The wavelength (\(\lambda\)) of light absorbed or emitted during a transition in a hydrogen atom can be related to the energy difference between the two states by the equation:
\[
\Delta E = \frac{R_H}{n_1^2} - \frac{R_H}{n_2^2}
\]
where \( R_H \) is the Rydberg constant, \( n_1 \) and \( n_2 \) are the principal quantum numbers of the initial and final orbits, respectively.
The energy and wavelength are inversely related:
\[
E = \frac{hc}{\lambda}
\]
where \( h \) is Planck's constant and \( c \) is the speed of light.
Thus, the ratio of the wavelengths is the inverse of the ratio of the energies.
Therefore, we calculate the energy differences for the two transitions:
1. For the n = 2 \(\rightarrow\) n = 3 transition:
\[
\Delta E_1 = \frac{R_H}{2^2} - \frac{R_H}{3^2} = R_H \left( \frac{1}{4} - \frac{1}{9} \right) = R_H \times \frac{5}{36}
\]
2. For the n = 4 \(\rightarrow\) n = 6 transition:
\[
\Delta E_2 = \frac{R_H}{4^2} - \frac{R_H}{6^2} = R_H \left( \frac{1}{16} - \frac{1}{36} \right) = R_H \times \frac{5}{144}
\]
Now, the ratio of the wavelengths (\( \lambda_1 / \lambda_2 \)) is the inverse of the ratio of the energy differences:
\[
\frac{\lambda_1}{\lambda_2} = \frac{\Delta E_2}{\Delta E_1} = \frac{\frac{5}{144}}{\frac{5}{36}} = \frac{36}{144} = \frac{1}{4}
\]
Thus, the ratio of the wavelengths is 1 : 16.
Therefore, the correct answer is (3) 1 : 4.