Step 1: Apply the Rydberg formula for wavelength. The wavelength \(\lambda\) of an emitted photon during an electronic transition is calculated using the Rydberg formula: \[ \frac{1}{\lambda} = R \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right), \] where \(R\) is the Rydberg constant, \(n_1\) is the final orbit number, and \(n_2\) is the initial orbit number (\(n_2>n_1\)).
Step 2: Calculate the wavelength for a transition from the 3rd orbit (\(n_2 = 3\)) to the 2nd orbit (\(n_1 = 2\)). This wavelength is denoted as \(\lambda\). Substituting these values into the Rydberg formula yields: \[ \frac{1}{\lambda} = R \left( \frac{1}{2^2} - \frac{1}{3^2} \right). \] Simplifying the expression gives: \[ \frac{1}{\lambda} = R \left( \frac{1}{4} - \frac{1}{9} \right) = R \left( \frac{9 - 4}{36} \right) = R \cdot \frac{5}{36}. \]
Step 3: Calculate the wavelength for a transition from the 4th orbit (\(n_2 = 4\)) to the 3rd orbit (\(n_1 = 3\)). This wavelength is denoted as \(\lambda'\). The formula becomes: \[ \frac{1}{\lambda'} = R \left( \frac{1}{3^2} - \frac{1}{4^2} \right). \] Simplifying this expression results in: \[ \frac{1}{\lambda'} = R \left( \frac{1}{9} - \frac{1}{16} \right) = R \left( \frac{16 - 9}{144} \right) = R \cdot \frac{7}{144}. \]
Step 4: Establish the relationship between \(\lambda'\) and \(\lambda\). Divide the equation for \(\lambda'\) by the equation for \(\lambda\): \[ \frac{1}{\lambda'} \div \frac{1}{\lambda} = \frac{R \cdot \frac{7}{144}}{R \cdot \frac{5}{36}}. \] Performing the simplification: \[ \frac{\lambda}{\lambda'} = \frac{\frac{7}{144}}{\frac{5}{36}} = \frac{7}{144} \cdot \frac{36}{5} = \frac{7 \cdot 36}{144 \cdot 5} = \frac{7}{20}. \] Rearranging to solve for \(\lambda'\): \[ \lambda' = \frac{20}{7} \lambda. \]
Step 5: Conclude the wavelength of the electron transition. The wavelength for an electron transitioning from the 4th orbit to the 3rd orbit is: \[ \boxed{\frac{20}{7} \lambda}. \]
