 | Astronomical Society of the Pacific - 1905 - 606 pages
...formed, and the further elaboration of the theory does not all depend upon this particular genetic history. It is sufficient to show that a spiral nebula...What will be the properties of a system formed from siich a nebula? As developed by Dr. MOULTON, they are as follows: — ( 1 ) The planets will all revolve... | |
 | 1905 - 382 pages
...nebula it is assumed (I) that the central mass was relatively very .great ; (2) that the knots were very irregular in size and placed .at irregular distances from the center ; and (3) that the nebulous portion* was very small relative to the central ,mass and probably large relative... | |
 | Newton Horace Winchell - 1905 - 482 pages
...nebula it is assumed (1) that the central mass was relatively very great; (2) that the knots were very irregular in size and placed at irregular distances from the center; and (3) that the nebulous portion was very small relative to the central mass and probably large relative... | |
 | Victoria Institute (Great Britain) - 1905 - 404 pages
...nebula it is assumed (L) that the central mass was relatively very great; (2) that the knots were very irregular in size and placed at irregular distances from the center; and (3) that the nebulous portion was very small relative to the central mass and probably large relative... | |
 | Carnegie Institution of Washington - 1905 - 340 pages
...it is assumed ( 1 ) that the central mass was relatively very great ; (2) that the knots were very irregular in size and placed at irregular distances from the center; and (3) that the nebulous portion was very small relative to the central mass and probably large relative... | |
 | Victoria Institute (Great Britain) - 1905 - 372 pages
...nebula it is assumed (I) that the central mass was relatively very great ; (2) that the knots were very irregular in size and placed -at irregular distances from the center ; and (3) that the nebulous portion was very small relative to the central mass and probably large relative... | |
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In the particular case of the solar nebula it is assumed (1) that the central mass was relatively very great; (2) that the knots were very irregular in size and placed at irregular distances from the center; and (3) that the nebulous portion was very... 