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Calculate the wavelength of radiation emited when an electron in a hydrogen atom makes a transition from an energy level with `n = 3` to a level with `n= 2`

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To calculate the wavelength of radiation emitted when an electron in a hydrogen atom transitions from an energy level with \( n = 3 \) to a level with \( n = 2 \), we can use the Rydberg formula for hydrogen: \[ \frac{1}{\lambda} = R_H \left( \frac{1}{n_2^2} - \frac{1}{n_1^2} \right) \] where: - \( \lambda \) is the wavelength of the emitted radiation, - \( R_H \) is the Rydberg constant for hydrogen, approximately \( 1.1 \times 10^7 \, \text{m}^{-1} \), - \( n_1 \) is the initial energy level (3 in this case), - \( n_2 \) is the final energy level (2 in this case). ### Step-by-Step Solution: 1. **Identify the values of \( n_1 \) and \( n_2 \)**: - Here, \( n_1 = 3 \) and \( n_2 = 2 \). 2. **Substitute the values into the Rydberg formula**: \[ \frac{1}{\lambda} = R_H \left( \frac{1}{n_2^2} - \frac{1}{n_1^2} \right) \] \[ \frac{1}{\lambda} = 1.1 \times 10^7 \left( \frac{1}{2^2} - \frac{1}{3^2} \right) \] 3. **Calculate \( \frac{1}{2^2} \) and \( \frac{1}{3^2} \)**: - \( \frac{1}{2^2} = \frac{1}{4} = 0.25 \) - \( \frac{1}{3^2} = \frac{1}{9} \approx 0.1111 \) 4. **Calculate \( \frac{1}{n_2^2} - \frac{1}{n_1^2} \)**: \[ \frac{1}{n_2^2} - \frac{1}{n_1^2} = 0.25 - 0.1111 = 0.1389 \] 5. **Substitute back into the equation**: \[ \frac{1}{\lambda} = 1.1 \times 10^7 \times 0.1389 \] 6. **Calculate \( \frac{1}{\lambda} \)**: \[ \frac{1}{\lambda} \approx 1.1 \times 10^7 \times 0.1389 \approx 1.538 \times 10^6 \, \text{m}^{-1} \] 7. **Calculate \( \lambda \)**: \[ \lambda = \frac{1}{1.538 \times 10^6} \approx 6.5 \times 10^{-7} \, \text{m} \] 8. **Convert to nanometers**: \[ \lambda \approx 6.5 \times 10^{-7} \, \text{m} = 650 \, \text{nm} \] ### Final Answer: The wavelength of radiation emitted when an electron transitions from \( n = 3 \) to \( n = 2 \) in a hydrogen atom is approximately **650 nm**.

To calculate the wavelength of radiation emitted when an electron in a hydrogen atom transitions from an energy level with \( n = 3 \) to a level with \( n = 2 \), we can use the Rydberg formula for hydrogen: \[ \frac{1}{\lambda} = R_H \left( \frac{1}{n_2^2} - \frac{1}{n_1^2} \right) \] where: - \( \lambda \) is the wavelength of the emitted radiation, ...
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