Answer:
0.134 m
Step-by-step explanation:
Given:
θ=50.0 × 10-7
λ=550 nm
angular resolution to distinguish two objects developed by Lord Rayleigh is given by:
θ= 1.22 λ/d
where λ is the wavelength of light (or other electromagnetic radiation) and D is the diameter of the aperture, lens, mirror, etc., with which the two objects are observed.
d= 1.22 λ/θ
d= (1.22 x 550 x
) / 50 x
d=0.134 m
Therefore, the smallest diameter objective lens that will resolve the stars is 0.134 m