To find the wave number of the last line of the Balmer series in the hydrogen spectrum, we can use the formula for the wave number (\( \bar{\nu} \)) in the hydrogen emission spectrum. The formula is given by the Rydberg formula:
where \( R_H \) is the Rydberg constant, \( n_1 \) is the lower energy level to which the electron falls, and \( n_2 \) is the higher energy level from which the electron falls. For the Balmer series, \( n_1 = 2 \) and \( n_2 \) should be larger.
For the last line of the Balmer series, the transition occurs from infinity to \( n=2 \). Therefore, \( n_2 = \infty \).
Using this, the formula for the wave number becomes:
Given the Rydberg constant \( R_H = 10^7 \, \text{m}^{-1} \), substituting the values, we have:
Hence, the wave number of the last line of the Balmer series in the hydrogen spectrum is 0.25 \times 10^7 \, \text{m}^{-1}.
Conclusion: The correct option is 0.25 \times 10^7 \, \text{m}^{-1}.