As the solar nebula began to collapse, gravity caused it to shrink and spin faster. This led to the formation of a protostar at the center, while the outer material flattened into a spinning disk. Within this disk, dust and gas started to clump together and eventually formed planetesimals, which further accreted to form planets.
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The force of gravity caused the solar nebula to contract. As the nebula collapsed under its own gravity, it began to spin and flatten into a disk shape, eventually forming the Sun and the planets. Additionally, the heat and pressure generated by the gravitational contraction contributed to the collapse of the nebula.
The solar nebula was a rotating cloud of gas and dust that formed our solar system about 4.6 billion years ago. It consisted mostly of hydrogen and helium, with traces of other elements. Over time, gravity caused the nebula to collapse and form the Sun and the planets.
A solar nebula begins to form when a cloud of gas and dust in space collapses under its own gravity. This collapse can be triggered by a nearby supernova explosion, a shockwave from a passing star, or other disturbances in the interstellar medium.
No, the solar nebula was primarily composed of hydrogen and helium, with trace amounts of other elements like carbon and iron. The solar system formed from the gravitational collapse of this nebula, leading to the formation of the Sun and planets.
The solar system formed from a spinning cloud of gas and dust called a nebula. Over time, this nebula collapsed under its own gravity to form the Sun and the rest of the solar system.