Thermonuclear reactions only occur in the core of the star because that's where the heat and pressure is so great that it overcomes the forces between the atoms. The surface stars is relatively cool. The Sun is only around 10,000° F on its surface. well below the several million degrees required for fusion.
Nuclear fusion requires large temperatures and pressure, which are only present in the core of a star.
Nuclear fusion occurs at the core of the sun as this is were it is hot enough for the positively charged nuclei to overcome the repelling nature and fuse together.
Because suns are like onions, they both have layers.
The Sun's core is hotter, and at a higher pressure, than the outer layers. I assume there is a very small amount of fusion in the outer layers, but not enough to make a real difference.
No. Hydrogen fusion occurs in the star's core.
When a main sequence star, such as our sun, exhausts it's supply of Hydrogen, fusion of Hydrogen to Helium ceases in the core. This results in cooling of the core and therefore causes it to contract. As the core contracts, the layers surrounding the star gain kinetic energy until the fusion of Hydrogen is possible in the outer layers. As these layers undergo fusion, they increase in temperature dramatically. The outer layers expand due to heat, and the star becomes massive; the main sequence star has evolved into a red giant. Fusion of Hydrogen to Helium continues in the outer layers, whilst the fusion of heavier elements such as carbon occurs in the core.
Nuclear fusion occurs in the solar core.
Near the core (center).Near the core (center).Near the core (center).Near the core (center).
material is hotter and denser
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The Sun's core is hotter, and at a higher pressure, than the outer layers. I assume there is a very small amount of fusion in the outer layers, but not enough to make a real difference.
Fusion occurs in the core of the sun and other stars.
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Fusion occurs in the core of the Sun
No. Hydrogen fusion occurs in the star's core.
In all stars, the fusion only occurs in the inner core.
When a main sequence star, such as our sun, exhausts it's supply of Hydrogen, fusion of Hydrogen to Helium ceases in the core. This results in cooling of the core and therefore causes it to contract. As the core contracts, the layers surrounding the star gain kinetic energy until the fusion of Hydrogen is possible in the outer layers. As these layers undergo fusion, they increase in temperature dramatically. The outer layers expand due to heat, and the star becomes massive; the main sequence star has evolved into a red giant. Fusion of Hydrogen to Helium continues in the outer layers, whilst the fusion of heavier elements such as carbon occurs in the core.
High temp and pressure
Nuclear fusion occurs in the solar core.
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.
There is no fire in the sun, that is a chemical process. The process in the core is thermonuclear fusion.