Popular Scientific Recreations: in Natural Philosphy, Astronomy, Geology, Chemistry, etc., etc., etc.Tissandier, Gaston
Science
Popular Scientific Recreations: in Natural Philosphy, Astronomy, Geology, Chemistry, etc., etc., etc.
Tissandier, Gaston
Scientific recreations
Light is distributed in rays. These rays are straight in all
directions. The velocity of light is almost inconceivable. It travels
at a rate of 186,500 miles a second. The latest computation with
electric light has given a rate of 187,200 miles a second; but the blue
rays in the light experimented on probably account for the difference,
for blue rays travel quicker by one per cent. than red rays. Römer
first found out the velocity of light, which comes to us from the
sun—ninety millions of miles—in eight minutes. Fizeau calculated the
velocity by means of a wheel, which was set moving with tremendous
speed by making the light pass between the teeth of the wheel and back
again.
When rays of light meet substances they are deflected, and the
phenomena under these circumstances are somewhat similar to the
phenomena of heat and sound. There are three particular conditions of
rays of light: (1) they are absorbed; (2) they are reflected; (3) they
are refracted.
Firstly. Let us see what we mean by light being absorbed; and this is
not difficult to understand, for any “black” substance shows us at once
that all the sunlight is taken in by the black object, and does not
come out again. It does not take in the light and radiate it, as it
might heat. The rose is red, because the rays of light pass through it,
and certain of them are reflected from within. So colour may be stated
to be the rays thrown out by the objects themselves—those they reject
or reflect being the “colour” of the object.
[Illustration: Fig. 85.—Angle of reflection, etc.]
Secondly. Bodies which reflect light very perfectly are known as
mirrors, and they are termed plane, concave, or convex mirrors,
according to form. A plane mirror reflects so that the reflected ray _d
i_ forms the same angle with the perpendicular as the incident ray _r
i_; in other words, the angle of incidence is always equal to the angle
of reflection, and these rays are perpendicular to the plane from which
they are reflected. The rays diverge, so that they appear to come from
a point as far behind the mirror as the luminous point is in front, and
the images reflected have the same appearance, but reversed. There is
another law, which is that “the angular velocity of a beam reflected
from a mirror is twice that of the mirror.” The Kaleidoscope, with
which we are all familiar, is based upon the fact of the multiplication
of images by two mirrors inclining towards each other.
[Illustration: Fig. 86.—Concave mirror.]
Public-domain text, read in full here on John Shaqi.
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