The sun's diameter is 1.4×109m and its distance from the earth is 1011m. The diameter of its image, formed by a convex lens of focal length 2m will be
0.7 cm
1.4 cm
2.8 cm
Zero (i.e. point image)
θ=AB1011=A′B′2⇒A′B′=2×1.4×1091011=2.8cm