The ratio of the diameter of the sun to the distance between the earth and the sun is approximately $0.009$. The approximate diameter of the image of the sun formed by a concave spherical mirror of radius of curvature $0.4 \ m$ is

  • A
    $4.5 \times 10^{-6} \ m$
  • B
    $4.0 \times 10^{-6} \ m$
  • C
    $3.6 \times 10^{-3} \ m$
  • D
    $1.8 \times 10^{-3} \ m$

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