Discussion:
Refer to the discussion on Analytical Spectroscopes for information on how
diffraction gratings produce spectra.
Glass prisms are heavy. The more separation one wants for the wavelengths,
the thicker the glass needs to be. Grading spectroscopes can do the
same job but are much lighter. A diffraction grating can spread out the spectrum
more than a prism can. This ability is called dispersion. Because gratings
are smaller and lighter, they are well suited for spacecraft where size and weight
are important considerations. Most research telescopes have some kind
of grating spectrograph attached. Spectrographs are spectroscopes that provide a record, photographic or digital, of the spectrum observed.
Notes:
- Most science supply houses sell diffraction grating material in sheets or rolls. One
sheet is usually enough for every student in a class to have a piece of grating to
build his or her own spectroscope. Holographic diffraction gratings
work best for this activity.
- Many light sources can be used for this activity, including flourescent and incandescent
lights and spectra tubes with power supplies. Spectra tubes and the power supplies to run
them are expensive. It may be possible to borrow tubes and supplies from another
school if your school does not have them. The advantage of spectrum tubes is that they
provide spectra from different gases such as hydrogen and helium.
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For Further Research:
- Using colored pencils or crayons, make sketches of the spectrum emitted by
different light sources. Try incandescent and flourescent lamps, bug lights, street lights
(mercury, low-pressure sodium, and high-pressure sodium), neon signs, and candle flames. How do these spectra differ?
- How do astronomers measure the spectra of objects in space? What do those
spectra tell us about these objects?
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