A View of Sir Isaac Newton's PhilosophyPemberton, Henry
Science
A View of Sir Isaac Newton's Philosophy
Pemberton, Henry
Newton, Isaac, 1642-1727. Principia
got into the situation I K L, the interval ζ η shall be expanded into
the present distance between α and β; and by that time likewise the
present distance of α from β will be contracted into their natural
interval: for this distance will be about the same time in contracting
it self, as has been taken up in its dilatation; seeing the string will
be as long in returning from its rectilinear figure, as it has been in
recovering it from its situation I ϰ L. This is the change which will
be made in the particles between α and ζ. As for those between ζ and
χ, because each preceding particle advances faster than that, which
immediately follows it, their distances will successively be dilated
into that, which is at present between ζ and η. And as soon as any two
particles are arrived at their natural distance, the hindermost of them
shall be stopt, and immediately after return, the distances between
the returning particles being greater than the natural. And this
dilatation of these distances shall extend so far, by that time the
chord is returned into its first situation I K L, that the particles ι
χ shall be removed to their natural distance. But the dilatation of ν
χ shall contract the interval τ φ into that at present between ν and
χ, and the contraction of the distance between those two particles τ
and φ will agitate a part of the air beyond; so that when the chord is
returned into the situation I K L, having made an intire vibration, the
moved particles of the air will take the rangement expressed by the
points, _l, m, n, o, p, q, r, s, t, u, w, x, y, z_, 1, 2, 3, 4, 5, 6,
7, 8: in which _l m_, are at the natural distance of the particles, the
distance _m n_ greater than _l m_ and _n o_ greater than _m n_, and so
on, till you come to _q r_, the widest of all: and then the distances
gradually diminish not only to the natural distance, as _w x_, but till
they are contracted as much as χ τ was before; which falls out in the
points 2, 3, from whence the distances augment again, till you come to
the part of the air untouched.
Public-domain text, read in full here on John Shaqi.
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