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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