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).
A star that burns hydrogen quickly would typically generate more light than a star that burns hydrogen slowly. This is because a faster-burning star, usually more massive, undergoes nuclear fusion at a higher rate, producing greater energy output and luminosity. In contrast, a slower-burning star, often less massive, has a lower rate of fusion and thus emits less light. Therefore, the rate of hydrogen consumption directly influences the star's brightness.
A star that burns hydrogen quickly would generate more light than one that burns it slowly. This is because a faster fusion rate produces more energy in a shorter period, resulting in a higher luminosity. In contrast, a star that burns hydrogen slowly would have a lower energy output, leading to dimmer light. Therefore, the rate of hydrogen fusion directly impacts the star's brightness.
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.
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.
A star that burns hydrogen quickly would typically generate more light than a star that burns hydrogen slowly. This is because a faster-burning star, usually more massive, undergoes nuclear fusion at a higher rate, producing greater energy output and luminosity. In contrast, a slower-burning star, often less massive, has a lower rate of fusion and thus emits less light. Therefore, the rate of hydrogen consumption directly influences the star's brightness.
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.
A star that burns hydrogen quickly would generate more light than one that burns it slowly. This is because a faster fusion rate produces more energy in a shorter period, resulting in a higher luminosity. In contrast, a star that burns hydrogen slowly would have a lower energy output, leading to dimmer light. Therefore, the rate of hydrogen fusion directly impacts the star's brightness.
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.
YES, this happens when hydrogen burns. 2H2 + O2 ==> 2H2O
its clears air
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