$A$ converging lens of a telescope with a diameter of $5 \text{ cm}$ has a focal length of $25 \text{ cm}$. In the focal plane of the lens, the distance between the centres of the Fraunhofer diffraction pattern is (wavelength of light used = $5000 \text{ Å}$, Rayleigh's criterion is satisfied).

  • A
    $2.5 \times 10^{-4} \text{ cm}$
  • B
    $3.05 \times 10^{-4} \text{ cm}$
  • C
    $5.0 \times 10^{-4} \text{ cm}$
  • D
    $6.1 \times 10^{-4} \text{ cm}$

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