I do not, however, in this place enter specially into the consideration

of the moon's stage of volcanic activity, because already, in the pages

of my Treatise on the Moon (Chapter VI.), I have given a full account

of that portion of my present subject. I may make a few remarks,

however, on the theory respecting lunar craters touched on in my work

on 'The Moon.' I have mentioned the possibility that some among the

enormous number of ring-shaped depressions which are seen on the moon's

surface may have been the result of meteoric downfalls in long past

ages of the moon's history. One or two critics have spoken of this view

as though it were too fantastic for serious consideration. Now, though

I threw out the opinion merely as a suggestion, distinctly stating

that I should not care to maintain it as a theory, and although my

own opinion is unfavourable to the supposition that any of the more

considerable lunar markings can be explained in the suggested way, yet

it is necessary to notice that on the general question whether the

moon's surface has been marked or not by meteoric downfalls scarcely

any reasonable doubts can be entertained. For, first, we can scarcely

question that the moon's surface was for long ages plastic, and though

we may not assign to this period nearly so great a length (350 millions

of years) as Tyndall--following Bischoff--assigns to the period when

our earth's surface was cooling from a temperature of 2000° C. to

200°, yet still it must have lasted millions of years; and, secondly,

we cannot doubt that the process of meteoric downfall now going on is

not a new thing, but, on the contrary, is rather the final stage of a

process which once took place far more actively. Now Prof. Newton has

estimated, by a fair estimate of observed facts, that each day on the

average 400 millions of meteors fall, of all sizes down to the minutest

discernible in a telescope, upon the earth's atmosphere, so that on

the moon's unprotected globe--with its surface one thirteenth of the

earth's--about 30 millions fall each day, even at the present time. Of

large meteoric masses only a few hundreds fall each year on the earth,

and perhaps about a hundred on the moon; but still, even at the present

rate of downfall, millions of large masses _must_ have fallen on the

moon during the time when her surface was plastic, while _probably_ a

much larger number--including many much larger masses--must have fallen

during that period. Thus, not only without straining probabilities, but

by taking only the most probable assumptions as to the past, we have

arrived at a result which compels us to believe that the moon's surface

has been very much marked by meteoric downfall, while it renders it by

no means unlikely that a large proportion of the markings so left would

be discernible under telescopic scrutiny.

I would, in conclusion, invite those who have the requisite leisure to

a careful study of the distribution of various orders of lunar marking.

It would be well if the moon's surface were isographically charted,

and the distribution of the seas, mountain ranges, and craters of

different dimensions and character, of rills, radiating streaks, bright

and dark regions, and so on, carefully compared _inter se_, with the

object of determining whether the different parts of the moon's surface

were probably brought to their present condition during earlier or

later periods, and of interpreting also the significance of the moon's

characteristic peculiarities. In this department of astronomy, as in

some others, the effectiveness of well-devised processes of charting

has been hitherto overlooked.

FOOTNOTES:

[Footnote 8: It would still be somewhat denser, because under the

circumstances it would be somewhat cooler.]

[Footnote 9: It is thus, and not by the effects due to increasing

pressure (effects which probably do not increase beyond a certain

point), that we are to explain the fact that the earth's density as a

whole is about twice the mean density of the matters which form its

solid surface. It may be that this consideration, supported by the

results of recent experimental researches, may give a significance

hitherto not noted to the relatively small mean density of the moon.]

[Footnote 10: I have occasion to make some remarks at this stage

to avoid possible and (my experience has shown me) not altogether

improbable misconception, or even misrepresentation. The theory

enunciated above will be regarded by some, who may have read a certain

review of my Treatise on the Moon, as totally different from what I

have advocated in that work, and, furthermore, as a theory which I

have borrowed from the aforesaid review. I should not be particularly

concerned if I had occasion to modify views I had formerly expressed,

since I apprehend that every active student of science should hope,

rather than dread, that as his work proceeds he would form new

opinions. But I must point out that earlier in my book I had advocated

the theory urged above. After describing the radiations from Tycho

and other craters, I proceed as follows in chapter iv.--'It appears

to me impossible to refer these phenomena to any general cause but

the reaction of the moon's interior overcoming the tension of the

crust, and to this degree Nasmyth's theory seems correct; but it

appears manifest, also, that the crust cannot have been fractured

in the ordinary sense of the word. Since, however, it results from

Mallet's investigations that the tension of the crust is called into

play in the earlier stages of contraction, and its power to resist

contraction in the later stages,--in other words, since the crust at

first contracts faster than the nucleus, and afterwards not so fast as

the nucleus,--we may assume that the radiating systems were formed in

so early an era that the crust was plastic. And it seems reasonable to

conclude that the outflowing matter would retain its liquid condition

long enough (the crust itself being intensely hot) to spread widely,--a

circumstance which would account at once for the breadth of many of

the rays, and for the restoration of level to such a degree that no

shadows are thrown. It appears probable, also, that not only (which is

manifest) were the craters formed later which are seen around and upon

the radiations, but that the central crater itself acquired its actual

form long after the epoch when the rays were formed.']

[Footnote 11: Where several ray centres are near together, a region

directly between two ray centres would be at a level intermediate

between that of the ray centres and that of a region centrally placed

within a triangle or quadrangle of ray centres; but the latter region

might be at a higher level than another very far removed from the part

where the ray centres were near together. For instance, the space in

the middle of the triangle having Copernicus, Aristarchus, and Kepler

at its angles (or more exactly between Milichius and Bessarion) is

lower than the surface around Hortensius (between Copernicus and

Kepler), but not so low as the Mare Imbrium, far away from the region

of ray centres of which Copernicus, Aristarchus, and Kepler are the

principal.]

[Footnote 12: It is important to notice that we may derive from these

considerations an argument as to the condition of the fluid matter now

existing beneath the solid crust of the earth.]

_A NEW CRATER IN THE MOON._

Dr. Klein, a German astronomer, has recently called the attention of

astronomers to a lunar crater some three miles wide, which had not

before been observed, and which, he feels sure, was not in existence

two years ago. Astronomers have long since given up all hope of tracing

either the signs of actual life upon the moon or traces of the past

existence of living creatures there. But there are still among them

those who believe that by sedulous and careful scrutiny processes of

material change may be recognised in that seemingly inert mass. In

reality, perhaps, the wonder rather is that signs of change should

not be often recognised, than that from time to time a new crater

should appear or the walls of old craters fall in. The moon's surface

is exposed to variations of temperature compared with which those

affecting the surface of our earth are altogether trifling. It is

true there is no summer or winter in the moon. Sir W. Herschel has

spoken of the lunar seasons as though they resembled our own, but

in reality they are very different. The sun's midday height at any

lunar station is only about three degrees greater in summer than in

winter; whereas our summer sun is 47° higher in the sky at noon than

our winter sun. In fact, a midsummer's day on the moon does not differ

more from a midwinter's day, as far as the sun's actual path on the

sky is concerned, than with us the 17th of March differs from the

25th, or the 19th of September from the 27th. It is the change from

day to night which chiefly affects the moon's surface. In the lunar

year of seasons, lasting 346-2/3 of our days, there are only 11-3/4

lunar days, each lasting 29-3/4 of ours. Thus day lasts more than a

fortnight, and is followed by a night of equal length. Nor is this

all. There is neither air nor moisture to produce such effects as are

produced by our air and the moisture it contains in mitigating the heat

of day and the cold of night. Under the sun's rays the moon's surface

becomes hotter and hotter as the long lunar day proceeds, until at

last its heat exceeds that of boiling water. But so soon as the sun

has set the heat thus received is rapidly radiated away into space (no

screen of moisture-laden air checking its escape), and long before

lunar midnight a cold exists compared with which the bitterest weather

ever experienced by Arctic voyagers would be oppressively hot. These

are not merely theoretical conclusions, though even as such they could

be thoroughly relied upon. The moon's heat has been measured by the

present Lord Rosse (using his father's splendid six-feet mirror). He

separated the heat which the moon simply reflects to us from that which

her heated surface itself gives out (or, technically, he separated

the reflected from the radiated heat), by using a glass screen which

allowed the former heat to pass while it intercepted the latter. He

thus found that about six-sevenths of the heat we receive from the moon

is due to the heating of her own substance. From the entire series of

observations it appeared that the change of temperature during the

entire lunar day--that is, from near midnight to near midday on the

moon--amounts to fully 500° Fahrenheit. If we assume that the cold at

lunar midnight corresponds with about 250° below zero (the greatest

cold experienced in Arctic travelling has never exceeded 140° below

zero), it would follow that the midday heat is considerably greater

than that of boiling water on the earth at the sea-level. But the range

of change is not a matter of speculation. It certainly amounts to about

500°, and in whatever way we distribute it, we must admit, first, that

no such life as we are familiar with could possibly exist on the moon;

and, secondly, that the moon's crust must possess a life of its own,

so to speak, expanding and contracting unceasingly and energetically.

Professor Newcomb, by the way, in his fine work on Popular Astronomy,

rejects the idea that the expansions and contractions due to these

great changes of temperature can cause any disintegration at the

present time. There might, he says, be bodies so friable that they

would crumble, 'but whatever crumbling might thus be caused would soon

be done with, and then no further change would occur.' For my own part,

I cannot consider that such a surface as the moon at present possesses

can undergo these continual expansions and contractions without slow

disintegration. It seems to me also extremely probable that from time

to time the overthrow of great masses, the breaking up of arched

crater-floors, and other sudden changes discernible from the earth,

might be expected to occur. Professor Newcomb has, I conceive, omitted

to consider the enormous volumetric expansion as distinguished from

mere lateral extension, resulting from the heating of the moon's crust

to considerable depths. On a very moderate computation, the surface

of the central region of the full moon must at that time rise above

its mean position to such a degree that hundreds, if not thousands,

of cubic miles of the moon's volume lie above the mean position of

the surface there. At new moon--that is, at lunar midnight for the

same region--the same enormous quantity of matter is correspondingly

depressed. And though the actual range in vertical height at any given

point may be small, we cannot doubt that the total effect produced

by these constant oscillations is considerable. Years or centuries

may pass without any great or sudden change, but from time to time

such catastrophes must surely occur. I believe that all the cases of

supposed change in the moon, if all were regarded as proved, could be

thus fully accounted for without any occasion to assume the action of

volcanic forces properly so called.

Before considering the evidence for the new lunar volcano to which Dr.

Klein has recently called the attention of astronomers, it may be well

briefly to describe the condition of the moon's surface.

This surface, which is equal in extent to about that of the American

Continent, or to Europe and Africa together (without their islands),

is divided into two chief portions--the higher levels, which are in

the main of lighter tint, and the lower levels, which are, almost

without exception, dark. It may be remarked in passing that very

erroneous ideas are commonly entertained respecting the moon's general

colour. The moon is very far from being white, as many suppose. On the

contrary, she is far more nearly black than white. It has been well

remarked by Tyndall that if the moon were covered with black velvet

(14,600,000 square miles of that material would be required for the

purpose), she would still appear white to us, for we should see her

disc projected on the blackness of star-strewn space. The actual tint

of the moon as a whole is nearly the same as that of gray weathered

sandstone. The brightest parts, however, are much whiter; Zöllner

infers from his photometric experiments that they can be compared with

the whitest of terrestrial substances. On the other hand, the darkest

parts of the moon are probably far darker than porphyry, even if they

are not so dark that on earth we should call them black. The fact

that the low-lying parts of the moon are much darker than the higher

regions is full of meaning, though hitherto its significance does not

seem to have been much noticed. Either we must assume that these lower

regions, the so-called seas (certainly now dry), are old sea bottoms,

and owe their darkness to the quality of the matter deposited there

in remote ages, or else we must suppose that the matter which last

remained fluid when the moon's surface was consolidating was of darker

material than the rest. For such matter would occupy the lowest lunar

regions. There is here room for a very profitable study of the moon's

aspect by geologists. I doubt not that, however different the general

past history of our earth may have been from the moon's, terrestrial

regions exist where the characteristic features of the moon's surface

are more or less closely illustrated. On the American continent, for

example, there are peculiarities of geological formation which seem

to correspond closely with some of the features of the lunar globe,

presently to be noticed; and it seems to me not improbable that

geologists might find in the study of certain regions in North America

the means of interpreting the difference of tint between higher and

lower levels on the moon. If so, light would probably be thrown on very

difficult questions relating to the remote past, not only of the moon,

but of our own earth.

The lunar feature which comes next in importance to the difference

of tint between the so-called 'seas' and the higher lands is the

existence of remarkable series of radiating streaks extending from

certain important craters--centres probably of past disturbance. It

is impossible to contemplate the disc of the full moon, as seen with

a powerful telescope, without feeling that these systems of rays must

have resulted from the operation of forces of the most stupendous

nature, though as yet their true meaning is hid from us. They would be

marvellous phenomena, even if they were not so mysterious--marvellous

in their enormous extension, their singular brightness, and

their manner of traversing 'seas,' craters, and mountain-ranges

indifferently. But their chief marvel resides in the mysterious manner

of their appearance as the moon approaches her full illumination.

Other lunar features are most clearly recognised when the moon is not

full, for then the shadows which afford our only means of estimating

the height of lunar irregularities are clearly seen along the border

between the bright and dark parts of her face, and we have only to

wait until this border passes over any object we wish to study to

obtain satisfactory evidence of its nature. It is quite otherwise with

the rays. The regions occupied by these radiating streaks are neither

raised nor depressed in such sort as either to throw shadows or to

lie in shadow when surrounding regions are in sunlight. But when the

moon approaches her full illumination, the radiating regions come into

view, as bright streaks--bright even on the light-tinted lunar uplands.

A mighty system of rays can be seen extending from the great crater

Tycho in all directions. Other systems, scarcely less wonderful, extend

from the battlemented crater, Copernicus, the brilliant Aristarchus,

and the solitary Kepler. One ray from Tycho can be traced round nearly

an entire hemisphere of the moon's surface. It is specially noteworthy

of this great ray that, where it crosses the lunar Sea of Serenity,

that great plain seems to be divided as by a sort of ridge line, the

slope of the plain from either side of the ray's track being clearly

discernible when the moon is near her first quarter.

What are these mysterious ray systems? How are we to explain the

circumstance that though only the most tremendous forces seem competent

to account for bands such as these, many miles broad and many hundreds

of miles in length, there are yet none of the usual signs of the action

of volcanic forces? If mighty rifts had been formed in the moon's crust

by the outbursting action of a hot nucleus, or through the contraction

of the crust on an unyielding nucleus (for the effect would be the same

in either case), we should scarcely expect to find that after such

rifts had formed no signs of any difference of level would appear. If

lava flowed out all along the rift, one would imagine that it would

form a long dyke which would throw an obvious shadow, except under full

solar illumination. If the rift were not filled with lava, the bottom

of the rift would certainly remain in shadow long after the surrounding

region was illuminated. That lava should exactly fill the rift along

its entire length seems incredible. This might happen by a strange

chance in the case of a single rift, but not with all the rifts of a

radiating system, still less with all the rifts of all the radiating

systems. Yet I believe that neither astronomers nor geologists can form

any other opinion respecting these mysterious ray-systems than that

they were caused by what Humboldt (speaking of the earth) calls the

reaction of the interior on the crust. Nasmyth has admirably indicated

their appearance, or rather their radiating form, by filling a globular

glass shell with water, hermetically closed, and then freezing the

water. The expansion of the water bursts the glass shell, and the lines

of fracture are found to extend in a series of rays from the part of

the shell which first gave way. But this experiment of itself does not

explain the mystery of the lunar rays. Accepting the theory that the

moon's crust yielded in some such way, we have still to explain how

the rifts which were thus formed came to be covered over with matter

lying nearly at the same level as the surrounding surface. It appears

to me that the only available way of explaining this is somewhat as

follows. First, from the way in which the streaks are covered like the

surrounding region with craters, we may conclude that the streaks are

older than any except the largest craters; from the great extension

of many of them, we may safely infer that the lunar crust possessed a

large measure of plasticity when they were formed (for otherwise it

would have yielded over a smaller area). It was, therefore, probably

still hot during the era (which may have lasted millions of years) to

which the formation of the rifts belonged: accordingly the lava which

flowed out through the rifts remained liquid for a considerable time,

and was thus able to spread widely on either side of the rift, forming

a broad band of lava-covered surface, instead of a steep and narrow

dyke. This seems not only to account for the most striking peculiarity

of the bands, but to accord well with all that is known about them,

and even to suggest explanations of some other lunar features which

had appeared perplexing. I understand that in certain regions of North

America there are lava-covered rifts large enough to form geographical

features, and, therefore, fairly comparable with the lunar radiating

streaks. But as yet American geologists have not presented in an

accessible form a description of the peculiar features of the American

continent; in fact, it may be doubted whether as yet the materials for

such a description exist.

The mountain-ranges of the moon do not differ to any marked degree

from those of our own earth. They are few in number; in fact,

mountain-ranges form a less important feature of lunar than of

terrestrial geography. On the other hand, the lunar ring-mountains and

craters far exceed those of our earth in size and importance. The large

craters may, in fact, be regarded as characteristic features of lunar

scenery. There are several craters exceeding 100 miles in diameter. It

is strange to consider that though the ringed wall surrounding some of

these larger craters exceeds 10,000 feet in height, no trace of the

highest peaks of such a wall would be visible from the middle of the

enclosed plain. Conversely, an observer standing on one of the highest

peaks beside one of these great craters, would not see half the floor

of the crater, while more than half the horizon line around him would

belong to the enclosed plain, and would appear as level as the horizon

seen from a height overlooking a great prairie. These ringed plains

and larger craters seem to belong to the third great era of the moon's

history. The bright high regions and dark low levels called seas must

have been formed while the greater part of the crust was intensely

hot. The contraction of the cooling crust on the nucleus, which cooled

far less slowly, led to the formation of the great ray systems. But

though such systems extend from great craters, these craters themselves

probably attained their present form far later. The crust having in

great part cooled, the nucleus began in turn to shrink more quickly

than the crust, having more heat to part with. Thus the crust, closing

in upon the shrinking nucleus, formed the corrugations and wrinkles

which can be seen under telescopic scrutiny in nearly every part of

the visible lunar surface. The process was accompanied necessarily

by the development of great heat--the thermal equivalent of the

mechanical process of contraction. Mallet has shown that the process

of contraction at present occurring in the earth's crust gives rise

to the greater part of the heat to which volcanic phenomena are due.

If this is so in the earth's case at present, how tremendous must have

been the heat evolved by the far more rapid contraction of the moon's

mass in the remote era we are considering, when probably her heat

passed into space unchecked by the action of a dense moisture-laden

atmosphere! We can well understand that enormous volumes of heated gas

would be formed--including steam, for there is good reason to believe

that water is present in large quantities in the moon's interior. The

imprisoned gas would find an outlet at points of least resistance,

the centres, namely, of the great radiating systems of streaks. These

centres would certainly be regions of outlet. But they would not be

sufficient. We can understand then why every ray system extends from

a great crater, though that crater was really formed after the system

of radiating streaks; and we can equally understand why these central

craters are not the only or even the chief of the great craters in the

moon. Here again I would suggest that possibly the careful study of

American geology might disclose features illustrating the great lunar

craters.

Rough Ways Made Smooth: A series of familiar essays on scientific subjects · 第 8 / 26 段