No. In a red giant, fusion occurs in a shell around the core.
During the red giant phase, a star has typically exhausted the hydrogen in its core, leading to hydrogen fusion occurring in a shell surrounding the inert helium core. The outer layers of the star may still contain some hydrogen, but the core hinders further hydrogen fusion. The amount of hydrogen present varies depending on the star's mass and its evolutionary history, but it is significantly less than during the main sequence phase.
All red giant stars will start helium fusion when their core is compressed.
A red giant has been greatly inflated by the energy from nuclear fusion in a shell around the core. In a white dwarf fusion has stopped, the core has collapsed, and the low-density outer layers have been expelled into space.
A red giant core collapses primarily due to the exhaustion of nuclear fuel in its core, specifically helium after hydrogen has been depleted. As nuclear fusion slows, the outward pressure from fusion decreases, allowing gravity to dominate and compress the core further. This collapse raises the core's temperature and pressure until it can ignite the next stage of fusion, often leading to the formation of heavier elements. Eventually, this process can trigger a supernova explosion if the star is massive enough.
A star is a giant ball of hot gases that undergo nuclear fusion in its core. The intense pressure and temperature at the core of a star cause hydrogen atoms to fuse together to form helium, releasing a tremendous amount of energy in the process.
A red giant's core is called a helium core. This is because as a red giant forms, the core of the star contracts and heats up, causing hydrogen fusion to transition to helium fusion.
Nuclear Fusion in a Giant Star involves Helium being fused into a hydrogen shell that surrounds the core, and Nuclear Fusion in a Main-Sequence star involves Hydrogen being fused into Helium to produce Energy inside of the core.
None. Nuclear fusion occurs in stars. Jupiter, for example, has all the right ingredients to be a star but as huge as it is, it doesn't have enough mass to generate the heat and internal pressure facilitate nuclear fusion. Hope this helps :-)
The very center of the core, where nuclear fusion is occurring; millions of degrees.
Nuclear Fusion in a Giant Star involves Helium being fused into a hydrogen shell that surrounds the core, and Nuclear Fusion in a Main-Sequence star involves Hydrogen being fused into Helium to produce Energy inside of the core.
During the red giant phase, a star has typically exhausted the hydrogen in its core, leading to hydrogen fusion occurring in a shell surrounding the inert helium core. The outer layers of the star may still contain some hydrogen, but the core hinders further hydrogen fusion. The amount of hydrogen present varies depending on the star's mass and its evolutionary history, but it is significantly less than during the main sequence phase.
The energy output of the sun can be estimated based on the rate of nuclear fusion occurring in its core. This energy output is crucial for sustaining life on Earth and understanding the sun's role in the solar system.
Thermonuclear fusion is still going on in the core of a red giant, but it is a different type of thermonuclear fusion. The center of the core has reached high enough temperature and pressure that it can now burn helium, producing carbon. 3 4He --> 12C The large amount of energy released by this type of fusion pushes the outer layers away, making a giant star. The expansion of volume of the surface layer causes it to cool, appearing red. Thus a red giant.
Like all stars, Betelgeuse emits light because it is very hot. The heat for that light comes from nuclear fusion reactions occurring in the star. Unlike in most other stars, the fusion is occurring in a shell around the core rather than in the core itself.
All red giant stars will start helium fusion when their core is compressed.
A red giant has been greatly inflated by the energy from nuclear fusion in a shell around the core. In a white dwarf fusion has stopped, the core has collapsed, and the low-density outer layers have been expelled into space.
A red giant core collapses primarily due to the exhaustion of nuclear fuel in its core, specifically helium after hydrogen has been depleted. As nuclear fusion slows, the outward pressure from fusion decreases, allowing gravity to dominate and compress the core further. This collapse raises the core's temperature and pressure until it can ignite the next stage of fusion, often leading to the formation of heavier elements. Eventually, this process can trigger a supernova explosion if the star is massive enough.