The Study of Astronomy, adapted to the capacities of youth: In twelve familiar dialogues, between a tutor and his pupil: explaining the general phænomena of the heavenly bodies, the theory of the tides, &c.Stedman, John, teacher of astronomy
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The Study of Astronomy, adapted to the capacities of youth: In twelve familiar dialogues, between a tutor and his pupil: explaining the general phænomena of the heavenly bodies, the theory of the tides, &c.
Stedman, John, teacher of astronomy
Astronomy -- Juvenile literature -- Early works to 1800
TUTOR. The periods of the planets, or the times they take to complete
their revolutions in their orbits, are exactly known; and the mean
distance of the earth from the sun has been also ascertained. Here,
then, we have the periods of all, and the mean distance of one, to find
the distances of the rest; which may be found by attending to the
following proportion:
As the square of the period of any one planet,
Is to the cube of its mean distance from the sun;
So is the square of the period of any other planet,
To the cube of its mean distance.
The cube root of this quotient will be the distance sought.
PUPIL. Here again I find myself at a loss, as I have not learnt to
extract the cube root.
TUTOR. I will give you [18]Doctor Turner’s rule, which I think will
answer your purpose.
[Footnote 18: Young Geometrician’s Companion.]
“First, having set down the given number, or resolvend, make a dot over
the unit figure, and so on over every third figure (towards the left
hand in whole numbers, but towards the right hand in decimals); and so
many dots as there are, so many figures will be in the root.
Next, seek the nearest cube to the first period; place its root in the
quotient, and its cube set under the first period. Subtract it
therefrom; and to the remainder bring down one figure only of the next
period, which will be a dividend.
Then, square the figure put in the quotient, and multiply it by 3, for a
divisor. Seek how often this divisor may be had in the dividend, and set
the figure in the quotient, which will be the second place in the root.
Now, cube the figures in the root, and subtract it from the two first
periods of the resolvend; and to the remainder bring down the first
figure of the next period, for a new dividend. Square the figures in the
quotient, and multiply it by 3, for a new divisor; then proceed in all
respects as before, till the whole is finished.”
The following example will, I trust, make it clear to you.
EXAMPLE.
It is required to find the cube root of 15625.
. .
15625 (25
8
─────
12) 76
15625
─────
.....
═════
Public-domain text, read in full here on John Shaqi.
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