) = focal length of the eyepiece lens.
Step 2: Substituting the Given Values
- Given: - \( f_o = 1m = 100cm \), - \( f_e = 1cm \). \[ M = \frac{100}{1} = 100 \]
Step 3: Conclusion
Thus, the magnifying power of this telescope is 100.
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\(^{-1}\).
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 …….
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.}
For a plane mirror, the focal length is ……..
If the value of \( \cos \alpha \) is \( \frac{\sqrt{3}}{2} \), then \( A + A = I \), where \[ A = \begin{bmatrix} \sin\alpha & -\cos\alpha \\ \cos\alpha & \sin\alpha \end{bmatrix}. \]