Simple answer: Red Giant.
However, there are several stages to a red giant.
The most common form is a shell burning red giant, where hydrogen is still being fused into helium but in a shell rather than the core. The core is still inactive helium. This is a red giant branch (RGB) star.
The other form is a asymptotic giant branch (AGB) star where helium is fused to form carbon by the triple-alpha process.
So the detailed answer is a red giant but only when it is on the AGB.
Once a sun-like star has used up almost all of the hydrogen in it's core it will start to burn helium as well. This starts it's Red Giant phase which drastically increases the size of the star to hundreds of it's original size. Once the star has used up all available fuel it will contract down to the size of the Earth. While shedding it's outer layers into a Nebula. The Star is now a White Dwarf and will slowly fade into a Black Dwarf after trillions of years.
Stars "burn" with a process called nuclear fusion. This process fuses two hydrogen atoms in to one helium atom. Stars have a finite amount of hydrogen in them, hence when they consume it all, they run out of it.
A supergiant or red giant. They are normally around 3,500 degrees C and are very bright, near -5 on the Hertzsprung-Russell Diagram. These are the largest stars in the galaxy and universe.
It all depends on the mass and age of the original star.
When it has used up all its FUEL (energy supply), a star the mass of our Sun will turn into a white dwarf.
It shrinks and heats up.
It becomes a dwarf.
a white dwarf
Shrink
Yes, if the star is massive enough when the core collapses a supernova explosion happens.
As an average star is dying and the core is contracting when the temperature reaches 100 million Kelvin Helium atoms fuse into
A neutron star
A protostar is a star that is just beginning to form out of a stellar nebular (under gravity). The core of the gravitational collapse is getting more and more massive and is heating up as a result of the gravimetric contraction but has not yet reached the point where nucleosynthesis has begun in its core. It is when this happens that it becomes a star.
A supernova happens when most of the core of the collapsing star has become neutrons, held up against gravity by neutron degeneracy pressure. At this point a shockwave reflects from the neutron star surface, driving the supernova explosion.So the answer to your question is neutrons.
the star that is large and compact is a g-type sunlike star.
The rest of the star expands.
the answer is white dwarf
its clears air
It increases
The core collapses
If there is no hydrogen left at the core of star then hydrogen fusion cannot occur. What happens in the core of a star before that happens is that helium begins to fuse, and then the other elements going up the periodic table until carbon. And then if the star explodes into a supernova, traces of the higher elements are fused as well.
It becomes a white dwarf.
Its blown into interstellar space - to enrich and mix with the gasses already out there.
The core of a star is located inside the star in a region where the temperature and pressures are sufficient to ignite nuclear fusion, converting atoms of hydrogen into helium, and releasing a tremendous amount of heat.
Yes, if the star is massive enough when the core collapses a supernova explosion happens.
As an average star is dying and the core is contracting when the temperature reaches 100 million Kelvin Helium atoms fuse into