A telescope of objective lens diameter 2m uses light of wavelength 5000˚A for viewing starts. The minimum angular separation between two stars whose image is just resolved by their telescope is:
Given that,
Diameter d=2m
Wave length λ=5000∘A
Now, minimum angular separation is
Δθ=1.22λd
Δθ=1.22×5000×10−102
Δθ=0.3×10−6rad
Hence, the resolving power is 0.3×10−6rad