In a Franck-Hertz experiment with hydrogen, the initial current dip at 10.2 V indicates the energy required to excite a hydrogen atom. This energy, when emitted as a photon upon de-excitation to the ground state, corresponds to a specific wavelength. We will calculate this wavelength.
The solution utilizes concepts from the Franck-Hertz experiment and the Bohr model of atomic excitation and photon emission.
Step 1: Determine the first excitation energy of the hydrogen atom.
The first excitation potential is \( V = 10.2 \, \text{V} \). The energy absorbed by a hydrogen atom is:
\[ \Delta E = e \times V = e \times 10.2 \, \text{V} = 10.2 \, \text{eV} \]This is the energy difference between the ground state (\(n=1\)) and the first excited state (\(n=2\)) of hydrogen.
Step 2: Determine the energy of the emitted photon.
When the excited hydrogen atom returns to the ground state, it emits a photon with energy equal to the excitation energy.
\[ E_{\text{photon}} = \Delta E = 10.2 \, \text{eV} \]Step 3: Calculate the wavelength of the emitted photon.
Using Planck's relation, the wavelength \( \lambda \) is:
\[ \lambda = \frac{hc}{E_{\text{photon}}} \]Given \( hc = 1245 \, \text{eV nm} \).
Step 4: Substitute the values and compute the result.
\[ \lambda = \frac{1245 \, \text{eV nm}}{10.2 \, \text{eV}} \] \[ \lambda \approx 122.0588 \, \text{nm} \]Rounding to the nearest integer yields:
\[ \lambda \approx 122 \, \text{nm} \]The wavelength of the light emitted when the hydrogen atom returns to its ground state from the first excitation level is 122 nm.
| List I (Spectral Lines of Hydrogen for transitions from) | List II (Wavelength (nm)) | ||
| A. | n2 = 3 to n1 = 2 | I. | 410.2 |
| B. | n2 = 4 to n1 = 2 | II. | 434.1 |
| C. | n2 = 5 to n1 = 2 | III. | 656.3 |
| D. | n2 = 6 to n1 = 2 | IV. | 486.1 |