By the force of imagination and reason combined we may penetrate this

mystery also. The cloud takes no note of size on the part of the waves

of ether, but reflects them all alike. It exercises no selective

action. Now the cause of this may be that the cloud particles are so

large in comparison with the size of the waves of ether as to reflect

them all indifferently. A broad cliff reflects an Atlantic roller as

easily as a ripple produced by a sea-bird’s wing; and in the presence

of large reflecting surfaces, the existing differences of magnitude

among the waves of ether may disappear. But supposing the reflecting

particles, instead of being very large, to be very small, in comparison

with the size of the waves. In this case, instead of the whole wave

being fronted and in great part thrown back, a small portion only is

shivered off. The great mass of the wave passes over such a particle

without reflection. Scatter then a handful of such minute foreign

particles in our atmosphere, and set imagination to watch their action

upon the solar waves. Waves of all sizes impinge upon the particles,

and you see at every collision a portion of the impinging wave struck

off by reflection. All the waves of the spectrum, from the extreme red

to the extreme violet, are thus acted upon. But in what proportions

will the waves be scattered? A clear picture will enable us to

anticipate the experimental answer. Remembering that the red waves are

to the blue much in the relation of billows to ripples, let us consider

whether those extremely small particles are competent to scatter

all the waves in the same proportion. If they be not--and a little

reflection will make it clear to you that they are not--the production

of colour must be an incident of the scattering. Largeness is a thing

of relation; and the smaller the wave, the greater is the relative

size of any particle on which the wave impinges, and the greater also

the ratio of the reflected portion to the total wave. A pebble placed

in the way of the ring-ripples produced by our heavy rain-drops on a

tranquil pond will throw back a large fraction of the ripple incident

upon it, while the fractional part of a larger wave thrown back by the

same pebble might be infinitesimal. Now we have already made it clear

to our minds that to preserve the solar light white, its constituent

proportions must not be altered; but in the act of division performed

by these very small particles we see that the proportions are altered;

an undue fraction of the smaller waves is scattered by the particles,

and, as a consequence, in the scattered light, blue will be the

predominant colour. The other colours of the spectrum must, to some

extent, be associated with the blue. They are not absent but deficient.

We ought, in fact, to have them all, but in diminishing proportions,

from the violet to the red.

We have here presented a case to the imagination, and, assuming the

undulatory theory to be a reality, we have, I think, fairly reasoned

our way to the conclusion, that were particles, small in comparison

to the size of the ether waves, sown in our atmosphere, the light

scattered by those particles would be exactly such as we observe in

our azure skies. When this light is analysed, all the colours of the

spectrum are found; but they are found in the proportions indicated by

our conclusion.

Let us now turn our attention to the light which passes unscattered

among the particles. How must it be finally affected? By its successive

collisions with the particles the white light is more and more robbed

of its shorter waves; it therefore loses more and more of its due

proportion of blue. The result may be anticipated. The transmitted

light, where short distances are involved, will appear yellowish.

But as the sun sinks towards the horizon the atmospheric distances

increase, and consequently the number of the scattering particles.

They abstract in succession the violet, the indigo, the blue, and even

disturb the proportions of green. The transmitted light under such

circumstances must pass from yellow through orange to red. This also is

exactly what we find in nature. Thus, while the reflected light gives

us at noon the deep azure of the Alpine skies, the transmitted light

gives us at sunset the warm crimson of the Alpine snows. The phenomena

certainly occur _as if_ our atmosphere were a medium rendered

slightly turbid by the mechanical suspension of exceedingly small

foreign particles.

Here, as before, we encounter our sceptical ‘_as if_.’ It is

one of the parasites of science, ever at hand, and ready to plant

itself and sprout, if it can, on the weak points of our philosophy.

But a strong constitution defies the parasite, and in our case, as we

question the phenomena, probability grows like growing health, until

in the end the malady of doubt is completely extirpated. The first

question that naturally arises is--Can small particles be really

proved to act in the manner indicated? No doubt of it. Each one of

you can submit the question to an experimental test. Water will not

dissolve resin, but spirit will; and when spirit which holds resin in

solution is dropped into water, the resin immediately separates in

solid particles, which render the water milky. The coarseness of this

precipitate depends on the quantity of the dissolved resin. You can

cause it to separate in thick clots or in exceedingly fine particles.

Professor Brücke has given us the proportions which produce particles

particularly suited to our present purpose. One gramme of clean mastic

is dissolved in eighty-seven grammes of absolute alcohol, and the

transparent solution is allowed to drop into a beaker containing clear

water kept briskly stirred. An exceedingly fine precipitate is thus

formed, which declares its presence by its action upon light. Placing a

dark surface behind the beaker, and permitting the light to fall into

it from the top or front, the medium is seen to be distinctly blue. It

is not perhaps so perfect a blue as I have seen on exceptional days,

this year, among the Alps, but it is a very fair sky-blue. A trace of

soap in water gives a tint of blue. London, and I fear Liverpool milk,

makes an approximation to the same colour through the operation of the

same cause; and Helmholtz has irreverently disclosed the fact that a

blue eye is simply a turbid medium.

The action of turbid media upon light was illustrated by Goethe,

who, though unacquainted with the undulatory theory, was led by his

experiments to regard the firmament as an illuminated turbid medium

with the darkness of space behind it. He describes glasses showing a

bright yellow by transmitted, and a beautiful blue by reflected light.

Professor Stokes, who was probably the first to discern the real nature

of the action of small particles on the waves of ether, describes a

glass of a similar kind.[3] Capital specimens of such glass are to be

found at Salviati’s in St. James’s Street. What artists call ‘chill’ is

no doubt an effect of this description. Through the action of minute

particles, the browns of a picture often present the appearance of

the bloom of a plum. By rubbing the varnish with a silk handkerchief

optical continuity is established, and the chill disappears. Some

years ago I witnessed Mr. Hirst experimenting at Zermatt on the turbid

water of the Visp, which was charged with the finely divided matter

ground down by the glaciers. When kept still for a day or so, the

grosser matter sank, but the finer matter remained suspended, and gave

a distinctly blue tinge to the water. The blueness of certain Alpine

lakes has been shown to be in part due to this cause. Prof. Roscoe has

noticed several striking cases of a similar kind. In a very remarkable

paper the late Principal Forbes showed that steam issuing from the

safety-valve of a locomotive, when favourably observed, exhibits at a

certain stage of its condensation the colours of the sky. It is blue by

reflected light, and orange or red by transmitted light. The effect,

as pointed out by Goethe, is to some extent exhibited by peat smoke.

More than ten years ago I amused myself at Killarney by observing on

a calm day the straight smoke-columns rising from the chimneys of the

cabins. It was easy to project the lower portion of a column against a

dark pine, and its upper portion against a bright cloud. The smoke in

the former case was blue, being seen mainly by reflected light; in the

latter case it was reddish, being seen mainly by transmitted light.

Such smoke was not in exactly the condition to give us the glow of the

Alps, but it was a step in this direction. Brücke’s fine precipitate

above referred to looks yellowish by transmitted light, but by duly

strengthening the precipitate you may render the white light of noon

as ruby-coloured as the sun when seen through Liverpool smoke, or upon

Alpine horizons. I do not, however, point to the gross smoke arising

from coal as an illustration of the action of small particles, because

such smoke soon absorbs and destroys the waves of blue instead of

sending them to the eyes of the observer.

These multifarious facts, and numberless others which cannot now be

referred to, are explained by reference to the single principle, that

where the scattering particles are small in comparison to the size

of the waves we have in the reflected light a greater proportion of

the smaller waves, and in the transmitted light a greater proportion

of the larger waves, than existed in the original white light. The

physiological consequence is that in the one light blue is predominant,

and in the other light orange or red. And now let us push our enquiries

forward. Our best microscopes can readily reveal objects not more than

¹⁄₅₀₀₀₀th of an inch in diameter. This is less than the length of a

wave of red light. Indeed a first-rate microscope would enable us to

discern objects not exceeding in diameter the length of the smallest

waves of the visible spectrum. By the microscope therefore we can

submit our particles to an experimental test. If they are as large as

the light-waves they will infallibly be seen; and if they are not seen

it is because they are smaller. I placed in the hands of our President

a bottle containing Brücke’s particles in greater number and coarseness

than those examined by Brücke himself. The liquid was a milky blue, and

Mr. Huxley applied to it his highest microscopic power. He satisfied

me at the time that had particles of even ¹⁄₁₀₀₀₀₀th of an inch in

diameter existed in the liquid they could not have escaped detection.

But no particles were seen. Under the microscope the turbid liquid was

not to be distinguished from distilled water. Brücke, I may say, also

found the particles to be of ultra-microscopic magnitude.

But we have it in our power to imitate far more closely than we have

hitherto done the natural conditions of this problem. We can generate

in air, as many of you know, artificial skies, and prove their perfect

identity with the natural one, as regards the exhibition of a number

of wholly unexpected phenomena. By a continuous process of growth

moreover we are able to connect sky-matter, if I may use the term,

with molecular matter on the one side, and with molar matter, or

matter in sensible masses, on the other. In illustration of this, I

will take an experiment described by M. Morren of Marseilles at the

last meeting of the British Association. Sulphur and oxygen combine to

form sulphurous acid gas. It is this choking gas that is smelt when a

sulphur match is burnt in air. Two atoms of oxygen and one of sulphur

constitute the molecule of sulphurous acid. Now it has been recently

shown in a great number of instances that waves of ether issuing from

a strong source, such as the sun or the electric light, are competent

to shake asunder the atoms of gaseous molecules. A chemist would call

this ‘decomposition’ by light; but it behoves us, who are examining

the power and function of the imagination, to keep constantly before

us the physical images which we hold to underlie our terms. Therefore

I say, sharply and definitely, that the components of the molecules

of sulphurous acid are shaken asunder by the ether waves. Enclosing

the substance in a suitable vessel, placing it in a dark room, and

sending through it a powerful beam of light, we at first see nothing:

the vessel containing the gas is as empty as a vacuum. Soon, however,

along the track of the beam a beautiful sky-blue colour is observed,

which is due to the liberated particles of sulphur. For a time the blue

grows more intense: it then becomes whitish; and from a whitish blue

it passes to a more or less perfect white. If the action be continued

long enough, we end by filling the tube with a dense cloud of sulphur

particles, which by the application of proper means may be rendered

visible.

Here then our ether waves untie the bond of chemical affinity, and

liberate a body--sulphur--which at ordinary temperatures is a solid,

and which therefore soon becomes an object of the senses. We have

first of all the free atoms of sulphur, which are both invisible and

incompetent to stir the retina sensibly with scattered light. But

these atoms gradually coalesce and form particles, which grow larger

by continual accretion until after a minute or two they appear as

sky-matter. In this condition they are invisible themselves, but

competent to send an amount of wave-motion to the retina sufficient to

produce the firmamental blue. The particles continue, or may be caused

to continue, in this condition for a considerable time, during which no

microscope can cope with them. But they continually grow larger, and

pass by insensible gradations into the state of _cloud_, when they

can no longer elude the armed eye. Thus without solution of continuity

we start with matter in the molecule, and end with matter in the mass,

sky-matter being the middle term of the series of transformations.

Instead of sulphurous acid, we might choose from a dozen other

substances, and produce the same effect with any of them. In the case

of some--probably in the case of all--it is possible to preserve

matter in the skyey condition for fifteen or twenty minutes under

the continual operation of the light. During these fifteen or twenty

minutes the particles are constantly growing larger, without ever

exceeding the size requisite to the production of the celestial blue.

Now when two vessels are placed before you, each containing sky-matter,

it is possible to state with great distinctness which vessel contains

the largest particles. The retina is very sensitive to differences

of light, when, as here, the eye is in comparative darkness, and when

the quantities of wave-motion thrown against the retina are small.

The larger particles declare themselves by the greater whiteness of

their scattered light. Call now to mind the observation, or effort

at observation, made by our President, when he failed to distinguish

the particles of mastic in Brücke’s medium, and when you have done so

follow me. I permitted a beam of light to act upon a certain vapour.

In two minutes the azure appeared, but at the end of fifteen minutes

it had not ceased to be azure. After fifteen minutes, for example,

its colour, and some other phenomena, pronounced it to be a blue of

distinctly smaller particles than those sought for in vain by Mr.

Huxley. These particles, as already stated, must have been less than

¹⁄₁₀₀₀₀₀th of an inch in diameter. And now I want you to submit to

your imagination the following question: Here are particles which have

been growing continually for fifteen minutes, and at the end of that

time are demonstrably smaller than those which defied the microscope

of Mr. Huxley:--_what must have been the size of these particles at

the beginning of their growth?_ What notion can you form of the

magnitude of such particles? The distances of stellar space give us

simply a bewildering sense of vastness without leaving any distinct

impression on the mind, and the magnitudes with which we have here to

do bewilder us equally in the opposite direction. We are dealing with

infinitesimals compared with which the test objects of the microscope

are literally immense.

From their perviousness to stellar light, and other considerations,

Sir John Herschel drew some startling conclusions regarding the

density and weight of comets. You know that these extraordinary and

mysterious bodies sometimes throw out tails 100,000,000 of miles in

length, and 50,000 miles in diameter. The diameter of our earth is

8,000 miles. Both it and the sky, and a good portion of space beyond

the sky, would certainly be included in a sphere 10,000 miles across.

Let us fill this sphere with cometary matter, and make it our unit

of measure. An easy calculation informs us that to produce a comet’s

tail of the size just mentioned about 300,000 such measures would

have to be emptied into space. Now suppose the whole of this stuff

to be swept together, and suitably compressed, what do you suppose

its volume would be? Sir John Herschel would probably tell you that

the whole mass might be carted away at a single effort by one of your

dray-horses. In fact, I do not know that he would require more than

a small fraction of a horse-power to remove the cometary dust. After

this you will hardly regard as monstrous a notion I have sometimes

entertained concerning the quantity of matter in our sky. Suppose a

shell to surround the earth at a height above the surface which would

place it beyond the grosser matter that hangs in the lower regions of

the air--say at the height of the Matterhorn or Mont Blanc. Outside

this shell we have the deep blue firmament. Let the atmospheric space

beyond the shell be swept clean, and let the sky-matter be properly

gathered up. What is its probable amount? I have sometimes thought that

a lady’s portmanteau would contain it all. I have thought that even a

gentleman’s portmanteau--possibly his snuffbox--might take it in. And

whether the actual sky be capable of this amount of condensation or

not, I entertain no doubt that a sky quite as vast as ours, and as good

in appearance, could be formed from a quantity of matter which might be

held in the hollow of the hand.

Small in mass, the vastness in point of number of the particles of

our sky may be inferred from the continuity of its light. It is not

in broken patches, nor at scattered points that the heavenly azure

is revealed. To the observer on the summit of Mont Blanc the blue

is as uniform and coherent as if it formed the surface of the most

close-grained solid. A marble dome would not exhibit a stricter

continuity. And Mr. Glaisher will inform you that if our hypothetical

shell were lifted to twice the height of Mont Blanc above the earth’s

surface, we should still have the azure overhead. Everywhere through

the atmosphere those sky-particles are strewn. They fill the Alpine

valleys, spreading like a delicate gauze in front of the slopes of

pine. They sometimes so swathe the peaks with light as to abolish

their definition. This year I have seen the Weisshorn thus dissolved

in opalescent air. By proper instruments the glare thrown from the

sky-particles against the retina may be quenched, and then the mountain

which it obliterated starts into sudden definition. Its extinction in

front of a dark mountain resembles exactly the withdrawal of a veil. It

is the light then taking possession of the eye, and not the particles

acting as opaque bodies, that interfere with the definition. By day

this light quenches the stars; even by moonlight it is able to exclude

from vision all stars between the fifth and the eleventh magnitude.

It may be likened to a noise, and the stellar radiance to a whisper

drowned by the noise. What is the nature of the particles which shed

light? The celebrated De la Rive ascribes the haze of the Alps in

fine weather to floating organic germs. Now the possible existence

of germs in such profusion has been held up as an absurdity. It has

been affirmed that they would darken the air, and on the assumed

impossibility of their existence in the requisite numbers, without

invasion of the solar light, a powerful argument has been based by

believers in spontaneous generation. Similar arguments have been used

by the opponents of the germ theory of epidemic disease, and both

parties have triumphantly challenged an appeal to the microscope and

the chemist’s balance to decide the question. Such arguments are

absolutely valueless. Without committing myself in the least to De la

Rive’s notion, without offering any objection here to the doctrine of

spontaneous generation, without expressing any adherence to the germ

theory of disease, I would simply draw attention to the fact that in

the atmosphere we have particles which defy both the microscope and the

balance, which do not darken the air, and which exist, nevertheless,

in multitudes sufficient to reduce to insignificance the Israelitish

hyperbole regarding the sands upon the seashore.

The varying judgments of men on these and other questions may perhaps

be, to some extent, accounted for by that doctrine of Relativity which

plays so important a part in philosophy. This doctrine affirms that

the impressions made upon us by any circumstance, or combination of

circumstances, depends upon our previous state. Two travellers upon

the same peak, the one having ascended to it from the plain, the other

having descended to it from a higher elevation, will be differently

affected by the scene around them. To the one nature is expanding, to

the other it is contracting, and feelings are sure to differ which

have two such different antecedent states. In our scientific judgments

the law of relativity may also play an important part. To two men, one

educated in the school of the senses, who has mainly occupied himself

with observation, and the other educated in the school of imagination

as well, and exercised in the conceptions of atoms and molecules to

which we have so frequently referred, a bit of matter, say ¹⁄₅₀₀₀₀th of

an inch in diameter, will present itself differently. The one descends

to it from his molar heights, the other climbs to it from his molecular

lowlands. To the one it appears small, to the other large. So also as

regards the appreciation of the most minute forms of life revealed by

the microscope. To one of these men they naturally appear conterminous

with the ultimate particles of matter, and he readily figures the

molecules from which they directly spring; with him there is but a

step from the atom to the organism. The other discerns numberless

organic gradations between both. Compared with his atoms, the smallest

vibrios and bacteria of the microscopic field are as behemoth and

leviathan. The law of relativity may to some extent explain the

different attitudes of these two men with regard to the question of

spontaneous generation. An amount of evidence which satisfies the

one entirely fails to satisfy the other; and while to the one the

last bold defence and startling expansion of the doctrine will appear

perfectly conclusive, to the other it will present itself as imposing a

profitless labour of demolition on subsequent investigators.[4]

Essays on the use and limit of the imagination in science · 第 2 / 5 段