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OTHER WORLDS

by

GARRETT P. SERVISS.



     *     *     *     *     *     *



OTHER WORLDS.

     Their Nature and Possibilities in the Light of the Latest
     Discoveries. Illustrated. 12mo. Cloth, $1.20 net; postage
     additional.

     No science has ever equaled astronomy in its appeal to the
     imagination, and recently popular interest in the wonders of the
     starry heavens has been stimulated by surprising discoveries and
     imaginary discoveries, as well as by a marked tendency of writers
     of fiction to include other worlds and their possible inhabitants
     within the field of romance.

     Mr. Serviss's new book on "Other Worlds, their Nature and
     Possibilities in the Light of the Latest Discoveries," summarizes
     what is known. With helpful illustrations, the most interesting
     facts about the planets Venus, Mars, Jupiter, Saturn, etc., as well
     as about the nearest of all other worlds, the moon, are presented
     in a popular manner, and always from the point of view of human
     interest--a point that is too seldom taken by writers on science.

ASTRONOMY WITH AN OPERA-GLASS.

     A Popular Introduction to the Study of the Starry Heavens with the
     simplest of Optical Instruments. Illustrated. 8vo. Cloth, $1.50.

     "By its aid thousands of people who have resigned themselves to the
     ignorance in which they were left at school, by our wretched system
     of teaching by the book only, will thank Mr. Serviss for the
     suggestions he has so well carried out."--_New York Times._

PLEASURES OF THE TELESCOPE.

     A Descriptive Guide to Amateur Astronomers and All Lovers of the
     Stars. Illustrated. 8vo. Cloth, $1.50.

     "The volume will be found interesting by those for whom it is
     written, and will inspire many with a love for the study of
     astronomy, one of the most far-reaching of the
     sciences."--_Milwaukee Journal._

D. APPLETON AND COMPANY, NEW YORK.



     *     *     *     *     *     *



[Illustration: CHART OF MARS. After Schiaparelli.]



OTHER WORLDS

Their Nature, Possibilities and Habitability in the Light of the Latest
Discoveries.

by

GARRETT P. SERVISS

Author of
"Astronomy with an Opera-glass" and "Pleasures of the Telescope"

With Charts and Illustrations




     "Shall we measure the councils of heaven by the narrow impotence of
     human faculties, or conceive that silence and solitude reign
     throughout the mighty empire of nature?"

     --DR. THOMAS CHALMERS.




New York
D. Appleton and Company
1901
Copyright, 1901,
by D. Appleton and Company.




TO THE MEMORY OF WILLIAM JAY YOUMANS.




PREFACE


The point of view of this book is human interest in the other worlds
around us. It presents the latest discoveries among the planets of the
solar system, and shows their bearing upon the question of life in those
planets. It points out the resemblances and the differences between the
earth and the other worlds that share with it in the light of the sun.
It shows what we should see and experience if we could visit those
worlds.

While basing itself upon facts, it does not exclude the discussion of
interesting probabilities and theories that have commanded wide popular
attention. It points out, for instance, what is to be thought of the
idea of interplanetary communication. It indicates what must be the
outlook of the possible inhabitants of some of the other planets toward
the earth. As far as may be, it traces the origin and development of the
other worlds of our system, and presents a graphic picture of their
present condition as individuals, and of their wonderful contrasts as
members of a common family.

In short, the aim of the author has been to show how wide, and how rich,
is the field of interest opened to the human mind by man's discoveries
concerning worlds, which, though inaccessible to him in a physical
sense, offer intellectual conquests of the noblest description.

And, finally, in order to assist those who may wish to recognize for
themselves these other worlds in the sky, this book presents a special
series of charts to illustrate a method of finding the planets which
requires no observatory and no instruments, and only such knowledge of
the starry heavens as anybody can easily acquire.

G.P.S.


BOROUGH OF BROOKLYN, NEW YORK CITY,
_September, 1901._




CONTENTS


CHAPTER I

_INTRODUCTORY_                                                1

     Remarkable popular interest in questions concerning
     other worlds and their inhabitants--Theories of
     interplanetary communication--The plurality of worlds in
     literature--Romances of foreign planets--Scientific interest
     in the subject--Opposing views based on telescopic and
     spectroscopic revelations--Changes of opinion--Desirability
     of a popular presentation of the latest facts--The natural
     tendency to regard other planets as habitable--Some of the
     conditions and limitations of the problem--The solar system
     viewed from outer space--The resemblances and contrasts of
     its various planets--Three planetary groups recognized--The
     family character of the solar system


CHAPTER II

_MERCURY, A WORLD OF TWO FACES AND MANY CONTRASTS_           18

     Grotesqueness of Mercury considered as a world--Its
     dimensions, mass, and movements--The question of an
     atmosphere--Mercury's visibility from the earth--Its
     eccentric orbit, and rapid changes of distance from the
     sun--Momentous consequences of these peculiarities--A
     virtual fall of fourteen million miles toward the sun
     in six weeks--The tremendous heat poured upon Mercury
     and its great variations--The little planet's singular
     manner of rotation on its axis--Schiaparelli's astonishing
     discovery--A day side and a night side--Interesting effects
     of libration--The heavens as viewed from Mercury--Can it
     support life?


CHAPTER III

_VENUS, THE TWIN OF THE EARTH_                               46

     A planet that matches ours in size--Its beauty in the
     sky--Remarkable circularity of its orbit--Probable
     absence of seasons and stable conditions of temperature
     and weather on Venus--Its dense and abundant atmosphere--Seeing
     the atmosphere of Venus from the earth--Is the real face of the
     planet hidden under an atmospheric veil?--Conditions of
     habitability--All planetary life need not be of the terrestrial
     type--The limit fixed by destructive temperature--Importance of
     air and water in the problem--Reasons why Venus may be a
     more agreeable abode than the earth--Splendor of our globe
     as seen from Venus--What astronomers on Venus might learn
     about the earth--A serious question raised--Does Venus, like
     Mercury, rotate but once in the course of a revolution about
     the sun?--Reasons for and against that view


CHAPTER IV

_MARS, A WORLD MORE ADVANCED THAN OURS_                      85

     Resemblances between Mars and the earth--Its seasons and its
     white polar caps--Peculiar surface markings--Schiaparelli's
     discovery of the canals--His description of their appearance
     and of their duplication--Influence of the seasons on the
     aspect of the canals--What are the canals?--Mr. Lowell's
     observations--The theory of irrigation--How the inhabitants
     of Mars are supposed to have taken advantage of the annual
     accession of water supplied by the melting of the polar
     caps--Wonderful details shown in charts of Mars--Curious
     effects that may follow from the small force of gravity
     on Mars--Imaginary giants--Reasons for thinking that
     Mars may be, in an evolutionary sense, older than the
     earth--Speculations about interplanetary signals from
     Mars, and their origin--Mars's atmosphere--The question of
     water--The problem of temperature--Eccentricities of Mars's
     moons


CHAPTER V

_THE ASTEROIDS, A FAMILY OF DWARF WORLDS_                   129

     Only four asteroids large enough to be measured--Remarkable
     differences in their brightness irrespective of size--Their
     widely scattered and intermixed orbits--Eccentric orbit of
     Eros--the nearest celestial body to the earth except the
     moon--Its existence recorded by photography before it was
     discovered--Its great and rapid fluctuations in light, and
     the curious hypotheses based upon them--Is it a fragment of
     an exploded planet?--The startling theory of Olbers as to
     the origin of the asteroids revived--Curious results of the
     slight force of gravity on an asteroid--An imaginary visit
     to a world only twelve miles in diameter


CHAPTER VI

_JUPITER, THE GREATEST OF KNOWN WORLDS_                     160

     Jupiter compared with our globe--His swift rotation on his
     axis--Remarkable lack of density--The force of gravity on
     Jupiter--Wonderful clouds--Strange phenomena of the great
     belts--Brilliant display of colors--The great red spot
     and the many theories it has given rise to--Curious facts
     about the varying rates of rotation of the huge planet's
     surface--The theory of a hidden world in Jupiter--When
     Jupiter was a companion star to the sun--The miracle of
     world-making before our eyes--Are Jupiter's satellites
     habitable?--Magnificent spectacles in the Jovian system


CHAPTER VII

_SATURN, A PRODIGY AMONG PLANETS_                           185

     The wonder of the great rings--Saturn's great distance and
     long year--The least dense of all the planets--It would
     float in water--What kind of a world is it?--Sir Humphry
     Davy's imaginary inhabitants of Saturn--Facts about the
     rings, which are a phenomenon unparalleled in the visible
     universe--The surprising nature of the rings, as revealed
     by mathematics and the spectroscope--The question of their
     origin and ultimate fate--Dr. Dick's idea of their
     habitability--Swedenborg's curious description of the
     appearance of the rings from Saturn--Is Saturn a globe of
     vapor, or of dust?--The nine satellites and "Roche's
     limit"--The play of spectacular shadows in the Saturnian
     system--Uranus and Neptune--Is there a yet undiscovered
     planet greater than Jupiter?


CHAPTER VIII

_THE MOON, CHILD OF THE EARTH AND THE SUN_                  212

     The moon a favorite subject for intellectual speculation--Its
     nearness to the earth graphically illustrated--Ideas of the
     ancients--Galileo's discoveries--What first raised a serious
     question as to its habitability--Singularity of the moon's
     motions--Appearance of its surface to the naked eye and with
     the telescope--The "seas" and the wonderful mountains and
     craters--A terrible abyss described--Tycho's mysterious
     rays--Difference between lunar and terrestrial
     volcanoes--Mountain-ringed valleys--Gigantic cracks in the
     lunar globe--Slight force of gravity of the moon and some
     interesting deductions--The moon a world of giantism--What
     kind of atmospheric gases can the moon contain--The question
     of water and of former oceans--The great volcanic cataclysm
     in the moon's history--Evidence of volcanic and other
     changes now occurring--Is there vegetation on the
     moon?--Lunar day and night--The earth as seen from the
     moon--Discoveries yet to be made


CHAPTER IX

_HOW TO FIND THE PLANETS_                                   256

     It is easy to make acquaintance with the planets and to
     follow them among the stars--The first step a knowledge of
     the constellations--How this is to be acquired--How to use
     the Nautical Almanac in connection with the charts in this
     book--The visibility of Mercury and Venus--The oppositions
     of Mars, Jupiter, and Saturn


INDEX                                                       277




LIST OF ILLUSTRATIONS


                                                                   PAGE
Chart of Mars                                             _Frontispiece_

Diagram showing causes of day and night on portions of Mercury       35

Regions of day and night on Mercury                                  38

Venus's atmosphere seen as a ring of light                           56

View of Jupiter                                            _facing_ 168

Three views of Saturn                                      _facing_ 186

Diagram showing the moon's path through space                       217

The lunar Alps, Apennines, and Caucasus                    _facing_ 222

The moon at first and last quarter                         _facing_ 226

Phases and rotation of the moon                                     250

Charts showing the zodiacal constellations:
  1. From right ascension 0 hours to 4 hours                        259
  2.    "           "     4   "   "  8   "                          261
  3.    "           "     8   "   "  2   "                          263
  4.    "           "    12   "   " 16   "                          265
  5.    "           "    16   "   " 20   "                          267
  6.    "           "    20   "   " 24   "                          269




OTHER WORLDS




CHAPTER I

INTRODUCTORY


Other worlds and their inhabitants are remarkably popular subjects of
speculation at the present time. Every day we hear people asking one
another if it is true that we shall soon be able to communicate with
some of the far-off globes, such as Mars, that circle in company with
our earth about the sun. One of the masters of practical electrical
science in our time has suggested that the principle of wireless
telegraphy may be extended to the transmission of messages across space
from planet to planet. The existence of intelligent inhabitants in some
of the other planets has become, with many, a matter of conviction, and
for everybody it presents a question of fascinating interest, which has
deeply stirred the popular imagination.

The importance of this subject as an intellectual phenomenon of the
opening century is clearly indicated by the extent to which it has
entered into recent literature. Poets feel its inspiration, and
novelists and romancers freely select other planets as the scenes of
their stories. One tells us of a visit paid by men to the moon, and of
the wonderful things seen, and adventures had, there. Lucian, it is
true, did the same thing eighteen hundred years ago, but he had not the
aid of hints from modern science to guide his speculations and lend
verisimilitude to his narrative.

Another startles us from our sense of planetary security with a
realistic account of the invasion of the earth by the terrible sons of
warlike Mars, seeking to extend their empire by the conquest of foreign
globes.

Sometimes it is a trip from world to world, a kind of celestial pleasure
yachting, with depictions of creatures more wonderful than--

    "The anthropophagi and men whose heads
    Do grow beneath their shoulders"--

that is presented to our imagination; and sometimes we are informed of
the visions beheld by the temporarily disembodied spirits of trance
mediums, or other modern thaumaturgists, flitting about among the
planets.

Then, to vary the theme, we find charming inhabitants of other worlds
represented as coming down to the earth and sojourning for a time on our
dull planet, to the delight of susceptible successors of father Adam,
who become, henceforth, ready to follow their captivating visitors to
the ends of the universe.

In short, writers of fiction have already established interplanetary
communication to their entire satisfaction, thus vastly and indefinitely
enlarging the bounds of romance, and making us so familiar with the
peculiarities of our remarkable brothers and sisters of Mars, Venus,
and the moon, that we can not help feeling, notwithstanding the many
divergences in the descriptions, that we should certainly recognize them
on sight wherever we might meet them.

But the subject is by no means abandoned to the tellers of tales and the
dreamers of dreams. Men of science, also, eagerly enter into the
discussion of the possibilities of other worlds, and become warm over
it.

Around Mars, in particular, a lively war of opinions rages. Not all
astronomers have joined in the dispute--some have not imagination
enough, and some are waiting for more light before choosing sides--but
those who have entered the arena are divided between two opposed camps.
One side holds that Mars is not only a world capable of having
inhabitants, but that it actually has them, and that they have given
visual proof of their existence and their intelligence through the
changes they have produced upon its surface. The other side maintains
that Mars is neither inhabited nor habitable, and that what are taken
for vast public works and engineering marvels wrought by its
industrious inhabitants, are nothing but illusions of the telescope, or
delusions of the observer's mind. Both adduce numerous observations,
telescopic and spectroscopic, and many arguments, scientific and
theoretic, to support their respective contentions, but neither side has
yet been able to convince or silence the other, although both have made
themselves and their views intensely interesting to the world at large,
which would very much like to know what the truth really is.

And not only Mars, but Venus--the beauteous twin sister of the earth,
who, when she glows in the evening sky, makes everybody a lover of the
stars--and even Mercury, the Moor among the planets, wearing "the
shadowed livery of the burnished sun," to whom he is "a neighbor and
near bred," and Jupiter, Saturn, and the moon itself--all these have
their advocates, who refuse to believe that they are lifeless globes,
mere reflectors of useless sunshine.

The case of the moon is, in this respect, especially interesting, on
account of the change that has occurred in the opinions held concerning
its physical condition. For a very long time our satellite was
confidently, and almost universally, regarded as an airless, waterless,
lifeless desert, a completely "dead world," a bare, desiccated skull of
rock, circling about the living earth.

But within a few years there has been a reaction from this extreme view
of the lifelessness of the moon. Observers tell us of clouds suddenly
appearing and then melting to invisibility over volcanic craters; of
evidences of an atmosphere, rare as compared with ours, yet manifest in
its effects; of variations of color witnessed in certain places as the
sunlight drifts over them at changing angles of incidence; of what seem
to be immense fields of vegetation covering level ground, and of
appearances indicating the existence of clouds of ice crystals and
deposits of snow among the mountainous lunar landscapes. Thus, in a
manner, the moon is rehabilitated, and we are invited to regard its
silvery beams not as the reflections of the surface of a desert, but as
sent back to our eyes from the face of a world that yet has some slight
remnants of life to brighten it.

The suggestion that there is an atmosphere lying close upon the shell of
the lunar globe, filling the deep cavities that pit its face and
penetrating to an unknown depth in its interior, recalls a speculation
of the ingenious and entertaining Fontenelle, in the seventeenth
century--recently revived and enlarged upon by the author of one of our
modern romances of adventure in the moon--to the effect that the lunar
inhabitants dwell beneath the surface of their globe instead of on the
top of it.

Now, because of this widespread and continually increasing interest in
the subject of other worlds, and on account of the many curious
revelations that we owe to modern telescopes and other improved means of
investigation, it is certainly to be desired that the most important and
interesting discoveries that have lately been made concerning the
various globes which together with the earth constitute the sun's
family, should be assembled in a convenient and popular form--and that
is the object of this book. Fact is admittedly often stranger and more
wonderful than fiction, and there are no facts that appeal more
powerfully to the imagination than do those of astronomy. Technical
books on astronomy usually either ignore the subject of the habitability
of the planets, or dismiss it with scarcely any recognition of the
overpowering human interest that it possesses. Hence, a book written
specially from the point of view of that subject would appear calculated
to meet a popular want; and this the more, because, since Mr. Proctor
wrote his Other Worlds than Ours and M. Flammarion his Pluralité des
Mondes Habités, many most important and significant discoveries have
been made that, in several notable instances, have completely altered
the aspect in which the planets present themselves for our judgment as
to their conditions of habitability.

No doubt the natural tendency of the mind is to regard all the planets
as habitable worlds, for there seems to be deeply implanted in human
nature a consciousness of the universality of life, giving rise to a
conviction that one world, even in the material sense, is not enough for
it, but that every planet must belong to its kingdom. We are apt to say
to ourselves: "The earth is one of a number of planets, all similarly
circumstanced; the earth is inhabited, why should not the others also be
inhabited?"

What has been learned of the unity in chemical constitution and
mechanical operation prevailing throughout the solar system, together
with the continually accumulating evidence of the common origin of its
various members, and the identity of the evolutionary processes that
have brought them into being, all tends to strengthen the _a priori_
hypothesis that life is a phenomenon general to the entire system, and
only absent where its essential and fundamental conditions, for special
and local, and perhaps temporary, reasons, do not exist.

If we look for life in the sun, for instance, while accepting the
prevalent conception of the sun as a center of intense thermal action,
we must abandon all our ideas of the physical organization of life
formed upon what we know of it from experimental evidence. We can not
imagine any form of life that has ever been presented to our senses as
existing in the sun.

But this is not generally true of the planets. Life, in our sense of it,
is a planetary, not a solar, phenomenon, and while we may find reasons
for believing that on some of the planets the conditions are such that
creatures organized like ourselves could not survive, yet we can not
positively say that every form of living organism must necessarily be
excluded from a world whose environment would be unsuited for us and our
contemporaries in terrestrial life.

Although our sole knowledge of animated nature is confined to what we
learn by experience on the earth, yet it is a most entertaining, and by
no means unedifying, occupation, to seek to apply to the exceedingly
diversified conditions prevailing in the other planets, as astronomical
observations reveal them to us, the principles, types, and limitations
that govern the living creatures of our world, and to judge, as best we
can, how far those types and limits may be modified or extended so that
those other planets may reasonably be included among the probable abodes
of life.

In order to form such judgments each planet must be examined by itself,
but first it is desirable to glance at the planetary system as a whole.
To do this we may throw off, in imagination, the dominance of the sun,
and suppose ourselves to be in the midst of open space, far removed both
from the sun and the other stars. In this situation it is only by
chance, or through foreknowledge, that we can distinguish our sun at
all, for it is lost among the stars; and when we discover it we find
that it is only one of the smaller and less conspicuous members of the
sparkling host.

We rapidly approach, and when we have arrived within a distance
comparable with that of its planets, we see that the sun has increased
in apparent magnitude, until now it enormously outshines all the other
stars, and its rays begin to produce the effect of daylight upon the
orbs that they reach. But we are in no danger of mistaking its apparent
superiority to its fellow stars for a real one, because we clearly
perceive that our nearness alone makes it seem so great and
overpowering.

And now we observe that this star that we have drawn near to has
attending it a number of minute satellites, faintly shining specks, that
circle about it as if charmed, like night-wandering insects, by its
splendor. It is manifest to us at the first glance that without the sun
these obedient little planets would not exist; it is his attraction that
binds them together in a system, and his rays that make them visible to
one another in the abyss of space. Although they vary in relative size,
yet we observe a striking similarity among them. They are all globular
bodies, they all turn upon their axes, they all travel about the sun in
the same direction, and their paths all lie very nearly in one plane.
Some of them have one or more moons, or satellites, circling about them
in imitation of their own revolution about the sun. Their family
relationship to one another and to the sun is so evident that it colors
our judgment about them as individuals; and when we happen to find, upon
closer approach, that one of them, the earth, is covered with vegetation
and water and filled with thousands of species of animated creatures, we
are disposed to believe, without further examination, that they are all
alike in this respect, just as they are all alike in receiving light and
heat from the sun.

This preliminary judgment, arising from the evident unity of the
planetary system, can only be varied by an examination of its members in
detail.

One striking fact that commands our attention as soon as we have entered
the narrow precincts of the solar system is the isolation of the sun and
its attendants in space. The solar system occupies a disk-shaped, or
flat circular, expanse, about 5,580,000,000 miles across and relatively
very thin, the sun being in the center. From the sun to the nearest
star, or other sun, the distance is approximately five thousand times
the entire diameter of the solar system. But the vast majority of the
stars are probably a hundred times yet more remote. In other words, if
the Solar system be represented by a circular flower-bed ten feet
across, the nearest star must be placed at a distance of nine and a half
miles, and the great multitude of the stars at a distance of nine
hundred miles!

Or, to put it in another way, let us suppose the sun and his planets to
be represented by a fleet of ships at sea, all included within a space
about half a mile across; then, in order that there might be no shore
relatively nearer than the nearest fixed star is to the sun, we should
have to place our fleet in the middle of the Pacific Ocean, while the
distance of the main shore of the starry universe would be so immense
that the whole surface of the earth would be far too small to hold the
expanse of ocean needed to represent it!

From these general considerations we next proceed to recall some of the
details of the system of worlds amid which we dwell. Besides the earth,
the sun has seven other principal planets in attendance. These eight
planets fall into two classes--the terrestrial planets and the major, or
jovian, planets. The former class comprises Mercury, Venus, the earth,
and Mars, and the latter Jupiter, Saturn, Uranus, and Neptune. I have
named them all in the order of their distance from the sun, beginning
with the nearest.

The terrestrial planets, taking their class name from _terra_, the
earth, are relatively close to the sun and comparatively small. The
major planets--or the jovian planets, if we give them a common title
based upon the name of their chief, Jupiter or Jove--are relatively
distant from the sun and are characterized both by great comparative
size and slight mean density. The terrestrial planets are all included
within a circle, having the sun for a center, about 140,000,000 miles
in radius. The space, or gap, between the outermost of them, Mars, and
the innermost of the jovian planets, Jupiter, is nearly two and a half
times as broad as the entire radius of the circle within which they are
included. And not only is the jovian group of planets widely separated
from the terrestrial group, but the distances between the orbits of its
four members are likewise very great and progressively increasing.
Between Jupiter and Saturn is a gap 400,000,000 miles across, and this
becomes 900,000,000 miles between Saturn and Uranus, and more than
1,000,000,000 miles between Uranus and Neptune. All of these distances
are given in round numbers.

Finally, we come to some very extraordinary worlds--if we can call them
worlds at all--the asteroids. They form a third group, characterized by
the extreme smallness of its individual members, their astonishing
number, and the unusual eccentricities and inclinations of their orbits.
They are situated in the gap between the terrestrial and the jovian
planets, and about 500 of them have been discovered, while there is
reason to think that their real number may be many thousands. The
largest of them is less than 500 miles in diameter, and many of those
recently discovered may be not more than ten or twenty miles in
diameter. What marvelous places of abode such little planets would be if
it were possible to believe them inhabited, we shall see more clearly
when we come to consider them in their turn. But without regard to the
question of habitability, the asteroids will be found extremely
interesting.

In the next chapter we proceed to take up the planets for study as
individuals, beginning with Mercury, the one nearest the sun.




CHAPTER II

MERCURY, A WORLD OF TWO FACES AND MANY CONTRASTS


Mercury, the first of the other worlds that we are going to consider,
fascinates by its grotesqueness, like a piece of Chinese ivory carving,
so small is it for its kind and so finished in its eccentric details. In
a little while we shall see how singular Mercury is in many of the
particulars of planetary existence, but first of all let us endeavor to
obtain a clear idea of the actual size and mass of this strange little
planet. Compared with the earth it is so diminutive that it looks as if
it had been cut out on the pattern of a satellite rather than that of an
independent planet. Its diameter, 3,000 miles, only exceeds the moon's
by less than one half, while both Jupiter and Saturn, among their
remarkable collections of moons, have each at least one that is
considerably larger than the planet Mercury. But, insignificant though
it be in size, it holds the place of honor, nearest to the sun.

It was formerly thought that Mercury possessed a mass greatly in excess
of that which its size would seem to imply, and some estimates, based
upon the apparent effect of its attraction on comets, made it equal in
mean density to lead, or even to the metal mercury. This led to curious
speculations concerning its probable metallic composition, and the
possible existence of vast quantities of such heavy elements as gold in
the frame of the planet. But more recent, and probably more correct,
computations place Mercury third in the order of density among the
members of the solar system, the earth ranking as first and Venus as
second. Mercury's density is now believed to be less than the earth's in
the ratio of 85 to 100. Accepting this estimate, we find that the force
of gravity upon the surface of Mercury is only one third as great as
upon the surface of the earth--i.e., a body weighing 300 pounds on the
earth would weigh only 100 pounds on Mercury.

This is an important matter, because not only the weight of bodies, but
the density of the atmosphere and even the nature of its gaseous
constituents, are affected by the force of gravity, and if we could
journey from world to world, in our bodily form, it would make a great
difference to us to find gravity considerably greater or less upon other
planets than it is upon our own. This alone might suffice to render some
of the planets impossible places of abode for us, unless a decided
change were effected in our present physical organization.

One of the first questions that we should ask about a foreign world to
which we proposed to pay a visit, would relate to its atmosphere. We
should wish to know in advance if it had air and water, and in what
proportions and quantities. However its own peculiar inhabitants might
be supposed able to dispense with these things, to _us_ their presence
would be essential, and if we did not find them, even a planet that
blazed with gold and diamonds only waiting to be seized would remain
perfectly safe from our invasion. Now, in the case of Mercury, some
doubt on this point exists.

Messrs. Huggins, Vogel, and others have believed that they found
spectroscopic proof of the existence of both air and the vapor of water
on Mercury. But the necessary observations are of a very delicate
nature, and difficult to make, and some astronomers doubt whether we
possess sufficient proof that Mercury has an atmosphere. At any rate,
its atmosphere is very rare as compared with the earth's, but we need
not, on that account, conclude that Mercury is lifeless. Possibly, in
view of certain other peculiarities soon to be explained, a rare
atmosphere would be decidedly advantageous.

Being much nearer the sun than the earth is, Mercury can be seen by us
only in the same quarter of the sky where the sun itself appears. As it
revolves in its orbit about the sun it is visible, alternately, in the
evening for a short time after sunset and in the morning for a short
time before sunrise, but it can never be seen, as the outer planets are
seen, in the mid-heaven or late at night. When seen low in the twilight,
at evening or morning, it glows with the brilliance of a bright
first-magnitude star, and is a beautiful object, though few casual
watchers of the stars ever catch sight of it. When it is nearest the
earth and is about to pass between the earth and the sun, it temporarily
disappears in the glare of the sunlight; and likewise, when it it is
farthest from the earth and passing around in its orbit on the opposite
side of the sun, it is concealed by the blinding solar rays.
Consequently, except with the instruments of an observatory, which are
able to show it in broad day, Mercury is never visible save during the
comparatively brief periods of time when it is near its greatest
apparent distance east or west from the sun.

The nearer a planet is to the sun the more rapidly it is compelled to
move in its orbit, and Mercury, being the nearest to the sun of all the
planets, is by far the swiftest footed among them. But its velocity is
subject to remarkable variation, owing to the peculiar form of the orbit
in which the planet travels. This is more eccentric than the orbit of
any other planet, except some of the asteroids. The sun being situated
in one focus of the elliptical orbit, when Mercury is at perihelion, or
nearest to the sun, its distance from that body is 28,500,000 miles, but
when it is at aphelion, or farthest from the sun, its distance is
43,500,000 miles. The difference is no less than 14,000,000 miles! When
nearest the sun Mercury darts forward in its orbit at the rate of
twenty-nine miles in a second, while when farthest from the sun the
speed is reduced to twenty-three miles.

Now, let us return for a moment to the consideration of the wonderful
variations in Mercury's distance from the sun, for we shall find that
their effects are absolutely startling, and that they alone suffice to
mark a wide difference between Mercury and the earth, considered as the
abodes of sentient creatures. The total change of distance amounts, as
already remarked, to 14,000,000 miles, which is almost half the entire
distance separating the planet from the sun at perihelion. This immense
variation of distance is emphasized by the rapidity with which it takes
place. Mercury's periodic time, i.e., the period required for it to make
a single revolution about the sun--or, in other words, the length of its
year--is eighty-eight of our days. In just one half of that time, or in
about six weeks, it passes from aphelion to perihelion; that is to say,
in six weeks the whole change in its distance from the sun takes place.
In six weeks Mercury falls 14,000,000 miles--for it _is_ a fall, though
in a curve instead of a straight line--falls 14,000,000 miles toward the
sun! And, as it falls, like any other falling body it gains in speed,
until, having reached the perihelion point, its terrific velocity
counteracts its approach and it begins to recede. At the end of the next
six weeks it once more attains its greatest distance, and turns again to
plunge sunward.

Of course it may be said of every planet having an elliptical orbit
that between aphelion and perihelion it is falling toward the sun, but
no other planet than Mercury travels in an orbit sufficiently eccentric,
and approaches sufficiently near to the sun, to give to the mind so
vivid an impression of an actual, stupendous fall!

Next let us consider the effects of this rapid fall, or approach, toward
the sun, which is so foreign to our terrestrial experience, and so
appalling to the imagination.

First, we must remember that the nearer a planet is to the sun the
greater is the amount of heat and light that it receives, the variation
being proportional to the inverse square of the distance. The earth's
distance from the sun being 93,000,000 miles, while Mercury's is only
36,000,000, it follows, to begin with, that Mercury gets, on the
average, more than six and a half times as much heat from the sun as the
earth does. That alone is enough to make it seem impossible that Mercury
can be the home of living forms resembling those of the earth, for
imagine the heat of the sun in the middle of a summer's day increased
six or seven fold! If there were no mitigating influences, the face of
the earth would shrivel as in the blast of a furnace, the very stones
would become incandescent, and the oceans would turn into steam.

Still, notwithstanding the tremendous heat poured upon Mercury as
compared with that which our planet receives, we can possibly, and for
the sake of a clearer understanding of the effects of the varying
distance, which is the object of our present inquiry, find a loophole to
admit the chance that yet there may be living beings there. We might,
for instance, suppose that, owing to the rarity of its atmosphere, the
excessive heat was quickly radiated away, or that there was something in
the constitution of the atmosphere that greatly modified the effective
temperature of the sun's rays. But, having satisfied our imagination on
this point, and placed our supposititious inhabitants in the hot world
of Mercury, how are we going to meet the conditions imposed by the
rapid changes of distance--the swift fall of the planet toward the sun,
followed by the equally swift rush away from it? For change of distance
implies change of heat and temperature.

It is true that we have a slight effect of this kind on the earth.
Between midsummer (of the northern hemisphere) and midwinter our planet
draws 3,000,000 miles nearer the sun, but the change occupies six
months, and, at the earth's great average distance, the effect of this
change is too slight to be ordinarily observable, and only the
astronomer is aware of the consequent increase in the apparent size of
the sun. It is not to this variation of the sun's distance, but rather
to the changes of the seasons, depending on the inclination of the
earth's axis, that we owe the differences of temperature that we
experience. In other words, the total supply of heat from the sun is not
far from uniform at all times of the year, and the variations of
temperature depend upon the distribution of that supply between the
northern and southern hemispheres, which are alternately inclined
sunward.

But on Mercury the supply of solar heat is itself variable to an
enormous extent. In six weeks, as we have seen, Mercury diminishes its
distance from the sun about one third, which is proportionally ten times
as great a change of distance as the earth experiences in six months.
The inhabitants of Mercury in those six pregnant weeks see the sun
expand in the sky to more than two and a half times its former
magnitude, while the solar heat poured upon them swiftly augments from
something more than four and a half times to above eleven times the
amount received upon the earth! Then, immediately, the retreat of the
planet begins, the sun visibly shrinks, as a receding balloon becomes
smaller in the eyes of its watchers, the heat falls off as rapidly as it
had previously increased, until, the aphelion point being reached, the
process is again reversed. And thus it goes on unceasingly, the sun
growing and diminishing in the sky, and the heat increasing and
decreasing by enormous amounts with astonishing rapidity. It is
difficult to imagine any way in which atmospheric influences could
equalize the effects of such violent changes, or any adjustments in the
physical organization of living beings that could make such changes
endurable.

But we have only just begun the story of Mercury's peculiarities. We
come next to an even more remarkable contrast between that planet and
our own. During the Paris Exposition of 1889 a little company of
astronomers was assembled at the Juvisy observatory of M. Flammarion,
near the French capital, listening to one of the most surprising
disclosures of a secret of nature that any _savant_ ever confided to a
few trustworthy friends while awaiting a suitable time to make it
public. It was a secret as full of significance as that which Galileo
concealed for a time in his celebrated anagram, which, when at length he
furnished the key, still remained a riddle, for then it read: "The
Mother of the Loves imitates the Shapes of Cynthia," meaning that the
planet Venus, when viewed with a telescope, shows phases like those of
the moon. The secret imparted in confidence to the knot of astronomers
at Juvisy came from a countryman of Galileo's, Signor G. V.
Schiaparelli, the Director of the Observatory of Milan, and its purport
was that the planet Mercury always keeps the same face directed toward
the sun. Schiaparelli had satisfied himself, by a careful series of
observations, of the truth of his strange announcement, but before
giving it to the world he determined to make doubly sure. Early in 1890
he withdrew the pledge of secrecy from his friends and published his
discovery.

No one can wonder that the statement was generally received with
incredulity, for it was in direct contradiction to the conclusions of
other astronomers, who had long believed that Mercury rotated on its
axis in a period closely corresponding with that of the earth's
rotation--that is to say, once every twenty-four hours. Schiaparelli's
discovery, if it were received as correct, would put Mercury, as a
planet, in a class by itself, and would distinguish it by a peculiarity
which had always been recognized as a special feature of the moon, viz.,
that of rotating on its axis in the same period of time required to
perform a revolution in its orbit, and, while this seemed natural enough
for a satellite, almost nobody was prepared for the ascription of such
eccentric conduct to a planet.

The Italian astronomer based his discovery upon the observation that
certain markings visible on the disk of Mercury remained in such a
position with reference to the direction of the sun as to prove that the
planet's rotation was extremely slow, and he finally satisfied himself
that there was but one rotation in the course of a revolution about the
sun. That, of course, means that one side of Mercury always faces toward
the sun while the opposite side always faces away from it, and neither
side experiences the alternation of day and night, one having perpetual
day and the other perpetual night. The older observations, from which
had been deduced the long accepted opinion that Mercury rotated, like
the earth, once in about twenty-four hours, had also been made upon the
markings on the planet's disk, but these are not easily seen, and their
appearances had evidently been misinterpreted.

The very fact of the difficulty of seeing any details on Mercury tended
to prevent or delay corroboration of Schiaparelli's discovery. But there
were two circumstances that contributed to the final acceptance of his
results. One of these was his well-known experience as an observer and
the high reputation that he enjoyed among astronomers, and the other was
the development by Prof. George Darwin of the theory of tidal friction
in its application to planetary evolution, for this furnished a
satisfactory explanation of the manner in which a body, situated as near
the sun as Mercury is, could have its axial rotation gradually reduced
by the tidal attraction of the sun until it coincided in period with its
orbital revolution.

Accepting the accuracy of Schiaparelli's discovery, which was
corroborated in every particular in 1896 by Percival Lowell in a special
series of observations on Mercury made with his 24-inch telescope at
Flagstaff, Arizona, and which has also been corroborated by others, we
see at once how important is its bearing on the habitability of the
planet. It adds another difficulty to that offered by the remarkable
changes of distance from the sun, and consequent variations of heat,
which we have already discussed. In order to bring the situation home to
our experience, let us, for a moment, imagine the earth fallen into
Mercury's dilemma. There would then be no succession of day and night,
such as we at present enjoy, and upon which not alone our comfort but
perhaps our very existence depends, but, instead, one side of our
globe--it might be the Asiatic or the American half--would be
continually in the sunlight, and the other side would lie buried in
endless night. And this condition, so suggestive of the play of pure
imagination, this plight of being a two-faced world, like the god
Janus, one face light and the other face dark, must be the actual state
of things on Mercury.

There is one interesting qualification. In the case just imagined for
the earth, supposing it to retain the present inclination of its axis
while parting with its differential rotation, there would be an
interchange of day and night once a year in the polar regions. On
Mercury, whose axis appears to be perpendicular, a similar phenomenon,
affecting not the polar regions but the eastern and western sides of the
planet, is produced by the extraordinary eccentricity of its orbit. As
the planet alternately approaches and recedes from the sun its orbital
velocity, as we have already remarked, varies between the limits of
twenty-three and thirty-five miles per second, being most rapid at the
point nearest the sun. But this variation in the speed of its revolution
about the sun does not, in any manner, affect the rate of rotation on
its axis. The latter is perfectly uniform and just fast enough to
complete one axial turn in the course of a single revolution about the
sun. The accompanying figure may assist the explanation.

[Illustration: DIAGRAM SHOWING THAT, OWING TO THE ECCENTRICITY OF ITS
ORBIT, AND ITS VARYING VELOCITY, MERCURY, ALTHOUGH MAKING BUT ONE TURN
ON ITS AXIS IN THE COURSE OF A REVOLUTION ABOUT THE SUN, NEVERTHELESS
EXPERIENCES ON PARTS OF ITS SURFACE THE ALTERNATION OF DAY AND NIGHT.]

Let us start with Mercury in perihelion at the point _A_. The little
cross on the planet stands exactly under the sun and in the center of
the illuminated hemisphere. The large arrows show the direction in which
the planet travels in its revolution about the sun, and the small curved
arrows the direction in which it rotates on its axis. Now, in moving
along its orbit from _A_ to _B_ the planet, partly because of its
swifter motion when near the sun, and partly because of the elliptical
nature of the orbit, traverses a greater angular interval with reference
to the sun than the cross, moving with the uniform rotation of the
planet on its axis, is able to traverse in the same time. As drawn in
the diagram, the cross has moved through exactly ninety degrees, or one
right angle, while the planet in its orbit has moved through
considerably more than a right angle. In consequence of this gain of the
angle of revolution upon the angle of rotation, the cross at _B_ is no
longer exactly under the sun, nor in the center of the illuminated
hemisphere. It appears to have shifted its position toward the west,
while the hemispherical cap of sunshine has slipped eastward over the
globe of the planet.

In the next following section of the orbit the planet rotates through
another right angle, but, owing to increased distance from the sun, the
motion in the orbit now becomes slower until, when the planet arrives at
aphelion, _C_, the angular difference disappears and the cross is once
more just under the sun. On returning from aphelion to perihelion the
same phenomena recur in reverse order and the line between day and night
on the planet first shifts westward, attaining its limit in that respect
at _D_, and then, at perihelion, returns to its original position.

Now, if we could stand on the sunward hemisphere of Mercury what, to our
eyes, would be the effect of this shifting of the sun's position with
regard to a fixed point on the planet's surface? Manifestly it would
cause the sun to describe a great arc in the sky, swinging to and fro,
in an east and west line, like a pendulum bob, the angular extent of the
swing being a little more than forty-seven degrees, and the time
required for the sun to pass from its extreme eastern to its extreme
western position and back again being eighty-eight days. But, owing to
the eccentricity of the orbit, the sun swings much faster toward the
east than toward the west, the eastward motion occupying about
thirty-seven days and the westward motion about fifty-one days.

[Illustration: THE REGIONS OF PERPETUAL DAY, PERPETUAL NIGHT, AND
ALTERNATE DAY AND NIGHT ON MERCURY. IN THE LEFT-HAND VIEW THE OBSERVER
LOOKS AT THE PLANET IN THE PLANE OF ITS EQUATOR; IN THE RIGHT-HAND VIEW
HE LOOKS DOWN ON ITS NORTH POLE.]

Another effect of the libratory motion of the sun as seen from Mercury
is represented in the next figure, where we have a view of the planet
showing both the day and the night hemisphere, and where we see that
between the two there is a region upon which the sun rises and sets once
every eighty-eight days. There are, in reality, two of these lune-shaped
regions, one at the east and the other at the west, each between 1,200
and 1,300 miles broad at the equator. At the sunward edge of these
regions, once in eighty-eight days, or once in a Mercurial year, the sun
rises to an elevation of forty-seven degrees, and then descends again
straight to the horizon from which it rose; at the nightward edge, once
in eighty-eight days, the sun peeps above the horizon and quickly sinks
from sight again. The result is that, neglecting the effects of
atmospheric refraction, which would tend to expand the borders of the
domain of sunlight, about one quarter of the entire surface of Mercury
is, with regard to day and night, in a condition resembling that of our
polar regions, where there is but one day and one night in the course of
a year--and on Mercury a year is eighty-eight days. One half of the
remaining three quarters of the planet's surface is bathed in perpetual
sunshine and the other half is a region of eternal night.

And now again, what of life in such a world as that? On the night side,
where no sunshine ever penetrates, the temperature must be extremely
low, hardly greater than the fearful cold of open space, unless
modifying influences beyond our ken exist. It is certain that if life
flourishes there, it must be in such forms as can endure continual
darkness and excessive cold. Some heat would be carried around by
atmospheric circulation from the sunward side, but not enough, it would
seem, to keep water from being perpetually frozen, or the ground from
being baked with unrelaxing frost. It is for the imagination to picture
underground dwellings, artificial sources of heat, and living forms
suited to unearthlike environment.

What would be the mental effects of perpetual night upon a race of
intelligent creatures doomed to that condition? Perhaps not quite so
grievous as we are apt to think. The constellations in all their
splendor would circle before their eyes with the revolution of their
planet about the sun, and with the exception of the sun itself--which
they could see by making a journey to the opposite hemisphere--all the
members of the solar system would pass in succession through their
mid-heaven, and two of them would present themselves with a magnificence
of planetary display unknown on the earth. Venus, when in opposition
under the most favorable circumstances, is scarcely more than 24,000,000
miles from Mercury, and, showing herself at such times with a fully
illuminated disk--as, owing to her position within the orbit of the
earth, she never can do when at her least distance from us--she must be
a phenomenon of unparalleled beauty, at least four times brighter than
we ever see her, and capable, of course, of casting a strong shadow.

The earth, also, is a splendid star in the midnight sky of Mercury, and
the moon may be visible to the naked eye as a little attendant circling
about its brilliant master. The outer planets are slightly less
conspicuous than they are to us, owing to increase of distance.

The revolution of the heavens as seen from the night side of Mercury is
quite different in period from that which we are accustomed to, although
the apparent motion is in the same direction, viz., from east to west.
The same constellations remain above the horizon for weeks at a time,
slowly moving westward, with the planets drifting yet more slowly, but
at different rates, among them; the nearer planets, Venus and the earth,
showing the most decided tendency to loiter behind the stars.

On the side where eternal sunlight shines the sky of Mercury contains no
stars. Forever the pitiless blaze of day; forever,

    "All in a hot and copper sky
    The bloody sun at noon."

As it is difficult to understand how water can exist on the night
hemisphere, except in the shape of perpetual snow and ice, so it is
hard to imagine that on the day hemisphere water can ever be
precipitated from the vaporous form. In truth, there can be very little
water on Mercury even in the form of vapor, else the spectroscope would
have given unquestionable evidence of its presence. Those who think that
Mercury is entirely waterless and almost, if not quite, airless may be
right. In these respects it would then resemble the moon, and, according
to some observers, it possesses another characteristic lunar feature in
the roughening of its surface by what seem to be innumerable volcanic
craters.

But if we suppose Mercury to possess an atmosphere much rarer than that
of the earth, we may perceive therein a possible provision against the
excessive solar heat to which it is subjected, since, as we see on high
mountains, a light air permits a ready radiation of heat, which does not
become stored up as in a denser atmosphere.

As the sun pours its heat without cessation upon the day hemisphere the
warmed air must rise and flow off on all sides into the night
hemisphere, while cold air rushes in below, to take its place, from the
region of frost and darkness. The intermediate areas, which see the sun
part of the time, as explained above, are perhaps the scene of
contending winds and tempests, where the moisture, if there be any, is
precipitated, through the rapid cooling of the air, in whelming floods
and wild snow-storms driven by hurrying blasts from the realm of endless
night.

Enough seems now to have been said to indicate clearly the hopelessness
of looking for any analogies between Mercury and the earth which would
warrant the conclusion that the former planet is capable of supporting
inhabitants or forms of life resembling those that swarm upon the
latter. If we would still believe that Mercury is a habitable globe we
must depend entirely upon the imagination for pictures of creatures able
to endure its extremes of heat and cold, of light and darkness, of
instability, swift vicissitude, and violent contrast.

In the next chapter we shall study a more peaceful and even-going world,
yet one of great brilliancy, which possesses some remarkable
resemblances to the earth, as well as some surprising divergences from
it.




CHAPTER III

VENUS, THE TWIN OF THE EARTH


We come now to a planet which seems, at the first glance, to afford a
far more promising outlook than Mercury does for the presence of organic
life forms bearing some resemblance to those of the earth. One of the
strongest arguments for regarding Venus as a world much like ours is
based upon its remarkable similarity to the earth in size and mass,
because thus we are assured that the force of gravity is practically the
same upon the two planets, and the force of gravity governs numberless
physical phenomena of essential importance to both animal and vegetable
life. The mean diameter of the earth is 7,918 miles; that of Venus is
7,700 miles. The difference is so slight that if the two planets were
suspended side by side in the sky, at such a distance that their disks
resembled that of the full moon, the eye would notice no inequality
between them.

The mean density of Venus is about nine tenths of that of the earth, and
the force of gravity upon its surface is in the ratio of about 85 to 100
as compared to its force on the surface of the earth. A man removed to
Venus would, consequently, find himself perceptibly lighter than he was
at home, and would be able to exert his strength with considerably
greater effect than on his own planet. But the difference would amount
only to an agreeable variation from accustomed conditions, and would not
be productive of fundamental changes in the order of nature.

Being, like Mercury, nearer to the sun than the earth is, Venus also is
visible to us only in the morning or the evening sky. But her distance
from the sun, slightly exceeding 67,000,000 miles, is nearly double that
of Mercury, so that, when favorably situated, she becomes a very
conspicuous object, and, instead of being known almost exclusively by
astronomers, she is, perhaps, the most popular and most admired of all
the members of the planetary system, especially when she appears in the
charming rôle of the "evening star." As she emerges periodically from
the blinding glare of the sun's immediate neighborhood and begins to
soar, bright as an electric balloon, in the twilight, she commands all
eyes and calls forth exclamations of astonishment and admiration by her
singular beauty. The intervals between her successive reappearances in
the evening sky, measured by her synodic period of 584 days, are
sufficiently long to give an element of surprise and novelty to every
return of so dazzling a phenomenon.

Even the light of the full moon silvering the tree tops does not
exercise greater enchantment over the mind of the contemplative
observer. In either of her rôles, as morning or as evening star, Venus
has no rival. No fixed star can for an instant bear comparison with her.
What she lacks in vivacity of light--none of the planets twinkles, as do
all of the true stars--is more than compensated by the imposing size of
her gleaming disk and the striking beauty of her clear lamplike rays.
Her color is silvery or golden, according to the state of the
atmosphere, while the distinction of her appearance in a dark sky is so
great that no eye can resist its attraction, and I have known an
unexpected glimpse of Venus to put an end to an animated conversation
and distract, for a long time, the attention of a party of ladies and
gentlemen from the social occupation that had brought them together.

As a telescopic object Venus is exceedingly attractive, even when
considered merely from the point of view of simple beauty. Both Mercury
and Venus, as they travel about the sun, exhibit phases like those of
the moon, but Venus, being much larger and much nearer to the earth than
Mercury, shows her successive phases more effectively, and when she
shines as a thin crescent in the morning or evening twilight, only a
very slight magnifying power is required to show the sickle form of her
disk.

A remarkable difference between Venus and Mercury comes out as soon as
we examine the shape of the former's orbit. Venus's mean distance from
the sun is 67,200,000 miles, and her orbit is so nearly a circle, much
more nearly than that of any other planet, that in the course of a
revolution her distance from the sun varies less than a million miles.
The distance of the earth varies 3,000,000 miles, and that of Mercury
14,000,000. Her period of revolution, or the length of her year, is 225
of our days. When she comes between the sun and the earth she approaches
us nearer than any other planet ever gets, except the asteroid Eros, her
distance at such times being 26,000,000 miles, or about one hundred and
ten times the distance of the moon.

Being nearer to the sun in the ratio of 67 to 93, Venus receives almost
twice as much solar light and heat as we get, but less than one third as
much as Mercury gets. There is reason to believe that her axis, instead
of being considerably inclined, like that of the earth, is perpendicular
to the plane of her orbit. Thus Venus introduces to us another novelty
in the economy of worlds, for with a perpendicular axis of rotation she
can have no succession of seasons, no winter and summer flitting, one
upon the other's heels, to and fro between the northern and southern
hemispheres; but, on the contrary, her climatic conditions must be
unchangeable, and, on any particular part of her surface, except for
local causes of variation, the weather remains the same the year around.
So, as far as temperature is concerned, Venus may have two regions of
perpetual winter, one around each pole; two belts of perpetual spring in
the upper middle latitudes, one on each side of the equator; and one
zone of perpetual summer occupying the equatorial portion of the planet.
But, of course, these seasonal terms do not strictly apply to Venus, in
the sense in which we employ them on the earth, for with us spring is
characterized rather by the change in the quantity of heat and other
atmospheric conditions that it witnesses than by a certain fixed and
invariable temperature.

To some minds it may appear very undesirable, from the point of view of
animate existences, that there should be no alternation of seasons on
the surface of a planet, but, instead, fixed conditions of climate; yet
it is not clear that such a state of affairs might not be preferable to
that with which we are familiar. Even on the earth, we find that
tropical regions, where the seasonal changes are comparatively moderate,
present many attractions and advantages in contrast with the violent and
often destructive vicissitudes of the temperate zones, and nature has
shown us, within the pale of our own planet, that she is capable of
bringing forth harvests of fruit and grain without the stimulus of
alternate frost and sunshine.

Even under the reign of perpetual summer the fields and trees find time
and opportunity to rest and restore their productive forces.

The circularity of Venus's orbit, and the consequently insignificant
change in the sun's distance and heating effect, are other elements to
be considered in estimating the singular constancy in the operation of
natural agencies upon that interesting planet, which, twin of the earth
though it be in stature, is evidently not its twin in temperament.

And next as to the all-important question of atmosphere. In what
precedes, the presence of an atmosphere has been assumed, and,
fortunately, there is very convincing evidence, both visual and
spectroscopic, that Venus is well and abundantly supplied with air, by
which it is not meant that Venus's air is precisely like the mixture of
oxygen and nitrogen, with a few other gases, which we breathe and call
by that name. In fact, there are excellent reasons for thinking that the
atmosphere of Venus differs from the earth's quite as much as some of
her other characteristics differ from those of our planet. But, however
it may vary from ours in constitution, the atmosphere of Venus contains
water vapor, and is exceedingly abundant. Listen to Professor Young:

"Its [Venus's] atmosphere is probably from one and a half to two times
as extensive and as dense as our own, and the spectroscope shows
evidence of the presence of water vapor in it."

And Prof. William C. Pickering, basing his statement on the result of
observations at the mountain observatory of Arequipa, says: "We may feel
reasonably certain that at the planet's [Venus's] surface the density of
its atmosphere is many times that of our own."

We do not have to depend upon the spectroscope for evidence that Venus
has a dense atmosphere, for we can, in a manner, _see_ her atmosphere,
in consequence of its refractive action upon the sunlight that strikes
into it near the edge of the planet's globe. This illumination of
Venus's atmosphere is witnessed both when she is nearly between the sun
and the earth, and when, being exactly between them, she appears in
silhouette against the solar disk. During a transit of this kind, in
1882, many observers, and the present writer was one, saw a bright
atmospheric bow edging a part of the circumference of Venus when the
planet was moving upon the face of the sun--a most beautiful and
impressive spectacle.

Even more curious is an observation made in 1866 by Prof. C.S. Lyman, of
Yale College, who, when Venus was very near the sun, saw her atmosphere
_in the form of a luminous ring_. A little fuller explanation of this
appearance may be of interest.

When approaching inferior conjunction--i.e., passing between the earth
and sun--Venus appears, with a telescope, in the shape of a very thin
crescent. Professor Lyman watched this crescent, becoming narrower day
after day as it approached the sun, and noticed that its extremities
gradually extended themselves beyond the limits of a semicircle, bending
to meet one another on the opposite side of the invisible disk of the
planet, until, at length, they did meet, and he beheld a complete ring
of silvery light, all that remained visible of the planet Venus! The
ring was, of course, the illuminated atmosphere of the planet refracting
the sunlight on all sides around the opaque globe.

In 1874 M. Flammarion witnessed the same phenomenon in similar
circumstances. One may well envy those who have had the good fortune to
behold this spectacle--to actually see, as it were, the air that the
inhabitants of another world are breathing and making resonant with all
the multitudinous sounds and voices that accompany intelligent life. But
perhaps some readers will prefer to think that even though an atmosphere
is there, there is no one to breathe it.

[Illustration: VENUS'S ATMOSPHERE SEEN AS A RING OF LIGHT.]

As the visibility of Venus's atmosphere is unparalleled elsewhere in the
solar system, it may be worth while to give a graphic illustration of
it. In the accompanying figure the planet is represented at three
successive points in its advance toward inferior conjunction. As it
approaches conjunction it slowly draws nearer the earth, and its
apparent diameter consequently increases. At _A_ a large part of the
luminous crescent is composed of the planet's surface reflecting the
sunshine; at _B_ the ratio of the reflecting surface to the illuminated
atmosphere has diminished, and the latter has extended, like the curved
arms of a pair of calipers, far around the unilluminated side of the
disk; at _C_ the atmosphere is illuminated all around by the sunlight
coming through it from behind, while the surface of the planet has
passed entirely out of the light--that is to say, Venus has become an
invisible globe embraced by a circle of refracted sunshine.

We return to the question of life. With almost twice as much solar heat
and light as we have, and with a deeper and denser atmosphere than ours,
it is evident, without seeking other causes of variation, that the
conditions of life upon Venus are notably different from those with
which we are acquainted. At first sight it would seem that a dense
atmosphere, together with a more copious supply of heat, might render
the surface temperature of Venus unsuitable for organic life as we
understand it. But so much depends upon the precise composition of the
atmosphere and upon the relative quantities of its constituents, that it
will not do to pronounce a positive judgment in such a case, because we
lack information on too many essential points.

Experiment has shown that the temperature of the air varies with changes
in the amount of carbonic acid and of water vapor that it contains. It
has been suggested that in past geologic ages the earth's atmosphere was
denser and more heavily charged with vapors than it is at present; yet
even then forms of life suited to their environment existed, and from
those forms the present inhabitants of our globe have been developed.
There are several lines of reasoning which may be followed to the
conclusion that Venus, as a life-bearing world, is younger than the
earth, and, according to that view, we are at liberty to imagine our
beautiful sister planet as now passing through some such period in its
history as that at which the earth had arrived in the age of the
carboniferous forests, or the age of the gigantic reptiles who ruled
both land and sea.

But, without making any assumptions as to the phase of evolution which
life may have attained on Venus, it is also possible to think that the
planet's thick shell of air, with its abundant vapors, may serve as a
shield against the excessive solar radiation. Venus is extraordinarily
brilliant, its reflective power being greatly in excess of Mercury's,
and it has often been suggested that this may be due to the fact that a
large share of the sunlight falling upon it is turned back before
reaching the planet's surface, being reflected both from the atmosphere
itself and from vast layers of clouds.

Even when viewed with the most powerful telescopes and in the most
favoring circumstances, the features of Venus's surface are difficult
to see, and generally extremely difficult. They consist of faint shadowy
markings, indefinite in outline, and so close to the limit of visibility
that great uncertainty exists not only as to their shape and their
precise location upon the planet, but even as to their actual existence.
No two observers have represented them exactly alike in drawings of the
planet, and, unfortunately, photography is as yet utterly unable to deal
with them. Mr. Percival Lowell, in his special studies of Venus in 1896,
using a 24-inch telescope of great excellence, in the clear and steady
air of Arizona, found delicate spokelike streaks radiating from a
rounded spot like a hub, and all of which, in his opinion, were genuine
and definite markings on the planet's surface. But others, using larger
telescopes, have failed to perceive the shapes and details depicted by
Mr. Lowell, and some are disposed to ascribe their appearances to
Venus's atmosphere. Mr. Lowell himself noticed that the markings seemed
to have a kind of obscuring veil over them.

In short, all observers of Venus agree in thinking that her atmosphere,
to a greater or less extent, serves as a mask to conceal her real
features, and the possibilities of so extensive an atmosphere with
reference to an adjustment of the peculiar conditions of the planet to
the requirements of life upon it, are almost unlimited. If we could
accurately analyze that atmosphere we would have a basis for more exact
conclusions concerning Venus's habitability.

But the mere existence of the atmosphere is, in itself, a strong
argument for the habitability of the planet, and as to the temperature,
we are really not compelled to imagine special adaptations by means of
which it may be brought into accord with that prevailing upon the earth.
As long as the temperature does not rise to the _destructive_ point,
beyond which our experience teaches that no organic life can exist, it
may very well attain an elevation that would mean extreme discomfort
from our point of view, without precluding the existence of life even in
its terrestrial sense.

And would it not be unreasonable to assume that vital phenomena on other
planets must be subject to exactly the same limitations that we find
circumscribing them in our world? That kind of assumption has more than
once led us far astray even in dealing with terrestrial conditions.

It is not so long ago, for instance, since life in the depths of the sea
was deemed to be demonstrably impossible. The bottom of the ocean, we
were assured, was a region of eternal darkness and of frightful
pressure, wherein no living creatures could exist. Yet the first dip of
the deep-sea trawl brought up animals of marvelous delicacy of
organization, which, although curiously and wonderfully adapted to live
in a compressed liquid, collapsed when lifted into a lighter medium, and
which, despite the assumed perpetual darkness of their profound abode,
were adorned with variegated colors and furnished with organs of
phosphorescence whereby they could create for themselves all the light
they needed.

Even the fixed animals of the sea, growing, like plants, fast to the
rocks, are frequently vivid with living light, and there is a splendid
suggestion of nature's powers of adaptation, which may not be entirely
inapplicable to the problems of life on strange planets, in Alexander
Agassiz's statement that species of sea animals, living below the depths
to which sunlight penetrates, "may dwell in total darkness and be
illuminated at times merely by the movements of abyssal fishes through
the forests of phosphorescent alcyonarians."

In attempting to judge the habitability of a planet such as Venus we
must first, as far as possible, generalize the conditions that govern
life and restrict its boundaries.

On the earth we find animated existence confined to the surface of the
crust of the globe, to the lower and denser strata of the atmosphere,
and to the film of water that constitutes the oceans. It does not exist
in the heart of the rocks forming the body of the planet nor in the void
of space surrounding it outside the atmosphere. As the earth condensed
from the original nebula, and cooled and solidified, a certain quantity
of matter remained at its surface in the form of free gases and unstable
compounds, and, within the narrow precincts where these things were,
lying like a thin shell between the huge inert globe of permanently
combined elements below, and the equally unchanging realm of the ether
above, life, a phenomenon depending upon ceaseless changes, combinations
and recombinations of chemical elements in unstable and temporary union,
made its appearance, and there only we find it at the present time.

It is because air and water furnish the means for the continual
transformations by which the bodies of animals and plants are built up
and afterward disintegrated and dispersed, that we are compelled to
regard their presence as prerequisites to the existence, on any planet,
of life in any of the forms in which we are acquainted with it. But if
we perceive that another world has an atmosphere, and that there is
water vapor in its atmosphere--both of which conditions are fulfilled by
Venus--and if we find that that world is bathed in the same sunshine
that stimulates the living forces of our planet, even though its
quantity or intensity may be different, then it would seem that we are
justified in averring that the burden of proof rests upon those who
would deny the capability of such a world to support inhabitants.

The generally accepted hypothesis of the origin of the solar system
leads us to believe that Venus has experienced the same process of
evolution as that which brought the earth into its present condition,
and we may fairly argue that upon the rocky shell of Venus exists a
region where chemical combinations and recombinations like those on the
surface of the earth are taking place. It is surely not essential that
the life-forming elements should exist in exactly the same states and
proportions as upon the earth; it is enough if some of them are
manifestly present. Even on the earth these things have undergone much
variation in the course of geological history, coincidently with the
development of various species of life. Just at present the earth
appears to have reached a stage where everything contributes to the
maintenance of a very high organization in both the animal and vegetable
kingdoms.

So each planet that has attained the habitable stage may have a typical
adjustment of temperature and atmospheric constitution, rendering life
possible within certain limits peculiar to that planet, and to the
special conditions prevailing there. Admitting, as there is reason for
doing, that different planets may be at different stages of development
in the geological and biological sense, we should, of course, not expect
to find them inhabited by the same living species. And, since there is
also reason to believe that no two planets upon arriving at the same
stage of evolution as globes would possess identical gaseous
surroundings, there would naturally be differences between their organic
life forms notwithstanding the similarity of their common phase of
development in other respects. Thus a departure from the terrestrial
type in the envelope of gases covering a planet, instead of precluding
life, would only tend to vary its manifestations.

After all, why should the intensity of the solar radiation upon Venus be
regarded as inimical to life? The sunbeams awaken life.

It is not impossible that relative nearness to the sun may be an
advantage to Venus from the biologic point of view. She gets less than
one third as much heat as Mercury receives on the average, and she gets
it with almost absolute uniformity. At aphelion Mercury is about two and
four tenths times hotter than Venus; then it rushes sunward, and within
forty-four days becomes six times hotter than Venus. In the meantime the
temperature of the latter, while high as compared with the earth's,
remains practically unchanged. Not only may Mercury's temperature reach
the destructive point, and thus be too high for organic life, but
Mercury gets nothing with either moderation or constancy. It is a world
both of excessive heat and of violent contrasts of temperature. Venus,
on the other hand, presents an unparalleled instance of invariableness
and uniformity. She may well be called the favorite of the sun, and,
through the advantages of her situation, may be stimulated by him to
more intense vitality than falls to the lot of the earth.

It is open, at least to the writers of the interplanetary romances now
so popular, to imagine that on Venus, life, while encompassed with the
serenity that results from the circular form of her orbit, and the
unchangeableness of her climates, is richer, warmer, more passionate,
more exquisite in its forms and more fascinating in its experiences,
keener of sense, capable of more delicious joys, than is possible to it
amid the manifold inclemencies of the colder earth.

We have seen that there is excellent authority for saying that Venus's
atmosphere is from one and a half to two times as dense and as extensive
as ours. Here is an interesting suggestion of aerial possibilities for
her inhabitants. If man could but fly, how would he take to himself
wings and widen his horizons along with the birds! Give him an
atmosphere the double in density of that which now envelopes him, take
off a little of his weight, thereby increasing the ratio of his strength
and activity, put into his nervous system a more puissant stimulus from
the life-giving sun, and perchance he _would_ fly.

Well, on Venus, apparently, these very conditions actually exist. How,
then, do intellectual creatures in the world of Venus take wing when
they choose? Upon what spectacle of fluttering pinions afloat in
iridescent air, like a Raphael dream of heaven and its angels, might we
not look down if we could get near enough to our brilliant evening star
to behold the intimate splendors of its life?

As Venus herself would be the most brilliant member of the celestial
host to an observer stationed on the night side of Mercury, so the earth
takes precedence in the midnight sky of Venus. For the inhabitants of
Venus Mercury is a splendid evening and morning star only, while the
earth, being an outer planet, is visible at times in that part of the
sky which is directly opposite to the place of the sun. The light
reflected from our planet is probably less dazzling than that which
Venus sends to us, both because, at our greater distance, the sunlight
is less intense, and because our rarer atmosphere reflects a smaller
proportion of the rays incident upon it. But the earth is, after all, a
more brilliant phenomenon seen from Venus than the latter is seen from
the earth, for the reason that the entire illuminated disk of the earth
is presented toward our sister planet when the two are at their nearest
point of approach, whereas, at that time, the larger part of the surface
of Venus that is turned earthward has no illumination, while the
illuminated portion is a mere crescent.

Owing, again, to the comparative rarity of the terrestrial atmosphere,
it is probable that the inhabitants of Venus--assuming their
existence--enjoy a superb view of the continents, oceans, polar snows,
and passing clouds that color and variegate the face of the earth. Our
astronomers can study the full disk of Venus only when she is at her
greatest distance, and on the opposite side of the sun from us, where
she is half concealed in the glare. The astronomers of Venus, on the
other hand, can study the earth under the most favorable conditions of
observation--that is to say, when it is nearest to them and when, being
in opposition to the sun, its whole disk is fully illuminated. In fact,
there is no planet in the entire system which enjoys an outlook toward a
sister world comparable with that which Venus enjoys with regard to the
earth. If there be astronomers upon Venus, armed with telescopes, it is
safe to guess that they possess a knowledge of the surface of the earth
far exceeding in minuteness and accuracy the knowledge that we possess
of the features of any heavenly body except the moon. They must long ago
have been able to form definite conclusions concerning the meteorology
and the probable habitability of our planet.

It certainly tends to increase our interest in Venus when, granting
that she is inhabited, we reflect upon the penetrating scrutiny of which
the earth may be the object whenever Venus--as happens once every 584
days--passes between us and the sun. The spectacle of our great planet,
glowing in its fullest splendor in the midnight sky, pied and streaked
with water, land, cloud, and snow, is one that might well excite among
the astronomers of another world, so fortunately placed to observe it,
an interest even greater than that which the recurrence of total solar
eclipses occasions upon the earth. For the inhabitants of Venus the
study of the earth must be the most absorbing branch of observational
astronomy, and the subject, we may imagine, of numberless volumes of
learned memoirs, far exceeding in the definiteness of their conclusions
the books that we have written about the physical characteristics of
other members of the solar system. And, if we are to look for attempts
on the part of the inhabitants of other worlds to communicate with us by
signals across the ether, it would certainly seem that Venus is the
most likely source of such efforts, for from no other planet can those
features of the earth that give evidence of its habitability be so
clearly discerned. Of one thing it would seem we may be certain: if
Venus has intellectual inhabitants they possess far more convincing
evidence of our existence than we are likely ever to have of theirs.

In referring to the view of the earth from Mercury it was remarked that
the moon is probably visible to the naked eye. From Venus the moon is
not only visible, but conspicuous, to the naked eye, circling about the
earth, and appearing at times to recede from it to a distance of about
half a degree--equal to the diameter of the full moon as we see it. The
disk of the earth is not quite four times greater in diameter than that
of the moon, and nowhere else in the solar system is there an instance
in which two bodies, no more widely different in size than are the moon
and the earth, are closely linked together. The moons of the other
planets that possess satellites are relatively so small that they
appear in the telescope as mere specks beside their primaries, but the
moon is so large as compared with the earth that the two must appear, as
viewed from Venus, like a double planet. To the naked eye they may look
like a very wide and brilliant double star, probably of contrasted
colors, the moon being silvery white and the earth, perhaps, now of a
golden or reddish tinge and now green or blue, according to the part of
its surface turned toward Venus, and according, also, to the season that
chances to be reigning over that part.

Such a spectacle could not fail to be of absorbing interest, and we can
not admit the possibility of intelligent inhabitants on Venus without
supposing them to watch the motions of the moon and the earth with the
utmost intentness. The passage of the moon behind and in front of the
earth, and its eclipses when it goes into the earth's shadow, could be
seen without the aid of telescopes, while, with such instruments, these
phenomena would possess the highest scientific interest and importance.

Because the earth has a satellite so easily observable, the astronomers
of Venus could not remain ignorant of the exact mass of our planet, and
in that respect they would outstrip us in the race for knowledge, since,
on account of the lack of a satellite attending Venus, we have been able
to do no more than make an approximate estimate of her mass.

With telescopes, too, in the case of a solar eclipse occurring at the
time of the earth's opposition, they could see the black spot formed by
the shadow of the moon, where the end of its cone moved across the earth
like the point of an invisible pencil, and could watch it traversing
continents and oceans, or thrown out in bold contrast upon the white
background of a great area of clouds. Indeed, the phenomena which our
globe and its satellite present to Venus must be so varied and wonderful
that one might well wish to visit that planet merely for the sake of
beholding them.

Thus far we have found so much of brilliant promise in the earth's twin
sister that I almost hesitate to approach another phase of the subject
which may tend to weaken the faith of some readers in the habitability
of Venus. It may have been observed that heretofore nothing has been
said as to the planet's rotation period, but, without specifically
mentioning it, I have tacitly assumed the correctness of the generally
accepted period of about twenty-four hours, determined by De Vico and
other observers. This period, closely accordant with the earth's, is, as
far as it goes, another argument for the habitability of Venus.

But now it must be stated that no less eminent an authority than
Schiaparelli holds that Venus, as well as Mercury, makes but a single
turn on its axis in the course of a revolution about the sun, and,
consequently, is a two-faced world, one side staring eternally at the
sun and the other side wearing the black mask of endless night.

Schiaparelli made this announcement concerning Venus but a few weeks
after publishing his discovery of Mercury's peculiar rotation. He
himself appears to be equally confident in both cases of the
correctness of his conclusions and the certainty of his observation. As
with Mercury, several other observers have corroborated him, and
particularly Percival Lowell in this country. Mr. Lowell, indeed, seems
unwilling to admit that any doubt can be entertained. Nevertheless, very
grave doubt is entertained, and that by many, and probably by the
majority, of the leading professional astronomers and observers. In
fact, some observers of great ability, equipped with powerful
instruments, have directly contradicted the results of Schiaparelli and
his supporters.

The reader may ask: "Why so readily accept Schiaparelli's conclusions
with regard to Mercury while rejecting them in the case of Venus?"

The reply is twofold. In the first place the markings on Venus, although
Mr. Lowell sketched them with perfect confidence in 1896, are, by the
almost unanimous testimony of those who have searched for them with
telescopes, both large and small, extremely difficult to see,
indistinct in outline, and perhaps evanescent in character. The sketches
of no two observers agree, and often they are remarkably unlike. The
fact has already been mentioned that Mr. Lowell noticed a kind of veil
partially obscuring the markings, and which he ascribed, no doubt
correctly, to the planet's atmosphere. But he thinks that,
notwithstanding the atmospheric veil, the markings noted by him were
unquestionably permanent features of the planet's real surface.
Inasmuch, however, as his drawings represent things entirely different
from what others have seen, there seems to be weight in the suggestion
that the radiating bands and shadings noticed by him were in some manner
illusory, and perhaps of atmospheric origin.

If the markings were evidently of a permanent nature and attached to the
solid shell of the planet, and if they were of sufficient distinctness
to be seen in substantially the same form by all observers armed with
competent instruments, then whatever conclusion was drawn from their
apparent motion as to the period of the planet's rotation would have to
be accepted. In the case of Mercury the markings, while not easily seen,
appear to be sufficiently distinct to afford confidence in the result of
observations based upon them, but Venus's markings have been represented
in so many different ways that it seems advisable to await more light
before accepting any extraordinary, and in itself improbable, conclusion
based upon them.

It should also be added that in 1900 spectroscopic observations by
Belopolski at Pulkova gave evidence that Venus really rotates rapidly on
her axis, in a period probably approximating to the twenty-four hours of
the earth's rotation, thus corroborating the older conclusions.

Belopolski's observation, it may be remarked, was based upon what is
known as the Doppler principle, which is employed in measuring the
motion of stars in the line of sight, and in other cases of rapidly
moving sources of light. According to this principle, when a source of
light, either original or reflected, is approaching the observer, the
characteristic lines in its spectrum are shifted toward the blue end,
and when it is retreating from the observer the lines are shifted toward
the red end. Now, in the case of a planet rotating rapidly on its axis,
it is clear that if the observer is situated in, or nearly in, the plane
of the planet's equator, one edge of its disk will be approaching his
eye while the opposite edge is retreating, and the lines in the spectrum
of a beam of light from the advancing edge will be shifted toward the
blue, while those in the spectrum of the light coming from the
retreating edge will be shifted toward the red. And, by carefully noting
the amount of the shifting, the velocity of the planet's rotation can be
computed. This is what was done by Belopolski in the case of Venus, with
the result above noted.

Secondly, the theory that Venus rotates but once in the course of a
revolution finds but slight support from the doctrine of tidal friction,
as compared with that which it receives when applied to Mercury. The
effectiveness of the sun's attraction in slowing down the rotation of a
planet through the braking action of the tides raised in the body of the
planet while it is yet molten or plastic, varies inversely as the sixth
power of the planet's distance. For Mercury this effectiveness is nearly
three hundred times as great as it is for the earth, while for Venus it
is only seven times as great. While we may admit, then, that Mercury,
being relatively close to the sun and subject to an enormous braking
action, lost rotation until--as occurred for a similar reason to the
moon under the tidal attraction of the earth--it ended by keeping one
face always toward its master, we are not prepared to make the same
admission in the case of Venus, where the effective force concerned is
comparatively so slight.

It should be added, however, that no certain evidence of polar
compression in the outline of Venus's disk has ever been obtained, and
this fact would favor the theory of a very slow rotation because a
plastic globe in swift rotation has its equatorial diameter increased
and its polar diameter diminished. If Venus were as much flattened at
the poles as the earth is, it would seem that the fact could not escape
detection, yet the necessary observations are very difficult, and Venus
is so brilliant that her light increases the difficulty, while her
transits across the sun, when she can be seen as a round black disk, are
very rare phenomena, the latest having occurred in 1874 and 1882, and
the next not being due until 2004.

Upon the whole, probably the best method of settling the question of
Venus's rotation is the spectroscopic method, and that, as we saw, has
already given evidence for the short period.

Even if it were established that Venus keeps always the same face to the
sun, it might not be necessary to abandon altogether the belief that she
is habitable, although, of course, the obstacles to that belief would be
increased. Venus's orbit being so nearly circular, and her orbital
motion so nearly invariable, she has but a very slight libration with
reference to the sun, and the east and west lunes on her surface, where
day and night would alternate once in her year of 225 days, would be so
narrow as to be practically negligible.

But, owing to her extensive atmosphere, there would be a very broad band
of twilight on Venus, running entirely around the planet at the inner
edge of the light hemisphere. What the meteorological conditions within
this zone would be is purely a matter of conjecture. As in the case of
Mercury, we should expect an interchange of atmospheric currents between
the light and dark sides of the planet, the heated air rising under the
influence of the unsetting sun in one hemisphere, and being replaced by
an indraught of cold air from the other. The twilight band would
probably be the scene of atmospheric conflicts and storms, and of
immense precipitation, if there were oceans on the light hemisphere to
charge the air with moisture.

It has been suggested that ice and snow might be piled in a vast circle
of glaciers, belting the planet along the line between perpetual day
and night, and that where the sunbeams touched these icy deposits near
the edge of the light hemisphere a marvelous spectacle of prismatic
hills of crystal would be presented!

It may be remarked that it would be the inhabitants of the dark
hemisphere who would enjoy the beautiful scene of the earth and the moon
in opposition.




CHAPTER IV

MARS, A WORLD MORE ADVANCED THAN OURS


Mars is the fourth planet in the order of distance from the sun, and the
outermost member of the terrestrial group. Its mean distance is
141,500,000 miles, variable, through the eccentricity of its orbit, to
the extent of about 13,000,000 miles. It will be observed that this is
only a million miles less than the variation in Mercury's distance from
the sun, from which, in a previous chapter, were deduced most momentous
consequences; but, in the case of Mars, the ratio of the variation to
the mean distance is far smaller than with Mercury, so that the effect
upon the temperature of the planet is relatively insignificant.

Mars gets a little less than half as much solar light and heat as the
earth receives, its situation in this respect being just the opposite
to that of Venus. Its period of orbital revolution, or the length of its
year, is 687 of our days. The diameter of Mars is 4,200 miles, and its
density is 73 per cent of the earth's density. Gravity on its surface is
only 38 per cent of terrestrial gravity--i.e., a one hundred-pound
weight removed from the earth to Mars would there weigh but thirty-eight
pounds. Mars evidently has an atmosphere, the details of which we shall
discuss later.

The poles of the planet are inclined from a perpendicular to the plane
of its orbit at very nearly the same angle as that of the earth's poles,
viz., 24° 50´. Its rotation on its axis is also effected in almost the
same period as the earth's, viz., 24 hours, 37 minutes.

When in opposition to the sun, Mars may be only about 35,000,000 miles
from the earth, but its average distance when in that position is more
than 48,000,000 miles, and may be more than 60,000,000. These
differences arise from the eccentricities of the orbits of the two
planets. When on the farther side of the sun--i.e., in conjunction with
the sun as seen from the earth--Mars's average distance from us is about
235,000,000 miles. In consequence of these great changes in its
distance, Mars is sometimes a very conspicuous object in the sky, and at
other times inconspicuous.

The similarity in the inclination of the axis of the two planets results
in a close resemblance between the seasons on Mars and on the earth,
although, owing to the greater length of its year, Mars's seasons are
much longer than ours. Winter and summer visit in succession its
northern and southern hemispheres just as occurs on the planet that we
inhabit, and the torrid, temperate, and frigid zones on its surface have
nearly the same angular width as on the earth. In this respect Mars is
the first of the foreign planets we have studied to resemble the earth.

Around each of its poles appears a circular white patch, which visibly
expands when winter prevails upon it, and rapidly contracts, sometimes
almost completely disappearing, under a summer sun. From the time of
Sir William Herschel the almost universal belief among astronomers has
been that these gleaming polar patches on Mars are composed of snow and
ice, like the similar glacial caps of the earth, and no one can look at
them with a telescope and not feel the liveliest interest in the planet
to which they belong, for they impart to it an appearance of likeness to
our globe which at first glance is all but irresistible.

To watch one of them apparently melting, becoming perceptibly smaller
week after week, while the general surface of the corresponding
hemisphere of the planet deepens in color, and displays a constantly
increasing wealth of details as summer advances across it, is an
experience of the most memorable kind, whose effect upon the mind of the
observer is indescribable.

Early in the history of the telescope it became known that, in addition
to the polar caps, Mars presented a number of distinct surface features,
and gradually, as instruments increased in power and observers in
skill, charts of the planet were produced showing a surface diversified
somewhat in the manner that characterizes the face of the earth,
although the permanent forms do not closely resemble those of our
planet.

Two principal colors exist on the disk of Mars--dark, bluish gray or
greenish gray, characterizing areas which have generally been regarded
as seas, and light yellowish red, overspreading broad regions looked
upon as continents. It was early observed that if the dark regions
really are seas, the proportion of water to land upon Mars is much
smaller than upon the earth.

For two especial reasons Mars has generally been regarded as an older or
more advanced planet than the earth. The first reason is that, accepting
Laplace's theory of the origin of the planetary system from a series of
rings left off at the periphery of the contracting solar nebula, Mars
must have come into existence earlier than the earth, because, being
more distant from the center of the system, the ring from which it was
formed would have been separated sooner than the terrestrial ring. The
second reason is that Mars being smaller and less massive than the earth
has run through its developments a cooling globe more rapidly. The
bearing of these things upon the problems of life on Mars will be
considered hereafter.

And now, once more, Schiaparelli appears as the discoverer of surprising
facts about one of the most interesting worlds of the solar system.
During the exceptionally favorable opposition of Mars in 1877, when an
American astronomer, Asaph Hall, discovered the planet's two minute
satellites, and again during the opposition of 1879, the Italian
observer caught sight of an astonishing network of narrow dark lines
intersecting the so-called continental regions of the planet and
crossing one another in every direction. Schiaparelli did not see the
little moons that Hall discovered, and Hall did not perceive the
enigmatical lines that Schiaparelli detected. Hall had by far the larger
and more powerful telescope; Schiaparelli had much the more steady and
favorable atmosphere for astronomical observation. Yet these differences
in equipment and circumstances do not clearly explain why each observer
should have seen what the other did not.

There may be a partial explanation in the fact that an observer having
made a remarkable discovery is naturally inclined to confine his
attention to it, to the neglect of other things. But it was soon found
that Schiaparelli's lines--to which he gave the name "canals," merely on
account of their shape and appearance, and without any intention to
define their real nature--were excessively difficult telescopic objects.
Eight or nine years elapsed before any other observer corroborated
Schiaparelli's observations, and notwithstanding the "sensation" which
the discovery of the canals produced they were for many years regarded
by the majority of astronomers as an illusion.

But they were no illusion, and in 1881 Schiaparelli added to the
astonishment created by his original discovery, and furnished additional
grounds for skepticism, by announcing that, at certain times, many of
the canals geminated, or became double! He continued his observations at
each subsequent opposition, adding to the number of the canals observed,
and charting them with classical names upon a detailed map of the
planet's surface.

At length in 1886 Perrotin, at Nice, detected many of Schiaparelli's
canals, and later they were seen by others. In 1888 Schiaparelli greatly
extended his observations, and in 1892 and 1894 some of the canals were
studied with the 36-inch telescope of the Lick Observatory, and in the
last-named year a very elaborate series of observations upon them was
made by Percival Lowell and his associates, Prof. William C. Pickering
and Mr. A.E. Douglass, at Flagstaff, Arizona. Mr. Lowell's charts of the
planet are the most complete yet produced, containing 184 canals to
which separate names have been given, besides more than a hundred other
markings also designated by individual appellations.

It should not be inferred from the fact that Schiaparelli's discovery
in 1877 excited so much surprise and incredulity that no glimpse of the
peculiar canal-like markings on Mars had been obtained earlier than
that. At least as long ago as 1864 Mr. Dawes, in England, had seen and
sketched half a dozen of the larger canals, or at least the broader
parts of them, especially where they connect with the dark regions known
as seas, but Dawes did not see them in their full extent, did not
recognize their peculiar character, and entirely failed to catch sight
of the narrower and more numerous ones which constitute the wonderful
network discovered by the Italian astronomer. Schiaparelli found no less
than sixty canals during his first series of observations in 1877.

Let us note some of the more striking facts about the canals which
Schiaparelli has described. We can not do better than quote his own
words:

"There are on this planet, traversing the continents, long dark lines
which may be designated as _canals_, although we do not yet know what
they are. These lines run from one to another of the somber spots that
are regarded as seas, and form, over the lighter, or continental,
regions a well-defined network. Their arrangement appears to be
invariable and permanent; at least, as far as I can judge from four and
a half years of observation. Nevertheless, their aspect and their degree
of visibility are not always the same, and depend upon circumstances
which the present state of our knowledge does not yet permit us to
explain with certainty. In 1879 a great number were seen which were not
visible in 1877, and in 1882 all those which had been seen at former
oppositions were found again, together with new ones. Sometimes these
canals present themselves in the form of shadowy and vague lines, while
on other occasions they are clear and precise, like a trace drawn with a
pen. In general they are traced upon the sphere like the lines of great
circles; a few show a sensible lateral curvature. They cross one another
obliquely, or at right angles. They have a breadth of two degrees, or
120 kilometres [74 miles], and several extend over a length of eighty
degrees, or 4,800 kilometres [nearly 3,000 miles]. Their tint is very
nearly the same as that of the seas, usually a little lighter. Every
canal terminates at both its extremities in a sea, or in another canal;
there is not a single example of one coming to an end in the midst of
dry land.

"This is not all. In certain seasons these canals become double. This
phenomenon seems to appear at a determinate epoch, and to be produced
simultaneously over the entire surface of the planet's continents. There
was no indication of it in 1877, during the weeks that preceded and
followed the summer solstice of that world. A single isolated case
presented itself in 1879. On the 26th of December, this year--a little
before the spring equinox, which occurred on Mars on the 21st of
January, 1880--I noticed the doubling of the Nile [a canal thus named]
between the Lakes of the Moon and the Ceraunic Gulf. These two regular,
equal, and parallel lines caused me, I confess, a profound surprise,
the more so because a few days earlier, on the 23d and the 24th of
December, I had carefully observed that very region without discovering
anything of the kind.

"I awaited with curiosity the return of the planet in 1881, to see if an
analogous phenomenon would present itself in the same place, and I saw
the same thing reappear on the 11th of January, 1882, one month after
the spring equinox--which occurred on the 8th of December, 1881. The
duplication was still more evident at the end of February. On this same
date, the 11th of January, another duplication had already taken place,
that of the middle portion of the canal of the Cyclops, adjoining
Elysium. [Elysium is a part of one of the continental areas.]

"Yet greater was my astonishment when, on the 19th of January, I saw the
canal Jamuna, which was then in the center of the disk, formed very
rigidly of two parallel straight lines, crossing the space which
separates the Niliac Lake from the Gulf of Aurora. At first sight I
believed it was an illusion, caused by fatigue of the eye and some new
kind of strabismus, but I had to yield to the evidence. After the 19th
of January I simply passed from wonder to wonder; successively the
Orontes, the Euphrates, the Phison, the Ganges, and the larger part of
the other canals, displayed themselves very clearly and indisputably
duplicated. There were not less than twenty examples of duplication, of
which seventeen were observed in the space of a month, from the 19th of
January to the 19th of February.

"In certain cases it was possible to observe precursory symptoms which
are not lacking in interest. Thus, on the 13th of January, a light,
ill-defined shade extended alongside the Ganges; on the 18th and the
19th one could only distinguish a series of white spots; on the 20th the
shadow was still indecisive, but on the 21st the duplication was
perfectly clear, such as I observed it until the 23d of February. The
duplication of the Euphrates, of the canal of the Titans, and of the
Pyriphlegethon also began in an uncertain and nebulous form.

"These duplications are not an optical effect depending on increase of
visual power, as happens in the observation of double stars, and it is
not the canal itself splitting in two longitudinally. Here is what is
seen: To the right or left of a pre-existing line, without any change in
the course and position of that line, one sees another line produce
itself, equal and parallel to the first, at a distance generally varying
from six to twelve degrees--i.e., from 350 to 700 kilometres (217 to 434
miles); even closer ones seem to be produced, but the telescope is not
powerful enough to distinguish them with certainty. Their tint appears
to be a quite deep reddish brown. The parallelism is sometimes
rigorously exact. There is nothing analogous in terrestrial geography.
Everything indicates that here there is an organization special to the
planet Mars, probably connected with the course of its seasons."[1]

[Footnote 1: L'Astronomie, vol. i, 1882, pp. 217 _et seq._]

Schiaparelli adds that he took every precaution to avoid the least
suspicion of illusion. "I am absolutely sure," he says, "of what I have
observed."

I have quoted his statement, especially about the duplication of the
canals, at so much length, both on account of its intrinsic interest and
because it has many times been argued that this particular phenomenon
must be illusory even though the canals are real.

One of the most significant facts that came out in the early
observations was the evident connection between the appearance of the
canals and the seasonal changes on Mars. It was about the time of the
spring equinox, when the white polar caps had begun to melt, that
Schiaparelli first noticed the phenomenon of duplication. As the season
advanced the doubling of the canals increased in frequency and the lines
became more distinct. In the meantime the polar caps were becoming
smaller. Broadly speaking, Schiaparelli's observation showed that the
doubling of the canals occurred principally a little after the spring
equinox and a little before the autumn equinox; that the phenomenon
disappeared in large part at the epoch of the winter solstice, and
disappeared altogether at the epoch of the summer solstice. Moreover, he
observed that many of the canals, without regard to duplication, were
invisible at times, and reappeared gradually; faint, scarcely visible
lines and shadows, deepened and became more distinct until they were
clearly and sharply defined, and these changes, likewise, were evidently
seasonal.

The invariable connection of the canals at their terminations with the
regions called seas, the fact that as the polar caps disappeared the
sealike expanses surrounding the polar regions deepened in color, and
other similar considerations soon led to the suggestion that there
existed on Mars a wonderful system of water circulation, whereby the
melting of the polar snows, as summer passed alternately from one
hemisphere to the other, served to reenforce the supply of water in the
seas, and, through the seas, in the canals traversing the broad
expanses of dry land that occupy the equatorial regions of the planet.
The thought naturally occurred that the canals might be of artificial
origin, and might indicate the existence of a gigantic system of
irrigation serving to maintain life upon the globe of Mars. The
geometrical perfection of the lines, their straightness, their absolute
parallelism when doubled, their remarkable tendency to radiate from
definite centers, lent strength to the hypothesis of an artificial
origin. But their enormous size, length, and number tended to stagger
belief in the ability of the inhabitants of any world to achieve a work
so stupendous.

After a time a change of view occurred concerning the nature of the
expanses called seas, and Mr. Lowell, following his observations of
1894, developed the theory of the water circulation and irrigation of
Mars in a new form. He and others observed that occasionally canals were
visible cutting straight across some of the greenish, or bluish-gray,
areas that had been regarded as seas. This fact suggested that, instead
of seas, these dark expanses may rather be areas of marshy ground
covered with vegetation which flourishes and dies away according as the
supply of water alternately increases and diminishes, while the reddish
areas known as continents are barren deserts, intersected by canals; and
as the water released by the melting of the polar snows begins to fill
the canals, vegetation springs up along their sides and becomes visible
in the form of long narrow bands.

According to this theory, the phenomena called canals are simply lines
of vegetation, the real canals being individually too small to be
detected. It may be supposed that from a central supply canal irrigation
ditches are extended for a distance of twenty or thirty miles on each
side, thus producing a strip of fertile soil from forty to sixty miles
wide, and hundreds, or in some cases two or three thousands, of miles in
length.

The water supply being limited, the inhabitants can not undertake to
irrigate the entire surface of the thirsty land, and convenience of
circulation induces them to extend the irrigated areas in the form of
long lines. The surface of Mars, according to Lowell's observation, is
remarkably flat and level, so that no serious obstacle exists to the
extension of the canal system in straight bands as undeviating as arcs
of great circles.

Wherever two or more canals meet, or cross, a rounded dark spot from a
hundred miles, or less, to three hundred miles in diameter, is seen. An
astonishing number of these appear on Mr. Lowell's charts. Occasionally,
as occurs at the singular spot named Lacus Solis, several canals
converging from all points of the compass meet at a central point like
the spokes of a wheel; in other cases, as, for instance, that of the
long canal named Eumenides, with its continuation Orcus, a single
conspicuous line is seen threading a large number of round dark spots,
which present the appearance of a row of beads upon a string. These
circular spots, which some have regarded as lakes, Mr. Lowell believes
are rather oases in the great deserts, and granting the correctness of
his theory of the canals the aptness of this designation is apparent.[2]

[Footnote 2: The reader can find many of these "canals" and "oases," as
well as some of the other regions on Mars that have received names, in
the frontispiece.]

Wherever several canals, that is to say, several bands of vegetation or
bands of life, meet, it is reasonable to assume that an irrigated and
habitable area of considerable extent will be developed, and in such
places the imagination may picture the location of the chief centers of
population, perhaps in the form of large cities, or perhaps in groups of
smaller towns and villages. The so-called Lacus Solis is one of these
localities.

So, likewise, it seems but natural that along the course of a broad,
well-irrigated band a number of expansions should occur, driving back
the bounds of the desert, forming rounded areas of vegetation, and thus
affording a footing for population. Wherever two bands cross such areas
would be sure to exist, and in almost every instance of crossing the
telescope actually shows them.

As to the gemination or duplication of many of the lines which, at the
beginning of the season, appear single, it may be suggested that, in the
course of the development of the vast irrigation system of the planet
parallel bands of cultivation have been established, one receiving its
water supply from the canals of the other, and consequently lagging a
little behind in visibility as the water slowly percolates through the
soil and awakens the vegetation. Or else, the character of the
vegetation itself may differ as between two such parallel bands, one
being supplied with plants that spring up and mature quickly when the
soil about their roots is moistened, while the plants in the twin band
respond more slowly to stimulation.

Objection has been made to the theory of the artificial origin of the
canals of Mars on the ground, already mentioned, that the work required
to construct them would be beyond the capacity of any race of creatures
resembling man. The reply that has been made to this is twofold. In the
first place, it should be remembered that the theory, as Mr. Lowell
presents it, does not assert that the visible lines are the actual
canals, but only that they are strips of territory intersected, like
Holland or the center of the plain of Lombardy, by innumerable
irrigation canals and ditches. To construct such works is clearly not an
impossible undertaking, although it does imply great industry and
concentration of effort.

In the second place, since the force of gravity on Mars is in the ratio
of only 38 to 100 compared with the earth's, it is evident that the
diminished weight of all bodies to be handled would give the inhabitants
of Mars an advantage over those of the earth in the performance of
manual labor, provided that they possess physical strength and activity
as great as ours. But, in consequence of this very fact of the slighter
force of gravity, a man upon Mars could attain a much greater size, and
consequently much greater muscular strength, than his fellows upon the
earth possess without being oppressed by his own weight. In other words,
as far as the force of gravity may be considered as the decisive factor,
Mars could be inhabited by giants fifteen feet tall, who would be
relatively just as active, and just as little impeded in their movements
by the weight of their bodies, as a six-footer is upon the earth. But
they would possess far more physical strength than we do, while, in
doing work, they would have much lighter materials to deal with.

Whether the theory that the canals of Mars really are canals is true or
not, at any rate there can now be no doubt as to the existence of the
strange lines which bear that designation. The suggestion has been
offered that their builders may no longer be in existence, Mars having
already passed the point in its history where life must cease upon its
surface. This brings us to consider again the statement, made near the
beginning of this chapter, that Mars is, perhaps, at a more advanced
stage of development than the earth. If we accept this view, then,
provided there was originally some resemblance between Mars's life forms
and those of the earth, the inhabitants of that planet would, at every
step, probably be in front of their terrestrial rivals, so that at the
present time they should stand well in advance. Mr. Lowell has, perhaps,
put this view of the relative advancement in evolution of Mars and its
inhabitants as picturesquely as anybody.

"In Mars," he says, "we have before us the spectacle of a world
relatively well on in years, a world much older than the earth. To so
much about his age Mars bears witness on his face. He shows unmistakable
signs of being old. Advancing planetary years have left their mark
legible there. His continents are all smoothed down; his oceans have all
dried up.... Mars being thus old himself, we know that evolution on his
surface must be similarly advanced. This only informs us of its
condition relative to the planet's capabilities. Of its actual state our
data are not definite enough to furnish much deduction. But from the
fact that our own development has been comparatively a recent thing, and
that a long time would be needed to bring even Mars to his present
geological condition, we may judge any life he may support to be not
only relatively, but really older than our own. From the little we can
see such appears to be the case. The evidence of handicraft, if such it
be, points to a highly intelligent mind behind it. Irrigation,
unscientifically conducted, would not give us such truly wonderful
mathematical fitness in the several parts to the whole as we there
behold.... Quite possibly such Martian folk are possessed of inventions
of which we have not dreamed, and with them electrophones and
kinetoscopes are things of a bygone past, preserved with veneration in
museums as relics of the clumsy contrivances of the simple childhood of
the race. Certainly what we see hints at the existence of beings who are
in advance of, not behind us, in the journey of life."[3]

[Footnote 3: Mars, by Percival Lowell, p. 207 _et seq._]

Granted the existence of such a race as is thus described, and to them
it might not seem a too appalling enterprise, when their planet had
become decrepit, with its atmosphere thinned out and its supply of water
depleted, to grapple with the destroying hand of nature and to prolong
the career of their world by feats of chemistry and engineering as yet
beyond the compass of human knowledge.

It is confidence, bred from considerations like these, in the superhuman
powers of the supposed inhabitants of Mars that has led to the popular
idea that they are trying to communicate by signals with the earth.
Certain enigmatical spots of light, seen at the edge of the illuminated
disk of Mars, and projecting into the unilluminated part--for Mars,
although an outer planet, shows at particular times a gibbous phase
resembling that of the moon just before or just after the period of full
moon--have been interpreted by some, but without any scientific
evidence, as of artificial origin.

Upon the assumption that these bright points, and others occasionally
seen elsewhere on the planet's disk, are intended by the Martians for
signals to the earth, entertaining calculations have been made as to the
quantity of light that would be required in the form of a "flash signal"
to be visible across the distance separating the two planets. The
results of the calculations have hardly been encouraging to possible
investors in interplanetary telegraphy, since it appears that
heliographic mirrors with reflecting surfaces measured by square miles,
instead of square inches, would be required to send a visible beam from
the earth to Mars or _vice versa_.

The projections of light on Mars can be explained much more simply and
reasonably. Various suggestions have been made about them; among others,
that they are masses of cloud reflecting the sunshine; that they are
areas of snow; and that they are the summits of mountains crowned with
ice and encircled with clouds. In fact, a huge mountain mass lying on
the terminator, or the line between day and night, would produce the
effect of a tongue of light projecting into the darkness without
assuming that it was snow-covered or capped with clouds, as any one may
convince himself by studying the moon with a telescope when the
terminator lies across some of its most mountainous regions. To be sure,
there is reason to think that the surface of Mars is remarkably flat;
yet even so the planet may have some mountains, and on a globe the
greater part of whose shell is smooth any projections would be
conspicuous, particularly where the sunlight fell at a low angle across
them.

Another form in which the suggestion of interplanetary communication has
been urged is plainly an outgrowth of the invention and surprising
developments of wireless telegraphy. The human mind is so constituted
that whenever it obtains any new glimpse into the arcana of nature it
immediately imagines an indefinite and all but unlimited extension of
its view in that direction. So to many it has not appeared unreasonable
to assume that, since it is possible to transmit electric impulses for
considerable distances over the earth's surface by the simple
propagation of a series of waves, or undulations, without connecting
wires, it may also be possible to send such impulses through the ether
from planet to planet.

The fact that the electric undulations employed in wireless telegraphy
pass between stations connected by the crust of the earth itself, and
immersed in a common atmospheric envelope, is not deemed by the
supporters of the theory in question as a very serious objection, for,
they contend, electric waves are a phenomenon of the ether, which
extends throughout space, and, given sufficient energy, such waves could
cross the gap between world and world.

But nobody has shown how much energy would be needed for such a purpose,
and much less has anybody indicated a way in which the required energy
could be artificially developed, or cunningly filched from the stores of
nature. It is, then, purely an assumption, an interesting figment of
the mind, that certain curious disturbances in the electrical state of
the air and the earth, affecting delicate electric instruments,
possessing a marked periodicity in brief intervals of time, and not yet
otherwise accounted for, are due to the throbbing, in the all-enveloping
ether, of impulses transmitted from instruments controlled by the
_savants_ of Mars, whose insatiable thirst for knowledge, and presumably
burning desire to learn whether there is not within reach some more
fortunate world than their half-dried-up globe, has led them into a
desperate attempt to "call up" the earth on their interplanetary
telephone, with the hope that we are wise and skilful enough to
understand and answer them.

In what language they intend to converse no one has yet undertaken to
tell, but the suggestion has sapiently been made that, mathematical
facts being invariable, the eternal equality of two plus two with four
might serve as a basis of understanding, and that a statement of that
truth sent by electric taps across the ocean of ether would be a
convincing assurance that the inhabitants of the planet from which the
message came at least enjoyed the advantages of a common-school
education.

But, while speculation upon this subject rests on unverified, and at
present unverifiable, assumptions, of course everybody would rejoice if
such a thing were possible, for consider what zest and charm would be
added to human life if messages, even of the simplest description, could
be sent to and received from intelligent beings inhabiting other
planets! It is because of this hold that it possesses upon the
imagination, and the pleasing pictures that it conjures up, that the
idea of interplanetary communication, once broached, has become so
popular a topic, even though everybody sees that it should not be taken
too seriously.

The subject of the atmosphere of Mars can not be dismissed without
further consideration than we have yet given it, because those who think
the planet uninhabitable base their opinion largely upon the assumed
absence of sufficient air to support life. It was long ago recognized
that, other things being equal, a planet of small mass must possess a
less dense atmosphere than one of large mass. Assuming that each planet
originally drew from a common stock, and that the amount and density of
its atmosphere is measured by its force of gravity, it can be shown that
Mars should have an atmosphere less than one fifth as dense as the
earth's.

Dr. Johnstone Stoney has attacked the problem of planetary atmospheres
in another way. Knowing the force of gravity on a planet, it is easy to
calculate the velocity with which a body, or a particle, would have to
start radially from the planet in order to escape from its gravitational
control. For the earth this critical velocity is about seven miles per
second; for Mars about three miles per second. Estimating the velocity
of the molecules of the various atmospheric gases, according to the
kinetic theory, Dr. Stoney finds that some of the smaller planets, and
the moon, are gravitationally incapable of retaining all of these gases
in the form of an atmosphere. Among the atmospheric constituents that,
according to this view, Mars would be unable permanently to retain is
water vapor. Indeed, he supposes that even the earth is slowly losing
its water by evaporation into space, and on Mars, owing to the slight
force of gravity there, this process would go on much more rapidly, so
that, in this way, we have a means of accounting for the apparent drying
up of that planet, while we may be led to anticipate that at some time
in the remote future the earth also will begin to suffer from lack of
water, and that eventually the chasms of the sea will yawn empty and
desolate under a cloudless sky.

But it is not certain that the original supply of atmospheric elements
was in every case proportional to the respective force of gravity of a
planet. The fact that Venus appears to have an atmosphere more extensive
and denser than the earth's, although its force of gravity is a little
less than that of our globe, indicates at once a variation as between
these two planets in the amount of atmospheric material at their
disposal. This may be a detail depending upon differences in the mode,
or in the stage, of their evolution. Thus, after all, Dr. Stoney's
theory may be substantially correct and yet Mars may retain sufficient
water to form clouds, to be precipitated in snow, and to fill its canals
after each annual melting of the polar caps, because the original supply
was abundant, and its escape is a gradual process, only to be completed
by age-long steps.

Even though the evidence of the spectroscope, as far as it goes, seems
to lend support to the theory that there is no water vapor in the
atmosphere of Mars, we can not disregard the visual evidence that,
nevertheless, water vapor exists there.

What are the polar caps if they are not snow? Frozen carbon dioxide, it
has been suggested; but this is hardly satisfactory, for it offers no
explanation of the fact that when the polar caps diminish, and in
proportion as they diminish, the "seas" and the canals darken and
expand, whereas a reasonable explanation of the correlation of these
phenomena is offered if we accept the view that the polar caps consist
of snow.

Then there are many observations on record indicating the existence of
clouds in Mars's atmosphere. Sometimes a considerable area of its
surface has been observed to be temporarily obscured, not by dense
masses of cloud such as accompany the progress of great cyclonic storms
across the continents and oceans of the earth, but by comparatively thin
veils of vapor such as would be expected to form in an atmosphere so
comparatively rare as that of Mars. And these clouds, in some instances
at least, appear, like the cirrus streaks and dapples in our own air, to
float at a great elevation. Mr. Douglass, one of Mr. Lowell's associates
in the observations of 1894 at Flagstaff, Arizona, observed what he
believed to be a cloud over the unilluminated part of Mars's disk,
which, by micrometric measurement and estimate, was drifting at an
elevation of about fifteen miles above the surface of the planet. This
was seen on two successive days, November 25th and November 26th, and it
underwent curious fluctuations in visibility, besides moving in a
northerly direction at the rate of some thirteen miles an hour. But,
upon the whole, as Mr. Lowell remarks, the atmosphere of Mars is
remarkably free of clouds.

The reader will remember that Mars gets a little less than half as much
heat from the sun as the earth gets. This fact also has been used as an
argument against the habitability of the planet. In truth, those who
think that life in the solar system is confined to the earth alone
insist upon an almost exact reproduction of terrestrial conditions as a
_sine qua non_ to the habitability of any other planet. Venus, they
think, is too hot, and Mars too cold, as if life were rather a happy
accident than the result of the operation of general laws applicable
under a wide variety of conditions. All that we are really justified in
asserting is that Venus may be too hot and Mars too cold for _us_. Of
course, if we adopt the opinion held by some that the temperature on
Mars is constantly so low that water would remain perpetually frozen, it
does throw the question of the kind of life that could be maintained
there into the realm of pure conjecture.

The argument in favor of an extremely low temperature on Mars is based
on the law of the diminution of radiant energy inversely as the square
of the distance, together with the assumption that no qualifying
circumstances, or no modification of that law, can enter into the
problem. According to this view, it could be shown that the temperature
on Mars never rises above -200° F. But it is a view that seems to be
directly opposed to the evidence of the telescope, for all who have
studied Mars under favorable conditions of observation have been
impressed by the rapid and extensive changes that the appearance of its
surface undergoes coincidently with the variation of the planet's
seasons. It has its winter aspect and its summer aspect, perfectly
distinct and recognizable, in each hemisphere by turns, and whether the
polar caps be snow or carbon dioxide, at any rate they melt and
disappear under a high sun, thus proving that an accumulation of heat
takes place.

Professor Young says: "As to the temperature of Mars we have no certain
knowledge. On the one hand, we know that on account of the planet's
distance from the sun the intensity of solar radiation upon its surface
must be less than here in the ratio of 1 to (1.524)^2--i.e., only about
43 per cent as great as with us; its 'solar constant' must be less than
13 calories against our 30. Then, too, the low density of its
atmosphere, probably less at the planet's surface than on the tops of
our highest mountains, would naturally assist to keep down the
temperature to a point far below the freezing-point of water. But, on
the other hand, things certainly _look_ as if the polar caps were really
masses of _snow_ and _ice_ deposited from vapor in the planet's
atmosphere, and as if these actually melted during the Martian summer,
sending floods of water through the channels provided for them, and
causing the growth of vegetation along their banks. We are driven,
therefore, to suppose either that the planet has sources of heat
internal or external which are not yet explained, or else, as long ago
suggested, that the polar 'snow' may possibly be composed of something
else than frozen _water_."[4]

[Footnote 4: General Astronomy, by Charles A. Young. Revised edition,
1898, p. 363.]

Even while granting the worst that can be said for the low temperature
of Mars, the persistent believer in its habitability could take refuge
in the results of recent experiments which have proved that bacterial
life is able to resist the utmost degree of cold that can be applied,
microscopic organisms perfectly retaining their vitality--or at least
their power to resume it--when subjected to the fearfully low
temperature of liquid air. But then he would be open to the reply that
the organisms thus treated are in a torpid condition and deprived of all
activity until revived by the application of heat; and the picture of a
world in a state of perpetual sleep is not particularly attractive,
unless the fortunate prince who is destined to awake the slumbering
beauty can also be introduced into the romance.[5]

[Footnote 5: Many of the present difficulties about temperatures on the
various planets would be beautifully disposed of if we could accept the
theory urged by Mr. Cope Whitehouse, to the effect that the sun is not
really a hot body at all, and that what we call solar light and heat are
only local manifestations produced in our atmosphere by the
transformation of some other form of energy transmitted from the sun;
very much as the electric impulses carried by a wire from the
transmitting to the receiving station on a telephone line are translated
by the receiver into waves of sound. According to this theory, which is
here mentioned only as an ingenuity and because something of the kind so
frequently turns up in one form or another in popular semi-scientific
literature, the amount of heat and light on a planet would depend mainly
upon local causes.]

To an extent which most of us, perhaps, do not fully appreciate, we are
indebted for many of the pleasures and conveniences and some of the
necessities of life on our planet to its faithful attendant, the moon.
Neither Mercury nor Venus has a moon, but Mars has two moons. This
statement, standing alone, might lead to the conclusion that, as far as
the advantages a satellite can afford to the inhabitants of its master
planet are concerned, the people of Mars are doubly fortunate. So they
would be, perhaps, if Mars's moons were bodies comparable in size with
our moon, but in fact they are hardly more than a pair of very
entertaining astronomical toys. The larger of the two, Phobos, is
believed to be about seven miles in diameter; the smaller, Deimos, only
five or six miles. Their dimensions thus resemble those of the more
minute of the asteroids, and the suggestion has even been made that they
may be captured asteroids which have fallen under the gravitational
control of Mars.

The diameters just mentioned are Professor Pickering's estimates, based
on the amount of light the little satellites reflect, for they are much
too small to present measurable disks. Deimos is 14,600 miles from the
center of Mars and 12,500 miles from its surface. Phobos is 5,800 miles
from the center of the planet and only 3,700 from the surface. Deimos
completes a revolution about the planet in thirty hours and eighteen
minutes, and Phobos in the astonishingly short period--although, of
course, it is in strict accord with the law of gravitation and in that
sense not astonishing--of seven hours and thirty-nine minutes.

Since Mars takes twenty-four hours and thirty-seven minutes for one
rotation on its axis, it is evident that Phobos goes round the planet
three times in the course of a single Martian day and night, rising,
contrary to the general motion of the heavens, in the west, running in a
few hours through all the phases that our moon exhibits in the course of
a month, and setting, where the sun and all the stars rise, in the east.
Deimos, on the other hand, has a period of revolution five or six hours
longer than that of the planet's axial rotation, so that it rises, like
the other heavenly bodies, in the east; but, because its motion is so
nearly equal, in angular velocity, to that of Mars's rotation, it shifts
very slowly through the sky toward the west, and for two or three
successive days and nights it remains above the horizon, the sun
overtaking and passing it again and again, while, in the meantime, its
protean face swiftly changes from full circle to half-moon, from
half-moon to crescent, from crescent back to half, and from half to
full, and so on without ceasing.

And during this time Phobos is rushing through the sky in the opposite
direction, as if in defiance of the fundamental law of celestial
revolution, making a complete circuit three times every twenty-four
hours, and changing the shape of its disk four times as rapidly as
Deimos does! Truly, if we were suddenly transported to Mars, we might
well believe that we had arrived in the mother world of lunatics, and
that its two moons were bewitched. Yet it must not be supposed that all
the peculiarities just mentioned would be clearly seen from the surface
of Mars by eyes like ours. The phases of Phobos would probably be
discernible to the naked eye, but those of Deimos would require a
telescope in order to be seen, for, notwithstanding their nearness to
the planet, Mars's moons are inconspicuous phenomena even to the
Martians themselves. Professor Young's estimate is that Phobos may shed
upon Mars one-sixtieth and Deimos one-twelve-hundredth as much reflected
moonlight as our moon sends to the earth. Accordingly, a "moonlit night"
on Mars can have no such charm as we associate with the phrase. But it
is surely a tribute to the power and perfection of our telescopes that
we have been able to discover the existence of objects so minute and
inconspicuous, situated at a distance of many millions of miles, and
half concealed by the glaring light of the planet close around which
they revolve.

If Mars's moons were as massive as our moon is they would raise
tremendous tides upon Mars, and would affect the circulation of water in
the canals, but, in fact, their tidal effects are even more
insignificant than their light-giving powers. But for astronomers on
Mars they would be objects of absorbing interest.

Upon quitting Mars we pass to the second distinctive planetary group of
the solar system, that of the asteroids.




CHAPTER V

THE ASTEROIDS, A FAMILY OF DWARF WORLDS


Beyond Mars, in the broad gap separating the terrestrial from the Jovian
planets, are the asteroids, of which nearly five hundred have been
discovered and designated by individual names or numbers. But any
statement concerning the known number of asteroids can remain valid for
but a short time, because new ones are continually found, especially by
the aid of photography. Very few of the asteroids are of measurable
size. Among these are the four that were the first to be
discovered--Ceres, Pallas, Juno, and Vesta. Their diameters, according
to the measurements of Prof. E.E. Barnard, of the Yerkes Observatory,
are as follows: Ceres, 477 miles; Pallas, 304 miles; Juno, 120 miles;
Vesta, 239 miles.

It is only necessary to mention these diameters in order to indicate how
wide is the difference between the asteroids and such planets as the
earth, Venus, or Mars. The entire surface of the largest asteroid,
Ceres, does not equal the republic of Mexico in area. But Ceres itself
is gigantic in comparison with the vast majority of the asteroids, many
of which, it is believed, do not exceed twenty miles in diameter, while
there may be hundreds or thousands of others still smaller--ten miles,
five miles, or perhaps only a few rods, in diameter!

Curiously enough, the asteroid which appears brightest, and which it
would naturally be inferred is the largest, really stands third in the
order of measured size. This is Vesta, whose diameter, according to
Barnard, is only 239 miles. It is estimated that the surface of Vesta
possesses about four times greater light-reflecting power than the
surface of Ceres. Some observations have also shown a variation in the
intensity of the light from Vesta, a most interesting fact, which
becomes still more significant when considered in connection with the
great variability of another most extraordinary member of the asteroidal
family, Eros, which is to be described presently.

The orbits of the asteroids are scattered over a zone about 200,000,000
miles broad. The mean distance from the sun of the nearest asteroid,
Eros, is 135,000,000 miles, and that of the most distant, Thule,
400,000,000 miles. Wide gaps exist in the asteroidal zone where few or
no members of the group are to be found, and Prof. Daniel Kirkwood long
ago demonstrated the influence of Jupiter in producing these gaps.
Almost no asteroids, as he showed, revolve at such a distance from the
sun that their periods of revolution are exactly commensurable with that
of Jupiter. Originally there may have been many thus situated, but the
attraction of the great planet has, in the course of time, swept those
zones clean.

Many of the asteroids have very eccentric orbits, and their orbits are
curiously intermixed, varying widely among themselves, both in
ellipticity and in inclination to the common plane of the solar system.

Considered with reference to the shape and position of its orbit, the
most unique of these little worlds is Eros, which was discovered in 1898
by De Witt, at Berlin, and which, on account of its occasional near
approach to the earth, has lately been utilized in a fresh attempt to
obtain a closer approximation to the true distance of the sun from the
earth. The mean distance of Eros from the sun is 135,000,000 miles, its
greatest distance is 166,000,000 miles, and its least distance
105,000,000 miles. It will thus be seen that, although all the other
asteroids are situated beyond Mars, Eros, at its mean distance, is
nearer to the sun than Mars is. When in aphelion, or at its greatest
distance, Eros is outside of the orbit of Mars, but when in perihelion
it is so much inside of Mars's orbit that it comes surprisingly near the
earth.

Indeed, there are times when Eros is nearer to the earth than any other
celestial body ever gets except the moon--and, it might be added,
except meteors and, by chance, a comet, or a comet's tail. Its least
possible distance from the earth is less than 14,000,000 miles, and it
was nearly as close as that, without anybody knowing or suspecting the
fact, in 1894, four years in advance of its discovery. Yet the fact,
strange as the statement may seem, had been recorded without being
recognized. After De Witt's discovery of Eros in 1898, at a time when it
was by no means as near the earth as it had been some years before,
Prof. E.C. Pickering ascertained that it had several times imprinted its
image on the photographic plates of the Harvard Observatory, with which
pictures of the sky are systematically taken, but had remained
unnoticed, or had been taken for an ordinary star among the thousands of
star images surrounding it. From these telltale plates it was
ascertained that in 1894 it had been in perihelion very near the earth,
and had shone with the brilliance of a seventh-magnitude star.

It will, unfortunately, be a long time before Eros comes quite as near
us as it did on that occasion, when we failed to see it, for its close
approaches to the earth are not frequent. Prof. Solon I. Bailey selects
the oppositions of Eros in 1931 and 1938 as probably the most favorable
that will occur during the first half of the twentieth century.

We turn to the extraordinary fluctuations in the light of Eros, and the
equally extraordinary conclusions drawn from them. While the little
asteroid, whose diameter is estimated to be in the neighborhood of
twenty or twenty-five miles, was being assiduously watched and
photographed during its opposition in the winter of 1900-1901, several
observers discovered that its light was variable to the extent of more
than a whole magnitude; some said as much as two magnitudes. When it is
remembered that an increase of one stellar magnitude means an accession
of light in the ratio of 2.5 to 1, and an increase of two magnitudes an
accession of 6.25 to 1, the significance of such variations as Eros
exhibited becomes immediately apparent. The shortness of the period
within which the cycle of changes occurred, about two hours and a half,
made the variation more noticeable, and at the same time suggested a
ready explanation, viz., that the asteroid was rapidly turning on its
axis, a thing, in itself, quite in accordance with the behavior of other
celestial bodies and naturally to be expected.

But careful observation showed that there were marked irregularities in
the light fluctuations, indicating that Eros either had a very strange
distribution of light and dark areas covering its surface, or that
instead of being a globular body it was of some extremely irregular
shape, so that as it rotated it presented successively larger and
smaller reflecting surfaces toward the sun and the earth. One
interesting suggestion was that the little planet is in reality double,
the two components revolving around their common center of gravity, like
a close binary star, and mutually eclipsing one another. But this theory
seems hardly competent to explain the very great fluctuation in light,
and a better one, probably, is that suggested by Prof. E.C. Pickering,
that Eros is shaped something like a dumb-bell.

We can picture such a mass, in imagination, tumbling end over end in its
orbit so as to present at one moment the broad sides of both bells,
together with their connecting neck, toward the sun, and, at the same
time, toward the observer on the earth, and, at another moment, only the
end of one of the bells, the other bell and the neck being concealed in
shadow. In this way the successive gain and loss of sixfold in the
amount of light might be accounted for. Owing to the great distance the
real form of the asteroid is imperceptible even with powerful
telescopes, but the effect of a change in the amount of reflecting
surface presented produces, necessarily, an alternate waxing and waning
of the light. As far as the fluctuations are concerned, they might also
be explained by supposing that the shape of the asteroid is that of a
flat disk, rotating about one of its larger diameters so as to present,
alternately, its edge and its broadside to the sun. And, perhaps, in
order completely to account for all the observed eccentricities of the
light of Eros, the irregularity of form may have to be supplemented by
certain assumptions as to the varying reflective capacity of different
parts of the misshapen mass.

The invaluable Harvard photographs show that long before Eros was
recognized as an asteroid its light variations had been automatically
registered on the plates. Some of the plates, Prof. E.C. Pickering says,
had had an exposure of an hour or more, and, owing to its motion, Eros
had formed a trail on each of these plates, which in some cases showed
distinct variations in brightness. Differences in the amount of
variation at different times will largely depend upon the position of
the earth with respect to the axis of rotation.

Another interesting deduction may be made from the changes that the
light of Eros undergoes. We have already remarked that one of the larger
asteroids, and the one which appears to the eye as the most brilliant
of all, Vesta, has been suspected of variability, but not so extensive
as that of Eros. Olbers, at the beginning of the last century, was of
the opinion that Vesta's variations were due to its being not a globe
but an angular mass. So he was led by a similar phenomenon to precisely
the same opinion about Vesta that has lately been put forth concerning
Eros. The importance of this coincidence is that it tends to revive a
remarkable theory of the origin of the asteroids which has long been in
abeyance, and, in the minds of many, perhaps discredited.

This theory, which is due to Olbers, begins with the startling
assumption that a planet, perhaps as large as Mars, formerly revolving
in an orbit situated between the orbits of Mars and Jupiter, was
destroyed by an explosion! Although, at first glance, such a catastrophe
may appear too wildly improbable for belief, yet it was not the
improbability of a world's blowing up that led to a temporary
abandonment of Olbers's bold theory. The great French mathematician
Lagrange investigated the explosive force "which would be necessary to
detach a fragment of matter from a planet revolving at a given distance
from the sun," and published the results in the Connaissance des Temps
for 1814.

"Applying his results to the earth, Lagrange found that if the velocity
of the detached fragment exceeded that of a cannon ball in the
proportion of 121 to 1 the fragment would become a comet with a direct
motion; but if the velocity rose in the proportion of 156 to 1 the
motion of the comet would be retrograde. If the velocity was less than
in either of these cases the fragment would revolve as a planet in an
elliptic orbit. For any other planet besides the earth the velocity of
explosion corresponding to the different cases would vary in the inverse
ratio of the square root of the mean distance. It would therefore
manifestly be less as the planet was more distant from the sun. In the
case of each of the four smaller planets (only the four asteroids,
Ceres, Pallas, Juno, and Vesta, were known at that time), the velocity
of explosion indicated by their observed motion would be less than
twenty times the velocity of a cannon ball."[6]

[Footnote 6: Grant's History of Physical Astronomy, p. 241.]

Instead, then, of being discredited by its assumption of so strange a
catastrophe, Olbers's theory fell into desuetude because of its apparent
failure to account for the position of the orbits of many of the
asteroids after a large number of those bodies had been discovered. He
calculated that the orbits of all the fragments of his exploded planet
would have nearly equal mean distances, and a common point of
intersection in the heavens, through which every fragment of the
original mass would necessarily pass in each revolution. At first the
orbits of the asteroids discovered seemed to answer to these conditions,
and Olbers was even able to use his theory as a means of predicting the
position of yet undetected asteroids. Only Ceres and Pallas had been
discovered when he put forth his theory, but when Juno and Vesta were
found they fell in with his predictions so well that the theory was
generally regarded as being virtually established; while the
fluctuations in the light of Vesta, as we have before remarked, led
Olbers to assert that that body was of a fragmental shape, thus strongly
supporting his explosion hypothesis.

Afterward, when the orbits of many asteroids had been investigated, the
soundness of Olbers's theory began to be questioned. The fact that the
orbits did not all intersect at a common point could easily be disposed
of, as Professor Newcomb has pointed out, by simply placing the date of
the explosion sufficiently far back, say millions of years ago, for the
secular changes produced by the attraction of the larger planets would
effectively mix up the orbits. But when the actual effects of these
secular changes were calculated for particular asteroids the result
seemed to show that "the orbits could never have intersected unless some
of them have in the meantime been altered by the attraction of the
small planets on each other. Such an action is not impossible, but it is
impossible to determine it, owing to the great number of these bodies
and our ignorance of their masses."[7]

[Footnote 7: Popular Astronomy, by Simon Newcomb, p. 335.]

Yet the theory has never been entirely thrown out, and now that the
discovery of the light fluctuations of Eros lends support to Olbers's
assertion of the irregular shape of some of the asteroids, it is very
interesting to recall what so high an authority as Professor Young said
on the subject before the discovery of Eros:

"It is true, as has often been urged, that this theory in its original
form, as presented by Olbers, can not be correct. No _single_ explosion
of a planet could give rise to the present assemblage of orbits, nor is
it possible that even the perturbations of Jupiter could have converted
a set of orbits originally all crossing at one point (the point of
explosion) into the present tangle. The smaller orbits are so small
that, however turned about, they lie wholly inside the larger and can
not be made to intersect them. If, however, we admit a _series_ of
explosions, this difficulty is removed; and if we grant an explosion at
all, there seems to be nothing improbable in the hypothesis that the
fragments formed by the bursting of the parent mass would carry away
within themselves the same forces and reactions which caused the
original bursting, so that they themselves would be likely enough to
explode at some time in their later history."[8]

[Footnote 8: General Astronomy, by Charles A. Young. Revised edition,
1898, p. 372.]

The rival theory of the origin of the asteroids is that which assumes
that the planetary ring originally left off from the contracting solar
nebula between the orbits of Mars and Jupiter was so violently perturbed
by the attraction of the latter planet that, instead of being shaped
into a single globe, it was broken up into many fragments. Either
hypothesis presents an attractive picture; but that which presupposes
the bursting asunder of a large planet, which might at least have borne
the germs of life, and the subsequent shattering of its parts into
smaller fragments, like the secondary explosions of the pieces of a
pyrotechnic bomb, certainly is by far the more impressive in its appeal
to the imagination, and would seem to offer excellent material for some
of the extra-terrestrial romances now so popular. It is a startling
thought that a world can possibly carry within itself, like a dynamite
cartridge, the means of its own disruption; but the idea does not appear
so extremely improbable when we recall the evidence of collisions or
explosions, happening on a tremendous scale, in the case of new or
temporary stars.[9]

[Footnote 9: "Since the discovery of Eros, the extraordinary position of
its orbit has led to the suggestion that possibly Mars itself, instead
of being regarded as primarily a major planet, belonging to the
terrestrial group, ought rather to be considered as the greatest of the
asteroids, and a part of the original body from which the asteroidal
system was formed."--J. Bauschinger, Astronomische Nachrichten, No.
3542.]

Coming to the question of life upon the asteroids, it seems clear that
they must be excluded from the list of habitable worlds, whatever we
may choose to think of the possible habitability of the original planet
through whose destruction they may have come into existence. The largest
of them possesses a force of gravity far too slight to enable it to
retain any of the gases or vapors that are recognized as constituting an
atmosphere. But they afford a captivating field for speculation, which
need not be altogether avoided, for it offers some graphic illustrations
of the law of gravitation. A few years ago I wrote, for the
entertainment of an audience which preferred to meet science attired in
a garb woven largely from the strands of fancy, an account of some of
the peculiarities of such minute globes as the asteroids, which I
reproduce here because it gives, perhaps, a livelier picture of those
little bodies, from the point of view of ordinary human interest, than
could be presented in any other way.


A WAIF OF SPACE

One night as I was waiting, watch in hand, for an occultation, and
striving hard to keep awake, for it had been a hot and exhausting
summer's day, while my wife--we were then in our honeymoon--sat
sympathetically by my side, I suddenly found myself withdrawn from the
telescope, and standing in a place that appeared entirely strange. It
was a very smooth bit of ground, and, to my surprise, there was no
horizon in sight; that is to say, the surface of the ground disappeared
on all sides at a short distance off, and beyond nothing but sky was
visible. I thought I must be on the top of a stupendous mountain, and
yet I was puzzled to understand how the face of the earth could be so
far withdrawn. Presently I became aware that there was some one by me
whom I could not see.

"You are not on a mountain," my companion said, and as he spoke a cold
shiver ran along my back-bone; "you are on an asteroid, one of those
miniature planets, as you astronomers call them, and of which you have
discovered several hundred revolving between the orbits of Mars and
Jupiter. This is the little globe that you have glimpsed occasionally
with your telescope, and that you, or some of your fellows, have been
kind enough to name Menippe."

Then I perceived that my companion, whose address had hardly been
reassuring, was a gigantic inhabitant of the little planet, towering up
to a height of three quarters of a mile. For a moment I was highly
amused, standing by his foot, which swelled up like a hill, and
straining my neck backward to get a look up along the precipice of his
leg, which, curiously enough, I observed was clothed in rough homespun,
the woolly knots of the cloth appearing of tremendous size, while it
bagged at the knee like any terrestrial trousers' leg. His great head
and face I could see far above me, as it were, in the clouds. Yet I was
not at all astonished.

"This is all right," I said to myself. "Of course on Menippe the people
must be as large as this, for the little planet is only a dozen miles
in diameter, and the force of gravity is consequently so small that a
man without loss of activity, or inconvenience, can grow three quarters
of a mile tall."

Suddenly an idea occurred to me. "Just to think what a jump I can make!
Why, only the other day I was figuring it out that a man could easily
jump a thousand feet high from the surface of Menippe, and now here I
actually am on Menippe. I'll jump."

The sensation of that glorious rise skyward was delightful beyond
expression. My legs seemed to have become as powerful as the engines of
a transatlantic liner, and with one spring I rose smoothly and swiftly,
and as straight as an arrow, surmounting the giant's foot, passing his
knee and attaining nearly to the level of his hip. Then I felt that the
momentum of my leap was exhausted, and despite my efforts I slowly
turned head downward, glancing in affright at the ground a quarter of a
mile below me, on which I expected to be dashed to pieces. But a
moment's thought convinced me that I should get no hurt, for with so
slight a force of gravity it would be more like floating than falling.
Just then the Menippean caught me with his monstrous hand and lifted me
to the level of his face.

"I should like to know," I said, "how you manage to live up here; you
are so large and your planet is so little."

"Now, you are altogether too inquisitive," replied the giant. "You go!"

He stooped down, placed me on the toe of his boot, and drew back his
foot to kick me off.

It flashed into my mind that my situation had now become very serious. I
knew well what the effects of the small attractive force of these
diminutive planets must be, for I had often amused myself with
calculations about them. In this moment of peril I did not forget my
mathematics. It was clear that if the giant propelled me with sufficient
velocity I should be shot into space, never to return. How great would
that velocity have to be? My mind worked like lightning on this problem.
The diameter of Menippe I knew did not exceed twelve miles. Its mean
density, as near as I could judge, was about the same as that of the
earth. Its attraction must therefore be as its radius, or nearly 660
times less than that of the earth. A well-known formula enables us to
compute the velocity a body would acquire in falling from an infinite
distance to the earth or any other planet whose size and force of
gravity are known. The same formula, taken in the opposite sense, of
course, shows how fast a body must start from a planet in order that it
may be freed from its control. The formula is V = square root of (2
gr.), in which "g" is the acceleration of gravity, equal for the earth
to 32 feet in a second, and "r" is the radius of the attracting body. On
Menippe I knew "g" must equal about one twentieth of a foot, and "r"
31,680 feet. Like a flash I applied the formula while the giant's
muscles were yet tightening for the kick: 31,680 × 1/20 × 2 = 3,168, the
square root of which is a fraction more than 56. Fifty-six feet in a
second, then, was the critical velocity with which I must be kicked off
in order that I might never return. I perceived at once that the giant
would be able to accomplish it. I turned and shouted up at him:

"Hold on, I have something to say to you!"

I dimly saw his mountainous face puckered into mighty wrinkles, out of
which his eyes glared fiercely, and the next moment I was sailing into
space. I could no more have kept a balance than the earth can stand
still upon its axis. I had become a small planet myself, and, like all
planets, I rotated. Yet the motion did not dizzy me, and soon I became
intensely interested in the panorama of creation that was spread around
me. For some time, whenever my face was turned toward the little globe
of Menippe, I saw the giant, partly in profile against the sky, with his
back bent and his hands upon his knees, watching me with an occasional
approving nod of his big head. He looked so funny standing there on his
little seven-by-nine world, like a clown on a performing ball, that,
despite my terrible situation, I shook my sides with laughter. There was
no echo in the profundity of empty space.

Soon Menippe dwindled to a point, and I saw her inhospitable inhabitant
no more. Then I watched the sun and the blazing firmament around, for
there was at the same time broad day and midnight for me. The sunlight,
being no longer diffused by an atmosphere, did not conceal the face of
the sky, and I could see the stars shining close to the orb of day. I
recognized the various planets much more easily than I had been
accustomed to do, and, with a twinge at my heart, saw the earth
traveling along in its distant orbit, splendid in the sunshine. I
thought of my wife sitting alone by the telescope in the darkness and
silence, wondering what had become of me. I asked myself, "How in the
world can I ever get back there again?" Then I smiled to think of the
ridiculous figure I cut, out here in space, exposed to the eyes of the
universe, a rotating, gyrating, circumambulating astronomer, an
animated teetotum lost in the sky. I saw no reason to hope that I should
not go on thus forever, revolving around the sun until my bones,
whitening among the stars, might be revealed to the superlative powers
of some future telescope, and become a subject of absorbing interest,
the topic of many a learned paper for the astronomers of a future age.
Afterward I was comforted by the reflection that in airless space,
although I might die and my body become desiccated, yet there could be
no real decay; even my garments would probably last forever. The
_savants_, after all, should never speculate on my bones.

I saw the ruddy disk of Mars, and the glinting of his icy poles, as the
beautiful planet rolled far below me. "If I could only get there," I
thought, "I should know what those canals of Schiaparelli are, and even
if I could never return to the earth, I should doubtless meet with a
warm welcome among the Martians. What a lion I should be!" I looked
longingly at the distant planet, the outlines of whose continents and
seas appeared most enticing, but when I tried to propel myself in that
direction I only kicked against nothingness. I groaned in desperation.

Suddenly something darted by me flying sunward; then another and
another. In a minute I was surrounded by strange projectiles. Every
instant I expected to be dashed in pieces by them. They sped with the
velocity of lightning. Hundreds, thousands of them were all about me. My
chance of not being hit was not one in a million, and yet I escaped. The
sweat of terror was upon me, but I did not lose my head. "A comet has
met me," I said. "These missiles are the meteoric stones of which it is
composed." And now I noticed that as they rushed along collisions took
place, and flashes of electricity darted from one to another. A pale
luminosity dimmed the stars. I did not doubt that, as seen from the
earth, the comet was already flinging the splendors of its train upon
the bosom of the night.

While I was wondering at my immunity amid such a rain of
death-threatening bolts, I became aware that their velocity was sensibly
diminishing. This fact I explained by supposing that I was drawn along
with them. Notwithstanding the absence of any collision with my body,
the overpowering attraction of the whole mass of meteors was overcoming
my tangential force and bearing me in their direction. At first I
rejoiced at this circumstance, for at any rate the comet would save me
from the dreadful fate of becoming an asteroid. A little further
reflection, however, showed me that I had gone from the frying-pan into
the fire. The direction of my expulsion from Menippe had been such that
I had fallen into an orbit that would have carried me around the sun
without passing very close to the solar body. Now, being swept along by
the comet, whose perihelion probably lay in the immediate neighborhood
of the sun, I saw no way of escape from the frightful fate of being
broiled alive. Even where I was, the untempered rays of the sun scorched
me, and I knew that within two or three hundred thousand miles of the
solar surface the heat must be sufficient to melt the hardest rocks. I
was aware that experiments with burning-glasses had sufficiently
demonstrated that fact.

But perforce I resigned myself to my fate. At any rate it would the
sooner be all over. In fact, I almost forgot my awful situation in the
interest awakened by the phenomena of the comet. I was in the midst of
its very head. I was one of its component particles. I was a meteor
among a million millions of others. If I could only get back to the
earth, what news could I not carry to Signor Schiaparelli and Mr.
Lockyer and Dr. Bredichin about the composition of comets! But, alas!
the world could never know what I now saw. Nobody on yonder gleaming
earth, watching the magnificent advance of this "specter of the skies,"
would ever dream that there was a lost astronomer in its blazing head. I
should be burned and rent to pieces amid the terrors of its perihelion
passage, and my fragments would be strewn along the comet's orbit, to
become, in course of time, particles in a swarm of aerolites. Perchance,
through the effects of some unforeseen perturbation, the earth might
encounter that swarm. Thus only could I ever return to the bosom of my
mother planet. I took a positive pleasure in imagining that one of my
calcined bones might eventually flash for a moment, a falling star, in
the atmosphere of the earth, leaving its atoms to slowly settle through
the air, until finally they rested in the soil from which they had
sprung.

From such reflections I was aroused by the approach of the crisis. The
head of the comet had become an exceedingly uncomfortable place. The
collisions among the meteors were constantly increasing in number and
violence. How I escaped destruction I could not comprehend, but in fact
I was unconscious of danger from that source. I had become in spirit an
actual component of the clashing, roaring mass. Tremendous sparks of
electricity, veritable lightning strokes, darted about me in every
direction, but I bore a charmed life. As the comet drew in nearer to
the sun, under the terrible stress of the solar attraction, the meteors
seemed to crowd closer, crashing and grinding together, while the whole
mass swayed and shrieked with the uproar of a million tormented devils.
The heat had become terrific. I saw stone and iron melted like snow and
dissipated in steam. Stupendous jets of white-hot vapor shot upward,
and, driven off by the electrical repulsion of the sun, streamed
backward into the tail.

Suddenly I myself became sensible of the awful heat. It seemed without
warning to have penetrated my vitals. With a yell I jerked my feet from
a boiling rock and flung my arms despairingly over my head.

"You had better be careful," said my wife, "or you'll knock over the
telescope."

I rubbed my eyes, shook myself, and rose.

"I must have been dreaming," I said.

"I should think it was a very lively dream," she replied.

I responded after the manner of a young man newly wed.

At this moment the occultation began.




CHAPTER VI

JUPITER, THE GREATEST OF KNOWN WORLDS


When we are thinking of worlds, and trying to exalt the imagination with
them, it is well to turn to Jupiter, for there is a planet worth
pondering upon! A world thirteen hundred times as voluminous as the
earth is a phenomenon calculated to make us feel somewhat as the
inhabitant of a rural village does when his amazed vision ranges across
the million roofs of a metropolis. Jupiter is the first of the outer and
greater planets, the major, or Jovian, group. His mean diameter is
86,500 miles, and his average girth more than 270,000 miles. An
inhabitant of Jupiter, in making a trip around his planet, along any
great circle of the sphere, would have to travel more than 30,000 miles
farther than the distance between the earth and the moon. The polar
compression of Jupiter, owing to his rapid rotation, amounts in the
aggregate to more than 5,000 miles, the equatorial diameter being 88,200
miles and the polar diameter 83,000 miles.

Jupiter's mean distance from the sun is 483,000,000 miles, and the
eccentricity of his orbit is sufficient to make this distance variable
to the extent of 21,000,000 miles; but, in view of his great average
distance, the consequent variation in the amount of solar light and heat
received by the planet is not of serious importance.

When he is in opposition to the sun as seen from the earth Jupiter's
mean distance from us is about 390,000,000 miles. His year, or period of
revolution about the sun, is somewhat less than twelve of our years
(11.86 years). His axis is very nearly upright to the plane of his
orbit, so that, as upon Venus, there is practically no variation of
seasons. Gigantic though he is in dimensions, Jupiter is the swiftest of
all the planets in axial rotation. While the earth requires twenty-four
hours to make a complete turn, Jupiter takes less than ten hours (nine
hours fifty-five minutes), and a point on his equator moves, in
consequence of axial rotation, between 27,000 and 28,000 miles in an
hour.

The density of the mighty planet is slight, only about one quarter of
the mean density of the earth and virtually the same as that of the sun.
This fact at once calls attention to a contrast between Jupiter and our
globe that is even more significant than their immense difference in
size. The force of gravity upon Jupiter's surface is more than two and a
half times greater than upon the earth's surface (more accurately 2.65
times), so that a hundred-pound weight removed from the planet on which
we live to Jupiter would there weigh 265 pounds, and an average man,
similarly transported, would be oppressed with a weight of at least 400
pounds. But, as a result of the rapid rotation of the great planet, and
the ellipticity of its figure, the unfortunate visitor could find a
perceptible relief from his troublesome weight by seeking the planet's
equator, where the centrifugal tendency would remove about twenty pounds
from every one hundred as compared with his weight at the poles.

If we could go to the moon, or to Mercury, Venus, or Mars, we may be
certain that upon reaching any of those globes we should find ourselves
upon a solid surface, probably composed of rock not unlike the rocky
crust of the earth; but with Jupiter the case would evidently be very
different. As already remarked, the mean density of that planet is only
one quarter of the earth's density, or only one third greater than the
density of water. Consequently the visitor, in attempting to set foot
upon Jupiter, might find no solid supporting surface, but would be in a
situation as embarrassing as that of Milton's Satan when he undertook to
cross the domain of Chaos:

    "Fluttering his pinions vain, plumb down he drops,
    Ten thousand fathom deep, and to this hour
    Down had been falling had not, by ill chance,
    The strong rebuff of some tumultuous cloud.
    Instinct with fire and niter, hurried him
    As many miles aloft; that fury stayed,
    Quenched in a boggy Syrtis, neither sea
    Nor good dry land, nigh foundered, as he fares,
    Treading the crude consistence, half on foot,
    Half flying."

The probability that nothing resembling a solid crust, nor, perhaps,
even a liquid shell, would be found at the visible surface of Jupiter,
is increased by considering that the surface density must be much less
than the mean density of the planet taken as a whole, and since the
latter but little exceeds the density of water, it is likely that at the
surface everything is in a state resembling that of cloud or smoke. Our
imaginary visitor upon reaching Jupiter would, under the influence of
the planet's strong force of gravity, drop out of sight, with the speed
of a shot, swallowed up in the vast atmosphere of probably hot, and
perhaps partially incandescent, gases. When he had sunk--supposing his
identity could be preserved--to a depth of thousands of miles he might
not yet have found any solid part of the planet; and, perchance, there
is no solid nucleus even at the very center.

The cloudy aspect of Jupiter immediately strikes the telescopic
observer. The huge planet is filled with color, and with the animation
of constant movement, but there is no appearance of markings, like those
on Mars, recalling the look of the earth. There are no white polar caps,
and no shadings that suggest the outlines of continents and oceans. What
every observer, even with the smallest telescope, perceives at once is a
pair of strongly defined dark belts, one on either side of, and both
parallel to, the planet's equator. These belts are dark compared with
the equatorial band between them and with the general surface of the
planet toward the north and the south, but they are not of a gray or
neutral shade. On the contrary, they show decided, and, at times,
brilliant colors, usually of a reddish tone. More delicate tints,
sometimes a fine pink, salmon, or even light green, are occasionally to
be seen about the equatorial zone, and the borders of the belts, while
near the poles the surface is shadowed with bluish gray, imperceptibly
deepening from the lighter hues of the equator.

All this variety of tone and color makes of a telescopic view of Jupiter
a picture that will not quickly fade from the memory; while if an
instrument of considerable power is used, so that the wonderful details
of the belts, with their scalloped edges, their diagonal filaments,
their many divisions, and their curious light and dark spots, are made
plain, the observer is deeply impressed with the strangeness of the
spectacle, and the more so as he reflects upon the enormous real
magnitude of that which is spread before his eye. The whole earth
flattened out would be but a small blotch on that gigantic disk!

Then, the visible rotation of the great Jovian globe, whose effects
become evident to a practised eye after but a few minutes' watching,
heightens the impression. And the presence of the four satellites, whose
motions in their orbits are also evident, through the change in their
positions, during the course of a single not prolonged observation,
adds its influence to the effectiveness of the scene. Indeed, color and
motion are so conspicuous in the immense spectacle presented by Jupiter
that they impart to it a powerful suggestion of life, which the mind
does not readily divest itself of when compelled to face the evidence
that Jupiter is as widely different from the earth, and as diametrically
opposed to lifelike conditions, as we comprehend them, as a planet
possibly could be.

The great belts lie in latitudes about corresponding to those in which
the trade-winds blow upon the earth, and it has often been suggested
that their existence indicates a similarity between the atmospheric
circulation of Jupiter and that of the world in which we live. No doubt
there are times when the earth, seen with a telescope from a distant
planet, would present a belted appearance somewhat resembling that of
Jupiter, but there would almost certainly be no similar display of
colors in the clouds, and the latter would exhibit no such persistence
in general form and position as characterizes those of Jupiter. Our
clouds are formed by the action of the sun, producing evaporation of
water; on Jupiter, whose mean distance from the sun is more than five
times as great as ours, the intensity of the solar rays is reduced to
less than one twenty-fifth part of their intensity on the earth, so that
the evaporation can not be equally active there, and the tendency to
form aerial currents and great systems of winds must be proportionally
slight. In brief, the clouds of Jupiter are probably of an entirely
different origin from that of terrestrial clouds, and rather resemble
the chaotic masses of vapor that enveloped the earth when it was still
in a seminebulous condition, and before its crust had formed.

Although the strongest features of the disk of Jupiter are the great
cloud belts, and the white or colored spots in the equatorial zone, yet
the telescope shows many markings north and south of the belts,
including a number of narrower and fainter belts, and small light or
dark spots. None of them is absolutely fixed in position with
reference to others. In other words, all of the spots, belts, and
markings shift their places to a perceptible extent, the changes being
generally very slow and regular, but occasionally quite rapid. The main
belts never entirely disappear, and never depart very far from their
mean positions with respect to the equator, but the smaller belts toward
the north and south are more or less evanescent. Round or oblong spots,
as distinguished from belts, are still more variable and transient. The
main belts themselves show great internal commotion, frequently
splitting up, through a considerable part of their length, and sometimes
apparently throwing out projections into the lighter equatorial zone,
which occasionally resemble bridges, diagonally spanning the broad space
between the belts.

[Illustration: JUPITER AS SEEN AT THE LICK OBSERVATORY IN 1889. THE
GREAT RED SPOT IS VISIBLE, TOGETHER WITH THE INDENTATION IN THE SOUTH
BELT.]

Perhaps the most puzzling phenomenon that has ever made its appearance
on Jupiter is the celebrated "great red spot," which was first noticed
in 1878, although it has since been shown to be probably identical with
a similar spot seen in 1869, and possibly with one noticed in 1857.
This spot, soon after its discovery in 1878, became a clearly defined
red oval, lying near the southern edge of the south belt in latitude
about 30°. Its length was nearly one third of the diameter of the disk
and its width almost one quarter as great as its length. Translated into
terrestrial measure, it was about 30,000 miles long and 7,000 miles
broad.

In 1879 it seemed to deepen in color until it became a truly wonderful
object, its redness of hue irresistibly suggesting the idea that it was
something hot and glowing. During the following years it underwent
various changes of appearance, now fading almost to invisibility and now
brightening again, but without ever completely vanishing, and it is
still (1901) faintly visible.

Nobody has yet suggested an altogether probable and acceptable theory as
to its nature. Some have said that it might be a part of the red-hot
crust of the planet elevated above the level of the clouds; others that
its appearance might be due to the clearing off of the clouds above a
heated region of the globe beneath, rendering the latter visible through
the opening; others that it was perhaps a mass of smoke and vapor
ejected from a gigantic volcano, or from the vents covering a broad area
of volcanic action; others that it might be a vast incandescent slag
floating upon the molten globe of the planet and visible through, or
above, the enveloping clouds; and others have thought that it could be
nothing but a cloud among clouds, differing, for unknown reasons, in
composition and cohesion from its surroundings. All of these hypotheses
except the last imply the existence, just beneath the visible cloud
shell, of a more or less stable and continuous surface, either solid or
liquid.

When the red spot began to lose distinctness a kind of veil seemed to be
drawn over it, as if light clouds, floating at a superior elevation, had
drifted across it. At times it has been reduced in this manner to a
faint oval ring, the rim remaining visible after the central part has
faded from sight.

One of the most remarkable phenomena connected with the mysterious spot
is a great bend, or scallop, in the southern edge of the south belt
adjacent to the spot. This looks as if it were produced by the spot, or
by the same cause to which the spot owes its existence. If the spot were
an immense mountainous elevation, and the belt a current of liquid, or
of clouds, flowing past its base, one would expect to see some such bend
in the stream. The visual evidence that the belt is driven, or forced,
away from the neighborhood of the spot seems complete. The appearance of
repulsion between them is very striking, and even when the spot fades
nearly to invisibility the curve remains equally distinct, so that in
using a telescope too small to reveal the spot itself one may discover
its location by observing the bow in the south belt. The suggestion of a
resemblance to the flowing of a stream past the foot of an elevated
promontory, or mountain, is strengthened by the fact, which was
observed early in the history of the spot, that markings involved in the
south belt have a quicker rate of rotation about the planet's axis than
that of the red spot, so that such markings, first seen in the rear of
the red spot, gradually overtake and pass it, and eventually leave it
behind, as boats in a river drift past a rock lying in the midst of the
current.

This leads us to another significant fact concerning the peculiar
condition of Jupiter's surface. Not only does the south belt move
perceptibly faster than the red spot, but, generally speaking, the
various markings on the surface of the planet move at different rates
according as they are nearer to or farther from the equator. Between the
equator and latitude 30° or 40° there is a difference of six minutes in
the rotation period--i.e., the equatorial parts turn round the axis so
much faster than the parts north and south of them, that in one rotation
they gain six minutes of time. In other words, the clouds over Jupiter's
equator flow past those in the middle latitudes with a relative
velocity of 270 miles per hour. But there are no sharp lines of
separation between the different velocities; on the contrary, the
swiftness of rotation gradually diminishes from the equator toward the
poles, as it manifestly could not do if the visible surface of Jupiter
were solid.

In this respect Jupiter resembles the sun, whose surface also has
different rates of rotation diminishing from the equator. Measured by
the motion of spots on or near the equator, Jupiter's rotation period is
about nine hours fifty minutes; measured by the motion of spots in the
middle latitudes, it is about nine hours fifty-six minutes. The red spot
completes a rotation in a little less than nine hours and fifty-six
minutes, but its period can not be positively given for the singular
reason that it is variable. The variation amounts to only a few seconds
in the course of several years, but it is nevertheless certain. The
phenomenon of variable motion is not, however, peculiar to the red spot.
Mr. W.F. Denning, who has studied Jupiter for a quarter of a century,
says:

"It is well known that in different latitudes of Jupiter there are
currents, forming the belts and zones, moving at various rates of speed.
In many instances the velocity changes from year to year. And it is a
singular circumstance that in the same current a uniform motion is not
maintained in all parts of the circumference. Certain spots move faster
than others, so that if we would obtain a fair value for the rotation
period of any current it is not sufficient to derive it from one marking
alone; we must follow a number of objects distributed in different
longitudes along the current and deduce a mean from the whole."[10]

[Footnote 10: The Observatory, No. 286, December, 1899.]

Nor is this all. Observation indicates that if we could look at a
vertical section of Jupiter's atmosphere we should behold an equally
remarkable contrast and conflict of motions. There is evidence that some
of the visible spots, or clouds, lie at a greater elevation than others,
and it has been observed that the deeper ones move more rapidly. This
fact has led some observers to conclude that the deep-lying spots may be
a part of the actual surface of the planet. But if we could think that
there is any solid nucleus, or core, in the body of Jupiter, it would
seem, on account of the slight mean density of the planet, that it can
not lie so near the visible surface, but must be at a depth of
thousands, perhaps tens of thousands, of miles. Since the telescope is
unable to penetrate the cloudy envelope we can only guess at the actual
constitution of the interior of Jupiter's globe. In a spirit of mere
speculative curiosity it has been suggested that deep under the clouds
of the great planet there may be a comparatively small solid globe, even
a habitable world, closed round by a firmament all its own, whose vault,
raised 30,000 or 40,000 miles above the surface of the imprisoned
planet, appears only an unbroken dome, too distant to reveal its real
nature to watchers below, except, perhaps, under telescopic scrutiny;
enclosing, as in a shell, a transparent atmosphere, and deriving its
illumination partly from the sunlight that may filter through, but
mainly from some luminous source within.

But is not Jupiter almost equally fascinating to the imagination, if we
dismiss all attempts to picture a humanly impossible world shut up
within it, and turn rather to consider what its future may be, guided by
the not unreasonable hypothesis that, because of its immense size and
mass, it is still in a chaotic condition? Mention has been made of the
resemblance of Jupiter to the sun by virtue of their similar manner of
rotation. This is not the only reason for looking upon Jupiter as being,
in some respects, almost as much a solar as a planetary body. Its
exceptional brightness rather favors the view that a small part of the
light by which it shines comes from its own incandescence. In size and
mass it is half-way between the earth and the sun. Jupiter is eleven
times greater than the earth in diameter and thirteen hundred times
greater in volume; the sun is ten times greater than Jupiter in diameter
and a thousand times greater in volume. The mean density of Jupiter, as
we have seen, is almost exactly the same as the sun's.

Now, the history of the solar system, according to the nebular
hypothesis, is a history of cooling and condensation. The sun, a
thousand times larger than Jupiter, has not yet sufficiently cooled and
contracted to become incrusted, except with a shell of incandescent
metallic clouds; Jupiter, a thousand times smaller than the sun, has
cooled and contracted until it is but slightly, if at all, incandescent
at its surface, while its thickening shell, although still composed of
vapor and smoke, and still probably hot, has grown so dense that it
entirely cuts off the luminous radiation from within; the earth, to
carry the comparison one step further, being more than a thousand times
smaller than Jupiter, has progressed so far in the process of cooling
that its original shell of vapor has given place to one of solid rock.

A sudden outburst of light from Jupiter, such as occurs occasionally in
a star that is losing its radiance through the condensation of
absorbing vapors around it, would furnish strong corroboration of the
theory that Jupiter is really an extinguished sun which is now on the
way to become a planet in the terrestrial sense.

Not very long ago, as time is reckoned in astronomy, our sun, viewed
from the distance of the nearer fixed stars, may have appeared as a
binary star, the brighter component of the pair being the sun itself and
the fainter one the body now called the planet Jupiter. Supposing the
latter to have had the same intrinsic brilliance, surface for surface,
as the sun, it would have radiated one hundred times less light than the
sun. A difference of one hundredfold between the light of two stars
means that they are six magnitudes apart; or, in other words, from a
point in space where the sun appeared as bright as what we call a
first-magnitude star, its companion, Jupiter, would have shone as a
sixth-magnitude star. Many stars have companions proportionally much
fainter than that. The companion of Sirius, for instance, is at least
ten thousand times less bright than its great comrade.

Looking at Jupiter in this way, it interests us not as the probable
abode of intelligent life, but as a world in the making, a world,
moreover, which, when it is completed--if it ever shall be after the
terrestrial pattern--will dwarf our globe into insignificance. That
stupendous miracle of world-making which is dimly painted in the grand
figures employed by the writers of Genesis, and the composers of other
cosmogonic legends, is here actually going on before our eyes. The
telescope shows us in the cloudy face of Jupiter the moving of the
spirit upon the face of the great deep. What the final result will be we
can not tell, but clearly the end of the grand processes there in
operation has not yet been reached.

The interesting suggestion was made and urged by Mr. Proctor that if
Jupiter itself is in no condition at present to bear life, its
satellites may be, in that respect, more happily circumstanced. It can
not be said that very much has been learned about the satellites of
Jupiter since Proctor's day, and his suggestion is no less and no more
probable now than it was when first offered.

There has been cumulative evidence that Jupiter's satellites obey the
same law that governs the rotation of our moon, viz., that which compels
them always to keep the same face turned toward their primary, and this
would clearly affect, although it might not preclude, their
habitability. With the exception of the minute fifth satellite
discovered by Barnard in 1892, they are all of sufficient size to retain
at least some traces of an atmosphere. In fact, one of them is larger
than the planet Mars, and another is of nearly the same size as that
planet, while the smallest of the four principal ones is about equal to
our moon. Under the powerful attraction of Jupiter they travel rapidly,
and viewed from the surface of that planet they would offer a wonderful
spectacle.

They are continually causing solar eclipses and themselves undergoing
eclipse in Jupiter's shadow, and their swiftly changing aspects and
groupings would be watched by an astronomer on Jupiter with undying
interest.

But far more wonderful would be the spectacle presented by Jupiter to
inhabitants dwelling on his moons. From the nearer moon, in particular,
which is situated less than 220,000 miles from Jupiter's surface, the
great planet would be an overwhelming phenomenon in the sky.

Its immense disk, hanging overhead, would cover a circle of the
firmament twenty degrees in diameter, or, in round numbers, forty times
the diameter of the full moon as seen from the earth! It would shed a
great amount of light and heat, and thus would more or less effectively
supply the deficit of solar radiation, for we must remember that Jupiter
and his satellites receive from the sun less than one twenty-fifth as
much light and heat as the earth receives.

The maze of contending motions, the rapid flow and eddying of cloud
belts, the outburst of strange fiery spots, the display of rich, varied,
and constantly changing colors, which astonish and delight the
telescopic observer on the earth, would be exhibited to the naked eye of
an inhabitant of Jupiter's nearest moon far more clearly than the
greatest telescope is able to reveal them to us.

Here, again, the mind is carried back to long past ages in the history
of the planet on which we dwell. It is believed by some that our moon
may have contained inhabitants when the earth was still hot and glowing,
as Jupiter appears to be now, and that, as the earth cooled and became
habitable, the moon gradually parted with its atmosphere and water so
that its living races perished almost coincidently with the beginning of
life on the earth. If we accept this view and apply it to the case of
Jupiter we may conclude that when that enormous globe has cooled and
settled down to a possibly habitable condition, its four attendant moons
will suffer the fate that overtook the earth's satellite, and in their
turn become barren and death-stricken, while the great orb that once
nurtured them with its light and heat receives the Promethean fire and
begins to bloom with life.




CHAPTER VII

SATURN, A PRODIGY AMONG PLANETS


One of the first things that persons unaccustomed to astronomical
observations ask to see when they have an opportunity to look through a
telescope is the planet Saturn. Many telescopic views in the heavens
disappoint the beginner, but that of Saturn does not. Even though the
planet may not look as large as he expects to see it from what he has
been told of the magnifying power employed, the untrained observer is
sure to be greatly impressed by the wonderful rings, suspended around it
as if by a miracle. No previous inspection of pictures of these rings
can rob them of their effect upon the eye and the mind. They are
overwhelming in their inimitable singularity, and they leave every
spectator truly amazed. Sir John Herschel has remarked that they have
the appearance of an "elaborately artificial mechanism." They have even
been regarded as habitable bodies! What we are to think of that
proposition we shall see when we come to consider their composition and
probable origin. In the meantime let us recall the main facts of
Saturn's dimensions and situation in the solar system.

Saturn is the second of the major, or Jovian, group of planets, and is
situated at a mean distance from the sun of 886,000,000 miles. We need
not consider the eccentricity of its orbit, which, although relatively
not very great, produces a variation of 50,000,000 miles in its distance
from the sun, because, at its immense mean distance, this change would
not be of much importance with regard to the planet's habitability or
non-habitability. Under the most favorable conditions Saturn can never
be nearer than 744,000,000 miles to the earth, or eight times the sun's
distance from us. It receives from the sun about one ninetieth of the
light and heat that we get.

[Illustration: SATURN IN ITS THREE PRINCIPAL PHASES AS SEEN FROM THE
EARTH. From a drawing by Bond.]

Saturn takes twenty-nine and a half years to complete a journey about
the sun. Like Jupiter, it rotates very rapidly on its axis, the period
being ten hours and fourteen minutes. Its axis of rotation is inclined
not far from the same angle as that of the earth's axis (26° 49´), so
that its seasons should resemble ours, although their alternations are
extremely slow in consequence of the enormous length of Saturn's year.

Not including the rings in the calculation, Saturn exceeds the earth in
size 760 times. The addition of the rings would not, however, greatly
alter the result of the comparison, because, although the total surface
of the rings, counting both faces, exceeds the earth's surface about 160
times, their volume, owing to their surprising thinness, is only about
six times the volume of the earth, and their mass, in consequence of
their slight density, is very much less than the earth's, perhaps,
indeed, inappreciable in comparison.

Saturn's mean diameter is 73,000 miles, and its polar compression is
even greater than that of Jupiter, a difference of 7,000 miles--almost
comparable with the entire diameter of the earth--existing between its
equatorial and its polar diameter, the former being 75,000 and the
latter 68,000 miles.

We found the density of Jupiter astonishingly slight, but that of Saturn
is slighter still. Jupiter would sink if thrown into water, but Saturn
would actually float, if not "like a cork," yet quite as buoyantly as
many kinds of wood, for its mean density is only three quarters that of
water, or one eighth of the earth's. In fact, there is no known planet
whose density is so slight as Saturn's. Thus it happens that,
notwithstanding its vast size and mass, the force of gravity upon Saturn
is nearly the same as upon our globe. Upon visiting Venus we should find
ourselves weighing a little less than at home, and upon visiting Saturn
a little more, but in neither case would the difference be very
important. If the relative weight of bodies on the surfaces of planets
formed the sole test of their habitability, Venus and Saturn would both
rank with the earth as suitable abodes for men.

But the exceedingly slight density of Saturn seems to be most reasonably
accounted for on the supposition that, like Jupiter, it is in a vaporous
condition, still very hot within--although but slightly, if at all,
incandescent at the surface--and, therefore, unsuited to contain life.
It is hardly worth while to speculate about any solid nucleus within,
because, even if such a thing were possible, or probable, it must lie
forever hidden from our eyes. But if we accept the theory that Saturn is
in an early formative stage, and that, millions of years hence, it may
become an incrusted and habitable globe, we shall, at least, follow the
analogy of what we believe to have been the history of the earth, except
that Saturn's immense distance from the sun will always prevent it from
receiving an amount of solar radiation consistent with our ideas of what
is required by a living world. Of course, since one can imagine what he
chooses, it is possible to suppose inhabitants suited to existence in a
world composed only of whirling clouds, and a poet with the imagination
of a Milton might give us very imposing and stirring images of such
creatures and their chaotic surroundings, but fancies like these can
have no basis in human experience, and consequently can make no claim
upon scientific recognition.

Or, as an alternative, it might be assumed that Saturn is composed of
lighter elements and materials than those which constitute the earth and
the other solid planets in the more immediate neighborhood of the sun.
But such an assumption would put us entirely at sea as regards the forms
of organic life that could exist upon a planet of that description, and,
like Sir Humphry Davy in the Vision, that occupies the first chapter of
his quaintly charming Consolations in Travel, or, the Last Days of a
Philosopher, we should be thrown entirely upon the resources of the
imagination in representing to ourselves the nature and appearance of
its inhabitants. Yet minds of unquestioned power and sincerity have in
all ages found pleasure and even profit in such exercises, and with
every fresh discovery arises a new flight of fancies like butterflies
from a roadside pool. As affording a glimpse into the mind of a
remarkable man, as well as a proof of the fascination of such subjects,
it will be interesting to quote from the book just mentioned Davy's
description of his imaginary inhabitants of Saturn:

"I saw below me a surface infinitely diversified, something like that of
an immense glacier covered with large columnar masses, which appeared as
if formed of glass, and from which were suspended rounded forms of
various sizes which, if they had not been transparent, I might have
supposed to be fruit. From what appeared to me to be analogous to
bright-blue ice, streams of the richest tint of rose color or purple
burst forth and flowed into basins, forming lakes or seas of the same
color. Looking through the atmosphere toward the heavens, I saw
brilliant opaque clouds, of an azure color, that reflected the light of
the sun, which had to my eyes an entirely new aspect and appeared
smaller, as if seen through a dense blue mist.

"I saw moving on the surface below me immense masses, the forms of which
I find it impossible to describe. They had systems for locomotion
similar to those of the morse, or sea-horse, but I saw, with great
surprise, that they moved from place to place by six extremely thin
membranes, which they used as wings. Their colors were varied and
beautiful, but principally azure and rose color. I saw numerous
convolutions of tubes, more analogous to the trunk of the elephant than
to anything else I can imagine, occupying what I supposed to be the
upper parts of the body. It was with a species of terror that I saw one
of them mounting upward, apparently flying toward those opaque clouds
which I have before mentioned.

"'I know what your feelings are,' said the Genius; 'you want analogies,
and all the elements of knowledge to comprehend the scene before you.
You are in the same state in which a fly would be whose microscopic eye
was changed for one similar to that of man, and you are wholly unable to
associate what you now see with your former knowledge. But those beings
who are before you, and who appear to you almost as imperfect in their
functions as the zoophytes of the polar sea, to which they are not
unlike in their apparent organization to your eyes, have a sphere of
sensibility and intellectual enjoyment far superior to that of the
inhabitants of your earth. Each of those tubes, which appears like the
trunk of an elephant, is an organ of peculiar motion or sensation. They
have many modes of perception of which you are wholly ignorant, at the
same time that their sphere of vision is infinitely more extended than
yours, and their organs of touch far more perfect and exquisite.'"

After descanting upon the advantages of Saturn's position for surveying
some of the phenomena of the solar system and of outer space, and the
consequent immense advances that the Saturnians have made in
astronomical knowledge, the Genius continues:

"'If I were to show you the different parts of the surface of this
planet you would see the marvelous results of the powers possessed by
these highly intellectual beings, and of the wonderful manner in which
they have applied and modified matter. Those columnar masses, which seem
to you as if rising out of a mass of ice below, are results of art, and
processes are going on within them connected with the formation and
perfection of their food. The brilliant-colored fluids are the results
of such operations as on the earth would be performed in your
laboratories, or more properly in your refined culinary apparatus, for
they are connected with their system of nourishment. Those opaque azure
clouds, to which you saw a few minutes ago one of those beings directing
his course, are works of art, and places in which they move through
different regions of their atmosphere, and command the temperature and
the quantity of light most fitted for their philosophical researches,
or most convenient for the purposes of life.'"[11]

[Footnote 11: Davy, of course, was aware that, owing to increase of
distance, the sun would appear to an inhabitant of Saturn with a disk
only one ninetieth as great in area as that which it presents to our
eyes.]

But, while Saturn does not appear, with our present knowledge, to hold
out any encouragement to those who would regard it as the abode of
living creatures capable of being described in any terms except those of
pure imagination, yet it is so unique a curiosity among the heavenly
bodies that one returns again and again to the contemplation of its
strange details. Saturn has nine moons, but some of them are relatively
small bodies--the ninth, discovered photographically by Professor
Pickering in 1899, being especially minute--and others are situated at
great distances from the planet, and for these reasons, together with
the fact that the sunlight is so feeble upon them that, surface for
surface, they have only one ninetieth as much illumination as our moon
receives, they can not make a very brilliant display in the Saturnian
sky. To astronomers on Saturn they would, of course, be intensely
interesting because of their perturbations and particularly the effect
of their attraction on the rings.

This brings us again to the consideration of those marvelous appendages,
and to the statement of facts about them which we have not yet recalled.

If the reader will take a ball three inches in diameter to represent the
globe of Saturn, and, out of the center of a circular piece of
writing-paper seven inches in diameter, will cut a round hole three and
three quarter inches across, and will then place the ball in the middle
of the hole in the paper, he will have a very fair representation of the
relative proportions of Saturn and its rings. To represent the main gap
or division in the rings he might draw, a little more than three eighths
of an inch from the outer edge of the paper disk, a pencil line about a
sixteenth of an inch broad.

Perhaps the most striking fact that becomes conspicuous in making such a
model of the Saturnian system is the exceeding thinness of the rings as
compared with their enormous extent. They are about 170,000 miles across
from outer edge to outer edge, and about 38,000 miles broad from outer
edge to inner edge--including the gauze ring presently to be
mentioned--yet their thickness probably does not surpass one hundred
miles! In fact, the sheet of paper in our imaginary model is several
times too thick to represent the true relative thickness of Saturn's
rings.

Several narrow gaps in the rings have been detected from time to time,
but there is only one such gap that is always clearly to be seen, the
one already mentioned, situated about 10,000 miles from the outer edge
and about 1,600 miles in width. Inside of this gap the broadest and
brightest ring appears, having a width of about 16,500 miles. For some
reason this great ring is most brilliant near the gap, and its
brightness gradually falls off toward its inner side. At a distance of
something less than 20,000 miles from the planet--or perhaps it would
be more correct to say above the planet, for the rings hang directly
over Saturn's equator--the broad, bright ring merges into a mysterious
gauzelike object, also in the form of a ring, which extends to within
9,000 or 10,000 miles of the planet's surface, and therefore itself has
a width of say 10,000 miles.

In consequence of the thinness of the rings they completely disappear
from the range of vision of small telescopes when, as occurs once in
every fifteen years, they are seen exactly edgewise from the earth. In a
telescope powerful enough to reveal them when in that situation they
resemble a thin, glowing needle run through the ball of the planet. The
rings will be in this position in 1907, and again in 1922.

The opacity of the rings is proved by the shadow which they cast upon
the ball of the planet. This is particularly manifest at the time when
they are edgewise to the earth, for the sun being situated slightly
above or below the plane of the rings then throws their shadow across
Saturn close to its equator. When they are canted at a considerable
angle to our line of sight their shadow is seen on the planet, bordering
their outer edge where they cross the ball.

The gauze ring, the detection of which as a faintly luminous phenomenon
requires a powerful telescope, can be seen with slighter telescopic
power in the form of a light shade projected against the planet at the
inner edge of the broad bright ring. The explanation of the existence of
this peculiar object depends upon the nature of the entire system,
which, instead of being, as the earliest observers thought it, a solid
ring or series of concentric rings, is composed of innumerable small
bodies, like meteorites, perhaps, in size, circulating independently but
in comparatively close juxtaposition to one another about Saturn, and
presenting to our eyes, because of their great number and of our
enormous distance, the appearance of solid, uniform rings. So a flock of
ducks may look from afar like a continuous black line or band, although
if we were near them we should perceive that a considerable space
separates each individual from his neighbors.

The fact that this is the constitution of Saturn's rings can be
confidently stated because it has been mathematically proved that they
could not exist if they were either solid or liquid bodies in a
continuous form, and because the late Prof. James E. Keeler demonstrated
with the spectroscope, by means of the Doppler principle, already
explained in the chapter on Venus, that the rings circulate about the
planet with varying velocities according to their distance from Saturn's
center, exactly as independent satellites would do.

It might be said, then, that Saturn, instead of having nine satellites
only, has untold millions of them, traveling in orbits so closely
contiguous that they form the appearance of a vast ring.

As to their origin, it may be supposed that they are a relic of a ring
of matter left in suspension during the contraction of the globe of
Saturn from a nebulous mass, just as the rings from which the various
planets are supposed to have been formed were left off during the
contraction of the main body of the original solar nebula. Other similar
rings originally surrounding Saturn may have become satellites, but the
matter composing the existing rings is so close to the planet that it
falls within the critical distance known as "Roche's limit," within
which, owing to the tidal effect of the planet's attraction, no body so
large as a true satellite could exist, and accordingly in the process of
formation of the Saturnian system this matter, instead of being
aggregated into a single satellite, has remained spread out in the form
of a ring, although its substance long ago passed from the vaporous and
liquid to the solid form. We have spoken of the rings as being composed
of meteorites, but perhaps their component particles may be so small as
to answer more closely to the definition of dust. In these rings of
dust, or meteorites, disturbances are produced by the attraction of the
planet and that of the outer satellites, and it is yet a question
whether they are a stable and permanent feature of Saturn, or will, in
the course of time, be destroyed.[12]

[Footnote 12: For further details about Saturn's rings, see The Tides,
by G.H. Darwin, chap. xx.]

It has been thought that the gauze ring is variable in brightness. This
would tend to show that it is composed of bodies which have been drawn
in toward the planet from the principal mass of the rings, and these
bodies may end their career by falling upon the planet. This process,
indefinitely continued, would result in the total disappearance of the
rings--Saturn would finally swallow them, as the old god from whom the
planet gets its name is fabled to have swallowed his children.

Near the beginning of this chapter reference was made to the fact that
Saturn's rings have been regarded as habitable bodies. That, of course,
was before the discovery that they were not solid. Knowing what we now
know about them, even Dr. Thomas Dick, the great Scotch popularizer of
astronomy in the first half of the nineteenth century, would have been
compelled to abandon his theory that Saturn's rings were crowded with
inhabitants. At the rate of 280 to the square mile he reckoned that they
could easily contain 8,078,102,266,080 people.

He even seems to have regarded their edges--in his time their actual
thinness was already well known--as useful ground for the support of
living creatures, for he carefully calculated the aggregate area of
these edges and found that it considerably exceeded the area of the
entire surface of the earth. Indeed, Dr. Dick found room for more
inhabitants on Saturn's rings than on Saturn itself, for, excluding the
gauze ring, undiscovered in his day, the two surfaces of the rings are
greater in area than the surface of the globe of the planet. He did not
attack the problem of the weight of bodies on worlds in the form of
broad, flat, thin, surfaces like Saturn's rings, or indulge in any
reflections on the interrelations of the inhabitants of the opposite
sides, although he described the wonderful appearance of Saturn and
other celestial objects as viewed from the rings.

But all these speculations fall to the ground in face of the simple fact
that if we could reach Saturn's rings we should find nothing to stand
upon, except a cloud of swiftly flying dust or a swarm of meteors,
swayed by contending attractions. And, indeed, it is likely that upon
arriving in the immediate neighborhood of the rings they would virtually
disappear! Seen close at hand their component particles might be so
widely separated that all appearance of connection between them would
vanish, and it has been estimated that from Saturn's surface the rings,
instead of presenting a gorgeous arch spanning the heavens, may be
visible only as a faintly gleaming band, like the Milky Way or the
zodiacal light. In this respect the mystic Swedenborg appears to have
had a clearer conception of the true nature of Saturn's rings than did
Dr. Dick, for in his book on The Earths in the Universe he says--using
the word "belt" to describe the phenomenon of the rings:

"Being questioned concerning that great belt which appears from our
earth to rise above the horizon of that planet, and to vary its
situations, they [the inhabitants of Saturn] said that it does not
appear to them as a belt, but only as somewhat whitish, like snow in the
heaven, in various directions."

In view of such observations as that of Prof. E.E. Barnard, in 1892,
showing that a satellite passing through the shadow of Saturn's rings
does not entirely disappear--a fact which proves that the rings are
partially transparent to the sunlight--one might be tempted to ask
whether Saturn itself, considering its astonishing lack of density, is
not composed, at least in its outer parts, of separate particles of
matter revolving independently about their center of attraction, and
presenting the appearance of a smooth, uniform shell reflecting the
light of the sun. In other words, may not Saturn be, exteriorly, a globe
of dust instead of a globe of vapor? Certainly the rings, incoherent and
translucent though they be, reflect the sunlight to our eyes, at least
from the brighter part of their surface, with a brilliance comparable
with that of the globe of the planet itself.

As bearing on the question of the interior condition of Saturn and
Jupiter, it should, perhaps, be said that mathematical considerations,
based on the figures of equilibrium of rotating liquid masses, lead to
the conclusion that those planets are comparatively very dense within.
Professor Darwin puts the statement very strongly, as follows: "In this
way it is known with certainty that the central portions of the planets
Jupiter and Saturn are much denser, compared to their superficial
portions, than is the case with the earth."[13]

[Footnote 13: The Tides, by G.H. Darwin, p. 333.]

The globe and rings of Saturn witness an imposing spectacle of gigantic
moving shadows. The great ball stretches its vast shade across the full
width of the rings at times, and the rings, as we have seen, throw their
shadow in a belt, whose position slowly changes, across the ball,
sweeping from the equator, now toward one pole and now toward the
other. The sun shines alternately on each side of the rings for a space
of nearly fifteen years--a day fifteen years long! And then, when that
face of the ring is turned away from the sun, there ensues a night of
fifteen years' duration also.

Whatever appearance the rings may present from the equator and the
middle latitudes on Saturn, from the polar regions they would be totally
invisible. As one passed toward the north, or the south, pole he would
see the upper part of the arch of the rings gradually sink toward the
horizon until at length, somewhere in the neighborhood of the polar
circle, it would finally disappear, hidden by the round shoulder of the
great globe.


URANUS, NEPTUNE, AND THE SUSPECTED ULTRANEPTUNIAN PLANET

What has been said of Jupiter and Saturn applies also to the remaining
members of the Jovian group of planets, Uranus and Neptune, viz., that
their density is so small that it seems probable that they can not, at
the present time, be in a habitable planetary condition. All four of
these outer, larger planets have, in comparatively recent times, been
solar orbs, small companions of the sun. The density of Uranus is about
one fifth greater than that of water, and slightly greater than that of
Neptune. Uranus is 32,000 miles in diameter, and Neptune 35,000 miles.
Curiously enough, the force of gravity upon each of these two large
planets is a little less than upon the earth. This arises from the fact
that in reckoning gravity on the surface of a planet not only the mass
of the planet, but its diameter or radius, must be considered. Gravity
varies directly as the mass, but inversely as the square of the radius,
and for this reason a large planet of small density may exercise a less
force of gravity at its surface than does a small planet of great
density.

The mean distance of Uranus from the sun is about 1,780,000,000 miles,
and its period of revolution is eighty-four years; Neptune's mean
distance is about 2,800,000,000 miles, and its period of revolution is
about 164 years.

Uranus has four satellites, and Neptune one. The remarkable thing about
these satellites is that they revolve _backward_, or contrary to the
direction in which all the other satellites belonging to the solar
system revolve, and in which all the other planets rotate on their axis.
In the case of Uranus, the plane in which the satellites revolve is not
far from a position at right angles to the plane of the ecliptic; but in
the case of Neptune, the plane of revolution of the satellites is tipped
much farther backward. Since in every other case the satellites of a
planet are situated nearly in the plane of the planet's equator, it may
be assumed that the same rule holds with Uranus and Neptune; and, that
being so, we must conclude that those planets rotate backward on their
axes. This has an important bearing on the nebular hypothesis of the
origin of the solar system, and at one time was thought to furnish a
convincing argument against that hypothesis; but it has been shown that
by a modification of Laplace's theory the peculiar behavior of Uranus
and Neptune can be reconciled with it.

Very little is known of the surfaces of Uranus and Neptune. Indications
of the existence of belts resembling those of Jupiter have been found in
the case of both planets. There are similar belts on Saturn, and as they
seem to be characteristic of large, rapidly rotating bodies of small
density, it was to be expected that they would be found on Uranus and
Neptune.

The very interesting opinion is entertained by some astronomers that
there is at least one other great planet beyond Neptune. The orbits of
certain comets are relied upon as furnishing evidence of the existence
of such a body. Prof. George Forbes has estimated that this, as yet
undiscovered, planet may be even greater than Jupiter in mass, and may
be situated at a distance from the sun one hundred times as great as the
earth's, where it revolves in an orbit a single circuit of which
requires a thousand years.

Whether this planet, with a year a thousand of our years in length, will
ever be seen with a telescope, or whether its existence will ever, in
some other manner, be fully demonstrated, can not yet be told. It will
be remembered that Neptune was discovered by means of computations based
upon its disturbing attraction on Uranus before it had ever been
recognized with the telescope. But when the astronomers in the
observatories were told by their mathematical brethren where to look
they found the planet within half an hour after the search began. So it
is possible the suspected great planet beyond Neptune may be within the
range of telescopic vision, but may not be detected until elaborate
calculations have deduced its place in the heavens. As a populous city
is said to furnish the best hiding-place for a man who would escape the
attention of his fellow beings, so the star-sprinkled sky is able to
conceal among its multitudes worlds both great and small until the most
painstaking detective methods bring them to recognition.




CHAPTER VIII

THE MOON, CHILD OF THE EARTH AND THE SUN


Very naturally the moon has always been a great favorite with those who,
either in a scientific or in a literary spirit, have speculated about
the plurality of inhabited worlds. The reasons for the preference
accorded to the moon in this regard are evident. Unless a comet should
brush us--as a comet is suspected of having done already--no celestial
body, of any pretensions to size, can ever approach as near to the earth
as the moon is, at least while the solar system continues to obey the
organic laws that now control it. It is only a step from the earth to
the moon. What are 240,000 miles in comparison with the distances of the
stars, or even with the distances of the planets? Jupiter, driving
between the earth and the moon, would occupy more than one third of the
intervening space with the chariot of his mighty globe; Saturn, with
broad wings outspread, would span more than two thirds of the distance;
and the sun, so far from being able to get through at all, would overlap
the way more than 300,000 miles on each side.

In consequence, of course, of its nearness, the moon is the only member
of the planetary system whose principal features are visible to the
naked eye. In truth, the naked eye perceives the larger configurations
of the lunar surface more clearly than the most powerful telescope shows
the details on the disk of Mars. Long before the time of Galileo and the
invention of the telescope, men had noticed that the face of the moon
bears a resemblance to the appearance that the earth would present if
viewed from afar off. In remote antiquity there were philosophers who
thought that the moon was an inhabited world, and very early the
romancers took up the theme. Lucian, the Voltaire of the second century
of our era, mercilessly scourged the pretenders of the earth from an
imaginary point of vantage on the moon, which enabled him to peer down
into their secrets. Lucian's description of the appearance of the earth
from the moon shows how clearly defined in his day had become the
conception of our globe as only an atom in space.

"Especially did it occur to me to laugh at the men who were quarreling
about the boundaries of their land, and at those who were proud because
they cultivated the Sikyonian plain, or owned that part of Marathon
around Oenoe, or held possession of a thousand acres at Acharnæ. Of
the whole of Greece, as it then appeared to me from above, being about
the size of four fingers, I think Attica was in proportion a mere speck.
So that I wondered on what condition it was left to these rich men to be
proud."[14]

[Footnote 14: Ikaromenippus; or, Above the Clouds. Prof. D.C. Brown's
translation.]

Such scenes as Lucian beheld, in imagination, upon the earth while
looking from the moon, many would fain behold, with telescopic aid,
upon the moon while looking from the earth. Galileo believed that the
details of the lunar surface revealed by his telescope closely resembled
in their nature the features of the earth's surface, and for a long
time, as the telescope continued to be improved, observers were
impressed with the belief that the moon possessed not only mountains and
plains, but seas and oceans also.

It was the discovery that the moon has no perceptible atmosphere that
first seriously undermined the theory of its habitability. Yet, as was
remarked in the introductory chapter, there has of late been some change
of view concerning a lunar atmosphere; but the change has been not so
much in the ascertained facts as in the way of looking at those facts.

But before we discuss this matter, it will be well to state what is
known beyond peradventure about the moon.

Its mean distance from the earth is usually called, for the sake of a
round number, 240,000 miles, but more accurately stated it is 238,840
miles. This is variable to the extent of more than 31,000 miles, on
account of the eccentricity of its orbit, and the eccentricity itself is
variable, in consequence of the perturbing attractions of the earth and
the sun, so that the distance of the moon from the earth is continually
changing. It may be as far away as 253,000 miles and as near as 221,600
miles.

Although the orbit of the moon is generally represented, for
convenience, as an ellipse about the earth, it is, in reality, a varying
curve, having the sun for its real focus, and always concave toward the
latter. This is a fact that can be more readily explained with the aid
of a diagram.

[Illustration: THE MOON'S PATH WITH RESPECT TO THE SUN AND THE EARTH.]

In the accompanying cut, when the earth is at _A_ the moon is between it
and the sun, in the phase called new moon. At this point the earth's
orbit about the sun is more curved than the moon's, and the earth is
moving relatively faster than the moon, so that when it arrives at _B_
it is ahead of the moon, and we see the latter to the right of the
earth, in the phase called first quarter. The earth being at this time
ahead of the moon, the effect of its attraction, combined with that of
the sun, tends to hasten the moon onward in its orbit about the sun, and
the moon begins to travel more swiftly, until it overtakes the earth at
_C_, and appears on the side opposite the sun, in the phase called full
moon. At this point the moon's orbit about the sun has a shorter radius
of curvature than the earth's. In traveling from _C_ to _D_ the moon
still moves more rapidly than the earth, and, having passed it, appears
at _D_ to the left of the earth, in the phase called third quarter. Now,
the earth being behind the moon, the effect of its attraction combined
with the sun's tends to retard the moon in its orbit about the sun,
with the result that the moon moves again less rapidly than the earth,
and the latter overtakes it, so that, upon reaching _E_, the two are
once more in the same relative positions that they occupied at _A_, and
it is again new moon. Thus it will be seen that, although the real orbit
of the moon has the sun for its center of revolution, nevertheless, in
consequence of the attraction of the earth, combined in varying
directions with that of the sun, the moon, once every month, makes a
complete circuit of our globe.

The above explanation should not be taken for a mathematical
demonstration of the moon's motion, but simply for a graphical
illustration of how the moon appears to revolve about the earth while
really obeying the sun's attraction as completely as the earth does.

There is no other planet that has a moon relatively as large as ours.
The moon's diameter is 2,163 miles. Its volume, compared with the
earth's, is in the ratio of 1 to 49, and its density is about six
tenths of the earth's. This makes its mass to that of our globe about as
1 to 81. In other words, it would take eighty-one moons to
counterbalance the earth. Before speaking of the force of gravity on the
moon we will examine the character of the lunar surface.

To the naked eye the moon's face appears variegated with dusky patches,
while a few points of superior brilliance shine amid the brighter
portions, especially in the southern and eastern quarters, where immense
craters like Tycho and Copernicus are visible to a keen eye, gleaming
like polished buttons. With a telescope, even of moderate power, the
surface of the moon presents a scene of astonishing complexity, in which
strangeness, beauty, and grandeur are all combined. The half of the moon
turned earthward contains an area of 7,300,000 square miles, a little
greater than the area of South America and a little less than that of
North America. Of these 7,300,000 square miles, about 2,900,000 square
miles are occupied by the gray, or dusky, expanses, called in lunar
geography, or selenography, _maria_--i.e., "seas." Whatever they may
once have been, they are not now seas, but dry plains, bordered in many
places by precipitous cliffs and mountains, varied in level by low
ridges and regions of depression, intersected occasionally by immense
cracks, having the width and depth of our mightiest river cañons, and
sprinkled with bright points and crater pits. The remaining 4,400,000
square miles are mainly occupied by mountains of the most extraordinary
character. Owing partly to roughness of the surface and partly to more
brilliant reflective power, the mountainous regions of the moon appear
bright in comparison with the dull-colored plains.

Some of the lunar mountains lie in long, massive chains, with towering
peaks, profound gorges, narrow valleys, vast amphitheaters, and beetling
precipices. Looking at them with a powerful telescope, the observer
might well fancy himself to be gazing down from an immense height into
the heart of the untraveled Himalayas. But these, imposing though they
are, do not constitute the most wonderful feature of the mountain
scenery of the moon.

Appearing sometimes on the shores of the "seas," sometimes in the midst
of broad plains, sometimes along the course of mountain chains, and
sometimes in magnificent rows, following for hundreds of miles the
meridians of the lunar globe, are tremendous, mountain-walled, circular
chasms, called craters. Frequently they have in the middle of their
depressed interior floors a peak, or a cluster of peaks. Their inner and
outer walls are seamed with ridges, and what look like gigantic streams
of frozen lava surround them. The resemblance that they bear to the
craters of volcanoes is, at first sight, so striking that probably
nobody would ever have thought of questioning the truth of the statement
that they are such craters but for their incredible magnitude. Many of
them exceed fifty miles in diameter, and some of them sink two, three,
four, and more miles below the loftiest points upon their walls! There
is a chasm, 140 miles long and 70 broad, named Newton, situated about
200 miles from the south pole of the moon, whose floor lies 24,000 feet
below the summit of a peak that towers just above it on the east! This
abyss is so profound that the shadows of its enclosing precipices never
entirely quit it, and the larger part of its bottom is buried in endless
night.

One can not but shudder at the thought of standing on the broken walls
of Newton, and gazing down into a cavity of such stupendous depth that
if Chimborazo were thrown into it, the head of the mighty Andean peak
would be thousands of feet beneath the observer.

A different example of the crater mountains of the moon is the
celebrated Tycho, situated in latitude about 43° south, corresponding
with the latitude of southern New Zealand on the earth. Tycho is nearly
circular and a little more than 54 miles across. The highest point on
its wall is about 17,000 feet above the interior. In the middle of its
floor is a mountain 5,000 or 6,000 feet high. Tycho is especially
remarkable for the vast system of whitish streaks, or rays, which
starting from its outer walls, spread in all directions over the face of
the moon, many of them, running, without deviation, hundreds of miles
across mountains, craters, and plains. These rays are among the greatest
of lunar mysteries, and we shall have more to say of them.

[Illustration: THE LUNAR ALPS, APENNINES, AND CAUCASUS.
Photographed with the Lick Telescope.]

Copernicus, a crater mountain situated about 10° north of the equator,
in the eastern hemisphere of the moon, is another wonderful object, 56
miles in diameter, a polygon appearing, when not intently studied, as a
circle, 11,000 or 12,000 feet deep, and having a group of relatively low
peaks in the center of its floor. Around Copernicus an extensive area of
the moon's surface is whitened with something resembling the rays of
Tycho, but more irregular in appearance. Copernicus lies within the edge
of the great plain named the _Oceanus Procellarum_, or "Ocean of
Storms," and farther east, in the midst of the "ocean," is a smaller
crater mountain, named Kepler, which is also enveloped by a whitish
area, covering the lunar surface as if it were the result of extensive
outflows of light-colored lava.

In one important particular the crater mountains of the moon differ from
terrestrial volcanoes. This difference is clearly described by Nasmyth
and Carpenter in their book on The Moon:

"While the terrestrial crater is generally a hollow on a mountain top,
with its flat bottom high above the level of the surrounding country,
those upon the moon have their lowest points depressed more or less
deeply below the general surface of the moon, the external height being
frequently only a half or one third of the internal depth."

It has been suggested that these gigantic rings are only "basal wrecks"
of volcanic mountains, whose conical summits have been blown away,
leaving vast crateriform hollows where the mighty peaks once stood; but
the better opinion seems to be that which assumes that the rings were
formed by volcanic action very much as we now see them. If such a crater
as Copernicus or the still larger one named Theophilus, which is
situated in the western hemisphere of the moon, on the shore of the "Sea
of Nectar," ever had a conical mountain rising from its rim, the height
attained by the peak, if the average slope were about 30°, would have
been truly stupendous--fifteen or eighteen miles!

There is a kind of ring mountains, found in many places on the moon,
whose forms and surroundings do not, as the craters heretofore described
do, suggest at first sight a volcanic origin. These are rather level
plains of an oval or circular outline, enclosed by a wall of mountains.
The finest example is, perhaps, the dark-gray Plato, situated in 50° of
north latitude, near an immense mountain uplift named the Lunar Alps,
and on the northern shore of the _Mare Imbrium_, or "Sea of Showers."
Plato appears as an oval plain, very smooth and level, about 60 miles in
length, and completely surrounded by mountains, quite precipitous on the
inner side, and rising in their highest peaks to an elevation of 6,000
to 7,000 feet. Enclosed plains, bearing more or less resemblance to
Plato--sometimes smooth within, and sometimes broken with small peaks
and craters or hilly ridges--are to be found scattered over almost all
parts of the moon. If our satellite was ever an inhabited world like the
earth, while its surface was in its present condition, these valleys
must have presented an extraordinary spectacle. It has been thought that
they may once have been filled with water, forming lakes that recall the
curious Crater Lake of Oregon.

[Illustration: THE MOON AT FIRST AND LAST QUARTER (WESTERN AND EASTERN
HEMISPHERES). Photographed with the Lick Telescope.]

It is not my intention to give a complete description of the various
lunar features, and I mention but one other--the "clefts" or "rills,"
which are to be seen running across the surface like cracks. One of the
most remarkable of these is found in the _Oceanus Procellarum_, near the
crater-mountain Aristarchus, which is famed for the intense brilliance
of its central peak, whose reflective power is so great that it was once
supposed to be aflame with volcanic fire. The cleft, or crack, in
question is very erratic in its course, and many miles in length, and
it terminates in a ringed plain named Herodotus not far east of
Aristarchus, breaking through the wall of the plain and entering the
interior. Many other similar chasms or cañons exist on the moon, some
crossing plains, some cleaving mountain walls, and some forming a
network of intersecting clefts. Mr. Thomas Gwyn Elger has this to say on
the subject of the lunar clefts:

"If, as seems most probable, these gigantic cracks are due to
contractions of the moon's surface, it is not impossible, in spite of
the assertions of the text-books to the effect that our satellite is now
a 'changeless world,' that emanations may proceed from these fissures,
even if, under the monthly alternations of extreme temperatures, surface
changes do not now occasionally take place from this cause also. Should
this be so, the appearance of new rills and the extension and
modification of those already existing may reasonably be looked for."

Mr. Elger then proceeds to describe his discovery in 1883, in the
ring-plain Mersenius, of a cleft never noticed before, and which seems
to have been of recent formation.[15]

[Footnote 15: The Moon, a Full Description and Map of its Principal
Features, by Thomas Gwyn Elger, 1895.

Those who desire to read detailed descriptions of lunar scenery may
consult, in addition to Mr. Elger's book, the following: The Moon,
considered as a Planet, a World, and a Satellite, by James Nasmyth and
James Carpenter, 1874; The Moon, and the Condition and Configurations of
its Surface, by Edmund Neison, 1876. See also Annals of Harvard College
Observatory, vol. xxxii, part ii, 1900, for observations made by Prof.
William H. Pickering at the Arequipa Observatory.]

We now return to the question of the force of lunar gravity. This we
find to be only one sixth as great as gravity on the surface of the
earth. It is by far the smallest force of gravity that we have found
anywhere except on the asteroids. Employing the same method of
comparison that was made in the case of Mars, we compute that a man on
the moon could attain a height of thirty-six feet without being
relatively more unwieldy than a six-foot descendant of Adam is on the
earth.

Whether this furnishes a sound reason for assuming that the lunar
inhabitants, if any exist or have ever existed, should be preposterous
giants is questionable; yet such an assumption receives a certain degree
of support from the observed fact that the natural features of the moon
are framed on an exaggerated scale as compared with the earth's. We have
just observed that the moon is characterized by vast mountain rings,
attaining in many cases a diameter exceeding fifty miles. If these are
volcanic craters, it is evident, at a glance, that the mightiest
volcanoes of the earth fall into insignificance beside them. Now, the
slight force of gravity on the moon has been appealed to as a reason why
volcanic explosions on the lunar globe should produce incomparably
greater effects than upon the earth, where the ejected materials are so
much heavier. The same force that would throw a volcanic bomb a mile
high on the earth could throw it six miles high on the moon. The giant
cannon that we have placed in one of our coast forts, which is said to
be able to hurl a projectile to a distance of fifteen miles, could send
the same projectile ninety miles on the moon. An athlete who can clear a
horizontal bar at a height of six feet on the earth could clear the same
bar at a height of thirty-six feet on the moon. In other words, he could
jump over a house, unless, indeed, the lunarians really are giants, and
live in houses proportioned to their own dimensions and to the size of
their mountains. In that case, our athlete would have to content himself
with jumping over a lunarian, whose head he could just clear--with the
hat off.

These things are not only amusing, but important. There can be no
question that the force of gravity on the moon actually is as slight as
it has just been described. So, even without calling in imaginary
inhabitants to lend it interest, the comparative inability of the moon
to arrest bodies in motion becomes a fact of much significance. It has
led to the theory that meteorites may have originally been shot out of
the moon's great volcanoes, when those volcanoes were active, and may
have circulated about the sun until various perturbations have brought
them down upon the earth. A body shot radially from the surface of the
moon would need to have a velocity of only about a mile and a half in a
second in order to escape from the moon's control, and we can believe
that a lunar volcano when in action could have imparted such a velocity,
all the more readily because with modern gunpowders we have been able to
give to projectiles a speed one half as great as that needed for
liberation from lunar gravity.

Another consequence of the small gravitative power of the moon bears
upon the all-important question of atmosphere. According to the theory
of Dr. Johnstone Stoney, heretofore referred to, oxygen, nitrogen, and
water vapor would all gradually escape from the moon, if originally
placed upon it, because, by the kinetic theory, the maximum velocities
of their molecules are greater than a mile and a half per second. The
escape would not occur instantly, nor all at once, for it would be only
the molecules at the upper surface of the atmosphere which were moving
with their greatest velocity, and in a direction radial to the center of
the moon, that would get away; but in the course of time this gradual
leakage would result in the escape of all of those gases.[16]

[Footnote 16: The discovery of free hydrogen in the earth's atmosphere,
by Professor Dewar, 1901, bears upon the theory of the escape of gases
from a planet, and may modify the view above expressed. Since hydrogen
is theoretically incapable of being permanently retained in the free
state by the earth, its presence in the atmosphere indicates either that
there is an influx from space or that it emanates from the earth's
crust. In a similar way it may be assumed that atmospheric gases can be
given off from the crust of the moon, thus, to a greater or less extent,
supplying the place of the molecules that escape.]

After it had been found that, to ordinary tests, the moon offered no
evidence of the possession of an atmosphere, and before Dr. Stoney's
theory was broached, it was supposed by many that the moon had lost its
original supply of air by absorption into its interior. The oxygen was
supposed to have entered into combination with the cooling rocks and
minerals, thus being withdrawn from the atmosphere, and the nitrogen was
imagined to have disappeared also within the lunar crust. For it seems
to have always been tacitly assumed that the phenomenon to be accounted
for was not so much the _absence_ of a lunar atmosphere as its
_disappearance_. But disappearance, of course, implies previous
existence. In like manner it has always been a commonly accepted view
that the moon probably once had enough water to form lakes and seas.

These, it has been calculated, could have been absorbed into the lunar
globe as it cooled off. But Johnstone Stoney's theory offers another
method by which they could have escaped, through evaporation and the
gradual flight of the molecules into open space. Possibly both methods
have been in operation, a portion of the constituents of the former
atmosphere and oceans having entered into chemical combinations in the
lunar crust, and the remainder having vanished in consequence of the
lack of sufficient gravitative force to retain them.

But why, it may be asked, should it be assumed that the moon ever had
things which it does not now possess? Perhaps no entirely satisfactory
reply can be made. Some observers have believed that they detected
unmistakable indications of alluvial deposits on lunar plains, and of
the existence of beaches on the shores of the "seas." Messrs. Loewy and
Puiseux, of the Paris Observatory, whose photographs of the moon are
perhaps the finest yet made, say on this subject:

"There exists, from the point of view of relief, a general similarity
between the 'seas' of the moon and the plateaux which are covered to-day
by terrestrial oceans. In these convex surfaces are more frequent than
concave basins, thrown back usually toward the verge of the depressed
space. In the same way the 'seas' of the moon present, generally at the
edges, rather pronounced depressions. In one case, as in the other, we
observe normal deformations of a shrinking globe shielded from the
erosive action of rain, which tends, on the contrary, in all the
abundantly watered parts of the earth to make the concave surfaces
predominate. The explanation of this structure, such as is admitted at
present by geologists, seems to us equally valid for the moon."[17]

[Footnote 17: Comptes Rendus, June 26, July 3, 1899.]

It might be urged that there is evidence of former volcanic activity on
the moon of such a nature that explosions of steam must have played a
part in the phenomena, and if there was steam, of course there was
water.

But perhaps the most convincing argument tending to show that the moon
once had a supply of water, of which some remnant may yet remain below
the surface of the lunar globe, is based upon the probable similarity in
composition of the earth and the moon. This similarity results almost
equally whether we regard the moon as having originated in a ring of
matter left off from the contracting mass that became the earth, or
whether we accept the suggestion of Prof. G.H. Darwin, that the moon is
the veritable offspring of the earth, brought into being by the
assistance of the tidal influence of the sun. The latter hypothesis is
the more picturesque of the two, and, at present, is probably the more
generally favored. It depends upon the theory of tidal friction, which
was referred to in Chapter III, as offering an explanation of the manner
in which the rotation of the planet Mercury has been slowed down until
its rotary period coincides with that of its revolution.

The gist of the hypothesis in question is that at a very early period in
its history, when the earth was probably yet in a fluid condition, it
rotated with extreme rapidity on its axis, and was, at the same time,
greatly agitated by the tidal attraction of the sun, and finally huge
masses were detached from the earth which, ultimately uniting, became
the moon.[18]

[Footnote 18: The Tides, by G.H. Darwin, chapter xvi.]

Born in this manner from the very substance of the earth, the moon would
necessarily be composed, in the main, of the same elements as the globe
on which we dwell, and is it conceivable that it should not have carried
with it both air and water, or the gases from which they were to be
formed? If the moon ever had enough of these prime requisites to enable
it to support forms of life comparable with those of the earth, the
disappearance of that life must have been a direct consequence of the
gradual vanishing of the lunar air and water. The secular drying up of
the oceans and wasting away of the atmosphere on our little neighbor
world involved a vast, all-embracing tragedy, some of the earlier scenes
of which, if theories be correct, are now reenacted on the
half-desiccated planet Mars--a planet, by the way, which in size, mass,
and ability to retain vital gases stands about half-way between the
earth and the moon.

One of the most interesting facts about the moon is that its surface
affords evidence of a cataclysm which has wiped out many, and perhaps
nearly all, of the records of its earlier history, that were once
written upon its face. Even on the earth there have been geological
catastrophes destroying or burying the accumulated results of ages of
undisturbed progress, but on the moon these effects have been
transcendent. The story of the tremendous disaster that overtook the
moon is partly written in its giant volcanoes. Although it may be true,
as some maintain, that there is yet volcanic action going on upon the
lunar surface, it is evident that such action must be insignificant in
comparison with that which took place ages ago.

There is a spot in the western hemisphere of the moon, on the border of
a placid bay or "sea," that I can never look at without a feeling of awe
and almost of shrinking. There, within a space about 250 miles in length
by 100 in width, is an exhibition of the most terrifying effects of
volcanic energy that the eye of man can anywhere behold. Three immense
craters--Theophilus, 64 miles across and 3-1/2 miles deep; Cyrillus, 60
miles across and 15,000 feet deep; and Catharina, 70 miles across and
from 8,000 to 16,000 feet deep--form an interlinked chain of mountain
rings, ridges, precipices, chasms, and bottomless pits that take away
one's breath.

But when the first impression of astonishment and dismay produced by
this overwhelming spectacle has somewhat abated, the thoughtful observer
will note that here the moon is telling him a part of her wonderful
story, depicted in characters so plain that he needs no instruction in
order to decipher their meaning. He will observe that this ruin was not
all wrought at once or simultaneously. Theophilus, the crater-mountain
at the northwestern end of the chain, whose bottom lies deepest of all,
is the youngest of these giants, though the most imposing. For a
distance of forty miles the lofty wall of Theophilus has piled itself
upon the ruins of the wall of Cyrillus, and the circumference of the
circle of its tremendous crater has been forcibly thrust within the
original rim of the more ancient crater, which was thus rudely compelled
to make room for its more vigorous rival and successor.

The observer will also notice that Catharina, the huge pit at the
southeastern end of the chain, bears evidence of yet greater age. Its
original walls, fragments of which still stand in broken grandeur,
towering to a height of 16,000 feet, have, throughout the greater part
of their circuit, been riddled by the outbreak of smaller craters, and
torn asunder and thrown down on all sides.

In the vast enclosure that was originally the floor of the
crater-mountain Catharina, several crater rings, only a third, a
quarter, or a fifth as great in diameter, have broken forth, and these
in turn have been partially destroyed, while in the interior of the
oldest of them yet smaller craters, a nest of them, mere Etnas,
Cotopaxis, and Kilaueas in magnitude, simple pinheads on the moon, have
opened their tiny jaws in weak and ineffective expression of the waning
energies of a still later epoch, which followed the truly heroic age of
lunar vulcanicity.

This is only one example among hundreds, scattered all over the moon,
which show how the surface of our satellite has suffered upheaval after
upheaval. It is possible that some of the small craters, not included
within the walls of the greater ones, may represent an early stage in
the era of volcanic activity that wrecked the moon, but where larger and
smaller are grouped together a certain progression can be seen, tending
finally to extinction. The internal energies reached a maximum and then
fell off in strength until they died out completely.

It can hardly be supposed that the life-bearing phase of lunar
history--if there ever was one--could survive the outbreak of the
volcanic cataclysm. North America, or Europe, if subjected to such an
experience as the continental areas of the moon have passed through,
would be, in proportion, worse wrecked than the most fearfully battered
steel victim of a modern sea fight, and one can readily understand that,
in such circumstances, those now beautiful and populous continents would
exhibit, from a distance, scarcely any token of their present
topographical features, to say nothing of any relics of their occupation
by living creatures.

There are other interesting glimpses to be had of an older world in the
moon than that whose scarred face is now beautified for us by distance.
Not far from Theophilus and the other great crater-mountains just
described, at the upper, or southern, end of the level expanse called
the "Sea of Nectar," is a broad, semicircular bay whose shores are
formed by the walls of a partially destroyed crater named Fracastorius.
It is evident that this bay, and the larger part of the "Sea of Nectar,"
have been created by an outwelling of liquid lavas, which formed a
smooth floor over a portion of the pre-existing surface of the moon, and
broke down and submerged a large part of the mountain ring of
Fracastorius, leaving the more ancient walls standing at the southern
end, while, outlined by depressions and corrugations in the rocky
blanket, are certain half-defined forms belonging to the buried world
beneath.

Near Copernicus, some years ago, as Dr. Edward S. Holden pointed out,
photographs made with the great Lick telescope, then under his
direction, showed, in skeleton outline, a huge ring buried beneath some
vast outflow of molten matter and undiscerned by telescopic observers.
And Mr. Elger, who was a most industrious observer and careful
interpreter of lunar scenery, speaks of "the undoubted existence of the
relics of an earlier lunar world beneath the smooth superficies of the
_maria_."

Although, as already remarked, it seems necessary to assume that any
life existing in the moon prior to its great volcanic outburst must have
ceased at that time, yet the possibility may be admitted that life could
reappear upon the moon after its surface had again become quiet and
comparatively undisturbed. Germs of the earlier life might have
survived, despite the terrible nature of the catastrophe. But the
conditions on the moon at present are such that even the most confident
advocates of the view that the lunar world is not entirely dead do not
venture to assume that anything beyond the lowest and simplest organic
forms--mainly, if not wholly, in the shape of vegetation--can exist
there. The impression that even such life is possible rests upon the
accumulating evidence of the existence of a lunar atmosphere, and of
visible changes, some apparently of a volcanic character and some not,
on the moon's surface.

Prof. William H. Pickering, who is, perhaps, more familiar with the
telescopic and photographic aspects of the moon than any other American
astronomer, has recorded numberless instances of change in minute
details of the lunar landscapes. He regards some of his observations
made at Arequipa as "pointing very strongly to the existence of
vegetation upon the surface of the moon in large quantities at the
present time." The mountain-ringed valley of Plato is one of the places
in the lunar world where the visible changes have been most frequently
observed, and more than one student of the moon has reached the
conclusion that something very like the appearances that vegetation
would produce is to be seen in that valley.

Professor Pickering has thoroughly discussed the observations relating
to a celebrated crater named Linné in the _Mare Serenitatis_, and after
reading his description of its changes of appearance one can hardly
reject his conclusion that Linné is an active volcanic vent, but
variable in its manifestations. This is only one of a number of similar
instances among the smaller craters of the moon. The giant ones are
evidently entirely extinct, but some of the minor vents give occasional
signs of activity. Nor should it be assumed that these relatively slight
manifestations of volcanic action are really insignificant. As Professor
Pickering shows, they may be regarded as comparable with the greatest
volcanic phenomena now witnessed on the earth, and, speaking again of
Plato, he says of its evidences of volcanic action:

"It is, I believe, more active than any area of similar size upon the
earth. There seems to be no evidences of lava, but the white streaks
indicate apparently something analogous to snow or clouds. There must be
a certain escape of gases, presumably steam and carbonic acid, the
former of which, probably, aids in the production of the white
markings."[19]

[Footnote 19: Annals of Harvard College Observatory, vol. xxxii, part
ii, 1900.]

To Professor Pickering we owe the suggestion that the wonderful rays
emanating from Tycho consist of some whitish substance blown by the
wind, not from Tycho itself, but from lines of little volcanic vents or
craters lying along the course of the rays. This substance may be
volcanic powder or snow, in the form of minute ice crystals. Mr. Elger
remarks of this theory that the "confused network of streaks" around
Copernicus seems to respond to it more happily than the rays of Tycho
do, because of the lack of definiteness of direction so manifest in the
case of the rays.

As an encouragement to amateur observers who may be disposed to find out
for themselves whether or not changes now take place in the moon, the
following sentence from the introduction to Professor Pickering's
chapter on Plato in the Harvard Observatory Annals, volume xxxii, will
prove useful and interesting:

"In reviewing the history of selenography, one must be impressed by the
singular fact that, while most of the astronomers who have made a
special study of the moon, such as Schroeter, Maedler, Schmidt, Webb,
Neison, and Elger, have all believed that its surface was still subject
to changes readily visible from the earth, the great majority of
astronomers who have paid little attention to the subject have quite as
strenuously denied the existence of such changes."

In regard to the lunar atmosphere, it may be said, in a word, that even
those who advocate the existence of vegetation and of clouds of dust or
ice crystals on the moon do not predicate any greater amount, or greater
density, of atmosphere than do those who consider the moon to be wholly
dead and inert. Professor Pickering himself showed, from his
observations, that the horizontal refraction of the lunar atmosphere,
instead of being less than 2´´, as formerly stated, was less than 0.4´´.
Yet he found visual evidence that on the sunlit side of the moon this
rare atmosphere was filled to a height of four miles with some absorbing
medium which was absent on the dark side, and which was apparently an
emanation from the lunar crust, occurring after sunrise. And Messrs.
Loewy and Puiseux, of the Paris Observatory, say, after showing reasons
for thinking that the great volcanic eruptions belong to a recent period
in the history of the moon, that "the diffusion of cinders to great
distances infers a gaseous envelope of a certain density.... The
resistance of the atmosphere must have been sufficient to retard the
fall of this dust [the reference is to the white trails, like those from
Tycho], during its transport over a distance of more than 1,000
kilometers [620 miles]."[20]

[Footnote 20: Comptes Rendus, June 23, July 3, 1899.]

We come now to a brief consideration of certain peculiarities in the
motions of the moon, and in the phenomena of day and night on its
surface. The moon keeps the same side forever turned toward the earth,
behaving, in this respect, as Mercury does with regard to the sun. The
consequence is that the lunar globe makes but one rotation on its axis
in the course of a month, or in the course of one revolution about the
earth. Some of the results of this practical identity of the periods of
rotation and revolution are illustrated in the diagram on page 250. The
moon really undergoes considerable libration, recalling the libration of
Mercury, which was explained in the chapter on that planet, and in
consequence we are able to see a little way round into the opposite
lunar hemisphere, now on this side and now on the other, but in the
diagram this libration has been neglected. If it had been represented we
should have found that, instead of only one half, about three fifths of
the total superficies of the moon are visible from the earth at one time
or another.

[Illustration: PHASES AND ROTATION OF THE MOON.]

Perhaps it should be remarked that in drawing the moon's orbit about the
earth as a center we offer no contradiction to what was shown earlier
in this chapter. The moon does travel around the earth, and its orbit
about our globe may, for our present purpose, be treated independently
of its motion about the sun. Let the central globe, then, represent the
earth, and let the sun be supposed to shine from the left-hand side of
the diagram. A little cross is erected at a fixed spot on the globe of
the moon.

At _A_ the moon is between the earth and the sun, or in the phase of new
moon. The lunar hemisphere facing the earth is now buried in night,
except so far as the light reflected from the earth illuminates it, and
this illumination, it is interesting to remember, is about fourteen
times as great--reckoned by the relative areas of the reflecting
surfaces--as that which the full moon sends to the earth. An inhabitant
of the moon, standing beside the cross, sees the earth in the form of a
huge full moon directly above his head, but, as far as the sun is
concerned, it is midnight for him.

In the course of about seven days the moon travels to _B_. In the
meantime it has turned one quarter of the way around its axis, and the
spot marked by the cross is still directly under the earth. For the
lunar inhabitant standing on that spot the sun is now on the point of
rising, and he sees the earth no longer in the shape of a full moon, but
in that of a half-moon. The lunar globe itself appears, at the same
time from the earth, as a half-moon, being in the position or phase that
we call first quarter.

Seven more days elapse, and the moon arrives at _C_, opposite to the
position of the sun, and with the earth between it and the solar orb. It
is now high noon for our lunarian standing beside the cross, while the
earth over his head appears, if he sees it at all, only as a black disk
close to the sun, or--as would sometimes be the case--covering the sun,
and encircled with a beautiful ring of light produced by the refraction
of its atmosphere. (Recall the similar phenomenon in the case of Venus.)
The moon seen from the earth is now in the phase called full moon.

Another lapse of seven days, and the moon is at _D_, in the phase called
third quarter, while the earth, viewed from the cross on the moon, which
is still pointed directly at it, appears again in the shape of a huge
half-moon.

During the next seven days the moon returns to its original position at
_A_, and becomes once more new moon, with "full earth" shining upon it.

Now it is evident that in consequence of the peculiar law of the moon's
rotation its days and nights are each about two of our weeks, or
fourteen days, in length. That hemisphere of the moon which is in the
full sunlight at _A_, for instance, is buried in the middle of night at
_C_. The result is different than in the case of Mercury, because the
body toward which the moon always keeps the same face directed is not
the luminous sun, but the non-luminous earth.

It is believed that the moon acquired this manner of rotation in
consequence of the tidal friction exercised upon it by the earth. The
tidal attraction of the earth exceeds that of the sun upon the moon
because the earth is so much nearer than the sun is, and tidal
attraction varies inversely as the cube of the distance. In fact, the
braking effect of tidal friction varies inversely as the sixth power of
the distance, so that the ability of the earth to stop the rotation of
the moon on its axis is immensely greater than that of the sun. This
power was effectively applied while the moon was yet a molten mass, so
that it is probable that the moon has rotated just as it does now for
millions of years.

As was remarked a little while ago, the moon traveling in an elliptical
orbit about the earth has a libratory movement which, if represented in
our picture, would cause the cross to swing now a little one way and now
a little the other, and thus produce an apparent pendulum motion of the
earth in the sky, similar to that of the sun as seen from Mercury. But
it is not necessary to go into the details of this phenomenon. The
reader, if he chooses, can deduce them for himself.

But we may inquire a little into the effects of the long days and nights
of the moon. In consequence of the extreme rarity of the lunar
atmosphere, it is believed that the heat of the sun falling upon it
during a day two weeks in length, is radiated away so rapidly that the
surface of the lunar rocks never rises above the freezing temperature
of water. On the night side, with no warm atmospheric blanket such as
the earth enjoys, the temperature may fall far toward absolute zero, the
most merciful figure that has been suggested for it being 200° below the
zero of our ordinary thermometers! But there is much uncertainty about
the actual temperature on the moon, and different experiments, in the
attempt to make a direct measurement of it, have yielded discordant
results. At one time, for instance, Lord Rosse believed he had
demonstrated that at lunar noon the temperature of the rocks rose above
the boiling-point of water. But afterward he changed his mind and
favored the theory of a low temperature.

In this and in other respects much remains to be discovered concerning
our interesting satellite, and there is plenty of room, and an abundance
of original occupation, for new observers of the lunar world.




CHAPTER IX

HOW TO FIND THE PLANETS


There is no reason why everybody should not know the principal planets
at sight nearly as well as everybody knows the moon. It only requires a
little intelligent application to become acquainted with the other
worlds that have been discussed in the foregoing chapters, and to be
able to follow their courses through the sky and recognize them wherever
they appear. No telescope, or any other instrument whatever, is required
for the purpose. There is but one preliminary requirement, just as every
branch of human knowledge presupposes its A B C. This is an acquaintance
with the constellations and the principal stars--not a difficult thing
to obtain.

Almost everybody knows the "Great Dipper" from childhood's days,
except, perhaps, those who have had the misfortune to spend their youth
under the glare of city lights. Some know Orion when he shines
gloriously in the winter heavens. Many are able to point out the north
star, or pole star, as everybody should be able to do. All this forms a
good beginning, and may serve as the basis for the rapid acquirement of
a general knowledge of the geography of the heavens.

If you are fortunate enough to number an astronomer among your
acquaintance--an amateur will do as well as a professor--you may, with
his aid, make a short cut to a knowledge of the stars. Otherwise you
must depend upon books and charts. My Astronomy with an Opera-Glass was
prepared for this very purpose. For simply learning the constellations
and the chief stars you need no opera-glass or other instrument. With
the aid of the charts, familiarize yourself with the appearance of the
constellations by noticing the characteristic arrangements of their
chief stars. You need pay no attention to any except the bright stars,
and those that are conspicuous enough to thrust themselves upon your
attention.

Learn by observation at what seasons particular constellations are on,
or near, the meridian--i.e., the north and south line through the middle
of the heavens. Make yourself especially familiar with the so-called
zodiacal constellations, which are, in their order, running around the
heavens from west to east: Aries, Taurus, Gemini, Cancer, Leo, Virgo,
Libra, Scorpio, Sagittarius, Capricornus, Aquarius, and Pisces. The
importance of these particular constellations arises from the fact that
it is across them that the tracks of the planets lie, and when you are
familiar with the fixed stars belonging to them you will be able
immediately to recognize a stranger appearing among them, and will
correctly conclude that it is one of the planets.[21] How to tell
which planet it may be, it is the object of this chapter to show you. As
an indispensable aid--unless you happen already to possess a complete
star atlas on a larger scale--I have drawn the six charts of the
zodiacal constellations and their neighbors that are included in this
chapter.

[Footnote 21: In our latitudes, planets are never seen in the northern
quarter of the sky. When on the meridian, they are always somewhere
between the zenith and the southern horizon.]

[Illustration: CHART NO. 1.--FROM RIGHT ASCENSION 0 HOURS TO 4 HOURS;
DECLINATION 30° NORTH TO 10° SOUTH.]

Having learned to recognize the constellations and their chief stars on
sight, one other step, an extremely easy one, remains to be taken before
beginning your search for the planets--buy the American Ephemeris and
Nautical Almanac for the current year. It is published under the
direction of the United States Naval Observatory at Washington, and can
be purchased for one dollar.

This book, which may appear to you rather bulky and formidable for an
almanac, contains hundreds of pages and scores of tables to which you
need pay no attention. They are for navigators and astronomers, and are
much more innocent than they look. The plain citizen, seeking only an
introduction to the planets, can return their stare and pass by,
without feeling in the least humiliated.

[Illustration: CHART NO. 2.--FROM RIGHT ASCENSION 4 HOURS TO 8 HOURS;
DECLINATION 30° NORTH TO 10° SOUTH.]

In the front part of the book, after the long calendar, and the tables
relating to the sun and the moon, will be found about thirty pages of
tables headed, in large black letters, with the names of the
planets--Mercury, Venus, Mars, Jupiter, Saturn, etc. Two months are
represented on each page, and opposite the number of each successive day
of the month the position of the planet is given in hours, minutes, and
seconds of right ascension, and degrees, minutes, and seconds of north
and south declination, the sign + meaning north, and the sign - south.
Do not trouble yourself with the seconds in either column, and take the
minutes only when the number is large. The hours of right ascension and
the degrees of declination are the main things to be noticed.

Right ascension, by the way, expresses the distance of a celestial body,
such as a star or a planet, east of the vernal equinox, or the first
point of Aries, which is an arbitrary point on the equator of the
heavens, which serves, like the meridian of Greenwich on the earth, as a
starting-place for reckoning longitude. The entire circuit of the
heavens along the equator is divided into twenty-four hours of right
ascension, each hour covering 15° of space. If a planet then is in right
ascension (usually printed for short R.A.) 0 h. 0 m. 0 s., it is on the
meridian of the vernal equinox, or the celestial Greenwich; if it is in
R.A. 1 h., it will be found 15° east of the vernal equinox, and so on.

[Illustration: CHART NO. 3.--FROM RIGHT ASCENSION 8 HOURS TO 12 HOURS;
DECLINATION 30° NORTH TO 10° SOUTH.]

Declination (printed D. or Dec.) expresses the distance of a celestial
body north or south of the equator of the heavens.

With these explanations we may proceed to find a planet by the aid of
the Nautical Almanac and our charts. I take, for example, the ephemeris
for the year 1901, and I look under the heading "Jupiter" on page 239,
for the month of July. Opposite the 15th day of the month I find the
right ascension to be 18 h. 27 m., neglecting the seconds. Now 27
minutes are so near to half an hour that, for our purposes, we may say
Jupiter is in R.A. 18 h. 30 m. I set this down on a slip of paper, and
then examine the declination column, where I find that on July 15
Jupiter is in south declination (the sign - meaning south, as before
explained) 23° 17´ 52´´, which is almost 23° 18´, and, for our purposes,
we may call this 23° 20´, which is what I set down on my slip.

[Illustration: CHART NO. 4.--FROM RIGHT ASCENSION 12 HOURS TO 16 HOURS;
DECLINATION 10° NORTH TO 30° SOUTH.]

Next, I turn to Chart No. 5, in this chapter, where I find the meridian
line of R.A. 18 h. running through the center of the chart. I know that
Jupiter is to be looked for about 30 m. east, or to the left, of that
line. At the bottom and top of the chart, every twenty minutes of R.A.
is indicated, so that it is easy, with the eye, or with the aid of a
ruler, to place the vertical line at some point of which Jupiter is to
be found.

[Illustration: CHART NO. 5.--FROM RIGHT ASCENSION 16 HOURS TO 20 HOURS;
DECLINATION 10° NORTH TO 30° SOUTH.]

Then I consult my note of the declination of the planet. It is south 23°
20´. On the vertical borders of the chart I find the figures of the
declination, and I observe that 0° Dec., which represents the equator of
the heavens, is near the top of the chart, while each parallel
horizontal line across the chart indicates 10° north or south of its
next neighbor. Next to the bottom of the chart I find the parallel of
20°, and I see that every five degrees is indicated by the figures at
the sides. By the eye, or with the aid of a ruler, I easily estimate
where the horizontal line of 23° would fall, and since 20´ is the third
of a degree I perceive that it is, for the rough purpose of merely
finding a conspicuous planet, negligible, although it, too, can be
included in the estimate, if thought desirable.

Having already found the vertical line on which Jupiter is placed and
having now found the horizontal line also, I have simply to regard their
crossing point, which will be the situation of the planet among the
stars. I note that it is in the constellation Sagittarius in a certain
position with reference to a familiar group of stars in that
constellation, and when I look at the heavens, there, in the place thus
indicated, Jupiter stands revealed.

[Illustration: CHART NO. 6.--FROM RIGHT ASCENSION 20 HOURS TO 24 HOURS
(0 II.); DECLINATION 10° NORTH TO 30° SOUTH.]

The reader will readily perceive that, in a precisely similar manner,
any planet can be located, at any time of the year, and at any point in
its course about the heavens. But it may turn out that the place
occupied by the planet is too near the sun to render it easily, or at
all, visible. Such a case can be recognized, either from a general
knowledge of the location of the constellations at various seasons, or
with the aid of the Nautical Almanac, where at the beginning of each set
of monthly tables in the calendar the sun's right ascension and
declination will be found. In locating the sun, if you find that its
right ascension differs by less than an hour, one way or the other, from
that of the planet sought, it is useless to look for the latter. If the
planet is situated west of the sun--to the right on the chart--then it
is to be looked for in the east before sunrise. But if it is east of the
sun--to the left on the chart--then you must seek it in the west after
sunset.

For instance, I look for the planet Mercury on October 12, 1901. I find
its R.A. to be 14 h. 40 m. and its Dec. 18° 36´. Looking at the sun's
place for October 12th, I find it to be R.A. 13 h. 8 m. and Dec. 7° 14´.
Placing them both on Chart No. 4, I discover that Mercury is well to the
east, or left hand of the sun, and will consequently be visible in the
western sky after sundown.

Additional guidance will be found by noting the following facts about
the charts:

The meridian (the north and south line) runs through the middle of Chart
No. 1 between 11 and 12 o'clock P.M. on November 1st, between 9 and 10
o'clock P.M. on December 1st, and between 7 and 8 o'clock P.M. on
January 1st.

The meridian runs through the middle of Chart No. 2 between 11 and 12
o'clock P.M. on January 1st, between 9 and 10 o'clock P.M. on February
1st, and between 7 and 8 o'clock P.M. on March 1st.

The meridian runs through the middle of Chart No. 3 between 11 and 12
o'clock P.M. on March 1st, between 9 and 10 o'clock P.M. on April 1st,
and between 7 and 8 o'clock P.M. on May 1st.

The meridian runs through the middle of Chart No. 4 between 11 and 12
o'clock P.M. on May 1st, between 9 and 10 o'clock P.M. on June 1st, and
between 7 and 8 o'clock P.M. on July 1st.

The meridian runs through the middle of Chart No. 5 between 11 and 12
o'clock P.M. on July 1st, between 9 and 10 o'clock P.M. on August 1st,
and between 7 and 8 o'clock P.M. on September 1st.

The meridian runs through the middle of Chart No. 6 between 11 and 12
o'clock P.M. on September 1st, between 9 and 10 o'clock P.M. on October
1st, and between 7 and 8 o'clock P.M. on November 1st.

Note well, also, these particulars about the charts: Chart No. 1
includes the first four hours of right ascension, from 0 h. to 4 h.
inclusive; Chart No. 2 includes 4 h. to 8 h.; Chart No. 3, 8 h. to 12
h.; Chart No. 4, 12 h. to 16 h.; Chart No. 5, 16 h. to 20 h.; and Chart
No. 6, 20 h. to 24 h., which completes the circuit. In the first three
charts the line of 0°, or the equator, is found near the bottom, and in
the last three near the top. This is a matter of convenience in
arrangement, based upon the fact that the ecliptic, which, and not the
equator, marks the center of the zodiac, indicates the position of the
tracks of the planets among the stars; and the ecliptic, being inclined
23° to the plane of the equator, lies half to the north and half to the
south of the latter.

Those who, after all, may not care to consult the ephemeris in order to
find the planets, may be able to locate them, simply from a knowledge of
their situation among the constellations. Some ordinary almanacs tell in
what constellations the principal planets are to be found at various
times of the year. Having once found them in this way, it is
comparatively easy to keep track of them thereafter through a general
knowledge of their movements. Jupiter, for instance, requiring a period
of nearly twelve years to make a single journey around the sun, moves
about 30° eastward among the stars every year. The zodiacal
constellations are roughly about 30° in length, and as Jupiter was in
Sagittarius in 1901, he will be in Capricornus in 1902. Saturn,
requiring nearly thirty years for a revolution around the sun, moves
only between 12° and 13° eastward every year, and, being in conjunction
with Jupiter in Sagittarius in 1901, does not get beyond the border of
that constellation in 1902.

Jupiter having been in opposition to the sun June 30, 1901, will be
similarly placed early in August, 1902, the time from one opposition of
Jupiter to the next being 399 days.

Saturn passes from one opposition to the next in 378 days, so that
having been in that position July 5, 1901, it reaches it again about
July 18, 1902.

Mars requires about 687 days to complete a revolution, and comes into
conjunction with the earth, or opposition to the sun--the best position
for observation--on the average once every 780 days. Mars was in
opposition near the end of February, 1901, and some of its future
oppositions will be in March, 1903; May, 1905; July, 1907; and
September, 1909. The oppositions of 1907 and 1909 will be unusually
favorable ones, for they will occur when the planet is comparatively
near the earth. When a planet is in opposition to the sun it is on the
meridian, the north and south line, at midnight.

Mercury and Venus being nearer the sun than the earth is, can never be
seen very far from the place of the sun itself. Venus recedes much
farther from the solar orb than Mercury does, but both are visible only
in the sunset or the sunrise sky. All almanacs tell at what times these
planets play their respective rôles as morning or as evening stars. In
the case of Mercury about 116 days on the average elapse between its
reappearances; in the case of Venus, about 584 days. The latter, for
instance, having become an evening star at the end of April, 1901, will
become an evening star again in December, 1902.

With the aid of the Nautical Almanac and the charts the amateur will
find no difficulty, after a little practise, in keeping track of any of
the planets.

In the back part of the Nautical Almanac will be found two pages headed
"Phenomena: Planetary Configurations." With the aid of these the student
can determine the position of the planets with respect to the sun and
the moon, and with respect to one another. The meaning of the various
symbols used in the tables will be found explained on a page facing the
calendar at the beginning of the book. From these tables, among other
things, the times of greatest elongation from the sun of the planets
Mercury and Venus can be found.

It may be added that only bright stars, and stars easily seen, are
included in the charts, and there will be no danger of mistaking any of
these stars for a planet, if the observer first carefully learns to
recognize their configurations. Neither Mars, Jupiter, nor Saturn ever
appears as faint as any of the stars, except those of the first
magnitude, included in the charts. Uranus and Neptune being invisible to
the naked eye--Uranus can occasionally be just glimpsed by a keen
eye--are too faint to be found without the aid of more effective
appliances.




INDEX


Agassiz, Alexander, on deep-sea animals, 63.

Asteroids, the, 16, 129.
  brightness of, 130.
  imaginary adventures on, 146.
  life on, 144.
  number of, known, 129.
  orbits of, 132.
  origin of, 138, 143.
  size of, 129.

Aristarchus, lunar crater, 226.

Atmosphere, importance of, 20.


Bailey, Solon I., on oppositions of Eros, 134.

Barnard, E.E., discovers fifth satellite of Jupiter, 181.
  measures asteroids, 129.
  on Saturn's rings, 205.

Belopolski, on rotation of Venus, 79.


Ceres, an asteroid, 129, 130.

Clefts in the moon, 226.

Copernicus, lunar crater, 223, 242.


Darwin, George H., on Jupiter and Saturn, 206.
  on origin of moon, 235.
  theory of tidal friction, 32.

Davy, Sir Humphry, on Saturn, 190.

Dawes sees canals on Mars, 93.

Deimos, satellite of Mars, 125.

Denning, W.F., description of Jupiter, 175.

De Vico on rotation of Venus, 76.

Dewar, James, discovers free hydrogen in air, 232.

De Witt discovers Eros, 133.

Dick, Thomas, on Saturn, 201.

Douglass, A.E., sees Mars's canals, 92.
  sees clouds in Mars, 119.

Doppler's principle, 79, 200.


Earth and moon's orbit, 217.
  birth of moon from, 236.
  change of distance from sun, 27.
  less advanced than Mars, 89.
  older than Venus, 58.
  seen from Mercury, 41.
  seen from Venus, 69-71, 75.
  seen from moon, 214.

Earth, similarity to Venus, 46.
  supposed signals to and from Mars, 110.

Elger, T.G., on cracks in moon, 227.
  on Tycho's rays, 246.

Ephemeris, how to use, 260, 264.

Eros, an asteroid, 131-134, 136, 137.


Flammarion, C., observes Venus's atmosphere, 56.
  on plurality of worlds, 8.

Forbes, Prof. George, on ultra-Neptunian planet, 210.


Galileo on lunar world, 215.

Gravity, as affecting life on planets, 20, 46.


Hall, Asaph, discovers Mars's moons, 90.

Herodotus, lunar crater, 227.

Herschel, Sir John, on Saturn, 185.

Holden, E.S., on photograph of lunar crater, 242.

Huggins on Mercury's atmosphere, 21.


Inhabitants of foreign planets, 1, 4, 5.

Interplanetary communication, 1, 3, 72, 110, 112.


Juno, an asteroid, 129.

Jupiter, cloudy aspect of, 165.
  density of, 162.
  distance of, 161.
  equatorial belts on, 165.
  future of, 180.
  gravity on, 162.
  great red spot on, 169.
  markings outside the belts, 168.
  and the nebular theory, 178.
  once a companion star, 179.
  polar compression of, 161.
  possibly yet incandescent, 177.
  question of a denser core, 176.
  resemblance of, to sun, 174.
  rotation of, 161, 173.
  satellites of, 166, 181.
  seen from satellites, 182.
  size of, 160.
  solar light and heat on, 182.
  south belt of, 172.
  surface conditions of, 163.
  theories about the red spot, 170.
  trade-winds and the belts of, 167.
  various rates of rotation of, 173.
  visibility of rotation of, 166.


Keeler, J.E., on Saturn's rings, 200.

Kepler, lunar crater, 223.

Kinetic theory of gases, 116.

Kirkwood, Daniel, on asteroids, 131.


Lagrange on Olbers's theory, 139.

Lick Observatory and Mars's canals, 92.

Life, a planetary phenomenon, 10.
  in sea depths, 62.
  on planets, 62, 63.
  prime requisites of, 64.
  resisting extreme cold, 123.
  universality of, 9.

Loewy and Puiseux, on lunar atmosphere, 248.
  on lunar "seas," 234.

Lowell, Percival, description of Mars, 108.
  on markings of Venus, 60.
  on Mercury's rotation, 33.
  on rotation of Venus, 77.
  sees Mars's canals, 92.
  theory of Martian canals, 101.

Lucian, on appearance of earth from moon, 213.

Lyman, C.S., observes Venus's atmosphere, 55.


Mars, age of, 89.
  atmosphere of, 86, 115, 117.
  bands of life on, 104.
  canals on, 90.
    described by Schiaparelli, 93.
    gemination of, 91, 105.
    have builders of, disappeared? 107.
    and irrigation, 101.
    and lines of vegetation, 102.
    and seasonal changes, 99.
    and water circulation, 100.
  carbon dioxide on, 118.
  circular spots or "oases" on, 103.
  colors of, 89.
  dimensions of, 86.
  distance of, 85, 86.
  enigmatical lights on, 111.
  gravity on, 86.
  inclination of axis, 86.
  length of year, 86.
  Lowell's theory of, 101.
  light and heat on, 85.
  moonlight on, 128.
  orbit of, 85.
  polar caps of, 87, 118.
  possible size of inhabitants, 106.
  satellites of, 90, 124, 126.
  seasons on, 87.
  supposed signals from, 110, 112.
  temperature of, 120, 122.
  water vapor on, 117.

Mercury, atmosphere of, 21, 28, 43, 44.
  day and night on, 34, 38, 40.
  dimensions, 18.
  earth seen from, 41.
  habitability of, 33, 40, 44.
  heavens seen from, 41, 42.
  heat and light on, 25, 28.
  holds place of honor, 19.
  length of year, 24.
  mass of, 19.
  moon visible from, 41.
  resemblances to moon, 43.
  rotation of, 30.
  shape of orbit, 23.
  sun as seen from, 37.
  velocity in orbit, 23.
  Venus seen from, 41.
  virtual fall toward sun, 24.
  visibility of, 21.
  water on, 43.

Moon, the area of surface, 219.
  atmosphere of, 7, 215, 231, 247, 248.
  clouds on, 6, 245.
  constitution of, 236.
  craters, 221.
  day and night on, 254.
  distance of, 212, 215.
  density of, 219.
  former cataclysm on, 237.
  former life on, 241, 243.
  giantism on, 228, 229.
  gravity on, 219, 228, 229.
  libration of, 249.
  meteorites and, 230.
  mountains on, 220.
  the older world in, 242.
  origin of, 235.
  phases and motions of, 250.
  rotation of, 249.
  seas of, 234.
  size of, 218.
  snow on, 246.
  speculation about, 212.
  temperature of, 255.
  vegetation on, 6, 244, 247.
  visibility of features of, 213.


Nasmyth and Carpenter on lunar craters, 224.

Neptune, description of, 208-210.

Newcomb, Simon, on Olbers's theory, 141.

Newton, lunar crater, 222.


Olbers's theory of planetary explosion, 138.
  on Vesta's light, 138.


Pallas, an asteroid, 129.

Perrotin sees canals on Mars, 92.

Phobos, satellite of Mars, 125.

Pickering, E.C., discovers ninth moon of Saturn, 195.
  finds Eros on Harvard plates, 133.
  on shape of Eros, 136.
  on light of Eros, 137.

Pickering, W.H., on lunar atmosphere, 247.
  observes changes in moon, 244.
  sees Mars's canals, 92.
  theory of Tycho's rays, 246.
  on Venus's atmosphere, 54.

Planets, classification of, 15.
  how to find, 256, 273.
  resemblances among, 12.

Plato, lunar ring plain, 225.

Plurality of worlds in literature, 2.
  subject ignored, 8.

Proctor, R.A., on Jupiter's moons, 180.
  on other worlds, 8.

Roche's limit, 201.

Rosse, Lord, on temperature of moon, 255.


Saturn, age of, 189.
  composition of, 190.
  density of, 188.
  distance of, 186.
  the gauze ring, 199-202.
  gravity on, 188.
  inclination of axis, 187.
  interior of, 206.
  length of year, 186.
  popular telescopic object, 185.
  rings of, 185, 196.
    gaps in, 197.
    origin of, 200.
    periodic disappearance of, 198.
    seen from planet, 207.
    shadow of, 198.
  rotation of, 187.
  satellites of, 195.
  size of, 187.

Schiaparelli discovers canals on Mars, 90.
  describes Martian canals, 93.
  discovers Mercury's rotation, 30, 32.
  on rotation of Venus, 76.

Solar system, shape and size of, 14.
  unity of, 9.
  viewed from space, 11.

Stoney, Johnstone, on atmospheres of planets, 116.
  on escape of gases from moon, 231.

Sun, the, isolation in space, 13.
  no life on, 10.
  resemblances with Jupiter, 174.

Swedenborg, on Saturn's rings, 204.


Tidal friction, 80, 81, 236, 253.

Tycho, lunar crater, 222.


Ultra-Neptunian planet, 210.

Uranus, description of, 208-210.


Venus, age of, 58.
  atmosphere of, 53, 55, 59, 61, 68.
  absence of seasons on, 51.
  density of, 47.
  distance of, 47, 50.
  gravity on, 46, 47.
  inclination of axis, 50.
  life on, 57, 58, 61, 65, 67, 68, 82, 117.
  light and heat on, 50-57.
  orbit of, 50.
  phases of, 49.
  resemblances of, to earth, 46.
  rotation of, 76, 79, 80.
  size of, 46.
  twilight on, 83.
  visibility of, 47.

Vesta, an asteroid, 129, 130, 138.

Vogel on Mercury's atmosphere, 21.


Wireless telegraphy, 1, 112.


Young, C.A., on Olbers's theory of asteroids, 142.
  on temperature of Mars, 122.
  on Venus's atmosphere, 53.


Zodiac, the, 258.


THE END




A NEW BOOK BY PROF. GROOS.

The Play of Man.

By KARL GROOS, Professor of Philosophy in the University of Basel, and
author of "The Play of Animals." Translated, with the author's
cooperation, by Elizabeth L. Baldwin, and edited, with a Preface and
Appendix, by Prof. J. Mark Baldwin, of Princeton University. 12mo.
Cloth, $1.50 net; postage, 12 cents additional.

     The results of Professor Groos's original and acute investigations
     are of peculiar value to those who are interested in psychology and
     sociology, and they are of great importance to educators. He
     presents the anthropological aspects of the subject treated in his
     psychological study of the Play of Animals, which has already
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