Final Answer:
The electron in the n = 6level of the hydrogen atom, relaxing and emitting light of
, transitions to the n = 3 principal level.
Step-by-step explanation:
When an electron transitions from a higher energy level n_i to a lower energy level n_f in a hydrogen atom, it emits light with a wavelength given by the Rydberg formula:
![\[ (1)/(\lambda) = R_H \left((1)/(n_f^2) - (1)/(n_i^2)\right), \]](https://img.qammunity.org/2024/formulas/physics/high-school/b7y1nho3j36dliz555l400ly0dc0bmnigj.png)
where R_H is the Rydberg constant for hydrogen
is the wavelength of the emitted light, and n_i and n_f are the principal quantum numbers of the initial and final energy levels, respectively.
In this case, the electron transitions from
, and the wavelength of the emitted light is given as
. By rearranging the formula, we can solve for
:
![\[ (1)/(93.8 * 10^(-9)) = 1.097 * 10^7 \left((1)/(n_f^2) - (1)/(6^2)\right). \]](https://img.qammunity.org/2024/formulas/physics/high-school/xl7tioe4w3ekq515gkqkm2e0sdoa5o4ck5.png)
Solving this equation yields
indicating that the electron relaxes to the
principal level. Understanding these quantum transitions is fundamental to explaining the spectral lines observed in hydrogen atoms.