Accession No

2951


Brief Description

diffraction grating, reflecting, Rowland-type, by John A. Brashear, U.S.A., 1888


Origin

U.S.A.; Massachussetts; Baltimore; and U.S.A.; Pennsylvania; Allegheny


Maker

Brashear, John A. [polished and figured] Theodore C. Schneider [ruled using Rowland's engine]


Class

optical


Earliest Date

1888


Latest Date

1888


Inscription Date

1888


Material

metal (speculum metal; brass); wood


Dimensions

plate 161mm x 135mm; ruled surface 146mm x 50mm box length 197mm; breadth 179mm; height 115mm


Special Collection


Provenance

Transferred from Department of Physical Chemistry, University of Cambridge, Cambridge, England, 03/1983.


Inscription

‘Ruled on Prof. H.A. Rowlands Engine 1888
John Hopkins University Baltimore Md USA
Radius of curvature 21 feet + 10,000 lines to in’ (scratched on surface)
‘Plate Polished and Corrected at the Astronomical
and Physical Instrument Works of
John A. Brashear Allegheny Pa U.S.A.’


Description Notes

Diffraction grating, reflecting, Rowland-type, by J. A. Brashear, U.S.A., 1888.

Rectangular speculum metal plate with raised polished platform, containing rectangular ruled surface. Wooden tray with two handles in fitted wooden box. Blank square brass plate.

Manuscript inscription reads:

‘Ruled on Prof. H.A. Rowlands Engine 1888
John Hopkins University Baltimore Md USA
Radius of curvature 21 feet + 10,000 lines to in’ (scratched on surface)
‘Plate Polished and Corrected at the Astronomical
and Physical Instrument Works of
John A. Brashear Allegheny Pa U.S.A.’

Condition


References


Events

Description
Diffraction grating
Grimaldi (an Italian physicist) saw that the edges of shadows are not completely sharp, but have fringes. Only later, in 1785, when multiple edges were placed next to one another to form a grating, was the full importance of this observation elucidated.

A diffraction grating consists of very closely spaced lines on a reflecting surface (the line ruling process must be very precise). The lines disperse light into component wavelengths (much like a prism does) and this is useful for precise determination of the magnitude of wavelengths.

18/10/2002
Created by: Saffron Clackson on 18/10/2002


FM:43460

Images (Click to view full size):