Chemical Science Lesson Plan

Title: Cellphone Spectrometer

Grade Level: High School

Prepared by: Alex Scheeline
Science standards

Science background for teachers

Activity procedure

Materials

Summary and discussion


Objectives: Students will learn about light and the interaction of light with matter. They will build a spectrometer using a cellphone camera and inexpensive supplies, and use it as a measuring device for an inquiry-based experiment.

Science standards

11.A.5b Design procedures to test the selected hypotheses

11.A.3f Interpret and represent results of analysis to produce findings.

12.C.3a Explain interactions of energy with matter including changes of state and conservation of mass and energy.

Science background for teachers

Theoretical Background for the Camera Spectrophotometer

Electromagnetic radiation

Electromagnetic radiation (EMR) is the type of energy that encompasses light, heat, and x-rays. It can be conveniently described using a sinusoidal wave model, where the properties of the radiation depend on the wavelength, frequency, and other parameters of the wave. For some purposes, usually when discussing the absorption and transmittance of the energy of the radiation, it makes more sense to describe the energy as a stream of light particles called photons, where the energy of the photons is proportional to the frequency of the radiation. The wave/particle duality applies to all elementary particles, and should be used as a complementary, rather than contradictory, description of the movement of the radiation.

Wave properties of electromagnetic radiation:
  • Amplitude (A): The height of the wave

  • Wavelength (λ): The distance between two crests of the wave

  • Crest and trough: The highest and lowest points, respectively, of a wave

  • Speed of light ( c ): The velocity of radiation as it travels through a vacuum. This quantity is the same for all forms of electromagnetic radiation, from x-rays to light to radio waves, and is constant within a particular transportation medium.The speed of light in vacuum is 2.99792 x 108 m/s. The speed of light in air is only 0.03% slower, and c in either medium is usually just rounded off to 3.00 x 108 m/s.

  • Frequency (ν): The number of waves that pass a fixed point per second

  • Period (T): The number of seconds it takes for a wave to pass a fixed point




  • ν = 1/T - The frequency of the wave is the reciprocal of the period.

  • λ ν = c (or ν = c/λ) - the product of frequency and wavelength is the speed of light. Alternatively, the frequency of a wave is inversely proportional to the velocity.

  • E = hν = hc/λ , where h is the Planck constant, 6.626 x 10-34 - The energy of the radiation is equal to the Plank constant multiplied by the frequency of the radiation.

The Electromagnetic Spectrum

Although all waves of electromagnetic radiation travel at the speed of light, different types of waves have vastly differing wavelengths, frequencies, and energies. The shorter the wavelength of the radiation, the greater the frequency and the larger the energy. The electromagnetic spectrum ranges from gamma (γ) radiation, which has the shortest wavelength, highest frequency, and greatest energy, to radio waves, which has the longest wavelength and lowest frequency and energy.


Movement of light between two substances

When light moves between two substances, both the speed and the direction of the electromagnetic wave will change. The refractive index, n, is given by the equation

n=c/vp

where c is the speed of light in vacuum and vp is the speed of light in that particular substance. The refractive index is unitless and simply provides a means to compare the relative speeds of light in transparent substances; the larger the refractive index of a material, the slower light will pass through it.

When the wave of light changes velocity, it also changes direction. This refraction can be related to the speeds of light in the substances using Snell's Law, where θ1 is the angle of incidence, θ2 is the angle of reflection, and v1 and v2 are the speeds of light in the first and second media, respectively.



In vacuum all types of radiation are refracted equally, but in other media the refractive index is related to the wavelength of the light. Because of this, light of different wavelengths is refracted to different degrees. This phenomenon is known as dispersion.

Dispersion of White Light in Gratings

White light is a mixture of all of the wavelengths of visible light. When a beam of white light is sent from one medium to another, the different wavelengths of light that make up the beam are refracted at different angles because they are traveling at different speeds and have different refractive indexes. This causes the different wavelengths to be separated from each other into the visible spectrum as shown at right.

Light can be separated using either prisms or diffraction gratings.

A transmission diffraction grating is made up of a transparent material with regularly spaced grooves cut into it so that a beam of light passing through is separated out into the component wavelengths.

The separation of the light is governed by the equation:

nλ = d(sin i + sin r)

where n is the diffraction order (a small whole number), d is the spacing between the grooves of the grating (usually calculated in nanometers/groove), and i and r are the angles of incidence and refraction, respectively.

Because there are several values for 'n', there are a number of spectra, found at different angles of refraction, which can be formed from a diffraction grating. Ordinarily, however, the first-order line is the most intense, and only the +1, 0, and -1 spectra can be seen.

Spectrophotometers

Spectrophotometers are instruments that measure the absorbance of wavelengths of light in solutions. The absorbance, A of a solution is a measure of how much light of a certain wavelength specific to the experiment passes through a solution versus how much is absorbed by the solution. Absorbance is defined using the Beer's Law



where I0 is the amount of the experimental wavelength of light present before the beam of light passes through the solution, and I is the amount of light present in the beam after it has passed through the solution. In general, the darker the solution, the less light that passes through the solution and the higher the absorbance.

Using our spectrophotometer, the students will be able to see which wavelengths of light in the visible spectrum are absorbed and which are transmitted. A deep red transparent solution, for example, allows red and orange light to pass through and absorbs the other colors in the spectrum. A pale red solution absorbs some of the blue and green light, but also lets some through, and a clear solution transmits the entire visible spectrum. This can be clearly seen in the diffracted spectrum through the grating.

Materials

  • A small white LED light bulb. Suggested: a Ultra-White LED 5mm
  • A power source for the light bulb. Suggested: a 3-V coin battery
  • A small visible-light grating. Suggested: A 500 line/mm linear diffraction grating, such as those sold at http://www.rainbowsymphonystore.com/difgratslidl1.html
  • A sample of colored liquid; primary colors give easily interpreted results. Suggested: Red Kool-aid, food coloring, or similar substance.
  • A cuvette (something to hold the liquid in). Suggested: A standard glass vial
  • A way to keep the light, cuvette, and grating stationary. Suggested: A piece of Styrofoam.
  • A camera


  • Activity procedure

    1. Read the general descriptions concerning measurement, precision, and accuracy on the website.

    2. Read the manuscript on the operation of the "Cell Phone Spectrometer" to the point where it turns into gobbledygook. Then look at the Figures. Make a note of where you stopped reading. The purpose of this note is to calibrate the author on where the class is.

    3. Read the lab instructions on the "Cell Phone Spectrometer."

    4. Bring either a digital camera or your cell phone (with camera) to class.

    5. If you have a Windows laptop, go to http://www.asdlib.org/onlineArticles/elabware/Scheeline_Kelly_Spectrophotometer/index.html and download the Executable Software. If you'd like real data on which to practice, a .zip file with raw .JPG data is available on the course website.


    Summary and discussion

    Answer the questions in this QuickQuiz:
    1. The idea of using a cell phone to collect science data is:
        a) A good way to engage students
        b) Violates the rules in my classroom
        c) Potentially puts analytical measurements in the hands of every citizen
        d) All of the above
        e) Additional comments, choices, or reactions include:

    2. In 2003, a white, powdery substance was found on the floor at the rear of an airplane that had just landed in Burlington, VT. The plane was impounded and treated as if it were a courier for drugs.
        a) When one sees an unknown white powder, it might be cocaine. Good call.
        b) It was probably artificial sweetener; impoundment is obvious overreaction.
        c) Without testing the chemical composition of the powder, it is hard to know what should have been done.
        d) Just mop up the mess and ignore what's going on.

    3. The Cell Phone Spectrometer paper has:
        a) Equations beyond what any high school student can relate to.
        b) Too little math to explain what is really going on.
        c) A good example of the relationship among algebra, trigonometry, chemistry, and optics.

      We will discuss the questions, but please turn in answers at the beginning of class. The preferred answer to the questions is not to actually answer them – it is to pose related questions that are better targeted at the real problems you face in the classroom!
EnLIST Chemistry Workshop, University of Illinois, 2010