From the Earth to the moon; and, round the moonVerne, Jules
Science
From the Earth to the moon; and, round the moon
Verne, Jules
Manned space flight -- Fiction; Moon -- Fiction; Science fiction; Space flight to the moon -- Fiction; Space ships -- Fiction
This new work was finished about three o’clock, and after taking all
these precautions there remained but to wait. But the projectile was
perceptibly nearing the moon, and evidently succumbed to her influence
to a certain degree; though its own velocity also drew it in an oblique
direction. From these conflicting influences resulted a line which
might become a tangent. But it was certain that the projectile would
not fall directly on the moon; for its lower part, by reason of its
weight, ought to be turned toward her.
Barbicane’s uneasiness increased as he saw his projectile resist the
influence of gravitation. The Unknown was opening before him, the
Unknown in interplanetary space. The man of science thought he had
foreseen the only three hypotheses possible—the return to the earth,
the return to the moon, or stagnation on the neutral line; and here a
fourth hypothesis, big with all the terrors of the Infinite, surged up
inopportunely. To face it without flinching, one must be a resolute
savant like Barbicane, a phlegmatic being like Nicholl, or an audacious
adventurer like Michel Ardan.
Conversation was started upon this subject. Other men would have
considered the question from a practical point of view; they would have
asked themselves whither their projectile carriage was carrying them.
Not so with these; they sought for the cause which produced this
effect.
“So we have become diverted from our route,” said Michel; “but why?”
“I very much fear,” answered Nicholl, “that, in spite of all
precautions taken, the Columbiad was not fairly pointed. An error,
however small, would be enough to throw us out of the moon’s
attraction.”
“Then they must have aimed badly?” asked Michel.
“I do not think so,” replied Barbicane. “The perpendicularity of the
gun was exact, its direction to the zenith of the spot incontestible;
and the moon passing to the zenith of the spot, we ought to reach it at
the full. There is another reason, but it escapes me.”
“Are we not arriving too late?” asked Nicholl.
“Too late?” said Barbicane.
“Yes,” continued Nicholl. “The Cambridge Observatory’s note says that
the transit ought to be accomplished in ninety-seven hours thirteen
minutes and twenty seconds; which means to say, that _sooner_ the moon
will _not_ be at the point indicated, and _later_ it will have passed
it.”
“True,” replied Barbicane. “But we started the 1st of December, at
thirteen minutes and twenty-five seconds to eleven at night; and we
ought to arrive on the 5th at midnight, at the exact moment when the
moon would be full; and we are now at the 5th of December. It is now
half-past three in the evening; half-past eight ought to see us at the
end of our journey. Why do we not arrive?”
“Might it not be an excess of speed?” answered Nicholl; “for we know
now that its initial velocity was greater than they supposed.”
Public-domain text, read in full here on John Shaqi.
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