_Fig. 217._ is a side view of the pendulum rod when together.

H H and I I are two flat rods of iron about an eighth of

an inch thick. K K is a bar of zinc placed between them, and is

nearly a quarter of an inch thick. The corners of the iron bars are

bevelled off, which gives them a much lighter appearance. These bars

are kept together by means of three screws, O O O, which

pass through oblong holes in the bars H H and K K, and screw

into the rod I I. The bar H H is fastened to the bar of zinc

K K, by the screw _m_, which is called the adjusting screw. This

screw is tapped into H H, and passes just through K K; but

that part of the screw which passes K K has its threads turned

off. The iron bar I I has a shoulder at its upper end, and rests

on the top of the zinc bar K K and is wholly supported by it.

There are several holes for the screw _m_, in order to adjust the

compensation.

The action of this pendulum is similar to that last described, the

zinc expanding upwards as much as the iron rods expand downwards, and

consequently the instance from the point of suspension to the centre

of oscillation remains the same.

[Illustration: _Captn. Kater, del._ _H. Adlard, sc._

_London, Pubd. by Longman & Co._]

Mr. Ward states that the expansion of the zinc he used (hammered zinc)

was greater than that given in the tables. He found that the true

length of the zinc bar should be about 23 inches; our computation would

make it nearly 26.

_The Compensation Tube of Julien le Roy._

We mention this merely to state that it is similar in principal to the

apparatus represented at _fig. 204._, with merely this difference,

that, instead of the steel rod being fixed to a cross piece proceeding

from the brass bar B R, it is attached to a cap fixed upon a brass

tube (through which it passes) of the same length as that of the brass

rod B R. Cassini spoke well of this pendulum, and it was used in

the observatory of Cluny about the year 1748.

_Deparcieux’s Compensation._

This was contrived in the same year as that invented by Julien le Roy.

It is represented at _fig. 218._, where A B D F

is a steel bar, the ends of which are to be fixed to the lower

sides of pieces forming a part of the cock of the pendulum.

G E I H is of brass, and stands with its extremities

resting on the horizontal part B D of the steel frame. The upper

part E I of the brass frame passes above the cock of the pendulum,

and admits the tapped wire K, to which the pendulum spring is fixed

through a squared hole in the middle. A nut upon this tapped wire gives

the adjustment for time. The spring passes through the slit in the cock

in the usual manner.

It may be easily perceived that this pendulum is in principle the

same as that of Le Roy; the expansion of the total length of steel

A B S C downwards being compensated by the equivalent

expansion of the brass bar G E upwards. It is, however, preferable

to Le Roy’s, because the compensation is contained in the clock case.

Deparcieux had previously published, in the year 1739, an improvement

of an imperfectly compensating pendulum, proposed in the year 1733 by

Regnauld, a clockmaker of Chalons. In this pendulum Deparcieux employed

a lever with unequal arms to increase the effect of the expansion of

the brass rod, which was too short.

We may here remark, that all fixed compensations are liable to the same

objection, namely, that of not moving with the pendulum, and therefore

not taking precisely the same temperature.

_Captain Kater’s Compensation Pendulum._

In Nicholson’s Journal, for July, 1808, is the description of a

compensation pendulum by the writer of this article. In this pendulum

the rod is of white deal, three quarters of an inch wide, and a quarter

of an inch thick. It was placed in an oven, and suffered to remain

there for a long time until it became a little charred. The ends were

then soaked in melted sealing-wax; and the rod, being cleaned, was

coated several times with copal varnish. To the lower extremity of the

rod a cap of brass was firmly fixed, from which a strong steel screw

proceeded for the purpose of regulating the pendulum for time in the

usual manner.

A square tube of zinc was cast, seven inches long and three quarters

of an inch square; the internal dimensions being four tenths of an

inch. The lower part of the pendulum rod was cut away on the two sides,

so as to slide with perfect freedom within the tube of zinc. To the

bottom of this zinc tube a piece of brass a quarter of an inch thick

was soldered, in which a circular hole was made nearly four tenths of

an inch in diameter, having a screw on the inside. A cylinder of zinc,

furnished with a corresponding screw on its surface, fitted into this

aperture, and a thin plate of brass screwed upon the cylinder, served

as a clamp to prevent any shake after the length of zinc necessary for

compensation should have been determined. A hole was made through the

axis of the cylinder, through which passed the steel screw terminating

the pendulum rod.

An opening was made through the bob of the pendulum, extending to its

centre, to admit the square tube of zinc which was fixed at its upper

extremity to the centre of the bob. The pendulum rod passed through the

bob in the usual manner, and the whole was supported by a nut on the

steel screw at the extremity.

In this form the compensation acts immediately upon the centre of the

bob, elevating it along the rod as much as the rod elongates downwards:

the method of calculating the length of the required compensation is

precisely the same as that we have before given.

Assuming the length of the deal rod to be 43 inches, and multiplying

this by ·1313 from Table II., we have 5·64 inches for the length of

the zinc necessary to counteract the expansion of the deal. The length

of the steel screw between the termination of the pendulum rod and the

nut was two inches, and that of the suspension spring one inch. Now,

3 inches of steel multiplied by ·3682 would give 1·10 inches for the

length of zinc which would compensate the steel, and, adding this to

5·64 inches, we have 6·74 inches for the whole length of zinc required.

In this pendulum, the length of the compensating part may be varied by

means of the zinc cylinder furnished with a screw for that purpose.

The bob of this pendulum and its compensation are represented at

_fig. 219._

It has been objected to the use of wooden pendulum rods, that it

is difficult, if not impossible, to secure them from the action of

moisture, which would at once be fatal to their correct performance.

The pendulum now before us has, however, been going with but little

intermission since it was first constructed: it is attached to a

sidereal clock, not of a superior description, and exposed to very

considerable variations of moisture and dryness; yet the change in its

rate has been so very trifling as to authorize the belief that moisture

has little or no effect upon a wooden rod prepared in the manner we

have described. Its rate, under different temperatures, shows that it

is over-compensated; the length of the zinc remaining, as stated in

Nicholson’s Journal 7·42 inches, instead of which it appears, by our

present compensation, that it should be 6·78 inches.

_Reid’s Compensation Pendulum._

Mr. Adam Reid of Woolwich presented to the Society of Arts, in 1809, a

compensation pendulum, for which he was rewarded with fifteen guineas.

This pendulum is the same in principle with that last described;

the rod, however, is of steel instead of wood, and the compensation

possesses no means of adjustment. This pendulum is represented at

_fig. 220._, where S B is the steel rod, a little thicker

where it enters the bob C, and of a lozenge shape to prevent the bob

turning, but above and below it is cylindrical.

A tube of zinc D passes to the centre of the bob from below, and the

bob is supported upon it by a piece which crosses its centre, and which

meets the upper end of the tube.

The rod being passed through the bob and zinc tube, a nut is applied

upon a screw at the lower extremity of the rod in the usual manner. If

the compensation should be too much, the zinc tube is to be shortened

until it is correct.

The length of the zinc tube will be the same in this pendulum as in

that of Mr. Ward--about 23 inches, if his experiments are to be relied

upon.

The objection to this pendulum appears to be its great length, which

amounts to 62 inches. We conceive it would be preferable to place the

zinc above the bob, as in the modification which we have suggested of

Benzenberg’s pendulum.

_Ellicott’s Pendulum._

It appears that the idea of combining the expansions of different

metals with a lever, so as to form a compensation pendulum,

originated with Mr. Graham; for Mr. Short, in the Philosophical

Transactions for 1752, states that he was informed by Mr. Shelton, that

Mr. Graham, in the year 1737, made a pendulum, consisting of three

bars, one of steel between two of brass; and that the steel bar acted

upon a lever so as to raise the pendulum when lengthened by heat, and

to let it down when shortened by cold.

[Illustration: _Captn. Kater, del._ _H. Adlard, sc._

_London, Pubd. by Longman & Co._]

This pendulum, however, was found upon trial to move by jerks, and was

therefore laid aside by the inventor to make way for the mercurial

pendulum.

Mr. Short also says that Mr. Fotheringham, a quaker of Lincolnshire,

caused a pendulum to be made, in the year 1738 or 1739, consisting of

two bars, one of brass and the other of steel, fastened together by

screws with levers to raise or let down the bob, and that these levers

were placed above the bob.

Mr. John Ellicott of London had made very, accurate experiments on the

relative expansions of seven different metals, which, however, will be

found to differ more or less from the results of the experiments of

others. It is not, however, from this to be concluded that Ellicott’s

determinations were erroneous; for the expansion of a metal will suffer

considerable change even by the processes to which it is necessarily

subjected in the construction of a pendulum. It is therefore desirable,

whenever a compensation pendulum is to be made, that the expansions

of the materials employed should be determined after the processes of

drilling, filing, and hammering have been gone through.

It had been objected to Harrison’s gridiron pendulum, that the

adjustments of the rods was inconvenient, and that the expansion of the

bob supported at its lower edge would, unless taken into the account,

vitiate the compensation. These considerations, it is supposed, gave

rise to Ellicott’s pendulum, which is nearly similar to those we have

just mentioned.

Ellicott’s pendulum is thus constructed:--A bar of brass and a bar of

iron are firmly fixed together at their upper ends, the bar of brass

lying upon the bar of iron, which is the rod of the pendulum. These

bars are held near each other by screws passing through oblong holes in

the brass, and tapped into the iron, and thus the brass is allowed to

expand or contract freely upon the iron with any change of temperature.

The brass bar passes to the centre of the bob of the pendulum, a little

above and below which the iron is left broader for the purpose of

attaching the levers to it, and the iron is made of a sufficient length

to pass quite through the bob of the pendulum.

The pivots of two strong steel levers turn in two holes drilled in

the broad part of the iron bar. The short arms of these levers are in

contact with the lower extremity of the brass bar, and their longer

arms support the bob of the pendulum by meeting the heads of two

screws which pass horizontally from each side of the bob towards its

centre. By advancing these screws towards the centre of the bob, the

longer arms of the lever are shortened, and thus the compensation may

be readily adjusted. At the lower end of the iron rod, under the bob,

a strong double spring is fixed, to support the greater part of the

weight of the bob by its pressure upwards against two points at equal

distances from the pendulum rod. Mr. Ellicott gave a description of

this pendulum to the Royal Society in 1752, but he says the thought was

executed in 1738. As this pendulum is very seldom met with, we think it

unnecessary to give a representation of it.

_Compensation by means of a Compound Bar of Steel and Brass._

Several compensations for pendulums have been proposed, by means of

a compound bar formed of steel and brass soldered together. In a

bar of this description, the brass expanding more than the steel,

the bar becomes curved by a change of temperature, the brass side

becoming convex and the steel concave with heat. Now, if a bar of

this description have its ends resting on supports on each side the

cock of the pendulum, the bar passing above the cock with the brass

uppermost, if the pendulum spring be attached to the middle of the bar,

and it pass in the usual manner through the slit of the cock, it is

evident that, by an increase of temperature, the bar will become curved

upwards, and the pendulum spring be drawn upwards through the slit, and

thus the elongation of the pendulum downwards will be compensated. The

compensation may be adjusted by varying the distance of the points of

support from the middle of the bar.

Such was one of the modes of compensation proposed by Nicholson. Others

of the same description (that is, with compound bars) have been brought

before the public by Mr. Thomas Doughty and Mr. David Ritchie; but as

they are supposed to be liable to many practical objections, we do not

think it requisite to describe them more particularly.

There is, however, a mode of compensation by means of a compound bar,

described by M. Biot in the first volume of his Traité de Physique,

which appears to possess considerable merit, of which he mentions

having first witnessed the successful employment by the inventor, a

clockmaker named Martin. At _fig. 221._, S C, is the rod of

the pendulum, made, in the usual manner, of iron or steel; this rod

passes through the middle of a compound bar of brass and steel (the

brass being undermost), which should be furnished with a short tube and

screws, by means of which, or by passing a pin through the tube and

rod, it may be securely fixed at any part of the pendulum rod.

Two small equal weights W W slide along the compound bar, and,

when their proper position has been determined, may be securely clamped.

The manner in which this compensation acts is thus:--Suppose the

temperature to increase, the brass expanding more than the steel, the

bar becomes curved, and its extremities carrying the weights W and W

are elevated, and thus the place of the centre of oscillation is made

to approach the point of suspension as much, when the compensation is

properly adjusted, as it had receded from it by the elongation of the

pendulum rod.

There are three methods of adjusting this compensation: the first, by

increasing or diminishing the weights W and W; the second, by varying

the distance of the weights W and W from the middle of the bar; and

the third, by varying the distance of the bar from the bob of the

pendulum, taking care not to pass the middle of the rod. The effect of

the compensation is greater as the weights W and W are greater or more

distant from the centre of the bar, and also as the bar is nearer to

the bob of the pendulum.

M. Biot says that he and M. Matthieu employed a pendulum of this kind

for a long time in making astronomical observations in which they were

desirous of attaining an extreme degree of precision, and that they

found its rate to be always perfectly regular.

In all the pendulums which we have described, the bob is supposed

to be fixed to the rod by a pin passing through its centre, and the

adjustment for time is to be made by means of a small weight sliding

upon the rod.

_Of the Mercurial Pendulum._

We have been guided, in our arrangement of the pendulums which we have

described, by the similarity in the mode of compensation employed; and

we have now to treat of that method of compensation which is effected

by the expansion of the material of which the bob itself of the

pendulum is composed.

On this subject, as we have before observed, an admirable paper, from

the pen of Mr. Francis Baily, may be found in the Memoirs of the

Astronomical Society of London, which leaves nothing to be desired

by the mathematical reader. But as our object is to simplify, and

to render our subjects as popular as may be, we must endeavour to

substitute for the perfect accuracy which Mr. Baily’s paper presents,

such rules as may be found not only readily intelligible, but

practically applicable, within the limits of those inevitable errors

which arise from a want of knowledge of the exact expansion of the

materials employed.

At _fig. 222._, let S B represent the rod of a pendulum, and

F C B a metallic tube or cylinder, supported by a nut

at the extremity of the pendulum rod, in the usual manner, and having

a greater expansibility than that of the rod. Now C, the centre of

gravity, supposing the rod to be without weight, will be in the middle

of the cylinder; and if C B, or half the cylinder, be of such

a length as to expand upwards as much as the pendulum rod S B

expands downwards, it is evident that the centre of gravity C will

remain, under any change of temperature, at the same distance from the

point of suspension S. M. Biot imagined that, in effecting this, a

compensation sufficiently accurate would be obtained; but Mr. Baily has

shown that this is by no means the fact.

Let us suppose the place of the centre of oscillation to be at O,

about three or four tenths of an inch, in a pendulum of the usual

construction, below the centre of gravity. Now, the object of the

compensation is to preserve the distance from S to O invariable, and

not the distance from S to C.

The distance of the centre of oscillation varies with the length of the

cylinder F B, and hence suffers an alteration in its distance from

the point of suspension by the elongation of the cylinder, although

the distance of the centre of gravity C from the point of suspension

remains unaltered.

We shall endeavour to render this perfectly familiar. Suppose a

metallic cylinder, 6 inches long, to be suspended by a thread 36 inches

long, thus forming a pendulum in which the distance of the centre

of gravity from the point of suspension is 39 inches: the centre of

oscillation in such a pendulum will be nearly one tenth of an inch

below the centre of gravity. Now let us imagine cylindrical portions of

equal lengths to be added to each end of the cylinder, until it reaches

the point of suspension; we shall then have a cylinder of 78 inches in

length, the centre of gravity of which will still be at the distance of

39 inches from the point of suspension. But it is well known that the

centre of oscillation of such a cylinder is at the distance of about

two thirds of its length from the point of suspension. The centre of

oscillation, therefore, has been removed, by the elongation of the

cylinder, about 13 inches below the centre of gravity, whilst the

centre of gravity has remained stationary.

Now the same thing as that which we have just described takes place,

though in a very minor degree, with our former cylinder, employed as a

compensating bob to a pendulum. The rod expands downwards, the centre

of gravity remains at the same distance from the point of suspension,

and the cylinder elongates both above and below this point; the

consequence of which is, that though the centre of gravity has remained

stationary, the distance of the centre of oscillation from the point

of suspension has increased. It is, therefore, evident that the length

of the compensation must be such as to carry the centre of gravity

a little nearer to the point of suspension than it was before the

expansion took place; by which means the centre of oscillation will be

restored to its former distance from the point of suspension.

Let us suppose the expansions to have taken place, and that the

centre of gravity, remaining at the same distance from the point of

suspension, the centre of oscillation is removed to a greater distance,

as we have before explained. It is well known that the product obtained

by multiplying the distance from the point of suspension to the centre

of gravity, by the distance from the centre of gravity to the centre

of oscillation, is a constant quantity; if, therefore, the distance

from the centre of gravity to the point of suspension be lessened, the

distance from the centre of gravity to the centre of oscillation will

be proportionally, though not equally, increased, and the centre of

oscillation will, therefore, be elevated. We see, then, if we elevate

the centre of gravity precisely the requisite quantity, by employing

a sufficient length of the compensating material, that although the

distance from the centre of gravity to the point of suspension is

lessened, yet the distance from the point of suspension to the centre

of oscillation will suffer no change.

The following rule for finding the length of the compensating material

in a pendulum of the kind we have been considering will be found

sufficiently accurate for all practical purposes:--

_Find in the manner before directed the length of the compensating

material, the expansion of which will be equal to that of the rod of

the pendulum. Double this length, and increase the product by its

one-tenth part, which will give the total length required._ We shall

give examples of this as we proceed.

_Graham’s Mercurial Pendulum._

It was in the year 1721 that Graham first put up a pendulum of this

description, and subjected it to the test of experiment; but it appears

to have been afterwards set aside to make way for Harrison’s gridiron

pendulum, or for others of a similar description. For some years past,

however, its merits have been more generally known, and it is not

surprising that it should be considered as preferable to others, both

from the simplicity of its construction, and the perfect ease with

which the compensation may be adjusted.

We have already alluded to Mr. Baily’s very able paper on this

pendulum, and we shall take the liberty of extracting from it the

following description:--

At _fig. 223._ is a drawing of the mercurial pendulum, as

constructed in the manner proposed by Mr. Baily.

A Treatise on Mechanics · 第 27 / 28 段