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In terms of Rydberg constant R, the shor...

In terms of Rydberg constant `R`, the shortest wavelength in the Balmer series of the hydrogen , atom spestrum will have wavelength

A

`1//R`

B

`4//R`

C

`3//2 R`

D

`9//R`

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To find the shortest wavelength in the Balmer series of the hydrogen atom spectrum in terms of the Rydberg constant \( R \), we can follow these steps: ### Step-by-Step Solution: 1. **Understand the Rydberg Formula**: The Rydberg formula for the wavelength of light emitted during electronic transitions in hydrogen is given by: \[ \frac{1}{\lambda} = RZ^2 \left( \frac{1}{n_f^2} - \frac{1}{n_i^2} \right) \] where: - \( \lambda \) is the wavelength, - \( R \) is the Rydberg constant, - \( Z \) is the atomic number (for hydrogen, \( Z = 1 \)), - \( n_f \) is the final energy level, - \( n_i \) is the initial energy level. 2. **Identify the Balmer Series**: In the Balmer series, the transitions end at the \( n_f = 2 \) level. The initial level \( n_i \) can be any level greater than 2. 3. **Determine the Shortest Wavelength**: The shortest wavelength corresponds to the transition from the highest energy level (which approaches infinity, \( n_i \to \infty \)) to \( n_f = 2 \). Thus, we set: - \( n_f = 2 \) - \( n_i = \infty \) 4. **Substitute into the Rydberg Formula**: Plugging these values into the Rydberg formula: \[ \frac{1}{\lambda} = R \cdot 1^2 \left( \frac{1}{2^2} - \frac{1}{\infty^2} \right) \] Simplifying this gives: \[ \frac{1}{\lambda} = R \left( \frac{1}{4} - 0 \right) = \frac{R}{4} \] 5. **Solve for Wavelength \( \lambda \)**: Taking the reciprocal to find \( \lambda \): \[ \lambda = \frac{4}{R} \] ### Conclusion: The shortest wavelength in the Balmer series of the hydrogen atom spectrum is: \[ \lambda = \frac{4}{R} \]

To find the shortest wavelength in the Balmer series of the hydrogen atom spectrum in terms of the Rydberg constant \( R \), we can follow these steps: ### Step-by-Step Solution: 1. **Understand the Rydberg Formula**: The Rydberg formula for the wavelength of light emitted during electronic transitions in hydrogen is given by: \[ \frac{1}{\lambda} = RZ^2 \left( \frac{1}{n_f^2} - \frac{1}{n_i^2} \right) ...
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