A telescope has an objective lens of focal length 150 cm and an eyepiece of focal length 5 cm. If a 50 cm tall tower at a distance of 1 Km is observed through this telescope in normal setting then the image of the tower is θ then θ is close to;
Magnification from mirror
m=hiho=−vu
Whereas
hi= Height of image from principal axis
ho= Height of object from principal axis
u= Object distance
v= Image distance
Angular magnification m=fofe=1505=30
∴tanβtanα=30⇒tanβ=tanα×30
tanβ=(501000×30)=1510=32
tanβ=32⇒tanβ=tan−1(32)
θ=β≃60∘