The upper one, on the right, is the view of a cloud prominence as it

appeared at _half-past twelve_ o’clock, on Sept. 7, 1871. Below it is

the same prominence at _one_ o’clock (half an hour later), when it

has been shattered by some inconceivable explosion, blowing it into

fragments, and driving the hydrogen to a height of two hundred thousand

miles. The lowest figure on the right shows another case where inclined

jets (of hydrogen) were seen to rise to a height of fifty thousand

miles.

Professor Young says of these:--

“Their form and appearance change with great rapidity, so that

the motion can almost be seen with the eye. Sometimes they

consist of pointed rays, diverging in all directions, like

hedgehog-spines. Sometimes they look like flames; sometimes like

sheaves of grain; sometimes like whirling water-spouts, capped

with a great cloud; occasionally they present most exactly the

appearance of jets of liquid fire, rising and falling in graceful

parabolas; frequently they carry on their edges spirals like the

volutes of an Ionic column; and continually they detach filaments

which rise to a great elevation, gradually expanding and growing

fainter as they ascend, until the eye loses them. There is no end

to the number of curious and interesting appearances which they

exhibit under varying circumstances. The velocity of the motions

often exceeds a hundred miles a second, and sometimes, though

very rarely, reaches two hundred miles.”

In the case of the particular phenomenon recorded by Professor Young in

the last illustration, Mr. Proctor, however, has calculated that the

initial velocity probably exceeded five hundred miles a second, which,

except for the resistance experienced by the sun’s own atmosphere,

would have hurled the ejected matter into space entirely clear of the

sun’s power to recall it, so that it would never return.

It adds to our interest in these flames to know that they at least are

connected with that up-rush of heated matter from the sun’s interior,

forming a part of the circulation which maintains both the temperature

of its surface and that radiation on which all terrestrial life

depends. The flames, indeed, add of themselves little to the heat the

sun sends us, but they are in this way the outward and visible signs of

a constant process within, by which we live; and so far they seem to

have a more immediate interest to us, though invisible, than the corona

which surrounds them. But we must remember when we lift our eyes to the

sun that this latter wonder is really there, whether man sees it or

not, and that the cause of its existence is still unknown.

We ask for its “object” perhaps with an unconscious assumption that the

whole must have been in some way provided to subserve _our_ wants; but

there is not as yet the slightest evidence connecting its existence

with any human need or purpose, and as yet we have no knowledge that,

in this sense, it exists to any “end” at all. “As the thought of man is

widened with the process of the suns,” let us hope that we shall one

day know more.

III.

THE SUN’S ENERGY.

“It is indeed,” says good Bishop Berkeley, “an opinion strangely

prevailing amongst men that ... all sensible objects have an existence

... distinct from their being perceived by the understanding. But

... some truths there are, so near and obvious to the mind, that a

man need only open his eyes to see them. Such I take this important

one to be, namely, that all the choir of heaven and furniture of the

earth--in a word, all those bodies which compose the mighty frame of

the world--have not any subsistence without a mind.”

We are not going to take the reader along “the high priori road” of

metaphysics, but only to speak of certain accepted conclusions of

modern experimental physics, which do not themselves, indeed, justify

all of Berkeley’s language, but to which these words of the author of

“A New Theory of Vision” seem to be a not unfit prelude.

When we see a rose-leaf, we see with it what we call a color, and we

are apt to think it is in the rose. But the color is in _us_, for it is

a sensation which something coming from the sun excites in the eye; so

that if the rose-leaf were still there, there would be no color unless

there were an eye to receive and a brain to interpret the sensation.

Every color that is lovely in the rainbow or the flower, every hue

that is vivid in a ribbon or sombre in the grave harmonies of some

old Persian rug, the metallic lustre of the humming-bird or the sober

imperial yellow of precious china,--all these have no existence as

color apart from the seeing eye, and all have their fount and origin in

the sun itself.

“Color” and “light,” then, are not, properly speaking, external things,

but names given to the sensations caused by an uncomprehended something

radiated from the sun, when this falls on our eyes. If this very same

something falls on our face, it produces another kind of sensation,

which we call “heat,” or if it falls on a thermometer it makes it rise;

while if it rests long on the face it will produce yet another effect,

“chemical action,” for it will _tan_ the cheek, producing a chemical

change there; or it will do the like work more promptly if it meet a

photographic plate. If we bear in mind that it is the identically same

thing (whatever that is) which produces all these diverse effects, we

see, some of us perhaps for the first time, that “color,” “light,”

“radiant heat,” “actinism,” etc., are only names given to the diverse

effects of some thing, not things themselves; so that, for instance,

all the splendor of color in the visible world _exists only in the

eye that sees it_. The reader must not suppose that he is here being

asked to entertain any metaphysical subtlety. We are considering a fact

almost universally accepted within the last few years by physicists,

who now generally admit the existence of a something coming from the

sun, which is not itself light, heat, or chemical action, but of which

these are effects. When we give this unknown thing a name, we call it

“radiant energy.”

How it crosses the void of space we cannot be properly said to know,

but all the phenomena lead us to think it is in the form of motion

in some medium,--somewhat (to use an imperfect analogy) like the

transmission through the air of the vibrations which will cause sound

when they reach an ear. This, at any rate, is certain, that there is an

action of some sort incessantly going on between us and the sun, which

enables us to experience the effects of light and heat. We assume

it to be a particular mode of vibration; but whatever it is, it is

repeated with incomprehensible rapidity. Experiments recently made by

the writer show that the _slower_ heat vibrations which reach us from

the sun succeed each other nearly 100,000,000,000,000 times in a single

second, while those which make us see, have long been known to be more

rapid still. These pass outward from the sun in every direction, in

ever-widening spheres; and in them, so far as we know, lies the potency

of life for the planet upon whose surface they fall.

Did the reader ever consider that next to the mystery of gravitation,

which draws all things on the earth’s surface down, comes that

mystery--not seen to be one because so familiar--of the occult force

in the sunbeams which lifts things _up_? The incomprehensible energy

of the sunbeam brought the carbon out of the air, put it together in

the weed or the plant, and lifted each tree-trunk above the soil. The

soil did not lift it, any more than the soil in Broadway lifted the

spire of Trinity. Men brought stones there in wagons to build the

church, and the sun brought the materials in its own way, and built up

alike the slender shaft that sustains the grass blade and the column

of the pine. If the tree or the spire fell, it would require a certain

amount of work of men or horses or engines to set it up again. So much

actual work, at least, the sun did in the original building; and if we

consider the number of trees in the forest, we see that this alone is

something great. But besides this, the sun locked up in each tree a

store of energy thousands of times greater than that which was spent in

merely lifting the trunk from the ground, as we may see by unlocking

it again, when we burn the tree under the boiler of an engine; for it

will develop a power equal to the lifting of thousands of its kind,

if we choose to employ it in this way. This is so true, that the tree

may fall, and turn to coal in the soil, and still keep this energy

imprisoned in it,--keep it for millions of years, till the black lump

under the furnace gives out, in the whirling spindles of the factory or

the turning wheel of the steamboat, the energy gathered in the sunshine

of the primeval world.

The most active rays in building up plant-life are said to be the

yellow and orange, though Nature’s fondness for green everywhere is

probably justified by some special utility. At any rate, the action

of these solar rays is to decompose the products of combustion, to

set free the oxygen, and to fix the carbon in the plant. Perhaps

these words do not convey a definite meaning to the reader, but it

is to be hoped they will, for the statement they imply is wonderful

enough. Swift’s philosopher at Laputa, who had a project for extracting

sunbeams out of cucumbers, was wiser than his author knew; for

cucumbers, like other vegetables, are now found to be really in large

part put together by sunbeams, and sunbeams, or what is scarcely

distinguishable from such, could with our present scientific knowledge

be extracted from cucumbers again, only the process would be too

expensive to pay. The sunbeam, however, does what our wisest chemistry

cannot do: it takes the burned out ashes and makes them anew into green

wood; it takes the close and breathed out air, and makes it sweet and

fit to breathe by means of the plant, whose food is the same as our

poison. With the aid of sunlight a lily would thrive on the deadly

atmosphere of the “black hole of Calcutta;” for this bane to us, we

repeat, is vital air to the plant, which breathes it in through all its

pores, bringing it into contact with the chlorophyl, its green blood,

which is to it what the red blood is to us; doing almost everything,

however, by means of the sun ray, for if this be lacking, the oxygen is

no longer set free or the carbon retained, and the plant dies. This too

brief statement must answer instead of a fuller description of how the

sun’s energy builds up the vegetable world.

But the ox, the sheep, and the lamb feed on the vegetable, and we in

turn on them (and on vegetables too); so that, though we might eat

our own meals in darkness and still live, the meals themselves are

provided literally at the sun’s expense, virtue having gone out of him

to furnish each morsel we put in our mouths. But while he thus prepares

the material for our own bodies, and while it is plain that without him

we could not exist any more than the plant, the processes by which he

acts grow more intricate and more obscure in our own higher organism,

so that science as yet only half guesses how the sun makes us. But the

making is done in some way by the sun, and so almost exclusively is

every process of life.

It is not generally understood, I think, how literally true this is

of every object in the organic world. In a subsequent illustration

we shall see a newspaper being printed by power directly and visibly

derived from the sunbeam. But all the power derived from coal, and all

the power derived from human muscles, comes originally from the sun,

in just as literal a sense; for the paper on which the reader’s eye

rests was not only made primarily from material grown by the sun, but

was stitched together by derived sun-power, and by this, also, each

page was printed, so that the amount of this solar radiation expended

for printing each chapter of this book could be stated with approximate

accuracy in figures. To make even the reader’s hand which holds this

page, or the eye which sees it, energy again went out from the sun; and

in saying this I am to be understood in the plain and common meaning of

the words.

Did the reader ever happen to be in a great cotton-mill, where many

hundreds of operatives watched many thousands of spindles? Nothing is

visible to cause the multiplied movement, the engine being perhaps away

in altogether another building. Wandering from room to room, where

everything is in motion derived from some unseen source, he may be

arrested in his walk by a sudden cessation of the hum and bustle,--at

once on the floor below, and on that above, and all around him. The

simultaneousness of this stoppage at points far apart when the steam

is turned off, strikes one with a sense of the intimate dependence of

every complex process going on upon some remote invisible motor. The

cessation is not, however, absolutely instantaneous; for the great

fly-wheel, in which a trifling part of the motor power is stored, makes

one or two turns more, till the energy in this also is exhausted,

and all is still. The coal-beds and the forests are to the sun what

the fly-wheel is to the engine: all their power comes from him; they

retain a little of it in store, but very little by comparison with the

original; and were the change we have already spoken of to come over

the sun’s circulation,--were the solar engine disconnected from us,--we

could go on perhaps a short time at the cost of this store, but when

this was over it would be over with us, and all would be still here too.

Is there not a special interest for us in that New Astronomy which

considers these things, and studies the sun, not only in the heavens as

a star, but in its workings here, and so largely in its relations to

man?

* * * * *

Since, then, we are the children of the sun, and our bodies a product

of its rays, as much as the ephemeral insects that its heat hatches

from the soil, it is a worthy problem to learn how things earthly

depend upon this material ruler of our days. But although we know it

does nearly all things done on the earth, and have learned a little of

the way it builds up the plant, we know so little of the way it does

many other things here that we are still often only able to connect the

terrestrial effect with the solar cause by noting what events happen

together. We are in this respect in the position of our forefathers,

who had not yet learned the science of electricity, but who noted

that when a flash of lightning came a clap of thunder followed, and

concluded as justly as Franklin or Faraday could have done that there

was a physical relation between them. Quite in this way, we who are in

a like position with regard to the New Astronomy, which we hope will

one day explain to us what is at present mysterious in our connection

with the sun, can as yet often only infer that when certain phenomena

there are followed or accompanied by others here, all are really

connected as products of one cause, however dissimilar they may look,

and however little we know what the real connection may be.

There is no more common inquiry than as to the influence of sun-spots

on the weather; but as we do not yet know the real nature of the

connection, if there be any, we can only try to find out by assembling

independent records of sun-spots and of the weather here, and noticing

if any changes in the one are accompanied by changes in the other; to

see, for instance, if when sun-spots are plenty the weather the world

over is rainy or not, or to see if when an unusual disturbance breaks

out in a sun-spot any terrestrial disturbance is simultaneously noted.

[Illustration: FIG. 48.--SUN-SPOTS AND PRICE OF GRAIN. (FROM

“OBSERVATIONS OF SOLAR SPOTS.”)]

When we remember how our lives depend on a certain circulation in

the sun, of which the spots appear to be special examples, it is of

interest not only to study the forms within them, as we have already

been doing here, but to ask whether the spots themselves are present

as much one year as another. The sun sometimes has numerous spots on

it, and sometimes none at all; but it does not seem to have occurred to

any one to see whether they had any regular period for coming or going,

till Schwabe, a magistrate in a little German town, who happened to

have a small telescope and a good deal of leisure, began for his own

amusement to note their number every day. He commenced in 1826, and

with German patience observed daily for forty years. He first found

that the spots grew more numerous in 1830, when there was no single

day without one; then the number declined very rapidly, till in 1833

they were about gone; then they increased in number again till 1838,

then again declined; and so on, till it became evident that sun-spots

do not come and go by chance, but run through a cycle of growth and

disappearance, on the average about once in every eleven years. While

amusing himself with his telescope, an important sequence in Nature had

thus been added to our knowledge by the obscure Hofrath Schwabe, who

indeed compares himself to Saul, going out to seek his father’s asses

and finding a kingdom. Old records made before Schwabe’s time have

since been hunted up, so that we have a fairly connected history of the

sun’s surface for nearly a hundred and fifty years; and the years when

spots will be plentiful or rare can now be often predicted from seeing

what has been in the past. Thus I may venture to say that the spots, so

frequent in 1885, will have probably nearly disappeared in 1888, and

will be probably very plentiful in 1894. I do not know at all why this

is likely to happen; I only know that it has repeatedly happened at

corresponding periods in the past.

“Now,” it may be asked, “have these things any connection with weather

changes, and is it of any practical advantage to know if they have?”

Would it be, it may be answered, of any practical interest to a

merchant in bread-stuffs to have private information of a reliable

character that crops the world over would be fine in 1888 and fail in

1894? The exclusive possession of such knowledge might plainly bring

“wealth beyond the dreams of avarice” to the user; or, to ascend

from the lower ground of personal interest to the higher aims of

philanthropy and science, could we predict the harvests, we should

be armed with a knowledge that might provide against coming years of

famine, and make life distinctly happier and easier to hundreds of

millions of toilers on the earth’s surface.

“But can we predict?” We certainly cannot till we have, at any rate,

first shown that there is a connection between sun-spots and the

weather. Since we know nothing of the ultimate causes involved, we can

only at present, as I say, collect records of the changes there, and

compare them with others of the changes here, to see if there is any

significant coincidence. To avoid columns of figures, and yet to enable

the reader to judge for himself in some degree of the evidence, I will

give the results of some of these records represented graphically by

curves, like those which he may perhaps remember to have seen used to

show the fluctuations in the value of gold and grain, or of stocks in

the stock-market. It is only fair to say that mathematicians used this

method long before it was ever heard of by business men, and that the

stockbrokers borrowed it from the astronomers, and not the astronomers

from them.

In Fig. 48, from Carrington’s work, each horizontal space represents

ten years of time, and the figures in the upper part represent the

fluctuations of the sun-spot curve. In the middle curve, variations

in vertical distances correspond to differences in the distance from

the sun of the planet Jupiter, the possibility of whose influence

on sun-spot periods can thus be examined. In the third and lowest,

suggested by Sir William Herschel, the figures at the side are

proportional to the price of wheat in the English market, rising when

wheat ruled high, falling when it was cheap. In all three curves

one-tenth of a horizontal spacing along the top or bottom corresponds

to one year; and in this way we have at a glance the condensed result

of observations and statistics for sixty years, which otherwise stated

would fill volumes. The result is instructive in more ways than one.

The variations of Jupiter’s distance certainly do present a striking

coincidence with the changes in spot frequency, and this may indicate

a real connection between the phenomena; but before we decide that

it does so, we must remember that the number of cycles of change

presented by the possible combination of planetary periods is all but

infinite. Thus we might safely undertake, with study enough, to find a

curve, depending solely on certain planetary configurations, which yet

would represent with quite striking agreement for a time the rise and

fall in any given railroad stock, the relative numbers of Democratic

and Republican congressmen from year to year, or anything else with

which the heavenly bodies have in reality as little to do. The third

curve (meant by the price of wheat to test the possible influence of

sun-spots on years of good or bad harvests) is not open to the last

objection, but involves a fallacy of another kind. In fact the price

of wheat depends on many things quite apart from the operations of

Nature,--on wars and legislation, for instance; and here the great

rise in the first years of the century is as clearly connected with the

great continental wars of the first Napoleon, which shut up foreign

ports, as the sudden fall about 1815, the year of Waterloo, is with

the subsequent peace. Meanwhile an immense amount of labor has been

spent in making tables of the weather, and of almost every conceivable

earthly phenomenon which may be supposed to have a similar periodic

character, with very doubtful success, nearly every one having brought

out some result which might be plausible if it stood alone, but which

is apt to be contradicted by the others. For instance, Mr. Stone,

at the Cape of Good Hope, and Dr. Gould, in South America, consider

that the observations taken at those places show a little diminution

of the earth’s temperature (amounting to one or two degrees) at a

sun-spot maximum. Mr. Chambers concludes, from twenty-eight years’

observations, that the hottest are those of most sun-spots. So each of

these contradicts the other. Then we have Gelinck, who, from a study of

numerous observations, concludes that all are wrong together, and that

there is really no change in either way.

[Illustration: FIG. 49.--SUN-SPOT OF NOV. 16, 1882, AND EARTH.]

I might go on citing names with no better result. One observer

tabulates observations of terrestrial temperature, or rain-fall, or

barometer, or ozone; another, the visitations of Asiatic cholera; while

still another (the late Professor Jevons) tabulates commercial crises

with the serious attempt to find a connection between the sun-spots and

business panics. Of making such cycles there is no end, and much study

of them would be a weariness I will not inflict.

[Illustration: FIG. 50.--GREENWICH RECORD OF DISTURBANCE OF MAGNETIC

NEEDLE, NOV. 16 AND 17, 1882.]

Our own conclusion is, that from such investigations of terrestrial

changes nothing is yet certainly known with regard to the influence

of sun-spots on the weather. There is, however, quite another way;

that is, to measure their effect at the origin in the sun itself.

The sun-spot is cooler than the rest of the surface, and it might be

thought that when there are many the sun would give less heat. As far

as the spots themselves are concerned, this is so, but in a very small

degree. I have been able to ascertain how much this deprivation of heat

amounts to, and find it is a real but a most insignificant quantity,

rising to about two-thirds of one degree Fahrenheit every eleven

years. This, it will be remembered, is the direct effect of the spots

considered merely as so many cool patches on the surface, and it does

not imply that when there are most spots the sun will necessarily give

less heat. In fact there may be a compensating action accompanying them

which makes the radiation greater than when they are absent. I will not

enter on a detailed explanation, but only say that in the best judgment

I can form by a good deal of study and direct experiment, there is no

certain evidence that the sun is hotter at one time than at another.

The New Astronomy · 第 4 / 14 段