From the Earth to the Moon by Verne, Jules

enterprise a hundredfold.

A Frenchman, an enthusiastic Parisian, as witty as he was bold,

asked to be enclosed in the projectile, in order that he might

reach the moon, and reconnoiter this terrestrial satellite.

The name of this intrepid adventurer was Michel Ardan. He landed

in America, was received with enthusiasm, held meetings, saw

himself carried in triumph, reconciled President Barbicane to

his mortal enemy, Captain Nicholl, and, as a token of

reconciliation, persuaded them both to start with him in

the projectile. The proposition being accepted, the shape

of the projectile was slightly altered. It was made of a

cylindro-conical form. This species of aerial car was lined with

strong springs and partitions to deaden the shock of departure.

It was provided with food for a year, water for some months,

and gas for some days. A self-acting apparatus supplied the

three travelers with air to breathe. At the same time, on one

of the highest points of the Rocky Mountains, the Gun Club had

a gigantic telescope erected, in order that they might be able

to follow the course of the projectile through space. All was

then ready.

On the 30th of November, at the hour fixed upon, from the midst

of an extraordinary crowd of spectators, the departure took place,

and for the first time, three human beings quitted the terrestrial

globe, and launched into inter-planetary space with almost a

certainty of reaching their destination. These bold travelers,

Michel Ardan, President Barbicane, and Captain Nicholl, ought to

make the passage in ninety-seven hours, thirteen minutes, and

twenty seconds. Consequently, their arrival on the lunar disc

could not take place until the 5th of December at twelve at night,

at the exact moment when the moon should be full, and not on the

4th, as some badly informed journalists had announced.

But an unforeseen circumstance, viz., the detonation produced

by the Columbiad, had the immediate effect of troubling the

terrestrial atmosphere, by accumulating a large quantity of

vapor, a phenomenon which excited universal indignation, for the

moon was hidden from the eyes of the watchers for several nights.

The worthy Joseph T. Maston, the staunchest friend of the three

travelers, started for the Rocky Mountains, accompanied by the

Hon. J. Belfast, director of the Cambridge Observatory, and

reached the station of Long’s Peak, where the telescope was

erected which brought the moon within an apparent distance of

two leagues. The honorable secretary of the Gun Club wished

himself to observe the vehicle of his daring friends.

The accumulation of the clouds in the atmosphere prevented all

observation on the 5th, 6th, 7th, 8th, 9th, and 10th of December.

Indeed it was thought that all observations would have to be put

off to the 3d of January in the following year; for the moon

entering its last quarter on the 11th, would then only present

an ever-decreasing portion of her disc, insufficient to allow

of their following the course of the projectile.

At length, to the general satisfaction, a heavy storm cleared

the atmosphere on the night of the 11th and 12th of December,

and the moon, with half-illuminated disc, was plainly to be seen

upon the black sky.

That very night a telegram was sent from the station of Long’s

Peak by Joseph T. Maston and Belfast to the gentlemen of the

Cambridge Observatory, announcing that on the 11th of December

at 8h. 47m. P.M., the projectile launched by the Columbiad of

Stones Hill had been detected by Messrs. Belfast and Maston–

that it had deviated from its course from some unknown cause,

and had not reached its destination; but that it had passed near

enough to be retained by the lunar attraction; that its

rectilinear movement had been changed to a circular one, and

that following an elliptical orbit round the star of night it

had become its satellite. The telegram added that the elements

of this new star had not yet been calculated; and indeed three

observations made upon a star in three different positions are

necessary to determine these elements. Then it showed that the

distance separating the projectile from the lunar surface “might”

be reckoned at about 2,833 miles.

It ended with the double hypothesis: either the attraction of

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