concave diffraction grating
Date1920-1940
Inventory Number1998-1-1324
ClassificationDiffraction Grating
Subject
Maker
American
User
Department of Physics, Harvard University
founded 1884
Cultural Region
Dimensionsgrating: 1.5 × 10 × 10 cm (9/16 × 3 15/16 × 3 15/16 in.)
box: 11 × 14.8 × 15.1 cm (4 5/16 × 5 13/16 × 5 15/16 in.)
box: 11 × 14.8 × 15.1 cm (4 5/16 × 5 13/16 × 5 15/16 in.)
Material
DescriptionConcave diffraction grating made of speculum metal. The number of lines per inch and the radius of curvature are unknown. The number "49" has been etched in one corner. The grating is screwed in place in the box.
Signedunsigned
FunctionA diffraction grating is a glass or mirror that has regularly spaced microscopic interruptions to the passage of light (lines) such that light passing through or reflected by it experiences interference phenomena, magnifying its magnitude at some angles and cancelling it at others. As this effect depends on the wavelength of light, a diffraction grating is an effective method of decomposing light into its constituent wavelengths, that will be transmitted at different angles (short wavelengths -- bluer -- are deflected less than longer -- redder -- ones). If one knows the line density (lines per inch) and the angle of deflection (with a spectrometer), one can deduce the exact wavelengths.
Diffraction gratings like this one were often used in astronomy to produce spectra of celestial objects. Begun in 1882, Rowland's gratings were more than an order of magnitude larger and more accurate than any previous one. With these, for instance, it became possible to measure the wavelength of light emitted by atoms to unprecedented accuracy. Rowland himself was able to draw a new and more accurate map of the solar spectrum.
For more information go to the following website.
Diffraction gratings like this one were often used in astronomy to produce spectra of celestial objects. Begun in 1882, Rowland's gratings were more than an order of magnitude larger and more accurate than any previous one. With these, for instance, it became possible to measure the wavelength of light emitted by atoms to unprecedented accuracy. Rowland himself was able to draw a new and more accurate map of the solar spectrum.
For more information go to the following website.
ProvenanceJefferson Laboratory, Department of Physics, Harvard University; transferred to CHSI January 19, 1977.
Adam Hilger Ltd.
Date: circa 1923
Accessories: wooden box
Object number: 2039
Robert W. Wood
Date: circa 1925
Accessories: wooden box
Object number: 2040
Robert W. Wood
Date: 1932
Accessories: wooden case
Object number: 2024
