The Lyman and Paschen series are part of the hydrogen atom's emission spectra. The Lyman series corresponds to transitions where the final state is \( n = 1 \), while the Paschen series corresponds to transitions where the final state is \( n = 3 \).
 
 The wavelength of light emitted during these transitions can be found using the Rydberg formula for hydrogen:
 
 \[
 \frac{1}{\lambda} = R_H \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right)
 \]
 
 where:
 - \( \lambda \) is the wavelength of the emitted radiation,
 - \( R_H \) is the Rydberg constant,
 - \( n_1 \) and \( n_2 \) are the principal quantum numbers of the initial and final states, respectively.
 
 For the Lyman series limit, the transition is from \( n_2 \to 1 \), and the wavelength corresponds to the transition where \( n_2 \to \infty \). Thus, for Lyman:
 
 \[
 \frac{1}{\lambda_{\text{Lyman}}} = R_H \left( \frac{1}{1^2} - \frac{1}{\infty^2} \right) = R_H
 \]
 
 For the Paschen series limit, the transition is from \( n_2 \to 3 \), and the wavelength corresponds to the transition where \( n_2 \to \infty \). Thus, for Paschen:
 
 \[
 \frac{1}{\lambda_{\text{Paschen}}} = R_H \left( \frac{1}{3^2} - \frac{1}{\infty^2} \right) = R_H \left( \frac{1}{9} \right)
 \]
 
 Now, the ratio of the wavelengths is the inverse of the ratio of the terms:
 
 \[
 \frac{\lambda_{\text{Lyman}}}{\lambda_{\text{Paschen}}} = \frac{9}{1} = 9
 \]
 
 Thus, the ratio of the wavelength of Lyman to Paschen is \( 9:1 \), meaning the wavelength of the Lyman series limit is 9 times greater than that of the Paschen series limit.