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
Upon these principles I constructed an instrument, in which I fixed
_permanently_, across the ends of the reflectors, pieces of coloured
glass, and other irregular objects; and I showed the instrument in this
state to some members of the Royal Society of Edinburgh, who were much
struck with the beauty of its effects. In this case, however, the forms
were nearly permanent; and slight, though beautiful, variations were
produced by varying the position of the instrument with respect to the
source of light.
The great step, however, towards the completion of the instrument
remained yet to be made; and it was not till some time afterwards that
the idea occurred to me _of giving motion to objects, such as pieces
of coloured glass, &c., which were either fixed or placed loosely in
a cell at the end of the instrument_. When this idea was carried into
execution, and the reflectors placed in a tube, and fitted up on the
preceding principles, the Kaleidoscope, in its _simple form_, was
completed.
In this form, however, the Kaleidoscope could not be considered as
a general philosophical instrument of universal application. The
least deviation of the object from the position of symmetry at the
end of the reflectors, produced a deviation from beauty and symmetry
in the figure, and this deviation increased with the distance of the
object. The use of the instrument was therefore limited to objects in
contact with the ends of the reflectors, or held close to them, and
consequently to objects, or groups of objects, whose magnitudes were
less than its triangular aperture.
The next, and by far the most important step of the invention, was
to remove this limitation, and to extend indefinitely the use and
application of the instrument. This effect was obtained by employing a
draw tube, containing a convex lens, or, what is better, an achromatic
object-glass of such a focal length, that the images of objects, of
all magnitudes and at all distances, might be distinctly formed at the
end of the reflectors, and introduced into the pictures created by the
instrument in the same manner as if they had been reduced in size, and
placed in the true position in which alone perfect symmetry could be
obtained.
Public-domain text, read in full here on John Shaqi.
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