In the hydrogen atom, the energy of the electron in the \( n^{th} \) orbit is given by: \[ E_n = - \frac{13.6}{n^2} \text{ eV} \] The wavelength of the emitted photon when the electron transitions from an upper orbit \( n_2 \) to a lower orbit \( n_1 \) can be found using the relation: \[ E_{\text{photon}} = E_{n_2} - E_{n_1} \] The energy of the photon is related to the wavelength \( \lambda \) by the equation: \[ E_{\text{photon}} = \frac{hc}{\lambda} \] where \( h \) is Planck's constant and \( c \) is the speed of light. For the transition from the 3rd orbit to the 2nd orbit, the energy difference is: \[ \Delta E_{3 \rightarrow 2} = E_3 - E_2 = - \frac{13.6}{9} - \left( - \frac{13.6}{4} \right) = \frac{13.6}{4} - \frac{13.6}{9} \] The wavelength of the emitted photon for this transition is: \[ \lambda = \frac{hc}{\Delta E_{3 \rightarrow 2}} = \frac{5}{27} \cdot \lambda \] For the transition from the 2nd orbit to the 1st orbit, the energy difference is: \[ \Delta E_{2 \rightarrow 1} = E_2 - E_1 = - \frac{13.6}{4} - \left( - \frac{13.6}{1} \right) = \frac{13.6}{1} - \frac{13.6}{4} \] The wavelength of the emitted photon for this transition is: \[ \lambda_{\text{new}} = \frac{hc}{\Delta E_{2 \rightarrow 1}} = \frac{5}{27} \cdot \lambda \]
Thus, the wavelength of the photon emitted when the electron jumps from the second to the first orbit is \( \frac{5\lambda}{27} \).