The Project Gutenberg eBook of Pioneers of Science
Title: Pioneers of Science
Author: Sir Oliver Lodge
Release date: April 26, 2009 [eBook #28613]
Language: English
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Transcriber’s Note
The punctuation and spelling from the original text have been faithfully preserved. Only obvious typographical errors have been corrected.
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φενόμενα
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PIONEERS OF SCIENCE
NEWTON
From the picture by Kneller, 1689, now at Cambridge
PIONEERS OF SCIENCE
BY
OLIVER LODGE, F.R.S.
PROFESSOR OF PHYSICS IN VICTORIA UNIVERSITY COLLEGE, LIVERPOOL
WITH PORTRAITS AND OTHER ILLUSTRATIONS
London
MACMILLAN AND CO.
AND NEW YORK
1893
Richard Clay and Sons, Limited,
LONDON AND BUNGAY.
PREFACE
This book takes its origin in a course of lectures on the history and progress of Astronomy arranged for me in the year 1887 by three of my colleagues (A.C.B., J.M., G.H.R.), one of whom gave the course its name.
The lectures having been found interesting, it was natural to write them out in full and publish.
If I may claim for them any merit, I should say it consists in their simple statement and explanation of scientific facts and laws. The biographical details are compiled from all readily available sources, there is no novelty or originality about them; though it is hoped that there may be some vividness. I have simply tried to present a living figure of each Pioneer in turn, and to trace his influence on the progress of thought.
I am indebted to many biographers and writers, among others to Mr. E.J.C. Morton, whose excellent set of lives published by the S.P.C.K. saved me much trouble in the early part of the course.
As we approach recent times the subject grows more complex, and the men more nearly contemporaries; hence the biographical aspect diminishes and the scientific treatment becomes fuller, but in no case has it been allowed to become technical and generally unreadable.
To the friends (C.C.C., F.W.H.M., E.F.R.) who with great kindness have revised the proofs, and have indicated places where the facts could be made more readily intelligible by a clearer statement, I express my genuine gratitude.
University College, Liverpool,
November, 1892.
CONTENTS
| PART I | |
| LECTURE I | |
| PAGE | |
| COPERNICUS AND THE MOTION OF THE EARTH | 2 |
| LECTURE II | |
| TYCHO BRAHÉ AND THE EARLIEST OBSERVATORY | 32 |
| LECTURE III | |
| KEPLER AND THE LAWS OF PLANETARY MOTION | 56 |
| LECTURE IV | |
| GALILEO AND THE INVENTION OF THE TELESCOPE | 80 |
| LECTURE V | |
| GALILEO AND THE INQUISITION | 108 |
| LECTURE VI | |
| DESCARTES AND HIS THEORY OF VORTICES | 136 |
| LECTURE VII | |
| SIR ISAAC NEWTON | 159 |
| LECTURE VIII | |
| NEWTON AND THE LAW OF GRAVITATION | 180 |
| LECTURE IX | |
| NEWTON'S "PRINCIPIA" | 203 |
PART II |
|
| LECTURE X | |
| ROEMER AND BRADLEY AND THE VELOCITY OF LIGHT | 232 |
| LECTURE XI | |
| LAGRANGE AND LAPLACE—THE STABILITY OF THE SOLAR SYSTEM, AND THE NEBULAR HYPOTHESIS | 254 |
| LECTURE XII | |
| HERSCHEL AND THE MOTION OF THE FIXED STARS | 273 |
| LECTURE XIII | |
| THE DISCOVERY OF THE ASTEROIDS | 294 |
| LECTURE XIV | |
| BESSEL—THE DISTANCES OF THE STARS, AND THE DISCOVERY OF STELLAR PLANETS | 304 |
| LECTURE XV | |
| THE DISCOVERY OF NEPTUNE | 317 |
| LECTURE XVI | |
| COMETS AND METEORS | 331 |
| LECTURE XVII | |
| THE TIDES | 353 |
| LECTURE XVIII | |
| THE TIDES, AND PLANETARY EVOLUTION | 379 |
ILLUSTRATIONS
| FIG. | PAGE | |||
| 1. | Archimedes | 8 | ||
| 2. | Leonardo da Vinci | 10 | ||
| 3. | Copernicus | 12 | ||
| 4. | Homeric Cosmogony | 15 | ||
| 5. | Egyptian Symbol of the Universe | 16 | ||
| 6. | Hindoo Earth | 17 | ||
| 7. | Order of ancient Planets corresponding to the Days of the Week | 19 | ||
| 8. | Ptolemaic System | 20 | ||
| 9. | Specimens of Apparent Paths of Venus and of Mars among the stars | 21 | ||
| 10. | Apparent Epicyclic Orbits of Jupiter and Saturn | 22 | ||
| 11. | Egyptian System | 24 | ||
| 12. | True Orbits of Earth and Jupiter | 25 | ||
| 13. | Orbits of Mercury and Earth | 25 | ||
| 14. | Copernican System as frequently represented | 26 | ||
| 15. | Slow Movement of the North Pole in a Circle among the Stars | 29 | ||
| 16. | Tychonic system, showing the Sun with all the Planets revolving round the Earth | 38 | ||
| 17. | Portrait of Tycho | 41 | ||
| 18. | Early out-door Quadrant of Tycho | 43 | ||
| 19. | Map of Denmark, showing the Island of Huen | 45 | ||
| 20. | Uraniburg | 46 | ||
| 21. | Astrolabe | 47 | ||
| 22. | Tycho's large Sextant | 48 | ||
| 23. | The Quadrant in Uraniburg | 49 | ||
| 24. | Tycho's Form of Transit Circle | 50 | ||
| 25. | A Modern Transit Circle | 51 | ||
| 26. | Orbits of some of the Planets drawn to scale | 60 | ||
| 27. | Many-sided Polygon or Approximate Circle enveloped by Straight Lines | 61 | ||
| 28. | Kepler's Idea of the Regular Solids | 62 | ||
| 29. | Diagram of Equant | 67 | ||
| 30. | Excentric Circle supposed to be divided into equal Areas | 68 | ||
| 31. | Mode of drawing an Ellipse | 70 | ||
| 32. | Kepler's Diagram proving Equable Description of Areas for an Ellipse | 71 | ||
| 33. | Diagram of a Planet's Velocity in Different Parts of its Orbit | 72 | ||
| 34. | Portrait of Kepler | 76 | ||
| 35. | Curve described by a Projectile | 82 | ||
| 36. | Two Forms of Pulsilogy | 87 | ||
| 37. | Tower of Pisa | 91 | ||
| 38. | View of the Half-Moon in small Telescope | 97 | ||
| 39. | Portion of the Lunar Surface more highly magnified | 98 | ||
| 40. | Another Portion of the Lunar Surface | 99 | ||
| 41. | Lunar Landscape showing Earth | 100 | ||
| 42. | Galileo's Method of estimating the Height of Lunar Mountain | 101 | ||
| 43. | Some Clusters and Nebulæ | 102 | ||
| 44. | Stages of the Discovery of Jupiter's Satellites | 103 | ||
| 45. | Eclipses of Jupiter's Satellites | 105 | ||
| 46. | Old Drawings of Saturn by Different Observers, with the imperfect Instruments of that day | 111 | ||
| 47. | Phases of Venus | 112 | ||
| 48. | Sunspots as seen with Low Power | 113 | ||
| 49. | A Portion of the Sun's Disk as seen in a powerful modern Telescope | 114 | ||
| 50. | Saturn and his Rings | 115 | ||
| 51. | Map of Italy | 118 | ||
| 52. | Portrait of Galileo | 126 | ||
| 53. | Portrait of Descartes | 148 | ||
| 54. | Descartes's Eye Diagram | 151 | ||
| 55. | Descartes's Diagram of Vortices from his "Principia" | 152 | ||
| 56. | Manor-house of Woolsthorpe | 162 | ||
| 57. | Projectile Diagram | 170 | ||
| 58. | } | { | 171 | |
| 59. | Diagrams illustrative of those near the Beginning of Newton's "Principia" | 174 | ||
| 60. | 175 | |||
| 61-2. | 175 | |||
| 63. | Prismatic Dispersion | 182 | ||
| 64. | A single Constituent of White Light is capable of no more Dispersion | 183 | ||
| 65. | Parallel Beam passing through a Lens | 184 | ||
| 66. | Newton's Telescope | 186 | ||
| 67. | The Sextant, as now made | 187 | ||
| 68. | Newton when young | 196 | ||
| 69. | Sir Isaac Newton | 200 | ||
| 70. | Another "Principia" Diagram | 207 | ||
| 71. | Well-known Model exhibiting the Oblate Spheroidal Form as a Consequence of spinning about a Central Axis | 219 | ||
| 72. | Jupiter | 221 | ||
| 73. | Diagram of Eye looking at a Light reflected in a Distant Mirror through the Teeth of a revolving Wheel | 238 | ||
| 74. | Fizeau's Wheel, showing the appearance of distant Image seen through its Teeth | 239 | ||
| 75. | Eclipses of one of Jupiter's Satellites | 241 | ||
| 76. | A Transit instrument for the British Astronomical Expedition, 1874 | 243 | ||
| 77. | Diagram of equatorially mounted Telescope | 245 | ||
| 78. | Aberration Diagram | 250 | ||
| 79. | Showing the three Conjunction Places in the Orbits of Jupiter and Saturn | 259 | ||
| 80. | Lord Rosse's Drawing of the Spiral Nebula in Canes Venatici | 269 | ||
| 81. | Saturn | 271 | ||
| 82. | Principle of Newtonian Reflector | 278 | ||
| 83. | Herschel's 40-foot telescope | 283 | ||
| 84. | William Herschel | 285 | ||
| 85. | Caroline Herschel | 287 | ||
| 86. | Double Stars | 288 | ||
| 87. | Old Drawing of the Cluster in Hercules | 290 | ||
| 88. | Old Drawing of the Andromeda Nebula | 291 | ||
| 89. | The Great Nebula in Orion | 292 | ||
| 90. | Planetary Orbits to scale | 297 | ||
| 91. | Diagram illustrating Parallax | 307 | ||
| 92. | The Königsberg Heliometer | 312 | ||
| 93. | Perturbations of Uranus | 320 | ||
| 94. | Uranus' and Neptune's Relative Positions | 325 | ||
| 95. | Meteorite | 333 | ||
| 96. | Meteor Stream crossing Field of Telescope | 334 | ||
| 97. | Diagram of Direction of Earth's Orbital Motion | 335 | ||
| 98. | Parabolic and Elliptic Orbits | 340 | ||
| 99. | Orbit of Halley's Comet | 341 | ||
| 100. | Various Appearances of Halley's Comet when last seen | 342 | ||
| 101. | Head of Donati's Comet of 1858 | 343 | ||
| 102. | Comet | 344 | ||
| 103. | Encke's Comet | 345 | ||
| 104. | Biela's Comet as last seen in two Portions | 346 | ||
| 105. | Radiant Point Perspective | 348 | ||
| 106. | Present Orbit of November Meteors | 349 | ||
| 107. | Orbit of November Meteors before and after Encounter with Uranus | 351 | ||
| 108. | The Mersey | 355 | ||
| 109. | Co-tidal Lines, showing the way the Tidal Wave reaches the British Isles from the Atlantic | 359 | ||
| 110. | Whirling Earth Model | 364 | ||
| 111. | Earth and Moon Model | 365 | ||
| 112. | Earth and Moon (Earth's Rotation Neglected) | 366 | ||
| 113. | Maps showing how comparatively Free from Land Obstruction the Ocean in the Southern Hemisphere Is | 369 | ||
| 114. | Spring and Neap Tides | 370 | ||
| 115. | Tidal Clock | 371 | ||
| 116. | Sir William Thomson (Lord Kelvin) | 373 | ||
| 117. | Tide-gauge for recording Local Tides | 375 | ||
| 118. | Harmonic Analyzer | 375 | ||
| 119. | Tide-predicter | 376 | ||
| 120. | Weekly Sheet of Curves | 377 |
PIONEERS OF SCIENCE
PART I
FROM DUSK TO DAYLIGHT
DATES AND SUMMARY OF FACTS FOR LECTURE I
Physical Science of the Ancients. Thales 640 B.C., Anaximander 610 B.C., Pythagoras 600 B.C., Anaxagoras 500 B.C., Eudoxus 400 B.C., Aristotle 384 B.C., Aristarchus 300 B.C., Archimedes 287 B.C., Eratosthenes 276 B.C., Hipparchus 160 B.C., Ptolemy 100 A.D.
Science of the Middle Ages. Cultivated only among the Arabs; largely in the forms of astrology, alchemy, and algebra.
Return of Science to Europe. Roger Bacon 1240, Leonardo da Vinci 1480, (Printing 1455), Columbus 1492, Copernicus 1543.
A sketch of Copernik's life and work. Born 1473 at Thorn in Poland. Studied mathematics at Bologna. Became an ecclesiastic. Lived at Frauenburg near mouth of Vistula. Substituted for the apparent motion of the heavens the real motion of the earth. Published tables of planetary motions. Motion still supposed to be in epicycles. Worked out his ideas for 36 years, and finally dedicated his work to the Pope. Died just as his book was printed, aged 72, a century before the birth of Newton. A colossal statue by Thorwaldsen erected at Warsaw in 1830.
PIONEERS OF SCIENCE
LECTURE I
COPERNICUS AND THE MOTION OF THE EARTH
The ordinary run of men live among phenomena of which they know nothing and care less. They see bodies fall to the earth, they hear sounds, they kindle fires, they see the heavens roll above them, but of the causes and inner working of the whole they are ignorant, and with their ignorance they are content.
"Understand the structure of a soap-bubble?" said a cultivated literary man whom I know; "I wouldn't cross the street to know it!"
And if this is a prevalent attitude now, what must have been the attitude in ancient times, when mankind was emerging from savagery, and when history seems composed of harassments by wars abroad and revolutions at home? In the most violently disturbed times indeed, those with which ordinary history is mainly occupied, science is quite impossible. It needs as its condition, in order to flourish, a fairly quiet, untroubled state, or else a cloister or university removed from the din and bustle of the political and commercial world. In such places it has taken its rise, and in such peaceful places and quiet times true science will continue to be cultivated.
The great bulk of mankind must always remain, I suppose, more or less careless of scientific research and scientific result, except in so far as it affects their modes of locomotion, their health and pleasure, or their purse.
But among a people hurried and busy and preoccupied, some in the pursuit of riches, some in the pursuit of pleasure, and some, the majority, in the struggle for existence, there arise in every generation, here and there, one or two great souls—men who seem of another age and country, who look upon the bustle and feverish activity and are not infected by it, who watch others achieving prizes of riches and pleasure and are not disturbed, who look on the world and the universe they are born in with quite other eyes. To them it appears not as a bazaar to buy and to sell in; not as a ladder to scramble up (or down) helter-skelter without knowing whither or why; but as a fact—a great and mysterious fact—to be pondered over, studied, and perchance in some small measure understood. By the multitude these men were sneered at as eccentric or feared as supernatural. Their calm, clear, contemplative attitude seemed either insane or diabolic; and accordingly they have been pitied as enthusiasts or killed as blasphemers. One of these great souls may have been a prophet or preacher, and have called to his generation to bethink them of why and what they were, to struggle less and meditate more, to search for things of true value and not for dross. Another has been a poet or musician, and has uttered in words or in song thoughts dimly possible to many men, but by them unutterable and left inarticulate. Another has been influenced still more directly by the universe around him, has felt at times overpowered by the mystery and solemnity of it all, and has been impelled by a force stronger than himself to study it, patiently, slowly, diligently; content if he could gather a few crumbs of the great harvest of knowledge, happy if he could grasp some great generalization or wide-embracing law, and so in some small measure enter into the mind and thought of the Designer of all this wondrous frame of things.
These last have been the men of science, the great and heaven-born men of science; and they are few. In our own day, amid the throng of inventions, there are a multitude of small men using the name of science but working for their own ends, jostling and scrambling just as they would jostle and scramble in any other trade or profession. These may be workers, they may and do advance knowledge, but they are never pioneers. Not to them is it given to open out great tracts of unexplored territory, or to view the promised land as from a mountain-top. Of them we shall not speak; we will concern ourselves only with the greatest, the epoch-making men, to whose life and work we and all who come after them owe so much. Such a man was Thales. Such was Archimedes, Hipparchus, Copernicus. Such pre-eminently was Newton.
Now I am not going to attempt a history of science. Such a work in ten lectures would be absurd. I intend to pick out a few salient names here and there, and to study these in some detail, rather than by attempting to deal with too many to lose individuality and distinctness.
We know so little of the great names of antiquity, that they are for this purpose scarcely suitable. In some departments the science of the Greeks was remarkable, though it is completely overshadowed by their philosophy; yet it was largely based on what has proved to be a wrong method of procedure, viz the introspective and conjectural, rather than the inductive and experimental methods. They investigated Nature by studying their own minds, by considering the meanings of words, rather than by studying things and recording phenomena. This wrong (though by no means, on the face of it, absurd) method was not pursued exclusively, else would their science have been valueless, but the influence it had was such as materially to detract from the value of their speculations and discoveries. For when truth and falsehood are inextricably woven into a statement, the truth is as hopelessly hidden as if it had never been stated, for we have no criterion to distinguish the false from the true.