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TE Activity: Building a Fancy Spectrograph Contributed by: Laboratory for Atmospheric and Space Physics (LASP), University of Colorado at Boulder
Pre-Req Knowledge (Return to Contents) Students should have some understanding of the nature of light (i.e., rainbows are formed with light, light can be different colors, light can be obscured by physical objects, burning creates light, etc.). Students should also be able to work with sharp cutting utensils and rulers. Learning Objectives (Return to Contents) After this activity, students should be able to:
Materials List (Return to Contents) Each group needs:
To share with the entire class:
Notes on materials: Ask students to bring oatmeal containers from home. Purchase holographic diffraction gratings in sheets or on card-mounted slides (2006 prices) from: Edmund Scientifics: http://scientificsonline.com/search.asp?t=ss&ss=diffraction+grating&x=0&y=0 A set of 2 12" x 6" sheets with 12,700 grooves/in for $8 A set of 15 2" x 2" card mounted slides with 12,700 grooves/in for $10 A set of 80 2" x 2" card mounted slides with 12,700 grooves/in for $40 Rainbow Symphony Store: http://store.rainbowsymphonystore.com A set of 10 12" x 6" linear sheets with 500 line/mm for $25 A set of 50 2" x 2" linear calibrated card mounted slides with 500 line/mm for $20 A set of 100 2" x 2" linear calibrated card mounted slides with 500 line/mm for $35 For Introduction/Motivation Section (optional):
Introduction/Motivation (Return to Contents) (Set up a prism, and have a slide projector pointing through the prism such that a rainbow is created. If a prism and slide projector are not available, use a rainbow as an example of light being diffracted by droplets in the clouds.) A diffraction grating is a special tool that acts like a prism, and a spectrograph is a special tool that allows you to channel light to your eyes. Pure white light is made up of a rainbow of colors that cannot be seen with your eyes. A rainbow is called diffracted light. Light is diffracted (or bent) by the water droplets in the air. A prism does the same thing to light from the projector. Some colors of light bend more than others, and the amount that they bend causes them to line up like a rainbow when they are diffracted. A holographic diffraction grating, like the kind we are going to use today, bends the light just like a prism or water droplets. Today, we will create a spectrograph, which is a special tool that uses a diffraction grating. This allows you to see things that you cannot see with just your eyes. Your job is to explore light with this new tool just like a scientist, and test your new tool, just like an engineer. Engineers have created different types of spectrographs to help answer questions that arise in astronomy. They test the spectrographs to see how well spectral lines can be seen. When you are building your spectrograph, think about the different factors that go into building it that may affect its accuracy. Vocabulary/Definitions (Return to Contents)
Procedure (Return to Contents) Background See also: Procedure-Background section from the "Graphing a Rainbow" activity. When photons pass through a gas, they encounter atoms and molecules. The photons hit the atoms and molecules, and produce new photons. When we see this light (these photons) through a spectrograph, we see a pattern of light and dark bands called a spectrum. If the gas that we are looking at is a hot gas, we see an emission spectrum (bright bands on a dark background). If the gas is cool, we see an absorption spectrum (dark bands on a bright background). If two gasses contain the same material and one is hot and the other cool, the hot gas produces bright lines in the exact same places that the cool gas produces dark lines. Where the lines are, whether they are dark or bright, only depends on the material inside the gas. This makes it relatively easy to tell what material is inside of a gas. The light sources that the students look at in this activity are emission spectra EXCEPT for the Sun's spectrum. The solar spectrum is an absorption spectrum because the "atmosphere" is cooler than the source of the Sun's light. Also, a few absorption lines in the solar spectrum are actually from Earth's atmosphere, which you cannot avoid while on Earth. Before the Activity
With the Students
Attachments (Return to Contents)
Safety Issues (Return to Contents)
Troubleshooting Tips (Return to Contents) Colorblind and vision-impaired children will have difficulty with portions of this lab. Students with corrective lenses will not have difficulty. Colorblind students can be paired with a student to assist them with the activity and homework. Students may need assistance adjusting the position of the grating so that a continuous spectrum appears. The lid must be rotated if a continuous spectrum is not visible. Also, the slit should be visible through the grating. The slit should not have any light leaking from the taped portion around it, or the spectrograph will not work properly. Make sure the index card is taped down so that the slit is perfectly straight, and that students have used the "manufactured" edge of the card, not the cut edge. Students may be confused when they see two spectra through the slit. The diffraction grating produces two spectra, and both are a complete spectrum of the source. Make sure the students choose one or the other, but not both, to draw in the activity and on the homework. The spectrum of the Sun is very faint through the diffraction grating. It should appear as thin, faint lines on top of the continuous spectrum. If it is cloudy, students will not be able to see the spectrum. Do not expect students to draw the lines exactly, but they should be able to see the very faint spectrum if they are looking carefully. An example appears here:
Assessment (Return to Contents) Pre-Lesson Assessment Brainstorming: Ask students what they believe causes rainbows to form. Post-Introduction Assessment Class Discussion: Ask students if they are familiar with any light that cannot be seen with the naked eye. Accept many answers. Ask if they know of any animals that see differently than humans (for example, snakes, bats, dogs). Post-Activity Assessment Engineering Communication Homework: Take students outside with their spectrographs, colored pencils, and homework page to look at the spectrum of the Sun. They can fill it in as their first light source. Never have students look directly at the Sun! Follow the instructions on the homework page to see the Sun's spectrum. Make sure students do not block the paper with their shadows. Upon returning to the class, emphasize that engineers share information through dialogue, conferences and written papers. Tell students that the way engineers get new ideas is through sharing with peers. Advise students to open their notebooks or engineering journals and write down something they did, discovered or wondered about during the lab. They can use the questions as a guide, or come up with their own statements. Give them a few minutes to write, and then ask for volunteers to share. If no one volunteers, choose a student to share. After the student finishes talking, allow other students to comment (respectfully). When the students finish the discussion, highlight key ideas on the board. Some ideas may be incorrect, but are still worthy of discussion. Be wary of labeling an answer "right" or "wrong" but rather have students demonstrate or discuss why something does or does not make sense. Ask students to write about the activity and what they learned in their journals. Note: After students complete the homework, call attention to the fact that the same light sources produce the same spectrum. Tie this to the "Patterns and Fingerprints" and "Graphing the Rainbow" activities. Also, note that streetlights that appear blue or whitish-blue to the naked eye are filled with mercury vapor, and streetlights that appear yellow are filled with sodium vapor, thus they have emission bands unique to the substance with which they are filled. Activity Extensions (Return to Contents) Complete the "Using a Fancy Spectrograph" activity. References (Return to Contents) Doherty, Paul, Rathjen, Don. Exploratorium Science Snacks. 1995/2006. Exploratorium: The Museum of Science, Art and Human Perception. 09/2006. http://www.exploratorium.edu/snacks/spectra.html Fisher, Diane. "Taking Apart the Light." "The Technology Teacher." March 2002. Contributors Laboratory for Atmospheric and Space Physics, University of Colorado at BoulderCopyright © 2007 by Regents of the University of Colorado.Supporting Program (Return to Contents) Laboratory for Atmospheric and Space Physics (LASP), University of Colorado at BoulderLast Modified: May 10, 2010
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