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have always made itself felt at no matter what distance. But as the
Earth is not the only celestial body possessing attraction, it is
evident that there may be a point in space where the respective
attractions may be entirely annihilated by mutual counteraction. Of this
phenomenon the present instance was a case in point. In a short time,
the Projectile and its contents would for a few moments be absolutely
and completely deprived of all weight whatsoever.
The path described by the Projectile was evidently a line from the Earth
to the Moon averaging somewhat less than 240,000 miles in length.
According as the distance between the Projectile and the Earth was
increasing, the terrestrial attraction was diminishing in the ratio of
the square of the distance, and the lunar attraction was augmenting in
the same proportion.
As before observed, the point was not now far off where, the two
attractions counteracting each other, the bullet would actually weigh
nothing at all. If the masses of the Earth and the Moon had been equal,
this should evidently be found half way between the two bodies. But by
making allowance for the difference of the respective masses, it was
easy to calculate that this point would be situated at the 9/10 of the
total distance, or, in round numbers, at something less than 216,000
miles from the Earth.
At this point, a body that possessed no energy or principle of movement
within itself, would remain forever, relatively motionless, suspended
like Mahomet's coffin, being equally attracted by the two orbs and
nothing impelling it in one direction rather than in the other.
Now the Projectile at this moment was nearing this point; if it reached
it, what would be the consequence?
To this question three answers presented themselves, all possible under
the circumstances, but very different in their results.
1. Suppose the Projectile to possess velocity enough to pass the neutral
point. In such case, it would undoubtedly proceed onward to the Moon,
being drawn thither by Lunar attraction.
2. Suppose it lacked the requisite velocity for reaching the neutral
point. In such a case it would just as certainly fall back to the Earth,
in obedience to the law of Terrestrial attraction.
3. Suppose it to be animated by just sufficient velocity to reach the
neutral point, but not to pass it. In that case, the Projectile would
remain forever in the same spot, perfectly motionless as far as regards
the Earth and the Moon, though of course following them both in their
annual orbits round the Sun.
Such was now the state of things, which Barbican tried to explain to his
friends, who, it need hardly be said, listened to his remarks with the
most intense interest. How were they to know, they asked him, the
precise instant at which the Projectile would reach the neutral point?
That would be an easy matter, he assured them. It would be at the very
moment when both themselves and all the other objects contained in the
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