Accession No

1611


Brief Description

sextant, by Dollond, English, 1850 (c)


Origin

England; London


Maker

Dollond


Class

navigation


Earliest Date

1850


Latest Date

1850


Inscription Date


Material

wood (ebony, mahogany, other); metal (brass); glass; ivory


Dimensions

box length 336mm; breadth 380mm; height 125mm


Special Collection


Provenance

On loan from Trinity Hall, University of Cambridge from 16/03/1972.


Inscription

‘Dollond London’


Description Notes

Sextant, by Dollond, English, 1850 (c).

Ebony frame sextant, with brass fittings. Adjustable index mirror with four shades. Horizon glass adjustable to plane of frame by knurled screw, and lever adjustment of zero moved by second knurled screw, with 3 shades. Knurled screw for lateral movement of telescope mount (missing). Telescope missing. Reinforced brass index arm, with subsidiary arm for reading glass (missing), type-B ivory vernier, clamp and tangent screws. Ivory scale divided -2-139 by 1˚, subdivided to 20’. Ivory nameplate (unmarked). Wooden handle fixed in brass mount. Three brass feet. Keystone mahogany box.


References


Events

Description
All sextants measure the angle between two distant objects. The navigator usually needs to measure the height of the sun, moon or some star above the horizon. The telescope faces the clear portion of a small half-silvered glass (the horizon mirror), while a mirror is fixed to the rotatable index arm. The star or other object is sighted through the telescope while adjusting the index arm until the direct image coincides with the same image reflected on the index mirror and then on the silvered portion of the horizon glass. The index arm is clamped on the arc, and the bearing of the object is then read off on the graduated scale of 60°, with the aid of the vernier. By this double reflection, angles of up to 120° may be measured.

When measuring the sun’s altitude, in order to calculate their latitude, the observer needs to look directly at the sun, which is harmful to the eyes. Tinted glass shades can be positioned between the telescope and the horizon mirror, to reduce the sun’s power.
04/08/2008
Created by: Dr Anita McConnell on 04/08/2008


FM:42767

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