ATTRACTION OF SPHERES.

Attraction of Spheres. 11. Spheres of the same homogeneous matter, attract particles placed on their surfaces, with forces proportional to their radii.

Spheres being similar solid figures, this proposition is no more than a particular case of what was before proved (8.).

Cor. If the spheres have different densities, the attractions at their surfaces are proportional to their radii multiplied by their densities (8. Cor.).

12. The force with which a particle, placed anywhere within a sphere of homogeneous matter, is urged towards the centre, is proportional to its distance from the centre.

Conceive a concentric sphere to be described, which contains the attracted particle in its surface; the matter between the two surfaces will exert no force on the particle (9.), which will therefore be urged to the centre, only by the attraction of the inner sphere, in the surface of which it is placed: but this force is proportional to the radius of the sphere, or to the distance of the particle from the centre (11.).

13. Let PNQ and ABC (fig. 7.) be two spheres of the same homogeneous matter, which attracts in the inverse proportion of the square of the distance: let the centres of the spheres be at M and D, and take MI equal to the radius of the sphere ABC, and ED equal to the radius of the sphere PNQ; the

attractions of the spheres upon particles placed at R and E are to one another as the squares of the radii of the spheres.

In the spheres draw two great circles perpendicular to the diameters PQ and AC, that pass through the points R and E; and let PpQ and AbC be two great circles, making equal indefinitely small angles NMP and BDd with the great circles PNQ and ABC. Let HK and FG, parallel to PQ and AC, be any two chords of the circles PpQ and AbC, that subtend similar arcs, or arcs containing the same number of degrees; and through HK and FG, let planes perpendicular to the circles PpQ and AbC, be drawn to cut the portions of the spheres contained in the angles NMP and BDd: join RH, RK, MH, MK, DF, DG, EF, EG. Because the arcs subtended by HK and FG, are like parts of their circumferences, it is plain, that the angle RMH = EDF, and RMK = EDG. And because ED = MH = MK, and RM = DF = DG (hyp.), therefore RH = EF, and RK = EG.

Conceive the chords HK and FG, together with the planes passing through them, to change their place a little, so as to describe two slender prisms, or elements of the portions of the spheres contained in the angles NMP and BDd. It is plain that MR and DO, the distances of the chords HG and FG from the centres of their circles, are constantly proportional to MN and DB, the radii of the spheres; wherefore RT and OS, the perpendicular sections of the small prisms, are similar figures, and have to one another the same ratio that MN^2 has to DO^2, or MN^2 to DB^2. Now, the attraction of the prism HK urging a particle at R to the centre M, is =

XT \times \left\{ \frac{1}{RH} - \frac{1}{RK} \right\} (10.); and the attraction of

the prism FG urging a particle at E to the centre D,

is = OS \times \left\{ \frac{1}{EF} - \frac{1}{EG} \right\}. But, in consequence

of what was proved, \frac{1}{RH} - \frac{1}{RK} = \frac{1}{EF} - \frac{1}{EG};

wherefore the attractions of the prisms are to one another as XT to OS, or as MN^2 to DB^2.—The same thing may be proved of all the elements of the two portions of the spheres contained in the angles NMP and BDd; wherefore those portions attract particles at R and E with forces proportional to the squares of the radii of the spheres. But because the small angles NMP and BDd are equal, each of the spheres may be divided into an equal number of such portions; wherefore the attractions of the whole spheres upon particles placed at R and E, are proportional to the squares of the radii of the spheres.

Cor. This proposition is true, when the particles of matter attract one another with forces proportional to any proposed function of the distance.

Let RH = EF = f, and RK = EG = f'; then, adopting the same notation as before (8. Cor.), the attractions of the prisms urging particles placed at R and E to the centres M and D, are respectively XT \times \pm \left\{ \Psi(f) - \Psi(f') \right\}, and OS \times \pm \left\{ \Psi(f) - \Psi(f') \right\}; consequently, those attractions have the same pro-

Attraction. portion that RT has to SO, or MN2 to DB2. Wherefore the attractions of the whole spheres are in the same proportion.

14. A particle placed anywhere without a sphere of homogeneous matter which attracts in the inverse proportion of the square of the distance, will be urged to the centre of the sphere, with a force that is inversely proportional to the square of the particle's distance from the centre.

Let ABC (Plate XXX. fig. 8.) be the sphere, O its centre, and P a particle without the sphere: conceive a concentric sphere PMN, of the same homogeneous matter with the sphere ABC, to be described with the radius PO. Then, by the last proposition, the attraction of the sphere ABC upon the particle P, is to the attraction of the sphere PMN upon a particle placed at A, as AO2 to PO2. But the attraction of the sphere PMN upon a particle placed at A, is equal to the attraction of the sphere ABC upon the same particle; for the attraction of the matter between the two spherical surfaces exerts no force upon a particle at A (9.). Wherefore, in the proportion set down above, the two middle terms are constantly the same wherever the point P is placed without the sphere ABC. Consequently, the first term of the proportion must follow the inverse ratio of the last term; that is, the attraction of the sphere ABC upon the external particle at P is inversely proportional to PO2.

15. The same law of attraction being supposed, a homogeneous sphere will attract a particle placed without it, with the same force as if all the matter of the sphere were collected in the centre.

Let f denote the distance of the particle from the centre; then it follows, from the last proposition, that the attraction of the sphere upon the particle will have, for its measure, \frac{A}{f^2}; A denoting a constant quantity that will be determined by any particular case; that is, by the actual attractive force corresponding to any determinate distance from the centre. Let r denote the radius of the sphere, and M its mass; then no part of the matter of the sphere being nearer the attracted particle than (f-r), and none of it more remote than (f+r), the attraction of the sphere on the particle will be

greater than \frac{M}{(f+r)^2}, and less than \frac{M}{(f-r)^2}. There-

fore \frac{A}{f^2} is always contained between those limits,

which requires that A = M. For, if A were greater than M, such values of f might be found as would

make \frac{A}{f^2} equal to, or greater than \frac{M}{(f-r)^2}; and, if A were less than M, such values of f might be found

as would make \frac{A}{f^2} equal to, or less than \frac{M}{(f+r)^2}. Therefore A = M; and the attraction of the sphere

is equal to \frac{M}{f^2}, or the same as if all the matter were

collected in the centre.

VOL. I. PART II.

If the radius of the sphere = r, the density of the matter contained in it = d; then the mass, or M =

\frac{4\pi r^3 d}{3} (\pi being the circumference of the circle whose diameter is unit), and the attraction of the sphere at

the distance f from the centre = \frac{4\pi r^3 d}{3f^2}. This is still

true at the surface of the sphere when f = r, so that

the attraction at the surface = \frac{4\pi r d}{3}; which expres-

sion, with the help of what is proved in (12.), enables us to compare the intensities of the attractions of homogeneous spheres, at all distances from the centre, without or within the surfaces.

Cor. 1. A shell of homogeneous matter contained between two concentric spherical surfaces, will attract a particle placed without it, with the same force as if all the matter of the shell were collected in its centre.

For the attractive force of such a shell is equal to the difference of the attractions of two concentric spheres of the same homogeneous matter with the shell.

Cor. 2. A sphere composed of concentric shells, that vary in their densities according to any law, will attract a particle placed without it, with the same force as if all the matter were collected in the centre.

For this having been proved of one shell (Cor. 1.), it must be true of any number of shells.

If \phi(r) denote the density at the distance r from the centre, the quantity of matter in the sphere will be 4\pi \int \phi(r) \cdot r^2 dr; and the attraction on a particle without the sphere at the distance f from the

centre = \frac{4\pi \int \phi(r) \cdot r^2 dr}{f^2}.

16. Two spheres, each composed of concentric shells of variable density, attract one another with the same force as if all the matter of each were collected in its centre.

For the attraction of a sphere A upon every particle of another sphere B will remain the same, if we suppose all the matter of A to be collected in its centre (15.). But the attraction of any particles of matter placed in A's centre, upon the sphere B, is equal and opposite to the attraction of B, upon the same matter so placed: and, again, the attraction of B upon all the particles placed in the centre of A, will remain unchanged, if we suppose the matter of B to be collected in its centre. Wherefore A attracts B with the same force as if the matter of each were collected in its centre.

17. Supposing that the particles of matter attract with a force proportional to the distance, a body of any shape will attract a particle of matter placed anywhere with the same force, and in the same direction, as if all the matter of the body were collected in its centre of gravity.

Suppose that the attracted particle is placed at P (fig. 9.), and the centre of gravity of the attracting body at G: join PG, and let any plane pass through that line. Let I be a small part, or element of the body, and

Attraction. from L draw LK perpendicular to the plane passing through PG, and KF perpendicular to PG; join PL and PK. Put dm to denote the quantity of matter, or the mass of the element L; then its attractive force, urging the particle in the direction PL, is = PL \times dm, which, by the resolution of forces, is equivalent to the two forces, PK \times dm and KL \times dm; and, again, the single force PK \times dm is equivalent to the two forces FK \times dm, and PF \times dm = PG \times dm + GF \times dm. Therefore, the attraction of the element L, upon the particle at P, is equivalent to these four separate forces, viz. PG \times dm, GF \times dm, FK \times dm, KL \times dm, which urge the particle P respectively in the directions, PG, GF, FK, KL. But, from the nature of the centre of gravity, the sum of all the forces, KL \times dm, that urge the particle P to one side of the plane passing through PG, is just equal to the sum of the forces that urge it to the other side of the same plane; and the sum of all the forces, FK \times dm, that urge P to one side of the line PG, is just equal to the sum of the forces that urge it to the other side of the same line; and the sum of all the forces, GF \times dm, that urge P towards the point G, is just equal to the sum of the forces that urge it from the same point. Wherefore all the preceding forces mutually destroy one another, excepting the forces, PG \times dm, the sum of which, when extended to all the elements of the attracting body, is = PG \times mass of the body. Wherefore the whole attraction upon P is the same as if all the matter of the body were collected in its centre of gravity.

Cor. Supposing that the particles of matter attract with a force proportional to the distance, a homogeneous sphere will attract a particle placed anywhere in the same manner as if all the matter of the sphere were collected in the centre.

For the centre of gravity of a homogeneous sphere, is the same as the centre of its figure. This corollary is likewise true of a sphere composed of concentric shells of variable density; and it is easy to apply the demonstration of (16.) to prove that, in this law of attraction, two spheres, each composed of concentric shells of variable density, will attract one another with the same force as if the matter of each were collected in its centre.

18. To investigate what are the laws of attraction, in regard to the distance, according to which a shell of homogeneous matter, contained between two concentric spherical surfaces, will attract a particle placed without it, in the same manner as if all the matter of the shell were collected in the centre.

It has been proved that this property actually belongs to homogeneous shells in the law of attraction which obtains in nature, and likewise when the particles of matter attract with a force proportional to the distance; but it is interesting to know whether it is confined to these two cases alone, or extends to other laws of attraction. This can only be discovered by a direct analysis.

Let r = PC (fig. 10.), the distance of the attracted point from the centre of the shell; u = CA the radius of the inner surface of the shell; f = PM, the distance of P from any point in the surface. Having drawn the diameter AD through P, let AMD and AND be two great circles, making, with one another,

an indefinitely small angle MAN = dq; and let two small circles BMG, bmG, indefinitely near one another, of which A and D are the poles, meet the former circles in M, N, m, n; and draw MS, NS to the centre of the circle BMG. Put \delta for the measure of the arc AM; then MS = u \sin. \delta; MN = dq \cdot u \sin. \delta; Mm = u d\delta; and the quadrilateral space MNmm = u^2 \cdot dq \cdot d\delta \sin. \delta. We may suppose the thickness of the shell indefinitely small; since, if the property belong to an elementary shell indefinitely thin, it will be true of one of a determinate thickness, which can be resolved into such elements. Suppose the thickness of the shell to be = du; then, the quantity of matter in the part standing upon the quadrilateral space MNmm = u^2 du \cdot dq \cdot d\delta \sin. \delta. Let \phi(f) represent the direct attraction of a particle at M in the direction PM; then its attraction directed to the

\text{centre } C = \phi(f) \times \frac{PS}{PM} = \frac{r - u \cos. \delta}{f} \times \phi(f);

and the attraction of the element of the shell in the same direction = u^2 du \cdot dq \cdot d\delta \sin. \delta \times \frac{r - u \cos. \delta}{f} \cdot \phi(f).

This expression is proportional to dq, when \delta and f remain constant; and, therefore (denoting by \sigma the circumference of the circle whose diameter is unit), the attraction of the whole zone contained between the small circles BMG, bmG, will be = 2\pi \cdot u^2 du \cdot d\delta \sin. \delta.

\frac{r - u \cos. \delta}{f} \cdot \phi(f); and the attractive force of the whole shell will be

2\pi \cdot u^2 du \int d\delta \sin. \delta \cdot \frac{r - u \cos. \delta}{f} \cdot \phi(f);

the fluent to be extended from \delta = 0 to \delta = \pi.

Again, the quantity of matter in the shell is = 4\pi \cdot u^2 du; and the attraction of this matter placed in the centre, at the distance r from P, is = 4\pi \cdot u^2 du \cdot \phi(r).

If now we equate the attraction of the shell, to the attraction of its matter placed in the centre, and leave out the factors common to both, we shall get

2\pi(r) = \int d\delta \sin. \delta \cdot \frac{r - u \cos. \delta}{f} \cdot \phi(f)

the limits of the integral being the same as before.

But f^2 = r^2 - 2ru \cos. \delta + u^2; then d\delta \sin. \delta = \frac{df}{r}; also r - u \cos. \delta = \frac{f^2 + r^2 - u^2}{2r}; wherefore,

by substitution, we get

4 \cdot r^2 \phi(r) \cdot u = \int (f^2 + r^2 - u^2) \cdot df \cdot \phi(f);

or, which is equivalent, 4 \cdot r^2 \phi(r) \cdot u =

(f^2 + r^2 - u^2) \cdot \int df \cdot \phi(f) - 2 \int f df \int df \cdot \phi(f),

the limits of this integral being from f = r - u to f = r + u, which correspond to \delta = 0 and \delta = \pi.

Now let \int df \cdot \phi(f) = \Psi(f); and \int f df \int df \cdot \phi(f) = \int f df \cdot \Psi(f) = \Psi'(f); then, by taking the fluents between the proper limits, we get

\underbrace{\text{Attraction.}}_{4r^2\phi(r).u = 2r \cdot \left\{ (r+u)\Psi(r+u) - (r-u)\Psi(r-u) \right\} - 2 \left\{ \Psi'(r+u) - \Psi'(r-u) \right\} }

If we develop the binomial functions in the last expression, all the even powers of u will disappear, and the odd powers only will remain; these last terms being all contained in this general formula,

\text{viz. } \frac{4}{1.2.3 \dots 2n+1} \cdot \left\{ r \cdot \frac{d^{2n+1} r \Psi(r)}{dr^{2n+1}} - \frac{d^{2n+1} r \Psi'(r)}{dr^{2n+1}} \right\} \cdot u^{2n+1};

and, observing that \frac{d \cdot \Psi'(r)}{dr} = r\Psi(r), the same expression will become \frac{4}{1.2.3 \dots 2n+1} \cdot \left\{ r \cdot \frac{d^{2n+1} r \Psi(r)}{dr^{2n+1}} - \frac{d^{2n+1} r \Psi(r)}{dr^{2n+1}} \right\} \cdot u^{2n+1};

which, again, is more simply expressed thus, viz.

\frac{4r^2}{1.2.3 \dots 2n+1} \cdot \frac{d}{dr} \left\{ \frac{1}{r} \cdot \frac{d^{2n} r \Psi(r)}{dr^{2n}} \right\} \cdot u^{2n+1}.

Wherefore, by substituting the development instead of the functions, and then, by dividing by \frac{1}{4} r^2 u, we get

\phi(r) = \frac{d \cdot \Psi(r)}{dr} + \frac{1}{1.2.3} \cdot \frac{d}{dr} \left\{ \frac{1}{r} \cdot \frac{d^2 r \Psi(r)}{dr^2} \right\} \cdot u^2 + \frac{1}{1.2.3.4.5} \cdot \frac{d}{dr} \left\{ \frac{1}{r} \cdot \frac{d^4 r \Psi(r)}{dr^4} \right\} \cdot u^4 + \&c.

From the nature of the function \Psi(r), we get \phi(r) = \frac{d \cdot \Psi(r)}{dr}; wherefore each of the remaining terms must be separately equal to nothing: Hence

\frac{d}{dr} \left\{ \frac{1}{r} \cdot \frac{d^2 r \Psi(r)}{dr^2} \right\} = 0;

from which we find r \Psi(r) = \frac{1}{2} A r^3 + A' r - A'', A, A', A'' being arbitrary constant quantities; and this value of r \Psi(r), it is plain, will likewise render all the succeeding terms of the development evanescent. Wherefore

\phi(r) = \frac{d \cdot \Psi(r)}{dr} = A r + \frac{A'}{r^2}.

Thus the most general expression of the law of attraction, that possesses the property in question, is a combination of the two laws above mentioned, with each of which it coincides, according as we make the one or other of the constant quantities equal to nothing. We have therefore a direct proof, that the law of nature is the only one which will make the attraction decrease as the distance increases, and in which a spherical shell, or a sphere, will attract in the same

manner as if all the matter were collected in the Attraction centre.

Laplace has arrived at the same conclusion by a different process. (Mech. Celeste, Liv. 2d. Chap. 2. No. 12. Rem. Part.)

ATTRACTION OF SPHEROIDS OF REVOLUTION.

19. Let APBQ (Plate XXXI. fig. 11.) and CMDN Attraction be two concentric ellipses, similar to one another, and similarly situated, of which AB and CD are either the greater, or less, axes; and let PQ be perpendicular to AB. Conceive the ellipses to revolve about PQ, so as to describe an indefinitely small angle; then, supposing the law of attraction to be inversely proportional to the square of the distance, the thin solid of homogeneous matter described by the ellipse APBQ, will attract a particle placed at P, in a direction perpendicular to any plane passing through PQ, with the same force that the thin solid of the same matter described by the ellipse CMDN, will attract a particle placed at C perpendicularly to the same plane.

From C draw CM, CN, making equal angles with CD, and PR, PT respectively parallel to CM, CN; and let Cm, Cn, Pr, Pt, be drawn in the same manner, and indefinitely near the former lines. While the ellipses revolve about PQ, the small sectors will describe pyramids that have their vertices at C and P. It is manifest that the pyramids so described are similar: for their angles at C and P in the planes of the ellipses are equal; and their other angles described by revolving about PQ are likewise equal, because the sectors are equally inclined to that axis. Wherefore, the direct attractions of all the small pyramids upon the particles P and C, are proportional to the lengths PR, PT, CM, CN (7); and consequently the forces that urge the particles P and C in a direction at right angles to any plane passing through PQ, are proportional to the perpendiculars let fall upon that plane from R, T, M, N. But, because PR, PT, CM, CN are equally inclined to PQ, they will make equal angles with any plane passing through PQ: wherefore the perpendiculars drawn to the plane from R, T, M, N, will be respectively proportional to CM, CN, PR, PT. But CM + CN = PR + PT (6): wherefore, the sum of the perpendiculars drawn to the plane from M and N, will be equal to the sum of the perpendiculars drawn to it from R and T. Consequently the force of the pyramids PR and PT, which urges the particle P at right angles to the plane, is equal to the force of the pyramids CM and CN, which urges the particle C in a parallel direction. The same thing is true of all the small pyramids that make up the thin solids described by the ellipses APBQ and CMDN; and it is therefore true of the whole solids.

It is to be observed, that when the pyramids PR and PT fall on opposite sides of PQ, it is the difference of their attractions which is equal to the sum of the attractions of CM and CN; and it is the difference of the perpendiculars let fall from T and R on opposite sides of the plane, which is equal to the sum of the perpendiculars let fall from M and N.

Attraction. 20. Let APBQ be a spheroid of revolution, PQ the axis of revolution, and ACB a plane through the centre perpendicular to PQ (Plate XXXI, fig. 12.). If D be a particle in the surface of the spheroid, and DL perpendicular to the plane ACB; then the attraction of the spheroid on a particle placed at the pole P, will be to the force with which a particle placed at C, is attracted in the direction DL, as PC is to DL.

Through D draw a plane parallel to the plane ACB, and let the plane so drawn cut the axis PQ in F: draw the straight line DFE to terminate in the spheroid, and describe another spheroid through F, having the same centre with the spheroid APBQ, and similar to it, and similarly situated. Conceive an indefinitely great number of planes, making indefinitely small angles with one another, to be drawn through DE, so as to divide the two spheroids into an indefinitely great number of thin solids, or slices: then the sections which every one of the planes make with the spheroids will be similar ellipses, having the same centre (5.): and it is manifest that a straight line drawn through F at right angles to DE, in any one of the planes, will pass through the centre of the two ellipses contained in it, and will coincide with an axis of each. Wherefore, the force with which every one of the slices, or elements, of the spheroid APBQ attracts a particle placed at D in the direction DL, is equal to the force with which the corresponding slice, or element, of the spheroid GFHK, attracts a particle placed at F in the direction FC (19.). Wherefore, the whole attraction of the spheroid APBQ upon a particle at D, in the direction DL, is equal to the whole attraction of the spheroid GFHK, upon a particle at F. But the attractions of the spheroids APBQ and GFHK, upon particles placed at P and F, are to one another as PC to FC (8.). Wherefore, the attraction of the spheroid APBQ upon a particle at P, is to the force with which the same spheroid attracts a particle at D, in the direction DL, as PC is to FC or DL.

21. Let APBQ be a spheroid of revolution, and PQ the axis of revolution, as before. If D be a particle in the surface, ADPB (fig. 13.) a section through D, and the axis PQ, and DL perpendicular to PQ; the attraction of the spheroid upon a particle at A, will be to the force with which a particle at D is attracted, in the direction DL, as AC is to DL.

Through D draw a plane perpendicular to AB, which cuts the section ADPB in the straight line DFE; and let a spheroid GFHK be described through F, having the same centre with the spheroid APBQ, and similar to it, and similarly situated. Then, conceiving the two spheroids to be divided into an indefinitely great number of thin slices by planes passing through DE, the force with which every slice, or element, of the spheroid APBQ attracts a particle at D in the direction DL, will be equal to the force with which the corresponding slice, or element, of the spheroid GFHK attracts a particle at F (19.). But the attractions of the spheroids APBQ and GFHK upon particles placed at A and F, are to one another as AC to CF (8.). Wherefore, the attraction of the spheroid APBQ upon a particle at A, is to the force with which the same

spheroid attracts a particle at D, in the direction DL, as AC to FL or DL. Attraction.

The two last propositions will enable us to find both the direction and the intensity of the attraction of a homogeneous spheroid of revolution upon a particle placed anywhere on the surface, when we have ascertained the attractive forces at the poles, and at the circumference of the circular section made by a plane through the centre perpendicular to the axis. For the whole attraction at any point, is the compound force arising from the attractions perpendicular to the axis, and parallel to it. The next object of our research is, therefore, to determine the two forces above-mentioned, viz. the attraction at the poles, and at the circular section, equally distant from both poles.

22. Let ABD be an indefinitely slender pyramid, of which the base BD is perpendicular to the edge AD (fig. 14.): let B = base BD, and f = length

AD; then \frac{B}{f^2} = the attraction of the whole matter of the pyramid upon a particle placed at the vertex A.

Let AM = x; then the section MN parallel to the base BD = \frac{B \cdot x^2}{f^2}; and, MP = element of the

prism = \frac{B \cdot x^2 dx}{f^2}; and the attraction of the element

upon a particle placed at A = \frac{MP}{AM^2} = \frac{B \cdot dx}{f^2}; the

fluent of which is = \frac{Bx}{f^2} = attraction of the pyramid

AM upon a particle at A. And, when x = f, this

becomes = \frac{B}{f} = attraction of the pyramid AD upon a particle placed at A.

23. To investigate the attraction of a homogeneous spheroid of revolution, upon a particle placed at the pole.

Let P (fig. 15.) be the pole, PCQ the axis of revolution, and APBQ a section of the spheroid by a plane passing through PQ, and any point M, in the surface; draw PM, Pm indefinitely near PM, and Mm perpendicular to Pm. Conceive the plane PMQ to revolve about PQ, so as to describe the indefinitely small angle BCO; then the small triangle MPm will describe a slender pyramid, having its vertex at P, and of which the base is a rectangle, contained by Mm and RT; for the point M moving parallel to R, it will describe a line equal and parallel to that described by R, namely, to RT.

Let PM = f; and the angle KPM, which PM makes with a perpendicular to the axis, = \theta; and the indefinitely small angle BCO = d\phi. Then Mm = fd\theta; RT = CR \times d\phi = f \cos. \theta \cdot d\phi; and B, the base of the slender pyramid described by the triangle MPm, = d\phi \cdot d\theta \cos. \theta \cdot f^2; wherefore, the direct attraction

of the pyramid on a particle at P = \frac{B}{f} (22) =

Attraction, d\phi \cdot d\theta \cos. \theta \cdot f; and the elementary attraction of the spheroid in the direction PC = direct attraction of the pyramid \times \frac{PS}{PM} = d\phi \cdot d\theta \cos. \theta \sin. \theta \cdot f.

Again, let MR = x, CR = y, PC = k, AC = k'; then y = f \cos. \theta; x = k - f \sin. \theta; if we substitute these values in the equation of the solid (1.), we get \frac{(k - f \sin. \theta)^2}{k^2} + \frac{f^2 \cos. \theta^2}{k'^2} = 1; whence

f = \frac{2k'^2 k}{k^2} \cdot \frac{\sin. \theta}{\cos. \theta^2 + \frac{k'^2}{k^2} \sin. \theta^2}.

By substituting the value of f just found in the preceding expression of the elementary attraction of spheroid, it will become

\frac{2k'^2 k}{k^2} d\phi \cdot \frac{d\theta \cos. \theta \cdot \sin. \theta}{\cos. \theta^2 + \frac{k'^2}{k^2} \sin. \theta^2};

which must be integrated from \phi = 0 to \phi = 2\pi; and from \theta = 0 to \theta = \frac{\pi}{2}; \tau denoting always the half-circumference when radius is unit.

In an oblate spheroid k is less than k'; put k'^2 - k^2 = k^2 \cdot e^2, and z = \sin. \theta; then the element of the attractive force will become, by substitution,

\frac{2k'^2 k}{k^2} d\phi \cdot \frac{z^2 dz}{1 + e^2 z^2} = \frac{2k'^2 k}{k^2 e^2} d\phi \cdot \left\{ e dz - \frac{e dz}{1 + e^2 z^2} \right\};

and by integrating from z = 0 to z = 1, we get,

\frac{2k'^2 k}{k^2 e^2} d\phi \cdot \left\{ e - \text{arc. tan. } e \right\};

for the force with which the matter between the planes PBQ and POQ urges the particle P to the centre. Wherefore the whole attractive force of the spheroid upon a particle at P is =

\frac{4\pi \cdot k'^2 k}{k^2 e^2} \cdot \left\{ e - \text{arc. tan. } e \right\};

And, because \frac{4\pi \cdot k'^2 k}{s} = mass of the spheroid = M, we get the measure of the attraction of the oblate spheroid upon a particle placed at the pole, equal to

k \cdot \frac{3M}{k^2 e^2} \cdot \left\{ e - \text{arc. tan. } e \right\}.

In an oblong spheroid, k is greater than k'; put k^2 - k'^2 = k^2 \cdot e^2; then the element of the attractive force will become, by substitution,

\frac{2k'^2 k}{k^2} d\phi \cdot \frac{z^2 dz}{1 - e^2 z^2} = \frac{2k'^2 k}{k^2 e^2} d\phi \cdot \left\{ \frac{e dz}{1 - e^2 z^2} - e dz \right\};

whence, by proceeding as before, we get the measure of the attractive force of the oblong spheroid on a particle placed at the pole, equal to

k \cdot \frac{3M}{k^2 e^2} \cdot \left\{ \frac{1}{2} \text{hyp. log. } \frac{1+e}{1-e} - e \right\}.

Cor. In an oblate spheroid differing little from a sphere, e^2 will be a very small fraction, of which we

may reject the higher powers. When this is done, Attraction, the preceding expression of the polar attraction, viz.

\frac{4\pi \cdot k k'^2}{k^2 e^2} \cdot (e - \text{arc. tan. } e),

will be = 4\pi k \cdot (1 + e^2) \left( \frac{1}{3} - \frac{1}{3} e^2 \right) = \frac{4\pi k}{3} \cdot \left( 1 + \frac{2}{5} e^2 \right).

And, if k' = k + \tau = k \sqrt{1 + e^2}, be the radius of the equator, then \frac{2}{k} = e^2; so that the attraction at the pole will be

\frac{4\pi k}{3} \cdot \left( 1 + \frac{4}{5} \cdot \frac{\tau}{k} \right).

24. To investigate the attraction of a homogeneous spheroid of revolution, on a particle placed in the circumference of the circular section, made by a plane through the centre, at right angles, to the axis of revolution.

Let P (Plate XXXI. fig. 16.) be the pole, PC the axis of revolution. A, a point in the circular section AOB, made by a plane through the centre perpendicular to PC. Let M be any point in the surface of the spheroid: AMO a section through A and M by a plane perpendicular to AOB; Am a line in that plane indefinitely near AM, and Mm perpendicular to Am; MR perpendicular to AO, and RS to AB. Conceive the plane AMO to revolve about A, so as to describe an indefinitely small angle OAQ; then the triangle AMm will describe a slender pyramid, having its vertex at A, and of which the base is equal to a rectangle contained by Mm and RT; for the point M moving parallel to the point R, it will describe a line equal to that described by R, namely to RT.

Let AM = f; the angle MAR = \theta; and the angle OAQ = d\phi; then Mm = f d\theta; and TR = AR \times d\phi = f \cos. \theta \cdot d\phi. Wherefore, B = base of the pyramid described by AMm = d\phi \cdot d\theta \cos. \theta \cdot f^2; and the direct attraction of the pyramid in the direction AM = \frac{B}{f} = d\phi \cdot d\theta \cos. \theta \cdot f. Wherefore, the elementary attraction of the spheroid, in the direction AC = direct attraction of the pyramid \times \frac{AR}{AM} \times \frac{AS}{AR} = d\phi \cos. \theta \cdot d\theta \cos. \theta \cdot f.

Again, let MR = x, RS = y, CS = z, CP = k and AC = k'; then (1.)

\frac{x^2}{k^2} + \frac{y^2 + z^2}{k'^2} = 1.

But x = f \sin. \theta; y = AR \cdot \sin. \phi = f \cos. \theta \sin. \phi; and z = k' - f \cos. \theta \cos. \phi; wherefore, by substitution, we get

\frac{f^2 \sin. \theta^2}{k^2} + \frac{f^2 \cos. \theta^2 \sin. \phi^2}{k'^2} + \frac{(k' - f \cos. \theta \cos. \phi)^2}{k'^2} = 1.

From this equation we get

f = 2k' \cdot \frac{\cos. \theta \cos. \phi}{\cos. \theta^2 + \frac{k'^2}{k^2} \sin. \theta^2}.

Let this value of f be substituted in the expression of the elementary attraction of the spheroid before found, and it will become

2k' \cdot d\varphi \cos^2 \varphi \cdot \frac{d\theta \cos^2 \theta}{\cos^2 \theta + \frac{k'^2}{k^2} \sin^2 \theta} :

which expression, when integrated from \varphi = 0 to \varphi = \pi, and from \theta = 0 to \theta = \frac{1}{2}\pi, will give the attraction of half the spheroid: and the double of it, viz.

4k' \cdot d\varphi \cos^2 \varphi \cdot \frac{d\theta \cos^2 \theta}{\cos^2 \theta + \frac{k'^2}{k^2} \sin^2 \theta},

being integrated between the same limits, will give the whole attraction of the spheroid.

In the oblate spheroid, k is less than k': Let k'^2 = k^2 + e^2, and z = \sin \varphi: and, by substitution, the element of the attractive force will become

4k' \cdot d\varphi \cos^2 \varphi \cdot \frac{dz(1-z^2)}{1+e^2z^2} = 4k' \cdot d\varphi \cos^2 \varphi \cdot \frac{1+e^2}{e^2} \cdot \left\{ \frac{e dz}{1+e^2z^2} - \frac{e dz}{1+e^2} \right\}.

And, by integrating from z = 0 to z = 1, we get

4k' \cdot d\varphi \cos^2 \varphi \cdot \frac{1+e^2}{e^2} \cdot \left\{ \text{arc. tan. } e - \frac{e}{1+e^2} \right\},

for the force with which the matter between the sections that contain the angle OAQ, attracts the particle A to the centre. But \int d\varphi \cos^2 \varphi =

\int \frac{d\varphi}{2} \cdot (1 + \cos^2 \varphi) = \frac{\varphi}{2} + \frac{1}{4} \sin 2\varphi; \text{ the value of}

which, between the limits \varphi = 0, and \varphi = \pi, is = \frac{\pi}{2}:

wherefore, the attraction of the spheroid on a particle at A, is equal to

2\pi \cdot k' \cdot \frac{1+e^2}{e^2} \cdot \left\{ \text{arc. tan. } e - \frac{e}{1+e^2} \right\}.
\text{Because } \frac{4\pi \cdot k'^2 k}{3} = \frac{4\pi \cdot k^2 \cdot (1+e^2)}{3} = M; \text{ we}
\text{get } 2\pi \cdot (1+e^2) = \frac{3M}{2k^2}; \text{ wherefore, the measure}

of the attractive force of the oblate spheroid on a particle placed anywhere in the circumference of the circular section made by a plane through the centre at right angles to the axis, is equal to

k' \cdot \frac{3M}{2k^2 \cdot e^2} \cdot \left\{ \text{arc. tan. } e - \frac{e}{1+e^2} \right\}.

In the oblong spheroid, k is greater than k'; put k^2 = k'^2 + e^2: then the element of the attractive force will become, by substitution,

4k' \cdot d\varphi \cos^2 \varphi \cdot \frac{dz(1-z^2)}{1-e^2z^2} = 4k' \cdot d\varphi \cos^2 \varphi \cdot \frac{1-e^2}{e^2} \cdot \left\{ \frac{e dz}{1-e^2} - \frac{e dz}{1-e^2z^2} \right\} :

whence, by proceeding as before, we get the measure of the attractive force of the oblong spheroid upon a particle placed anywhere in the circumference of the circular section, made by a plane through the centre at right angles to the axis, equal to

k' \cdot \frac{3M}{2k^2 \cdot e^2} \cdot \left\{ \frac{e}{1-e^2} - \frac{1}{2} \text{hyp. log. } \frac{1+e}{1-e} \right\}. \quad \text{Attraction.}

Cor. In an oblate spheroid, differing little from a sphere, the higher powers of e^2 may be neglected. The expression of the attractive force at the equator,

\text{viz. } 2\pi \cdot k' \cdot \frac{1+e^2}{e^2} \cdot \left\{ \text{arc. tan. } e - \frac{e}{1+e^2} \right\}

will then become

2\pi \cdot k' \cdot (1+e^2) \left( \frac{2}{3} - \frac{4}{5} e^2 \right) = \frac{4\pi k'}{3} \cdot (1 - \frac{1}{5} e^2).

And if k', the radius of the equator, = k + \tau; then

\frac{2\pi}{k} = e^2 \text{ (23. Cor.)}; \text{ and the attraction at the equator}

will be equal to

\frac{4\pi k}{3} \cdot \left( 1 + \frac{\tau}{k} \right) \cdot \left( 1 - \frac{2}{5} \cdot \frac{\tau}{k} \right) = \frac{4\pi k}{3} \cdot \left( 1 + \frac{3}{5} \cdot \frac{\tau}{k} \right).

25. An oblate spheroid of revolution being given, it is required to find the measures of the attractive forces that urge a particle placed anywhere in the surface, in a direction perpendicular to the axis, and in a direction parallel to it.

Let k and k' be the semiaxes of the ellipse by the revolution of which the spheroid is described, k being the axis about which it revolves: and let b be the perpendicular distance of the particle from the axis, and a its distance from the plane, drawn through the centre at right angles to the axis: Then, from which was proved in (20.) and (21.), the attractions sought will be found by multiplying the attractions at the pole, and at the circular section equally distant from both poles, by \frac{a}{k} and \frac{b}{k'}.

Thus we get the attraction in the direction of a, equal to

a \times \frac{3M}{k \cdot e^2} \cdot \left\{ e - \text{arc. tan. } e \right\};

and the attraction in the direction of b, equal to

b \times \frac{3M}{2k^2 \cdot e^2} \cdot \left\{ \text{arc. tan. } e - \frac{e}{1+e^2} \right\}.

The same formulae likewise serve for finding the attractions upon a particle placed anywhere within the spheroid. For the attraction upon a particle within the spheroid is equal to the attraction of a similar concentric spheroid, which contains the particle in its surface (9.); and it is evident, that the coefficients, which multiply a and b in the above expressions, depend only upon the proportion of k and k'; and they are therefore the same for all similar spheroids.

If we denote by A and B the coefficients of a and b in the expressions of the attractive force found above, the whole attraction of the spheroid, which is compounded of the forces a \cdot A and b \cdot B, will

be = \sqrt{a^2 A^2 + b^2 B^2}. And if \Psi denote the angle which the direction of this force makes with a, or

with the axis of the spheroid; then \tan. \Psi = \frac{b \cdot B}{a \cdot A}.

Attraction. Cor. In the very same manner we may determine the attractions of an oblong spheroid of revolution, upon a point in the surface, or within the solid.

26. If k, k', k'', the semiaxes of a homogeneous ellipsoid, be related to those of another ellipsoid of the same matter, h, h', h'', so that k^2 - k'^2 = h^2 - h'^2 and k'^2 - k''^2 = h'^2 - h''^2, the attractions perpendicular to the planes of the principal sections, which the first ellipsoid (Plate XXI. fig. 17.) exerts upon a point determined by the coordinates h \sin m, h' \cos m \sin n, h'' \cos m \cos n, respectively parallel to k, k', k'', will be to the attractions which the second ellipsoid exerts upon a point determined by the coordinates k \sin m, k' \cos m \sin n, k'' \cos m \cos n, respectively parallel to h, h', h'', in the direct proportion of the areas of the principal sections to which the attractions are perpendicular.

This proposition is an extension to all elliptical spheroids of what was proved of the sphere in (13.). It is here enunciated of the ellipsoid, because the demonstration is not more difficult for that solid than for spheroids of revolution.

Let ABDM be an ellipsoid, the semiaxes of which are BC = k, EC = k', AC = k''; and acdm another ellipsoid, of which the semiaxes are, bc = h, ec = h', ac = h''; those quantities being so related, that k^2 - k'^2 = h^2 - h'^2, and k'^2 - k''^2 = h'^2 - h''^2. Also, let G be a point about the ellipsoid ABDM, so determined that GH, parallel to BC, = h \sin m; HK, parallel to CE, = h' \cos m \sin n; and CK = h'' \cos m \cos n; and let g be a point about the ellipsoid acdm, so determined that gh, parallel to bc, = k \sin m; hk, parallel to ce, = k' \cos m \sin n; and ck = k'' \cos m \cos n. Then the force with which the ellipsoid ABDM attracts a particle placed at G in the direction GH, will be to the force with which the ellipsoid acdm attracts a particle placed at g in the direction gh, as the area of the section AEDM to the area of the section acdm, or as k' k'' to h' h''.

Let RP = k \sin \theta; PO = k' \cos \theta \sin \phi; and CO = k'' \cos \theta \cos \phi; which suppositions are allowable, because they satisfy the equation of the ellipsoid (1.), whatever be the angles \theta and \phi. Draw CPM through the centre, and CN indefinitely near it; then CP = \cos \theta \sqrt{k'^2 \sin^2 \phi + k''^2 \cos^2 \phi}; and when \cos \theta = 1, CM = \sqrt{k'^2 \sin^2 \phi + k''^2 \cos^2 \phi}:

wherefore \frac{CP}{CM} = \cos \theta. Let the angle DCM = \Psi;

then \tan \Psi = \frac{PO}{CO} = \frac{k'}{k''} \tan \phi; and, by taking the

fluxions, \frac{d\Psi}{\cos^2 \Psi} = \frac{k'}{k''} \cdot \frac{d\phi}{\cos^2 \phi}; but \frac{1}{\cos^2 \Psi} = 1 +

\tan^2 \Psi = \frac{k'^2 \sin^2 \phi + k''^2 \cos^2 \phi}{k''^2 \cos^2 \phi} = \frac{CM^2}{k''^2 \cos^2 \phi};

wherefore d\Psi \cdot CM^2 = twice the sector MCN = k' k'' d\phi.

And, in like manner, in the other ellipsoid, if rp = h \sin \theta; po = h' \cos \theta \sin \phi; and co = h'' \cos \theta \cos \phi:

then \frac{cp}{co} = \cos \theta, and twice the sector mcn = h' h'' d\phi.

It is plain, from what has been shown, that, when Attraction, \theta varies, and \phi remains constant in the expressions of the coordinates, the points P and p will move along

CM and cm, so that, in every position, \frac{PC}{MC} = \frac{pc}{mc}.

Let Q and q be indefinitely near P and p; and through P and Q draw lines parallel to MN; and through p and q draw lines parallel to mn. Let S denote the quadrilateral contained between the parallels drawn through P and Q; and S' that contained between

the lines drawn through p and q: Then \frac{S}{MCN} =

\frac{QC^2 - PC^2}{MC^2}; and \frac{S'}{MCN} = \frac{qc^2 - pc^2}{mc^2}; wherefore,

since \frac{PC}{MC} = \frac{pc}{mc}, and \frac{QC}{MC} = \frac{qc}{mc}, it is manifest that

\frac{S}{MCN} = \frac{k' k''}{h' h''}.

Upon the quadrilaterals S and S' let upright prisms RS and rs be erected, and be prolonged to meet the surfaces of the spheroids; join GR, GS, gr, gs. Then,

GR^2 = (h \sin m - k \sin \theta)^2 + (h' \cos m \sin n - k' \cos \theta \sin \phi)^2;

+ (h'' \cos m \cos n - k'' \cos \theta \cos \phi)^2;

gr^2 = (k \sin m - h \sin \theta)^2 + (k' \cos m \sin n - h' \cos \theta \sin \phi)^2;

+ (k'' \cos m \cos n - h'' \cos \theta \cos \phi)^2;

And, by expanding these expressions, we get

GR^2 = \left\{ (h^2 + (k'^2 - k^2) \cos^2 m \sin^2 n + (h''^2 - k''^2) \cos^2 m \cos^2 n) \right.

+ (k^2 + (k'^2 - k^2) \cos^2 \theta \sin^2 \phi + (k''^2 - k''^2) \cos^2 \theta \cos^2 \phi)

- 2(hk \sin m \sin \theta + h'k' \cos m \cos \theta \sin n \sin \phi + h''k'' \cos m \cos \theta \cos n \cos \phi) \left. \right\};

gr^2 = \left\{ (k^2 + (k'^2 - k^2) \cos^2 m \sin^2 n + (k''^2 - k''^2) \cos^2 m \cos^2 n) \right.

+ (h^2 + (h'^2 - h^2) \cos^2 \theta \sin^2 \phi + (h''^2 - h''^2) \cos^2 \theta \cos^2 \phi)

- 2(hk \sin m \sin \theta + h'k' \cos m \cos \theta \sin n \sin \phi + h''k'' \cos m \cos \theta \cos n \cos \phi) \left. \right\}.

These expressions are equal, because k'^2 - k^2 = h'^2 - h^2, and k''^2 - k^2 = h''^2 - h^2: wherefore RG = rg = f. And, in like manner, it is shown, that GS = gs = f'.

Now, the attraction of the prism RS urging a particle at G in the direction GH, is equal to

S \times \left\{ \frac{1}{f} - \frac{1}{f'} \right\} (10); and the attraction of the prism rs urging a particle at g in the direction gh,

is S' \times \left\{ \frac{1}{f} - \frac{1}{f'} \right\}: wherefore these attractions

Attraction. are to one another as S to S', or as k'k'' to h'h''. The same thing may be proved of all the elementary prisms that make up the two portions of the spheroids contained between the planes BCM, BCN, and bcn, bcn': wherefore, those portions attract particles at G and g, with forces proportional to k'k'' and h'h''. But the two spheroids may be divided into an equal number of such portions: wherefore the spheroids attract particles placed at G and g, in the directions GH and gh, with forces proportional to k'k'' and h'h'', or to the sections AMDE and amde.

Cor. 1. This proposition is true when the law of attraction is expressed by any function of the distance. The demonstration is the same as in the corollary of (13).

Cor. 2. If the two ellipsoids be so placed, that their centres, and the planes of their principal sections, shall coincide, the surface of the one will be entirely within the other. Also the point which one ellipsoid attracts, will be in the surface of the other, as is plain from the expressions of the coordinate. And hence, the attraction of one ellipsoid upon a point without the surface, is made to depend upon the attraction of another ellipsoid upon a point within the surface.

Cor. 3. When the ellipsoids become spheroids of revolution, the two principal sections through the axis of revolution become equal, and will be represented by any two sections whatever passing through the axis at right angles to one another. But, in this case, the attractions of the spheroids on the points may be reduced to two, one acting perpendicular to the axis, and one parallel to it: And it is plain, that these attractions will be to one another as the areas of the sections, perpendicular to their directions.

27. To find the attraction of an oblate spheroid upon a particle placed without the surface.

Let k' be the radius of the equator, and k the axis of revolution: and let a be the perpendicular distance of the point without the spheroid from the plane of the equator, and b its distance from the axis. In the first place, it is necessary to determine the semiaxis of another oblate spheroid that shall contain the given point in its surface, and such, that it shall have the same centre, and its equator in the same plane, as the given spheroid; and likewise, the difference of the squares of its semiaxes equal to the difference of the squares of the semiaxes of the given spheroid. Let h' denote the radius of the equator, and h the semiaxis of the required spheroid: then, because the attracted point is to be in the surface of

the solid, we have \frac{a^2}{h^2} + \frac{b^2}{h'^2} = 1: and, because

h'^2 - k^2 = k'^2 - k^2 = i^2; \text{ we get}
\frac{a^2}{k^2} + \frac{b^2}{k'^2} = 1:

Whence,

2k^2 = a^2 + b^2 - i^2 + \sqrt{(a^2 + b^2 - i^2)^2 + 4a^2i^2};

and when h is determined, then h' = \sqrt{k^2 + i^2}.

In consequence of the equation \frac{a^2}{h^2} + \frac{b^2}{h'^2} = 1, Attraction.

we may suppose, a = h \sin. m, and b = h' \cos. m;

let a' = k \sin. m, and b' = k' \cos. m; or a' = \frac{k}{h} a,

and b' = \frac{k'}{h'} \times b: then the point determined by the

coordinates a' and b' will be in the surface of the given spheroid, and, consequently, it will be within the surface of the other spheroid. Let M' denote the mass of the spheroid of which the axis is h; and let

e'^2 = \frac{h'^2 - k^2}{h^2} = \frac{k'^2 - k^2}{h^2}; \text{ then (25.) the attractions}

of this spheroid upon the point within its surface, determined by the coordinates a and b, are these, viz.

That perpendicular to the equator, equal to

a' \times \frac{3M'}{h^3 e'^3} \cdot \left\{ e' - \text{arc. tan. } e' \right\};

and that perpendicular to the axis, equal to

b' \times \frac{3M'}{2h^3 e'^3} \cdot \left\{ \text{arc. tan. } e' - \frac{e'}{1 + e'^2} \right\}.

But (26. Cor. 3.) the attractions of the given spheroid, whose semiaxis are k and k' upon the point without its surface determined by the coordinates a and b, will be found by multiplying the preceding expressions respectively by \frac{k'^2}{k^2} and \frac{kk'}{hh'}. Let M be the

mass of the given spheroid; then \frac{M}{M'} = \frac{k'^2 k}{h^2 h'}; conse-

quently \frac{k'^2}{k^2} = \frac{M}{M'} \cdot \frac{h}{k} = \frac{M}{M'} \cdot \frac{a}{a'}; and \frac{kk'}{hh'} =

\frac{M}{M'} \cdot \frac{h'}{k'} = \frac{M}{M'} \cdot \frac{b}{b'}: Wherefore, the attractions of the given oblate spheroid upon a point, without the surface determined by the coordinates a and b, are as follows, viz.

The attraction perpendicular to the equator, equal to

a \times \frac{3M}{h^3 e'^3} \cdot \left\{ e' - \text{arc. tan. } e' \right\};

and that perpendicular to the axis, equal to

b \times \frac{3M}{2h^3 e'^3} \cdot \left\{ \text{arc. tan. } e' - \frac{e'}{1 + e'^2} \right\}.

Cor. In the very same manner we may determine the attractions of an oblong spheroid of revolution upon a point without the surface.

ATTRACTIONS OF ELLIPSOIDS.

28. Let AMBN be one of the principal sections of Attractions an ellipsoid, C the centre, AB and MN the axes, D a point in the periphery of the section, and DO perpendicular to MN (Plate XXXI. fig. 18.); the attraction of the ellipsoid upon a particle placed at the pole A, is to the force with which a particle placed at D is attracted in the direction DO, as AC to DO.

Attraction. Draw DFG perpendicular to AB, and through F describe an ellipsoid similar to the given ellipsoid, and similarly situated, and having the same centre. Conceive an indefinitely great number of planes making indefinitely small angles with one another, to be drawn through DG, so as to divide the two ellipsoids into an indefinitely great number of thin solids or slices: Then, the sections of the ellipsoids made by every one of the planes will be similar and concentric ellipses, each of them having an axis perpendicular to DG (5.). Wherefore the attractions of the elements of the ellipsoid FHKL upon a particle at F, are respectively equal to the attractions of the elements of the ellipsoid AMBN, upon a particle at D in the direction DO (19.). Wherefore, the whole attraction of the ellipsoid FHKL upon a particle at F, is equal to the attraction of the ellipsoid AMBN upon a particle at D, in the direction DO. But the attractions of the ellipsoids AMBN, and FHKL upon particles at A and F, are to one another as AC to CF (8.). Wherefore, the attraction of the ellipsoid AMBN upon a particle at the pole A, is to the force with which it attracts a particle at D in the direction DO, as AC to DO.

29. The attractions of ellipsoids upon particles placed in the surface, urging them in directions perpendicular to any of the principal sections, are proportional to the distances of the particles from that section.

Let AMBN be one of the principal sections of an ellipsoid, C the centre, AB and MN the axes of the section, and P a point in the surface of the solid; the attraction of the ellipsoid upon a particle at the pole A (Plate XXXI. fig. 19.), is to the force with which a particle at P is attracted in a direction parallel to AB, as the semiaxis AC is to the distance of P from the principal section perpendicular to AC.

Draw PDQ perpendicular to the section AMBN, and let it meet the surface again in Q; through D describe an ellipsoid similar to AMBN, similarly situated, and having the same centre; and through P draw a section SPRQ perpendicular to AB. As before, divide the solids into an indefinitely great number of thin slices by planes drawn through PQ: the sections made by every one of those planes will be similar, and concentric ellipses having an axis of each perpendicular to PQ (5.). Wherefore, the attractions of the elements of the ellipsoid AMBN, upon a particle at P, in a direction perpendicular to the plane PRQS, are respectively equal to the attractions of the elements of the ellipsoid FHKL, upon a particle at D, in a direction perpendicular to the same plane (19.). Wherefore, the attraction of the ellipsoid AMBN, upon a particle at P, in a direction parallel to the axis AB, is equal to the attraction of the ellipsoid FHKL, upon a particle at D in the same direction. But the ellipsoids AMBN and FHKL being similar, their attractions upon particles at A and F, are to one another as AC to CF (8.); and the attraction of the ellipsoid FHKL, upon a particle at the pole F, is to its attraction upon a particle at D, in a direction parallel to AC, as FC to CN (28.). Wherefore (ex aequali), the attraction of the ellipsoid AMBN, upon a particle, at the pole A, is to the force with which it attracts a particle at P, in the direction AC, as AC to CN.

This proposition will enable us to find the attraction.

VOL. I. PART II.

tions of an ellipsoid on all points on the surface, or Attraction. within the solid, when the attractions at the poles are determined.

30. To investigate the differential expressions of the attractions at the poles of an ellipsoid.

Let APD be an ellipsoid; C the centre; AC, CE, and PC, the semiaxes; and PMB a section made by a plane through PC and any point, M in the surface: draw PM (fig. 20.) Pm indefinitely near PM, and Mm perpendicular to Pm: also MR perpendicular to the plane ADB, MS perpendicular to PC, and RH perpendicular to AD. Conceive the plane PCB to revolve about PC, so as to describe an indefinitely small angle BCO; and let PM = f; the angle KPM, which PM makes with a perpendicular to the axis, = \theta; and the angle DCB = \varphi: then by proceeding as in (23), it will be found that the attraction of the small pyramid described by the triangle MPm, urging a particle at P to the centre of the ellipsoid, is = d\varphi \cdot d\theta \cos. \theta \sin. \theta \cdot f.

Again, let MR = x, HR = y, CH = z; also let PC = k, AC = k', CE = k''; then x = k \sin. \theta; y = f \cos. \theta \sin. \varphi; z = f \cos. \theta \cos. \varphi; and if we substitute these values in the equation of the ellipsoid (1.), we shall get

\frac{(k - f \sin. \theta)^2}{k^2} + \frac{f^2 \cos. \theta \sin. \varphi}{k'^2} + \frac{f^2 \cos. \theta \cos. \varphi}{k''^2}

= 1: whence

f = \frac{k}{k^2} \cdot \frac{2 \sin. \theta}{\frac{\sin. \theta}{k^2} + \frac{\cos. \theta \sin. \varphi}{k'^2} + \frac{\cos. \theta \cos. \varphi}{k''^2}}

This is the value of f at the pole of k; and, by a like procedure, its values at the poles of k' and k'' may be found, viz.

f = \frac{k'}{k'^2} \cdot \frac{2 \sin. \theta}{\frac{\sin. \theta}{k^2} + \frac{\cos. \theta \sin. \varphi}{k^2} + \frac{\cos. \theta \cos. \varphi}{k''^2}}
f = \frac{k''}{k''^2} \cdot \frac{2 \sin. \theta}{\frac{\sin. \theta}{k^2} + \frac{\cos. \theta \sin. \varphi}{k^2} + \frac{\cos. \theta \cos. \varphi}{k^2}}

Suppose that k is the least of the semiaxes; and let k^2 = \frac{k^2}{m}, and k'^2 = \frac{k^2}{n}: then the values of f at the poles of k, k', k'', will be, respectively,

f = \frac{2k \sin. \theta}{\sin. \theta + m \cos. \theta \sin. \varphi + n \cos. \theta \cos. \varphi}
f = \frac{2k' \sin. \theta \times m}{m \sin. \theta + \cos. \theta \sin. \varphi + n \cos. \theta \cos. \varphi}
f = \frac{2k'' \sin. \theta \times n}{n \sin. \theta + \cos. \theta \sin. \varphi + m \cos. \theta \cos. \varphi}

Now, let A, A', A'', denote the attractions of the spheroid upon particles placed at the poles of k, k', k''; then, by substituting the values of f just found in the foregoing differential expression, we get

A = k \times \iint \frac{2 d\varphi d\theta \cos. \theta \sin. \theta}{\sin. \theta + m \cos. \theta \sin. \varphi + n \cos. \theta \cos. \varphi}

A M

\text{Attraction.} \quad A' = k' \times \iint \frac{m \times 2 d\phi \cdot d\theta \cos. \theta \sin. 2\theta}{m \sin. 2\theta + \cos. 2\theta \sin. 2\phi + n \cos. 2\theta \cos. 2\phi}
A'' = k'' \times \iint \frac{n \times 2 d\phi \cdot d\theta \cos. \theta \sin. 2\theta}{n \sin. 2\theta + \cos. 2\theta \sin. 2\phi + m \cos. 2\theta \cos. 2\phi}

the limits of the integrals being from \theta = 0 and \phi = 0 to \theta = \frac{\pi}{2} and \phi = 2\pi.

31. To reduce the expressions of the polar attractions to the most simple integrals.

Let us consider the general expression

\iint \frac{d\phi \cdot d\theta \cos. \theta \sin. 2\theta}{\alpha \sin. 2\theta + \beta \cos. 2\theta \sin. 2\phi + \gamma \cos. 2\theta \cos. 2\phi}

which includes all the formulas found in (30.) Let p = \alpha \sin. 2\theta + \beta \cos. 2\theta; and q = \alpha \sin. 2\theta + \gamma \cos. 2\theta; then the above expression will become

\iint \frac{d\phi \cdot d\theta \cos. \theta \sin. 2\theta}{p \sin. 2\phi + q \cos. 2\phi}.

Suppose \sqrt{\frac{q}{p}} \cdot \frac{\sin. \phi}{\cos. \phi} = \frac{\sin. u}{\cos. u}; then the preceding expression will become, by substitution,

\iint \frac{du \cdot d\theta \cos. \theta \sin. 2\theta}{\sqrt{p \cdot q}};

the limits of u being from 0 to 2\pi; wherefore, by integrating with regard to u, and restoring the values of p and q, the integral becomes

2\pi \cdot \int \frac{d\theta \cdot \cos. \theta \sin. 2\theta}{\sqrt{(\alpha \sin. 2\theta + \beta \cos. 2\theta) \cdot (\alpha \sin. 2\theta + \gamma \cos. 2\theta)}}

and, by putting x = \sin. \theta, the integral, which is to be taken from \theta = 0 to \theta = \frac{\pi}{2}, or from x = 0 to x = 1, will become

2\pi \cdot \int \frac{x^2 dx}{\sqrt{\{\beta + (\alpha - \beta)x^2\} \cdot \{\gamma + (\alpha - \gamma)x^2\}}}

If now we take \alpha, \beta, \gamma, so as to make the assumed expression coincide with the quantities A, A', A'', respectively, we shall get

A = 4\pi k \cdot \int \frac{x^2 dx}{\sqrt{\{m + (1-m)x^2\} \cdot \{n + (1-n)x^2\}}}
A' = 4\pi k' \cdot \int \frac{m \cdot x^2 dx}{\sqrt{\{1 + (m-1)x^2\} \cdot \{n + (m-n)x^2\}}}
A'' = 4\pi k'' \cdot \int \frac{n \cdot x^2 dx}{\sqrt{\{1 + (n-1)x^2\} \cdot \{m + (n-m)x^2\}}}

These expressions have the inconvenience of containing different factors in the denominators; but they may be reduced to others having the same factors, by putting x = \frac{\tau}{\sqrt{m + (1-m)\tau^2}} in the second and x =

\frac{\tau}{\sqrt{n + (1-n)\tau^2}} in the third; we thus get

A = 4\pi k \cdot \int \frac{x^2 dx}{\sqrt{\{m + (1-m)x^2\} \cdot \{n + (1-n)x^2\}}} \quad \text{Attraction.}
A' = 4\pi k' \cdot \int \frac{m \cdot \tau^2 d\tau}{\sqrt{\{m + (1-m)\tau^2\} \cdot \{n + (1-n)\tau^2\}}}
A'' = 4\pi k'' \cdot \int \frac{n \cdot \tau^2 d\tau}{\sqrt{\{n + (1-n)\tau^2\} \cdot \{m + (1-m)\tau^2\}}}

Now let

\frac{1-m}{m} = \frac{k^2 - k'^2}{k^2} = \lambda^2; \text{ and } \frac{1-n}{n} = \frac{k'^2 - k^2}{k^2} = \lambda'^2;

Also let the mass of the ellipsoid = M = \frac{4\pi k k' k''}{3}; then \frac{3M}{k^3} = \frac{4\pi}{\sqrt{mn}}; wherefore, by substitution, we get

A = k \cdot \frac{3M}{k^3} \cdot \int \frac{x^2 dx}{\sqrt{(1 + \lambda^2 x^2) \cdot (1 + \lambda'^2 x^2)}}
A' = k' \cdot \frac{3M}{k^3} \cdot \int \frac{x^2 dx}{\sqrt{\{1 + \lambda^2 x^2\} \cdot \{1 + \lambda'^2 x^2\}}}
A'' = k'' \cdot \frac{3M}{k^3} \cdot \int \frac{x^2 dx}{\sqrt{\{1 + \lambda^2 x^2\} \cdot \{1 + \lambda'^2 x^2\}}}

the integrations extending from x = 0 to x = 1.

These integrals cannot be expressed in finite terms. When \lambda and \lambda', or the eccentricities of the ellipsoid are small, the values of the integrals may easily be found to a sufficient degree of exactness, by series. They may likewise be all expressed by means of this fluent, viz.

F = \int \frac{dx}{\sqrt{(1 + \lambda^2 x^2) \cdot (1 + \lambda'^2 x^2)}} \quad (\text{from } x = 0 \text{ to } x = 1) \text{ and its partial fluxions. Thus we have, in general,}
\frac{x^2}{\sqrt{(1 + \lambda^2 x^2) \cdot (1 + \lambda'^2 x^2)}} = \frac{1}{\lambda} \cdot \left( \frac{dF}{d\lambda} \right) + \frac{1}{\lambda'} \cdot \left( \frac{dF}{d\lambda'} \right)

Wherefore, making x = 1, we get

A = k \cdot \frac{3M}{k^3} \cdot \left\{ \frac{1}{\sqrt{(1 + \lambda^2) \cdot (1 + \lambda'^2)}} + \frac{1}{\lambda} \left( \frac{dF}{d\lambda} \right) + \frac{1}{\lambda'} \left( \frac{dF}{d\lambda'} \right) \right\}
A' = k' \cdot \frac{3M}{k^3} \cdot \frac{1}{\lambda} \cdot \left( \frac{dF}{d\lambda} \right).
A'' = k'' \cdot \frac{3M}{k^3} \cdot \frac{1}{\lambda'} \cdot \left( \frac{dF}{d\lambda'} \right).

32. To find the forces with which a homogeneous ellipsoid attracts a particle placed in the surface, or within the solid, in directions perpendicular to the principal sections.

Let k, k', k'', denote the semiaxes of an ellipsoid,

Attraction, and a, b, c (respectively parallel to k, k', k''), the perpendicular distances of a particle placed in the surface, or within the solid, from the principal sections: then, from what is proved in (29.), the attractions we are seeking will be found by multiplying the polar attractions by \frac{a}{k}, \frac{b}{k'}, \frac{c}{k''}. Wherefore the forces that urge the particle in the directions of a, b, and c, are respectively, a \times \frac{3M}{k^3}.

\left\{ \frac{1}{\sqrt{(1+\lambda^2)(1+\lambda'^2)}} + \frac{1}{\lambda} \left( \frac{dF}{d\lambda} \right) + \left( \frac{dF}{d\lambda'} \right) \right\}; b \times \frac{3M}{k'^3} \cdot \frac{1}{\lambda} \left( \frac{dF}{d\lambda} \right); c \times \frac{3M}{k''^3} \cdot \frac{1}{\lambda'} \left( \frac{dF}{d\lambda'} \right);

Which formulas serve both for points in the surface, and within the solid, for the reason already explained in (25.).

33. To find the attractions of an ellipsoid upon a particle placed without the surface.

Let k, k', k'' be the semiaxes of the ellipsoid, and a, b, c (respectively parallel to k, k', k''), the coordinates of a particle without the surface. Let h, h', h'', so related to k, k', k'', that k^2 - h^2 = k'^2 - h'^2 and k''^2 - h''^2 = k'^2 - h'^2, denote the semiaxes of another ellipsoid, which contains the attracted point in its surface, and has its principal sections in the same planes as the given ellipsoid: then, because the attracted point is in the surface, we have (1.)

\frac{a^2}{h^2} + \frac{b^2}{h'^2} + \frac{c^2}{h''^2} = 1:

And, because h^2 - h'^2 = k^2 - k'^2 = i^2, and h''^2 - h'^2 = k''^2 - k'^2 = i^2, we get

\frac{a^2}{h^2} + \frac{b^2}{h^2 + i^2} + \frac{c^2}{h^2 + i^2} = 1.

This equation now contains only one unknown quantity; and it is plain, that one value of h, and only one, can be found from it. For, when h = 0, the function on the left hand side is infinitely great: And while h increases from 0 ad infinitum, the same function decreases continually from being infinitely great, to be infinitely little. When h is found, then h' = \sqrt{h^2 + i^2}, and h'' = \sqrt{h^2 + i^2}. Because a, b, c, are the coordinates of a point in the surface of the ellipsoid, we may suppose a = h \sin. m, b = h' \cos. m \sin. n, c = h'' \cos. m \cos. n: let a' = k \sin. m, b' = k' \cos. m \sin. n, c' = k'' \cos. m \cos. n; or a' = \frac{k}{h} \times a,

b' = \frac{k'}{h'} \times b, c' = \frac{k''}{h''} \times c; \text{ then } a', b', c', \text{ will be the}

coordinates of a point in the surface of the given ellipsoid, and consequently, it will be within the other solid. Let M' denote the mass of the ellipsoid of

which h, h', h'' are the semiaxes; also let \lambda^2 = \frac{k^2 - h^2}{k^2} = \frac{k'^2 - h'^2}{k'^2}; and \lambda'^2 = \frac{h'^2 - h^2}{h'^2} = \frac{k'^2 - h'^2}{h'^2}; Attraction.

then, F denoting the same fluent as before, the attractions of this ellipsoid upon the point within it, determined by the coordinates a', b', c', in the directions of those coordinates, are (32.) respectively equal to

a' \times \frac{3M'}{h^3} \left\{ \frac{1}{\sqrt{(1+\lambda^2)(1+\lambda'^2)}} + \frac{1}{\lambda} \left( \frac{dF}{d\lambda} \right) + \frac{1}{\lambda'} \left( \frac{dF}{d\lambda'} \right) \right\}; b' \times \frac{3M'}{h'^3} \times \frac{1}{\lambda} \left( \frac{dF}{d\lambda} \right), c' \times \frac{3M'}{h''^3} \times \frac{1}{\lambda'} \left( \frac{dF}{d\lambda'} \right).

Now, the attractions of the given ellipsoid upon the point without the surface, determined by the coordinates a, b, c, will be found (26.) by multiplying the preceding expressions respectively by \frac{k}{h}, \frac{k'}{h'}, \frac{k''}{h''},

Let M be the mass of the given ellipsoid; then \frac{M}{M'} = \frac{k k' k''}{h h' h''}; consequently \frac{k k'}{h h'} = \frac{M}{M'} \frac{h}{k} = \frac{M}{M'}.

\frac{a}{a'} = \frac{h}{k} \times \frac{k'}{h'} = \frac{M}{M'} \times \frac{b}{b'}; \text{ and } \frac{k k'}{h h'} = \frac{M}{M'} \times \frac{c}{c'};
\frac{a}{a'} = \frac{h}{k} \times \frac{k'}{h'} = \frac{M}{M'} \times \frac{b}{b'}; \text{ and } \frac{k k'}{h h'} = \frac{M}{M'} \times \frac{c}{c'};

wherefore, the attractions of the given ellipsoid upon the point without the surface, determined by a, b, c, in the directions of those coordinates, are respectively equal

\text{to } a \times \frac{3M}{h^3} \times \left\{ \frac{1}{\sqrt{(1+\lambda^2)(1+\lambda'^2)}} + \frac{1}{\lambda} \left( \frac{dF}{d\lambda} \right) + \frac{1}{\lambda'} \left( \frac{dF}{d\lambda'} \right) \right\}, b \times \frac{3M}{h'^3} \times \frac{1}{\lambda} \left( \frac{dF}{d\lambda} \right) c \times \frac{3M}{h''^3} \times \frac{1}{\lambda'} \left( \frac{dF}{d\lambda'} \right).

The preceding propositions contain a complete theory of homogeneous elliptical spheroids. They enable us to compute the attractive force with which a solid of this kind urges a particle placed anywhere in the surface, or within the solid, or without it. It remains, indeed, to find the exact value of the function F in its general form, to which we can do no more than approximate by series; but this is an analytical difficulty, which it is impossible to overcome; because the nature of this function is such, that it cannot be expressed in finite terms by the received notation of analysis.

Attraction
||
Atwood.

In the preceding investigations, we have followed the method of Maclaurin for points situated in the surface of a spheroid, or within the solid. This method has always been justly admired; but neither its inventor, nor, as far as we know, any other Geometer, has applied it, except to spheroids of revolution; and it is here, for the first time, extended to ellipsoids. In regard to points without the surface, we have employed the method first given by Mr Ivory, in the Philosophical Transactions for 1809. The combination of these two methods has enabled us to derive the attractions of an ellipsoid on a point placed anywhere, from the attractions at the poles. Thus, this extremely complicated problem has, by geometrical reasoning of no great difficulty, been reduced to the investigation of the polar attractions, which are the only cases that require a direct computation.

34. Of the attractions of spheroids composed of elliptical shells that vary in their densities and figures according to any law. Attraction
||
Atwood.

When a spheroid is composed of concentric elliptical shells of variable density and figure, we may consider every shell as the difference of two homogeneous spheroids of the same density with the shells, and having their surfaces coinciding with the surfaces of the shell. The attractions of the spheroids being computed by the preceding methods, their difference will be equal to the attractions of the shell; and the integral obtained by summing the attractions of all the shells, will give the attractions of the heterogeneous spheroid. This case, therefore, gives rise to no new difficulties, except what are purely mathematical, and depend upon the law, according to which, the densities and figures of the shells are supposed to vary. (cc.)

ATTRACTION OF MOUNTAINS. See MOUNTAINS, ATTRACTION OF, in the Encyclopædia, and in this Supplement.

ATWOOD (GEORGE), an Author celebrated for the accuracy of his mathematical and mechanical investigations, and considered as particularly happy in the clearness of his explanations, and the elegance of his experimental illustrations, was born in the early part of the year 1746. He was educated at Westminster school, where he was admitted in 1759. Six years afterwards he was elected off to Trinity College, Cambridge. He took his degree of Bachelor of Arts in 1769, with the rank of third wrangler, Dr Parkinson, of Christ's College, being senior of the year. This distinction was amply sufficient to give him a claim to further advancement in his own College, on the list of which he stood foremost of his contemporaries; and, in due time, he obtained a fellowship, and was afterwards one of the tutors of the College. He became Master of Arts in 1772; and, in 1776, was elected a Fellow of the Royal Society of London.

The higher branches of the Mathematics had, at this period, been making some important advances at Cambridge, under the auspices of Dr Waring, and many of the younger members of the University became diligent labourers in this extensive field. Mr Atwood chose, for his peculiar department, the illustration of mechanical and experimental philosophy, by elementary investigations and ocular demonstrations of their fundamental truths. He delivered, for several successive years, a course of lectures in the Observatory of Trinity College, which were very generally attended, and greatly admired. In the year 1784, some circumstances occurred which made it desirable for him to discontinue his residence at Cambridge; and soon afterwards Mr Pitt, who had become acquainted with his merits by attending his lectures, bestowed on him a patent office, which required but little of his attendance, in order to have

a claim on the employment of his mathematical abilities in a variety of financial calculations, to which he continued to devote a considerable portion of his time and attention throughout the remainder of his life.*

The following, we believe, is a correct list of Mr Atwood's publications:

  1. 1. A Description of Experiments to illustrate a Course of Lectures. 8vo. About 1775, or 1776.
  2. 2. This work was reprinted with additions, under the title of An Analysis of a Course of Lectures on the Principles of Natural Philosophy. 8vo. Cambr. 1784.
  3. 3. A General Theory for the Mensuration of the Angle subtended by two objects, of which one is observed by Rays after two Reflections from plane Surfaces, and the other by Rays coming directly to the Spectator's Eye. Phil. Trans. 1781, p. 395.
  4. 4. A Treatise on the Rectilinear Motion and Rotation of Bodies, with a Description of Original Experiments relative to the Subject. 8vo. Cambr. 1784.
  5. 5. Investigations founded on the Theory of Motion, for determining the Times of Vibration of Watch Balances. Phil. Trans. 1794, p. 119.
  6. 6. The Construction and Analysis of Geometrical Propositions, determining the positions assumed by homogeneous bodies, which float freely, and at rest, on a fluid's surface; also Determining the Stability of Ships, and of other Floating Bodies. Phil. Trans. 1796, p. 46.
  7. 7. A Disquisition on the Stability of Ships. Phil. Trans. 1798, p. 201.
  8. 8. A Review of the Statutes and Ordinances of Assize, which have been established in England from the 4th year of King John, 1202, to the 37th of his present Majesty. 4to. Lond. 1801.
  9. 9. A Dissertation on the Construction and Properties of Arches. 4to. Lond. 1801.
  10. 10. A Supplement to a Tract entitled a Treatise on the Construction and Properties of Arches, published

* See Literary Memoirs of Living Authors, 2 vol. 8vo, Lond. 1798; Morning Herald, 17th July 1807; Nichols's Literary Anecdotes of the Eighteenth Century, Vol. VIII. 8vo, Lond. 1814.

Fig. 1.
Geometric diagram Fig. 1 showing a circular segment with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z.

A geometric diagram showing a circular segment with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The segment is bounded by points A and B, with points C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z distributed along the arc and the chord.

Fig. 2.
Geometric diagram Fig. 2 showing two concentric circles with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z.

A geometric diagram showing two concentric circles with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The points are distributed along the circumference of both circles and the radii connecting their centers.

Geometric diagram Fig. 3 showing a perspective view of a rectangular prism with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z.

A perspective view of a rectangular prism with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The prism is shown in perspective, with lines connecting the vertices to a vanishing point.

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Geometric diagram Fig. 5 showing a perspective view of a rectangular prism with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z.

A perspective view of a rectangular prism with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The prism is shown in perspective, with lines connecting the vertices to a vanishing point.

Fig. 3.
Geometric diagram Fig. 4 showing two concentric circles with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z.

A geometric diagram showing two concentric circles with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The points are distributed along the circumference of both circles and the radii connecting their centers.

Fig. 5.
Geometric diagram Fig. 6 showing two concentric circles with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z.

A geometric diagram showing two concentric circles with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The points are distributed along the circumference of both circles and the radii connecting their centers.

Fig. 6.
Geometric diagram Fig. 7 showing a perspective view of a rectangular prism with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z.

A perspective view of a rectangular prism with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The prism is shown in perspective, with lines connecting the vertices to a vanishing point.

Fig. 7.
Geometric diagram Fig. 8 showing a circle with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z.

A geometric diagram showing a circle with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The points are distributed along the circumference of the circle and the radii connecting their centers.

Fig. 7.
Geometric diagram Fig. 9 showing a circle with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z.

A geometric diagram showing a circle with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The points are distributed along the circumference of the circle and the radii connecting their centers.

Fig. 8.
Geometric diagram Fig. 10 showing two concentric circles with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z.

A geometric diagram showing two concentric circles with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The points are distributed along the circumference of both circles and the radii connecting their centers.

Fig. 9.
Geometric diagram Fig. 10 showing a circle with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z.

A geometric diagram showing a circle with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The points are distributed along the circumference of the circle and the radii connecting their centers.

Fig. 10.
Geometric diagram Fig. 11 showing a circle with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z.

A geometric diagram showing a circle with points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The points are distributed along the circumference of the circle and the radii connecting their centers.

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Fig. 11.
Geometric diagram Fig. 11 showing two concentric ellipses. The outer ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The inner ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. Lines connect various points on the outer ellipse to the center C and to points on the inner ellipse.
Fig. 12.
Geometric diagram Fig. 12 showing two concentric ellipses. The outer ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The inner ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. Lines connect various points on the outer ellipse to the center C and to points on the inner ellipse.
Fig. 14.
Geometric diagram Fig. 14 showing a perspective view of a cone with a rectangular base. The base has vertices A, B, C, D. The cone's apex is at the top. Points P, Q, R, S are marked on the cone's surface.
Fig. 15.
Geometric diagram Fig. 15 showing two concentric ellipses. The outer ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The inner ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. Lines connect various points on the outer ellipse to the center C and to points on the inner ellipse.
Fig. 15.
Geometric diagram Fig. 15 showing two concentric ellipses. The outer ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The inner ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. Lines connect various points on the outer ellipse to the center C and to points on the inner ellipse.
Fig. 17.
Geometric diagram Fig. 17 showing two concentric ellipses. The outer ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The inner ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. Lines connect various points on the outer ellipse to the center C and to points on the inner ellipse.
Fig. 16.
Geometric diagram Fig. 16 showing two concentric ellipses. The outer ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The inner ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. Lines connect various points on the outer ellipse to the center C and to points on the inner ellipse.
Fig. 19.
Geometric diagram Fig. 19 showing two concentric ellipses. The outer ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The inner ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. Lines connect various points on the outer ellipse to the center C and to points on the inner ellipse.
Fig. 18.
Geometric diagram Fig. 18 showing two concentric ellipses. The outer ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The inner ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. Lines connect various points on the outer ellipse to the center C and to points on the inner ellipse.
Fig. 17.
Geometric diagram Fig. 17 showing two concentric ellipses. The outer ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The inner ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. Lines connect various points on the outer ellipse to the center C and to points on the inner ellipse.
Fig. 20.
Geometric diagram Fig. 20 showing two concentric ellipses. The outer ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. The inner ellipse has points A, B, C, D, E, F, G, H, I, K, L, M, N, O, P, Q, R, S, T, U, V, W, X, Y, Z. Lines connect various points on the outer ellipse to the center C and to points on the inner ellipse.
A blank, aged, cream-colored page with faint, repeating circular patterns and some minor stains.This image shows a blank, aged, cream-colored page, likely an endpaper or flyleaf from an old book. The paper has a slightly textured appearance with some minor discoloration and faint, repeating circular patterns that suggest a watermark or a decorative design. There are also some small, dark spots or stains scattered across the surface. The right edge of the page shows a slight shadow, indicating it is part of a bound volume.