Step 1: Understanding the Rayleigh Criterion. The limit of resolution (θ) of a telescope is given by Rayleigh's criterion: \[ \theta = \frac{1.22 \lambda}{D} \] where: - \( \lambda \) is the wavelength of light (540 nm = \( 540 \times 10^{-9} \) m), - \( D \) is the diameter of the telescope’s objective (3.6 m), - The factor \( 1.22 \) is derived from diffraction theory.
Step 2: Substituting the values. \[ \theta = \frac{1.22 \times 540 \times 10^{-9}}{3.6} \] \[ \theta = \frac{658.8 \times 10^{-9}}{3.6} \] \[ \theta = 1.83 \times 10^{-7} \text{ rad} \] Final Answer: \[ \boxed{1.83 \times 10^{-7} \text{ rad}} \]
A source and an observer move away from each other with same velocity of 10 m-1 with respect to the ground. If the observer finds the frequency of sound coming from the source as 1980 Hz, then the actual frequency of the source is (speed of sound in air = 340 ms-1)
Two convex lenses of focal lengths 20 cm and 30 cm are placed in contact with each other co-axially. The focal length of the combination is: