 | Thomas Chrowder Chamberlin, Rollin D. Salisbury - 1905 - 740 Seiten
...moved about the central mass in elliptical orbits of considerable, but not excessive, eccentricity. It postulates a simple mode of origin of the nebula connected...approach of the ancestral sun to another large body, but the main hypothesis is not dependent on this postulate. It assigns the gathering-in of the planetesimals... | |
 | American Geographical Society of New York - 1906 - 906 Seiten
...moved about the central mass in elliptical orbits of considerable, but not excessive, eccentricity. It postulates a simple mode of origin of the nebula connected...approach of the ancestral sun to another large body, but the main hypothesis is not dependent on this postulate. It assigns the gathering-in of the planetesimals... | |
 | Oklahoma Geological Survey - 1914 - 56 Seiten
...moved about the central mass in elliptical orbits of considerable, but not excessive, eccentricity. It postulates a simple mode of origin of the nebula connected...approach of the ancestral sun to another large body, but the main hypothesis is not dependent on this postulate. It assigns the' gathering-in of the planetesimals... | |
 | Oklahoma Geological Survey - 1914 - 52 Seiten
...moved about the central mass in elliptical orbits of considerable, but not excessive, eccentricity. It postulates a simple mode of origin of the nebula connected...approach of the ancestral sun to another large body, but the main hypothesis is not dependent on this postulate. It assigns the gathering-in of the planetesimals... | |
 | Oklahoma Geological Survey - 1914 - 60 Seiten
...moved about the central mass in elliptical orbits of considerable, but not excessive, eccentricity. It postulates a simple mode of origin of the nebula connected...approach of the ancestral sun to another large body, but the main hypothesis is not dependent on this postulate. It assigns the gathering-in of the planetesimals... | |
 | American Geographical Society of New York - 1906 - 954 Seiten
...moved about the central mass in elliptical orbits of considerable, but not excessive, eccentricity. It postulates a simple mode of origin of the nebula connected...approach of the ancestral sun to another large body, but the main hypothesis is not dependent on this postulate. It assigns the gathering-in of the planetesimals... | |
| |
... the nebula as the nuclei of the future planets, and the nebulous haze as matter to be added to these nuclei to form the planets. It assumes that both the knots and the particles of the nebulous haze moved about the central mass in elliptical orbits... 