Transcript 10-102 Spectral Lines A few introductory words of explanation about this transcript. This transcript includes the words sent to the narrator for inclusion in the latest version of the associated video. Occasionally, the narrator changes a few words on the fly in order to improve the flow. It is written in a manner that suggests to the narrator where emphasis and pauses might go, so it is not intended to be grammatically correct. The Scene numbers are left in this transcript although they are not necessarily observable by watching the video. There will also be occasional passages in blue that are NOT in the video but that might be useful corollary information. There may be occasional figures that suggest what might be on the screen at that time. 410 Excited States Electrons occupying the energy shells in an atom take the form of a cloud surrounding the much smaller nucleus. Since only two electrons can fit into each of the energy shells, it is interesting to look at the characteristics of these different shells or energy states. These states are defined first by a primary quantum number called “n” and also by a secondary quantum number called “l”. And for each state, the electron has a different energy, which results from the shape of the electron cloud. For n=1, called the ground state, the shape is a symmetric cloud…the same in all directions. For n=2, the shape can take on two forms depending on the value of “l” …although both shapes have the same energy… One shape is a double spherical cloud – one sphere inside the other. While the other shape for n=2 is in the shape of a dumbbell. For other values of n and l, the shapes can be pretty strange… Like this torus PLUS dumbbell shape. From 5-415 Spectral Lines An electron in the lowest energy shell in an atom can be struck by and absorb the energy of a photon giving it enough energy to jump to the next energy shell. And the reverse process allows the electron to jump back down into the lowest energy shell and emit a photon. The color of the photon depends on the energy difference between the two shells. This explains the spectral lines that identify an element. Since white light contains all the colors in the spectrum, when we shine white light on a sample of an element under the right conditions, The atoms absorb all of the photons that allow their electrons to jump to other energy shells. SO the absorption spectrum is all the colors in white light minus those that match the difference in energy shells within the atom. And when those electrons spontaneously jump back down to the lowest energy levels, that emission spectrum contains only those lines that match the difference in energy shells within the atom. Hydrogen Spectra Here is a piece of the spectra from hydrogen. The primary quantum number n is shown on the right alongside the line representing that energy level. When an electron jumps from the n=3 shell to the n=2 shell, red light is emitted When an electron jumps from the n=4 shell to the n=2 shell, aqua light is emitted When an electron jumps from the n=5 shell to the n=2 shell, blue light is emitted When an electron jumps from the n=6 shell to the n=2 shell, violet light is emitted When an electron jumps from the n=7 shell to the n=2 shell, ultraviolet light is emitted No jumps to n=1 are shown because they are all in the deep ultra-violet.