The kaleidoscope : $b its history, theory and construction. With its application to the fine and useful artsBrewster, David
Science
The kaleidoscope : $b its history, theory and construction. With its application to the fine and useful arts
Brewster, David
Kaleidoscopes
If the plates of glass have been skilfully cut with the diamond, so as
to have their edges perfectly straight, and free from chips, two of
the edges may be placed together, as in Fig. 17 (p. 49), or one edge
of one plate may be placed against the surface of the other plate, as
shown in the section of Mr. Bates’s Kaleidoscope. But if the edges are
rough and uneven, one of them may be made quite straight, and freed
from all imperfections, by grinding it upon a flat surface, with very
fine emery, or with the powder scraped from a hone. When the two plates
are laid together, so as to form a perfect junction, they are then to
be placed in a brass or any other tube, so as to form an angle of 45°,
36°, 30°, or any even aliquot part of a circle. In order to do this
with perfect accuracy, direct the tube containing the reflectors to
any line, such as _m n_, Fig. 2, placed very obliquely to one of the
reflectors =A O=, and open or shut the plates till the figure of a star
is formed, composed of 8, 10, or 12 sectors, or with 4, 5, or 6 points,
corresponding to angles of 45°, 36°, and 30°. When all the points of
the star are equally perfect, and none of the lines which form the
salient and re-entering angles disunited, the reflectors must be fixed
in that position by small arches of brass or wood =A B=, =_a b_=, Fig.
21, filed down till they exactly fit the space between the open ends of
the plates. The plates must then be kept in this position by pieces or
wedges of cork or wood, or any other substance pushed between them and
the tube. The greatest care, however, must be taken that these wedges
press lightly upon the reflectors, for a very slight force is capable
of bending and altering the figure even of very thick plates of glass.
When the reflectors are thus placed in the tube, as in Fig. 21, their
extremities =_a_ E=, =_b_ E=, next the eye, must reach to the very end
of the tube, as it is of the greatest importance that the eye get as
near as possible to the reflectors. The other ends of the reflectors
=A O=, =B O=, must also extend to the other extremity of the tube, in
order that they may be brought into contact with the objects which are
to be applied to the instrument. In using transparent objects the cell
or box which contains them may be screwed into the end of the tube, so
as to reach the ends of the reflectors, if they happen to terminate
within the tube; but an instrument thus constructed is incapable of
being applied to opaque objects, or to transparent objects seen by
reflected light.
[Illustration: FIG. 21.]
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