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Result From Rotating Gas Cloud

Result From Rotating Gas Cloud. Conservation Of Angular Momentum. The reason for the high rate of rotation of the gas giants is not well understood but the theory is that they were formed through the orderly collapse of a rotating gas cloud so that the angular.

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Formation of an accretion disc by infall of a rotating gas cloud onto a central object was first treated by Ulrich 1976 in the context of star formation and accretion discs around protostars. Of a rotating gas cloud held together by gravitational attraction to a central mass. A small body from which a planet originated in the early stages of development of the solar system is called a A.

Conservation Of Angular Momentum.

Nebulae nebulae or nebulas is an interstellar cloud of dust hydrogen helium and other ionized gasesOriginally the term was used to describe any diffused astronomical object including galaxies beyond the Milky WayThe Andromeda Galaxy for instance was once referred to as the Andromeda Nebula and spiral galaxies in general as spiral nebulae. A small body from which a planet originated in the early stages of development of the solar system is called a A. The molecular cloud cores from which stars form are of order one million times larger than the ultimate stellar diameter. What is the form of the collapse under gravitational forces of a uniformly rotating spheroidal gas cloud.