Solar System Formation of the Solar System Many scientists believed that the solar system was formed when in space a cloud of gas and dust was disturbed, by the explosion of a close by star known as a supernova. This explosion made waves in space which compressed the cloud of gas and dust. The cloud starts to collapse after getting pressed, as gravity together...
Solar System Formation of the Solar System Many scientists believed that the solar system was formed when in space a cloud of gas and dust was disturbed, by the explosion of a close by star known as a supernova. This explosion made waves in space which compressed the cloud of gas and dust. The cloud starts to collapse after getting pressed, as gravity together pulled the gas and dust, and formed a solar nebula. Thus, the cloud began to spin as it collapsed (UCAR).
Picture of Solar System Finally, as the cloud grew more hot and dense in the center, surrounded by a disk of gas and dust, which was hot in the center and cooler at the edges. And as the disk became thinner and thinner, particles started to stick together and form clumps, where few clumps got bigger, forming particles while, small clumps stuck to them, ultimately forming planets or moons (UCAR).
Thus, as the materials condensed and clump into chunks of rock/metal in the inner solar system and while ice in the outer solar system and eventually formed the planets called planetestimals. The picture below shows small planetestimals forming a thin disk and orbiting the new Sun (UCAR). Now near the center of the cloud, where planets like Earth formed, materials that were only rocky could stand the great heat.
On the other hand, icy matter was settled in the outer regions of the disk along with rocky material, forming giant planets such as Jupiter. It was the initial first billion years that there was still a significant amount of large pieces of rock and ice flying around the solar system. These were the materials that had not accreted into a planet, until about 3.8 billion years ago rife in collisions were formed. The following picture shows the same (The Columbia Encyclopedia, 2004).
As the cloud continued to fall in, eventually the center got so hot that it became a star, the Sun, and thus, blew most of the gas and dust of the new solar system with a strong stellar wind. The figure given below shows our solar system. This sets the horizontal scale (in AU). The picture has solar system with 9 different stars that are orbited by a planet. In the middle of the diagram the name of the star.
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