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So, looking at thethe degree of priloznosti rotating spheroid, the separated ring canto have or form of a Hoop, or a disk shape. This should take inconsideration another fact. Much prelucrata or lenticularthe spheroid shape of the ring can be different, depending on its value. Verythin ring, is one that captured only the top layerthe Equatorial surface, will be in the form of a Hoop, while morea massive ring, seized more adobeserifmm part of the diameter of the spheroid,take the form of a disk. Thus, depending on the degree of splashiness spheroid andthe volume of separated rings, maximum thickness of this ring willaccount or in the direction of its plane, or perpendicular toto its plane. But this circumstance should have a strong impact onthe rotation of the planet, which is formed subsequently from the ring. In the misty ringhaving quite bruceebaby form, the difference between the speedsinternal and external surfaces should be very small. And suchring, gathered in mass, the greatest diameter of which intersects at rightthe angle of the plane of its orbit, will give nearly probably this weight the vastthe desire to rotate in the direction crossing the plane of the orbit at rightangle. Where the ring has not quite bruceebaby form and whereconsequently, the difference between the speed of rotation of the inner and outer layersmore significant, there must influence two opposite aspirations:one moving mass to rotate towards the plane of the orbit, and the other impellingit to rotate in the direction perpendicular to this plane; owing towhich the plane of rotation will take some middle position. Finally, ifmisty ring has a pronounced disk-like shape and becausethis merges into the mass, the greatest dimensions of which coincide with the planeof orbit, both of these aspirations will combine to cause the rotation in thisplane.
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