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
glass before the aperture =A O B=. The tube may be directed to the
brightest part of the sky in the day-time, or in the evening to a
candle, or an Argand Lamp, so as to transmit the light directly through
the coloured fragments; but it will always be found to give richer and
more brilliant effects if the tube is directed to the window-shutter,
a little to one side of the light, or is held to one side of the
candle—or, what is still better, between two candles or lamps placed
as near each other as possible. In this way the picture created by the
instrument is not composed of the harsh tints formed by transmitted
light; but of the various reflected and softened colours which are
thrown into the tube from the sides and angles of the glass fragments.
When the pattern remains fixed in any position of the instrument, a
variety of beautiful changes may be effected by making the end of the
tube revolve round a candle or a bright gas flame, placed near the
object-plate. The general pattern remains the same, but its colours
vary both in their position and intensity, as the light falls upon
different sides of the fragments of glass.
In the preceding method of applying the objects to the reflectors,
the fragments of coloured glass are introduced before the aperture,
and pass across it in concentric circles; and as the fragments always
descend by their own gravity, the changes in the picture, though
infinite in number, constantly take place in a similar manner. This
defect may be remedied, and a great degree of variety exhibited in
the motion of the fragments, by making the object-plates rectangular
instead of circular, and moving them through a groove cut in the cell
at =M N=, in the same manner as is done with the pictures or sliders
for the magic lantern and solar microscope. By this means the different
fragments that present themselves to the aperture may be made to pass
across it in every possible direction, and very interesting effects may
be produced by a combination of the rotatory and rectilineal motions of
the object-plate. When the object or objects are fixed, and the tube
with the reflectors moved round a centre, as described in Chapter
II.,[3] we have the same succession of symmetrical pictures; but in
this case every alternate sector is stationary, and the same number in
motion, the moving figures always changing their form, and assuming
that of the figures in the stationary sectors, which of course change,
while the ends of the mirror pass over the fixed objects.
[3] See Chapter X.
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