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In this physics lab, students use boston university's emission spectra lab simulation to explore atomic transitions using the bohr model. The lab involves observing emission spectra for various elements, including hydrogen, helium, lithium, sodium, and mercury, and determining the energy levels (n) involved in each transition using the rydberg formula for the balmer series.
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In this lab you are using Boston University’s Emission Spectra Lab simulation: http://physics.bu.edu/~duffy/HTML5/emission_spectra.html Procedure First, a bit of background information. In the atom of each element, an electron (or electrons) can transition from one energy level to another by absorption of photons or emission of photons. To get a clearer picture of this phenomenon, we will use the simplified but not wholly accurate Bohr model of the atom. Here electrons orbit the nucleus at fixed select energy levels with higher energy level orbits or shells being positioned farther away from the (center) nucleus. Figure 1. Bohr model atom: Electron absorbs photon energy – promoted to higher level, electron emits photon energy – falls to a lower level When an electron moves from a higher energy level to a lower energy level it releases a photon with energy equivalent to the difference between these two levels in the atom. In figure 2, illustration shows there are three different series which are associated with electron transition emissions.
Figure 2. Spectral Series and associated wavelengths. Figures 3 and 4. Electron energy level transitions in atom with energy graph