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Silbermann-type heliostat
Silbermann-type heliostat

Silbermann-type heliostat

Datecirca 1885
Inventory Number1997-1-1587
ClassificationHeliostat
Subject
    Maker Paul Garnier 1801 - 1869
    Cultural Region
      Place of Origin
        Dimensions48.6 x 32 x 28 cm (19 1/8 x 12 5/8 x 11 in.)
        Material
          DescriptionThis is a later version of a heliostat originally devised around 1843 by French physicist Johann Theobald Silbermann (1806-1865).

          The device consists of a mercury-amalgam glass mirror with an elongated octagonal shape. The mirror is supported by an adjustable brass and steel frame consisting of a semicircular fork whose axis is attached to clockwork in a metal drum.

          The angle of the mirror can be adjusted for solar declination, which is marked in initials of the months every 5 days on one half of the fork. There exists a spot aperture and target for fine adjustment on this declination arm. There are three knurled adjustment screws to alter the azimuth and altitude of the mirror. The azimuth is clock driven and marked on a plate below the mirror with French names for the cardinal directions.

          The main axis of the instrument goes through a cross-piece, which runs between two legs. Its angle is adjustable for latitude using a quadrant, which is divided into 30' intervals, with a vernier scale on one leg giving 1' divisions. There is a knurled tightening screw.

          The other leg is marked with a Radcliffe inventory number: RAD-0.

          The two legs are supported on a turntable on a base with three leveling screw feet. The turntable has a bubble level. Its limb is divided 10-0-10 every 1. The clock drum has two silvered dials. Both read 0-60 every 1. A blued needle pointer turns to "A" and "M." Another blued needle marks slow adjustments between
          "R" and "A." There is purplish varnish on the side of the drum.

          The heliostat is signed by Jules Deuboscq & Philibert Pellin. The clock work is signed by Paul Garnier.
          Signedon body: Mon Jules Duboscq / Ph. Pellin / Paris clock movement: PAUL GARNIER / PARIS / 17846
          FunctionThe heliostat is designed to reflect a beam of sunlight in a fixed direction, and uses a clockwork driven mirror to counteract the apparent motion of the sun through the sky. The resulting steady beam of sunlight would often be projected into a laboratory for experiments requiring intense light, physical optics studies, microscopy, analysis of the solar spectrum, etc.

          For more information on how this type of heliostat worked, see the following website (in French).
          Historical AttributesInstrument came from the Optics Lab in Byerly Hall, Radcliffe on 13 October 1964. The "RAD-O" markings most likely stand for "Radcliffe-Optics" and are found on many other instruments in CHSI.
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