Red giant, then a planetary nebula, then 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.
After a planetary nebula occurs, the core of the star collapses and becomes a white dwarf. This white dwarf slowly cools down over billions of years until it eventually becomes a cold, dark remnant known as a black dwarf.
Star matter is recycled through various processes such as supernova explosions, where heavier elements are formed and released back into space, eventually becoming part of new stars, planets, and other celestial bodies. This recycling of star matter is essential for the creation of diverse elements and the continuation of the universe's evolution.
An average star like the Sun will eventually exhaust its nuclear fuel and expand into a red giant before shedding its outer layers to form a planetary nebula. What remains will be a dense core called a white dwarf, which will gradually cool over billions of years.
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.
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 cloud of dust that becomes a star forms through the process of gravitational collapse. As the dust particles come together, they begin to heat up and eventually ignite nuclear fusion, which results in the birth of a new star.
sup.
-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
After a planetary nebula occurs, the core of the star collapses and becomes a white dwarf. This white dwarf slowly cools down over billions of years until it eventually becomes a cold, dark remnant known as a black dwarf.
Star matter is recycled through various processes such as supernova explosions, where heavier elements are formed and released back into space, eventually becoming part of new stars, planets, and other celestial bodies. This recycling of star matter is essential for the creation of diverse elements and the continuation of the universe's evolution.
The mass of the star.
I don't know u answer it
An average star like the Sun will eventually exhaust its nuclear fuel and expand into a red giant before shedding its outer layers to form a planetary nebula. What remains will be a dense core called a white dwarf, which will gradually cool over billions of years.
Gravitational collapse is a crucial step in the process of star formation. When a cloud of gas and dust in space collapses under its own gravity, it becomes denser and hotter, eventually leading to the formation of a protostar. This gravitational collapse is what initiates the fusion reactions in the core of the protostar, eventually leading to the birth of a new star.
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.
after a nova star becomes bright it turns into a dwarf and explodes.