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 IV - STARS WITH BANDED SPECTRA
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
The shining face of each one of the innumerable suns aggregated into the vast system of the galaxy is, as we have said, veiled by absorbing vapours; but in widely varying degrees. The light of Vega, though indelibly stamped with the characteristic lines of hydrogen, reaches our upper air without sensible general modification. Sunlight is not only charged with significant inscriptions, but throughout toned down and mellowed; while in Aldebaran, the process of stoppage in the blue has been carried so far as to leave the red rays visibly predominant. In Aldebaran, too, the first symptoms begin to appear of a generic change in the manner of absorption through the emergence of dark bands in addition to the dark lines of the spectrum.
This change is full of meaning. Isolated rays of definite wave-lengths, forming in the spectrum what we call ‘lines,’ bright or dark, are emitted only at very high temperatures. They represent perhaps the fundamental vibrations of the ‘atoms’ of each different substance. But these, at lower grades of heat, are not free to thrill separately. Bound together into ‘molecules,’ they give rise, by their associated vibrations, to complex systems of light-waves, dispersed into sets of prismatic ‘flutings,’ each with a sharp and a nebulous side. The fluted spectra thus constituted are derived from chemical compounds such as oxides and chlorides, as well as from ‘elementary’ substances, both metallic and non-metallic, at moderate degrees of heat.
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- The System of the Stars , pp. 52 - 65Publisher: Cambridge University PressPrint publication year: 2010First published in: 1890