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
In the construction of instruments of this kind, it is necessary to
make the prism of glass longer than the distance at which the eye
can see objects with perfect distinctness; that is, if the eye is
capable of seeing objects distinctly at the distance of five inches,
it will not perceive the same objects distinctly when they are placed
at the end of a prism of glass five inches long. This singular effect
arises from a property of plain lenses or pieces of plain glass, in
consequence of which, they cause divergent rays to diverge from a point
nearer the lens or plate, than that from which they radiated. It will
therefore be more convenient, for many reasons, to make the glass prism
only two or three inches long, and obtain distinct vision by means
of a lens placed at the eye-end of it; but, for the reason already
mentioned, the focal length of the lens must be less than the length of
the glass prism. The lens may even be joined to the prism, by grinding
the eye-end into a spherical form, but the degree of convexity must be
calculated upon the principles already stated.
The solid form of the Kaleidoscope is peculiarly fitted for polycentral
instruments, as we have only to polish the side, which would otherwise
have been left rough, the prism being supposed to be cut to the angles
which are necessary to give symmetrical forms, according to the
principles stated in Chapter XIII.
CHAPTER XV.
ON THE APPLICATION OF THE KALEIDOSCOPE TO THE MAGIC
LANTERN, SOLAR MICROSCOPE, AND CAMERA OBSCURA.
[Illustration: FIG. 50.]
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