Before we begin some points of safety must be noted:
First and foremost your safety comes first and then the equipments'
Be careful when handling the Mercury Vapor Bulb (in case you need to) and all glass tubing
Check the cords, cables, and machinery in use for any damage or possible electrocution points on fuses of machinery by making sure the power cords' protective grounding conductor must be connected to ground
Make sure the areas containing and around the experiment are clear of obstacles
Purpose
The purpose of this lab is to observe and classify spectra lines of the hydrogen and deuterium atoms. By using electrical stimulation to excite the atoms to higher energy levels we can measure the emitted photons of wavelengths equivalent to the energy of our excited electrons. Through this lab and our measurements we should also be able to experimentally determine Rydberg's constant, R, that is used in the Hydrogen Spectrum equation:
This process will be applied to both hydrogen vapor and deuterium vapor.
Brief Description of Balmer Series
The Balmer series is one of six series in which the spectral line emissions of hydrogen are designated. There are four different emission wavelengths of visible light by which the hydrogen spectrum is defined. These wavelengths can be calculated using the Balmer formula (found by Johann Balmer, 1885) written above in the "Purpose" and reflect emissions of photons by transitions of electrons between principal quantum number levels from [math]\displaystyle{ n\geq 3 }[/math] to [math]\displaystyle{ n=2\,\! }[/math].
[1]
Brief Description of Deuterium
Compared to the Hydrogen atom, which contains one proton in the nucleus, the Deuterium atom, contains a proton and a neutron in its nucleus. Thus the Deuterium atom is heavier than the regular Hydrogen atom.
First we adjusted the spectrometer, bringing the cross-hairs into focus by sliding the ocular to suit our vision
Then we brought the slit into focus, turning the large ring near the center of the viewing telescope making sure to turn the screw in only one direction to avoid error due to "gear back lash"
Next, we attached the mercury bulb and turned on the mercury tube power supply to let it warm up
Using the spectrometer with a wide slit, we found a line of the mercury spectrum and then narrowed the slit until the line became narrow and sharp
Then we located as many mercury spectra as we could and noted the orientation and value of our spectrometer dial
While using the wavelengths of light given in Gold's Manual (page 29), we finished calibrating the system
To solve for Rydberg's constant we correlated our data to the appropriate quantum numbers and used the equation given (page 30)
Finally, we repeated this process for deuterium as well.
Note: The first two steps are to make certain that no parallax exists between the cross-hairs and the slit when in sharp focus
This is our raw data:
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Using our raw data tables we used the functions in Excel for mean and standard deviation to find the standard error margins. From that we formulated a total mean:
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SJK 12:28, 24 October 2009 (EDT)
Calculations
According to page 30 of Gold's manual [3], the present-day accepted value Rydberg's constant is calculated as:
The [math]\displaystyle{ \pm 0.0025\,\! }[/math] and [math]\displaystyle{ \pm 0.0007\,\! }[/math] come from the SEM of the values that we used to calculate the mean.
Notes About Uncertainty
The lab lasted over two days, with a week interval. During that interval another group had used the same device that we were using for ours, so re-calibration for our set of data was necessary during the second day.
As for using the 'scope, we took care to avoid gear back lash by turning the knob all the way back before remeasuring spectra for each trial.