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Nebulae begin to contract primarily due to gravitational forces. A disturbance, such as shock waves from nearby supernovae or collisions with other gas clouds, can trigger this contraction. As the gas and dust within the nebula clump together, gravitational attraction increases, leading to further collapse and the eventual formation of stars and planetary systems. Additionally, the cooling of the gas can enhance the process by allowing particles to come closer together.

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What causes the gas and dust in a nebula to contract?

Gravity.


When the pressure and temperature of a nebula increases what is formed?

When the pressure and temperature of a nebula increase, it can lead to the formation of protostars. As gravity causes the nebula to contract and heat up, eventually nuclear fusion can begin at the core of the protostar, leading to the formation of a new star.


What causes a solar nebula initially begin to form a solar system?

An explosion from outside the nebula


What causes solar nebula to begin to form a solar system?

Gravity.


What is a force that causes a nebula to contract?

A key force that causes a nebula to contract is gravity. The mass of the gas and dust within the nebula generates gravitational attraction, pulling particles closer together. As these particles coalesce, their density increases, leading to further gravitational collapse. Additionally, other factors such as shock waves from nearby supernovae can trigger the contraction process by compressing the nebula.


What force causes nebula to collapse?

Gravity is the force that causes nebulae to collapse. As particles within the nebula are pulled together by gravity, they begin to clump and form denser regions. This leads to the eventual formation of stars and planetary systems within the collapsing nebula.


Why would the nebula begin to contract?

A nebula begins to contract due to gravitational forces overcoming the pressure from its internal gas and dust. As the material within the nebula begins to clump together, the gravitational attraction increases, leading to further contraction. This process can be triggered by external factors such as shock waves from nearby supernovae or collisions with other clouds, which can compress the nebula and initiate star formation. As the nebula contracts, it can lead to the formation of stars and planetary systems.


Is a nebula held together of the outward force of gravity?

Yes, a nebula is held together by gravity. Gravity causes the gas and dust within a nebula to contract and clump together, eventually forming stars and other celestial bodies.


Why do nebula begin to contract?

Nebulae begin to contract primarily due to gravitational forces. As gas and dust within the nebula clump together, their gravitational attraction pulls more material inward, increasing density and temperature. This process can be triggered by external factors, such as shock waves from nearby supernovae or interactions with other cosmic structures, which compress the material and initiate star formation. As the nebula contracts, it may eventually lead to the formation of new stars and planetary systems.


What is matter from nebula that has begun to condense under the weight of gravity to begin formation of star?

The matter from a nebula that has begun to condense under gravity to form a star is called a protostar. As gravity causes the protostar to contract, the core temperatures rise until nuclear fusion ignites, and a star is born. This marks the transition from a cloud of gas and dust to a shining star.


What force causes a nebula to become a star?

Gravitational attraction pulls gas and dust together in a nebula, causing it to condense and heat up. When the pressure and temperature in the core of the nebula become high enough, nuclear fusion reactions begin, initiating the process of becoming a star.


What causes a solar nebula to initially begin to form a solar?

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.