Question:

The transition of electron that gives rise to the formation of the second spectral line of the Balmer series in the spectrum of hydrogen atom corresponds to:

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For the Balmer series, transitions end at $n_f = 2$. The spectral lines are numbered based on the value of $n_i$ (e.g., $n_i = 3$ for the first line, $n_i = 4$ for the second line).
Updated On: Feb 16, 2025
  • $n_f = 2$ and $n_i = 3$
  • $n_f = 3$ and $n_i = 4$
  • $n_f = 2$ and $n_i = 4$
  • $n_f = 2$ and $n_i = \infty$
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The Correct Option is C

Solution and Explanation

The Balmer series corresponds to transitions where the final energy level is $n_f = 2$. The second spectral line occurs when the transition happens from $n_i = 4$ to $n_f = 2$. Using the formula for the wavelength of emitted radiation: \[ \frac{1}{\lambda} = R_H \left( \frac{1}{n_f^2} - \frac{1}{n_i^2} \right), \] where: \begin{itemize} \item $R_H$ is the Rydberg constant, \item $n_f = 2$ and $n_i = 4$ for the second spectral line. \end{itemize} Substitute $n_f = 2$ and $n_i = 4$ into the equation: \[ \frac{1}{\lambda} = R_H \left( \frac{1}{2^2} - \frac{1}{4^2} \right) = R_H \left( \frac{1}{4} - \frac{1}{16} \right). \] Simplify: \[ \frac{1}{\lambda} = R_H \cdot \frac{4 - 1}{16} = R_H \cdot \frac{3}{16}. \] Thus, the correct transition for the second line in the Balmer series is: \[ \boxed{n_f = 2 \text{ and } n_i = 4}. \]
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