KEPLER'S THIRD LAW ONLY APPROXIMATELY TRUE.

But it may be asked: If there be a modifying force in astronomy derived

from another source than that of gravitation, why is it that the

elements of the various members of the system derived solely from

gravitation should be so perfect? To this it may be answered, that

although astronomers have endeavored to derive every movement in the

heavens from that great principle, they have but partially succeeded.

Let us not surrender our right of examining Nature to the authority of a

great name, nor call any man master, either in moral or physical

science. It is well known that Kepler's law of the planetary distances

and periods, is a direct consequence of the Newtonian Law of

gravitation, and that the squares of the periodic times ought to be

proportional to the cubes of the mean distances. These times are given

accurately by the planets themselves, by the interval elapsing between

two consecutive passages of the node, and as in the case of the ancient

planets we have observations for more than two thousand years past,

these times are known to the fraction of the second. The determination

of the distances however, depends on the astronomer, and a tyro in the

science might suppose that these distances were actually measured; and

so they are roughly; but the astronomer does not depend on his

instruments, he trusts to _analogy_, and the mathematical perfection of

a law, which in the abstract is true; but which he does not know is

rigidly exact when applied to physical phenomena. From the immense

distance of the planets and the smallness of the earth, man is unable to

command a base line sufficiently long, to make the horizontal parallax a

sensible angle for the more distant planets; and there are difficulties

of no small magnitude to contend with, with those that are the nearest.

In the occasional transit of Venus across the sun, however, he is

presented with a means of measuring on an enlarged scale, from which the

distance of the sun is determined; and by _analogy_ the distance of all

the planets. Even the parallax of the sun itself is only correct, by

supposing that the square of the periodic time of Venus is in the same

proportion to the square of the periodic time of the earth as the cube

of her distance is to the cube of the earth's distance. Our next nearest

planet is Mars, and observations on this planet at its opposition to the

sun, invariably give a larger parallax for the sun--Venus giving 8.5776"

while Mars gives about 10". It is true that the first is obtained under

more favorable circumstances; but this does not prove the last to be

incorrect. It is well known that the British Nautical Almanac contains a

list of stars lying in the path of the planet Mars about opposition,

(for the very purpose of obtaining a correct parallax,) that minute

differences of declination may be detected by simultaneous observations

in places having great differences of latitude. Yet strange to say, the

result is discredited when not conformable to the parallax given by

Venus. If then, we cannot trust the parallax of Mars, _a fortiori_, how

can we trust the parallax of Jupiter, and say that his mean distance

exactly corresponds to his periodic time? Let us suppose, for instance,

that the radius vector of Jupiter fell short of that indicated by

analogy by 10,000 miles, we say that it would be extremely difficult,

nay, utterly impossible, to detect it by instrumental means. Let not

astronomers, therefore, be too sure that there is not a modifying cause,

independent of gravitation, which they will yet have to recognize. The

moon's distance is about one-fourth of a million of miles, and Neptune's

2854 millions, or in the ratio of 10,000 to 1; yet even the moon's

parallax is not trusted in determining her mass, how then shall we

determine the parallax of Neptune? It is therefore _possible_ that the

effective action of the sun is in some small degree different, on the

different planets, whether due to the action of the ether, to the

similarity or dissimilarity of material elements, to the temperature of

the different bodies, or to all combined, is a question yet to be

considered.

As another evidence of the necessity of modifying the strict wording of

the Newtonian law, it is found that the disturbing action of Jupiter on

different bodies, gives different values for the mass of Jupiter. The

mass deduced from Jupiter's action on his satellites, is different from

that derived from the perturbations of Saturn, and this last does not

correspond with that given by Juno: Vesta also gives a different mass

from the comet of Encke, and both vary from the preceding values.[41]

In the analytical investigation of planetary disturbances, the

disturbing force is usually divided into a radial and tangential force;

the first changing the law of gravitation, to which law the elliptic

form of the orbit is due. The radial disturbing force, therefore, being

directed to or from the centre, can have no influence over the first law

of Kepler, which teaches that the radius vector of each planet having

the sun as the centre, describes equal areas in equal times. If the

radial disturbing force be exterior to the disturbed body, it will

diminish the central force, and cause a progressive motion in the

aphelion point of the orbit. In the case of the moon this motion is very

rapid, the apogee making an entire revolution in 3232 days. Does this,

however, correspond with the law of gravitation? Sir Isaac Newton, in

calculating the effect of the sun's disturbing force on the motion of

the moon's apogee, candidly concludes thus: "Idoque apsis summa singulis

revolutionibus progrediendo conficit 1d 31' 28". Apsis lunae est duplo

velocior circiter." As there was a necessity for reconciling this

stubborn fact with the theory, his followers have made up the deficiency

by resorting to the tangential force, or, as Clairant proposed, by

continuing the approximations to terms of a higher order, or to the

square of the disturbing force.

Now, in a circular orbit, this tangential force will alternately

increase and diminish the velocity of the disturbed body, without

producing any permanent derangement, the same result would obtain in an

elliptical orbit, if the position of the major axis were stationary. In

the case of the moon, the apogee is caused to advance by the disturbing

power of the radial force, and, consequently, an exact compensation is

not effected: there remains a small excess of velocity which geometers

have considered equivalent to a doubling of the radial force, and have

thus obviated the difficulty. To those not imbued with the profound

penetration of the modern analyst, there must ever appear a little

inconsistency in this result. The major axis of a planet's orbit depends

solely on the velocity of the planet at a given distance from the sun,

and the tangential portion of the disturbance due to the sun, and

impressed upon the moon, must necessarily increase and diminish

alternately the velocity of the moon, and interfere with the equable

description of the areas. If, then, there be left outstanding a small

excess of velocity over and above the elliptical velocity of the moon,

at the end of each synodical revolution, in consequence of the motion

impressed on the moon's apogee by the radial force, the _legitimate_

effect would be a small enlargement of the lunar orbit every revolution

in a rapidly-increasing ratio, until the moon would at last be taken

entirely away. In the great inequality of Jupiter and Saturn, this

tangential force is not compensated at each revolution, in consequence

of continual changes in the configuration of the two planets at their

heliocentric conjunctions, with respect to the perihelion of their

orbits, and the near commensurability of their periods; and the effect

of the tangential force is, in this case, legitimately impressed on the

major axes of the orbits. But why (we may ask) should not this also be

expended on the motion of the aphelion as well as in the case of the

moon? Astronomy can make no distinctions between the orbit of a planet

and the orbit of a satellite. And, we might also ask, why the tangential

resistance to the comet of Encke should not also produce a retrograde

motion in the apsides of the orbit, instead of diminishing its period?

To the honor of Newton, be it remembered, that he never resorted to an

explanation of this phenomenon, which would vitiate that fundamental

proposition of his theory, in which the major axis of the orbit is shown

to depend on the velocity at any given distance from the focus.

Some cause, however, exists to double the motion of the apogee, and

that there is an outstanding excess of orbital velocity due to the

tangential force, is also true. This excess may tell in the way

proposed, provided some other arrangement exists to _prevent_ a

permanent dilation of the lunar orbit; and this provision may be found

in the increasing density of the ether, which prevents the moon

overstepping the bounds prescribed by her own density, and the force of

the radial stream of the terral vortex. In the case of Jupiter and

Saturn, their mutual action is much less interfered with by change of

density in the ether in the enlarged or contracted orbit, and,

consequently, the effect is natural. Thus, we have in the law of density

of the ethereal medium a better safeguard to the stability of the

dynamical balance of the system, than in the profound and beautiful

Theorems of La Grange. It will, of course, occur to every one, that we

are not to look for the same law in every vortex, and it will,

therefore, appear as if the satellites of Jupiter, whose theory is so

well known, should render apparent any deviation between their periodic

times and the periodic times of the contiguous parts of the vortex,

which would obtain, if the density of the ether in the Jovian vortex

were not as the square roots of the distances directly. But, we have

shown how there can be a balance preserved, if the tangential resistance

of the vortex shall be equal and contrary at the different distances at

which the satellites are placed; that is, if these two forces shall

follow the same law. These are matters, however, for future

investigation.

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