The energy levels of a hydrogen atom are given by the formula:
\[
E_n = - \frac{13.6}{n^2} \, \text{eV}
\]
where \( n \) is the principal quantum number of the energy level.
- The ground state energy corresponds to \( n = 1 \), so:
\[
E_1 = - \frac{13.6}{1^2} = -13.6 \, \text{eV}
\]
- The energy of the third excited state corresponds to \( n = 4 \), so:
\[
E_4 = - \frac{13.6}{4^2} = - \frac{13.6}{16} = -0.85 \, \text{eV}
\]
Now, the energy of the radiation emitted is the difference between the energy of the third excited state and the ground state:
\[
\Delta E = E_1 - E_4 = (-13.6) - (-0.85) = -13.6 + 0.85 = -12.75 \, \text{eV}
\]
Therefore, the energy of the radiation emitted is \( 12.75 \, \text{eV} \).