In the hydrogen atom, the energy levels are given by the formula:
\[
E_n = - \frac{13.6}{n^2} \, \text{eV}
\]
Where:
- \( E_n \) is the energy of the nth level,
- \( n \) is the principal quantum number,
- 13.6 eV is the Rydberg energy for hydrogen.
1. Energy Level Diagram for Hydrogen:
The energy levels in the hydrogen atom are shown in the diagram below:
In this diagram:
- The energy of the electron decreases as it moves closer to the nucleus.
- The ground state corresponds to \( n = 1 \), and higher levels correspond to \( n = 2, 3, 4, .... \).
2. Lyman Series Transitions:
The Lyman series corresponds to transitions where the final state is \( n = 1 \) (the ground state). The first line of the Lyman series occurs when the electron transitions from \( n = 2 \) to \( n = 1 \). The energy difference between these levels is:
\[
\Delta E_1 = E_2 - E_1 = \left( - \frac{13.6}{2^2} \right) - \left( - \frac{13.6}{1^2} \right) = -3.4 \, \text{eV} + 13.6 \, \text{eV} = 10.2 \, \text{eV}
\]
The wavelength \( \lambda_1 \) of this transition is given by the formula:
\[
\lambda_1 = \frac{hc}{\Delta E_1}
\]
Substituting the values (\( h = 6.626 \times 10^{-34} \, \text{J} . \text{s} \), \( c = 3 \times 10^8 \, \text{m/s} \), and \( \Delta E_1 = 10.2 \, \text{eV} \)):
\[
\lambda_1 = \frac{6.626 \times 10^{-34} \times 3 \times 10^8}{10.2 \times 1.602 \times 10^{-19}} \approx 121.6 \, \text{nm}
\]
3. Balmer Series Transitions:
The Balmer series corresponds to transitions where the final state is \( n = 2 \). The second line of the Balmer series occurs when the electron transitions from \( n = 3 \) to \( n = 2 \). The energy difference is:
\[
\Delta E_2 = E_3 - E_2 = \left( - \frac{13.6}{3^2} \right) - \left( - \frac{13.6}{2^2} \right) = -1.511 \, \text{eV} + 3.4 \, \text{eV} = 1.889 \, \text{eV}
\]
The wavelength \( \lambda_2 \) of this transition is:
\[
\lambda_2 = \frac{hc}{\Delta E_2} = \frac{6.626 \times 10^{-34} \times 3 \times 10^8}{1.889 \times 1.602 \times 10^{-19}} \approx 656.3 \, \text{nm}
\]
4. Ratio of the Wavelengths:
The ratio of the wavelengths is:
\[
\frac{\lambda_1}{\lambda_2} = \frac{121.6 \, \text{nm}}{656.3 \, \text{nm}} \approx 0.185
\]
Thus, the ratio of the wavelengths of the first line of the Lyman series and the second line of the Balmer series is approximately 0.185.