Step 1: The emitted radiation's wavelength indicates a specific hydrogen atom transition. The energy difference between energy levels determines the hydrogen spectrum series.
Step 2: Hydrogen atom energy levels are calculated using the formula:
\[
E_n = - \frac{13.6 \, \text{eV}}{n^2}
\]
Here, \( n \) represents the principal quantum number.
Step 3: The energy difference between two levels, \( n_1 \) and \( n_2 \), is calculated as:
\[
\Delta E = E_{n_1} - E_{n_2} = 13.6 \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right) \, \text{eV}
\]
Step 4: The transition corresponding to a wavelength of \( 486 \, \text{nm} \) involves the \( n_2 = 3 \) and \( n_1 = 2 \) levels of the hydrogen atom. This transition is part of the Balmer series, which includes transitions from higher levels (where \( n_2 \geq 3 \)) to \( n_1 = 2 \).
Step 5: Given that the wavelength 486 nm corresponds to this transition, it is categorized within the Balmer series of the hydrogen spectrum.