Philosophical transactions, Vol. L. Part I. For the year 1757.: Giving some account of the present undertakings, studies, and labours, of the ingenious, in many considerable parts of the world.Various
History
Philosophical transactions, Vol. L. Part I. For the year 1757.: Giving some account of the present undertakings, studies, and labours, of the ingenious, in many considerable parts of the world.
Various
Science -- Periodicals
That expert geometrician M. Cha. Walmsley, in his Essay on the
Precession of the Equinox, printed in the last volume of the
Philosophical Transactions, has judiciously avoided all mistakes of
this last kind, respecting the sun’s force, by pursuing the method,
pointed out by Sir Isaac Newton; but, in determining the effect of that
force, has fallen into others, not less considerable than those above
adverted to.
In his third Lemma, the momentum of the whole Earth, about its
diameter, is computed on a supposition, that the momentum or force of
each particle is proportional to its distance from the axis of motion,
or barely as the quantity of motion in such particle, considered
abstractedly. No regard is, therefore, had to the lengths of the
unequal levers, whereby the particles are supposed to receive and
communicate their motion: which, without doubt, ought to have been
included in the consideration.
In his first proposition, he determines, in a very ingenious and
concise manner, the true annual motion of the nodes of a ring (or of
a single satellite) at the earth’s equator, revolving with the earth
itself, about its center, in the time of one siderial day. This motion
he finds to be = (3co-s. 23° 29´/4 rad.) × (⅟366¼) × 360°. Then, in
order to infer from thence, the motion of the equinoctial points of the
earth itself, he, first, diminishes that quantity, in the ratio of 2
to 5: Because (as is demonstrated by Sir Isaac Newton in his 2d Lemma)
the whole force of all the particles situated without the surface of a
sphere, inscribed in the spheroid, to turn the body about its center,
will be only 2-5ths of the force of an equal number of particles
uniformly disposed round the whole circumference of the equator, in
the fashion of a ring. The quantity ((3co-s. 23° 29´/4 rad.) × ⅖ ×
(⅟366¼) × 360°) thus arising, will, therefore, express the true motion
of the equinoctial points of a ring, equal in quantity of matter to the
excess of the whole earth above the inscribed sphere, when the force
whereby the ring tends to turn about its diameter is supposed equal
to the force whereby the earth itself tends to turn about the same
diameter, in consequence of the sun’s attraction. Thus far our author
agrees with Sir Isaac Newton; but, in deriving from hence the motion
of the equinoctial points of the earth itself, he differs from him;
and, in the corollary to his third Lemma, assigns the reasons, why he
thinks Sir Isaac Newton, in this particular, has _wandered a little
from the truth_. Instead of diminishing the quantity above exhibited
(as Sir Isaac has done) in the ratio of all the motion in the ring to
the motion in the whole earth, he diminishes it in the ratio of the
motion of all the matter above the surface of the inscribed sphere to
the motion of the whole earth: which matter, tho’ equal to that of the
ring, has nevertheless a different momentum, arising from the different
situation of the particles in respect to the axis of motion.
Public-domain text, read in full here on John Shaqi.
Philosophical transactions, Vol. L. Part I. For the year 1757.: Giving some account of the present undertakings, studies, and labours, of the ingenious, in many considerable parts of the world. — John Shaqi
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