The principle of interference, as just stated, applies to the waves of

light as it does to the waves of water and the waves of sound. And the

conditions of interference are the same in all three. If two series of

light-waves of the same length start at the same moment from a common

origin (say A, fig. 11), crest coincides with crest, sinus with sinus,

and the two systems blend together to a single system (A _m_ _n_) of

double amplitude. If both series start at the same moment, one of them

being, at starting, a whole wavelength in advance of the other, they

also add themselves together, and we have an augmented luminous

effect. The same occurs when the one system of waves is any _even_

number of semi-undulations in advance of the other. But if the one

system be half a wave-length (as at A' _a_', fig. 12), or any _odd_

number of half wavelengths, in advance, then the crests of the one

fall upon the sinuses of the other; the one system, in fact, tends to

_lift_ the particles of ether at the precise places where the other

tends to _depress_ them; hence, through the joint action of these

opposing forces (indicated by the arrows) the light-ether remains

perfectly still. This stillness of the ether is what we call darkness,

which corresponds with a dead level in the case of water.

[Illustration: Fig. 12.]

It was said in our first lecture, with reference to the colours

produced by absorption, that the function of natural bodies is

selective, not creative; that they extinguish certain constituents of

the white solar light, and appear in the colours of the unextinguished

light. It must at once occur to you that, inasmuch as we have in

interference an agency by which light may be self-extinguished, we may

have in it the conditions for the production of colour. But this would

imply that certain constituents are quenched by interference, while

others are permitted to remain. This is the fact; and it is entirely

due to the difference in the lengths of the waves of light.

§ 7. _Colours of thin Films. Observations of Boyle and Hooke_.

This subject may be illustrated by the phenomena which first suggested

the undulatory theory to the mind of Hooke. These are the colours of

thin transparent films of all kinds, known as the _colours of thin

plates_. In this relation no object in the world possesses a deeper

scientific interest than a common soap-bubble. And here let me say

emerges one of the difficulties which the student of pure science

encounters in the presence of 'practical' communities like those of

America and England; it is not to be expected that such communities

can entertain any profound sympathy with labours which seem so far

removed from the domain of practice as are many of the labours of the

man of science. Imagine Dr. Draper spending his days in blowing

soap-bubbles and in studying their colours! Would you show him the

necessary patience, or grant him the necessary support? And yet be it

remembered it was thus that minds like those of Boyle, Newton and

Hooke were occupied; and that on such experiments has been founded a

theory, the issues of which are incalculable. I see no other way for

you, laymen, than to trust the scientific man with the choice of his

inquiries; he stands before the tribunal of his peers, and by their

verdict on his labours you ought to abide.

Whence, then, are derived the colours of the soap-bubble? Imagine a

beam of white light impinging on the bubble. When it reaches the first

surface of the film, a known fraction of the light is reflected back.

But a large portion of the beam enters the film, reaches its second

surface, and is again in part reflected. The waves from the second

surface thus turn back and hotly pursue the waves from the first

surface. And, if the thickness of the film be such as to cause the

necessary retardation, the two systems of waves interfere with each

other, producing augmented or diminished light, as the case may be.

But, inasmuch as the waves of light are of different lengths, it is

plain that, to produce extinction in the case of the longer waves, a

greater thickness of film is necessary than in the case of the shorter

ones. Different colours, therefore, must appear at different

thicknesses of the film.

Take with you a little bottle of spirit of turpentine, and pour it

into one of your country ponds. You will then see the glowing of those

colours over the surface of the water. On a small scale we produce

them thus: A common tea-tray is filled with water, beneath the surface

of which dips the end of a pipette. A beam of light falls upon the

water, and is reflected by it to the screen. Spirit of turpentine is

poured into the pipette; it descends, issues from the end in minute

drops, which rise in succession to the surface. On reaching it, each

drop spreads suddenly out as a film, and glowing colours immediately

flash forth upon the screen. The colours change as the thickness of

the film changes by evaporation. They are also arranged in zones, in

consequence of the gradual diminution of thickness from the centre

outwards.

Any film whatever will produce these colours. The film of air between

two plates of glass squeezed together, exhibits, as shown by Hooke,

rich fringes of colour. A particularly fine example of these fringes

is now before you. Nor is even air necessary; the rupture of optical

continuity suffices. Smite with an axe the black, transparent

ice--black, because it is pure and of great depth--under the moraine

of a glacier; you readily produce in the interior flaws which no air

can reach, and from these flaws the colours of thin plates sometimes

break like fire. But the source of most historic interest is, as

already stated, the soap-bubble. With one of the mixtures employed by

the eminent blind philosopher, Plateau, in his researches on the

cohesion figures of thin films, we obtain in still air a bubble ten or

twelve inches in diameter. You may look at the bubble itself, or you

may look at its projection upon the screen; rich colours arranged in

zones are, in both cases, exhibited. Rendering the beam parallel, and

permitting it to impinge upon the sides, bottom, and top of the

bubble, gorgeous fans of colour, reflected from the bubble, overspread

the screen, rotating as the beam is carried round. By this experiment

the internal motions of the film are also strikingly displayed.

Not in a moment are great theories elaborated: the facts which demand

them become first prominent; then, to the period of observation

succeeds a period of pondering and of tentative explanation. By such

efforts the human mind is gradually prepared for the final theoretic

illumination. The colours of thin plates, for example, occupied the

attention of Robert Boyle. In his 'Experimental History of Colours' he

contends against the schools which affirmed that colour was 'a

penetrative quality that reaches to the innermost parts of the

object,' adducing opposing facts. 'To give you a first instance,' he

says, 'I shall need but to remind you of what I told you a little

after the beginning of this essay, touching the blue and red and

yellow that may be produced upon a piece of tempered steel; for these

colours, though they be very vivid, yet if you break the steel they

adorn, they will appear to be but superficial.' He then describes, in

phraseology which shows the delight he took in his work, the following

beautiful experiment:--

'We took a quantity of clean lead, and melted it with a strong fire,

and then immediately pouring it out into a clean vessel of convenient

shape and matter (we used one of iron, that the great and sudden heat

might not injure it), and then carefully and nimbly taking off the

scum that floated on the top, we perceived, as we expected, the smooth

and glossy surface of the melted matter to be adorned with a very

glorious colour, which, being as transitory as delightful, did almost

immediately give place to another vivid colour, and that was as

quickly succeeded by a third, and this, as it were, chased away by a

fourth; and so these wonderfully vivid colours successively appeared

and vanished till the metal ceasing to be hot enough to hold any

longer this pleasing spectacle, the colours that chanced to adorn the

surface when the lead thus began to cool remained upon it, but were so

superficial that how little soever we scraped off the surface of the

lead, we did, in such places, scrape off all the colour.' 'These

things,' he adds, 'suggested to me some thoughts or ravings which I

have not now time to acquaint you with.'[13]

He extends his observations to essential oils and spirits of wine,

'which being shaken till they have good store of bubbles, those

bubbles will (if attentively considered) appear adorned with various

and lovely colours, which all immediately vanish upon the

retrogressing of the liquid which affords these bubbles their skins

into the rest of the oil.' He also refers to the colour of glass

films. 'I have seen one that was skilled in fashioning glasses by the

help of a lamp blowing some of them so strongly as to burst them;

whereupon it was found that the tenacity of the metal was such that

before it broke it suffered itself to be reduced into films so

extremely thin that they constantly showed upon their surface the

varying colours of the rainbow.'[14]

Subsequent to Boyle the colours of thin plates occupied the attention

of Robert Hooke, in whose writings we find a dawning of the undulatory

theory of light. He describes with great distinctness the colours

obtained with thin flakes of 'Muscovy glass' (talc), also those

surrounding flaws in crystals where optical continuity is destroyed.

He shows very clearly the dependence of the colour upon the thickness

of the film, and proves by microscopic observation that plates of a

uniform thickness yield uniform colours. 'If,' he says, 'you take any

small piece of the Muscovy glass, and with a needle, or some other

convenient instrument, cleave it oftentimes into thinner and thinner

laminæ, you shall find that until you come to a determinate thinness

of them they shall appear transparent and colourless; but if you

continue to split and divide them further, you shall find at last that

each plate shall appear most lovely tinged or imbued with a

determinate colour. If, further, by any means you so flaw a pretty

thick piece that one part begins to cleave a little from the other,

and between these two there be gotten some pellucid medium, those

laminated or pellucid bodies that fill that space shall exhibit

several rainbows or coloured lines, the colours of which will be

disposed and ranged according to the various thicknesses of the

several parts of the plate.' He then describes fully and clearly the

experiment with pressed glasses already referred to:--

'Take two small pieces of ground and polished looking-glass plate,

each about the bigness of a shilling: take these two dry, and with

your forefingers and thumbs press them very hard and close together,

and you shall find that when they approach each other very near there

will appear several irises or coloured lines, in the same manner

almost as in the Muscovy glass; and you may very easily change any of

the colours of any part of the interposed body by pressing the plates

closer and harder together, or leaving them more lax--that is, a part

which appeared coloured with a red, may presently be tinged with a

yellow, blue, green, purple, or the like. 'Any substance,' he says,

'provided it be thin and transparent, will show these colours.' Like

Boyle, he obtained them with glass films; he also procured them with

bubbles of pitch, rosin, colophony, turpentine, solutions of several

gums, as gum arabic in water, any glutinous liquor, as wort, wine,

spirit of wine, oyl of turpentine, glare of snails, &c.

Hooke's writings show that even in his day the idea that both light

and heat are modes of motion had taken possession of many minds.

'First,' he says, 'that all kind _of fiery burning bodies_ have their

parts in motion I think will be easily granted me. That the spark

struck from a flint and steel is in rapid agitation I have elsewhere

made probable;... that heat argues a motion of the internal parts is

(as I said before) generally granted;... and that in all extremely hot

shining bodies there is a very quick motion that causes light, as well

as a more robust that causes heat, may be argued from the celerity

wherewith the bodies are dissolved. Next, it must be _a vibrative

motion.'_ His reference to the quick motion of light and the more

robust motion of heat is a remarkable stroke of sagacity; but Hooke's

direct insight is better than his reasoning; for the proofs he adduces

that light is 'a vibrating motion' have no particular bearing upon the

question.

Still the Undulatory Theory had undoubtedly dawned upon the mind of

this remarkable man. In endeavouring to account for the colours of

thin plates, he again refers to the relation of colour to thickness:

he dwells upon the fact that the film which shows these colours must

be transparent, proving this by showing that however thin an opaque

body was rendered no colours were produced. 'This,' he says, 'I have

often tried by pressing a small globule of mercury between two smooth

plates of glass, whereby I have reduced that body to a much greater

thinness than was requisite to exhibit the colours with a transparent

body.' Then follows the sagacious remark that to produce the colours

'there must be a considerable reflecting body adjacent to the under or

further side of the lamina or plate: for this I always found, that the

greater that reflection was the more vivid were the appearing colours.

From which observation,' he continues, 'it is most evident, _that the

reflection from the further or under side of the body is the principal

cause of the production of these colours._'

He draws a diagram, correctly representing the reflection at the two

surfaces of the film; but here his clearness ends. He ascribes the

colours to a coalescence or confusion of the two reflecting pulses;

the principal of interference being unknown to him, he could not go

further in the way of explanation.

§ 8. _Newton's Rings. Relation of Colour to Thickness of Film_.

[Illustration: Fig. 13]

In this way, then, by the active operation of different minds, facts

are observed, examined, and the precise conditions of their

appearance determined. All such work in science is the prelude to

other work; and the efforts of Boyle and Hooke cleared the way for the

optical career of Newton. He conquered the difficulty which Hooke had

found insuperable, and determined by accurate measurements the

relation of the thickness of the film to the colour it displays. In

doing this his first care was to obtain a film of variable and

calculable depth. On a plano-convex glass lens (D B E, fig. 13) of

very feeble curvature he laid a plate of glass (A C) with a plane

surface, thus obtaining a film of air of gradually increasing depth

from the point of contact (B) outwards. On looking at the film in

monochromatic light he saw, with the delight attendant on fulfilled

prevision, surrounding the place of contact, a series of bright rings

separated from each other by dark ones, and becoming more closely

packed together as the distance from the point of contact augmented

(as in fig. 14). When he employed red light, his rings had certain

diameters; when he employed blue light, the diameters were less. In

general terms, the more refrangible the light the smaller were the

rings. Causing his glasses to pass through the spectrum from red to

blue, the rings gradually contracted; when the passage was from blue

to red, the rings expanded. This is a beautiful experiment, and

appears to have given Newton the most lively satisfaction. When white

light fell upon, the glasses, inasmuch as the colours were not

superposed, a series _of iris-coloured_ circles was obtained. A

magnified image of _Newton's rings_ is now before you, and, by

employing in succession red, blue, and white light, we obtain all the

effects observed by Newton. You notice that in monochromatic light the

rings run closer and closer together as they recede from the centre.

This is due to the fact that at a distance the film of air thickens

more rapidly than near the centre. When white light is employed, this

closing up of the rings causes the various colours to be superposed,

so that after a certain thickness they are blended together to white

light, the rings then ceasing altogether. It needs but a moment's

reflection to understand that the colours of thin plates, produced by

white light, are never unmixed or monochromatic.

[Illustration: Fig. 14]

Newton compared the tints obtained in this way with the tints of his

soap-bubble, and he calculated the corresponding thickness. How he did

this may be thus made plain to you: Suppose the water of the ocean to

be absolutely smooth; it would then accurately represent the earth's

curved surface. Let a perfectly horizontal plane touch the surface at

any point. Knowing the earth's diameter, any engineer or mathematician

in this room could tell you how far the sea's surface will lie below

this plane, at the distance of a yard, ten yards, a hundred yards, or

a thousand yards from the point of contact of the plane and the sea.

It is common, indeed, in levelling operations, to allow for the

curvature of the earth. Newton's calculation was precisely similar.

His plane glass was a tangent to his curved one. From its refractive

index and focal distance he determined the diameter of the sphere of

which his curved glass formed a segment, he measured the distances of

his rings from the place of contact, and he calculated the depth

between the tangent plane and the curved surface, exactly as the

engineer would calculate the distance between his tangent plane and

the surface of the sea. The wonder is, that, where such infinitesimal

distances are involved, Newton, with the means at his disposal, could

have worked with such marvellous exactitude.

To account for these rings was the greatest optical difficulty that

Newton, ever encountered. He quite appreciated the difficulty. Over

his eagle eye there was no film--no vagueness in his conceptions. At

the very outset his theory was confronted by the question, Why, when a

beam of light is incident on a transparent body, are some of the

light-particles reflected and some transmitted? Is it that there are

two kinds of particles, the one specially fitted for transmission and

the other for reflection? This cannot be the reason; for, if we allow

a beam of light which has been reflected from one piece of glass to

fall upon another, it, as a general rule, is also divided into a

reflected and a transmitted portion. The particles once reflected are

not always reflected, nor are the particles once transmitted always

transmitted. Newton saw all this; he knew he had to explain why it is

that the self-same particle is at one moment reflected and at the next

moment transmitted. It could only he through _some change in the

condition of the particle itself_. The self-same particle, he

affirmed, was affected by 'fits' of easy transmission and reflection.

§ 9. _Theory of 'Fits' applied to Newton's Rings_.

If you are willing to follow me in an attempt to reveal the

speculative groundwork of this theory of fits, the intellectual

discipline will, I think, repay you for the necessary effort of

attention. Newton was chary of stating what he considered to be the

cause of the fits, but there can hardly be a doubt that his mind

rested on a physical cause. Nor can there be a doubt that here, as in

all attempts at theorising, he was compelled to fall back upon

experience for the materials of his theory. Let us attempt to restore

his course of thought and observation. A magnet would furnish him with

the notion of attracted and repelled poles; and he who habitually saw

in the visible an image of the invisible would naturally endow his

light-particles with such poles. Turning their attracted poles towards

a transparent substance, the particles would be sucked in and

transmitted; turning their repelled poles, they would be driven away

or reflected. Thus, by the ascription of poles, the transmission and

reflection of the self-same particle at different times might be

accounted for.

Consider these rings of Newton as seen in pure red light: they are

alternately bright and dark. The film of air corresponding to the

outermost of them is not thicker than an ordinary soap-bubble, and it

becomes thinner on approaching the centre; still Newton, as I have

said, measured the thickness corresponding to every ring, and showed

the difference of thickness between ring and ring. Now, mark the

result. For the sake of convenience, let us call the thickness of the

film of air corresponding to the first dark ring _d_; then Newton

found the distance corresponding to the second dark ring 2 _d_; the

thickness corresponding to the third dark ring 3 _d_; the thickness

corresponding to the tenth dark ring 10 _d_, and so on. Surely there

must be some hidden meaning in this little distance, _d_, which turns

up so constantly? One can imagine the intense interest with which

Newton pondered its meaning. Observe the probable outcome of his

thought. He had endowed his light-particles with poles, but now he is

forced to introduce the notion of _periodic recurrence_. Here his

power of transfer from the sensible to the subsensible would render it

easy for him to suppose the light-particles animated, not only with a

motion of translation, but also with a motion of rotation. Newton's

astronomical knowledge rendered all such conceptions familiar to him.

The earth has such a double motion. In the time occupied in passing

over a million and a half of miles of its orbit--that is, in

twenty-four hours--our planet performs a complete rotation; and in the

time required to pass over the distance _d_, Newton's light-particle

might be supposed to perform a complete rotation. True, the

light-particle is smaller than the planet, and the distance _d_,

instead of being a million and a half of miles, is a little over the

ninety thousandth of an inch. But the two conceptions are, in point of

intellectual quality, identical.

Imagine, then, a particle entering the film of air where it possesses

this precise thickness. To enter the film, its attracted end must be

presented. Within the film it is able to turn _once_ completely round;

at the other side of the film its attracted pole will be again

presented; it will, therefore, enter the glass at the opposite side of

the film _and be lost to the eye_. All round the place of contact,

wherever the film possesses this precise thickness, the light will

equally disappear--we shall therefore have a ring of darkness.

And now observe how well this conception falls in with the law of

proportionality discovered by Newton. When the thickness of the film

is 2 _d_, the particle has time to perform, _two_ complete rotations

within the film; when the thickness is 3 _d, three_ complete

rotations; when 10 _d, ten_ complete rotations are performed. It is

manifest that in each of these cases, on arriving at the second

surface of the film, the attracted pole of the particle will be

presented. It will, therefore, be transmitted; and, because no light

is sent to the eye, we shall have a ring of darkness at each of these

places.

The bright rings follow immediately from the same conception. They

occur between the dark rings, the thicknesses to which they correspond

being also intermediate between those of the dark ones. Take the case

of the first bright ring. The thickness of the film is ½_d_; in this

interval the rotating particle can perform only half a rotation. When,

therefore, it reaches the second surface of the film, its repelled

pole is presented; it is, therefore, driven back and reaches the eye.

At all distances round the centre corresponding to this thickness the

same effect is produced, and the consequence is a ring of brightness.

The other bright rings are similarly accounted for. At the second one,

where the thickness is 1½_d_, a rotation and a half is performed; at

the third, two rotations and a half; and at each of these places the

particles present their repelled poles to the lower surface of the

film. They are therefore sent back to the eye, and produce there the

impression of brightness. This analysis, though involving difficulties

when closely scrutinised, enables us to see how the theory of fits may

have grown into consistency in the mind of Newton.

Six Lectures on Light Delivered In The United States In 1872-1873 · 第 4 / 15 段