During the Red Giant stage, all the hydrogen of the star will be used up and helium will start to fuse.
Because helium burning reactions are extremely sensitive to temperature, this causes great instability. Massive pulsations build up, which eventually causes the outer layers to be ejected, potentially forming a planetary nebula.
At the center of the nebula remains the core of the star, which will cool down to become a white dwarf.
white dwarf
A white dwarf is a star that is dying and is in its final evolutionary stage.
white dwarf. unless you count black dwarf of which none have been observed, only theorized.
Before a white dwarf, a star would undergo the red giant phase. After a white dwarf, a star may end its life cycle as a black dwarf, although no black dwarfs are currently known to exist in the universe due to the long timescales required for a white dwarf to cool down.
False. The sun is a yellow main sequence star.
white dwarf
The Neutron stage follows the White Dwarf stage of star development.
the next stage of a white dwarf is the black dwarf which is form when the degenerate electron slowly cools down by thermal radiation but the time required for a white dwarf to become a black dwarf is bigger than the current age of universe so the evidence of a black dwarf isn't found yet
No, the sun will eventually evolve into a red giant before shedding its outer layers and becoming a white dwarf. The white dwarf stage marks the end of its evolution, where it will slowly cool down over billions of years.
A white dwarf is the death of a medium sized star - similar to our own Sun.
A white dwarf is a star that is dying and is in its final evolutionary stage.
White Dwarf then Black Dwarf=Dead Star
white dwarf/nova
white dwarf
white dwarf. unless you count black dwarf of which none have been observed, only theorized.
Before a white dwarf, a star would undergo the red giant phase. After a white dwarf, a star may end its life cycle as a black dwarf, although no black dwarfs are currently known to exist in the universe due to the long timescales required for a white dwarf to cool down.
The sun's life cycle includes the stages of formation, main-sequence, red giant, and white dwarf. It is currently in the main-sequence stage, where it fuses hydrogen into helium in its core. Eventually, it will expand into a red giant before shedding its outer layers and becoming a white dwarf.