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When a high mass star collapes why doesnt it rekindle?
Because all the material that could rekindle it has run out - there is none left.
Why is the center of a collapsing nebula forms a star?
When a nebula collapses due to gravitational forces, the center becomes denser and hotter. As the material in the center becomes more compact, the pressure and temperature increase, eventually triggering nuclear fusion reactions that sustain a star's energy. This marks the birth of a new star in the center of the collapsing nebula.
What may form as a direct result of the star collapsing?
A direct result of a star collapsing could be the formation of a black hole. This occurs when the core of a massive star collapses under its own gravity, creating a region of space with such strong gravitational pull that not even light can escape.
What does the equilibruim between the outward pressures of radiaion and the force of gravity do?
The equilibrium between the outward pressure of radiation and the force of gravity in stars enables them to maintain their size and shape. This balance prevents the star from collapsing under its own gravity or expanding due to the radiation pressure, allowing it to remain stable over a long period of time.
What is a star that has been exhausted of its supply of hydrogen?
A star that has exhausted its supply of hydrogen will evolve into a red giant or supergiant, depending on its initial mass. Eventually, it may undergo a helium flash and fusion of heavier elements before collapsing into a white dwarf or supernova.
How were dark holes made?
An old star collapsing in on itself, to put it in simple terms.
When a high mass star collapes why doesnt it rekindle?
Because all the material that could rekindle it has run out - there is none left.
What star is Explosion created by a rapidly collapsing star?
Super nova
What does the equilibrium between the outward pressures of radiation and the force gravity do?
"While the star can produce energy, that keeps the star in balance - it keeps the star from collapsing. By the way, another outward force is the gas pressure, but that, by itself, is not enough to counteract the force of gravity in the case of a star."
How did the first black hole start?
By a Star collapsing on its self.
The balance of forces that keeps a star from collapsing is called .?
hydrostatic
What do you call the death of a star?
The death of a star is called a supernova or stellar explosion. This is a catastrophic event that occurs when a star reaches the end of its life cycle and can result in the star either collapsing into a dense core (neutron star or black hole) or completely exploding.
When The balance of forces that keep a star from collapsing is called?
The balance of forces that keep a star from collapsing is called hydrostatic equilibrium. This equilibrium is maintained between the inward force of gravity and the outward force generated by gas pressure within the star.
What do you call The balance of forces that keeps a star from collapsing?
Dynamic equilibrium.
Why is the center of a collapsing nebula forms a star?
When a nebula collapses due to gravitational forces, the center becomes denser and hotter. As the material in the center becomes more compact, the pressure and temperature increase, eventually triggering nuclear fusion reactions that sustain a star's energy. This marks the birth of a new star in the center of the collapsing nebula.
What may form as a direct result of the star collapsing?
A direct result of a star collapsing could be the formation of a black hole. This occurs when the core of a massive star collapses under its own gravity, creating a region of space with such strong gravitational pull that not even light can escape.
What does the equilibruim between the outward pressures of radiaion and the force of gravity do?
The equilibrium between the outward pressure of radiation and the force of gravity in stars enables them to maintain their size and shape. This balance prevents the star from collapsing under its own gravity or expanding due to the radiation pressure, allowing it to remain stable over a long period of time.
