|
Williams |
In December, 1672,
Newton was elected a Fellow of the Royal Society, and at this meeting a
paper describing his invention of the refracting telescope was read. A
few days later he wrote to the secretary, making some inquiries as to the
weekly meetings of the society, and intimating that he had an account of
an interesting discovery that he wished to lay before the society. When
this communication was made public, it proved to be an explanation of the
discovery of the composition of white light. We have seen that the question
as to the nature of color had commanded the attention of such investigators
as Huygens, but that no very satisfactory solution of the question had
been attained. Newton proved by demonstrative experiments that white light
is composed of the blending of the rays of diverse colors, and that the
color that we ascribe to any object is merely due to the fact that the
object in question reflects rays of that color, absorbing the rest. That
white light is really made up of many colors blended would seem incredible
had not the experiments by which this composition is demonstrated become
familiar to every one. The experiments were absolutely novel when Newton
brought them forward, and his demonstration of the composition of light
was one of the most striking expositions ever brought to the attention
of the Royal Society. It is hardly necessary to add that, notwithstanding
the conclusive character of Newton's work, his explanations did not for
a long time meet with general acceptance.
Newton was led to his discovery by some
experiments made with an ordinary glass prism applied to a hole in the
shutter of a darkened room, the refracted rays of the sunlight being received
upon the opposite wall and forming there the familiar spectrum. "It was
a very pleasing diversion," he wrote, "to view the vivid and intense colors
produced thereby; and after a time, applying myself to consider them very
circumspectly, I became surprised to see them in varying form, which, according
to the received laws of refraction, I expected should have been circular.
They were terminated at the sides with straight lines, but at the ends
the decay of light was so gradual that it was difficult to determine justly
what was their figure, yet they seemed semicircular.
"Comparing the length of this colored spectrum
with its breadth, I found it almost five times greater; a disproportion
so extravagant that it excited me to a more than ordinary curiosity of
examining from whence it might proceed. I could scarce think that the various
thicknesses of the glass, or the termination with shadow or darkness, could
have any influence on light to produce such an effect; yet I thought it
not amiss, first, to examine those circumstances, and so tried what would
happen by transmitting light through parts of the glass of divers thickness,
or through holes in the window of divers bigness, or by setting the prism
without so that the light might pass through it and be refracted before
it was transmitted through the hole; but I found none of those circumstances
material. The fashion of the colors was in all these cases the same.
"Then I suspected whether by any unevenness
of the glass or other contingent irregularity these colors might be thus
dilated. And to try this I took another prism like the former, and so placed
it that the light, passing through them both, might be refracted contrary
ways, and so by the latter returned into that course from which the former
diverted it. For, by this means, I thought, the regular effects of the
first prism would be destroyed by the second prism, but the irregular ones
more augmented by the multiplicity of refractions. The event was that the
light, which by the first prism was diffused into an oblong form, was by
the second reduced into an orbicular one with as much regularity as when
it did not all pass through them. So that, whatever was the cause of that
length, 'twas not any contingent irregularity.
"I then proceeded to examine more critically
what might be effected by the difference of the incidence of rays coming
from divers parts of the sun; and to that end measured the several lines
and angles belonging to the image. Its distance from the hole or prism
was 22 feet; its utmost length 13 1/4 inches; its breadth 2 5/8; the diameter
of the hole 1/4 of an inch; the angle which the rays, tending towards the
middle of the image, made with those lines, in which they would have proceeded
without refraction, was 44 degrees 56'; and the vertical angle of the prism,
63 degrees 12'. Also the refractions on both sides of the prism - that
is, of the incident and emergent rays - were, as near as I could make them,
equal, and consequently about 54 degrees 4'; and the rays fell perpendicularly
upon the wall. Now, subducting the diameter of the hole from the length
and breadth of the image, there remains 13 inches the length, and 2 3/8
the breadth, comprehended by those rays, which, passing through the centre
of the said hole, which that breadth subtended, was about 31', answerable
to the sun's diameter; but the angle which its length subtended was more
than five such diameters, namely 2 degrees 49'.
"Having made these observations, I first
computed from them the refractive power of the glass, and found it measured
by the ratio of the sines 20 to 31. And then, by that ratio, I computed
the refractions of two rays flowing from opposite parts of the sun's discus,
so as to differ 31' in their obliquity of incidence, and found that the
emergent rays should have comprehended an angle of 31', as they did, before
they were incident.
"But because this computation was founded
on the hypothesis of the proportionality of the sines of incidence and
refraction, which though by my own experience I could not imagine to be
so erroneous as to make that angle but 31', which in reality was 2 degrees
49', yet my curiosity caused me again to make my prism. And having placed
it at my window, as before, I observed that by turning it a little about
its axis to and fro, so as to vary its obliquity to the light more than
an angle of 4 degrees or 5 degrees, the colors were not thereby sensibly
translated from their place on the wall, and consequently by that variation
of incidence the quantity of refraction was not sensibly varied. By this
experiment, therefore, as well as by the former computation, it was evident
that the difference of the incidence of rays flowing from divers parts
of the sun could not make them after decussation diverge at a sensibly
greater angle than that at which they before converged; which being, at
most, but about 31' or 32', there still remained some other cause to be
found out, from whence it could be 2 degrees 49'."
All this caused Newton to suspect that
the rays, after their trajection through the prism, moved in curved rather
than in straight lines, thus tending to be cast upon the wall at different
places according to the amount of this curve. His suspicions were increased,
also, by happening to recall that a tennis-ball sometimes describes such
a curve when "cut" by a tennis-racket striking the ball obliquely.
"For a circular as well as a progressive
motion being communicated to it by the stroke," he says, "its parts on
that side where the motions conspire must press and beat the contiguous
air more violently than on the other, and there excite a reluctancy and
reaction of the air proportionately greater. And for the same reason, if
the rays of light should possibly be globular bodies, and by their oblique
passage out of one medium into another acquire a circulating motion, they
ought to feel the greater resistance from the ambient ether on that side
where the motions conspire, and thence be continually bowed to the other.
But notwithstanding this plausible ground of suspicion, when I came to
examine it I could observe no such curvity in them. And, besides (which
was enough for my purpose), I observed that the difference 'twixt the length
of the image and diameter of the hole through which the light was transmitted
was proportionable to their distance.
"The gradual removal of these suspicions
at length led me to the experimentum crucis, which was this: I took two
boards, and, placing one of them close behind the prism at the window,
so that the light must pass through a small hole, made in it for the purpose,
and fall on the other board, which I placed at about twelve feet distance,
having first made a small hole in it also, for some of the incident light
to pass through. Then I placed another prism behind this second board,
so that the light trajected through both the boards might pass through
that also, and be again refracted before it arrived at the wall. This done,
I took the first prism in my hands and turned it to and fro slowly about
its axis, so much as to make the several parts of the image, cast on the
second board, successively pass through the hole in it, that I might observe
to what places on the wall the second prism would refract them. And I saw
by the variation of these places that the light, tending to that end of
the image towards which the refraction of the first prism was made, did
in the second prism suffer a refraction considerably greater than the light
tending to the other end. And so the true cause of the length of that image
was detected to be no other than that LIGHT consists of RAYS DIFFERENTLY
REFRANGIBLE, which, without any respect to a difference in their incidence,
were, according to their degrees of refrangibility, transmitted towards
divers parts of the wall."[1] |
|