The longest wavelength of spectral lines in the Balmer series is determined by examining the energy levels of hydrogen and the relevant electron transitions.
Step 1: Lyman Series Analysis
The energy-wavelength relationship for the Lyman series is expressed as:
\[ \frac{hc}{\lambda} = -13.6 \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right) \quad (\text{in eV}), \]
where \( n_1 = 1 \) and \( n_2 \) varies. The shortest wavelength observed in the Lyman series is:
\[ \lambda_{\text{Lyman}} = 915 \, \text{\AA}. \]
Step 2: Balmer Series Calculation
For the Balmer series, the initial and final energy levels are:
- \( n_1 = 2 \)
- \( n_2 = 3 \) for the longest wavelength transition.
The energy difference for this transition is:
\[ \frac{hc}{\lambda_1} = -13.6 \left( \frac{1}{2^2} - \frac{1}{3^2} \right). \]
This simplifies to:
\[ \frac{hc}{\lambda_1} = -13.6 \left( \frac{1}{4} - \frac{1}{9} \right). \]
Further simplification yields:
\[ \frac{hc}{\lambda_1} = -13.6 \left( \frac{5}{36} \right). \]
Step 3: Wavelength Relationship Determination
Utilizing the data from the Lyman series, the wavelength for the transition in the Balmer series can be related as follows:
\[ \lambda_1 = \lambda_{\text{Lyman}} \times \frac{36}{5}. \]
Substituting the known value for \( \lambda_{\text{Lyman}} \):
\[ \lambda_1 = 915 \times \frac{36}{5} = 6588 \, \text{\AA}. \]
Consequently, the longest wavelength spectral line in the Balmer series measures \( 6588 \, \text{\AA} \).
