CHAPTER XL.--THE KALEIDOSCOPE, AND HOW TO MAKE IT.

BY W. J. GORDON.

The kaleidoscope is the most successful scientific toy of modern times.

Immediately after its patenting by Sir David Brewster over three hundred

thousand were sold in three months. Essentially it consists of a couple

of mirrors arranged at an angle forming some even sub-multiple of three

hundred and sixty. The angle usually chosen is the sixth, or sixty

degrees.

Before proceeding to make a kaleidoscope for home use, it would be well

to try a few experiments with two common pieces of looking-glass.

Arrange them as in the diagram (Fig. 1), and placing an object at A, or

standing them on a piece of colour work, notice the beautiful

geometrical pattern formed by the various reflectors. Having

experimented with various articles at the angle given, try the effect at

another angle, and note how the slightest change affects the design.

Having grasped the general principle you can proceed to make one of the

commoner varieties of the instrument as usually sold. These have three

mirrors.

[Illustration: Fig. 1.]

[Illustration: Fig. 2.]

[Illustration: Fig. 3.]

Cut three pieces of common glass into the shape here given. Let them be

seven and a half inches long, one inch and five-eighths wide at A, and

one inch wide at B (Fig. 2). If they are silvered on the back so much

the better; if they are not, paint them black on one side. A very good

black paint for the purpose is made by mixing vegetable black with gold

size until it is as thick as cream. Seven-pennyworth of gold size and a

pennyworth of vegetable black, obtained from the nearest oil-shop, will

give you enough paint for a dozen kaleidoscopes, and be useful for other

purposes into the bargain. The three mirrors are to be arranged in a

tube, with their blackened sides outwards (see Fig. 3); and the tube is

to be made accordingly. An old copy-book cover can be rolled into the

shape, or a well-pasted strip of newspaper rolled round and round on a

stick, as described in the chapter on the telescope, will give the tube

with very little trouble. To fit the mirrors we have cut the tube should

be eight and a quarter inches long, two inches in diameter at the broad

end, and one inch and an eighth in diameter at the narrow. Of course the

tube is not absolutely necessary; a square box two inches wide and eight

inches and a quarter long will answer every purpose, but then the

mirrors, instead of being kept in position by the sides of the case,

will have to be wedged up by pieces of cork or balls of paper.

[Illustration: Fig. 4.]

Having made the case, fix an eyepiece of tin or cardboard at one end, so

that a hole a quarter of an inch in diameter comes in the centre of the

angle made by the mirrors. This hole is shown in position in Fig. 4,

which represents the top of the tube or box.

At the other end of the tube a round piece of clear glass is to be

fixed, and if the box is used a square piece will take its place. The

round can be easily made from the square by chipping off the corners. An

American glass-cutter, costing sixpence, can be obtained from most

tool-shops, which will be found very useful in cutting glass for this

and many other purposes. The secret in working wheel glass-cutters of

all kinds is to keep the handle as nearly upright as possible and to

bear firmly and equally on all parts of the work.

Having cut the plain glass end and fitted it close up against the broad

end of the mirrors, the next thing is to cut a piece of ground-glass of

the same size to fit over it. This ground-glass may be patterned, as in

the kaleidoscopes of commerce. It is, however, more satisfactory to have

it plain. Between the glasses you place the pieces of broken glass to

form the designs.

‘The objects which give the finest outlines by inversion are those which

have a curvilinear form, such as circles, ellipses, looped curves like

the figure 8, curves like the figure 3 and the letter S; spirals and

other forms, such as squares, rectangles, and triangles, may be applied

with advantage. Glass, both spun and twisted, and of all colours and

shades of colours, should be formed into the preceding shapes; and when

these are mixed with pieces of flat coloured glass, blue vitriol, native

sulphur, yellow ochre, and differently coloured fluids, enclosed and

moving in small vessels of glass, they will make the finest transparent

objects for the kaleidoscope. When the objects are to be laid upon a

mirror plate, fragments of opaquely-coloured glass should be added to

the transparent fragments, along with pieces of brass wire, of coloured

foils, and grains of spelter. In selecting transparent objects, the

greatest care must be taken to reject fragments of opaque glass, and

dark colours that do not transmit much light; and all the pieces of spun

glass, or coloured plates, should be as thin as possible.’

As far as the harmony of colour is concerned, it may be as well to note

that the deepest red harmonises with an equal mixture of blue and green;

that red goes best with green and blue, the blue being predominant; that

orange-red requires a blue with a good deal of indigo; that

orange-yellow wants pure indigo; that light yellow is best with violet

and indigo half and half; that greenish-yellow shows off best by the

side of pale violet; that green goes with a full violet; that

greenish-blue combines with violet and red; blue with orange and red;

indigo with orange-yellow; and violet with green.

Satisfactory effects can, however, be produced with almost anything

bright and shining. The first kaleidoscope we, in the thirst for

knowledge, took apart was found to have for its objects about forty

pieces of red, green, blue, and brown stained glass, smashed up into

irregular fragments of about a quarter of an inch in width and length,

and as the shapes were varied and the colours crude, the patterns at

every shake were almost as startling as those produced by a sixpenny

catharine-wheel on the 5th of November.

The ground glass should be fitted into a cap, so as to be removable at

pleasure, and the fragments of coloured glass to form the patterns

should be left free to move between the glasses.

Having made this kaleidoscope, and coaxed it into acting properly,

experiments with other contrivances should be made. Mirrors should be

arranged at ninety, forty-five, and forty-five; at ninety, sixty, and

thirty, and other angular combinations. A lens should be fitted at the

end of the tube for magnifying purposes, and the tube should be attached

to a magic lantern, and the patterns, almost equalling the chromatrope,

thrown on the screen.

[Illustration: Fig. 5.]

Having worked the fixed mirrors to the point of weariness, shifting

mirrors should be tried, and then two mirrors, made to alter their

angles by an arrangement of screws (see Fig. 5), as in the adjustable

form of the instrument, should be experimented with.

You will soon find that when the inclination of the mirrors is not an

aliquot part of 360 the reflections will not join, and then the

following table from Sir David Brewster’s manual of the kaleidoscope may

prove useful:--

No. of No. of No. of Direct

Inclination. Reflections. Pictures. Pictures.

120 3 2 1

72 5 2 3

51-3/7 7 4 3

40 9 4 5

32-8/11 11 6 5

27-9/13 13 6 7

24 15 8 7

21-3/17 17 8 9

18-18/19 19 10 9

17-1/7 21 10 11

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