It caused the solar system to form in the shape of a disk.
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.
rotating clouds mademostly of helium & hydrogen
A solar nebula is a rotating cloud of gas and dust from which the sun and planets formed. I hope this helps :))
The hypothesis on how the solar system was formed is known as the solar nebula theory. This theory posits that the solar system formed from a massive, rotating cloud of gas and dust called the solar nebula. Over time, gravity caused the material in the nebula to clump together, eventually forming the sun and the planets.
The theoretical source of the nebula from which our solar system was formed is a solar nebula, a rotating cloud of gas and dust. This nebula likely originated from the remnants of older stars that exploded in supernovae, enriching the surrounding interstellar medium with heavy elements. Over time, gravitational forces caused the nebula to collapse, leading to the formation of the Sun and the surrounding planets through a process called accretion. This event is theorized to have occurred about 4.6 billion years ago.
Because the star that blew it off of itself was rotating. Conservation of rotational momentum.
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.
rotating clouds mademostly of helium & hydrogen
A solar nebula is a rotating cloud of gas and dust from which the sun and planets formed. I hope this helps :))
The hypothesis on how the solar system was formed is known as the solar nebula theory. This theory posits that the solar system formed from a massive, rotating cloud of gas and dust called the solar nebula. Over time, gravity caused the material in the nebula to clump together, eventually forming the sun and the planets.
The theoretical source of the nebula from which our solar system was formed is a solar nebula, a rotating cloud of gas and dust. This nebula likely originated from the remnants of older stars that exploded in supernovae, enriching the surrounding interstellar medium with heavy elements. Over time, gravitational forces caused the nebula to collapse, leading to the formation of the Sun and the surrounding planets through a process called accretion. This event is theorized to have occurred about 4.6 billion years ago.
A rotating cloud of gas and dust that formed into the Sun and planets is called a solar nebula. This nebula collapsed under its own gravity, leading to the formation of the Sun at its center and the planets in the surrounding disk. The process of accretion within this rotating cloud eventually resulted in the diverse bodies of our solar system.
The nebular hypothesis suggests that our solar system evolved from a huge rotating cloud of gas and dust called a solar nebula. Over time, gravity caused the nebula to collapse and spin faster, forming the sun at the center and the planets and other objects in orbit around it. This process is supported by evidence from observations of other star systems and the composition of our own solar system.
The Crab Nebula was formed when it's host star exploded as a supernova [See related question]
The nebular model explains how our solar system formed from a rotating cloud of gas and dust called a solar nebula. Gravity caused the nebula to collapse, forming a central protostar surrounded by a spinning disk. Over time, the material in the disk clumped together to form planets and other solar system bodies.
1) The collapse is not bound to be perfectly symmetrical. Some pieces of matter will randomly move in one direction, or in another. The net result is that there is some rotation.2) Roughly speaking, anything that rotates will continue rotating.
The pressure caused by the thermal energy of the gas within the nebula pushes outward in all directions, preventing the nebula from collapsing under its own gravity. This pressure acts to counterbalance the force of gravity, maintaining the nebula's size and structure.