It increases
The rest of the star expands.
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 contracts under the force of its own gravity. This contraction increases the temperature in the core.
The rest of the star expands.
its clears air
The core collapses
It becomes a white dwarf.
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.
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
The temperature in the core of a star depends, to a great extent, on:* The star's mass. The general tendency is that high-mass stars are hotter. * Where the star is in its life cycle. The star's core temperature will vary over time. On the other hand, the star's surface temperature also depends on its size. Thus, it is possible that PRECISELY because a star is hotter in the core, it gets bigger, and the surface temperature DECREASES (though its total energy output increases).
When a star uses the hydrogen in its core it will start burning hydrogen in a shell around the core and become a red giant. After that the star will either collapse into a white dwarf or start fusing helium, depending on its mass.
The core of a star contracts under the force of its own gravity. This contraction increases the temperature in the core.