Our setup was as shown.
We placed a light source at the origin of the 2 rulers, placed a diffraction grating at a distance from the bulb, and looked through it and measured the range of wavelengths.We use the following formula:
where λ is the wavelength, d is the slit spacing on the diffraction grating, D is the observed horizontal distance from the light source to the band of light, L is the distance from the diffraction grating to the light.
We took readings at 2 distances to minimize error.
L (m) | Red(D) | Violet (D) |
---|---|---|
1.5 | 0.65 | 0.3 |
1.8 | 0.745 | 0.35 |
We were then given a gas discharge tube, and our job was to determine what type of gas was in the tube based on the spectral lines we observe.
We compared the spectral bands with a chart of different gasses' spectral lines, and they corresponded almost perfectly with mercury.
color | D (m) | Measured λ | Theoretical λ |
---|---|---|---|
Red | 0.75 | 690 | 690 |
Yellow | 0.61 | 589 | 580 |
Green | 0.54 | 535 | 545 |
Violet | 0.42 | 439 | 435 |
We plot the measured values against the theoretical values to get a correction value of 75 nm.
We were then given a hydrogen discharge tube, and measured the spectral lines of hydrogen.
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The different spectral lines indicate the different energy levels that the hydrogen can transition between. For each of these transitions, the hydrogen emits a photon corresponding to a specific wavelength. This method can be used to analyze an unknown gas and determine it's composition based on the energy levels.
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