From the Earth to the Moon by Verne, Jules

But the sight of this desolate world did not fail to captivate

them by its very strangeness. They were moving over this region

as if they had been borne on the breath of some storm, watching

heights defile under their feet, piercing the cavities with their

eyes, going down into the rifts, climbing the ramparts, sounding

these mysterious holes, and leveling all cracks. But no trace

of vegetation, no appearance of cities; nothing but stratification,

beds of lava, overflowings polished like immense mirrors,

reflecting the sun’s rays with overpowering brilliancy.

Nothing belonging to a _living_ world– everything to a dead

world, where avalanches, rolling from the summits of the mountains,

would disperse noiselessly at the bottom of the abyss, retaining

the motion, but wanting the sound. In any case it was the image

of death, without its being possible even to say that life had ever

existed there.

Michel Ardan, however, thought he recognized a heap of ruins,

to which he drew Barbicane’s attention. It was about the 80th

parallel, in 30@ longitude. This heap of stones, rather

regularly placed, represented a vast fortress, overlooking a

long rift, which in former days had served as a bed to the

rivers of prehistorical times. Not far from that, rose to a

height of 17,400 feet the annular mountain of Short, equal to

the Asiatic Caucasus. Michel Ardan, with his accustomed ardor,

maintained “the evidences” of his fortress. Beneath it he

discerned the dismantled ramparts of a town; here the still

intact arch of a portico, there two or three columns lying under

their base; farther on, a succession of arches which must have

supported the conduit of an aqueduct; in another part the sunken

pillars of a gigantic bridge, run into the thickest parts of

the rift. He distinguished all this, but with so much imagination

in his glance, and through glasses so fantastical, that we must

mistrust his observation. But who could affirm, who would dare

to say, that the amiable fellow did not really see that which

his two companions would not see?

Moments were too precious to be sacrificed in idle discussion.

The selenite city, whether imaginary or not, had already

disappeared afar off. The distance of the projectile from the

lunar disc was on the increase, and the details of the soil were

being lost in a confused jumble. The reliefs, the circles,

the craters, and the plains alone remained, and still showed

their boundary lines distinctly. At this moment, to the left,

lay extended one of the finest circles of lunar orography,

one of the curiosities of this continent. It was Newton,

which Barbicane recognized without trouble, by referring to

the _Mappa Selenographica_.

Newton is situated in exactly 77@ south latitude, and 16@

east longitude. It forms an annular crater, the ramparts of

which, rising to a height of 21,300 feet, seemed to be impassable.

Barbicane made his companions observe that the height of this

mountain above the surrounding plain was far from equaling the

depth of its crater. This enormous hole was beyond all

measurement, and formed a gloomy abyss, the bottom of which the

sun’s rays could never reach. There, according to Humboldt,

reigns utter darkness, which the light of the sun and the earth

cannot break. Mythologists could well have made it the mouth of hell.

“Newton,” said Barbicane, “is the most perfect type of these

annular mountains, of which the earth possesses no sample.

They prove that the moon’s formation, by means of cooling, is

due to violent causes; for while, under the pressure of internal

fires the reliefs rise to considerable height, the depths withdraw

far below the lunar level.”

“I do not dispute the fact,” replied Michel Ardan.

Some minutes after passing Newton, the projectile directly

overlooked the annular mountains of Moret. It skirted at some

distance the summits of Blancanus, and at about half-past seven

in the evening reached the circle of Clavius.

This circle, one of the most remarkable of the disc, is situated

in 58@ south latitude, and 15@ east longitude. Its height is

estimated at 22,950 feet. The travelers, at a distance of

twenty-four miles (reduced to four by their glasses) could

admire this vast crater in its entirety.

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