Magnifying power of a telescope is defined as the ratio of the angle subtended at the eye by the image formed at the least distance of distinct vision to the angle subtended at the eye by the object lying in infinity.
Magnifying power M = f0/fe (1 + fe/D)
f0 = focal length of the object = 150 cm;
fe = focal length of the eyepiece = 5 cm ;
D = least distance of the distinct vision = 25 cm
M = -150/5 (1 + 5/25) = -36
M = β/α = tanβ/tanα (As angles are small)
tanα = H/u = 100/3000 = 1/30
where H = height of the object and u = distance of the object from the objective.
M = tanβ/(1/30) = -36
30 = H'/D; H' = height of the image and D = distance of the image formation
Thus, H' = -36 × 25/30 = -30cm
Negative sign indicate that we get an inverted image.