Sort of disc-shaped with a lump, like one of those "dog frisbees" with the ball in the middle and the rings around it.
A solar nebula is a rotating cloud of gas and dust from which the sun and planets formed. I hope this helps :))
rotating clouds mademostly of helium & hydrogen
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.
the material to flatten into a disk shape due to centrifugal forces. This conservation of angular momentum led to the formation of the solar system as we know it, with the Sun in the center and the planets orbiting in a plane.
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.
A solar nebula is a rotating cloud of gas and dust from which the sun and planets formed. I hope this helps :))
rotating clouds mademostly of helium & hydrogen
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.
the material to flatten into a disk shape due to centrifugal forces. This conservation of angular momentum led to the formation of the solar system as we know it, with the Sun in the center and the planets orbiting in a plane.
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 motions of the Sun and the planets reflect to disk shape of the solar nebula because they follow the same rotation as this disk shape. The rotation of the Sun and the planets is not a perfect circle.
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 hypothesis you're referring to is the Nebular Hypothesis. It proposes that the solar system formed from a giant rotating cloud of gas and dust, known as a solar nebula. As this nebula collapsed under its own gravity, it spun faster and flattened into a disk, leading to the formation of the Sun at its center and the planets from the surrounding material. This process explains the structure and composition of the solar system as we observe it today.
The theory that explains the formation of planets through the condensing of a solar nebula is known as the Solar Nebula Theory. According to this theory, the solar system originated from a rotating cloud of gas and dust, known as the solar nebula. As the nebula collapsed under its gravity, it spun faster and flattened into a disk, allowing particles to collide and stick together, eventually forming larger bodies that became the planets. This process highlights the role of gravity and angular momentum in the formation of celestial bodies.
A solar nebula is related to the formation of our Solar System, any other nebula is just a nebula.
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 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.