| List I (Spectral Lines of Hydrogen for transitions from) | List II (Wavelength (nm)) | ||
| A. | n2 = 3 to n1 = 2 | I. | 410.2 |
| B. | n2 = 4 to n1 = 2 | II. | 434.1 |
| C. | n2 = 5 to n1 = 2 | III. | 656.3 |
| D. | n2 = 6 to n1 = 2 | IV. | 486.1 |
Step 1: Review Balmer Series Formula
The Balmer series defines transitions to \( n_1 = 2 \) in hydrogen atoms. The wavelength of emitted light is calculated using:
$$ \frac{1}{\lambda} = R \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right) $$
Where:
\(\lambda\) represents the wavelength of emitted light.
R is the Rydberg constant.
n₁ is the lower energy level, fixed at \( n_1 = 2 \) for the Balmer series.
n₂ is the higher energy level, with \( n_2 > 2 \).
Step 2: Correlate Wavelengths
Observed wavelengths for each transition are matched as follows:
\( n_2 = 3 \rightarrow n_1 = 2 \) corresponds to 656.3 nm → (A-III)
\( n_2 = 4 \rightarrow n_1 = 2 \) corresponds to 486.1 nm → (B-IV)
\( n_2 = 5 \rightarrow n_1 = 2 \) corresponds to 434.1 nm → (C-II)
\( n_2 = 6 \rightarrow n_1 = 2 \) corresponds to 410.2 nm → (D-I)
Step 3: Final Matching
The accurate correspondence is:
A-III
B-IV
C-II
D-I