Step 1: The energy of a photon emitted during the transition of an electron from \( n = 5 \) to \( n = 1 \) is given by the energy difference between the two states. Using the formula for the energy levels of the hydrogen atom: \[ E_n = -\frac{13.6 \, {eV}}{n^2}. \] The energy of the photon emitted is: \[ \Delta E = E_5 - E_1 = \left(-\frac{13.6}{5^2}\right) - \left(-\frac{13.6}{1^2}\right) = -\frac{13.6}{25} + 13.6 = 13.6 \left( 1 - \frac{1}{25} \right) = 13.6 \times \frac{24}{25} = 13.056 \, {eV}. \] Now converting the energy to joules: \[ E = 13.056 \, {eV} \times 1.602 \times 10^{-19} \, {J/eV} = 2.09 \times 10^{-18} \, {J}. \] Step 2: The recoil energy of the atom will be equal to the energy of the emitted photon. By conservation of momentum, the recoil energy of the hydrogen atom is: \[ E_{{recoil}} = \frac{p^2}{2m_H}, \] where \( p \) is the momentum and \( m_H \) is the mass of the hydrogen atom (\( m_H = 1.67 \times 10^{-27} \, {kg} \)).
Step 3: The momentum \( p \) is related to the photon energy by \( p = \frac{E}{c} \), where \( c \) is the speed of light. So, \[ E_{{recoil}} = \frac{(E/c)^2}{2m_H} = \frac{(2.09 \times 10^{-18} / 3 \times 10^8)^2}{2 \times 1.67 \times 10^{-27}}. \] Solving this gives: \[ v_{{recoil}} = \sqrt{\frac{2E_{{recoil}}}{m_H}} \approx 4.17 \, {m/s}. \]