Round the Moon by Jules Verne (read aloud txt) ๐
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This sequel to From the Earth to the Moon narrates the eventful journey to the Moon of three passengersโImpey Barbicane, president of the Gun Club, Captain Nicholl, Barbicaneโs rival and then collaborator, and Michel Ardan, a French scientistโaboard a hollow cannonball. They orbit the Moon and perform geographical observations, but the projectile fails to land, propelling them instead toward the Earth. Theyโre rescued at sea and widely celebrated as the first humans to leave Earth.
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- Author: Jules Verne
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Michel spoke with as much animation as if the tap were still full on. But with one sentence Barbicane damped his enthusiasm.
โAll that is very well, friend Michel,โ he said, โbut now perhaps you will tell us where those fowls that joined in our concert came from.โ
โThose fowls?โ
โYes.โ
In fact, half-a-dozen hens and a superb cock were flying hither and thither.
โAh, the stupids!โ cried Michel. โIt was the oxygen that put them in revolt.โ
โBut what are you going to do with those fowls?โ asked Barbicane.
โAcclimatise them in the moon of course! For the sake of a joke, my worthy president; simply a joke that has unhappily come to nothing! I wanted to let them out on the lunar continent without telling you! How astounded you would have been to see these terrestrial poultry pecking the fields of the moon!โ
โAh, gamin, you eternal boy!โ answered Barbicane, โyou donโt want oxygen to make you out of your senses! You are always what we were under the influence of this gas! You are always insane!โ
โAh! how do we know we were not wiser then?โ replied Michel Ardan.
After this philosophical reflection the three friends repaired the disorder in the projectile. Cock and hens were put back in their cage. But as they were doing this Barbicane and his two companions distinctly perceived a fresh phenomenon.
Since the moment they had left the earth their own weight, that of the bullet and the objects it contained, had suffered progressive diminution. Though they could not have any experience of this in the projectile, a moment must come when the effect upon themselves and the tools and instruments they used would be felt.
Of course scales would not have indicated this loss of weight, for the weights used would have lost precisely as much as the object itself; but a spring weighing-machine, the tension of which is independent of attraction, would have given the exact valuation of this diminution.
It is well known that attraction, or weight, is in proportion to the bulk, and in inverse proportion to the square of distances. Hence this consequence. If the earth had been alone in space, if the other heavenly bodies were to be suddenly annihilated, the projectile, according to Newtonโs law, would have weighed less according to its distance from the earth, but without ever losing its weight entirely, for the terrestrial attraction would always have made itself felt, no matter at what distance.
But in the case with which we are dealing, a moment must come when the projectile would not be at all under the law of gravitation, after allowing for the other celestial bodies, whose effect could not be set down as zero.
In fact, the trajectory of the projectile was between the earth and the moon. As it went farther away from the earth terrestrial attraction would be diminished in inverse proportion to the square of distances, but the lunar attraction would be augmented in the same proportion. A point must, therefore, be reached where these two attractions would neutralise each other, and the bullet would have no weight at all. If the volumes of the moon and earth were equal, this point would have been reached at an equal distance between the two bodies. But by taking their difference of bulk into account it was easy to calculate that this point would be situated at โดโทโโ โ of the journey, or at 78,114 leagues from the earth.
At this point a body that had no principle of velocity or movement in itself would remain eternally motionless, being equally attracted by the two heavenly bodies, and nothing drawing it more towards one than the other.
Now if the force of impulsion had been exactly calculated the projectile ought to reach that point with no velocity, having lost all weight like the objects it contained.
What would happen then? Three hypotheses presented themselves.
Either the projectile would have kept some velocity, and passing the point of equal attraction, would fall on the moon by virtue of the excess of lunar attraction over terrestrial attraction.
Or velocity sufficient to reach the neutral point being wanting, it would fall back on the earth by virtue of the excess of terrestrial attraction over lunar attraction.
Or lastly, endowed with sufficient velocity to reach the neutral point, but insufficient to pass it, it would remain eternally suspended in the same place, like the pretended coffin of Muhammad, between the zenith and nadir.
Such was the situation, and Barbicane clearly explained the consequences to his travelling companions. They were interested to the highest degree. How were they to know when they had reached this neutral point, situated at 78,114 leagues from the earth, at the precise moment when neither they nor the objects contained in the projectile should be in any way subject to the laws of weight?
Until now the travellers, though they had remarked that this action diminished little by little, had not yet perceived its total absence. But that day, about 11 a.m., Nicholl having let a tumbler escape from his hand, instead of falling, it remained suspended in the air.
โAh!โ cried Michel Ardan, โthis is a little amusing chemistry!โ
And immediately different objects, weapons, bottles, etc., left to themselves, hung suspended as if by miracle. Diana, too, lifted up by Michel into space, reproduced, but without trickery,
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