The nebular theory posits that the solar system formed from a rotating cloud of gas and dust, known as a solar nebula. The major steps include the gravitational collapse of the nebula, leading to the formation of a protostar at its center, while the remaining material flattened into a rotating disk. Within this disk, particles collided and coalesced to form planetesimals, which eventually grew into planets. Finally, the remaining gas and debris were cleared away, leading to the stable solar system we observe today.
The steps of the Nebular Theory consist of: The collapse of the nebula and formation of the protoplanetary disk and protosun. The condensation of planetessimals. The Accretion of planetessimals to form planet seeds. The Formation of Jovian planets through nebular capture and the solar wind of young sun clears away the remaining gas.
Pierre Simon de Laplace
Pierre Simon de laplace
It fits the known data.
The nebular theory was proposed in 1755 by the German philosopher Immanuel Kant and was further developed by French mathematician and astronomer Pierre-Simon Laplace in 1796.
The steps of the Nebular Theory consist of: The collapse of the nebula and formation of the protoplanetary disk and protosun. The condensation of planetessimals. The Accretion of planetessimals to form planet seeds. The Formation of Jovian planets through nebular capture and the solar wind of young sun clears away the remaining gas.
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Pierre Simon de Laplace
Pierre Simon de laplace