Accession No
4433
Brief Description
table spectrometer, by John Browning, English, c. 1880 - 1890
Origin
England; London
Maker
Browning, John
Class
optical
Earliest Date
1880
Latest Date
1890
Inscription Date
Material
metal (brass, silver); glass; wood
Dimensions
box height 450mm; breadth 425mm; depth 377mm
Special Collection
Provenance
Transferred from the Department of Engineering, University of Cambridge.
Inscription
‘John Browning, London.’ (on circular stage)
‘Position of Collmtr for 2 Prisms’ (on stage)
‘Position of Collmtr for 1 Prism’ (on stage)
‘Position of Collmtr for 5 Prisms’ (on stage)
‘Position of Telescope’ (on stage)
Description Notes
Table spectrometer, by John Browning, English, c. 1880 - 1890.
Brass table spectrometer. Brass collimator tube with threaded joint, screws into mount which pivots about centre, with clamp. Brass telescope, rack and pinion focus, with threaded joint, screws into mount with clamp and slow motion screws and vernier. Circular stage with silvered scale, 0-360 degrees subdivided to 10’. Third mount for magnifying glass for vernier (? - magnifying glass missing) moves around scale. Tripod platform with upper platform with mounts for five prisms. Brass pillar stand with flat tripod base and three brass feet secured to wooden base. Comes in a wooden case.
Condition: fair (brass is part-oxidised; rack and pinion on telescope damaged); incomplete (no prisms; eyepieces for telescope and slit for collimator missing).
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:44841
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