Chapter 15 - Page 2
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enough, in fact, for them to perceive easily in the dark the great round
screen which she formed between themselves and the Projectile on one
side, and the Earth, Sun, and stars on the other. But as to the exact
distance at which she lay from them--they had no possible means of
calculating it. The Projectile, impelled and maintained by forces
inexplicable and even incomprehensible, had come within less than thirty
miles from the Moon's north pole. But during those two hours of
immersion in the dark shadow, had this distance been increased or
diminished? There was evidently no stand-point whereby to estimate
either the Projectile's direction or its velocity. Perhaps, moving
rapidly away from the Moon, it would be soon out of her shadow
altogether. Perhaps, on the contrary, gradually approaching her surface,
it might come into contact at any moment with some sharp invisible peak
of the Lunar mountains--a catastrophe sure to put a sudden end to the
trip, and the travellers too.
An excited discussion on this subject soon sprang up, in which all
naturally took part. Ardan's imagination as usual getting the better of
his reason, he maintained very warmly that the Projectile, caught and
retained by the Moon's attraction, could not help falling on her
surface, just as an aerolite cannot help falling on our Earth.
"Softly, dear boy, softly," replied Barbican; "aerolites _can_ help
falling on the Earth, and the proof is, that few of them _do_ fall--most
of them don't. Therefore, even granting that we had already assumed the
nature of an aerolite, it does not necessarily follow that we should
fall on the Moon."
"But," objected Ardan, "if we approach only near enough, I don't see how
we can help--"
"You don't see, it may be," said Barbican, "but you can see, if you only
reflect a moment. Have you not often seen the November meteors, for
instance, streaking the skies, thousands at a time?"
"Yes; on several occasions I was so fortunate."
"Well, did you ever see any of them strike the Earth's surface?" asked
Barbican.
"I can't say I ever did," was the candid reply, "but--"
"Well, these shooting stars," continued Barbican, "or rather these
wandering particles of matter, shine only from being inflamed by the
friction of the atmosphere. Therefore they can never be at a greater
distance from the Earth than 30 or 40 miles at furthest, and yet they
seldom fall on it. So with our Projectile. It may go very close to the
Moon without falling into it."
"But our roving Projectile must pull up somewhere in
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