CHAPTER TEN

Pseudo heart of a phantom thing—it is Keplerism, pulsating with Sir

Isaac Newton’s regularizations.

If triangulation can not be depended upon accurately to measure distance

greater than a mile or two between objects and observers, the aspects of

Keplerism that depend upon triangulation should be of no more concern to

us than two pins in a cushion 180 miles away: nevertheless so affected

by something like seasickness are we by the wobbling deductions of the

conventionalists that we shall have direct treatment, or independent

expressions, whenever we can have, or seem to have, them. Kepler saw a

planetary system, and he felt that, if that system could be formulated

in terms of proportionality, by discovering one of the relations

quantitatively, all its measurements could be deduced. I take from

Newcomb, in _Popular Astronomy_, that, in Kepler’s view, there was

system in the arrangement and motions of the four little traitors that

sneak around Jupiter; that Kepler, with no suspicions of these little

betrayers, reasoned that this central body and its accompaniments were a

representation, upon a small scale, of the solar system, as a whole.

Kepler found that the cubes of mean distances of neighboring satellites

of Jupiter, divided by the squares of their times, gave the same

quotients. He reasoned that the same relations subsisted among planets,

if the solar system be only an enlargement of the Jovian system.

_Observatory_, December, 1920: “The discordances between theory and

observation (as to the motions of Jupiter’s satellites) are of such

magnitude that continued observations of their precise moments of

eclipses are very much to be desired.” In the Report of the Jupiter

Section of the British Astronomical Society (_Mems. B. A. A._, 8-83) is

a comparison between observed times and calculated times of these

satellites. 65 observations, in the year 1899, are listed. In one

instance prediction and observation agree. Many differences of 3 or 4

minutes are noted, and there are differences of 5 or 6 minutes.

Kepler formulated his law of proportionality between times and distances

of Jupiter’s satellites without knowing what the times are. It should be

noted that the observations in the year 1899 took into consideration

fluctuations that were discovered by Roemer, long after Kepler’s time.

Just for the sake of having something that looks like opposition, let us

try to think that Kepler was miraculously right anyway. Then, if

something that may resemble Kepler’s Third Law does subsist in the

Jovian satellites that were known to Kepler, by what resemblance to

logicality can that proportionality extend to the whole solar system, if

a solar system can be supposed?

In the year 1892, a fifth satellite of Jupiter was discovered. Maybe it

would conform to Kepler’s law, if anybody could find out accurately in

what time the faint speck does revolve. The sixth and the seventh

satellites of Jupiter revolve so eccentrically that, in line of sight,

their orbits intersect. Their distances are subject to very great

variations; but, inasmuch as it might be said that their mean distances

do conform to Kepler’s Third Law, or would, if anybody could find out

what their mean distances are, we go on to the others. The eight and the

ninth conform to nothing that can be asserted. If one of them goes

around in one orbit at one time, the next time around it goes in some

other orbit, and in some other plane. Inasmuch then as Kepler’s Third

Law, deduced from the system of Jupiter’s satellites, can not be thought

to extend even within that minor system, one’s thoughts stray into

wondering what two pins in a cushion in Louisville, Ky., look like from

somewhere up in the Bronx, rather than to dwell any more upon extension

of any such pseudo-proportionality to the supposed solar system, as a

whole.

It seems that in many of Kepler’s demonstrations was this failure to

have grounds for a starting-point, before extending his reasoning. He

taught the doctrine of the music of the spheres, and assigned bass

voices to Saturn and Jupiter, then tenor to Mars, contralto to the

female planet, and soprano, or falsetto, rather, to little Mercury. And

that is all very well and consistently worked out in detail, and it does

seem reasonable that, if ponderous, if not lumpy, Jupiter, does sing

bass, the other planets join in, according to sex and huskiness—however,

one does feel dissatisfied.

We have dealt with Newcomb’s account. But other conventionalists say

that Kepler worked out his Third Law by triangulation upon Venus and

Mercury, when at greatest elongation, “finding” that the relation

between Mercury and Venus is the same as the relation between Venus and

this earth. If, according to conventionalists, there was no “proof” that

this earth moves, in Kepler’s time, Kepler started by assuming that this

earth moves between Venus and Mars; he assumed that the distance of

Venus from the sun, at greatest elongation, represents mean distance; he

assumed that observations upon Mercury indicated Mercury’s orbit, an

orbit that to this day defies analysis. However, for the sake of seeming

to have opposition, we shall try to think that Kepler’s data did give

him material for the formulation of his law. His data were chiefly the

observations of Tycho Brahé. But, by the very same data, Tycho had

demonstrated that this earth does not move between Venus and Mars; that

this earth is stationary. That stoutest of conventionalists, but at the

same time seeming colleague of ours, Richard Proctor, says that Tycho

Brahé’s system was consistent with all data. I have never heard of an

astronomer who denies this. Then the heart of modern astronomy is not

Keplerism, but is one diversion of data that beat for such a monstrosity

as something like Siamese Twins, serving both Keplerism and the Tychonic

system. I fear that some of our attempts to find opposition are not very

successful.

So far, this mediæval doctrine, restricting to times and distances,

though for all I know the planets sing proportionately as well as move

proportionately, has data to interpret or to misinterpret. But, when it

comes to extending Kepler’s Third Law to the exterior planets, I have

never read of any means that Kepler had of determining their

proportional distances. He simply said that Mars and Jupiter and Saturn

were at distances that proportionalized with their times. He argued,

reasonably enough, perhaps, that the slower-moving planets are the

remoter, but that has nothing to do with proportional remoteness.

This is the pseudo heart of phantom astronomy.

To it Sir Isaac Newton gave a seeming of coherence.

I suspect that it was not by chance that the story of an apple should so

importantly appear in two mythologies. The story of Newton and the apple

was first told by Voltaire. One has suspicions of Voltaire’s meanings.

Suppose Newton did see an apple fall to the ground, and was so inspired,

or victimized, into conceiving in terms of universal attraction. But had

he tried to take a bone away from a dog, he would have had another

impression, and would have been quite as well justified in explaining in

terms of universal repulsion. If, as to all inter-acting things,

electric, biologic, psychologic, economic, sociologic, magnetic, chemic,

as well as canine, repulsion is as much of a determinant as is

attraction, the Law of Gravitation, which is an attempt to explain in

terms of attraction only, is as false as would be dogmas upon all other

subjects if couched in terms of attraction only. So it is that the law

of gravitation has been a rule of chagrin and fiasco. So, perhaps

accepting, or passionately believing in every symbol of it, a Dr. Adams

calculates that the Leonids will appear in November, 1899—but chagrin

and fiasco—the Leonids do not appear. The planet Neptune was not

discovered mathematically, because, though it was in the year 1846,

somewhere near the position of the formula, in the year 1836 or 1856, it

would have been nowhere near the orbit calculated by Leverrier and

Adams. Some time ago, against the clamor that a Trans-Uranian planet had

been discovered mathematically, it was our suggestion that, if this be

not a myth, let the astronomer now discover the Trans-Neptunian planet

mathematically. That there is no such mathematics, in the face of any

number of learned treatises, is far more strikingly betrayed by those

shining little misfortunes, the satellites of Jupiter. Satellite after

satellite of Jupiter was discovered, but by accident or by observation,

and not once by calculation: never were the perturbations of the earlier

known satellites made the material for deducing the positions of other

satellites. Astronomers have pointed to the sky, and there has been

nothing; one of them pointed in four directions at once, and four times

over, there was nothing; and many times when they have not pointed at

all, there has been something.

Apples fall to the ground, and dogs growl, if their bones are taken

away: also flowers bloom in the spring, and a trodden worm turns.

Nevertheless strong is the delusion that there is gravitational

astronomy, and the great power of the Law of Gravitation, in popular

respectfulness, is that it is mathematically expressed. According to my

view, one might as well say that it is fetishly expressed. Descartes was

as great a mathematician as Newton: veritably enough may it be said that

he invented, or discovered, analytic geometry; only patriotically do

Englishmen say that Newton invented, or discovered, the infinitesimal

calculus. Descartes, too, formulated a law of the planets and not by a

symbol was he less bewildering and convincing to the faithful, but his

law was not in terms of gravitation, but in terms of vorticose motion.

In the year 1732, the French Academy awarded a prize to John Bernouli,

for his magnificent mathematical demonstration, which was as

unintelligible as anybody’s. Bernouli, too, formulated, or said he

formulated, planetary inter-actions, as mathematically as any of his

hypnotized admirers could have desired: it, too, was not gravitational.

The fault that I find with a great deal of mathematics in astronomy is

the fault that I should find in architecture, if a temple, or a

skyscraper, were supposed to prove something. Pure mathematics is

architecture: it has no more place in astronomy than has the Parthenon.

It is the arbitrary: it will not spoil a line nor dent a surface for a

datum. There is a faint uniformity in every chaos: in discolorations on

an old wall, anybody can see recognizable appearances; in such a mixture

a mathematician will see squares and circles and triangles. If he would

merely elaborate triangles and not apply his diagrams to theories upon

the old wall itself, his constructions would be as harmless as poetry.

In our metaphysics, unity can not, of course, be the related. A

mathematical expression of unity can not, except approximately, apply to

a planet, which is not final, but is part of something.

Sir Isaac Newton lived long ago. Every thought in his mind was a

reflection of his era. To appraise his mind at all comprehensively,

consider his works in general. For some other instances of his love of

numbers, see, in his book upon the Prophecies of Daniel, his

determinations upon the eleventh horn of Daniel’s fourth animal. If that

demonstration be not very acceptable nowadays, some of his other works

may now be archaic. For all I know Jupiter may sing bass, either

smoothly or lumpily, and for all I know there may be some formulable

ratio between an eleventh horn of a fourth animal and some other

quantity: I complain against the dogmas that have solidified out of the

vaporings of such minds, but I suppose I am not very substantial,

myself. Upon general principles, I say that we take no ships of the time

of Newton for models for the ships of today, and build and transport in

ways that are magnificently, or perhaps disastrously, different, but

that, at any rate, are not the same; and that the principles of biology

and chemistry and all the other sciences, except astronomy, are not what

they were in Newton’s time, whether every one of them is a delusion or

not. My complaint is that the still mediæval science of astronomy holds

back alone in a general appearance of advancement, even though there

probably never has been real advancement.

There is something else to be said upon Keplerism and Newtonism. It is a

squirm. I fear me that our experiences have sophisticated us. We have

noted the division in Keplerism, by which, like everything else that we

have examined, it is as truly interpretable one way as it is another

way.

The squirm:

To lose all sense of decency and value of data, but to be agreeable; but

to be like everybody else, and intend to turn our agreeableness to

profit;

To agree with the astronomers that Kepler’s three laws are, not

absolutely true, of course, but are approximations, and that the planets

do move, as in Keplerian doctrine they are said to move—but then to

require only one demonstration that this earth is one of the planets;

To admire Newton’s _Principia_ from the beginning to the end of it,

having, like almost all other admirers, never even seen a copy of it; to

accept every theorem in it, without having the slightest notion what any

one of them means; to accept that moving bodies do obey the laws of

motion, and must move in one of the conic sections—but then to require

only one demonstration that this earth is a moving body.

Kepler’s three laws are popularly supposed to demonstrate that this

earth moves around the sun. This is a mistake. There is something wrong

with everything that is popular. As was said, by us, before, accept that

this earth is stationary, and Kepler’s doctrines apply equally well to a

sun around which proportionately inter-spaced planets move in ellipses,

the whole system moving around a central and stationary earth. All

observations upon the motions of heavenly bodies are in accord with this

interpretation of Kepler’s laws. Then as to nothing but a quandary,

which means that this earth is stationary, or which means that this

earth is not stationary, just as one pleases, Sir Isaac Newton selected,

or pleased himself and others. Without one datum, without one little

indication more convincing one way than the other, he preferred to think

that this earth is one of the moving planets. To this degree had he the

“profundity” that we read about. He wrote no books upon the first and

second horns of his dilemma: he simply disregarded the dilemma.

To anybody who may be controversially inclined, I offer simplification.

He may feel at a disadvantage against batteries of integrals and

bombardments of quaternions, transcendental functions, conics, and all

the other stores of an astronomer’s munitions—

Admire them. Accept that they do apply to the bodies that move around

the sun. Require one demonstration that this earth is one of those

bodies. For treatment of any such “demonstration,” see our disquisition,

or our ratiociations upon the Three Abstrusities, or our intolerably

painful attempts to write seriously upon the Three Abstrusities.

We began with three screams from an exhilarated mathematician. We have

had some doubtful adventures, trying hard to pretend that monsters, or

little difficulties, did really oppose us. We have reached, not the

heart of a system, but the crotch of quandary.

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