concave diffraction grating
Date1908-1912
Inventory Number2029
ClassificationDiffraction Grating
Subject
Owner
Theodore Lyman IV
1874 - 1954
User
Frederick Albert Saunders
1875 - 1963
User
Department of Physics, Harvard University
founded 1884
Cultural Region
Place of Origin
Dimensionsdiffraction grating: 6.3 × 6.3 × 1.2 cm (2 1/2 × 2 1/2 × 1/2 in.)
case: 8.3 × 7.8 × 2.4 cm (3 1/4 × 3 1/16 × 15/16 in.)
case: 8.3 × 7.8 × 2.4 cm (3 1/4 × 3 1/16 × 15/16 in.)
Material
Accessorieswooden box
DescriptionConcave diffraction grating made from speculum metal, divided with 31,995 lines per inch and a radius of curvature of 99.3 cm. It is stored in a wooden box (not original).
Signedunsigned
Inscribedhandwritten with a pencil: 152-C-3 / 31995 lines / 5.42 cm / Jan 27 1912 / 1908c / JAA / This refers to one meter grating (FAS) in phys 2b.
Curatorial RemarksThe date suggests that it was made before Saunders arrived at Harvard. It was apparently used for experimental on Balmer lines.
Considering the number of gratings found in the CHSI collection coming from the "Rowland factory" at Johns Hopkins University, this one, unsigned, could also have the same provenance.
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.
ProvenanceFrom the Department of Physics, Lyman Laboratory, Harvard University.
Robert W. Wood
Date: circa 1925
Accessories: wooden box
Object number: 2040
Henry A. Rowland
Date: circa 1884
Accessories: wooden box; key
Object number: 2031
Adam Hilger Ltd.
Date: circa 1923
Accessories: wooden box
Object number: 2039
Robert W. Wood
Date: 1928
Accessories: wooden box
Object number: 2022
Robert W. Wood
Date: 1932
Accessories: wooden case
Object number: 2024
