





Study with the several resources on Docsity
Earn points by helping other students or get them with a premium plan
Prepare for your exams
Study with the several resources on Docsity
Earn points to download
Earn points by helping other students or get them with a premium plan
Every atom emits a unique set of energies known as its emission spectrum. Once measured, these spectra allow scientists to identify atoms or molecules based ...
Typology: Lecture notes
1 / 9
This page cannot be seen from the preview
Don't miss anything!






Introduction When an atom is excited it eventually falls back to its ground state, releasing the extra energy as photons. Since the energy of these photons directly corresponds to the gap between different energy levels in the atom, we can study the energy structure of the atom by measuring the wavelengths of these photons. Every atom emits a unique set of energies known as its emission spectrum. Once measured, these spectra allow scientists to identify atoms or molecules based purely on the light they emit: a technique known as spectroscopy. This technique allows us to investigate the material composition of objects ranging from very small samples to distant stars. In this lab you will use a diffraction based spectrometer to measure the emission spectrum of hydrogen and use the Rydberg formula to match each line in the spectrum with an atomic transition. You will then use the spectrometer to identify three different elements enclosed in electric discharge tubes.
The Bohr model coupled with the photon theory of light accurately describes the spectrum of hydrogen. We only need classical mechanics and Bohrโs assumption that angular momentum is quantized according to ๐ฟ = ๐โ, where โ = ! !! is the reduced Planckโs constant and^ n^ is an integer. In the Bohr model of the hydrogen atom, the electron orbits the proton in a fixed, perfectly circular orbit. We start with Coulombโs law, which gives the magnitude of the force of the proton on the electron: ๐น =
where ๐ = ! !!!!^ is Coulombโs constant,^ r^ is the distance of the electron from the proton, and^ e^ is the charge on the electron. In order for the electron to maintain a circular orbit, as assumed, the proton must exert a force of magnitude ๐!๐ฃ! ๐ where ๐! is the mass of the electron and v is the velocity of the electron. Equating these forces yields ๐น =
Now we can substitute in Planckโs quantization assumption. Note that
Diffraction Grating The spectrophotometer uses a diffraction grating to separate the component wavelengths of incident light. As we saw in the diffraction lab, a diffraction grating with line separation d will yield a pattern with maxima at angles ฮธ from the normal for ๐ ๐๐๐๐ = ๐๐, ๐ = ( 0 , 1 , 2 , 3 โฆ ) Measuring the peak positions of a known spectrum allows the separation d to be calculated precisely. This relation can then be used to find the wavelengths in unknown spectra.
Setup