(123.) If velocity be estimated by the space through which the body
would move uniformly in one second, then the final velocity of a body
falling for one second will be 2; for with that final velocity the body
would in one second move through twice the height through which it has
fallen.
(124.) Since the final velocity increases in the same proportion as
the time, it follows that after two seconds it is twice its amount
after one, and after three seconds thrice that, and so on. Thus, the
following table exhibits the final velocities corresponding to the
times of descent:
+---------------+---+---+---+---+----+----+----+----+----+----+
|Time | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 |
+---------------+---+---+---+---+----+----+----+----+----+----+
|Final velocity | 2 | 4 | 6 | 8 | 10 | 12 | 14 | 16 | 18 | 20 |
+---------------+---+---+---+---+----+----+----+----+----+----+
The numbers in the second row express the spaces through which a body
with the final velocity would move in one second, the unit being, as
usual, the space through which a body falls freely in one second.
(125.) Having thus developed theoretically the laws which characterise
the descent of bodies, falling freely by the force of gravity, or by
any other uniform force of the same kind, it is necessary that we
should show how these laws can be exhibited by actual experiment.
There are some circumstances attending the fall of heavy bodies which
would render it difficult, if not impossible, to illustrate, by the
direct observation of this phenomenon, the properties which have
been explained in this chapter. A body falling freely by the force
of gravity, as we shall hereafter prove, descends in one second of
time through a height of about 16 feet[1]; in two seconds, it would,
therefore, fall through four times that space, or 64 feet; in three
seconds, through 9 times the height, or 144 feet; and in four seconds,
through 256 feet. In order, therefore, to be enabled to observe the
phenomena for only four seconds, we should command an height of at
least 256 feet. But further; the velocity at the end of the first
second would be at the rate of 32 feet per second; at the end of the
second second, it would be 64 feet per second; and towards the end of
the fall it would be about 120 feet per second. It is evident that this
great degree of rapidity would be a serious impediment to accurate
observation, even though we should be able to command the requisite
height. It appears therefore that the number expressed by _g_ in the
preceding formulæ is 16·083.
[1] More exactly through 16-1/12 feet, or 193 inches.
Public-domain text, read in full here on John Shaqi.
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