Statement I: The Balmer series involves electronic transitions to the n=2 energy level. The lowest energy transition within this series occurs from n=3 to n=2. The wavenumber ($\tilde{u}$) for this transition is calculated using the Rydberg formula:
\[ \tilde{u} = R_\text{H} \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right) \]
For the lowest energy Balmer transition ($n_1$=2, $n_2$=3):
\[ \tilde{u} = R_H \left( \frac{1}{2^2} - \frac{1}{3^2} \right) = R_H \left( \frac{1}{4} - \frac{1}{9} \right) = R_H \left( \frac{9 - 4}{36} \right) = \frac{5}{36} R_H \]
The calculated wavenumber is $\frac{5}{36} R_H$ cm$^{-1}$, confirming statement I is true.
Statement II: Wien's displacement law establishes an inverse relationship between the wavelength of maximum intensity of blackbody radiation and its temperature. Consequently, an increase in temperature leads to a shift in the wavelength of maximum intensity towards shorter wavelengths. Thus, statement II is true.
