PLATE VI. Fig. I.]

435. _Another_ ORRERY. In this Machine, which is the simplest I ever

saw, for shewing the diurnal and annual motions of the Earth, together

with the motion of the Moon and her Nodes; _A_ and _B_ are two oblong

square Plates held together by four upright pillars; of which three

appear at _f_, _g_, and _g_2. Under the Plate _A_ is an endless screw on

the Axis of the handle _b_, which works in a wheel fixed on the same

Axis with the double grooved wheel _E_; and on the top of this Axis is

fixed the toothed wheel _i_, which turns the pinion _k_, on the top of

whose Axis is the pinion _k_2 which turns another pinion _b_2, and that

other turns a third, on the Axis _a_2 of which is the Earth _U_ turning

round; this last Axis inclining 23-1/2 Degrees. The supporter _X_2, in

which the Axis of the Earth turns, is fixed to the moveable Plate _C_.

In the fixed Plate _B_, beyond _H_, is fixed the strong wire _d_, on

which hangs the Sun _T_ so as it may turn round the wire. To this Sun is

fixed the wire or solar ray _Z_, which (as the Earth _U_ turns round its

Axis) points to all the places that the Sun passes vertically over,

every day of the year. The Earth is half covered with a black cap _a_,

as in the former Orrery, for dividing the day from the night; and, as

the different places come out from below the edge of the cap, or go in

below it, they shew the times of Sun-rising and setting every day of the

year. This cap is fixed on the wire _b_, which has a forked piece _C_

turning round the wire _d_: and, as the Earth goes round the Sun, it

carries the Cap, Wire, and solar Ray round him; so that the solar Ray

constantly points towards the Earth’s Center.

On the Axis of the pinion _k_ is the pinion _m_, which turns a wheel on

the cock or supporter _n_, and on the Axis of this wheel nearest _n_ is

a pinion (hid from view) under the Plate _C_, which pinion turns a wheel

that carries the Moon _V_ round the Earth _U_; the Moon’s Axis rising

and falling in the socket _W_, which is fixed to the triangular piece

above _Z_; and this piece is fixed to the top of the Axis of the last

mentioned wheel. The socket _W_ is slit on the outermost side; and in

this slit the two pins near _Y_, fixed in the Moon’s Axis, move up and

down; one of them being above the inclined Plane _YX_, and the other

below it. By this mechanism, the Moon _V_ moves round the Earth _T_ in

the inclined Orbit _q_, parallel to the Plane of the Ring _YX_; of which

the Descending Node is at _X_, and the Ascending Node opposite to it,

but hid by the supporter _X_2.

The small wheel _E_ turns the large wheels _D_ and _F_, of equal

diameters, by cat-gut strings crossing between them: and the Axis of

these two wheels are cranked at _G_ and _H_, above the Plate _B_. The

upright stems of these cranks going through the Plate _C_, carry it over

and over the fixed Plate _B_, with a motion which carries the Earth _U_

round the Sun _T_, keeping the Earth’s Axis always parallel to itself;

or still inclining towards the left-hand of the Plate; and shewing the

vicissitudes of seasons, as described in the tenth chapter. As the Earth

goes round the Sun the pinion _k_ goes round the wheel _i_, for the Axis

of _k_ never touches the fixed Plate _B_; but turns on a wire fixed into

the Plate _C_.

On the top of the crank _G_ is an Index _L_, which goes round the Circle

_m_2 in the time that the Earth goes round the Sun; and points to the

days of the months; which, together with the names of the seasons, are

marked in this Circle.

This Index has a small grooved wheel _L_ fixed upon it, round which, and

the Plate _Z_, goes a cat-gut string crossing between them; and by this

means the Moon’s inclined Plane _YX_ with its Nodes is turned backward,

for shewing the times and returns of Eclipses § 319, 320.

The following parts of this machine must be considered as distinct from

those already described.

Towards the right hand, let _S_ be the Earth hung on the wire _e_, which

is fixed into the Plate _B_; and let _O_ be the Moon fixed on the Axis

_M_, and turning round within the cap _P_, in which, and in the Plate

_C_ the crooked wire _Q_ is fixed. On the Axis _M_ is also fixed the

Index _K_, which goes round a Circle _h_2, divided into 29-1/2 equal

parts, which are the days of the Moon’s age: but to avoid confusion in

the scheme, it is only marked with the numeral figures 1 2 3 4, for the

Quarters. As the crank _H_ carries this Moon round the Earth _S_ in the

Orbit _t_, she shews all her Phases by means of the cap _P_ for the

different days of her age, which are shewn by the Index _K_; this Index,

turning just as the Moon _O_ does, demonstrates her turning round her

Axis as she still keeps the same side towards the Earth _S_ § 262.

[Sidenote: PL. VIII.]

At the other end of the Plate _C_, a Moon _N_ goes round an Earth _R_ in

the Orbit _p_; but this Moon’s Axis is stuck fast into the Plate _C_ at

_S_2; so that neither Moon nor Axis can turn round; and as this Moon

goes round her Earth she shews herself all round to it; which proves,

that if the Moon was seen all round from the Earth in a Lunation, she

could not turn round her Axis.

_N. B._ If there were only the two wheels _D_ and _F_, with a cat-gut

string over them, but not crossing between them, the Axis of the Earth

_U_ would keep its parallelism round the Sun _T_, and shew all the

seasons; as I sometimes make these Machines: and the Moon _O_ would go

round the Earth _S_, shewing her Phases as above; as likewise would the

Moon _N_ round the Earth _R_; but then, neither could the diurnal motion

of the Earth _U_ on its Axis be shewn, nor the motion of the Moon _V_

round that Earth.

[Sidenote: The CALCULATOR.]

436. In the year 1746 I contrived a very simple Machine, and described

it’s performance in a small treatise upon the Phenomena of the Harvest

Moon, published in the year 1747. I improved it soon after, by adding

another wheel, and called it _the Calculator_. It may be easily made by

any Gentleman who has a mechanical Genius.

[Sidenote: Fig. I.]

The great flat Ring supported by twelve pillars, and on which the twelve

Signs with their respective Degrees are laid down, is the Ecliptic;

nearly in the center of it is the Sun _S_ supported by the strong

crooked Wire _I_; and from the Sun proceeds a Wire _W_, called _the

Solar Ray_, pointing towards the center of the Earth _E_, which is

furnished with a moveable Horizon _H_, together with a brazen Meridian,

and Quadrant of Altitude. _R_ is a small Ecliptic, whose Plane

co-incides with that of the great one, and has the like Signs and

Degrees marked upon it; and is supported by two Wires _D_ and _D_, which

enter into the Plate _PP_, but may be taken off at pleasure. As the

Earth goes round the Sun, the Signs of this small Circle keep parallel

to themselves, and to those of the great Ecliptic. When it is taken off,

and the solar Ray _W_ drawn farther out, so as almost to touch the

Horizon _H_, or the Quadrant of Altitude, the Horizon being rectified to

any given Latitude, and the Earth turned round its Axis by hand, the

point of the Wire _W_ shews the Sun’s Declination in passing over the

graduated brass Meridian, and his height at any given time upon the

Quadrant of Altitude, together with his Azimuth, or point of Bearing

upon the Horizon at that time; and likewise his Amplitude, and time of

Rising and Setting by the hour Index, for any day of the year that the

annual Index _U_ points to in the Circle of Months below the Sun. _M_ is

a solar Index or Pointer supported by the Wire _L_ which is fixed into

the knob _K_: the use of this Index is to shew the Sun’s place in the

Ecliptic every day in the year; for it goes over the Signs and Degrees

as the Index _U_ goes over the months and days; or rather as they pass

under the Index _U_, in moving the cover plate with the Earth and its

Furniture round the Sun; for the Index _U_ is fixed tight on the

immoveable Axis in the Center of the Machine. _K_ is a knob or handle

for moving the Earth round the Sun, and the Moon round the Earth.

As the Earth is carried round the Sun, its Axis constantly keeps the

same oblique direction, or parallel to itself § 48, 202, shewing thereby

the different lengths of days and nights at different times of the year,

with all the various seasons. And, in one annual revolution of the

Earth, the Moon _M_ goes 12-1/3 times round it from Change to Change,

having an occasional provision for shewing her different Phases. The

lower end of the Moon’s Axis bears by a small friction wheel upon the

inclined Plane _T_, which causes the Moon to rise above and sink below

the Ecliptic _R_ in every Lunation; crossing it in her Nodes, which

shift backward through all the Signs and Degrees of the said Ecliptic,

by the retrograde Motion of the inclined Plane _T_, in 18 years and 225

days. On this Plane the Degrees and Parts of the Moon’s North and South

Latitude are laid down from both the Nodes, one of which, _viz._ the

Descending Node appears at 0, by _DN_ above _B_; the other Node being

hid from Sight on this Plane by the plate _PP_; and from both Nodes, at

proper distances, as in the other Orrery, the limits of Eclipses are

marked, and all the solar and lunar Eclipses are shewn in the same

manner, for any given year, within the limits of 6000, either before or

after the Christian Æra. On the plate that covers the wheel-work, under

the Sun _S_, and round the knob _K_ are Astronomical Tables, by which

the Machine may be rectified to the beginning of any given year within

these limits, in three or four minutes of time; and when once set right,

may be turned backward for 300 years past, or forward for as many to

come, without requiring any new rectification. There is a method for its

adding up the 29th of _February_ every fourth year, and allowing only 28

days to that month for every other three: but all this being performed

by a particular manner of cutting the teeth of the wheels, and dividing

the month circle, too long and intricate to be described here, I shall

only shew how these motions may be performed near enough for common use,

by wheels with grooves and cat-gut strings round them, only here I must

put the Operator in mind that the grooves are to be made sharp (not

round) bottomed to keep the strings from slipping.

The Moon’s Axis moves up and down in the socket _N_ fixed into the bar

_O_ (which carries her round the Earth) as she rises above or sinks

below the Ecliptic; and immediately below the inclined Plane _T_ is a

flat circular plate (between _Y_ and _T_) on which the different

Excentricities of the Moon’s Orbit are laid down; and likewise her mean

Anomaly and elliptic Equation by which her true Place may be very nearly

found at any time. Below this Apogee-plate, which shews the Anomaly,

&_c_. is a Circle _Y_ divided into 29-1/2 equal parts which are the days

of the Moon’s age: and the forked end _A_ of the Index _AB_ (Fig II) may

be put into the Apogee-part of this plate; there being just such another

Index to put into the inclined Plane _T_ at the Ascending Node; and then

the curved points _B_ of these Indexes shew the direct motion of the

Apogee, and retrograde motion of the Nodes through the Ecliptic _R_,

with their Places in it at any given time. As the Moon _M_ goes round

the Earth _E_, she shews her Place every day in the Ecliptic _R_, and

the lower end of her Axis shews her Latitude and distance from her Node

on the inclined Plane _T_, also her distance from her Apogee and

Perigee, together with her mean Anomaly, the then Excentricity of her

Orbit, and her elliptic Equation, all on the Apogee Plate, and the day

of her age in the Circle _Y_ of 29-1/2 equal parts; for every day of the

year pointed out by the annual Index _U_ in the Circle of months.

Having rectified the Machine by the Tables for the beginning of any

year, move the Earth and Moon forward by the knob _K_, until the annual

Index comes to any given day of the month; then stop, and not only all

the above Phenomena may be shewn for that day, but also, by turning the

Earth round its Axis, the Declination, Azimuth, Amplitude, Altitude of

the Moon at any hour, and the times of her Rising and Setting, are shewn

by the Horizon, Quadrant of Altitude, and hour Index. And in moving the

Earth round the Sun, the days of all the New and Full Moons and Eclipses

in any given year are shewn. The Phenomena of the Harvest Moon, and

those of the Tides, by such a cap as that in Plate 9 Fig. 10. put upon

the Earth and Moon, together with the solution of many problems not here

related, are made conspicuous.

[Sidenote: PL. VIII.]

The easiest, though not the best way, that I can instruct any mechanical

person to make the wheel-work of such a machine, is as follows; which is

the way that I made it, before I thought of numbers exact enough to make

it worth the trouble of cutting teeth in the wheels.

[Sidenote: Fig. III.]

Fig. 3d of Plate 8 is a section of this Machine; in which _ABCD_ is a

frame of wood held together by four pillars at the corners, whereof two

appear at _AC_ and _BD_. In the lower Plate _CD_ of this Frame are three

small friction-wheels, at equal distances from each other; two of them

appearing at _e_ and _e_. As the frame is moved round, these wheels run

upon the fixed bottom Plate _EE_ which supports the whole work.

In the Center of this last mentioned Plate is fixed the upright Axis _f_

_FFG_, and on the same Axis is fixed the wheel _HHH_ in which are four

grooves _I_, _X_, _k_, _L_ of different Diameters. In these grooves are

cat-gut strings going also round the separate wheels _M_, _N_, _O_ and

_P_.

The wheel _M_ is fixed on a solid Spindle or Axis, the lower pivot of

which turns at _R_ in the under Plate of the moveable frame _ABCD_; and

on the upper end of this Axis is fixed the Plate _o o_ (which is _PP_,

under the Earth, in Fig. I.) and to this Plate is fixed, at an Angle of

23-1/2 Degrees inclination, the Dial-plate below the Earth _T_; on the

Axis of which, the Index _q_ is turned round by the Earth. This Axis,

together with the Wheel _M_, and Plate _o o_, keep their parallelism in

going round the Sun _S_.

On the Axis of the wheel _M_ is a moveable socket on which the small

wheel _N_ is fixed, and on the upper end of this socket is put on tight

(but so as it may be occasionally turned by hand) the bar _ZZ_ (_viz._

the bar _O_ in Fig. I.) which carries the Moon _m_ round the Earth _T_,

by the Socket _n_, fixed into the bar. As the Moon goes round the Earth

her Axis rises and falls in the Socket _n_; because, on the lower end of

her Axis, which is turned inward, there is a small friction Wheel _s_

running on the inclined Plane _X_ (which is _T_ in Fig. I.) and so

causes the Moon alternately to rise above and sink below the little

Ecliptic _VV_ (_R_ in Fig. I.) in every Lunation.

On the Socket or hollow Axis of the Wheel _N_, there is another Socket

on which the Wheel _O_ is fixed; and the Moon’s inclined Plane _X_ is

put tightly on the upper end of this Socket, not on a square, but on a

round, that it may be occasionally set by hand without wrenching the

Wheel or Axle.

Lastly, on the hollow Axis of the Wheel _O_ is another Socket on which

is fixed the Wheel _P_, and on the upper end of this Socket is put on

tightly the Apogee-plate _Y_, (that immediately below _T_ in Fig. I.)

all these Axles turn in the upper Plate of the moveable frame at _Q_

which Plate is covered with the thin Plate _cc_ (screwed to it) whereon

are the fore-mentioned Tables and month Circle in Fig. I.

The middle part of the thick fixed Wheel _HHH_ is much broader than the

rest of it, and comes out between the Wheels _M_ and _O_ almost to the

Wheel _N_. To adjust the diameters of the grooves of this fixed wheel to

the grooves of the separate Wheels _M_, _N_, _O_ and _P_, so as they may

perform their motions in the proper times, the following method must be

observed.

The Groove of the Wheel _M_, which keeps the parallelism of the Earth’s

Axis, must be precisely of the same Diameter as the lower Groove _I_ of

the fixed Wheel _HHH_; but, when this Groove is so well adjusted as to

shew, that in ever so many annual revolutions of the Earth, its Axis

keeps its parallelism, as may be observed by the solar Ray _W_ (Fig. I.)

always coming precisely to the same Degree of the small Ecliptic _R_ at

the end of every annual revolution, when the Index _M_ points to the

like Degree in the great Ecliptic; then, with the edge of a thin File

give the Groove of the Wheel _M_ a small rub all round; and by that

means, lessening the Diameter of the Groove, perhaps about the 20th part

of a hair’s breadth, it will cause the Earth to shew the precession of

the Equinoxes; which, in many annual revolutions will begin to be

sensible as the Earth’s Axis slowly deviates from its parallelism § 246,

towards the antecedent Signs of the Ecliptic.

The Diameter of the Groove of the Wheel _N_, which carries the Moon

round the Earth, must be to the Diameter of the Groove _X_ as a Lunation

is to a year; that is, as 29-1/2 to 365-1/4.

The Diameter of the Groove of the Wheel _O_, which turns the inclined

Plane _X_ with the Moon’s Nodes backward, must be to the Diameter of the

Groove _k_ as 20 to 18-225/365. And,

Lastly, the Diameter of the Groove of the Wheel _P_, which carries the

Moon’s Apogee forward, must be to the Diameter of the Groove _L_ as 70

to 62.

[Sidenote: PLATE IV.]

But, after all this nice adjustment of the Grooves to the proportional

times of their respective Wheels turning round, and which seems to

promise very well in Theory, there will still be found a necessity of a

farther adjustment by hand; because proper allowance must be made for

the Diameters of the cat-gut strings: and the Grooves must be so

adjusted by hand, as, that in the time the Earth is moved once round the

Sun, the Moon must perform 12 synodical revolutions round the Earth, and

be almost 11 days old in her 13th revolution. The inclined Plane with

its Nodes must go once round backward through all the Signs and Degrees

of the small Ecliptic in 18 annual revolutions of the Earth and 225 days

over. And the Apogee-plate must go once round forward, so as its Index

may go over all the Signs and Degrees of the small Ecliptic in eight

years (or so many annual revolutions of the Earth) and 312 days over.

_N. B._ The string which goes round the Grooves _X_ and _N_ for the

Moon’s Motion must cross between these Wheels; but all the rest of the

strings go in their respective Grooves _IM_, _kO_, and _LP_ without

crossing.

[Sidenote: The COMETARIUM.]

437. The COMETARIUM. This curious Machine shews the Motion of a Comet or

excentric Body moving round the Sun, describing equal Areas in equal

times § 152, and may be so contrived as to shew such a Motion for any

Degree of Excentricity. It was invented by the late Dr. _Desaguliers_.

[Sidenote: Fig. IV.]

The dark elliptical Groove round the letters _abcdefghiklm_ is the Orbit

of the Comet _Y_: this Comet is carried round in the Groove according to

the order of letters, by the Wire _W_, fixed in the Sun _S_, and slides

on the Wire as it approaches nearer to or recedes farther from the Sun,

being nearest of all in the Perihelion _a_, and farthest in the Aphelion

_g_. The Areas _aSb_, _bSc_, _cSd_ &c. or contents of these several

Triangles are all equal; and in every turn of the Winch _N_ the Comet

_Y_ is carried over one of these Areas; consequently in as much time as

it moves, from _f_ to _g_, or from _g_ to _h_, it moves from _m_ to _a_,

or from _a_ to _b_; and so of the rest, being quickest of all at _a_,

and slowest at _g_. Thus, the Comet’s velocity in its Orbit continually

decreases from the Perihelion _a_ to the Aphelion _g_; and increases in

the same proportion from _g_ to _a_.

[Sidenote: PLATE IV.]

The elliptic Orbit is divided into 12 equal Parts or Signs with their

respective Degrees, and so is the Circle _n o p q r s t n_ which

represents a great Circle in the Heavens, and to which all the fixed

Stars in the Comet’s way are referred. Whilst the Comet moves from _f_

to _g_ in its Orbit it appears to move only about 5 Degrees in this

Circle, as is shewn by the small knob on the end of the Wire _W_; but in

as short time as the Comet moves from _m_ to _a_, or from _a_ to _b_,

and it appears to describe the large space _tn_ or _no_ in the Heavens,

either of which spaces contains 120 Degrees or four Signs. Were the

Excentricity of its Orbit greater, the greater still would be the

difference of its Motion, and _vice versâ_.

_ABCDEFGHIKLMA_ is a circular Orbit for shewing the equable Motion of a

Body round the Sun _S_, describing equal Areas _ASB_, _BSC_, &c. in

equal times with those of the Body _Y_ in its elliptical Orbit above

mentioned; but with this difference, that the circular Motion describes

the equal Arcs _AB_, _BC_, &c. in the same equal times that the

elliptical Motion describes the unequal Arcs _ab_, _bc_, &c.

Now, suppose the two Bodies _Y_ and I to start from the Points _a_ and

_A_ at the same moment of time, and each having gone round its

respective Orbit, to arrive at these Points again at the same instant,

the Body _Y_ will be forwarder in its Orbit than the Body I all the way

from _a_ to _g_, and from _A_ to _G_; but I will be forwarder than _Y_

through all the other half of the Orbit; and the difference is equal to

the Equation of the Body _Y_ in its Orbit. At the Points _a_, _A_, and

_g_, _G_, that is, in the Perihelion and Aphelion, they will be equal;

and then the Equation vanishes. This shews why the Equation of a Body

moving in an elliptic Orbit, is added to the mean or supposed circular

Motion from the Perihelion to the Aphelion, and subtracted from the

Aphelion to the Perihelion, in Bodies moving round the Sun, or from the

Perigee to the Apogee, and from the Apogee to the Perigee in the Moon’s

Motion round the Earth, according to the Precepts in the 355th Article;

only we are to consider, that when Motion is turned into Time, it

reverses the titles in the Table of _The Moon’s elliptic Equation_.

[Sidenote: Fig. V.]

This curious Motion is performed in the following manner. _ABC_ is a

wooden bar (in the box containing the wheel-work) above which are the

wheels _D_ and _E_; and below it the elliptic Plates _FF_ and _GG_; each

Plate being fixed on an Axis in one of its Focuses, at _E_ and _K_; and

the Wheel _E_ is fixed on the same Axis with the Plate _FF_. These

Plates have Grooves round their edges precisely of equal Diameters to

one another, and in these Grooves is the cat-gut string _gg_, _gg_

crossing between the Plates at _h_. On _H_, the Axis of the handle or

winch _N_ in Fig. 4th, is an endless screw in Fig. 5, working in the

Wheels _D_ and _E_, whose numbers of teeth being equal, and should be

equal to the number of lines _aS_, _bS_, _cS_, &c. in Fig. 4, they turn

round their Axes in equal times to one another, and to the Motion of the

elliptic Plates. For, the Wheels _D_ and _E_ having equal numbers of

teeth, the Plate _FF_ being fixed on the same Axis with the Wheel _E_,

and the Plate _FF_ turning the equally big Plate _GG_ by a cat-gut

string round them both, they must all go round their Axes in as many

turns of the handle _N_ as either of the Wheels has teeth.

’Tis easy to see, that the end _h_ of the elliptical Plate _FF_ being

farther from its Axis _E_ than the opposite end _i_ is, must describe a

Circle so much the larger in proportion; and therefore move through so

much more space in the same time; and for that reason the end _h_ moves

so much faster than the end _i_, although it goes no sooner round the

Center _E_. But then, the quick-moving end _h_ of the Plate _FF_ leads

about the short end _hK_ of the Plate _GG_ with the same velocity; and

the slow moving end _i_ of the Plate _FF_ coming half round as to _B_,

must then lead the long end _k_ of the Plate _GG_ as slowly about: So

that the elliptical Plate _FF_ and it’s Axis _E_ move uniformly and

equally quick in every part of its revolution; but the elliptical Plate

_GG_, together with its Axis _K_ must move very unequally in different

parts of its revolution; the difference being always inversely as the

distance of any point of the Circumference of _GG_ from its Axis at _K_:

or in other words, to instance in two points, if the distance _Kk_ be

four, five, or six times as great as the distance _Kh_, the Point _h_

will move in that position four, five, or six times as fast as the Point

_k_ does, when the Plate _GG_ has gone half round: and so on for any

other Excentricity or difference of the Distances _Kk_ and _Kh_. The

tooth _i_ on the Plate _FF_ falls in between the two teeth at _k_ on the

Plate _GG_, by which means the revolution of the latter is so adjusted

to that of the former, that they can never vary from one another.

On the top of the Axis of the equally moving Wheel _D_, in Fig. 5th, is

the Sun _S_ in Fig. 4th; which Sun, by the Wire _Z_ fixed to it, carries

the Ball I round the Circle _ABCD_, &c. with an equable Motion according

to the order of the letters: and on the top of the Axis _K_ of the

unequally moving Ellipsis _GG_, in Fig. 5th, is the Sun _S_ in Fig. 4th,

carrying the Ball _Y_ unequably round in the elliptical Groove _a b c

d_, &c. _N.B._ This elliptical Groove must be precisely equal and

similar to the verge of the Plate _GG_, which is also equal to that of

_FF_.

In this manner, Machines may be made to shew the true Motion of the Moon

about the Earth, or of any Planet about the Sun; by making the

elliptical Plates of the same Excentricities, in proportion to the

Radius, as the Orbits of the Planets are whose Motions they represent:

and so, their different Equations in different parts of their Orbits may

be made plain to sight; and clearer Ideas of these Motions and Equations

acquired in half an hour, than could be gained from reading half a day

about such Motions and Equations.

[Sidenote: The improved CELESTIAL GLOBE.

Astronomy Explained Upon Sir Isaac Newton's Principles And made easy to those who have not studied mathematics · 第 239 / 275 题