Book contents
- Frontmatter
- PREFACE
- Contents
- ILLUSTRATIONS
- ADDENDA
- CHAPTER I THE TASK OF SIDEREAL ASTRONOMY
- CHAPTER II THE METHODS OF SIDEREAL RESEARCH
- CHAPTER III SIRIAN AND SOLAR STARS
- CHAPTER IV STARS WITH BANDED SPECTRA
- CHAPTER V GASEOUS STARS AND NEBULÆ
- CHAPTER VI SIDEREAL EVOLUTION
- CHAPTER VII TEMPORARY STARS
- CHAPTER VIII VARIABLE STARS OF LONG PERIOD
- CHAPTER IX VARIABLE STARS OF SHORT PERIOD
- CHAPTER X THE COLOURS OF THE STARS
- CHAPTER XI DOUBLE STARS
- CHAPTER XII VARIABLE DOUBLE STARS
- CHAPTER XIII STELLAR ORBITS
- CHAPTER XIV MULTIPLE STARS
- CHAPTER XV THE PLEIADES
- CHAPTER XVI STAR CLUSTERS
- CHAPTER XVII THE FORMS OF NEBULÆ
- CHAPTER XVIII THE GREAT NEBULÆ
- CHAPTER XIX THE NATURE AND CHANGES OF NEBULÆ
- CHAPTER XX THE DISTANCES OF THE STARS
- CHAPTER XXI TRANSLATION OF THE SOLAR SYSTEM
- CHAPTER XXII THE PROPER MOTIONS OF THE STARS
- CHAPTER XXIII THE MILKY WAY
- CHAPTER XXIV STATUS OF THE NEBULÆ
- CHAPTER XXV THE CONSTRUCTION OF THE HEAVENS
- APPENDIX.—TABLES OF STELLAR DATA
- INDEX
- Plate section
CHAPTER XV - THE PLEIADES
Published online by Cambridge University Press: 05 July 2011
- Frontmatter
- PREFACE
- Contents
- ILLUSTRATIONS
- ADDENDA
- CHAPTER I THE TASK OF SIDEREAL ASTRONOMY
- CHAPTER II THE METHODS OF SIDEREAL RESEARCH
- CHAPTER III SIRIAN AND SOLAR STARS
- CHAPTER IV STARS WITH BANDED SPECTRA
- CHAPTER V GASEOUS STARS AND NEBULÆ
- CHAPTER VI SIDEREAL EVOLUTION
- CHAPTER VII TEMPORARY STARS
- CHAPTER VIII VARIABLE STARS OF LONG PERIOD
- CHAPTER IX VARIABLE STARS OF SHORT PERIOD
- CHAPTER X THE COLOURS OF THE STARS
- CHAPTER XI DOUBLE STARS
- CHAPTER XII VARIABLE DOUBLE STARS
- CHAPTER XIII STELLAR ORBITS
- CHAPTER XIV MULTIPLE STARS
- CHAPTER XV THE PLEIADES
- CHAPTER XVI STAR CLUSTERS
- CHAPTER XVII THE FORMS OF NEBULÆ
- CHAPTER XVIII THE GREAT NEBULÆ
- CHAPTER XIX THE NATURE AND CHANGES OF NEBULÆ
- CHAPTER XX THE DISTANCES OF THE STARS
- CHAPTER XXI TRANSLATION OF THE SOLAR SYSTEM
- CHAPTER XXII THE PROPER MOTIONS OF THE STARS
- CHAPTER XXIII THE MILKY WAY
- CHAPTER XXIV STATUS OF THE NEBULÆ
- CHAPTER XXV THE CONSTRUCTION OF THE HEAVENS
- APPENDIX.—TABLES OF STELLAR DATA
- INDEX
- Plate section
Summary
From multiple stars the transition is easy to star-clusters. These seem to embody completely the idea contained in germ in the former class of objects. They are collections, often on the grandest scale, of sunlike bodies small and large, united in origin and history, acted upon by identical forces, tending towards closely related ends. The manner and measure of their aggregation, however, vary widely, and with them the cogency of the evidence as to their organic oneness. There are innumerable cases in which it absolutely excludes doubt; there are some in which it is rather persuasive than convincing. It is not then always easy to distinguish between a casual ‘sprinkle’ of stars and a genuine cluster. Nor can the movement-test, by which so many physical have been discriminated from optical double-stars, be here applied. Internal displacements of a circulatory character have not yet become apparent in any cluster, and there is only one with an ascertained common proper motion.
This is the immemorial group of the Pleiades, famous in legend, and instructive, above all others, to exact inquirers—the meeting-place in the skies of mythology and science. The vivid and picturesque aspect of these stars riveted, from the earliest ages, the attention of mankind; a peculiar sacredness attached to them, and their concern with human destinies was believed to be especially close and direct.
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- The System of the Stars , pp. 220 - 233Publisher: Cambridge University PressPrint publication year: 2010First published in: 1890