THE CONSTITUTION OF THE SUN.

[_First published in_ The Reader _for February_ 25, 1865. _I

reproduce this essay chiefly to give a place to the speculation

concerning the solar spots which forms the latter portion of it._]

The hypothesis of M. Faye, described in your numbers for January 28 and

February 4, respectively, is to a considerable extent coincident with

one which I ventured to suggest in an article on "Recent Astronomy and

the Nebular Hypothesis," published in the _Westminster Review_ for July,

1858. In considering the possible causes of the immense differences of

specific gravity among the planets, I was led to question the validity

of the tacit assumption that each planet consists of solid or liquid

matter from centre to surface. It seemed to me that any other internal

structure which was mechanically stable, might be assumed with equal

legitimacy. And the hypothesis of a solid or liquid shell, having its

cavity filled with gaseous matter at high pressure and temperature [and

of great density], was one which seemed worth considering.

Hence arose the inquiry--What structure will result from the process of

nebular condensation? [Here followed a long speculation respecting the

processes going on in a concentrating nebulous spheroid; the general

outcome of which is implied in Note III of the foregoing essay. I do not

reproduce it because, not having the guidance of Prof. Andrew's

researches, I had concluded that the formation of a molten shell would

occur universally, instead of occasionally, as is now argued in the

note named. The essay then proceeded thus:--]

The process of condensation being in its essentials the same for all

concentrating nebular spheroids, planetary or solar, it was argued that

the Sun is still passing through that incandescent stage which all the

planets have long ago passed through: his later aggregation, joined with

the immensely greater ratio of his mass to his surface, involving

comparative lateness of cooling. Supposing the sun to have reached the

state of a molten shell, inclosing a gaseous nucleus, it was concluded

that this molten shell, ever radiating its heat, but ever acquiring

fresh heat by further integration of the Sun's mass, must be constantly

kept up to that temperature at which its substance evaporates.

[Here followed part of the paragraph quoted in the preceding essay on p.

155; and there succeeded, in subsequent editions, a paragraph aiming to

show that the inferred structure of the Sun's interior was congruous

with the low specific gravity of the Sun--a conclusion which, as

indicated on p. 156, implies some very problematical assumptions

respecting the natures of the unknown elements of the Sun. There then

came this passage:--]

The conception of the Sun's constitution thus set forth, is like that of

M. Faye in so far as the successive changes, the resulting structures,

and the ultimate state, are concerned; but unlike it in so far as the

Sun is supposed to have reached a later stage of concentration. As I

gather from your abstract of M. Faye's paper [this referred to an

article in _The Reader_], he considers the Sun to be at present a

gaseous spheroid, having an envelope of metallic matters precipitated in

the shape of luminous clouds, the local dispersions of which, caused by

currents from within, appear to us as spots; and he looks forward to the

future formation of a liquid film as an event that will soon be followed

by extinction. Whereas the above hypothesis is that the liquid film

already exists beneath the visible photosphere, and that extinction

cannot result until, in the course of further aggregation, the gaseous

nucleus has become so much reduced, and the shell so much thickened,

that the escape of the heat generated is greatly retarded.... M. Faye's

hypothesis appears to be espoused by him, partly because it affords an

explanation of the spots, which are considered as openings in the

photosphere, exposing the comparatively non-luminous gases filling the

interior. But if these interior gases are non-luminous from the absence

of precipitated matter, must they not for the same reason be

transparent? And if transparent, will not the light from the remote side

of the photosphere seen through them, be nearly as bright as that of the

side next to us? By as much as the intensely-heated gases of the

interior are disabled by the dissociation of their molecules from giving

off luminiferous undulations, by so much must they be disabled from

absorbing the light transmitted through them. And if their great

light-transmitting power is exactly complementary to their small

light-emitting power, there seems no reason why the interior of the Sun,

disclosed to us by openings in the photosphere, should not appear as

bright as its exterior.

Take, on the other hand, the supposition that a more advanced state of

concentration has been reached. A shell of molten metallic matter

enclosing a gaseous nucleus still higher in temperature than itself,

will be continually kept at the highest temperature consistent with its

state of liquid aggregation. Unless we assume that simple radiation

suffices to give off all the heat generated by progressing integration,

we must conclude that the mass will be raised to that temperature at

which part of its heat is absorbed in vaporizing its superficial parts.

The atmosphere of metallic gases hence resulting, cannot continue to

accumulate without reaching a height above the Sun's surface, at which

the cooling due to radiation and rarefaction will cause condensation

into cloud--cannot, indeed, cease accumulating until the precipitation

from the upper limit of the atmosphere balances the evaporation from its

lower limit. This upper limit of the atmosphere of metallic gases,

whence precipitation is perpetually taking place, will form the visible

photosphere--partly giving off light of its own, partly letting through

the more brilliant light of the incandescent mass below. This conclusion

harmonizes with the appearances. Sir John Herschel, advocating though he

does an antagonist hypothesis, gives a description of the Sun's surface

which agrees completely with the processes here supposed. He says:--

"There is nothing which represents so faithfully this appearance as

the slow subsidence of some flocculent chemical precipitates in a

transparent fluid, when viewed perpendicularly from above: so

faithfully, indeed, that it is hardly possible not to be impressed

with the idea of a luminous medium intermixed, but not confounded,

with a transparent and non-luminous atmosphere, either floating as

clouds in our air, or pervading it in vast sheets and columns like

flame, or the streamers of our northern lights".--_Treatise on

Astronomy_, p. 208.

If the constitution of the Sun be that which is above inferred, it does

not seem difficult to conceive still more specifically the production of

these appearances. Everywhere throughout the atmosphere of metallic

vapours which clothes the solar surface, there must be ascending and

descending currents. The magnitude of these currents must obviously

depend on the depth of this atmosphere. If it is shallow, the currents

must be small; but if many thousands of miles deep, the currents may be

wide enough to render visible to us the places at which they severally

impinge on the limit of the atmosphere, and the places whence the

descending currents commence. The top of an ascending current will be a

space over which the thickness of condensed cloud is the least, and

through which the greatest amount of light from beneath penetrates. The

clouds perpetually formed at the top of such a current, will be

perpetually thrust aside by the uncondensed gases from below them; and,

growing while they are thrust aside, will collect in the spaces between

the ascending currents, where there will result the greatest degree of

opacity. Hence the mottled appearance--hence the "pores," or dark

interspaces, separating the light-giving spots.[25]

Of the more special appearances which the photosphere presents, let us

take first the faculae. These are ascribed to waves in the photosphere;

and the way in which such waves might produce an excess of light has

been variously explained in conformity with various hypotheses. What

would result from them in a photosphere constituted and conditioned as

above supposed? Traversing a canopy of cloud, here thicker and there

thinner, a wave would cause a disturbance very unlikely to leave the

thin and thick parts without any change in their average permeability to

light. There would probably be, at some parts of the wave, extensions in

the areas of the light-transmitting clouds, resulting in the passage of

more rays from below. Another phenomenon, less common but more striking,

appears also to be in harmony with the hypothesis. I refer to those

bright spots, of a brilliancy greater than that of the photosphere,

which are sometimes observed. In the course of a physical process so

vast and so active as that here supposed to be going on in the Sun, we

may expect that concurrent causes will occasionally produce ascending

currents much hotter than usual, or more voluminous, or both. One of

these, on reaching the stratum of luminous and illuminated cloud forming

the photosphere, will burst through it, dispersing and dissolving it,

and ascending to a greater height before it begins itself to condense:

meanwhile allowing to be seen, through its transparent mass, the

incandescent molten shell of the sun's body.

[The foregoing passages, to most of which I do not commit myself as more

than possibilities, I republish chiefly as introductory to the following

speculation, which, since it was propounded in 1865, has met with some

acceptance.]

"But what of the spots commonly so called?" it will be asked. In the

essay on the Nebular hypothesis, above quoted from, it was suggested

that refraction of the light passing through the depressed centres of

cyclones in this atmosphere of metallic gases, might possibly be the

cause; but this, though defensible as a "true cause," appeared on

further consideration to be an inadequate cause. Keeping the question in

mind, however, and still taking as a postulate the conclusion of Sir

John Herschel, that the spots are in some way produced by cyclones, I

was led, in the course of the year following the publication of the

essay, to an hypothesis which seemed more satisfactory. This, which I

named at the time to Prof. Tyndall, had a point in common with the one

afterward published by Prof. Kirchhoff, in so far as it supposed cloud

to be the cause of darkness; but differed in so far as it assigned the

cause of such cloud. More pressing matters prevented me from developing

the idea for some time; and, afterwards, I was deterred from including

it in the revised edition of the essay, by its inconsistency with the

"willow-leaf" doctrine, at that time dominant. The reasoning was as

follows:--The central region of a cyclone must be a region of

rarefaction, and, consequently, a region of refrigeration. In an

atmosphere of metallic gases rising from a molten surface, and presently

reaching a limit at which condensation takes place, the molecular state,

especially toward its upper part, must be such that a moderate

diminution of density, and fall of temperature, will cause

precipitation. That is to say, the rarefied interior of a solar cyclone

will be filled with cloud: condensation, instead of taking place only

at the level of the photosphere, will here extend to a great depth below

it, and over a wide area. What will be the characters of a cloud thus

occupying the interior of a cyclone? It will have a rotatory motion; and

this it has been seen to have. Being funnel-shaped, as analogy warrants

us in assuming, its central parts will be much deeper than its

peripheral parts, and therefore more opaque. This, too, corresponds with

observation. Mr. Dawes has discovered that in the middle of the spot

there is a blacker spot: just where there would exist a funnel-shaped

prolongation of the cyclonic cloud down toward the Sun's body, the

darkness is greater than elsewhere. Moreover, there is furnished an

adequate reason for the depression which one of these dark spaces

exhibits. In a whirlwind, as in a whirlpool, the vortex will be below

the general level, and all around, the surface of the medium will

descend toward it. Hence a spot seen obliquely, as when carried toward

the Sun's limb, will have its umbra more and more hidden, while its

penumbra still remains visible. Nor are we without some interpretation

of the penumbra. If, as is implied by what has been said, the so-called

"willow-leaves," or "rice-grains," are the tops of the currents

ascending from the Sun's body, what changes of appearance are they

likely to undergo in the neighbourhood of a cyclone? For some distance

round a cyclone there will be a drawing in of the superficial gases

toward the vortex. All the luminous spaces of more transparent cloud

forming the adjacent photosphere, will be changed in shape by these

centripetal currents. They will be greatly elongated; and there will so

be produced that "thatch"-like aspect which the penumbra presents.

* * * * *

[The explanation of the solar spots above suggested, which was

originally propounded in opposition to that of M. Faye, was eventually

adopted by him in place of his own. In the _Comptes Rendus_ for 1867,

Vol. LXIV., p. 404, he refers to the article in the _Reader_, partly

reproduced above, and speaks of me as having been replied to in a

previous note. Again in the _Comptes Rendus_ for 1872, Vol. LXXV., p.

1664, he recognizes the inadequacy of his hypothesis, saying:--"Il est

certain que l'objection de M. Spencer, reproduit et developpee par M.

Kirchoff, est fondee jusqu'a un certain point; l'interieur des taches,

si ce sont des lacunes dans la photosphere, doit etre froid

relativement.... Il est donc impossible qu'elles proviennent d'eruptions

ascendantes." He then proceeds to set forth the hypothesis that the

spots are caused by the precipitation of vapour in the interiors of

cyclones. But though, as above shown, he refers to the objection made in

the foregoing essay to his original hypothesis, and recognizes its

cogency, he does not say that the hypothesis which he thereupon

substitutes is also to be found in the foregoing essay. Nor does he

intimate this in the elaborate paper on the subject read before the

French Association for the Advancement of Science, and published in the

_Revue Scientifique_ for the 24th March 1883. The result is that the

hypothesis is now currently ascribed to him.[26]

About four months before I had to revise this essay on "The Constitution

of the Sun," while staying near Pewsey, in Wiltshire, I was fortunate

enough to witness a phenomenon which furnished, by analogy, a

verification of the above hypothesis, and served more especially to

elucidate one of the traits of solar spots, otherwise difficult to

understand. It was at the close of August, when there had been a spell

of very hot weather. A slight current of air from the West, moving along

the line of the valley, had persisted through the day, which, up to 5

o'clock, had been cloudless, and, with the exception now to be named,

remained cloudless. The exception was furnished by a strange-looking

cloud almost directly overhead. Its central part was comparatively dense

and structureless. Its peripheral part, or to speak strictly, the

two-thirds of it which were nearest and most clearly visible, consisted

of _converging streaks_ of comparatively thin cloud. Possibly the third

part on the remoter side was similarly constituted; but this I could not

see. It did not occur to me at the time to think about its cause,

though, had the question been raised, I should doubtless have concluded

that as the sky still remained cloudless everywhere else, this

precipitated mass of vapour must have resulted from a local eddy. In the

space of perhaps half-an-hour, the gentle breeze had carried this cloud

some miles to the East; and now its nature became obvious. That central

part which, seen from underneath, seemed simply a dense, confused part,

apparently no nearer than the rest, now, seen sideways, was obviously

much lower than the rest and rudely funnel-shaped--nipple-shaped one

might say; while the wide thin portion of cloud above it was

disk-shaped: the converging streaks of cloud being now, in perspective,

merged together. It thus became manifest that the cloud was produced by

a feeble whirlwind, perhaps a quarter to half-a-mile in diameter.

Further, the appearances made it clear that this feeble whirlwind was

limited to the lower stratum of air: the stratum of air above it was not

implicated in the cyclonic action. And then, lastly, there was the

striking fact that the upper stratum, though not involved in the whirl,

was, by its proximity to a region of diminished pressure, slightly

rarified; and that its precipitated vapour was, by the draught set up

towards the vortex below, drawn into converging streaks. Here, then, was

an action analogous to that which, as above suggested, happens around a

sun-spot, where the masses of illuminated vapour constituting the

photosphere are drawn towards the vortex of the cyclone, and

simultaneously elongated into striae: so forming the penumbra. At the

same time there was furnished an answer to the chief objection to the

cyclonic theory of solar spots. For if, as here seen, a cyclone in a

lower stratum may fail to communicate a vortical motion to the stratum

above it, we may comprehend how, in a solar cyclone, the photosphere

commonly fails to give any indication of the revolving currents below,

and is only occasionally so entangled in these currents as itself to

display a vortical motion.

Let me add that apart from the elucidations furnished by the phenomenon

above described, the probabilities are greatly in favour of the cyclonic

origin of the solar spots. That some of them exhibit clear marks of

vortical motion is undeniable; and if this is so, the question

arises--What is the degree of likelihood that there are two causes for

spots? Considering that they have so many characters in common, it is

extremely improbable that their common characters are in some cases the

concomitants of vortical motion and in other cases the concomitants of a

different kind of action. Recognizing this great improbability, even in

the absence of a reconciliation between the apparently conflicting

traits, it is, I think, clear that when, in the way above shown, we are

enabled to understand how it happens that the vortical motion, not

ordinarily implicating the photosphere, may consequently be in most

cases unapparent, the reasons for accepting the cyclonic theory become

almost conclusive.]

Essays: Scientific, Political, & Speculative; Vol. 1 of 3 Library Edition (1891), Containing Seven Essays not before Republished, and Various other Additions. · 第 33 / 55 题