The Foundations of Science: Science and Hypothesis, The Value of Science, Science and Method
CHAPTER II
FRENCH GEODESY
Every one understands our interest in knowing the form and dimensions of our earth; but some persons will perhaps be surprised at the exactitude sought after. Is this a useless luxury? What good are the efforts so expended by the geodesist?
Should this question be put to a congressman, I suppose he would say: "I am led to believe that geodesy is one of the most useful of the sciences; because it is one of those costing us most dear." I shall try to give you an answer a little more precise.
The great works of art, those of peace as well as those of war, are not to be undertaken without long studies which save much groping, miscalculation and useless expense. These studies can only be based upon a good map. But a map will be only a valueless phantasy if constructed without basing it upon a solid framework. As well make stand a human body minus the skeleton.
Now, this framework is given us by geodesic measurements; so, without geodesy, no good map; without a good map, no great public works.
These reasons will doubtless suffice to justify much expense; but these are arguments for practical men. It is not upon these that it is proper to insist here; there are others higher and, everything considered, more important.
So we shall put the question otherwise; can geodesy aid us the better to know nature? Does it make us understand its unity and harmony? In reality an isolated fact is of slight value, and the conquests of science are precious only if they prepare for new conquests.
If therefore a little hump were discovered on the terrestrial ellipsoid, this discovery would be by itself of no great interest. On the other hand, it would become precious if, in seeking the cause of this hump, we hoped to penetrate new secrets.
Well, when, in the eighteenth century, Maupertuis and La Condamine braved such opposite climates, it was not solely to learn the shape of our planet, it was a question of the whole world-system.
If the earth was flattened, Newton triumphed and with him the doctrine of gravitation and the whole modern celestial mechanics.
And to-day, a century and a half after the victory of the Newtonians, think you geodesy has nothing more to teach us?
We know not what is within our globe. The shafts of mines and borings have let us know a layer of 1 or 2 kilometers thickness, that is to say, the millionth part of the total mass; but what is beneath?
Of all the extraordinary journeys dreamed by Jules Verne, perhaps that to the center of the earth took us to regions least explored.
But these deep-lying rocks we can not reach, exercise from afar their attraction which operates upon the pendulum and deforms the terrestrial spheroid. Geodesy can therefore weigh them from afar, so to speak, and tell us of their distribution. Thus will it make us really see those mysterious regions which Jules Verne only showed us in imagination.
This is not an empty illusion. M. Faye, comparing all the measurements, has reached a result well calculated to surprise us. Under the oceans, in the depths, are rocks of very great density; under the continents, on the contrary, are empty spaces.
New observations will modify perhaps the details of these conclusions.
In any case, our venerated dean has shown us where to search and what the geodesist may teach the geologist, desirous of knowing the interior constitution of the earth, and even the thinker wishing to speculate upon the past and the origin of this planet.
And now, why have I entitled this chapter _French Geodesy_? It is because, in each country, this science has taken, more than all others, perhaps, a national character. It is easy to see why.
There must be rivalry. The scientific rivalries are always courteous, or at least almost always; in any case, they are necessary, because they are always fruitful. Well, in those enterprises which require such long efforts and so many collaborators, the individual is effaced, in spite of himself, of course; no one has the right to say: this is my work. Therefore it is not between men, but between nations that rivalries go on.
So we are led to seek what has been the part of France. Her part I believe we are right to be proud of.
At the beginning of the eighteenth century, long discussions arose between the Newtonians who believed the earth flattened, as the theory of gravitation requires, and Cassini, who, deceived by inexact measurements, believed our globe elongated. Only direct observation could settle the question. It was our Academy of Sciences that undertook this task, gigantic for the epoch.
While Maupertuis and Clairaut measured a degree of meridian under the polar circle, Bouguer and La Condamine went toward the Andes Mountains, in regions then under Spain which to-day are the Republic of Ecuador.
Our envoys were exposed to great hardships. Traveling was not as easy as at present.
Truly, the country where Maupertuis operated was not a desert and he even enjoyed, it is said, among the Laplanders those sweet satisfactions of the heart that real arctic voyagers never know. It was almost the region where, in our days, comfortable steamers carry, each summer, hosts of tourists and young English people. But in those days Cook's agency did not exist and Maupertuis really believed he had made a polar expedition.
Perhaps he was not altogether wrong. The Russians and the Swedes carry out to-day analogous measurements at Spitzbergen, in a country where there is real ice-cap. But they have quite other resources, and the difference of time makes up for that of latitude.
The name of Maupertuis has reached us much scratched by the claws of Doctor Akakia; the scientist had the misfortune to displease Voltaire, who was then the king of mind. He was first praised beyond measure; but the flatteries of kings are as much to be dreaded as their displeasure, because the days after are terrible. Voltaire himself knew something of this.
Voltaire called Maupertuis, my amiable master in thinking, marquis of the polar circle, dear flattener out of the world and Cassini, and even, flattery supreme, Sir Isaac Maupertuis; he wrote him: "Only the king of Prussia do I put on a level with you; he only lacks being a geometer." But soon the scene changes, he no longer speaks of deifying him, as in days of yore the Argonauts, or of calling down from Olympus the council of the gods to contemplate his works, but of chaining him up in a madhouse. He speaks no longer of his sublime mind, but of his despotic pride, plated with very little science and much absurdity.
I care not to relate these comico-heroic combats; but permit me some reflections on two of Voltaire's verses. In his 'Discourse on Moderation' (no question of moderation in praise and criticism), the poet has written:
You have confirmed in regions drear What Newton discerned without going abroad.
These two verses (which replace the hyperbolic praises of the first period) are very unjust, and doubtless Voltaire was too enlightened not to know it.
Then, only those discoveries were esteemed which could be made without leaving one's house.
To-day, it would rather be theory that one would make light of.
This is to misunderstand the aim of science.
Is nature governed by caprice, or does harmony rule there? That is the question. It is when it discloses to us this harmony that science is beautiful and so worthy to be cultivated. But whence can come to us this revelation, if not from the accord of a theory with experiment? To seek whether this accord exists or if it fails, this therefore is our aim. Consequently these two terms, which we must compare, are as indispensable the one as the other. To neglect one for the other would be nonsense. Isolated, theory would be empty, experiment would be blind; each would be useless and without interest.
Maupertuis therefore deserves his share of glory. Truly, it will not equal that of Newton, who had received the spark divine; nor even that of his collaborator Clairaut. Yet it is not to be despised, because his work was necessary, and if France, outstripped by England in the seventeenth century, has so well taken her revenge in the century following, it is not alone to the genius of Clairauts, d'Alemberts, Laplaces that she owes it; it is also to the long patience of the Maupertuis and the La Condamines.
We reach what may be called the second heroic period of geodesy. France is torn within. All Europe is armed against her; it would seem that these gigantic combats might absorb all her forces. Far from it; she still has them for the service of science. The men of that time recoiled before no enterprise, they were men of faith.
Delambre and Méchain were commissioned to measure an arc going from Dunkerque to Barcelona. This time there was no going to Lapland or to Peru; the hostile squadrons had closed to us the ways thither. But, though the expeditions are less distant, the epoch is so troubled that the obstacles, the perils even, are just as great.
In France, Delambre had to fight against the ill-will of suspicious municipalities. One knows that the steeples, which are visible from so far, and can be aimed at with precision, often serve as signal points to geodesists. But in the region Delambre traversed there were no longer any steeples. A certain proconsul had passed there, and boasted of knocking down all the steeples rising proudly above the humble abode of the sans-culottes. Pyramids then were built of planks and covered with white cloth to make them more visible. That was quite another thing: with white cloth! What was this rash person who, upon our heights so recently set free, dared to raise the hateful standard of the counter-revolution? It was necessary to border the white cloth with blue and red bands.
Méchain operated in Spain; the difficulties were other; but they were not less. The Spanish peasants were hostile. There steeples were not lacking: but to install oneself in them with mysterious and perhaps diabolic instruments, was it not sacrilege? The revolutionists were allies of Spain, but allies smelling a little of the stake.
"Without cease," writes Méchain, "they threaten to butcher us." Fortunately, thanks to the exhortations of the priests, to the pastoral letters of the bishops, these ferocious Spaniards contented themselves with threatening.
Some years after Méchain made a second expedition into Spain: he proposed to prolong the meridian from Barcelona to the Balearics. This was the first time it had been attempted to make the triangulations overpass a large arm of the sea by observing signals installed upon some high mountain of a far-away isle. The enterprise was well conceived and well prepared; it failed however.
The French scientist encountered all sorts of difficulties of which he complains bitterly in his correspondence. "Hell," he writes, perhaps with some exaggeration--"hell and all the scourges it vomits upon the earth, tempests, war, the plague and black intrigues are therefore unchained against me!"
The fact is that he encountered among his collaborators more of proud obstinacy than of good will and that a thousand accidents retarded his work. The plague was nothing, the fear of the plague was much more redoubtable; all these isles were on their guard against the neighboring isles and feared lest they should receive the scourge from them. Méchain obtained permission to disembark only after long weeks upon the condition of covering all his papers with vinegar; this was the antisepsis of that time.
Disgusted and sick, he had just asked to be recalled, when he died.
Arago and Biot it was who had the honor of taking up the unfinished work and carrying it on to completion.
Thanks to the support of the Spanish government, to the protection of several bishops and, above all, to that of a famous brigand chief, the operations went rapidly forward. They were successfully completed, and Biot had returned to France when the storm burst.
It was the moment when all Spain took up arms to defend her independence against France. Why did this stranger climb the mountains to make signals? It was evidently to call the French army. Arago was able to escape the populace only by becoming a prisoner. In his prison, his only distraction was reading in the Spanish papers the account of his own execution. The papers of that time sometimes gave out news prematurely. He had at least the consolation of learning that he died with courage and like a Christian.
Even the prison was no longer safe; he had to escape and reach Algiers. There, he embarked for Marseilles on an Algerian vessel. This ship was captured by a Spanish corsair, and behold Arago carried back to Spain and dragged from dungeon to dungeon, in the midst of vermin and in the most shocking wretchedness.
If it had only been a question of his subjects and his guests, the dey would have said nothing. But there were on board two lions, a present from the African sovereign to Napoleon. The dey threatened war.
The vessel and the prisoners were released. The port should have been properly reached, since they had on board an astronomer; but the astronomer was seasick, and the Algerian seamen, who wished to make Marseilles, came out at Bougie. Thence Arago went to Algiers, traversing Kabylia on foot in the midst of a thousand perils. He was long detained in Africa and threatened with the convict prison. Finally he was able to get back to France; his observations, which he had preserved and safeguarded under his shirt, and, what is still more remarkable, his instruments had traversed unhurt these terrible adventures. Up to this point, not only did France hold the foremost place, but she occupied the stage almost alone.
In the years which follow, she has not been inactive and our staff-office map is a model. However, the new methods of observation and calculation have come to us above all from Germany and England. It is only in the last forty years that France has regained her rank. She owes it to a scientific officer, General Perrier, who has successfully executed an enterprise truly audacious, the junction of Spain and Africa. Stations were installed on four peaks upon the two sides of the Mediterranean. For long months they awaited a calm and limpid atmosphere. At last was seen the little thread of light which had traversed 300 kilometers over the sea. The undertaking had succeeded.
To-day have been conceived projects still more bold. From a mountain near Nice will be sent signals to Corsica, not now for geodesic determinations, but to measure the velocity of light. The distance is only 200 kilometers; but the ray of light is to make the journey there and return, after reflection by a mirror installed in Corsica. And it should not wander on the way, for it must return exactly to the point of departure.
Ever since, the activity of French geodesy has never slackened. We have no more such astonishing adventures to tell; but the scientific work accomplished is immense. The territory of France beyond the sea, like that of the mother country, is covered by triangles measured with precision.
We have become more and more exacting and what our fathers admired does not satisfy us to-day. But in proportion as we seek more exactitude, the difficulties greatly increase; we are surrounded by snares and must be on our guard against a thousand unsuspected causes of error. It is needful, therefore, to create instruments more and more faultless.
Here again France has not let herself be distanced. Our appliances for the measurement of bases and angles leave nothing to desire, and, I may also mention the pendulum of Colonel Defforges, which enables us to determine gravity with a precision hitherto unknown.
The future of French geodesy is at present in the hands of the Geographic Service of the army, successively directed by General Bassot and General Berthaut. We can not sufficiently congratulate ourselves upon it. For success in geodesy, scientific aptitudes are not enough; it is necessary to be capable of standing long fatigues in all sorts of climates; the chief must be able to win obedience from his collaborators and to make obedient his native auxiliaries. These are military qualities. Besides, one knows that, in our army, science has always marched shoulder to shoulder with courage.
I add that a military organization assures the indispensable unity of action. It would be more difficult to reconcile the rival pretensions of scientists jealous of their independence, solicitous of what they call their fame, and who yet must work in concert, though separated by great distances. Among the geodesists of former times there were often discussions, of which some aroused long echoes. The Academy long resounded with the quarrel of Bouguer and La Condamine. I do not mean to say that soldiers are exempt from passion, but discipline imposes silence upon a too sensitive self-esteem.
Several foreign governments have called upon our officers to organize their geodesic service: this is proof that the scientific influence of France abroad has not declined.
Our hydrographic engineers contribute also to the common achievement a glorious contingent. The survey of our coasts, of our colonies, the study of the tides, offer them a vast domain of research. Finally I may mention the general leveling of France which is carried out by the ingenious and precise methods of M. Lallemand.
With such men we are sure of the future. Moreover, work for them will not be lacking; our colonial empire opens for them immense expanses illy explored. That is not all: the International Geodetic Association has recognized the necessity of a new measurement of the arc of Quito, determined in days of yore by La Condamine. It is France that has been charged with this operation; she had every right to it, since our ancestors had made, so to speak, the scientific conquest of the Cordilleras. Besides, these rights have not been contested and our government has undertaken to exercise them.
Captains Maurain and Lacombe completed a first reconnaissance, and the rapidity with which they accomplished their mission, crossing the roughest regions and climbing the most precipitous summits, is worthy of all praise. It won the admiration of General Alfaro, President of the Republic of Ecuador, who called them 'los hombres de hierro,' the men of iron.
The final commission then set out under the command of Lieutenant-Colonel (then Major) Bourgeois. The results obtained have justified the hopes entertained. But our officers have encountered unforeseen difficulties due to the climate. More than once, one of them has been forced to remain several months at an altitude of 4,000 meters, in the clouds and the snow, without seeing anything of the signals he had to aim at and which refused to unmask themselves. But thanks to their perseverance and courage, there resulted from this only a delay and an increase of expense, without the exactitude of the measurements suffering therefrom.
GENERAL CONCLUSIONS
What I have sought to explain in the preceding pages is how the scientist should guide himself in choosing among the innumerable facts offered to his curiosity, since indeed the natural limitations of his mind compel him to make a choice, even though a choice be always a sacrifice. I have expounded it first by general considerations, recalling on the one hand the nature of the problem to be solved and on the other hand seeking to better comprehend that of the human mind, which is the principal instrument of the solution. I then have explained it by examples; I have not multiplied them indefinitely; I also have had to make a choice, and I have chosen naturally the questions I had studied most. Others would doubtless have made a different choice; but what difference, because I believe they would have reached the same conclusions.
There is a hierarchy of facts; some have no reach; they teach us nothing but themselves. The scientist who has ascertained them has learned nothing but a fact, and has not become more capable of foreseeing new facts. Such facts, it seems, come once, but are not destined to reappear.
There are, on the other hand, facts of great yield; each of them teaches us a new law. And since a choice must be made, it is to these that the scientist should devote himself.
Doubtless this classification is relative and depends upon the weakness of our mind. The facts of slight outcome are the complex facts, upon which various circumstances may exercise a sensible influence, circumstances too numerous and too diverse for us to discern them all. But I should rather say that these are the facts we think complex, since the intricacy of these circumstances surpasses the range of our mind. Doubtless a mind vaster and finer than ours would think differently of them. But what matter; we can not use that superior mind, but only our own.
The facts of great outcome are those we think simple; may be they really are so, because they are influenced only by a small number of well-defined circumstances, may be they take on an appearance of simplicity because the various circumstances upon which they depend obey the laws of chance and so come to mutually compensate. And this is what happens most often. And so we have been obliged to examine somewhat more closely what chance is.
Facts where the laws of chance apply become easy of access to the scientist who would be discouraged before the extraordinary complication of the problems where these laws are not applicable. We have seen that these considerations apply not only to the physical sciences, but to the mathematical sciences. The method of demonstration is not the same for the physicist and the mathematician. But the methods of invention are very much alike. In both cases they consist in passing up from the fact to the law, and in finding the facts capable of leading to a law.
To bring out this point, I have shown the mind of the mathematician at work, and under three forms: the mind of the mathematical inventor and creator; that of the unconscious geometer who among our far distant ancestors, or in the misty years of our infancy, has constructed for us our instinctive notion of space; that of the adolescent to whom the teachers of secondary education unveil the first principles of the science, seeking to give understanding of the fundamental definitions. Everywhere we have seen the rôle of intuition and of the spirit of generalization without which these three stages of mathematicians, if I may so express myself, would be reduced to an equal impotence.
And in the demonstration itself, the logic is not all; the true mathematical reasoning is a veritable induction, different in many regards from the induction of physics, but proceeding like it from the particular to the general. All the efforts that have been made to reverse this order and to carry back mathematical induction to the rules of logic have eventuated only in failures, illy concealed by the employment of a language inaccessible to the uninitiated. The examples I have taken from the physical sciences have shown us very different cases of facts of great outcome. An experiment of Kaufmann on radium rays revolutionizes at the same time mechanics, optics and astronomy. Why? Because in proportion as these sciences have developed, we have the better recognized the bonds uniting them, and then we have perceived a species of general design of the chart of universal science. There are facts common to several sciences, which seem the common source of streams diverging in all directions and which are comparable to that knoll of Saint Gothard whence spring waters which fertilize four different valleys.
And then we can make choice of facts with more discernment than our predecessors who regarded these valleys as distinct and separated by impassable barriers.
It is always simple facts which must be chosen, but among these simple facts we must prefer those which are situated upon these sorts of knolls of Saint Gothard of which I have just spoken.
And when sciences have no direct bond, they still mutually throw light upon one another by analogy. When we studied the laws obeyed by gases we knew we had attacked a fact of great outcome; and yet this outcome was still estimated beneath its value, since gases are, from a certain point of view, the image of the milky way, and those facts which seemed of interest only for the physicist, ere long opened new vistas to astronomy quite unexpected.
And finally when the geodesist sees it is necessary to move his telescope some seconds to see a signal he has set up with great pains, this is a very small fact; but this is a fact of great outcome, not only because this reveals to him the existence of a small protuberance upon the terrestrial globe, that little hump would be by itself of no great interest, but because this protuberance gives him information about the distribution of matter in the interior of the globe, and through that about the past of our planet, about its future, about the laws of its development.
* * * * *
INDEX
aberration of light, 315, 496
Abraham, 311, 490-1, 505-7, 509, 515-6
absolute motion, 107 orientation, 83 space, 85, 93, 246, 257, 353
acceleration, 94, 98, 486, 509
accidental constant, 112 errors, 171, 402
accommodation of the eyes, 67-8
action at a distance, 137
addition, 34
aim of mathematics, 280
alchemists, 11
Alfaro, 543
algebra, 379
analogy, 220
analysis, 218-9, 279
analysis situs, 53, 239, 381
analyst, 210, 221
ancestral experience, 91
Andrade, 93, 104, 228
Andrews, 153
angle sum of triangle, 58
Anglo-Saxons, 3
antinomies, 449, 457, 477
Arago, 540-1
Aristotle, 205, 292, 460
arithmetic, 34, 379, 441, 463
associativity, 35
assumptions, 451, 453
astronomy, 81, 289, 315, 512
Atwood, 446
axiom, 60, 63, 65, 215
Bacon, 128
Bartholi, 503
Bassot, 542
beauty, 349, 368
Becquerel, 312
Beltrami, 56, 58
Bergson, 321
Berkeley, 4
Berthaut, 542
Bertrand, 156, 190, 211, 395
Betti, 239
Biot, 540
bodies, solid, 72
Boltzmann, 304
Bolyai, 56, 201, 203
Borel, 482
Bouguer, 537, 542
Bourgeois, 543
Boutroux, 390, 464
Bradley, 496
Briot, 298
Brownian movement, 152, 410
Bucherer, 507
Burali-Forti, 457-9, 477, 481-2
Caen, 387-8
Calinon, 228
canal rays, 491-2
canals, semicircular, 276
Cantor, 11, 448-9, 457, 459, 477
Cantorism, 381, 382, 480, 484
capillarity, 298
Carlyle, 128
Carnot's principle, 143, 151, 300, 303-5, 399
Cassini, 537
cathode rays, 487-92
cells, 217
center of gravity, 103
central forces, 297
Chaldeans, 290
chance, 395, 408
change of position, 70 state, 70
chemistry of the stars, 295
circle-squarers, 11
Clairaut, 537-8
Clausius, 119, 123, 143
color sensation, 252
Columbus, 228
commutativity, 35-6
compensation, 72
complete induction, 40
Comte, 294
Condorcet, 411
contingence, 340
continuity, 173
continuum, 43 amorphous, 238 mathematical, 46 physical, 46, 240 tridimensional, 240
convention, 50, 93, 106, 125, 173, 208, 317, 440, 451
convergence, 67-8
coordinates, 244
Copernicus, 109, 291, 354
Coulomb, 143, 516
Couturat, 450, 453, 456, 460, 462-3, 467, 472-6
creation, mathematical, 383
creed, 1
Crémieu, 168-9, 490
crisis, 303
Crookes, 195, 488, 527-8
crude fact, 326, 330
Curie, 312-3, 318
current, 186
curvature, 58-9
curve, 213, 346
curves without tangents, 51
cut, 52, 256
cyclones, 353
d'Alembert, 538
Darwin, 518-9
De Cyon, 276, 427
Dedekind, 44-5
Defforges, 542
definitions, 430, 453
deformation, 73, 415
Delage, 277
Delambre, 539
Delbeuf, 414
Descartes, 127
determinism, 123, 340
dictionary, 59
didymium, 333
dilatation, 76
dimensions, 53, 68, 78, 241, 256, 426
direction, 69
Dirichlet, 213
dispersion, 141
displacement, 73, 77, 247, 256
distance, 59, 292
distributivity, 36
Du Bois-Reymond, 50
earth, rotation of, 326, 353
eclipse, 326
electricity, 174
electrified bodies, 117
electrodynamic attraction, 308 induction, 188 mass, 311
electrodynamics, 184, 282
electromagnetic theory of light, 301
electrons, 316, 492-4, 505-8, 510, 512-4
elephant, 217, 436
ellipse, 215
Emerson, 203
empiricism, 86, 271
Epimenides, 478-9
equation of Laplace, 283
Erdély, 203
errors, accidental, 171, 402 law of, 119 systematic, 171, 402 theory of, 402, 406
ether, 145, 351
ethics, 205
Euclid, 62, 86, 202-3, 213
Euclidean geometry, 65, 235-6, 337
Euclid's postulate, 83, 91, 124, 353, 443, 453, 468, 470-1
experience, 90-1
experiment, 127, 317, 336, 446
fact, crude, 326, 330 in the rough, 327 scientific, 326
facts, 362, 371
Fahrenheit, 238
Faraday, 150, 192
Faye, 536
Fechner, 46, 52
Fehr, 383
finite, 57
Fitzgerald, 415-6, 500-1, 505
Fizeau, 146, 149, 309, 498, 504
Flammarion, 400, 406-7
flattening of the earth, 353
force, 72, 98, 444 direction of, 445 -flow, 284
forces, central, 297 equivalence of, 445 magnitude of, 445
Foucault's pendulum, 85, 109, 353
four dimensions, 78
Fourier, 298-9
Fourier's problem, 317 series, 286
Franklin, 513-4
Fresnel, 132, 140, 153, 174, 176, 181, 351, 498
Fuchsian, 387-8
function, 213 continuous, 218, 288
Galileo, 97, 331, 353-4
gaseous pressure, 141
gases, theory of, 400, 405, 523
Gauss, 384-5, 406
Gay-Lussac, 157
generalize, 342
geodesy, 535
geometer, 83, 210, 438
geometric space, 66
geometry, 72, 81, 125, 207, 380, 428, 442, 467 Euclidean, 65, 93 fourth, 62 non-Euclidean, 55 projective, 201 qualitative, 238 rational, 5, 467 Riemann's, 57 spheric, 59
Gibbs, 304
Goldstein, 492
Gouy, 152, 305, 410
gravitation, 512
Greeks, 93, 368
Hadamard, 459
Halsted, 3, 203, 464, 467
Hamilton, 115
helium, 294
Helmholtz, 56, 115, 118, 141, 190, 196
Hercules, 449
Hermite, 211, 220, 222, 285
Herschel, 528
Hertz, 102, 145, 194-5, 427, 488, 498, 502, 504, 510
Hertzian oscillator, 309, 317
Hilbert, 5, 11, 203, 433, 450-1, 464-8, 471, 475-7, 484
Himstedt, 195
Hipparchus, 291
homogeneity, 74, 423
homogeneous, 67
hydrodynamics, 284
hyperbola, 215
hypotheses, 6, 15, 127, 133
hysteresis, 151
identity of spaces, 268 of two points, 259
illusions, optical, 202
incommensurable numbers, 44
induction, complete, 40, 452-3, 467-8 electromagnetic, 188 mathematical, 40, 220 principle of, 481
inertia, 93, 486, 489, 507
infinite, 448
infinitesimals, 50
inquisitor, 331
integration, 139
interpolation, 131
intuition, 210, 213, 215
invariant, 333
Ionians, 127
ions, 152
irrational number, 44
irreversible phenomena, 151
isotropic, 67
Japanese mice, 277, 427
Jevons, 451
John Lackland, 128
Jules Verne, 111, 536
Jupiter, 131, 157, 231, 289
Kant, 16, 64, 202-3, 450-1, 471
Kauffman, 311, 490-1, 495, 506-7, 522, 545
Kazan, 203
Kelvin, 145, 523-4, 526-7
Kepler, 120, 133, 153, 282, 291-2
Kepler's laws, 136, 516
kinematics, 337
kinetic energy, 116 theory of gases, 141
Kirchhoff, 98-9, 103-5
Klein, 60, 211, 287
knowledge, 201
König, 144, 477
Kovalevski, 212, 286
Kronecker, 44
Lacombe, 543
La Condamine, 535, 537-8, 542-3
Lagrange, 98, 151, 179
Laisant, 383
Lallamand, 543
Langevin, 509
Laplace, 298, 398, 514-5, 518, 522, 538
Laplace's equation, 283, 287
Larmor, 145, 150
Lavoisier's principle, 301, 310, 312
law, 207, 291, 395
Leibnitz, 32, 450, 471
Le Roy, 28, 321-6, 332, 335, 337, 347-8, 354, 468
Lesage, 517-21
Liard, 440
Lie, 62-3, 212
light sensations, 252 theory of, 351 velocity of, 232, 312
Lindemann, 508
line, 203, 243
linkages, 144
Lippmann, 196
Lobachevski, 29, 56, 60, 62, 83, 86, 203
Lobachevski's space, 239
local time, 306-7, 499
logic, 214, 435, 448, 460-2, 464
logistic, 457, 472-4
logisticians, 472
Lorentz, 147, 149, 196-7, 306, 308, 311, 315, 415-6, 492, 498-502, 504-9, 512, 514-6, 521
Lotze, 264
luck, 399
Lumen, 407-8
MacCullagh, 150
Mach, 375
Mach-Delage, 276
magnetism, 149
magnitude, 49
Mariotte's law, 120, 132, 157, 342, 524
Maros, 203
mass, 98, 312, 446, 486, 489, 494, 515
mathematical analysis, 218 continuum, 46 creation, 383 induction, 40, 220 physics, 136, 297, 319
mathematics, 369, 448
matter, 492
Maupertuis, 535, 537-8
Maurain, 543
Maxwell, 140, 152, 175, 177, 181, 193, 282-3, 298, 301, 304-5, 351, 503, 524-5
Maxwell-Bartholi, 309, 503-4, 519, 521
Mayer, 119, 123, 300, 312, 318
measurement, 49
Méchain, 539-40
mechanical explanation, 177 mass, 312
mechanics, 92, 444, 486, 496, 512 anthropomorphic, 103 celestial, 279 statistical, 304
Méray, 211
metaphysician, 221
meteorology, 398
mice, 277
Michelson, 306, 309, 311, 316, 498, 500-1
milky way, 523-30
Mill, Stuart, 60-1, 453-4
Monist, 4, 89, 464
moons of Jupiter, 233
Morley, 309
motion of liquids, 283 of moon, 28 of planets, 341 relative, 107, 487 without deformation, 236
multiplication, 36
muscular sensations, 69
Nagaoka, 317
nature, 127
navigation, 289
neodymium, 333
neomonics, 283
Neumann, 181
Newton, 85, 96, 98, 109, 153, 291, 370, 486, 516, 536, 538
Newton's argument, 108, 334, 343 law, 111, 118, 132, 136, 149, 157, 233, 282, 292, 512, 514-5, 518, 525 principle, 146, 300, 308-9, 312
no-class theory, 478
nominalism, 28, 125, 321, 333, 335
non-Euclidean geometry, 55, 59, 388 language, 127 space, 55, 235, 237 straight, 236, 470 world, 75
number, 31 big, 88 imaginary, 283 incommensurable, 44 transfinite, 448-9 whole, 44, 469
objectivity, 209, 347, 349, 408
optical illusions, 202
optics, 174, 496
orbit of Saturn, 341
order, 385
orientation, 83
osmotic, 141
Padoa, 463
Panthéon, 414
parallax, 470
parallels, 56, 443
Paris time, 233
parry, 419-22, 427
partition, 45
pasigraphy, 456-7
Pasteur, 128
Peano, 450, 456-9, 463, 472
Pender, 490
pendulum, 224
Perrier, 541
Perrin, 195
phosphorus, 333, 468, 470-1
physical continuum, 46
physics, 127, 140, 144, 279, 297
physics of central forces, 297 of the principles, 299
Pieri, 11, 203
Plato, 292
Poincaré, 473
point, 89, 244
Poncelet, 215
postulates, 382
potential energy, 116
praseodymium, 333
principle, 125, 299 Carnot's, 143, 151, 300, 303-5, 399 Clausius', 119, 123, 143 Hamilton's, 115 Lavoisier's, 300, 310 Mayer's, 119, 121, 123, 300, 312, 318 Newton's, 146, 300, 308-9, 312 of action and reaction, 300, 487, 502 of conservation of energy, 300 of degradation of energy, 300 of inertia, 93, 486, 507 of least action, 118, 300 of relativity, 300, 305, 498, 505
Prony, 445
psychologist, 383
Ptolemy, 110, 291, 353-4
Pythagoras, 292
quadrature of the circle, 161
qualitative geometry, 238 space, 207 time, 224
quaternions, 282
radiometer, 503
radium, 312, 318, 486-7
Rados, 201
Ramsay, 313
rational geometry, 5, 467
reaction, 502
reality, 217, 340, 349
Réaumur, 238
recurrence, 37
Regnault, 170
relativity, 83, 305, 417, 423, 498, 505
Richard, 477-8, 480-1
Riemann, 56, 62, 145, 212, 239, 243, 381, 432 surface, 211, 287
Roemer, 233
Röntgen, 511, 520
rotation of earth, 225, 331, 353
roulette, 403
Rowland, 194-7, 305, 489
Royce, 202
Russell, 201, 450, 460-2, 464-7, 471-4, 477-82, 484-5
St. Louis exposition, 208, 320
Sarcey, 442
Saturn, 231, 317
Schiller, 202
Schliemann, 19
science, 205, 321, 323, 340, 354
Science and Hypothesis, 205-7, 220, 240, 246-7, 319, 353, 452
semicircular canals, 276
series, development in, 287 Fourier's, 286
Sirius, 226, 229
solid bodies, 72
space, 55, 66, 89, 235, 256 absolute, 85, 93 amorphous, 417 Bolyai, 56 Euclidean, 65 geometric, 66 Lobachevski's, 239 motor, 69 non-Euclidean, 55, 235, 237 of four dimensions, 78 perceptual, 66, 69 tactile, 68, 264 visual, 67, 252
spectra, 316
spectroscope, 294
Spencer, 9
sponge, 219
Stallo, 10
stars, 292
statistical mechanics, 304
straight, 62, 82, 236, 433, 450, 470
Stratonoff, 531
surfaces, 58
systematic errors, 171
tactile space, 68, 264
Tait, 98
tangent, 51
Tannery, 43
teaching, 430, 437
thermodynamics, 115, 119
Thomson, 98, 488
thread, 104
time, 223 equality, 225 local, 306, 307 measure of, 223-4
Tisserand, 515-6
Tolstoi, 354, 362, 368
Tommasina, 519
Transylvania, 203
triangle, 58 angle sum of, 58
truth, 205
Tycho Brahe, 133, 153, 228
unity of nature, 130
universal invariant, 333
Uriel, 203
van der Waals, 153
Vauban, 210
Veblen, 203
velocity of light, 232, 312
Venus of Milo, 201
verification, 33
Virchow, 21
visual impressions, 252 space, 67, 252
Volga, 203
Voltaire, 537-8
Weber, 117, 515-6
Weierstrass, 11, 212, 432
Whitehead, 472, 481-2
whole numbers, 44
Wiechert, 145, 488
x-rays, 152, 511, 520
Zeeman effect, 152, 196, 317, 494
Zeno, 382
Zermelo, 477, 482-3
zigzag theory, 478
zodiac, 398, 404
* * * * *
Transcriber's Note: The Greek alphabets are represented within square brackets. For example, [alpha] stands for first Greek alphabet alpha. Square root of a number is represented using the symbol (sqrt). That is to say, sqrt(25) stands for square root of 25. The superscript is shown with carat (^) symbol, example, 10^{5} stands for 5th power of 10. Similarly, subscript is represented by underscore (_) symbol. For instance, n_{3} stands for letter n with subscript 3.