Accession No

1121


Brief Description

table spectroscope, Browning’s ‘Students Spectroscope’, by John Browning, English, c. 1890


Origin

England; London; 63 Strand


Maker

Browning, John


Class

optical


Earliest Date

1890


Latest Date

1890


Inscription Date


Material

metal (brass, oxidised brass); glass; wood


Dimensions

length 780mm; breadth 218mm; height 320mm


Special Collection


Provenance

Gift in 12/1951.


Inscription

‘John Browning,
63 Strand, London’


Description Notes

Table spectroscope, Browning’s ‘Students Spectroscope’, by John Browning, English, c. 1890.

Brass table spectrometer - Browning’s ‘Students Spectroscope’ - part oxidised brass. Slit, brass jaws, width adjustable by knurled screw, reflecting prism on pivoted arm. Slit cover. Slit mount screws on to brass draw tube. Brass collimator tube with threaded joint in centre, screws into mount on stand, screw-in lens at prism end. Trunkated prism in brass mount held on tripod platform by arm and clamping screw. Circular stage, part divided -5-115 by 1˚, subdivided to 20’ on brass. Mount for telescope pivots about centre of stage with vernier and clamp. Screw-in telescope with screw-in objective, threaded central joint, 2 draw tubes and screw-in eye-end consisting of 2 threaded adaptors, single draw tube with lens and screw-in eyepiece lens. Brass pillar stand with flat tripod base and 3 brass feet secured to wooden base.
Cf. 1852 (and file).


References


Events

Description
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:44815

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