(a) If s = object distance, s' = average distance, L = luminance of the sounce, ΔS = area of the source as sumed to be a plane surface held normal to the principal axis, then we find for the flux ΔΦ incident on the lens
Here we are assuming D « s, and ignoring the variation of L since a is small
Then if L' is the luminance of the image, and is the area of the image then similarly
(b) In this case the image on the white screen from a Lambert source. Then if its luminance is L0 its luminosity will be the πL0 and
since s' depends on f, s but not on D.