Question:

In hydrogen atom, during the transition of electron from \( n \)th outer orbit to first Bohr orbit, a photon of wavelength \( \lambda \) is emitted. The value of \( n \) is: [\( R \) = Rydberg's constant]

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The Rydberg formula allows us to calculate the wavelength of emitted radiation for electron transitions in hydrogen atoms.
Updated On: Feb 9, 2026
  • \( \frac{\lambda R}{\sqrt{\lambda R - 1}} \)
  • \( \sqrt{\frac{R - 1}{\lambda R}} \)
  • \( \sqrt{R (\lambda R - 1)} \)
  • \( \sqrt{\lambda (R - 1)} \)
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The Correct Option is A

Solution and Explanation

Step 1: Using the Rydberg Formula.
The wavelength of emitted radiation when an electron transitions between two orbits in a hydrogen atom is given by the Rydberg formula: \[ \frac{1}{\lambda} = R \left( \frac{1}{n^2} - \frac{1}{1^2} \right) \] For transition from \( n \)th orbit to the first orbit, we can rewrite the equation: \[ \frac{1}{\lambda} = R \left( 1 - \frac{1}{n^2} \right) \] Thus, solving for \( n \), we get: \[ n = \frac{\lambda R}{\sqrt{\lambda R - 1}} \] Step 2: Conclusion.
Thus, the value of \( n \) is \( \frac{\lambda R}{\sqrt{\lambda R - 1}} \).
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