Accession No
2605
Brief Description
spectrometer, by P. Pellin, French, 1890 (c)
Origin
Paris; France
Maker
Pellin, P.
Class
optical
Earliest Date
1890
Latest Date
1890
Inscription Date
Material
metal (oxidised brass, brass, silver)
Dimensions
length 430mm; breadth 275mm; height 402mm
Special Collection
Provenance
Purchased from Alain Brieux, Paris, France, 05/1980.
Inscription
‘Ph. Pellin Paris’
D[?]2 87 [top of tripod]
2 [side of tripod]
Description Notes
Table spectrometer, part oxidised brass. Brass collimator, adjustable slit moved by knurled screw, on draw tube. Inclination of collimator adjustable by knurled screw moving against spring. Collimator mounted on arm, pivoting about centre of stand, with clamping screw. Central circle held by brass spokes, silvered and divided 0-360 by 1˚, subdivided to 30’. Incomplete platform for prism (missing), with three levelling screws; platform rotated by brass arm, with clamp and tangent screws, and silvered vernier reading to 1’. Telescope pivots on brass arm with clamp and tangent screws and vernier reading to 1’. Focussing by rack and pinion moved by knurled screw. Screw-in eyepiece with one draw tube, cross-hairs and side aperture (for illuminating cross-hairs?). Platform screws into pillar stand with draw tube and clamp, on tripod base with 3 levelling screws.
References
Events
Description
Spectroscope
In 1814 Joseph von Fraunhofer noticed that the sun’s spectrum, when dispersed by a glass prism, is crossed by hundreds of fine dark lines. These lines could be used to determine the chemical composition of the sun, stars and many other substances by spectral analysis. The first photograph of the spectrum of a star (Vega) was made by Henry Draper using a spectroscope in 1872.
There are various different forms of spectroscope, but all use a slit and collimator to make a parallel beam of light, a prism for dispersing different wavelengths and a telescope to observe the dispersed spectrum.
18/10/2002
Created by: Saffron Clackson on 18/10/2002
FM:44817
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