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Problems in astrophysics

Clerke, Agnes M. (Agnes Mary) · Public domain text

194,740 words · about 13 h 38 min to read

About this edition

The text of Problems in astrophysics comes from Project Gutenberg e-text #79177. It is public domain in the United States. Project Gutenberg’s header and license text are removed, and RedLectern sets the text out for reading on screen; no words of the book are rewritten or summarized. More formats (EPUB, Kindle) · How RedLectern is built

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About this book

Author
Agnes M. Clerke (1842–1907)
Language
English
Subjects
Astrophysics
Length
194,740 words · about 13 h 38 min
Sections
58 reader sections · Table of contents
Contents (58)
  1. Opening under 1 min
  2. Preface about 21 min
  3. I. PROGRESS OF SOLAR PHYSICS about 11 min
  4. II. THE CHEMISTRY OF THE SUN about 18 min
  5. III. PECULIARITIES OF THE SOLAR SPECTRUM about 10 min
  6. IV. THE REVERSING LAYER about 11 min
  7. V. HYDROGEN, HELIUM, AND CORONIUM about 13 min
  8. VI. THE PHOTOSPHERE AND ITS DUSKY VEIL about 15 min
  9. VII. STRUCTURE AND MOVEMENTS OF SUN-SPOTS about 18 min
  10. VIII. THE SPECTRUM OF SUN-SPOTS about 12 min
  11. IX. FACULÆ AND PROMINENCES about 17 min
  12. X. THE CHROMOSPHERIC SPECTRUM about 13 min
  13. XI. THE CORONA about 27 min
  14. XII. THE SUN’S ROTATION about 11 min
  15. XIII. THE SOLAR CYCLE about 13 min
  16. XIV. THE SUN AS A WHOLE about 10 min
  17. I. PROGRESS OF SIDEREAL PHYSICS about 11 min
  18. II. THE CLASSIFICATION OF STELLAR SPECTRA about 14 min
  19. III. HELIUM STARS about 11 min
  20. IV. HYDROGEN STARS about 9 min
  21. V. SOLAR STARS about 8 min
  22. VI. STARS WITH FLUTED SPECTRA about 8 min
  23. VII. CARBON STARS about 9 min
  24. VIII. STARS WITH FLUTED SPECTRA SHOWING BRIGHT LINES about 9 min
  25. IX. HELIUM STARS WITH BRIGHT LINES about 10 min
  26. X. WOLF-RAYET STARS about 8 min
  27. XI. THE GENERAL QUESTION OF BRIGHT LINES IN STELLAR SPECTRA about 3 min
  28. XII. ANOMALOUS AND VARIABLE SPECTRA about 8 min
  29. XIII. COLOUR VARIABILITY about 15 min
  30. XIV. THE SPECTRA OF DOUBLE STARS about 11 min
  31. XV. THE EVOLUTION OF THE STARS about 13 min
  32. XVI. ROTATION OF THE STARS about 7 min
  33. XVII. SPECTROSCOPIC BINARIES about 19 min
  34. XVIII. ECLIPSING STARS about 28 min
  35. XIX. SHORT-PERIOD VARIABLES about 11 min
  36. XX. SHORT-PERIOD VARIABLES—Continued about 11 min
  37. XXI. THE PROBLEM OF BETA LYRÆ about 12 min
  38. XXII. STARS VARIABLE IN LONG PERIODS about 18 min
  39. XXIII. PECULIAR AND IRREGULAR VARIABLES about 15 min
  40. XXIV. TEMPORARY STARS about 31 min
  41. XXV. DARK STARS about 6 min
  42. XXVI. THE GENERAL QUESTION OF STELLAR VARIABILITY about 6 min
  43. XXVII. IRREGULAR STAR CLUSTERS about 8 min
  44. XXVIII. NEBULOUS CLUSTERS—THE PLEIADES about 9 min
  45. XXIX. NEBULOUS CLUSTERS—Continued. about 7 min
  46. XXX. GLOBULAR CLUSTERS about 14 min
  47. XXXI. WHITE NEBULÆ about 19 min
  48. XXXII. DOUBLE NEBULÆ about 9 min
  49. XXXIII. NEBULOUS STARS about 12 min
  50. XXXIV. PLANETARY NEBULÆ about 21 min
  51. XXXV. ANNULAR NEBULÆ about 15 min
  52. XXXVI. THE ORION NEBULA about 15 min
  53. XXXVII. OTHER IRREGULAR NEBULÆ about 13 min
  54. XXXVIII. NONDESCRIPT NEBULÆ about 7 min
  55. XXXIX. VARIABLE NEBULÆ about 10 min
  56. XL. THE NATURE OF NEBULÆ about 10 min
  57. XLI. THE PHYSICS OF THE MILKY WAY about 12 min
  58. Appendix about 1 h 42 min

The opening of Preface

The object of the present work is not so much to instruct as to suggest. It represents a sort of reconnaissance, and embodies the information collected by scouts and skirmishers regarding practicable lines of advance and accessible points of attack, with a view to annexing for the realm of knowledge some further strips and corners from the territory of ignorance. Its inspiring motive, in short, is the desire for a rectification of the frontier in the interests of science. Material resources for the furtherance of such encroachments are not lacking. The globe is studded with observatories, variously and admirably equipped. Yet innumerable objects in the sidereal heavens remain neglected, mainly through inadvertence to the extraordinary interest of the questions pending with respect to them. In the following pages it has been sought to indicate some of these individually, and in their relations to the larger meanings of cosmical research. But this could be done effectually only from the vantage-ground of our actual acquirements; hence the book, although primarily designed to stimulate the progress of astrophysics, necessarily includes an account of its present state. Before attempting to add to our store of learning, we must realise what is already possessed.

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