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Round the Moon, A
Chapter XIII - Lunar Landscapes
Jules Verne
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       Chapter XIII - Lunar Landscapes
       At half-past two in the morning, the projectile was over the
       thirteenth lunar parallel and at the effective distance of five
       hundred miles, reduced by the glasses to five. It still seemed
       impossible, however, that it could ever touch any part of the disc.
       Its motive speed, comparatively so moderate, was inexplicable to
       President Barbicane. At that distance from the moon it must have
       been considerable, to enable it to bear up against her attraction.
       Here was a phenomenon the cause of which escaped them again.
       Besides, time failed them to investigate the cause. All lunar
       relief was defiling under the eyes of the travelers, and they
       would not lose a single detail.
       Under the glasses the disc appeared at the distance of five
       miles. What would an aeronaut, borne to this distance from the
       earth, distinguish on its surface? We cannot say, since the
       greatest ascension has not been more than 25,000 feet.
       This, however, is an exact description of what Barbicane and his
       companions saw at this height. Large patches of different
       colors appeared on the disc. Selenographers are not agreed upon
       the nature of these colors. There are several, and rather
       vividly marked. Julius Schmidt pretends that, if the
       terrestrial oceans were dried up, a Selenite observer could not
       distinguish on the globe a greater diversity of shades between
       the oceans and the continental plains than those on the moon
       present to a terrestrial observer. According to him, the color
       common to the vast plains known by the name of "seas" is a dark
       gray mixed with green and brown. Some of the large craters
       present the same appearance. Barbicane knew this opinion of the
       German selenographer, an opinion shared by Boeer and Moedler.
       Observation has proved that right was on their side, and not on
       that of some astronomers who admit the existence of only gray on
       the moon's surface. In some parts green was very distinct, such
       as springs, according to Julius Schmidt, from the seas of
       "Serenity and Humors." Barbicane also noticed large craters,
       without any interior cones, which shed a bluish tint similar to
       the reflection of a sheet of steel freshly polished. These colors
       belonged really to the lunar disc, and did not result, as some
       astronomers say, either from the imperfection in the objective
       of the glasses or from the interposition of the terrestrial atmosphere.
       Not a doubt existed in Barbicane's mind with regard to it, as he
       observed it through space, and so could not commit any optical error.
       He considered the establishment of this fact as an acquisition
       to science. Now, were these shades of green, belonging to
       tropical vegetation, kept up by a low dense atmosphere? He could
       not yet say.
       Farther on, he noticed a reddish tint, quite defined. The same
       shade had before been observed at the bottom of an isolated
       enclosure, known by the name of Lichtenburg's circle, which is
       situated near the Hercynian mountains, on the borders of the
       moon; but they could not tell the nature of it.
       They were not more fortunate with regard to another peculiarity
       of the disc, for they could not decide upon the cause of it.
       Michel Ardan was watching near the president, when he noticed
       long white lines, vividly lighted up by the direct rays of the sun.
       It was a succession of luminous furrows, very different from the
       radiation of Copernicus not long before; they ran parallel with
       each other.
       Michel, with his usual readiness, hastened to exclaim:
       "Look there! cultivated fields!"
       "Cultivated fields!" replied Nicholl, shrugging his shoulders.
       "Plowed, at all events," retorted Michel Ardan; "but what
       laborers those Selenites must be, and what giant oxen they must
       harness to their plow to cut such furrows!"
       "They are not furrows," said Barbicane; "they are _rifts_."
       "Rifts? stuff!" replied Michel mildly; "but what do you mean by
       `rifts' in the scientific world?"
       Barbicane immediately enlightened his companion as to what he
       knew about lunar rifts. He knew that they were a kind of furrow
       found on every part of the disc which was not mountainous; that
       these furrows, generally isolated, measured from 400 to 500
       leagues in length; that their breadth varied from 1,000 to 1,500
       yards, and that their borders were strictly parallel; but he
       knew nothing more either of their formation or their nature.
       Barbicane, through his glasses, observed these rifts with
       great attention. He noticed that their borders were formed of
       steep declivities; they were long parallel ramparts, and with some
       small amount of imagination he might have admitted the existence
       of long lines of fortifications, raised by Selenite engineers.
       Of these different rifts some were perfectly straight, as if cut
       by a line; others were slightly curved, though still keeping
       their borders parallel; some crossed each other, some cut through
       craters; here they wound through ordinary cavities, such as
       Posidonius or Petavius; there they wound through the seas, such
       as the "Sea of Serenity."
       These natural accidents naturally excited the imaginations of
       these terrestrial astronomers. The first observations had not
       discovered these rifts. Neither Hevelius, Cassin, La Hire, nor
       Herschel seemed to have known them. It was Schroeter who in
       1789 first drew attention to them. Others followed who studied
       them, as Pastorff, Gruithuysen, Boeer, and Moedler. At this
       time their number amounts to seventy; but, if they have been
       counted, their nature has not yet been determined; they are
       certainly _not_ fortifications, any more than they are the
       ancient beds of dried-up rivers; for, on one side, the waters,
       so slight on the moon's surface, could never have worn such
       drains for themselves; and, on the other, they often cross
       craters of great elevation.
       We must, however, allow that Michel Ardan had "an idea," and
       that, without knowing it, he coincided in that respect with
       Julius Schmidt.
       "Why," said he, "should not these unaccountable appearances be
       simply phenomena of vegetation?"
       "What do you mean?" asked Barbicane quickly.
       "Do not excite yourself, my worthy president," replied Michel;
       "might it not be possible that the dark lines forming that
       bastion were rows of trees regularly placed?"
       "You stick to your vegetation, then?" said Barbicane.
       "I like," retorted Michel Ardan, "to explain what you savants
       cannot explain; at least my hypotheses has the advantage of
       indicating why these rifts disappear, or seem to disappear, at
       certain seasons."
       "And for what reason?"
       "For the reason that the trees become invisible when they lose
       their leaves, and visible again when they regain them."
       "Your explanation is ingenious, my dear companion," replied
       Barbicane, "but inadmissible."
       "Why?"
       "Because, so to speak, there are no seasons on the moon's surface,
       and that, consequently, the phenomena of vegetation of which you
       speak cannot occur."
       Indeed, the slight obliquity of the lunar axis keeps the sun at
       an almost equal height in every latitude. Above the equatorial
       regions the radiant orb almost invariably occupies the zenith,
       and does not pass the limits of the horizon in the polar
       regions; thus, according to each region, there reigns a
       perpetual winter, spring, summer, or autumn, as in the planet
       Jupiter, whose axis is but little inclined upon its orbit.
       What origin do they attribute to these rifts? That is a
       question difficult to solve. They are certainly anterior to the
       formation of craters and circles, for several have introduced
       themselves by breaking through their circular ramparts. Thus it
       may be that, contemporary with the later geological epochs, they
       are due to the expansion of natural forces.
       But the projectile had now attained the fortieth degree of lunar
       latitude, at a distance not exceeding 40 miles. Through the
       glasses objects appeared to be only four miles distant.
       At this point, under their feet, rose Mount Helicon, 1,520 feet
       high, and round about the left rose moderate elevations,
       enclosing a small portion of the "Sea of Rains," under the name
       of the Gulf of Iris. The terrestrial atmosphere would have to
       be one hundred and seventy times more transparent than it is,
       to allow astronomers to make perfect observations on the moon's
       surface; but in the void in which the projectile floated no
       fluid interposed itself between the eye of the observer and
       the object observed. And more, Barbicane found himself carried
       to a greater distance than the most powerful telescopes had
       ever done before, either that of Lord Rosse or that of the
       Rocky Mountains. He was, therefore, under extremely favorable
       conditions for solving that great question of the habitability
       of the moon; but the solution still escaped him; he could
       distinguish nothing but desert beds, immense plains, and toward
       the north, arid mountains. Not a work betrayed the hand of man;
       not a ruin marked his course; not a group of animals was to be
       seen indicating life, even in an inferior degree. In no part
       was there life, in no part was there an appearance of vegetation.
       Of the three kingdoms which share the terrestrial globe between
       them, one alone was represented on the lunar and that the mineral.
       "Ah, indeed!" said Michel Ardan, a little out of countenance;
       "then you see no one?"
       "No," answered Nicholl; "up to this time, not a man, not an
       animal, not a tree! After all, whether the atmosphere has taken
       refuge at the bottom of cavities, in the midst of the circles,
       or even on the opposite face of the moon, we cannot decide."
       "Besides," added Barbicane, "even to the most piercing eye a man
       cannot be distinguished farther than three and a half miles off;
       so that, if there are any Selenites, they can see our projectile,
       but we cannot see them."
       Toward four in the morning, at the height of the fiftieth
       parallel, the distance was reduced to 300 miles. To the left
       ran a line of mountains capriciously shaped, lying in the
       full light. To the right, on the contrary, lay a black hollow
       resembling a vast well, unfathomable and gloomy, drilled into
       the lunar soil.
       This hole was the "Black Lake"; it was Pluto, a deep circle
       which can be conveniently studied from the earth, between the
       last quarter and the new moon, when the shadows fall from west
       to east.
       This black color is rarely met with on the surface of
       the satellite. As yet it has only been recognized in the depths
       of the circle of Endymion, to the east of the "Cold Sea," in the
       northern hemisphere, and at the bottom of Grimaldi's circle, on
       the equator, toward the eastern border of the orb.
       Pluto is an annular mountain, situated in 51@ north latitude,
       and 9@ east longitude. Its circuit is forty-seven miles long
       and thirty-two broad.
       Barbicane regretted that they were not passing directly above
       this vast opening. There was an abyss to fathom, perhaps some
       mysterious phenomenon to surprise; but the projectile's course
       could not be altered. They must rigidly submit. They could not
       guide a balloon, still less a projectile, when once enclosed
       within its walls. Toward five in the morning the northern
       limits of the "Sea of Rains" was at length passed. The mounts
       of Condamine and Fontenelle remained-- one on the right, the
       other on the left. That part of the disc beginning with 60@ was
       becoming quite mountainous. The glasses brought them to within
       two miles, less than that separating the summit of Mont Blanc
       from the level of the sea. The whole region was bristling with
       spikes and circles. Toward the 60@ Philolaus stood predominant
       at a height of 5,550 feet with its elliptical crater, and seen
       from this distance, the disc showed a very fantastical appearance.
       Landscapes were presented to the eye under very different
       conditions from those on the earth, and also very inferior to them.
       The moon having no atmosphere, the consequences arising from
       the absence of this gaseous envelope have already been shown.
       No twilight on her surface; night following day and day following
       night with the suddenness of a lamp which is extinguished or
       lighted amid profound darkness-- no transition from cold to
       heat, the temperature falling in an instant from boiling point
       to the cold of space.
       Another consequence of this want of air is that absolute
       darkness reigns where the sun's rays do not penetrate.
       That which on earth is called diffusion of light, that luminous
       matter which the air holds in suspension, which creates the
       twilight and the daybreak, which produces the _umbrae_ and
       _penumbrae_, and all the magic of _chiaro-oscuro_, does not
       exist on the moon. Hence the harshness of contrasts, which
       only admit of two colors, black and white. If a Selenite
       were to shade his eyes from the sun's rays, the sky would seem
       absolutely black, and the stars would shine to him as on the
       darkest night. Judge of the impression produced on Barbicane
       and his three friends by this strange scene! Their eyes
       were confused. They could no longer grasp the respective
       distances of the different plains. A lunar landscape without
       the softening of the phenomena of _chiaro-oscuro_ could not be
       rendered by an earthly landscape painter; it would be spots of
       ink on a white page-- nothing more.
       This aspect was not altered even when the projectile, at the
       height of 80@, was only separated from the moon by a distance
       of fifty miles; nor even when, at five in the morning, it
       passed at less than twenty-five miles from the mountain of
       Gioja, a distance reduced by the glasses to a quarter of a mile.
       It seemed as if the moon might be touched by the hand!
       It seemed impossible that, before long, the projectile would
       not strike her, if only at the north pole, the brilliant arch
       of which was so distinctly visible on the black sky.
       Michel Ardan wanted to open one of the scuttles and throw
       himself on to the moon's surface! A very useless attempt; for
       if the projectile could not attain any point whatever of the
       satellite, Michel, carried along by its motion, could not attain
       it either.
       At that moment, at six o'clock, the lunar pole appeared. The disc
       only presented to the travelers' gaze one half brilliantly lit up,
       while the other disappeared in the darkness. Suddenly the
       projectile passed the line of demarcation between intense light
       and absolute darkness, and was plunged in profound night!
       Content of Chapter XIII - Lunar Landscapes [Jules Verne's novel: A trip around the Moon]
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