\( \frac{1}{9} \)
The series limit is defined by transitions from \( n = \infty \) to a fixed lower energy level. The energy of a photon emitted during a transition in hydrogen is given by: \[ E = 13.6 \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right)\text{ eV} \] For the series limit, \( n_2 \to \infty \), thus: \[ E_{\text{limit}} = 13.6 \left( \frac{1}{n_1^2} \right) \]
- For the Lyman series: \( n_1 = 1 \) \[ E_L = 13.6 \cdot \frac{1}{1^2} = 13.6\ \text{eV} \] - For the Paschen series: \( n_1 = 3 \) \[ E_P = 13.6 \cdot \frac{1}{3^2} = 13.6 \cdot \frac{1}{9} = 1.51\ \text{eV} \]
The energy of a photon is related to its wavelength by \( E = \frac{hc}{\lambda} \), indicating that wavelength is inversely proportional to energy: \[ \lambda \propto \frac{1}{E} \] Consequently, the ratio of wavelengths is: \[ \frac{\lambda_L}{\lambda_P} = \frac{E_P}{E_L} = \frac{1.51}{13.6} = \frac{1}{9} \]
\(\boxed{\frac{1}{9}}\)