![]() | The Scientific Monthly | ![]() |
The average eccentricity of the orbits of the four inner planets (per unit mass) is 0.0221, and of the four outer planets is 0.0489.
It would seem that all rotating nebulæ should in reality possess some of the attributes of spiral motion. Whether the spiral structure should be visible or invisible to a terrestrial observer would depend upon the sizes and distances of the nebulæ, upon the distribution of materials composing them, and perhaps upon other factors. See developed the hypothesis that spiral nebulæ owe their origin to the collision of two nebulæ. Collisions of this kind could readily occur because of the enormous dimensions of the nebulæ, and motions of rotation and consequently spiral structure might readily result therefrom. The abnormally high speeds of the spiral nebulæ are apparently a very strong objection to the hypothesis.
![]() | The Scientific Monthly | ![]() |