In astronomical observations, signals observed from the distant stars are generally weak. If the photon detector receives a total of 3.15 \times 10^{-18} J from the radiations of 600 \mathrm{~nm}, calculate the number of photons received by the detector.
In astronomical observations, signals observed from the distant stars are generally weak. If the photon detector receives a total of 3.15 \times 10^{-18} J from the radiations of 600 \mathrm{~nm}, calculate the number of photons received by the detector.

From the expression of energy of one photon (E),
E=\frac{h c}{\lambda}
Where,
\lambda denotes the wavelength of the radiation
\mathrm{h} is Planck’s constant
c denotes the velocity of the radiation
Substituting these values in the expression for E :
E=\frac{\left(6.626 \times 10^{-34} J s\right)\left(3 \times 10^{8} \mathrm{~ms}^{-1}\right)}{\left(600 \times 10^{-9}\right)}=3.313 \times 10^{-19} \mathrm{~J}
Energy held by one photon =3.313 \times 10^{-19} J
No. photons received with 3.15 \times 10^{-18} J energy
=\frac{3.15 \times 10^{-18} J}{3.313 \times 10^{-19} J}
=9.5
\approx 10