Spectroscopy Lab Report

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Feb 20, 2024

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5 Spectroscopy Lab Report Rowan Paulsen Lab Section 099 13 October 2022
6 Introduction The purpose of this experiment is to use a spectrometer to view the emission spectra of different sources. A spectrometer contains a prism which separates light from a particular element into its constituent wavelengths. These wavelengths are indicated as bright lines on a dark background, known as an emission spectra. We will also use Bohr’s model of the atom to determine the energy level of an electron in a hydrogen atom. Bohr’s model of the atom states that electrons will always orbit around the nucleus in fixed, quantized energy levels. An electron in the ground state of a hydrogen atom will occupy n=1, the energy level closest to the nucleus, because electrons are attracted to protons. If this electron happens to absorb energy, it can become excited and move up energy levels, further from the nucleus. The excited electron has a lot of potential energy, so it naturally moves to a more relaxed state with less potential energy. This movement to a relaxed state results in the emission of a photon. When an electron lands in n=2, visible light is produced which can be seen by the naked eye. This model works perfectly for hydrogen as it only has one electron, but it will not work for elements with more than one electron. For this reason, we will find the initial energy level of the electrons in the hydrogen atom, but not in the other sources. We will be measuring the visible light emitted from hydrogen, fluorescent light, neon, mercury, helium, incandescent bulbs, and sunlight. Because incandescent bulbs and sunlight produce white light, their light spectrum is continuous. It contains light of all wavelengths. The other substances emit specific, discrete lines known as a line spectrum. For hydrogen, we will be calculating the energy of the photon and the initial energy level. To calculate E photon , we will use E photon = hc/ λ. To calculate the initial energy level we will use these two equations: - ΔE electron (released) = E photon (absorbed) and -ΔE = -R(1/n f 2 – 1/n i 2 ) w here R =
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7 2.18 E -18J, c = 3 E 8m/s, and h = 6.626 E -34. It is important to note that n f will always equal 2 because we are dealing with visible light which is only emitted at n=2. For the other sources, we will calculate energy of the photon and frequency. Photon energy will be found using the equation listed above, and frequency will be found using v=c/ λ. Calculations and Discussion 1. Line Spectrum a. Hydrogen Color Wavelength (nm) Energy (photon) n (initial) Red 650nm 3.06E-19J n = 3 Orange 590nm 3.37E-19J n = 3 According to Figure 2.12 of Chemistry : Structure and Properties, Second Edition by Nivaldo J. Tro, the energy level corresponding to the red wavelength is correct. An electron that was excited to n=3, then relaxed to n=2 would emit a photon of red light with a wavelength of 657nm. This is very close to our recorded value of 650nm. However, my partner and I did not record any blue-violet or blue-green light as indicated by the figure. b. Florescent Light Color Wavelength (nm) Frequency (Hz) Energy (photon) Red 610nm 4.92E14Hz 3.26E-19J Green 540nm 5.56E14Hz 3.68E-19J Blue 440nm 6.82E14Hz 4.52E-19J
8 c. Neon Color Wavelength (nm) Frequency (Hz) Energy (photon) Red 640nm 4.69E14Hz 3.11E-19J Orange 600nm 5E14Hz 3.31E-19J d. Mercury Color Wavelength (nm) Frequency (Hz) Energy (photon) Green 550nm 5.45E14Hz 3.61E-19J Blue 440nm 6.81E14Hz 4.52E-19J e. Helium Color Wavelength (nm) Frequency (Hz) Energy (photon) Red 660nm 4.54E14Hz 3.01E-19J Yellow - Orange 580nm 5.17E14Hz 3.43E-19J Green 500nm 6E14 3.98E-19J Blue 450nm 6.67E14Hz 4.42E-19J 2. Continuous Spectrum a. Incandescent Bulb Color Wavelength (nm) Frequency (Hz) Energy (photon) Blue 450nm 6.67E14Hz 4.42E-19J Orange 590nm 5.08E14Hz 3.37E-19J
9 Green 520nm 5.77E14Hz 3.82E-19J Red 640nm 4.69E14Hz 3.11E-19J b. Sunlight Color Wavelength (nm) Frequency (Hz) Energy (photon) Green 540nm 5.56E14Hz 3.68E-19J Blue 450nm 6.67E14Hz 4.42E-19J Orange 600nm 5E14Hz 3.31E-19J Red 620nm 4.84E14Hz 3.21E-19J The measurements for continuous spectra are supposed to be in ranges, but my partner and I recorded the midpoint of a band of colors rather than the beginning and end of each band. For this reason, the frequency and energy measurements are given as fixed points rather than a range. Example of energy calculation: Example of energy level calculation:
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10 Example of frequency calculation: Conclusion The purpose of this experiment was to learn how to record the wavelengths of a given light source and use those values to determine frequency, energy level, and the energy of the photon emitted. My findings were somewhat supported by the expected, theoretical results. The reason some of my data differed from previous scientific evidence is because of inaccurate measurements. When aiming the spectrometer at a light source, we may have been slightly off and therefore unable to record certain photons. We also may have had a slightly uncalibrated spectrometer. However, the wavelengths we were able to record correspond to the expected results. Ultimately, during this experiment I learned how to use a spectrometer and how it works.
11 I also learned why the Bohr model only works for hydrogen and that wavelength and frequency are inversely proportional.