So, looking at the the degree of priloznosti rotating spheroid, the separated ring can to have or form of a Hoop, or a disk shape. This should take in consideration another fact. Much prelucrata or lenticular the spheroid shape of the ring can be different, depending on its value. Very thin ring, is one that captured only the top layer the Equatorial surface, will be in the form of a Hoop, while more a 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 and the volume of separated rings, maximum thickness of this ring will account or in the direction of its plane, or perpendicular to to its plane. But this circumstance should have a strong impact on the rotation of the planet, which is formed subsequently from the ring. In the misty ring having quite bruceebaby form, the difference between the speeds internal and external surfaces should be very small. And such ring, gathered in mass, the greatest diameter of which intersects at right the angle of the plane of its orbit, will give nearly probably this weight the vast the desire to rotate in the direction crossing the plane of the orbit at right angle. Where the ring has not quite bruceebaby form and where consequently, the difference between the speed of rotation of the inner and outer layers more significant, there must influence two opposite aspirations: one moving mass to rotate towards the plane of the orbit, and the other impelling it to rotate in the direction perpendicular to this plane; owing to which the plane of rotation will take some middle position. Finally, if misty ring has a pronounced disk-like shape and because this merges into the mass, the greatest dimensions of which coincide with the plane of orbit, both of these aspirations will combine to cause the rotation in this plane.
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So, looking at the
the degree of priloznosti rotating spheroid, the separated ring can
to have or form of a Hoop, or a disk shape. This should take in
consideration another fact. Much prelucrata or lenticular
the spheroid shape of the ring can be different, depending on its value. Very
thin ring, is one that captured only the top layer
the Equatorial surface, will be in the form of a Hoop, while more
a 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 and
the volume of separated rings, maximum thickness of this ring will
account or in the direction of its plane, or perpendicular to
to its plane. But this circumstance should have a strong impact on
the rotation of the planet, which is formed subsequently from the ring. In the misty ring
having quite bruceebaby form, the difference between the speeds
internal and external surfaces should be very small. And such
ring, gathered in mass, the greatest diameter of which intersects at right
the angle of the plane of its orbit, will give nearly probably this weight the vast
the desire to rotate in the direction crossing the plane of the orbit at right
angle. Where the ring has not quite bruceebaby form and where
consequently, the difference between the speed of rotation of the inner and outer layers
more significant, there must influence two opposite aspirations:
one moving mass to rotate towards the plane of the orbit, and the other impelling
it to rotate in the direction perpendicular to this plane; owing to
which the plane of rotation will take some middle position. Finally, if
misty ring has a pronounced disk-like shape and because
this merges into the mass, the greatest dimensions of which coincide with the plane
of orbit, both of these aspirations will combine to cause the rotation in this
plane.
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