The wave number \( \tilde{\nu} \) (in cm\(^{-1}\)) of any transition in the hydrogen atom can be found using the Rydberg formula for the Balmer series:
\[
\tilde{\nu} = R_H \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right)
\]
where:
- \( R_H \) is the Rydberg constant for hydrogen (\( R_H = 1.097 \times 10^5 \, \text{cm}^{-1} \)),
- \( n_1 \) is the lower energy level for the transition,
- \( n_2 \) is the higher energy level for the transition.
For the longest wavelength transition in the Balmer series, the transition occurs from \( n_2 = 2 \) to \( n_1 = 3 \). Thus, we can calculate the wave number:
\[
\tilde{\nu} = 1.097 \times 10^5 \left( \frac{1}{2^2} - \frac{1}{3^2} \right)
\]
\[
\tilde{\nu} = 1.097 \times 10^5 \left( \frac{1}{4} - \frac{1}{9} \right)
\]
\[
\tilde{\nu} = 1.097 \times 10^5 \left( \frac{5}{36} \right)
\]
\[
\tilde{\nu} = 15233.3 \, \text{cm}^{-1}
\]
Therefore, the wave number for the longest wavelength transition in the Balmer series of the hydrogen spectrum is \( 15233.3 \, \text{cm}^{-1} \).