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2 most common scenarios:

1 - early universe was a cloud of gases (mainly hydrogen), so a certain part of the cloud starts to collapse dragging more and more gas by the force of gravity, enough for a gas planet to form, but not too much that a star forms.

2 - After a huge star burns out its fuel, it collapses or explodes in a huge supernova shooting off material containing all chemical elements. A planet might form from these material when they collapse under the force of gravity.

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What are the small bodies made of rock and ice that became the building blocks for planets called?

They are called planetesimals. These small bodies collided and merged to form larger bodies like planets and moons during the early stages of the solar system's formation.


What effect do collisions among planetesimals of greatly varying size have on the formation of planets?

Collisions among planetesimals of greatly varying size can lead to a process called accretion, where smaller planetesimals combine to form larger bodies. This can be a critical step in the formation of planets, as larger bodies have stronger gravitational pull and can continue to grow through further collisions. However, collisions with very large planetesimals could disrupt the growing planetesimal or lead to fragmentation, affecting the final size and composition of the resulting planets.


Collided to form planets?

Dust and gas particles in a protoplanetary disk collided and stuck together to form planetesimals, which then collided and accreted to form planets. The process of gravitational attraction and collisions led to the formation of larger bodies within the disk, eventually forming planets.


What does the protoplanet hypothesis describe the formation of?

The protoplanet hypothesis describes the formation of planets from the dust and gas present in the early solar system. It suggests that small planetesimals collided and merged to form larger celestial bodies, eventually leading to the creation of the planets we see today.


What substances existed as solid flakes within the inner 0.3 of the solar system before planets began to form?

I think that "0.3" is probably meant to be 0.3 AU. The answer is: the denser substances of the solar system which later formed the rocky inner planets. The gases were likely to form gas giant planets, further away from the Sun.

Related Questions

What collided to form planets with13 letters?

Planetesimals.


What are planetesimals and protoplanets and how are related to one another?

Planetesimals are small solid objects that form in the protoplanetary disk around a young star, while protoplanets are larger bodies that develop from the accumulation and collision of planetesimals. Planetesimals are the building blocks that come together to form protoplanets, and eventually, planets. So, planetesimals are like the "seeds" that grow into protoplanets.


What are the small bodies made of rock and ice that became the building blocks for planets called?

They are called planetesimals. These small bodies collided and merged to form larger bodies like planets and moons during the early stages of the solar system's formation.


What effect do collisions among planetesimals of greatly varying size have on the formation of planets?

Collisions among planetesimals of greatly varying size can lead to a process called accretion, where smaller planetesimals combine to form larger bodies. This can be a critical step in the formation of planets, as larger bodies have stronger gravitational pull and can continue to grow through further collisions. However, collisions with very large planetesimals could disrupt the growing planetesimal or lead to fragmentation, affecting the final size and composition of the resulting planets.


Why did earth start?

Rings of gas and dust orbiting stars may condense to form young planets or another term planetesimals. After this, it attracts more matter and increase in size to form planets. This is the basic steps of how planets was formed Dark matter ---->galaxy-------> star--------> planets


What causes dust clouds to form individual planets over time?

Dust clouds in space can gradually clump together due to gravitational attraction between particles, forming planetesimals. These planetesimals then collide and merge to form larger bodies, eventually accumulating enough mass to become planets. This process, known as accretion, is a key step in the formation of individual planets from dust clouds.


Collided to form planets?

Dust and gas particles in a protoplanetary disk collided and stuck together to form planetesimals, which then collided and accreted to form planets. The process of gravitational attraction and collisions led to the formation of larger bodies within the disk, eventually forming planets.


How the rocky inner planets were formed?

By "accretion" of "planetesimals" from the "protoplanetary disk".


What causes planetesimals to stay together forming planets when they collide?

Planetesimals stick together due to gravitational attraction and potentially other forces, such as electrostatic forces or chemical bonds. When two planetesimals collide with enough energy, they can merge and form larger bodies, eventually leading to the formation of planets. The exact mechanisms depend on factors like the size, composition, and relative velocities of the colliding bodies.


What is the difference between protoplanets and planetesimals?

Protoplanets are larger bodies in the process of forming into planets, usually by accreting material from a protoplanetary disk. Planetesimals are small celestial bodies that are precursors to planets, often ranging in size from meters to hundreds of kilometers and are believed to be building blocks for planets. Essentially, protoplanets are further along in the planet formation process compared to planetesimals.


Will the planets colide?

No, the solar system planets are all in stable orbits. That may not be the case for the asteroids, comets, and distant planetesimals.


Which process is necessary for the formation of a planet?

Planet formation occurs through the process of accretion, where dust and gas in a protoplanetary disk clump together to form planetesimals, and eventually planets. Gravity plays a crucial role in this process, pulling material together to form larger and larger bodies. Over time, these planetesimals collide and merge, forming planets.