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 applying the compound Kaleidoscope to distant objects, the cell is
removed and the lens substituted in its place. The instrument is then
directed to the objects, and the tube =A B= drawn out till the inverted
images of the objects are seen perfectly distinct, or in focus, and
the pattern consequently perfectly symmetrical. When this is done, the
pattern is varied, both by turning the instrument round its axis, and
by moving it in any direction over the object to which it is pointed.
When the object is about four inches from the lens, the tube requires
to be pulled out as far as possible, and for greater distances it must
be pushed in. The points suited to different distances can easily
be determined by experiment, and marked on the inner tube, if it
should be found convenient. In most of the instruments there is, near
the middle of the tube =A B=, a mark which is nearly suited to all
distances beyond _three feet_. The object-plates held in the hand, or
the mirror-box placed upon a table, at a distance greater than five
or six inches, may be also used when the lens =L= is in the tube. The
furniture of a room, books and papers lying on a table, pictures on
the wall, a blazing fire, the moving branches and foliage of trees and
shrubs, bunches of flowers, horses and cattle in a park, carriages in
motion, the currents of a river, waterfalls, moving insects, the sun
shining through clouds or trees, and, in short, every object in nature
may be introduced by the aid of the lens into the figures created by
the instrument.
The patterns which are thus presented to the eye are essentially
different from those exhibited by the simple Kaleidoscope. Here the
objects are independent of the observer, and all their movements are
represented with the most singular effect in the symmetrical picture,
which is as much superior to what is given by the simple instrument,
as the sight of living or moving objects is superior to an imperfect
portrait of them. When the flame of a blazing fire is the object, the
Kaleidoscope creates from it the most magical fireworks, in which the
currents of flame which compose the picture can be turned into every
possible direction.
In order to mark with accuracy the points on the tube =A B=, suited to
different distances, the instrument should be directed to a straight
line, inclined like _m n_, Fig. 3, to the line bisecting the angular
aperture =A O B=, and brought nearer to the centre =O= of the field.
The perfect junction of the reflected images of the line at the points
_mʹ nʹ_, &c., so as to form a star, or a polygon with salient and
re-entering angles, will indicate with great nicety, that the tube has
been pulled out the proper length for the given distance. In this way,
a scale for different distances, and scales for different lenses, may
be marked on the tube.
Public-domain text, read in full here on John Shaqi.
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