Red giant, then a planetary nebula, then a white dwarf.
A white dwarf.
In fact, the sun is not massive. It is an average, yellow star. When the sun goes into its next stage, it becomes a red giant. This could consume the whole solar system. Then, when it burns out, the gases escape into space, and it becomes a little tiny star called a white dwarf. Eventually it will burn out, and that's how the sun's lifecycle works.
A star eventually uses up all of it's hydrogen in nuclear fusion. They fusion of hydrogen into helium is what makes the star glow bright and hot. When all the helium is fused, the star collapses inward on itself, and becomes a small "white dwarf" star, essentially a pile of "stellar embers". That's the end of a star's life.
a star explodes or becomes a white dwarf, then the matter of that star becomes other things.
It loses its outer layers because it has expanded to the point where gravity can no longer hold it together. The inner part of the star becomes a white dwarf, called a white dwarf because it is still glowing with the remaining heat of the dead star. It eventually becomes a black dwarf, where it has radiated all its energy out and no longer glows.
Eventually, yes. A mid-size star becomes a white dwarf, which eventually cools to become a black dwarf.
A white dwarf.
In fact, the sun is not massive. It is an average, yellow star. When the sun goes into its next stage, it becomes a red giant. This could consume the whole solar system. Then, when it burns out, the gases escape into space, and it becomes a little tiny star called a white dwarf. Eventually it will burn out, and that's how the sun's lifecycle works.
-average size -expands and becomes a red giant -cools and contracts, becomes a white dwarf star -massive sized stars -swell and become red supergiants -explode (called a supernova) -become a black hole -become a neutron star
sup.
A star eventually uses up all of it's hydrogen in nuclear fusion. They fusion of hydrogen into helium is what makes the star glow bright and hot. When all the helium is fused, the star collapses inward on itself, and becomes a small "white dwarf" star, essentially a pile of "stellar embers". That's the end of a star's life.
a star explodes or becomes a white dwarf, then the matter of that star becomes other things.
It loses its outer layers because it has expanded to the point where gravity can no longer hold it together. The inner part of the star becomes a white dwarf, called a white dwarf because it is still glowing with the remaining heat of the dead star. It eventually becomes a black dwarf, where it has radiated all its energy out and no longer glows.
The mass of the star.
I don't know u answer it
Earth's sun is currently a main sequence star which has a small mass. Eventually it will expand into Red Giant star once the core runs out of hydrogen and then helium gas. After the Red Giant phase, the star throws off its outer layers and then becomes a planetary nebula. A sun-like star will either become a white dwarf or black dwarf following the planetary nebula.
after a nova star becomes bright it turns into a dwarf and explodes.