New Lands (8 page)
Authors: Charles Fort
That the word “worthless” does apply to observations upon transits of Venus:
In
Old and New Astronomy,
Proctor says that the observations upon the transits of 1761 and 1769 were “altogether unsatisfactory.” One supposes that anything that is altogether unsatisfactory can’t be worth much. In the next transit, of 1874, various nations cooperated. The observations were so disappointing that the Russian, Italian, and Austrian governments refused to participate in the expeditions of 1882. In
Reminiscences of an Astronomer,
p. 181, Newcomb says that the United States Commission, of which he was secretary, had up to 1902 never published in full its observations, and probably never would, because by that time all other members were either dead or upon the retired list.
Method of Mars—more monotony—because of criticisms of the taking of parallax by simultaneous observations, Dr. David Gill went to the Island of Ascension, during the opposition of Mars of 1877, to determine alone, by the diurnal method, the distance of this earth from the sun, from positions of Mars. For particulars of Gill’s method, see, for instance, Poor’s
Solar System,
p. 86. Here Prof. Poor says that, of course, the orbital motion of Mars had to be allowed for, in Gill’s calculations. If so, then of course this earth’s orbital motion had to be allowed for. If Dr. Gill knew the space traversed by this earth in its orbit, and the curvature of its path, he knew the size and shape of the orbit, and consequently the distance from the sun. Then he took for the basis of his allowance that this earth is about 93,000,000 miles from the sun, and calculated that this earth is about 93,000,000 miles from the sun. For this classic deduction from the known to the same known, he received a gold medal.
In our earlier surveys, we were concerned with the false claim that there can be application of celestial mechanics to celestial phenomena; but, as to later subjects, the method is different. The method of all these calculations is triangulation.
One simple question:
To what degree can triangulation be relied upon?
To great degree in measuring the height of a building, or in the little distances of a surveyor’s problems. It is clear enough that astronomers did not invent the telescope. They adopted the spectroscope from another science. Their primary mathematical principle of triangulation they have taken from the surveyors, to whom it is serviceable. The triangle is another emblem of the sterility of the science of astronomy. Upon the coat of arms of this great mule of the sciences, I would draw a prism within a triangle.
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According to Prof. Newcomb, for instance, the distance of the sun is about 380 times the distance of the moon—as determined by triangulation. But, upon page 22,
Popular Astronomy,
Newcomb tells of another demonstration, with strikingly different results—as determined by triangulation.
A split god.
The god Triangulation is not one undivided deity.
The other method with strikingly different results is the method of Aristarchus. It cuts down the distance of the sun, from 380 to twenty times the distance of the moon. When an observer upon this earth sees the moon half-illumined, the angle at the moon, between observer and sun, is a right angle; a third line between observer and sun completes a triangle. According to Aristarchus, the tilt of the third line includes an angle of eighty-six degrees, making the sun-earth line twenty times longer than the moon-earth line.
“In principle,” says Newcomb, “the method is quite correct and very ingenious, but it cannot be applied in practice.” He says that Aristarchus measured wrong; that the angle between the moon-earth line and the earth-sun line is almost ninety degrees and not eighty-six degrees. Then he says that the method cannot be applied because no one can determine this angle that he had said is of almost ninety degrees. He says something that is so incongruous with the inflations of astronomers that they’d sizzle if their hypnotized readers could read and think at the same time. Newcomb says that the method of Aristarchus cannot be applied because no astronomer can determine when the moon is half-illumined.
We have had some experience.
Does anybody who has been through what we’ve been through suppose that there is a Prof. Keeler in the world who would not declare that trigonometrically and spectroscopically and micrometrically he had determined the exact moment and exasperating, or delightful, decimal of a moment of semi-illumination of the moon, were it not that, according to at least as good a mathematician as he, determination based upon that demonstration does show that the sun is only twenty times as far away as the moon? But suppose we agree that this simple thing cannot be done.
Then instantly we think of some of the extravagant claims with which astronomers have stuffed supine credulities. Crawling in their unsightly confusion that sickens for simplification, is this offense to harmony:
That astronomers can tell under which Crusade, or its decimalated moment, a shine left a star, but cannot tell when a shine reaches a line on the moon—
Glory and triumph and selectness and inflation—or that we shall have renown as evangelists, spreading the homely and wholesome doctrine of humility. Hollis, in
Chats on Astronomy,
tells us that the diameter of this earth, at the equator, is 41,851,160 feet. But blessed be the meek, we tell him. In the
Observatory,
19-118, is published the determination, by the astronomer Brenner, of the time of rotation of Venus, as to which other astronomers differ by hundreds of days. According to Brenner, the time is 23 hours, 57 minutes, 7.5459 seconds. I do note that this especial refinement is a little too ethereal for the Editor of the
Observatory:
he hopes Brenner will pardon him, but is it necessary to carry out the finding to the fourth decimal of a second? However, I do not mean to say that all astronomers are as refined as Brenner, for instance. In the
Jour. B.A.A.,
1-382, Edwin Holmes, perhaps coarsely, expresses some views. He says that such “exactness” as Capt. Noble’s in writing that the diameter of Neptune is 38,133 miles and that of Uranus is 33,836 miles is bringing science into contempt, because very little is known of these planets; that, according to Neison, these diameters are 27,000 miles and 28,500 miles. Macpherson, in
A Century’s Progress in Science,
quotes Prof. Serviss: that the average parallax of a star, which is an ordinary astronomic quantity, is “about equal to the apparent distance between two pins, placed one inch apart, and viewed from a distance of one hundred and eighty miles.” Stick pins in a cushion, in New York—go to Saratoga and look at them be overwhelmed with the more than human powers of the scientifically anointed—or ask them when shines half the moon.
The moon’s surface is irregular. I do not say that anybody with brains enough to know when he has half a shoe polished should know when the sun has half the moon shined. I do say that if this simple thing cannot be known, the crowings of astronomers as to enormously more difficult determinations are mere barnyard disturbances.
Triangulation that, according to his little priests, straddles orbits and on his apex wears a star—that he’s a false Colossus; shrinking, at the touch of data, back from the stars, deflating below the sun and moon; stubbing down below the clouds of this earth, so that the different stories that he told to Aristarchus and to Newcomb are the conflicting vainglories of an earth-tied squatter—
The blow that crumples a god:
That, by triangulation, there is not an astronomer in the world who can tell the distance of a thing only five miles away.
Humboldt,
Cosmos,
5-138:
Height of Mauna Loa: 18,410 feet, according to Cook; 16,611, according to Marchand; 13,761, according to Wilkes—according to triangulation.
In the
Scientific American,
119-31, a mountain climber calls the Editor to account for having written that Mt. Everest is 29,002 feet high. He says that, in his experience, there is always an error of at least ten percent, in calculating the height of a mountain, so that all that can be said is that Mt. Everest is between 26,100 and 31,900 feet high. In the
Scientific American,
102-183, and 319, Miss Annie Peck cites two measurements of a mountain in India: they differ by 4,000 feet.
The most effective way of treating this subject is to find a list of measurements of a mountain’s height before the mountain was climbed, and compare with the barometric determination, when the mountain was climbed. For a list of eight measurements, by triangulation, of the height of Mt. St. Elias, see the
Alpine Journal,
22-150: they vary from 12,672 to 19,500 feet. D’Abruzzi climbed Mt. St. Elias, Aug. 1, 1897. See a paper, in the
Alpine Journal,
19-125. D’Abruzzi barometric determination—18,092 feet.
Suppose that, in measuring, by triangulation, the distance of anything five miles away, the error is, say, ten percent. But, as to anything ten miles away, there is no knowing what the error would be. By triangulation, the moon has been “found” to be 240,000 miles away. It may be 240 or 240,000,000 miles away.
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Pseudo heart of a phantom thing—it is Keplerism, pulsating with Sir Isaac Newton’s regularizations. If triangulation cannot 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
(Mens. B.A.A.,
8-83) is a comparison between observed times and calculated times of these satellites. Sixty-five observations, in the year 1899, are listed. In one instance prediction and observation agree. Many differences of three or four minutes are noted, and there are differences of five or six 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 eighth 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, cannot 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 Brand’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 mediaeval 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 interacting 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, 1893—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 interactions, 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 cannot, of course, be the related. A mathematical expression of unity cannot, 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 mediaeval 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 interspaced 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 pleasts, 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, conies, and all the other stores of an astronomer’s munitions—