Atomic Emission Spectra

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Atomic Emission Spectra of H2
Asif Nazerally,
Tashiana L., Monica H-S.
B. C. Boivin
SPH 4U, Grade 12 University Physics, Rockland District High School
Friday, April 19th, 2013
2
Introduction
In this experiment, Niels Bohr’s atomic emission spectroscopy lab will be recreated for
hydrogen gas with the equipment available. Atomic emission
spectroscopy is a way to determine the amount of an element in a
sample of light. The identity of the element is demonstrated by the
wavelength, while the amplitude
determines the number of atoms
Figure 1. A picture
of Niels Bohr
(Simon, 2013).
(Kkmurray, 2013).
Niels Henrik David Bohr (see
Figure 1) received a Nobel Prize for his contributions as a physicist
to the better understanding of quantum mechanics and atomic
Figure 2. Bohr model
of hydrogen atom
(JabberWok, 2007).
structure (Manske, 2013). Bohr created the Bohr model (see Figure 2) which describes that
electrons orbit around the nucleus of an atom, from attraction of electrostatic forces (Knott,
2013).
Max Planck, theoretical physicist and creator of quantum theory, developed Planck’s
constant (6.63x10-34 m2kg/s) which describes (on atomic level) how
particles and waves behave (Hosch, 2006). He created the formula 𝐸 =
Figure 3. Planck’s
equation (Wittke,
2008).
β„Žπ‘£ to determine the energy of a photon (see Figure 3).
The electromagnetic spectrum refers to the range that
encompasses all frequencies of electromagnetic radiation, from radio waves (the weakest) all
the way to gamma rays (the strongest). All but the visible light spectrum (see Figure 4) which
ranges from the colour red (lowest frequency) to the colour violet (highest frequency) is
3
Figure 4. The visible light spectrum (Jones, 2012).
invisible to the naked human eye (Newman, 2013). The empirical values of wavelength being
used in this lab are, in nanometres, 400, 445, 475, and 650, for violet, indigo, teal and red,
respectively (Madigan, 2011).
The purpose of this lab is to measure quanta by reenacting Bohr’s atomic emission
spectroscopy lab using a spectroscope and observing light from a discharge tube.
4
Theory
𝑐 = 𝑓λ
βˆ†πΈ = β„Žπ‘“
Variables
𝑐 – Speed of light constant
βˆ†πΈ – Change in energy
𝑓 – Frequency
β„Ž – Planck’s constant
λ – Wavelength
Materials and Methods
The materials and methods used were that of the SPH4U Physics class on Thursday, April 11,
2013.
Figure 5. Lab setup
(Hendrix-Sicard, 2013).
5
Results and Observations
Table 1. Atomic emission spectra for H2.
Spectral Line
Wavelength
Frequency (Hz)
Colour
(nm)
Violet
440
6.82x1014
Blue
450
6.67x1014
Teal
500
6.00x1014
Red
670
4.48x1014
Calculations
Calculations for Violet
𝑐 = πœ†π‘“
𝑓=
𝑐
πœ†
π‘“π‘£π‘–π‘œπ‘™π‘’π‘‘ =
3.00π‘₯108
4.4π‘₯10−7
π‘“π‘£π‘–π‘œπ‘™π‘’π‘‘ = 6.82π‘₯1014 𝐻𝑧
βˆ†πΈ = ħ𝑓
βˆ†πΈπ‘£π‘–π‘œπ‘™π‘’π‘‘ = 6.63π‘₯10−34 (6.82π‘₯1014 )
βˆ†πΈπ‘£π‘–π‘œπ‘™π‘’π‘‘ = 4.52π‘₯10−19 𝐽
Percentage of Error for Violet
% πΈπ‘Ÿπ‘Ÿπ‘œπ‘Ÿ =
|πΈπ‘šπ‘π‘–π‘Ÿπ‘–π‘π‘Žπ‘™ − π‘€π‘’π‘Žπ‘ π‘’π‘Ÿπ‘’π‘‘|
π‘₯ 100%
πΈπ‘šπ‘π‘–π‘Ÿπ‘–π‘π‘Žπ‘™
% πΈπ‘Ÿπ‘Ÿπ‘œπ‘Ÿ =
|400 − 440|
π‘₯ 100%
400
% πΈπ‘Ÿπ‘Ÿπ‘œπ‘Ÿ = 10.0%
Change in Energy (J)
4.52x10-19
4.42x10-19
3.98x10-19
2.97x10-19
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Discussion
It was determined mathematically that the potential energy was 0.2J for the 50g weight,
0.9J for the 200g weight and 2.5J for the 500g weight. It was then determined experimentally
that the kinetic energy was 0.0756J for the 50g weight, 0.4044J for the 200g weight and 1.0045J
for the 500g weight, after twenty complete swings of the weights. These results appear to be
inaccurate due to the large margin of possible errors, primarily that the pendulum lost a great
deal of momentum and energy due to the instability of the pendulum.
There were many possible sources of errors throughout this experiment. One of them
would be that a lot of the potential energy is being lost through the pendulum. The reason is
because the pendulum being used were quite old, therefore unstable and wobbly, and making
the results of the experiment inaccurate. A possible solution to this would be to perhaps invest
in more modern or reliable equipment or to clamp down the pendulum (but that would still
leave the upright pole unstable).
Another possible source of error would be the energy lost in the string. The string that
the weight was hung from was tied around a metal ring, which was attached to the pendulum.
When one of the heavier weights were used, the string was susceptible to sliding, which would
render the results inaccurate since there is energy being lost. A solution to this issue would be
to tape down or glue down the string to the metal ring.
A third possible source of error could be that the desks that the pendulum stood on
were uneven or crooked, thus making the swinging difficult to go one way and easier to go the
other. To fix this issue, the desk’s legs could have been measured until they were made even.
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All of these possible sources of error could have negatively affected the results of this
experiment.
Conclusion
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Selected References
Anome, T. (2013, April 3). Quantum. Retrieved April 18, 2013, from Wikipedia:
http://en.wikipedia.org/wiki/Quantum
Hendrix-Sicard, M. (2013, April 14). Physics 11/12 2012. Retrieved April 16, 2013, from
Facebook: https://fbcdn-sphotos-d-a.akamaihd.net/hphotos-aksnc7/420934_534585586585237_1503022242_n.jpg
Hosch, W. L. (2006, May 18). Planck's constant. Retrieved April 18, 2013, from Encyclopædia
Britannica: http://www.britannica.com/EBchecked/topic/462917/Plancks-constant
JabberWok. (2007, February 23). File:Bohr-atom-PAR.svg. Retrieved April 18, 2013, from
Wikipedia: http://upload.wikimedia.org/wikipedia/commons/thumb/5/55/Bohr-atomPAR.svg/310px-Bohr-atom-PAR.svg.png
Jones, C. (2012, November 27). Why Artificial Light Feels Wrong, Part 1. Retrieved April 18,
2013, from NextGenLite:
http://nextgenlite.com/images/VisibleLightSpectrumGradientForWeb.jpg
Kkmurray. (2013, February 27). Atomic emission spectroscopy. Retrieved April 18, 2013, from
Wikipedia: http://en.wikipedia.org/wiki/Atomic_emission_spectroscopy
Knott, T. (2013, March 20). Bohr model. Retrieved April 18, 2013, from Wikipedia:
http://en.wikipedia.org/wiki/Bohr_model
Madigan, J. (2011, November 15). What Wavelength Goes With a Color? Retrieved April 18,
2013, from National Aeronautics and Space Administration: http://scienceedu.larc.nasa.gov/EDDOCS/Wavelengths_for_Colors.html
Manske, M. (2013, April 12). Niels Bohr. Retrieved March 18, 2013, from Wikipedia:
http://en.wikipedia.org/wiki/Niels_Bohr
Newman, P. (2013, March 21). Electromagnetic Spectrum. Retrieved April 18, 2013, from
Goddard Space Flight Center:
http://imagine.gsfc.nasa.gov/docs/science/know_l1/emspectrum.html
Simon, A. (2013). Who's talking about Niel? Retrieved April 18, 2013, from Whotalking:
https://lh4.googleusercontent.com/-dKL1Se5jv7I/S3opYzS21uI/AAAAAAAAAXQ/JcQY9Wv81c/s288/Niels%252520Bohr.jpg
Wittke, J. H. (2008). Signals. Retrieved April 18, 2013, from Microanalysis:
http://www4.nau.edu/microanalysis/Microprobe-SEM/Images/Equation01-1.jpg
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