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What happened when the solar nebula began to collapse?

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.


The solar nebula was 98?

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.


What type of forces cuased the solar nebula to contract?

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.


What is the theoretical source of the nebula from which your solar system was formed?

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.


How did pressure and gravity become unbalanced in the solar nebula?

Pressure and gravitymay have become unbalanced in thesolar nebula because of an externalforce such as a collision of the solarnebula with another nebula or from anearby exploding star. This type offorce, was strong enough to overcomethe pressure of the nebula and triggerits collapse.

Related Questions

What happened when the solar nebula began to collapse?

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.


Which did not occur during the collapse of the solar nebula?

One of the events that did not occur during the collapse of the solar nebula was the formation of the first stars in the universe. Instead, the collapse of the solar nebula led to the formation of our solar system.


The solar nebula was 98?

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.


How did Earth form after the Big Bang?

Earth formed about 4.5 billion years ago from a cloud of gas and dust called the solar nebula. Gravity caused the nebula to collapse, forming the Sun at the center and the remaining material to clump together to form planets like Earth.


What type of forces cuased the solar nebula to contract?

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.


What formed at the center of our solar nebula?

The Sun.


Why did the solar system exist?

The solar system formed from a rotating cloud of gas and dust called the solar nebula about 4.6 billion years ago. Gravity caused this cloud to collapse and form the sun at its center, with the remaining material forming the planets, moons, asteroids, and other objects in the solar system.


The nebular hypothesis suggests that our solar system evolved from a huge?

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.


In the formation of our solar system nearly all the mass of the solar nebula became?

In the formation of our solar system, nearly all the mass of the solar nebula became the Sun, which accounts for about 99.86% of the solar system's total mass. The remaining material formed the planets, moons, asteroids, and comets. This process involved the gravitational collapse of the nebula, leading to the Sun's formation at the center, while the residual matter coalesced into the various celestial bodies orbiting it.


What is the theoretical source of the nebula from which your solar system was formed?

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.


How did pressure and gravity become unbalanced in the solar nebula?

Pressure and gravitymay have become unbalanced in thesolar nebula because of an externalforce such as a collision of the solarnebula with another nebula or from anearby exploding star. This type offorce, was strong enough to overcomethe pressure of the nebula and triggerits collapse.


The extra matter at the center of the solar nebula became the?

Inner planets