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
32f. That's because the force is directly proportional to the product of the masses and inversely proportional to the square of the distance. So you get 2•(1/1/4)^2=2•16=32