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.
When a large star runs out of fuel, it undergoes a supernova explosion, where the core collapses and releases a huge amount of energy. The outer layers are expelled into space, forming a nebula, while the core either forms a neutron star or a black hole, depending on its mass.
The rest of the star expands.
When a star exhausts its hydrogen fuel in the core, nuclear fusion ceases, leading to a drop in outward pressure. This causes the core to collapse under gravity, increasing temperature and pressure until it becomes hot enough to fuse helium into heavier elements. As the core contracts, the outer layers may expand and cool, often transforming the star into a red giant. Eventually, this process leads to the star's evolution into later stages, such as a supernova or a white dwarf, depending on its mass.
The main factor that causes a star like the Sun to evolve away from being a main sequence star is the depletion of hydrogen fuel in its core. As the hydrogen fuel is used up, the core contracts and heats up, leading to the outward expansion of the star's outer layers. This expansion and change in structure lead the star to evolve into a red giant.
Neutron stars do not have fuel. A neutron star is a remnant of a star that has already died.
When a large star runs out of fuel, it undergoes a supernova explosion, where the core collapses and releases a huge amount of energy. The outer layers are expelled into space, forming a nebula, while the core either forms a neutron star or a black hole, depending on its mass.
As a star ages and runs out of fuel in its core, it can expand in size as it transitions into a red giant. During this phase, fusion reactions occur in the outer layers of the star, causing it to expand and cool. This expansion happens when the star exhausts its hydrogen fuel and begins fusing helium in its core.
The rest of the star expands.
A star's core consists mostly of hydrogen. As the star ages, the amount of helium, carbon and other elements in the core increases as they are the result "ash" resulting from the consumption of the hydrogen fuel.
When a star exhausts its hydrogen fuel in the core, nuclear fusion ceases, leading to a drop in outward pressure. This causes the core to collapse under gravity, increasing temperature and pressure until it becomes hot enough to fuse helium into heavier elements. As the core contracts, the outer layers may expand and cool, often transforming the star into a red giant. Eventually, this process leads to the star's evolution into later stages, such as a supernova or a white dwarf, depending on its mass.
The main factor that causes a star like the Sun to evolve away from being a main sequence star is the depletion of hydrogen fuel in its core. As the hydrogen fuel is used up, the core contracts and heats up, leading to the outward expansion of the star's outer layers. This expansion and change in structure lead the star to evolve into a red giant.
Neutron stars do not have fuel. A neutron star is a remnant of a star that has already died.
its clears air
Towards the end of its life, a star with a size similar to ours will expand to a red giant star as the core contracts and heats up and the hydrogen fuel supply is consumed. It will eventually lose the outer layers and all that will be left is a core, a white dwarf reminant that will slowly cool over millions of years.
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.
When a star exhausts its core hydrogen fuel, it begins to fuse heavier elements like helium, carbon, and oxygen. This fusion process generates more energy in the core and causes the star to expand and become a huge star. This stage is known as a red giant or supergiant.
When a star exhausts its hydrogen fuel, it can no longer sustain the nuclear fusion processes that power it. As a result, the core contracts and heats up, eventually leading to the fusion of heavier elements like helium. This causes the outer layers of the star to expand, transforming it into a red giant. Eventually, the star may shed its outer layers, resulting in a planetary nebula, while the core remains as a white dwarf.