To find absorption lines in a hydrogen atom with n=10, you can use a spectroscope or a spectrometer. These instruments can measure the light emitted from the atom and detect any absorption lines.
Absorption lines in a hydrogen atom are caused by the absorption of light at specific frequencies by the electrons in the atom. This absorption occurs when the energy of the light matches the energy difference between different energy levels in the atom, specifically the n=10 energy level in this case.
Absorption lines and emission lines can be distinguished by their appearance on a spectrum. Absorption lines appear as dark lines, while emission lines appear as bright lines. Absorption lines occur when light is absorbed by the atom, while emission lines occur when the atom emits light.
There are other elements and molecules that can produce absorption lines at the n=10 energy level, but they may not be as prominent as in a hydrogen atom. Each element and molecule has its own unique energy levels, so absorption lines at the n=10 level may not be as easily detectable in other substances.
Yes, absorption lines at the n=10 energy level can be used for various practical applications. They are commonly used in astronomy to study the composition and structure of stars, as well as in spectroscopy and chemical analysis to identify and quantify different substances based on their absorption spectra.