The star first expands into a red giant (or a supergiant star if the original star was a giant star) and then explodes in a fusion flash (sun-size star), nova (slightly larger), or supernova (for a supergiant).
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.
A main sequence star burns hydrogen to helium. Once a main sequence star exhausts all of the hydrogen, it begins to expand and burn helium causing if to become a red giant.
Nuclear fusion, converting hydrogen nuclei into helium nuclei.
Stars convert hydrogen into helium over time.However, please note that they do so at very different rates; a massive star burns its fuel (hydrogen) much faster than a less massive star - so you can well have a massive star, which is only a few million years old, but which already burnt much of its fuel.
When a star burns up all of its hydrogen,it becomes red in color.As hydrogen is the fuel for star and it will burst after it.
When a star runs out of hydrogen fuel in its core, nuclear fusion slows down and the core contracts while the outer layers expand. The star becomes a red giant as it fuses heavier elements in its shell, until eventually it sheds its outer layers forming a planetary nebula, leaving behind a dense core known as a white dwarf.
it dies out (burns out)
Hydrogen "burns" as it were, in "nuclear fusion" reactions to give helium and release energy.
The defining characteristic of a main sequence star burns hydrogen to helium in its core.
After a star burns up all it's hydrogen, it becomes a red giant.
its clears air
YES, this happens when hydrogen burns. 2H2 + O2 ==> 2H2O
it burns and seperates actually it burns and oxygen burns it , methane is the gas that we mostly use in southern countries for cooking
because the star burns and fuses hydrogen and helium (like the sun) making heat an light
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.