in broad day close beside the sun! This was the first authenticated
instance of that kind, but the occurrence was to be repeated, as we
shall see in a moment, less than forty years later.
The splendid comet of 1858, usually called Donati’s, is remembered by
many persons yet living. It was, perhaps, both as seen by the naked eye
and with the telescope, the most beautiful comet of which we have any
record. It too marked a rich vintage year, still remembered in the
vineyards of France, where there is a popular belief that a great comet
ripens the grape and imparts to the wine a flavor not attainable by the
mere skill of the cultivator. There are “comet wines,” carefully
treasured in certain cellars, and brought forth only when their owner
wishes to treat his guests to a sip from paradise.
The year 1861 saw another very remarkable comet, of an aspect strangely
vast and diffuse, which is believed to have swept the earth with its
immense tail when it passed between us and the sun on the night of June
30th, an event which produced no other known effect than the appearance
of an unwonted amount of scattered light in the sky.
The next very notable comet was the “Great Southern Comet” of 1880,
which was not seen from the northern hemisphere. It mimicked the aspect
of the famous comet of 1843, and to the great surprise of astronomers
appeared to be traveling in the same path. This proved to be the rising
of the curtain for an astronomical sensation unparalleled in its kind;
for two years later another brilliant comet appeared, first in the
southern hemisphere, _and it too followed the same track._ The
startling suggestion was now made that this comet was identical with
those of 1843 and 1880, its return having been hastened by the
resistance experienced in passing twice through the coronal envelope,
and there were some who thought that it would now swing swiftly round
and then plunge straight into the sun, with consequences that might be
disastrous to us on account of the “flash of heat” that would be
produced by the impact. Nervous people were frightened, but observation
soon proved that the danger was imaginary, for although the comet
almost grazed the sun, and must have rushed through two or three
million miles of the coronal region, no retardation of its immense
velocity was perceptible, and it finally passed away in a damaged
condition, as before remarked, and has never since appeared.
Then the probable truth was perceived—_viz.,_ that the three comets
(1843, 1880, and 1882) were not one identical body, but three separate
ones all traveling in the same orbit. It was found, too, that a comet
seen in 1668 bore similar insignia of relationship. The natural
inference was that these four bodies had once formed a single mass
which had been split apart by the disruptive action of the sun.
Strength was lent to this hypothesis by the fact that the comet of 1882
was apparently torn asunder during its perihelion passage, retreating
into space in a dissevered state. But Prof. George Forbes has a theory
that the splitting of the original cometary mass was effected by an
unknown planet, probably greater than Jupiter, situated at a hundred
times the earth’s distance from the sun, and revolving in a period of a
thousand years. He supposes that the original comet was not that of
1668, but one seen in 1556, which has since been “missing,” and that
its disruption occurred from an encounter with the supposititious
planet about the year 1700. Truly from every point of view comets are
the most extraordinary of adventurers!
The comet of 1882 was likewise remarkable for being visible, like its
predecessor of 1843, in full daylight in close proximity to the sun.
The story of its detection when almost in contact with the solar disk
is dramatic. It had been discovered in the southern hemisphere only a
couple of weeks before its perihelion, which occurred on September
17th, and on the forenoon of that day it was seen by Doctor Common in
England, and by Doctor Elkin and Mr Finlay at the Cape of Good Hope,
almost touching the sun. It looked like a dazzling white bird with
outspread wings. The southern observers watched it go _right into the
sun,_ when it instantly disappeared. What had happened was that the
comet in passing its perihelion point had swung exactly between the
earth and the sun. On the following morning it was seen from all parts
of the world close by the sun on the opposite side, and it remained
thus visible for three days, gradually receding from the solar disk. It
then became visible for northern observers in the morning sky before
sunrise, brandishing a portentous sword-shaped tail which, if it had
been in the evening sky, would have excited the wonder of hundreds of
millions, but situated where it was, comparatively few ever saw it.
[Illustration: Daniels’ comet. August 11, 1907]
The application of photography to the study of comets has revealed many
curious details which might otherwise have escaped detection, or at
best have remained subject to doubt. It has in particular shown not
only the precise form of the tails, but the remarkable vicissitudes
that they undergo. Professor Barnard’s photographs of Brooks’ comet in
1893 suggested, by the extraordinary changes in the form of the tail
which they revealed, that the comet was encountering a series of
obstructions in space which bent and twisted its tail into fantastic
shapes. The reader will observe the strange form into which the tail
was thrown on the night of October 21st. A cloud of meteors through
which the comet was passing might have produced such deformations of
its tail. In the photograph of Daniels’ comet of 1907, a curious
striping of the tail will be noticed. The short bright streaks seen in
the photograph, it may be explained, are the images of stars which are
drawn out into lines in consequence of the fact that the photographic
telescope was adjusted to follow the motion of the comet while the
stars remained at rest.
But the adventures of comets are not confined to possible encounters
with unknown obstacles. We have referred to the fact that the great
planets, and especially Jupiter, frequently interfere with the motions
of comets. This interference is not limited to the original alteration
of their orbits from possible parabolas to ellipses, but is sometimes
exercised again and again, turning the bewildered comets into
elliptical paths of all degrees of eccentricity. A famous example of
this kind of planetary horse-play is furnished by the story of Lexell’s
missing comet. This comet was first seen in 1770. Investigation showed
that it was moving in an orbit which should bring it back to perihelion
every five and a half years; yet it had never been seen before and,
although often searched for, has never been seen since. Laplace and
Leverrier proved mathematically that in 1767 it had approached so close
to Jupiter as to be involved among the orbits of his satellites. What
its track had been before is not known, but on that occasion the giant
planet seized the interloper, threw it into a short elliptic orbit and
sent it, like an arrested vagrant, to receive sentence at the bar of
the sun. On this journey it passed within less than 1,500,000 miles of
the earth. The form of orbit which Jupiter had impressed required, as
we have said, its return in about five and a half years; but soon after
1770 it had the misfortune a second time to encounter Jupiter at close
range, and he, as if dissatisfied with the leniency of the sun, or
indignant at the stranger’s familiarity, seized the comet and hurled it
out of the system, or at any rate so far away that it has never since
been able to rejoin the family circle that basks in the immediate rays
of the solar hearth. Nor is this the only instance in which Jupiter has
dealt summarily with small comets that have approached him with too
little deference.
[Illustration: Brooks’ comet. Photographed by Barnard, October 21,
1893]
The function which Jupiter so conspicuously fulfills as master of the
hounds to the sun is worth considering a little more in detail. To
change the figure, imagine the sun in its voyage through space to be
like a majestic battleship surrounded by its scouts. Small vessels (the
comets, as they are overhauled by the squadron, are taken in charge by
the scouts, with Jupiter for their chief, and are forced to accompany
the fleet, but not all are impressed. If a strange comet undertakes to
run across Jupiter’s bows the latter brings it to, and makes prize of
it by throwing it into a relatively small ellipse with the sun for its
focus. Thenceforth, unless, as happened to the unhappy comet of Lexell,
it encounters Jupiter again in such a way as to be diverted by him into
a more distant orbit, it can never get away. About thirty comets are
now known to have thus been captured by the great planet, and they are
called “Jupiter’s Comet Family.” But, on the other hand, if a wandering
comet crosses the wake of the chief planetary scout the latter simply
drives it away by accelerating its motion and compels it to steer off
into open space. The transformation of comets into meteors will be
considered in the next chapter, but here, in passing, mention may be
made of the strange fate of one member of Jupiter’s family, Biela’s
comet, which, having become over bold in its advances to its captor,
was, after a few revolutions in is impressed orbit, torn to pieces and
turned into a flock of meteors.
And now let us return to the mystery of comets’ tails. That we are
fully justified in speaking of the tails of comets as mysterious is
proved by the declaration of Sir John Herschel, who averred, in so many
words, that “there is some profound secret and mystery of nature
concerned in this phenomenon,” and this profound secret and mystery has
not yet been altogether cleared up. Nevertheless, the all-explaining
hypothesis of Arrhenius offers us once more a certain amount of aid.
Comets’ tails, Arrhenius assures us, are but another result of the
pressure of light. The reader will recall the applications of this
theory to the Zodiacal Light and the Aurora. In the form in which we
now have to deal with it, the supposition is made that as a comet
approaches the sun eruptions of vapor, due to the solar heat, occur in
its nucleus. These are naturally most active on the side which is
directly exposed to the sun, whence the appearance of the immense
glowing envelopes that surround the nucleus on the sunward side. Among
the particles of hydro-carbon, and perhaps solid carbon in the state of
fine dust, which are thus set free there will be many whose size is
within the critical limit which enables the light-waves from the sun to
drive them away. Clouds of such particles, then, will stream off behind
the advancing comet, producing the appearance of a tail. This accounts
for the fact that the tails of comets are always directed away from the
sun, and it also explains the varying forms of the tails and the
extraordinary changes that they undergo. The speed of the particles
driven before the light-waves must depend upon their size and weight,
the lightest of a given size traveling the most swiftly. By accretion
certain particles might grow, thus losing velocity and producing the
appearance of bunches in the tail, such as have been observed. The
hypothesis also falls in with the researches of Bredichin, who has
divided the tails of comets into three principal classes—_viz.:_ (1)
Those which appear as long, straight rays; (2) Those which have the
form of curved plumes or scimitars; (3) Those which are short, brushy,
and curved sharply backward along the comet’s path. In the first type
he calculates the repulsive force at from twelve to fifteen times the
force of gravity; in the second at from two to four times; and in the
third at about one and a half times. The straight tails he ascribes to
hydrogen because the hydrogen atom is the lightest known; the
sword-shaped tails to hydro-carbons; and the stumpy tails to vaporized
iron. It will be seen that, if the force driving off the tails is that
which Arrhenius assumes it to be, the forms of those appendages would
accord with those that Bredichin’s theory calls for. At the same time
we have an explanation of the multiple tails with which some comets
have adorned themselves. The comet of 1744, for instance, had at one
time no less than seven tails spread in a wide curved brush behind it.
Donati’s comet of 1858 also had at least two tails, the principal one
sword-shaped and the other long, narrow, and as straight as a rule.
According to Bredichin, the straight tail must have been composed of
hydrogen, and the other of some form of hydro-carbon whose atoms are
heavier than those of hydrogen, and, consequently, when swept away by
the storm of light-waves, followed a curvature depending upon the
resultant of the forces operating upon them. The seven tails of the
comet of 1744 presented a kind of diagram graphically exhibiting its
complex composition, and, if we knew a little more about the
constituents of a comet, we might be able to say from the amount of
curvature of the different tails just what were the seven substances of
which that comet consisted.
If these theories seem to the reader fantastic, at any rate they are no
more fantastic than the phenomena that they seek to explain.
XI
Meteors, Fire-Balls, and Meteorites
One of the most terrorizing spectacles with which the heavens have ever
caused the hearts of men to quake occurred on the night of November 13,
1833. On that night North America, which faced the storm, was under a
continual rain of fire from about ten o’clock in the evening until
daybreak.
_The fragments of a comet had struck the earth._
But the meaning of what had happened was not discovered until long
afterward. To the astronomers who, with astonishment not less than that
of other people, watched the wonderful scene, it was an unparalleled
“shower of meteors.” They did not then suspect that those meteors had
once formed the head of a comet. Light dawned when, a year later, Prof.
Denison Olmsted, of Yale College, demonstrated that the meteors had all
moved in parallel orbits around the sun, and that these orbits
intersected that of the earth at the point where our planet happened to
be on the memorable night of November 13th. Professor Olmsted even went
so far as to suggest that the cloud of meteors that had encountered the
earth might form a diffuse comet; but full recognition of the fact that
they were cometary débris came later, as the result of further
investigation. The key to the secret was plainly displayed in the
spectacle itself, and was noticed without being understood by thousands
of the terror-stricken beholders. It was _an umbrella of fire_ that had
opened overhead and covered the heavens; in other words, the meteors
all radiated from a particular point in the constellation Leo, and,
being countless as the snowflakes in a winter tempest, they ribbed the
sky with fiery streaks. Professor Olmsted showed that the radiation of
the meteors from a fixed point was an effect of perspective, and in
itself a proof that they were moving in parallel paths when they
encountered the earth. The fact was noted that there had been a
similar, but incomparably less brilliant, display of meteors on the
same day of November, 1832, and it was rightly concluded that these had
belonged to the same stream, although the true relationship of the
phenomena was not immediately apprehended. Olmsted ascribed to the
meteors a revolution about the sun once in every six months, bringing
them to the intersection of their orbit with that of the earth every
November 13th; but later investigators found that the real period was
about thirty-three and one-quarter years, so that the great displays
were due three times in a century, and their return was confidently
predicted for the year 1866. The appearance of the meteors in 1832, a
year before the great display, was ascribed to the great length of the
stream which they formed in space—so great that they required more than
two years to cross the earth’s orbit. In 1832 the earth had encountered
a relatively rare part of the stream, but in 1833, on returning to the
crossing-place, it found there the richest part of the stream pouring
across its orbit. This explanation also proved to be correct, and the
predicted return in 1866 was duly witnessed, although the display was
much less brilliant than in 1833. It was followed by another in 1867.
[Illustration: Curious forms of meteorite trains
Nos. 1 to 6 show the changes undergone by a train left by a meteorite
which passed near the “Great Dipper”; 7 shows the changes and drift of
a train seen in the constellation Virgo; 8 is the singular train of the
meteorite of February 22, 1909, near the Pole Star. (From _La
Nature_.)]
In the mean time Olmsted’s idea of a cometary relationship of the
meteors was demonstrated to be correct by the researches of
Schiaparelli and others, who showed that not only the November meteors,
but those of August, which are seen more or less abundantly every year,
traveled in the tracks of well-known comets, and had undoubtedly an
identical origin with those comets. In other words the comets and the
meteor-swarms were both remnants of original masses which had probably
been split up by the action of the sun, or of some planet to which they
had made close approaches. The annual periodicity of the August meteors
was ascribed to the fact that the separation had taken place so long
ago that the meteors had become distributed all around the orbit, in
consequence of which the earth encountered some of them every year when
it arrived at the crossing-point. Then Leverrier showed that the
original comet associated with the November meteors was probably
brought into the system by the influence of the planet Uranus in the
year 126 of the Christian era. Afterward Alexander Herschel identified
the tracks of no less than seventy-six meteor-swarms (most of them
inconspicuous) with those of comets. The still more recent researches
of Mr W. F. Denning make it probable that there are no meteors which do
not belong to a flock or system probably formed by the disintegration
of a cometary mass; even the apparently sporadic ones which shoot
across the sky, “lost souls in the night,” being members of flocks
which have become so widely scattered that the earth sometimes takes
weeks to pass through the region of space where their paths lie.
The November meteors should have exhibited another pair of spectacles
in 1899 and 1900, and their failure to do so caused at first much
disappointment, until it was made plain that a good reason existed for
their absence. It was found that after their last appearance, in 1867,
they had been disturbed in their movements by the planets Jupiter and
Saturn, whose attractions had so shifted the position of their orbit
that it no longer intersected that of the earth, as it did before.
Whether another planetary interference will sometime bring the
principal mass of the November meteors back to the former point of
intersection with the earth’s orbit is a question for the future to
decide. It would seem that there may be several parallel streams of the
November meteors, and that some of them, like those of August, are
distributed entirely around the orbit, so that every mid-November we
see a few of them.
We come now to a very remarkable example of the disintegration of a
comet and the formation of a meteor-stream. In 1826 Biela, of
Josephstadt, Austria, discovered a comet to which his name was given.
Calculation showed that it had an orbital period of about six and a
half years, belonging to Jupiter’s “family.” On one of its returns, in
1846, it astonished its watchers by suddenly splitting in two. The two
comets thus formed out of one separated to a distance of about one
hundred and sixty thousand miles, and then raced side by side,
sometimes with a curious ligature connecting them, like Siamese twins,
until they disappeared together in interplanetary space. In 1852 they
came back, still nearly side by side, but now the distance between them
had increased to a million and a quarter of miles. After that, at every
recurrence of their period, astronomers looked for them in vain, until
1872, when an amazing thing happened. On the night of November 28th,
when the earth was crossing the plane of the orbit of the missing
comet, a brilliant shower of meteors burst from the northern sky,
traveling nearly in the track which the comet should have pursued. The
astronomers were electrified. Klinkerfues, of Göttingen, telegraphed to
Pogson, of Madras: _“Biela touched earth; search near Theta Centauri.”_
Pogson searched in the place indicated and saw a cometary mass
retreating into the southern heavens, where it was soon swallowed from
sight!
[Illustration: Section of the atmosphere up to 100 kilometers.
Showing the mean elevation at which meteorites and meteors make their
appearance. Below are shown the elevation of Mount Everest, the highest
manned balloon ascent by M. Berson; the height of cirrus clouds; the
highest free balloon ascent; and the elevation attained by the clouds
of fire-dust ejected by the Krakatoa eruption in 1883. (From _La
Nature_)]
Since then the Biela meteors have been among the recognized periodic
spectacles of the sky, and few if any doubt that they represent a
portion of the missing comet whose disintegration began with the
separation into two parts in 1846. The comet itself has never since
been seen. The first display of these meteors, sometimes called the
“Andromedes,” because they radiate from the constellation Andromeda,
was remarkable for the great brilliancy of many of the fire-balls that
shot among the shower of smaller sparks, some of which were described
as equaling the full moon in size. None of them is known to have
reached the earth, but during the display of the same meteors in 1885 a
meteoric mass fell at Mazapil in Northern Mexico (it is now in the
Museum at Vienna), which many have thought may actually be a piece of
the original comet of Biela. This brings us to the second branch of our
subject.
More rare than meteors or falling stars, and more startling, except
that they never appear in showers, are the huge balls of fire which
occasionally dart through the sky, lighting up the landscapes beneath
with their glare, leaving trains of sparks behind them, often producing
peals of thunder when they explode, and in many cases falling upon the
earth and burying themselves from a few inches to several feet in the
soil, from which, more than once, they have been picked up while yet
hot and fuming. These balls are sometimes called bolides. They are not
really round in shape, although they often look so while traversing the
sky, but their forms are fragmentary, and occasionally fantastic. It
has been supposed that their origin is different from that of the true
meteors; it has even been conjectured that they may have originated
from the giant volcanoes of the moon or have been shot out from the sun
during some of the tremendous explosions that accompany the formation
of eruptive prominences. By the same reasoning some of them might be
supposed to have come from some distant star. Others have conjectured
that they are wanderers in space, of unknown origin, which the earth
encounters as it journeys on, and Lord Kelvin made a suggestion which
has become classic because of its imaginative reach—_viz.,_ that the
first germs of life may have been brought to the earth by one of these
bodies, “a fragment of an exploded world.”
It is a singular fact that astronomers and scientific men in general
were among the last to admit the possibility of solid masses falling
from the sky. The people had believed in the reality of such phenomena
from the earliest times, but the savants shook their heads and talked
of superstition. This was the less surprising because no scientifically
authenticated instance of such an occurrence was known, and the stones
popularly believed to have fallen from the sky had become the objects
of worship or superstitious reverence, a fact not calculated to
recommend them to scientific credence. The celebrated “black stone”
suspended in the Kaaba at Mecca is one of these reputed gifts from
heaven; the “Palladium” of ancient Troy was another; and a stone which
fell near Ensisheim, in Germany, was placed in a church as an object to
be religiously venerated. Many legends of falling stones existed in
antiquity, some of them curiously transfigured by the imagination, like
the “Lion of the Peloponnesus,” which was said to have sprung down from
the sky upon the Isthmus of Corinth. But near the beginning of the
nineteenth century, in 1803, a veritable shower of falling stones
occurred at L’Aigle, in Northern France, and this time astronomers took
note of the phenomenon and scientifically investigated it. Thousands of
the strange projectiles came from the sky on this occasion, and were
scattered over a wide area of country, and some buildings were hit.
Four years later another shower of stones occurred at Weston, Conn.,
numbering thousands of individuals. The local alarm created in both
cases was great, as well it might be, for what could be more
intimidating than to find the blue vault of heaven suddenly hurling
solid missiles at the homes of men? After these occurrences it was
impossible for the most skeptical to doubt any longer, and the regular
study of “aerolites,” or “meteorites,” began.
One of the first things recognized was the fact that fire-balls are
solid meteorites in flight, and not gaseous exhalations in the air, as
some had assumed. They burn in the air during their flight, and
sometimes, perhaps, are entirely consumed before reaching the ground.
Their velocity before entering the earth’s atmosphere is equal to that
of the planets in their orbits—_viz.,_ from twenty to thirty miles per
second—a fact which proves that the sun is the seat of the central
force governing them. Their burning in the air is not difficult to
explain; it is the heat of friction which so quickly brings them to
incandescence. Calculation shows that a body moving through the air at
a velocity of about a mile per second will be brought, superficially,
to the temperature of “red heat” by friction with the atmosphere. If
its velocity is twenty miles per second the temperature will become
thousands of degrees. This is the state of affairs with a meteorite
rushing into the earth’s atmosphere; its surface is liquefied within a
few seconds after the friction begins to act, and the melted and
vaporized portion of its mass is swept backward, forming the train of
sparks that follows every great fire-ball. However, there is one
phenomenon connected with the trains of meteorites which has never been
satisfactorily explained: they often persist for long periods of time,
drifting and turning with the wind, but not ceasing to glow with a
phosphorescent luminosity. The question is, Whence comes this light? It
must be light without heat, since the fine dust or vapor of which the
train can only consist would not retain sufficient heat to render it
luminous for so long a time. An extremely remarkable incident of this
kind occurred on February 22, 1909, when an immense fire-ball that
passed over southern England left a train that remained visible during
two hours, assuming many curious shapes as it was drifted about by
currents in the air.
[Illustration: A meteor photographed in flight]
But notwithstanding the enormous velocity with which meteorites enter
the air they are soon slowed down to comparatively moderate speed, so
that when they disappear they are usually traveling not faster than a
mile a second. The courses of many have been traced by observers
situated along their track at various points, and thus a knowledge has
been obtained of their height above the ground during their flight and
of the length of their visible courses. They generally appear at an
elevation of eighty or a hundred miles, and are seldom visible after
having descended to within five miles of the ground, unless the
observer happens to be near the striking-point, when he may actually
witness the fall. Frequently they burst while high in the air and their
fragments are scattered like shrapnel over the surface of the ground,
sometimes covering an area of several square miles, but of course not
thickly; different fragments of the same meteorite may reach the ground
at points several miles apart. The observed length of their courses in
the atmosphere varies from fifty to five hundred miles. If they
continued a long time in flight after entering the air, even the
largest of them would probably be consumed to the last scrap, but their
fiery career is so short on account of their great speed that the heat
does not have time to penetrate very deeply, and some that have been
picked up immediately after their fall have been found cold as ice
within. Their size after reaching the ground is variable within wide
limits; some are known which weigh several tons, but the great majority
weigh only a few pounds and many only a few ounces.
Meteorites are of two kinds: _stony_ meteorites and _iron_ meteorites.
The former outnumber the latter twenty to one; but many stone
meteorites contain grains of iron. Nickel is commonly found in iron
meteorites, so that it might be said that that redoubtable alloy
nickel-steel is of cosmical invention. Some twenty-five chemical
elements have been found in meteorites, including carbon and the
“sun-metal,” helium. The presence of the latter is certainly highly
suggestive in connection with the question of the origin of meteorites.
The iron meteorites, besides metallic iron and nickel, of which they
are almost entirely composed, contain hydrogen, helium, and carbonic
oxide, and about the only imaginable way in which these gases could
have become absorbed in the iron would be through the immersion of the
latter while in a molten or vaporized state in a hot and dense
atmosphere composed of them, a condition which we know to exist only in
the envelopes of the sun and the stars.
The existence of carbon in the Canyon Diablo iron meteorites is
attended by a circumstance of the most singular character—a very “fairy
tale of science.” In some cases _the carbon has become diamond!_ These
meteoric diamonds are very small; nevertheless, they are true diamonds,
resembling in many ways the little black gems produced by Moissan’s
method with the aid of the electric furnace. The fact that they are
found embedded in these iron meteorites is another argument in favor of
the hypothesis of the solar or stellar origin of the latter. To
appreciate this it is necessary to recall the way in which Moissan made
his diamonds. It was by a combination of the effects of great heat,
great pressure, and sudden or rapid superficial cooling on a mass of
iron containing carbon. When he finally broke open his iron he found it
a pudding stuffed with miniature black diamonds. When a fragment of the
Canyon Diablo meteoric iron was polished in Philadelphia over fifteen
years ago it cut the emery-wheel to pieces, and examination showed that
the damage had been effected by microscopic diamonds peppered through
the mass. How were those diamonds formed? If the sun or Sirius was the
laboratory that prepared them, we can get a glimpse at the process of
their formation. There is plenty of heat, plenty of pressure, and an
abundance of vaporized iron in the sun and the stars. When a great
solar eruption takes place, masses of iron which have absorbed carbon
may be shot out with a velocity which forbids their return. Plunged
into the frightful cold of space, their surfaces are quickly cooled, as
Moissan cooled his prepared iron by throwing it into water, and thus
the requisite stress is set up within, and, as the iron solidifies, the
included carbon crystallizes into diamonds. Whether this explanation
has a germ of truth in it or not, at any rate it is evident that iron
meteorites were not created in the form in which they come to us; they
must once have been parts of immeasurably more massive bodies than
themselves.
The fall of meteorites offers an appreciable, though numerically
insignificant, peril to the inhabitants of the earth. Historical
records show perhaps three or four instances of people being killed by
these bodies. But for the protection afforded by the atmosphere, which
acts as a very effective shield, the danger would doubtless be very
much greater. In the absence of an atmosphere not only would more
meteorites reach the ground, but their striking force would be
incomparably greater, since, as we have seen, the larger part of their
original velocity is destroyed by the resistance of the air. A
meteorite weighing many tons and striking the earth with a velocity of
twenty or thirty miles per second, would probably cause frightful
havoc.
[Illustration: Looking across Coon Butte crater from northern rim]
It is a singular fact that recent investigations seem to have proved
that an event of this kind actually happened in North America—perhaps
not longer than a thousand or two thousand years ago. The scene of the
supposed catastrophe is in northern central Arizona, at Coon Butte,
where there is a nearly circular crater in the middle of a circular
elevation or small mountain. The crater is somewhat over four thousand
feet in diameter, and the surrounding rim, formed of upturned strata
and ejected rock fragments, rises at its highest point one hundred and
sixty feet above the plain. The crater is about six hundred feet in
depth—that is, from the rim to the visible floor or bottom of the
crater. There is no evidence that volcanic action has ever taken place
in the immediate neighborhood of Coon Butte. The rock in which the
crater has been made is composed of horizontal sandstone and limestone
strata. Between three hundred and four hundred million tons of rock
fragments have been detached, and a large portion hurled by some cause
out of the crater. These fragments lie concentrically distributed
around the crater, and in large measure form the elevation known as
Coon Butte. The region has been famous for nearly twenty years on
account of the masses of meteoric iron found scattered about and known
as the “Canyon Diablo” meteorites. It was one of these masses, which
consist of nickel-iron containing a small quantity of platinum, and of
which in all some ten tons have been recovered for sale to the various
collectors throughout the world, that as before mentioned destroyed the
grinding-tool at Philadelphia through the cutting power of its embedded
diamonds. These meteoric irons are scattered about the crater-hill, in
concentric distribution, to a maximum distance of about five miles.
When the suggestion was first made in 1896 that a monster meteorite
might have created by its fall this singular lone crater _in stratified
rocks,_ it was greeted with incredulous smiles; but since then the
matter has assumed a different aspect. The Standard Iron Company,
formed by Messrs. D. M. Barringer, B. C. Tilghman, E. J. Bennitt, and
S. J. Holsinger, having become, in 1903, the owner of this freak of
nature, sunk shafts and bored holes to a great depth in the interior of
the crater, and also trenched the slopes of the mountain, and the
result of their investigations has proved that the meteoric hypothesis
of origin is correct. (See the papers published in the _Proceedings of
the Academy of Natural Sciences of Philadelphia,_ December, 1905,
wherein it is proved that the United States Geological Survey was wrong
in believing this crater to have been due to a steam explosion. Since
that date there has been discovered a great amount of additional
confirmatory proof). Material of unmistakably meteoric origin was found
by means of the drills, mixed with crushed rock, to a depth of six
hundred to seven hundred feet below the floor of the crater, and a
great deal of it has been found admixed with the ejected rock fragments
on the outer slopes of the mountain, absolutely proving synchronism
between the two events, the formation of this great crater and the
falling of the meteoric iron out of the sky. The drill located in the
bottom of the crater was sent, in a number of cases, much deeper (over
one thousand feet) into unaltered horizontal red sandstone strata, but
no meteoric material was found below this depth (seven hundred feet, or
between eleven and twelve hundred feet below the level of the
surrounding plain), which has been assumed as being about the limit of
penetration. It is not possible to sink a shaft at present, owing to
the water which has drained into the crater, and which forms, with the
finely pulverized sandstone, a very troublesome quicksand encountered
at about two hundred feet below the visible floor of the crater. As
soon as this water is removed by pumping it will be easy to explore the
depths of the crater by means of shafts and drifts. The rock strata
(sandstone and limestone) of which the walls consist present every
appearance of having been violently upturned by a huge body penetrating
the earth like a cannon-ball. The general aspect of the crater
strikingly resembles the impression made by a steel projectile shot
into an armor-plate. Mr Tilghman has estimated that a meteorite about
five hundred feet in diameter and moving with a velocity of about five
miles per second would have made just such a perforation upon striking
rocks of the character of those found at this place. There was some
fusion of the colliding masses, and the heat produced some steam from
the small amount of water in the rocks. As a result there has been
found at depth a considerable amount of fused quartz (original
sandstone), and with it innumerable particles or sparks of fused
nickel-iron (original meteorite). A projectile of that size penetrating
eleven to twelve hundred feet into the rocky shell of the globe must
have produced a shock which was perceptible several hundred miles away.
[Illustration: Trail on south side, Coon Butte crater]
The great velocity ascribed to the supposed meteorite at the moment of
striking could be accounted for by the fact that it probably plunged
nearly vertically downward, for it formed a circular crater in the
rocky crust of the earth. In that case it would have been less retarded
by the resistance of the atmosphere than are meteorites which enter the
air at a lower angle and shoot ahead hundreds of miles until friction
has nearly destroyed their original motion when they drop upon the
earth. Some meteoric masses of great size, such as Peary’s iron
meteorite found at Cape York, Greenland, and the almost equally large
mass discovered at Bacubirito, Mexico, appear to have penetrated but
slightly on striking the earth. This may be explained by supposing that
they pursued a long, horizontal course through the air before falling.
The result would be that, their original velocity having been
practically destroyed, they would drop to the ground with a velocity
nearly corresponding to that which gravity would impart within the
perpendicular distance of their final fall. A
six-hundred-and-sixty-pound meteorite, which fell at Knyahinya,
Hungary, striking at an angle of 27° from the vertical, penetrated the
ground to a depth of eleven feet.
It has been remarked that the Coon Butte meteorite may have fallen not
longer ago than a few thousand years. This is based upon the fact that
the geological indications favor the supposition that the event did not
occur more than five thousand years ago, while on the other hand the
rings of growth in the cedar-trees growing on the slopes of the crater
show that they have existed there about seven hundred years. Prof.
William H. Pickering has recently correlated this with an ancient
chronicle which states that at Cairo, Egypt, in the year 1029, “many
stars passed with a great noise.” He remarks that Cairo is about 100°,
by great circle, from Coon Butte, so that if the meteorite that made
the crater was a member of a flock of similar bodies which encountered
the earth moving in parallel lines, some of them might have traversed
the sky tangent to the earth’s surface at Cairo. That the spectacle
spoken of in the chronicle was caused by meteorites he deems
exceedingly probable because of what is said about “a great noise;”
meteorites are the only celestial phenomena attended with perceptible
sounds. Professor Pickering conjectures that this supposed flock of
great meteorites may have formed the nucleus of a comet which struck
the earth, and he finds confirmation of the idea in the fact that out
of the ten largest meteorites known, no less than seven were found
within nine hundred miles of Coon Butte. It would be interesting if we
could trace back the history of that comet, and find out what malicious
planet caught it up in its innocent wanderings and hurled it with so
true an aim at the earth! This remarkable crater is one of the most
interesting places in the world, for there is absolutely no record of
such a mass, possibly an iron-headed comet, from outer space having
come into collision with our earth. The results of the future
exploration of the depths of the crater will be awaited with much
interest.
XII
The Wrecking of the Moon
There are sympathetic moods under whose influence one gazes with a
certain poignant tenderness at the worn face of the moon; that little
“fossil world” (the child of our mother earth, too) bears such terrible
scars of its brief convulsive life that a sense of pity is awakened by
the sight. The moon is the wonder-land of the telescope. Those towering
mountains, whose “proud aspiring peaks” cast silhouettes of shadow that
seem drawn with india-ink; those vast plains, enchained with gentle
winding hills and bordered with giant ranges; those oval “oceans,”
where one looks expectant for the flash of wind-whipped waves; those
enchanting “bays” and recesses at the seaward feet of the Alps; those
broad straits passing between guardian heights incomparably mightier
than Gibraltar; those locket-like valleys as secluded among their
mountains as the Vale of Cashmere; those colossal craters that make us
smile at the pretensions of Vesuvius, Etna, and Cotopaxi; those strange
white ways which pass with the unconcern of Roman roads across
mountain, gorge, and valley—all these give the beholder an irresistible
impression that it is truly a world into which he is looking, a world
akin to ours, and yet no more like our world than Pompeii is like
Naples. Its air, its waters, its clouds, its life are gone, and only a
skeleton remains—a mute but eloquent witness to a cosmical tragedy
without parallel in the range of human knowledge.
One cannot but regret that the moon, if it ever was the seat of
intelligent life, has not remained so until our time. Think what the
consequences would have been if this other world at our very door had
been found to be both habitable and inhabited! We talk rather airily of
communicating with Mars by signals; but Mars never approaches nearer
than 35,000,000 miles, while the moon when nearest is only a little
more than 220,000 miles away. Given an effective magnifying power of
five thousand diameters, which will perhaps be possible at the mountain
observatories as telescopes improve, and we should be able to bring the
moon within an apparent distance of about forty miles, while the
corresponding distance for Mars would be more than seven thousand
miles. But even with existing telescopic powers we can see details on
the moon no larger than some artificial constructions on the earth. St
Peter’s at Rome, with the Vatican palace and the great piazza, if
existing on the moon, would unquestionably be recognizable as something
else than a freak of nature. Large cities, with their radiating lines
of communication, would at once betray their real character. Cultivated
tracts, and the changes produced by the interference of intelligent
beings, would be clearly recognizable. The electric illumination of a
large town at night would probably be markedly visible. Gleams of
reflected sunlight would come to us from the surfaces of the lakes and
oceans, and a huge “liner” traversing a lunar sea could probably be
followed by its trail of smoke. As to communications by “wireless”
signals, which certain enthusiasts have thought of in connection with
Mars, in the case of the moon they should be a relatively simple
matter, and the feat might actually be accomplished. Think what a
literature would grow up about the moon if it were a living world! Its
very differences from the earth would only accentuate its interest for
us. Night and day on the moon are each two weeks in length; how
interesting it would be to watch the manner in which the lunarians
dealt with such a situation as that. Lunar and terrestrial history
would keep step with each other, and we should record them both. Truly
one might well wish to have a neighbor world to study; one would feel
so much the less alone in space.
It is not impossible that the moon did at one time have inhabitants of
some kind. But, if so, they vanished with the disappearance of its
atmosphere and seas, or with the advent of its cataclysmic age. At the
best, its career as a living world must have been brief. If the water
and air were gradually absorbed, as some have conjectured, by its
cooling interior rocks, its surface might, nevertheless, have retained
them for long ages; but if, as others think, their disappearance was
due to the escape of their gaseous molecules in consequence of the
inability of the relatively small lunar gravitation to retain them,
then the final catastrophe must have been as swift as it was
inevitable. Accepting Darwin’s hypothesis, that the moon was separated
from the earth by tidal action while both were yet plastic or nebulous,
we may reasonably conclude that it began its career with a good supply
of both water and air, but did not possess sufficient mass to hold them
permanently. Yet it may have retained them long enough for life to
develop in many forms upon its surface; in fact, there are so many
indications that air and water have not always been lacking to the
lunar world that we are driven to invent theories to explain both their
former presence and their present absence.
[Illustration: The craters Clavius, Longomontanus, Tycho, etc.]
But whatever the former condition of the moon may have been, its
existing appearance gives it a resistless fascination, and it bears so
clearly the story of a vast catastrophe sculptured on its rocky face
that the thoughtful observer cannot look upon it without a feeling of
awe. The gigantic character of the lunar features impresses the
beholder not less than the universality of the play of destructive
forces which they attest. Let us make a few comparisons. Take the lunar
crater called “Tycho”, which is a typical example of its kind. In the
telescope Tycho appears as a perfect ring surrounding a circular
depression, in the center of which rises a group of mountains. Its
superficial resemblance to some terrestrial volcanic craters is very
striking. Vesuvius, seen from a point vertically above, would no doubt
look something like that (the resemblance would have been greater when
the Monte del Cavallo formed a more complete circuit about the crater
cone). But compare the dimensions. The remains of the outer crater ring
of Vesuvius are perhaps half a mile in diameter, while the active
crater itself is only two or three hundred feet across at the most;
Tycho has a diameter of fifty-four miles! The group of relatively
insignificant peaks in the center of the crater floor of Tycho is far
more massive than the entire mountain that we call Vesuvius. The
largest known volcanic crater on the earth, Aso San, in Japan, has a
diameter of seven miles; it would take _sixty_ craters like Aso San to
equal Tycho in area! And Tycho, though one of the most perfect, is by
no means the largest crater on the moon. Another, called “Theophilus,”
has a diameter of sixty-four miles, and is eighteen thousand feet deep.
There are hundreds from ten to forty miles in diameter, and thousands
from one to ten miles. They are so numerous in many places that they
break into one another, like the cells of a crushed honeycomb.
The lunar craters differ from those of the earth more fundamentally
than in the matter of mere size; _they are not situated on the tops of
mountains._ If they were, and if all the proportions were the same, a
crater like Tycho might crown a conical peak fifty or one hundred miles
high! Instead of being cavities in the summits of mountains, the lunar
craters are rather gigantic sink-holes whose bottoms in many cases lie
two or three miles below the general surface of the lunar world. Around
their rims the rocks are piled up to a height of from a few hundred to
two or three thousand feet, with a comparatively gentle inclination,
but on the inner side they fall away in gigantic broken precipices
which make the dizzy cliffs of the Matterhorn seem but “lover’s leaps.”
Down they drop, ridge below ridge, crag under crag, tottering wall
beneath wall, until, in a crater named “Newton,” near the south lunar
pole, they attain a depth where the rays of the sun never reach.
Nothing more frightful than the spectacle which many of these terrible
chasms present can be pictured by the imagination. As the lazy lunar
day slowly advances, the sunshine, unmitigated by clouds or atmospheric
veil of any kind, creeps across their rims and begins to descend the
opposite walls. Presently it strikes the ragged crest of a ridge which
had lain hidden in such darkness as we never know on the earth, and
runs along it like a line of kindling fire. Rocky pinnacles and needles
shoot up into the sunlight out of the black depths. Down sinks the line
of light, mile after mile, and continually new precipices and cliffs
are brought into view, until at last the vast floor is attained and
begins to be illuminated. In the meanwhile the sun’s rays, darting
across the gulf, have touched the summits of the central peaks, twenty
or thirty miles from the crater’s inmost edge, and they immediately
kindle and blaze like huge stars amid the darkness. So profound are
some of these awful craters that days pass before the sun has risen
high enough above them to chase the last shadows from their depths.
Although several long ranges of mountains resembling those of the earth
exist on the moon, the great majority of its elevations assume the
crateriform aspect. Sometimes, instead of a crater, we find an immense
mountain ring whose form and aspect hardly suggest volcanic action. But
everywhere the true craters are in evidence, even on the sea-beds,
although they attain their greatest number and size on those parts of
the moon—covering sixty per cent of its visible surface—which are
distinctly mountainous in character and which constitute its most
brilliant portions. Broadly speaking, the southwestern half of the moon
is the most mountainous and broken, and the northeastern half the least
so. Right down through the center, from pole to pole, runs a wonderful
line of craters and crateriform valleys of a magnitude stupendous even
for the moon. Another similar line follows the western edge. Three or
four “seas” are thrust between these mountainous belts. By the effects
of “libration” parts of the opposite hemisphere of the moon which is
turned away from the earth are from time to time brought into view, and
their aspect indicates that that hemisphere resembles in its surface
features the one which faces the earth. There are many things about the
craters which seem to give some warrant for the hypothesis which has
been particularly urged by Mr G. K. Gilbert, that they were formed by
the impact of meteors; but there are also many things which militate
against that idea, and, upon the whole, the volcanic theory of their
origin is to be preferred.
The enormous size of the lunar volcanoes is not so difficult to account
for when we remember how slight is the force of lunar gravity as
compared with that of the earth. With equal size and density, bodies on
the moon weigh only one-sixth as much as on the earth. Impelled by the
same force, a projectile that would go ten miles on the earth would go
sixty miles on the moon. A lunar giant thirty-five feet tall would
weigh no more than an ordinary son of Adam weighs on his greater
planet. To shoot a body from the earth so that it would not drop back
again, we should have to start it with a velocity of seven miles per
second; a mile and a half per second would serve on the moon. It is by
no means difficult to believe, then, that a lunar volcano might form a
crater ring eight or ten times broader than the greatest to be found on
the earth, especially when we reflect that in addition to the
relatively slight force of gravity, the materials of the lunar crust
are probably lighter than those of our terrestrial rocks.
[Illustration: Western part of the Mare Serenitatis]
For similar reasons it seems not impossible that the theory mentioned
in a former chapter—that some of the meteorites that have fallen upon
the earth originated from the lunar volcanoes—is well founded. This
would apply especially to the stony meteorites, for it is hardly to be
supposed that the moon, at least in its superficial parts, contains
much iron. It is surely a scene most strange that is thus presented to
the mind’s eye—that little attendant of the earth’s (the moon has only
one-fiftieth of the volume, and only one-eightieth of the mass of the
earth) firing great stones back at its parent planet! And what can have
been the cause of this furious outbreak of volcanic forces on the moon?
Evidently it was but a passing stage in its history; it had enjoyed
more quiet times before. As it cooled down from the plastic state in
which it parted from the earth, it became incrusted after the normal
manner of a planet, and then oceans were formed, its atmosphere being
sufficiently dense to prevent the water from evaporating and the
would-be oceans from disappearing continually in mist. This, if any,
must have been the period of life in the lunar world. As we look upon
the vestiges of that ancient world buried in the wreck that now covers
so much of its surface, it is difficult to restrain the imagination
from picturing the scenes which were once presented there; and, in such
a case, should the imagination be fettered? We give it free rein in
terrestrial life, and it rewards us with some of our greatest
intellectual pleasures. The wonderful landscapes of the moon offer it
an ideal field with just enough half-hidden suggestions of facts to
stimulate its powers.
The great plains of the _Mare Imbrium_ and the _Mare Serenitatis_ (the
“Sea of Showers” and the “Sea of Serenity”), bordered in part by lofty
mountain ranges precisely like terrestrial mountains, scalloped along
their shores with beautiful bays curving back into the adjoining
highlands, and united by a great strait passing between the nearly
abutting ends of the “Lunar Apennines” and the “Lunar Caucasus,” offer
the elements of a scene of world beauty such as it would be difficult
to match upon our planet. Look at the finely modulated bottom of the
ancient sea in Mr Ritchey’s exquisite photograph of the western part of
the _Mare Serenitatis,_ where one seems to see the play of the watery
currents heaping the ocean sands in waving lines, making shallows,
bars, and deeps for the mariner to avoid or seek, and affording a
playground for the creatures of the main. What geologist would not wish
to try his hammer on those rocks with their stony pages of fossilized
history? There is in us an instinct which forbids us to think that
there was never any life there. If we could visit the moon, there is
not among us a person so prosaic and unimaginative that he would not,
the very first thing, begin to search for traces of its inhabitants. We
would look for them in the deposits on the sea bottoms; we would
examine the shores wherever the configuration seemed favorable for
harbors and the sites of maritime cities—forgetting that it may be a
little ridiculous to ascribe to the ancient lunarians the same ideas
that have governed the development of our race; we would search through
the valleys and along the seeming courses of vanished streams; we would
explore the mountains, not the terrible craters, but the pinnacled
chains that recall our own Alps and Rockies; seeking everywhere some
vestige of the transforming presence of intelligent life. Perhaps we
should find such traces, and perhaps, with all our searching, we should
find nothing to suggest that life had ever existed amid that universal
ruin.
[Illustration: Mare Tranquilitatis and surroundings]
Look again at the border of the “Sea of Serenity”—what a name for such
a scene!—and observe how it has been rent with almost inconceivable
violence, the wall of the colossal crater Posidonius dropping
vertically upon the ancient shore and obliterating it, while its giant
neighbor, Le Monnier, opens a yawning mouth as if to swallow the sea
itself. A scene like this makes one question whether, after all, those
may not be right who have imagined that the so-called sea bottoms are
really vast plains of frozen lava which gushed up in floods so
extensive that even the mighty volcanoes were half drowned in the fiery
sea. This suggestion becomes even stronger when we turn to another of
the photographs of Mr Ritchey’s wonderful series, showing a part of the
_Mare Tranquilitatis_ (“Sea of Tranquility”!). Notice how near the
center of the picture the outline of a huge ring with radiating ridges
shows through the sea bottom; a fossil volcano submerged in a petrified
ocean! This is by no means the only instance in which a buried world
shows itself under the great lunar plains. Yet, as the newer craters in
the sea itself prove, the volcanic activity survived this other
catastrophe, or broke out again subsequently, bringing more ruin to
pile upon ruin.
Yet notwithstanding the evidence which we have just been considering in
support of the hypothesis that the “seas” are lava floods, Messrs.
Loewy and Puiseux, the selenographers of the Paris Observatory, are
convinced that these great plains bear characteristic marks of the
former presence of immense bodies of water. In that case we should be
forced to conclude that the later oceans of the moon lay upon vast
sheets of solidified lava; and thus the catastrophe of the lunar world
assumes a double aspect, the earliest oceans being swallowed up in
molten floods issuing from the interior, while the lands were reduced
to chaos by a universal eruption of tremendous volcanoes; and then a
period of comparative quiet followed, during which new seas were
formed, and new life perhaps began to flourish in the lunar world, only
to end in another cataclysm, which finally put a term to the existence
of the moon as a life-supporting world.
Suppose we examine two more of Mr Ritchey’s illuminating photographs,
and, first, the one showing the crater Theophilus and its surroundings.
We have spoken of Theophilus before, citing the facts that it is
sixty-four miles in diameter and eighteen thousand feet deep. It will
be noticed that it has two brother giants—Cyrillus the nearer, and
Catharina the more distant; but Theophilus is plainly the youngest of
the trio. Centuries, and perhaps thousands of years, must have elapsed
between the periods of their upheaval, for the two older craters are
partly filled with débris, while it is manifest at a glance that when
the south eastern wall of Theophilus was formed, it broke away and
destroyed a part of the more ancient ring of Cyrillus. There is no more
tremendous scene on the moon than this; viewed with a powerful
telescope, it is absolutely appalling.
[Illustration: Lunar craters Theophilus and surrounding region]
The next photograph shows, if possible, a still wilder region. It is
the part of the moon lying between Tycho and the south pole. Tycho is
seen in the lower left-hand part of the picture. To the right, at the
edge of the illuminated portion of the moon, are the crater-rings,
Longomontanus and Wilhelm I, the former being the larger. Between them
are to be seen the ruins of two or three more ancient craters which,
together with portions of the walls of Wilhelm I and Longomontanus,
have been honeycombed with smaller craters. The vast crateriform
depression above the center of the picture is Clavius, an unrivaled
wonder of lunar scenery, a hundred and forty-two miles in its greatest
length, while its whole immense floor has sunk two miles below the
general surface of the moon outside the ring. The monstrous
shadow-filled cavity above Clavius toward the right is Blancanus, whose
aspect here gives a good idea of the appearance of these chasms when
only their rims are in the sunlight. But observe the indescribable
savagery of the entire scene. It looks as though the spirit of
destruction had gone mad in this spot. The mighty craters have broken
forth one after another, each rending its predecessor; and when their
work was finished, a minor but yet tremendous outbreak occurred, and
the face of the moon was gored and punctured with thousands of smaller
craters. These relatively small craters (small, however, only in a
lunar sense, for many of them would appear gigantic on the earth)
recall once more the theory of meteoric impact. It does not seem
impossible that some of them may have been formed by such an agency.
One would not wish for our planet such a fate as that which has
overtaken the moon, but we cannot be absolutely sure that something of
the kind may not be in store for it. We really know nothing of the
ultimate causes of volcanic activity, and some have suggested that the
internal energies of the earth may be accumulating instead of dying
out, and may never yet have exhibited their utmost destructive power.
Perhaps the best assurance that we can find that the earth will escape
the catastrophe that has overtaken its satellite is to be found in the
relatively great force of its gravitation. The moon has been the victim
of its weakness; given equal forces, and the earth would be the better
able to withstand them. It is significant, in connection with these
considerations, that the little planet Mercury, which seems also to
have parted with its air and water, shows to the telescope some
indications that it is pitted with craters resembling those that have
torn to pieces the face of the moon.
Upon the whole, after studying the dreadful lunar landscapes, one
cannot feel a very enthusiastic sympathy with those who are seeking
indications of the continued existence of some kind of life on the
moon; such a world is better without inhabitants. It has met its fate;
let it go! Fortunately, it is not so near that it cannot hide its scars
and appear beautiful—except when curiosity impels us to look with the
penetrating eyes of the astronomer.
[Illustration: Mare Crisium]
XIII
The Great Mars Problem
Let any thoughtful person who is acquainted with the general facts of
astronomy look up at the heavens some night when they appear in their
greatest splendor, and ask himself what is the strongest impression
that they make upon his mind. He may not find it easy to frame an
answer, but when he has succeeded it will probably be to the effect
that the stars give him an impression of the universality of
intelligence; they make him feel, as the sun and the moon cannot do,
that his world is not alone; that all this was not made simply to form
a gorgeous canopy over the tents of men. If he is of a devout turn of
mind, he thinks, as he gazes into those fathomless deeps and among
those bewildering hosts, of the infinite multitude of created beings
that the Almighty has taken under his care. The narrow ideas of the old
geocentric theology, which made the earth God’s especial footstool, and
man his only rational creature, fall away from him like a veil that had
obscured his vision; they are impossible in the presence of what he
sees above. Thus the natural tendency, in the light of modern progress,
is to regard the universe as everywhere filled with life.
But science, which is responsible for this broadening of men’s thoughts
concerning the universality of life, itself proceeds to set limits. Of
spiritual existences it pretends to know nothing, but as to physical
beings, it declares that it can only entertain the supposition of their
existence where it finds evidence of an environment suited to their
needs, and such environment may not everywhere exist. Science, though
repelled by the antiquated theological conception of the supreme
isolation of man among created beings, regards with complacency the
probability that there are regions in the universe where no organic
life exists, stars which shine upon no inhabited worlds, and planets
which nourish no animate creatures. The astronomical view of the
universe is that it consists of matter in every stage of evolution:
some nebulous and chaotic; some just condensing into stars (suns) of
every magnitude and order; some shaped into finished solar bodies
surrounded by dependent planets; some forming stars that perhaps have
no planets, and will have none; some constituting suns that are already
aging, and will soon lose their radiant energy and disappear; and some
aggregated into masses that long ago became inert, cold, and rayless,
and that can only be revivified by means about which we can form
conjectures, but of which we actually know nothing.
As with the stars, so with the planets, which are the satellites of
stars. All investigations unite to tell us that the planets are not all
in the same state of development. As some are large and some small, so
some are, in an evolutionary sense, young, and some old. As they depend
upon the suns around which they revolve for their light, heat, and
other forms of radiant energy, so their condition varies with their
distance from those suns. Many may never arrive at a state suitable for
the maintenance of life upon their surfaces; some which are not at
present in such a state may attain it later; and the forms of life
themselves may vary with the peculiar environment that different
planets afford. Thus we see that we are not scientifically justified in
affirming that life is ubiquitous, although we are thus justified in
saying that it must be, in a general sense, universal. We might liken
the universe to a garden known to contain every variety of plant. If on
entering it we see no flowers, we examine the species before us and
find that they are not of those which bloom at this particular season,
or perhaps they are such as never bear flowers. Yet we feel no doubt
that we shall find flowers somewhere in the garden, because there _are_
species which bloom at this season, and the garden contains _all_
varieties.
While it is tacitly assumed that there are planets revolving around
other stars than the sun, it would be impossible for us to see them
with any telescope yet invented, and no instrument now in the
possession of astronomers could assure us of their existence; so the
only planetary system of which we have visual knowledge is our own.
Excluding the asteroids, which could not from any point of view be
considered as habitable, we have in the solar system eight planets of
various sizes and situated at various distances from the sun. Of these
eight we know that one, the earth, is inhabited. The question, then,
arises: Are there any of the others which are inhabited or habitable?
Since it is our intention to discuss the habitability of only one of
the seven to which the question applies, the rest may be dismissed in a
few words. The smallest of them, and the nearest to the sun, is
Mercury, which is regarded as uninhabitable because it has no
perceptible supply of water and air, and because, owing to the
extraordinary eccentricity of its orbit, it is subjected to excessive
and very rapid alterations in the amount of solar heat and light poured
upon its surface, such alterations being inconsistent with the
supposition that it can support living beings. Even its average
temperature is more than six and a half times that prevailing on the
earth! Another circumstance which militates against its habitability is
that, according to the results of the best telescopic studies, it
always keeps the same face toward the sun, so that one half of the
planet is perpetually exposed to the fierce solar rays, and the other
half faces the unmitigated cold of open space. Venus, the next in
distance from the sun, is almost the exact twin of the earth in size,
and many arguments may be urged in favor of its habitability, although
it is suspected of possessing the same peculiarity as Mercury, in
always keeping the same side sunward. Unfortunately its atmosphere
appears to be so dense that no permanent markings on its surface are
certainly visible, and the question of its actual condition must, for
the present, be left in abeyance. Mars, the first planet more distant
from the sun than the earth, is the special subject of this chapter,
and will be described and discussed a few lines further on. Jupiter,
Saturn, Uranus, and Neptune, the four giant planets, all more distant
than Mars, and each more distant than the other in the order named, are
all regarded as uninhabitable because none of them appears to possess
any degree of solidity. They may have solid or liquid nuclei, but
exteriorly they seem to be mere balls of cloud. Of course, one can
imagine what he pleases about the existence of creatures suited to the
physical constitution of such planets as these, but they must be
excluded from the category of habitable worlds in the ordinary sense of
the term. We go back, then, to Mars.
It will be best to begin with a description of the planet. Mars is 4230
miles in diameter; its surface is not much more than one-quarter as
extensive as that of the earth (.285). Its mean distance from the sun
is 141,500,000 miles, 48,500,000 miles greater than that of the earth.
Since radiant energy varies inversely as the square of distance, Mars
receives less than half as much solar light and heat as the earth gets.
Mars’ year (period of revolution round the sun) is 687 days. Its mean
density is 71 per cent of the earth’s, and the force of gravity on its
surface is 38 per cent of that on the surface of the earth; _i.e.,_ a
body weighing one hundred pounds on the earth would, if transported to
Mars, weigh but thirty-eight pounds. The inclination of its equator to
the plane of its orbit differs very little from that of the earth’s
equator, and its axial rotation occupies 24 hours 37 minutes. so that
the length of day and night, and the extent of the seasonal changes on
Mars, are almost precisely the same as on the earth. But owing to the
greater length of its year, the seasons of Mars, while occurring in the
same order, are almost twice as long as ours. The surface of the planet
is manifestly solid, like that of our globe, and the telescope reveals
many permanent markings on it, recalling the appearance of a globe on
which geographical features have been represented in reddish and dusky
tints. Around the poles are plainly to be seen rounded white areas,
which vary in extent with the Martian seasons, nearly vanishing in
summer and extending widely in winter. The most recent spectroscopic
determinations indicate that Mars has an atmosphere perhaps as dense as
that to be found on our loftiest mountain peaks, and there is a
perceptible amount of watery vapor in this atmosphere. The surface of
the planet appears to be remarkably level, and it has no mountain
ranges. No evidences of volcanic action have been discovered on Mars.
The dusky and reddish areas were regarded by the early observers as
respectively seas and lands, but at present it is not believed that
there are any bodies of water on the planet. There has never been much
doubt expressed that the white areas about the poles represent snow.
It will be seen from this brief description that many remarkable
resemblances exist between Mars and the earth, and there is nothing
wonderful in the fact that the question of the habitability of the
former has become one of extreme and wide-spread interest, giving rise
to the most diverse views, to many extraordinary speculations, and
sometimes to regrettably heated controversy. The first champion of the
habitability of Mars was Sir William Herschel, although even before his
time the idea had been suggested. He was convinced by the revelations
of his telescopes, continually increasing in power, that Mars was more
like the earth than any other planet. He could not resist the testimony
of the polar snows, whose suggestive conduct was in such striking
accord with what occurs upon the earth. Gradually, as telescopes
improved and observers increased in number, the principal features of
the planet were disclosed and charted, and “areography,” as the
geography of Mars was called, took its place among the recognized
branches of astronomical study. But it was not before 1877 that a
fundamentally new discovery in areography gave a truly sensational turn
to speculation about life on “the red planet.” In that year Mars made
one of its nearest approaches to the earth, and was so situated in its
orbit that it could be observed to great advantage from the northern
hemisphere of the earth. The celebrated Italian astronomer,
Schiaparelli, took advantage of this opportunity to make a
trigonometrical survey of the surface of Mars—as coolly and confidently
as if he were not taking his sights across a thirty-five-million-mile
gulf of empty space—and in the course of this survey he was astonished
to perceive that the reddish areas, then called continents, were
crossed in many directions by narrow, dusky lines, to which he gave the
suggestive name of “canals.” Thus a kind of firebrand was cast into the
field of astronomical speculation, which has ever since produced
disputes that have sometimes approached the violence of political
faction. At first the accuracy of Schiaparelli’s observations was
contested; it required a powerful telescope, and the most excellent
“seeing,” to render the enigmatical lines visible at all, and many
searchers were unable to detect them. But Schiaparelli continued his
studies in the serene sky of Italy, and produced charts of the
gridironed face of Mars containing so much astonishing detail that one
had either to reject them _in toto_ or to confess that Schiaparelli was
right. As subsequent favorable oppositions of Mars occurred, other
observers began to see the “canals” and to confirm the substantial
accuracy of the Italian astronomer’s work, and finally few were found
who would venture to affirm that the “canals” did not exist, whatever
their meaning might be.
[Illustration: Schiaparelli’s chart of Mars, showing the so-called
system of canals]
When Schiaparelli began his observations it was generally believed, as
we have said, that the dusky areas on Mars were seas, and since
Schiaparelli thought that the “canals” invariably began and ended at
the shores of the “seas,” the appropriateness of the title given to the
lines seemed apparent. Their artificial character was immediately
assumed by many, because they were too straight and too suggestively
geometrical in their arrangement to permit the conclusion that they
were natural watercourses. A most surprising circumstance noted by
Schiaparelli was that the “canals” made their appearance _after_ the
melting of the polar snow in the corresponding hemisphere had begun,
and that they grew darker, longer, and more numerous in proportion as
the polar liquidation proceeded; another very puzzling observation was
that many of them became double as the season advanced; close beside an
already existing “canal,” and in perfect parallelism with it, another
would gradually make its appearance. That these phenomena actually
existed and were not illusions was proved by later observations, and
today they are seen whenever Mars is favorably situated for
observation.
In the closing decade of the nineteenth century, Mr Percival Lowell
took up the work where Schiaparelli had virtually dropped it, and soon
added a great number of “canals” to those previously known, so that in
his charts the surface of the wonderful little planet appears covered
as with a spider’s web, the dusky lines criss-crossing in every
direction, with conspicuous knots wherever a number of them come
together. Mr Lowell has demonstrated that the areas originally called
seas, and thus named on the earlier charts, are not bodies of water,
whatever else they may be. He has also found that the mysterious lines
do not, as Schiaparelli supposed, begin and end at the edges of the
dusky regions, but often continue on across them, reaching in some
cases far up into the polar regions. But Schiaparelli was right in his
observation that the appearance of the “canals” is synchronous with the
gradual disappearance of the polar snows, and this fact has become the
basis of the most extraordinary theory that the subject of life in
other worlds has ever given birth to.
Now, the effect of such discoveries, as we have related, depends upon
the type of mind to whose attention they are called. Many are content
to accept them as strange and inexplicable at present, and to wait for
further light upon them; others insist upon an immediate inquiry
concerning their probable nature and meaning. Such an inquiry can only
be based upon inference proceeding from analogy. Mars, say Mr Lowell
and those who are of his opinion, is manifestly a solidly incrusted
planet like the earth; it has an atmosphere, though one of great
rarity; it has water vapor, as the snows in themselves prove; it has
the alternation of day and night, and a succession of seasons closely
resembling those of the earth; its surface is suggestively divided into
regions of contrasting colors and appearance, and upon that surface we
see an immense number of lines geometrically arranged, with a system of
symmetrical intersections where the lines expand into circular and oval
areas—and all connected with the annual melting of the polar snows in a
way which irresistibly suggests the interference of intelligence
directed to a definite end. Why, with so many concurrent circumstances
to support the hypothesis, should we not regard Mars as an inhabited
globe?
But the differences between Mars and the earth are in many ways as
striking as their resemblances. Mars is relatively small; it gets less
than half as much light and heat as we receive; its atmosphere is so
rare that it would be distressing to us, even if we could survive in it
at all; it has no lakes, rivers, or seas; its surface is an endless
prairie. and its “canals” are phenomena utterly unlike anything on the
earth. Yet it is precisely upon these divergences between the earth and
Mars, this repudiation of terrestrial standards, that the theory of
“life on Mars,” for which Mr Lowell is mainly responsible, is based.
Because Mars is smaller than the earth, we are told it must necessarily
be more advanced in planetary evolution, the underlying cause of which
is the gradual cooling and contraction of the planet’s mass. Mars has
parted with its internal heat more rapidly than the earth; consequently
its waters and its atmosphere have been mostly withdrawn by chemical
combinations, but enough of both yet remain to render life still
possible on its surface. As the globe of Mars is evolutionally older
than that of the earth, so its forms of organic life may be
proportionally further advanced, and its inhabitants may have attained
a degree of cultivated intelligence much superior to what at present
exists upon the earth. Understanding the nature and the causes of the
desiccation of their planet, and possessing engineering science and
capabilities far in advance of ours, they may be conceived to have
grappled with the stupendous problem of keeping their world in a
habitable condition as long as possible. Supposing them to have become
accustomed to live in their rarefied atmosphere (a thing not
inconceivable, since men can live for a time at least in air hardly
less rare), the most pressing problem for them is that of a
water-supply, without which plant life cannot exist, while animal life
in turn depends for its existence upon vegetation. The only direction
in which they can seek water is that of the polar regions, where it is
alternately condensed into snow and released in the liquid form by the
effect of the seasonal changes. It is, then, to the annual melting of
the polar snow-fields that the Martian engineers are supposed to have
recourse in supplying the needs of their planet, and thus providing the
means of prolonging their own existence. It is imagined that they have
for this purpose constructed a stupendous system of irrigation
extending over the temperate and equatorial regions of the planet. The
“canals” represent the lines of irrigation, but the narrow streaks that
we see are not the canals themselves, but the irrigated bands covered
by them. Their dark hue, and their gradual appearance after the polar
melting has begun, are due to the growth of vegetation stimulated by
the water. The rounded areas visible where several “canals” meet and
cross are called by Mr Lowell “oases.” These are supposed to be the
principal centers of population and industry. It must be confessed that
some of them, with their complicated systems of radiating lines, appear
to answer very well to such a theory. No attempt to explain them by
analogy with natural phenomena on the earth has proved successful.
But a great difficulty yet remains: How to explain the seemingly
miraculous powers of the supposed engineers? Here recourse is had once
more to the relative smallness of the planet. We have remarked that the
force of gravity on Mars is only thirty-eight per cent of that on the
earth. A steam-shovel driven by a certain horse-power would be nearly
three times as effective there as here. A man of our stature on Mars
would find his effective strength increased in the same proportion. But
just because of the slight force of gravity there, a Martian might
attain to the traditional stature of Goliath without finding his own
weight an encumbrance to his activity, while at the same time his huge
muscles would come into unimpeded play, enabling him single-handed to
perform labors that would be impossible to a whole gang of terrestrial
workmen. The effective powers of huge machines would be increased in
the same way; and to all this must be added the fact that the mean
density of the materials of which Mars is composed is much less than
that of the constituents of the earth. Combining all these
considerations, it becomes much less difficult to conceive that public
works might be successfully undertaken on Mars which would be
hopelessly beyond the limits of human accomplishment.
Certain other difficulties have also to be met; as, for instance, the
relative coldness of the climate of Mars. At its distance it gets
considerably less than half as much light and heat as we receive. In
addition to this, the rarity of its atmosphere would naturally be
expected to decrease the effective temperature at the planet’s surface,
since an atmosphere acts somewhat like the glass cover of a hot-house
in retaining the solar heat which has penetrated it. It has been
calculated that, unless there are mitigating circumstances of which we
know nothing, the average temperature at the surface of Mars must be
far below the freezing-point of water. To this it is replied that the
possible mitigating circumstances spoken of evidently exist in fact,
because we can _see_ that the watery vapor condenses into snow around
the poles in winter, but melts again when summer comes. The mitigating
agent may be supposed to exist in the atmosphere where the presence of
certain gases would completely alter the temperature gradients.
It might also be objected that it is inconceivable that the Martian
engineers, however great may be their physical powers, and however
gigantic the mechanical energies under their control, could force water
in large quantities from the poles to the equator. This is an
achievement that measures up to the cosmical standard. It is admitted
by the champions of the theory that the difficulty is a formidable one;
but they call attention to the singular fact that on Mars there can be
found no chains of mountains, and it is even doubtful if ranges of
hills exist there. The entire surface of the planet appears to be
almost “as smooth as a billiard ball,” and even the broad regions which
were once supposed to be seas apparently lie at practically the same
level as the other parts, since the “canals” in many cases run
uninterruptedly across them. Lowell’s idea is that these sombre areas
may be expanses of vegetation covering ground of a more or less marshy
character, for while the largest of them appear to be permanent, there
are some which vary coincidently with the variations of the canals.
As to the kind of machinery employed to force the water from the poles,
it has been conjectured that it may have taken the form of a gigantic
system of pumps and conduits; and since the Martians are assumed to be
so far in advance of us in their mastery of scientific principles, the
hypothesis will at least not be harmed by supposing that they have
learned to harness forces of nature whose very existence in a
manageable form is yet unrecognized on the earth. If we wish to let the
imagination loose, we may conjecture that they have conquered the
secret of those intra-atomic forces whose resistless energy is
beginning to become evident to us, but the possibility of whose
utilization remains a dream, the fulfillment of which nobody dares to
predict.
Such, in very brief form, is the celebrated theory of Mars as an
inhabited world. It certainly captivates the imagination, and if we
believe it to represent the facts, we cannot but watch with the deepest
sympathy this gallant struggle of an intellectual race to preserve its
planet from the effects of advancing age and death. We may, indeed,
wonder whether our own humanity, confronted by such a calamity, could
be counted on to meet the emergency with equal stoutness of heart and
inexhaustibleness of resource. Up to the present time we certainly have
shown no capacity to confront Nature toe to toe, and to seize her by
the shoulders and turn her round when she refuses to go our way. If we
could get into wireless telephonic communication with the Martians we
might learn from their own lips the secret of their more than “Roman
recovery.”
XIV
The Riddle of the Asteroids
Between the orbits of Mars and Jupiter revolves the most remarkable
system of little bodies with which we are acquainted—the Asteroids, or
Minor Planets. Some six hundred are now known, and they may actually
number thousands. They form virtually a ring about the sun. The most
striking general fact about them is that they occupy the place in the
sky which should be occupied, according to Bode’s Law, by a single
large planet. This fact, as we shall see, has led to the invention of
one of the most extraordinary theories in astronomy—_viz.,_ that of the
explosion of a world!
Bode’s Law, so-called, is only an empiric formula, but until the
discovery of Neptune it accorded so well with the distances of the
planets that astronomers were disposed to look upon it as really
representing some underlying principle of planetary distribution. They
were puzzled by the absence of a planet in the space between Mars and
Jupiter, where the “law” demanded that there should be one, and an
association of astronomers was formed to search for it. There was a
decided sensation when, in 1801, Piazzi, of Palermo, announced that he
had found a little planet which apparently occupied the place in the
system which belonged to the missing body. He named it Ceres, and it
was the first of the Asteroids. The next year Olbers, of Bremen, while
looking for Ceres with his telescope, stumbled upon another small
planet which he named Pallas. Immediately he was inspired with the idea
that these two planets were fragments of a larger one which had
formerly occupied the vacant place in the planetary ranks, and he
predicted that others would be found by searching in the neighborhood
of the intersection of the orbits of the two already discovered. This
bold prediction was brilliantly fulfilled by the finding of two
more—Juno in 1804, and Vesta in 1807. Olbers would seem to have been
led to the invention of his hypothesis of a planetary explosion by the
faith which astronomers at that time had in Bode’s Law. They appear to
have thought that several planets revolving in the gap where the “law”
called for but one could only be accounted for upon the theory that the
original _one_ had been broken up to form the several. Gravitation
demanded that the remnants of a planet blown to pieces, no matter how
their orbits might otherwise differ, should all return at stated
periods to the point where the explosion had occurred; hence Olbers’
prediction that any asteroids that might subsequently be discovered
would be found to have a common point of orbital intersection. And
curiously enough all of the first asteroids found practically answered
to this requirement. Olbers’ theory seemed to be established.
After the first four, no more asteroids were found until 1845, when one
was discovered; then, in 1847, three more were added to the list; and
after that searchers began to pick them up with such rapidity that by
the close of the century hundreds were known, and it had become almost
impossible to keep track of them. The first four are by far the largest
members of the group, but their actual sizes remained unknown until
less than twenty years ago. It was long supposed that Vesta was the
largest, because it shines more brightly than any of the others; but
finally, in 1895, Barnard, with the Lick telescope, definitely measured
their diameters, and proved to everybody’s surprise that Ceres is
really the chief, and Vesta only the third in rank. His measures are as
follows: Ceres, 477 miles; Pallas, 304 miles; Vesta, 239 miles; and
Juno, 120 miles. They differ greatly in the reflective power of their
surfaces, a fact of much significance in connection with the question
of their origin. Vesta is, surface for surface, rather more than three
times as brilliant as Ceres, whence the original mistake about its
magnitude.
Nowadays new asteroids are found frequently by photography, but
physically they are most insignificant bodies, their average diameter
probably not exceeding twenty miles, and some are believed not to
exceed ten. On a planet only ten miles in diameter, assuming the same
mean density as the earth’s, which is undoubtedly too much, the force
of gravity would be so slight that an average man would not weigh more
than three ounces, and could jump off into space whenever he liked.
Although the asteroids all revolve around the sun in the same direction
as that pursued by the major planets, their orbits are inclined at a
great variety of angles to the general plane of the planetary system,
and some of them are very eccentric—almost as much so as the orbits of
many of the periodic comets. It has even been conjectured that the two
tiny moons of Mars and the four smaller satellites of Jupiter may be
asteroids gone astray and captured by those planets. Two of the
asteroids are exceedingly remarkable for the shapes and positions of
their orbits; these are Eros, discovered in 1898, and T. G., 1906,
found eight years later. The latter has a mean distance from the sun
slightly greater than that of Jupiter, while the mean distance of Eros
is less than that of Mars. The orbit of Eros is so eccentric that at
times it approaches within 15,000,000 miles of the earth, nearer than
any other regular member of the solar system except the moon, thus
affording an unrivaled means of measuring the solar parallax. But for
our present purpose the chief interest of Eros lies in its
extraordinary changes of light.
These changes, although irregular, have been observed and photographed
many times, and there seems to be no doubt of their reality. Their
significance consists in their possible connection with the form of the
little planet, whose diameter is generally estimated at not more than
twenty miles. Von Oppolzer found, in 1901, that Eros lost three-fourths
of its brilliancy once in every two hours and thirty-eight minutes.
Other observers have found slightly different periods of variability,
but none as long as three hours. The most interesting interpretation
that has been offered of this phenomenon is that it is due to a great
irregularity of figure, recalling at once Olbers’ hypothesis. According
to some, Eros may be double, the two bodies composing it revolving
around each other at very close quarters; but a more striking, and it
may be said probable, suggestion is that Eros has a form not unlike
that of a dumb-bell, or hour-glass, turning rapidly end over end so
that the area of illuminated surface presented to our eyes continually
changes, reaching at certain times a minimum when the amount of light
that it reflects toward the earth is reduced to a quarter of its
maximum value. Various other bizarre shapes have been ascribed to Eros,
such, for instance, as that of a flat stone revolving about one of its
longer axes, so that sometimes we see its face and sometimes its edge.
All of these explanations proceed upon the assumption that Eros cannot
have a simple globular figure like that of a typical planet, a figure
which is prescribed by the law of gravitation, but that its shape is
what may be called accidental; in a word, it is a _fragment,_ for it
seems impossible to believe that a body formed in interplanetary space,
either through nebular condensation or through the aggregation of
particles drawn together by their mutual attractions, should not be
practically spherical in shape. Nor is Eros the only asteroid that
gives evidence by variations of brilliancy that there is something
abnormal in its constitution; several others present the same
phenomenon in varying degrees. Even Vesta was regarded by Olbers as
sufficiently variable in its light to warrant the conclusion that it
was an angular mass instead of a globe. Some of the smaller ones show
very notable variations, and all in short periods, of three or four
hours, suggesting that in turning about one of their axes they present
a surface of variable extent toward the sun and the earth.
The theory which some have preferred—that the variability of light is
due to the differences of reflective power on different parts of the
surface—would, if accepted, be hardly less suggestive of the origin of
these little bodies by the breaking up of a larger one, because the
most natural explanation of such differences would seem to be that they
arose from variations in the roughness or smoothness of the reflecting
surface, which would be characteristic of fragmentary bodies. In the
case of a large planet alternating expanses of land and water, or of
vegetation and desert, would produce a notable variation in the amount
of reflection, but on bodies of the size of the asteroids neither water
nor vegetation could exist, and an atmosphere would be equally
impossible.
One of the strongest objections to Olbers’ hypothesis is that only a
few of the first asteroids discovered travel in orbits which measurably
satisfy the requirement that they should all intersect at the point
where the explosion occurred. To this it was at first replied that the
perturbations of the asteroidal orbits, by the attractions of the major
planets, would soon displace them in such a manner that they would
cease to intersect. One of the first investigations undertaken by the
late Prof. Simon Newcomb was directed to the solution of this question,
and he arrived at the conclusion that the planetary perturbations could
not explain the actual situation of the asteroidal orbits. But
afterward it was pointed out that the difficulty could be avoided by
supposing that not one but a series of explosions had produced the
asteroids as they now are. After the primary disruption the fragments
themselves, according to this suggestion, may have exploded, and then
the resulting orbits would be as “tangled” as the heart could wish.
This has so far rehabilitated the explosion theory that it has never
been entirely abandoned, and the evidence which we have just cited of
the probably abnormal shapes of Eros and other asteroids has lately
given it renewed life. It is a subject that needs a thorough
rediscussion.
We must not fail to mention, however, that there is a rival hypothesis
which commends itself to many astronomers—_viz.,_ that the asteroids
were formed out of a relatively scant ring of matter, situated between
Mars and Jupiter and resembling in composition the immensely more
massive rings from which, according to Laplace’s hypothesis, the
planets were born. It is held by the supporters of this theory that the
attraction of the giant Jupiter was sufficient to prevent the small,
nebulous ring that gave birth to the asteroids from condensing like the
others into a single planet.
But if we accept the explosion theory, with its corollary that minor
explosions followed the principal one, we have still an unanswered
question before us: What caused the explosions? The idea of _a world
blowing up_ is too Titanic to be shocking; it rather amuses the
imagination than seriously impresses it; in a word, it seems
essentially chimerical. We can by no appeal to experience form a mental
picture of such an occurrence. Even the moon did not blow up when it
was wrecked by volcanoes. The explosive nebulæ and new stars are far
away in space, and suggest no connection with such a catastrophe as the
bursting of a planet into hundreds of pieces. We cannot conceive of a
great globe thousands of miles in diameter resembling a pellet of
gunpowder only awaiting the touch of a match to cause its sudden
disruption. Somehow the thought of human agency obtrudes itself in
connection with the word “explosion,” and we smile at the idea that
giant powder or nitro-glycerine could blow up a planet. Yet it would
only need _enough_ of them to do it.
After all, we may deceive ourselves in thinking, as we are apt to do,
that explosive energies lock themselves up only in small masses of
matter. There are many causes producing explosions in nature, every
volcanic eruption manifests the activity of some of them. Think of the
giant power of confined steam; if enough steam could be suddenly
generated in the center of the earth by a downpour of all the waters of
the oceans, what might not the consequences be for our globe? In a
smaller globe, and it has never been estimated that the original
asteroid was even as large as the moon, such a catastrophe would,
perhaps, be more easily conceivable; but since we are compelled in this
case to assume that there was a series of successive explosions, steam
would hardly answer the purpose; it would be more reasonable to suppose
that the cause of the explosion was some kind of chemical reaction, or
something affecting the atoms composing the exploding body. Here Dr
Gustav Le Bon comes to our aid with a most startling suggestion, based
on his theory of the dissipation of intra-atomic energy. It will be
best to quote him at some length from his book on _The Evolution of
Forces._
“It does not seem at first sight,” says Doctor Le Bon,
very comprehensible that worlds which appear more and more stable as
they cool could become so unstable as to afterward dissociate entirely.
To explain this phenomenon, we will inquire whether astronomical
observations do not allow us to witness this dissociation.
We know that the stability of a body in motion, such as a top or a
bicycle, ceases to be possible when its velocity of rotation descends
below a certain limit. Once this limit is reached it loses its
stability and falls to the ground. Prof. J. J. Thomson even interprets
radio-activity in this manner, and points out that when the speed of
the elements composing the atoms descends below a certain limit they
become unstable and tend to lose their equilibria. There would result
from this a commencement of dissociation, with diminution of their
potential energy and a corresponding increase of their kinetic energy
sufficient to launch into space the products of intra-atomic
disintegration.
It must not be forgotten that the atom being an enormous reservoir of
energy is by this very fact comparable with explosive bodies. These
last remain inert so long as their internal equilibria are undisturbed.
So soon as some cause or other modifies these, they explode and smash
everything around them after being themselves broken to pieces.
Atoms, therefore, which grow old in consequence of the diminution of a
part of their intra-atomic energy gradually lose their stability. A
moment, then, arrives when this stability is so weak that the matter
disappears by a sort of explosion more or less rapid. The bodies of the
radium group offer an image of this phenomenon—a rather faint image,
however, because the atoms of this body have only reached a period of
instability when the dissociation is rather slow. It probably precedes
another and more rapid period of dissociation capable of producing
their final explosion. Bodies such as radium, thorium, etc., represent,
no doubt, a state of old age at which all bodies must some day arrive,
and which they already begin to manifest in our universe, since all
matter is slightly radio-active. It would suffice for the dissociation
to be fairly general and fairly rapid for an explosion to occur in a
world where it was manifested.
These theoretical considerations find a solid support in the sudden
appearances and disappearances of stars. The explosions of a world
which produce them reveal to us, perhaps, how the universes perish when
they become old.
As astronomical observations show the relative frequency of these rapid
destructions, we may ask ourselves whether the end of a universe by a
sudden explosion after a long period of old age does not represent its
most general ending.
Here, perhaps, it will be well to stop, since, entrancing as the
subject may be, we know very little about it, and Doctor Le Bon’s
theory affords a limitless field for the reader’s imagination.