THE SOURCE AND MODE OF SOLAR ENERGY. STATEMENT OF THE PROBLEM OF SOLAR ENERGY. THE CONSTITUTION AND PHENOMENA OF THE SUN. THE DISTRIBUTION AND CONSERVATION OF SOLAR ENERGY. TEMPORARY STARS, METEORS, AND COMETS. INTERPRETATION OF COMETIC PHENOMENA. THE RESOLVABLE NEBULAE, STAR-CLUSTERS AND GALAXIES. THE NEBULAR HYPOTHESIS: ITS BASIS AND ITS DIFFICULTIES. THE GENESIS OF SOLAR SYSTEMS AND GALAXIES. CONCLUSION. THE HARMONY OF NATURE'S LAWS AND OPERATIONS. REFERENCE INDEX OF AUTHORITIES CITED. Typical stages in development of a solar system. (Reproduced from nature. See Chapter XIII.)—1. Newton’s comet, A.D. 1680. 2. Comet of 1811, from Guillemin. 3. Donati’s comet, 1858, from Proctor. 4. Nebula in ship Argo, from Flammarion. 5. Open spiral nebula in Virgo, Plate XV., Nichol’s “Architecture of the Heavens,” after Lord Rosse. 6. Plate XII. of same work, nebula in Canes Venatici: a partially closed spiral. 7. Frontispiece of same, an almost completed spiral, in the Lion, seen obliquely: rupture of convolutions preparatory to formation of planets. 8. Ideal solar system. Original Title Page. THE SOURCE AND MODE OF SOLAR ENERGY THROUGHOUT THE UNIVERSE. ILLUSTRATED. PHILADELPHIA: J. B. LIPPINCOTT COMPANY. 1895. |