When sunlight falls normally on Earth,a luminous flux density (illuminance) of $1.57 \times 10^5 \; lm/m^2$ is produced on Earth. The distance of Earth from the Sun is $1.5 \times 10^8 \; km$. The luminous intensity of the Sun in candela is:

  • A
    $3.53 \times 10^{27}$
  • B
    $3.53 \times 10^{25}$
  • C
    $3.53 \times 10^{29}$
  • D
    $3.53 \times 10^{21}$

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