LUNAR CHARACTERISTICS.

The moon, in consequence of its orbital revolution, having no connecting

axial motion, has always presented but one side to the earth, so that in

process of forming a crust, from its incipient molten state, it became,

by the constant attraction of the earth upon one side, elongated toward

our globe, now generally admitted to be by calculation about thirty

miles, and proved by photographs, which also show an elongation. The

necessary consequence of this constant attraction upon one side, has

been not only to intensify volcanic action there, by the continued

effect of gravitation, so long as its interior remained in a molten

state, but from the same reasoning, to confine all such volcanic action

exclusively to this side of the moon. Thus we have the reason for the

violently disrupted state which that luminary presents to the telescopic

observer, exceeding any analogy to be found upon our globe, as the

earth's axial motion has prevented any similar concentrated action upon

any particular part of its surface, either from solar or lunar

attraction. Another marked effect of the elongation of the moon toward

the earth has been to elevate its visible side high above its atmosphere

(which would have enveloped it as a round body), and in consequence into

an intensely cold region, producing congelation, in the form of frost

and snow, which necessarily envelop its entire visible surface. These

effects took place while yet the crust was thin and frequently disrupted

by volcanic action, and wherever such action took place, the fiery

matter ejected necessarily dissolved the contiguous masses of frost and

snow, and these floods of water, as soon as they receded from the fiery

element, were immediately converted into lengthened ridges of ice,

diverging from the mountain summits like streams of lava. Hence many of

the apparent lava streams are but ridges of ice, and in consequence,

depending upon the angle of reflection (determined by the age of the

moon, which is but its relative position between the sun and earth), all

observers are struck with the brilliancy of the reflected light from

many of those long lines of ridges.

The general surface of the moon presents to the telescopic observer just

that drear, cold, and chalk-like aspect, which our snow-clad mountains

exhibit when the angle of reflection is similar to that in which we

behold the lunar surface. In consequence, its mild light is due to the

myriads of sparkling crystals, which diffusively reflect the rays of the

sun.

As an attentive observer of the moon, I have been much puzzled to know

why none of the hosts of observers, or scientific treatises, have taken

this rational view of such necessary condition of the moon, deduced from

the main facts of its original formation, here named and generally

conceded. In the place of which, we still have stereotyped, in many late

editions on astronomy, the names and localities of numerous seas and

lakes, which advancing knowledge should long since have discarded.

Besides the above conclusions, which necessitate a snowy covering to the

moon, none of the planets exhibit that drear white, except the poles of

Mars, which are admitted to be snow by all astronomers, as we see them

come and go with the appropriate seasons of that planet; whereas the

continents of Mars appear dark, as analogously they do upon our earth,

under the same solar effulgence. The analogy of sunlight, when reflected

from our lofty mountains (at say thirty or forty miles distant) not

covered with snow, viewed under the most favorable circumstances of

brilliant light and the best angle of reflection, with no more of

intervening atmosphere, always present sombre tints; whether viewed with

the unaided eye or through a telescope. Such analogy clearly proves that

no objects short of an absolute white could present such an appearance

as light does upon lunar objects, viewed with high powers, in which the

same drear white remains, without any greater concentration of light (as

we can see objects in the moon whose diameter is five hundred feet) than

is presented to our unaided eye from our own mountain masses. In viewing

the moon with high powers, there is, in fact, a much greater amount of

visible atmosphere intervening than can possibly apply in beholding

objects on our earth, at even a few miles' distance, since if we look at

lunar objects with a power of one thousand times, our atmosphere is thus

magnified a thousand times also.

The main physical features of the visible half of the moon, with a good

telescopic power, present an enormously elevated table land, traversed,

here and there, with slightly elevated long ridges, and the general

surface largely pitted with almost innumerable deep cusps or valleys, of

every size, from a quarter of a mile to full thirty miles in diameter;

generally circular and surrounded with elevated ridges, some rising to

lofty jagged summits above the surrounding plain. These ridges, on their

inner sides, show separate terraces and mural precipices, while their

outer slopes display deeply scarred ravines and long spurs at their

bases. These cusps, or deep valleys, are the craters of extinct

volcanoes, and in their centres have generally one or two isolated

sub-mountain peaks, occasionally with divided summits, which were the

centres of expiring volcanic action, similar to those that exist in our

own volcanic regions. Besides which the Lunar Apennines, so called,

present to the eye a long range of mountains with serrated summits, on

one side gradually sloped, with terraces, spurs, and ravines, and the

other side mostly precipitous, casting long shadows, which clearly

define the forms of their summits--all these objects presenting the same

dead white everywhere.

Doubtless the farther side of the moon, which has not been subject to

the same elongating or elevating process, nor the above-named causes for

volcanic disruption, presents a climate and vegetation fitted for the

abode of sentient beings. This side alone presenting an aspect of

extreme desolation, far surpassing our polar regions.

It is generally stated in astronomical works, that shadows projected

from lunar objects are intensely black, owing, it is stated, to there

being no reflecting atmosphere; whereas in my long-continued habit of

observation, those shadows appear no more black than those on our earth,

when they fall on contrasting snowy surfaces. The reason for which, in

the absence of a lunar atmosphere, to render light diffusive, is the

brilliant reflection from snow crystals, upon all contiguous objects,

which lie in an angle to receive the same, and in consequence I have

often observed the forms of objects not directly illuminated by the sun.

The occasional apparent retention of a star on the limb of the moon,

just before or after an occultation, seen by some observers, and thus

evidencing the existence of some atmosphere, is doubtless due to the

slight oscillations of the moon, by which we see a trifle more than half

of that body, during which the atmosphere of its opposite side slightly

impinges upon this.

The Continental Monthly, Vol. 6, No 4, August, 1864 Devoted To Literature And National Policy · 第 13 / 46 题