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Asked in CBSE AIPMT 2008 · Lens formula and magnification
Given: f=10 cm=0.10 m, the sun's diameter O=1.39×10⁹ m and its distance u=1.5×10¹¹ m.
Idea: the sun is effectively at infinity, so its image forms in the focal plane and v=f.
Object and image subtend the same angle at the lens, so I/O=v/u.
I=1.39×10⁹×(0.10)/(1.5×10¹¹)=(1.39×10⁸)/(1.5×10¹¹)
I=9.27×10⁻⁴ m, printed in the options as 9.2×10⁻⁴ m.
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