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التركية - الإنجليزية

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(Astronomi) solar nebula

A disc-shaped cloud of gas and dust left over from the formation of the Sun

(Astronomi) The rotating flattened cloud of gas and dust from which the sun and the rest of the bodies in the solar system

Gaseous cloud from which, in the nebular hypothesis of the origin of the solar system, the Sun and planets formed by condensation. In 1755 Immanuel Kant suggested that a nebula gradually pulled together by its own gravity developed into the Sun and planets. Pierre-Simon Laplace in 1796 proposed a similar model, in which a rotating and contracting cloud of gas the young Sun shed concentric rings of matter that condensed into the planets. James Clerk Maxwell showed that if all the matter in the known planets had once been distributed this way, shearing forces would have prevented such condensation. Another objection was that the Sun has less angular momentum than the theory seems to require. In the early 20th century most astronomers preferred the collision theory: that the planets formed as a result of a close approach to the Sun by another star. Eventually, however, stronger objections were mounted to the collision theory than to the nebular hypothesis, and a modified version of the latter, in which a rotating matter disk gave rise to the planets through successively larger aglommerations from dust grains through planetesimals and protoplanets, became the prevailing theory of the solar system's origin

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