Concept: The wavelength ($\lambda$) of a spectral line for a hydrogen-like species is governed by the Rydberg formula: $\frac{1}{\lambda} = R Z^2 \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right)$. For the same electronic transition, the wavelength is inversely proportional to the square of the atomic number ($Z^2$), meaning $\lambda \propto \frac{1}{Z^2}$.
Step 1: Identify the atomic numbers (Z) for Hydrogen and Helium ion.
For Hydrogen ($H$), the atomic number $Z = 1$. For the Helium ion ($He^+$), the atomic number $Z = 2$.
Step 2: Establish the relationship between wavelengths.
Since $\lambda_{ion} = \frac{\lambda_H}{Z^2}$, we apply this to the helium ion:
\[
\lambda_{He^+} = \frac{\lambda_H}{Z_{He}^2} = \frac{\lambda_H}{2^2} = \frac{\lambda_H}{4}
\]
Step 3: Calculate the final wavelength.
Given the initial wavelength for hydrogen $\lambda_H = 656.4$ nm, we calculate the wavelength for the $He^+$ ion as follows:
\[
\lambda_{He^+} = \frac{656.4 \text{ nm}}{4} = 164.1 \text{ nm}
\]