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قراءة كتاب Man's Place in the Universe A Study of the Results of Scientific Research in Relation to the Unity or Plurality of Worlds, 3rd Edition

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Man's Place in the Universe
A Study of the Results of Scientific Research in Relation to the Unity or Plurality of Worlds, 3rd Edition

Man's Place in the Universe A Study of the Results of Scientific Research in Relation to the Unity or Plurality of Worlds, 3rd Edition

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دار النشر: Project Gutenberg
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CONTENTS

CHAP. PAGE
I. Early Ideas, 1
II. Modern Ideas, 7
III. The New Astronomy, 24
IV. The Distribution of the Stars, 47
V. Distances of Stars: the Sun's Motion, 73
VI. Unity and Evolution of the Star-System, 99
VII. Are the Stars Infinite? 135
VIII. Our Relation To the Milky Way, 156
IX. The Uniformity of Matter and its Laws, 183
X. The Essential Characters of Organisms, 191
XI. Physical Conditions essential for Life, 206
XII. The Earth in relation to Life, 218
XIII. The Atmosphere in relation to Life, 243
XIV. The Other Planets are not Habitable, 262
XV. The Stars: Have they Planets? Are they useful to Us? 282
XVI. Stability of the Star-System: Importance of Central Position: Summary and Conclusion, 295
Index, 326

EIGHT DIAGRAMS IN THE TEXT AND

TWO STAR CHARTS AT END.


'Who is man, and what his place? Anxious asks the heart, perplext In this recklessness of space, Worlds with worlds thus intermixt: What has he, this atom creature, In the infinitude of Nature?'

F.T. Palgrave.


MAN'S PLACE IN THE UNIVERSE


CHAPTER I

EARLY IDEAS AS TO THE UNIVERSE AND ITS

RELATION TO MAN

When men attained to sufficient intelligence for speculations as to their own nature and that of the earth on which they lived, they must have been profoundly impressed by the nightly pageant of the starry heavens. The intense sparkling brilliancy of Sirius and Vega, the more massive and steady luminosity of Jupiter and Venus, the strange grouping of the brighter stars into constellations to which fantastic names indicating their resemblance to various animals or terrestrial objects seemed appropriate and were soon generally adopted, together with the apparently innumerable stars of less and less brilliancy scattered broadcast over the sky, many only being visible on the clearest nights and to the acutest vision, constituted altogether a scene of marvellous and impressive splendour of which it must have seemed almost impossible to attain any real knowledge, but which afforded an endless field for the imagination of the observer.

The relation of the stars to the sun and moon in their respective motions was one of the earliest problems for the astronomer, and it was only solved by careful and continuous observation, which showed that the invisibility of the former during the day was wholly due to the blaze of light, and this is said to have been proved at an early period by the observed fact that from the bottom of very deep wells stars can be seen while the sun is shining. During total eclipses of the sun also the brighter stars become visible, and, taken in connection with the fixity of position of the pole-star, and the course of those circumpolar stars which never set in the latitudes of Greece, Egypt, and Chaldea, it soon became possible to frame a simple hypothesis which supposed the earth to be suspended in space, while at an unknown distance from it a crystal sphere revolved upon an axis indicated by the pole-star,

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