The kaleidoscope : $b its history, theory and construction. With its application to the fine and useful arts — John Shaqi
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
When we look through a Kaleidoscope in which the mirrors are placed
at an angle of 18° or 22½°, the eye will perceive a very obvious
difference in the intensity of the light in different parts of the
field. If the inclination of the mirrors be about 30°, and the eye
properly placed near the angular point, the intensity of the light is
tolerably uniform; and a person who is unaccustomed to the comparison
of different lights, will find it extremely difficult to distinguish
the direct sector from the reflected ones. This difficulty will be
still greater if the mirrors are made of finely polished steel, or
of the best speculum metal, and the observer will not hesitate in
believing that he is looking through a tube whose diameter is equal to
that of the circular field. This approximation to uniformity in the
intensity of the light in all the sectors, which arises wholly from the
determination of the proper position of the eye, is one of the most
curious and unexpected properties of the Kaleidoscope, and is one which
could not have been anticipated from any theoretical views, or from
any experimental results obtained from the ancient mode of combining
plain mirrors. It is that property, too, which gives it all its value;
for, if the eye observed the direct sector with its included objects
distinguished from all the rest by superior brilliancy, not only would
the illusion vanish, but the picture itself would cease to afford
pleasure, from the want of symmetry in the light of the field.
[Illustration: FIG. 18.]
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