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Hydrogen (essentially a proton-proton reaction)
The proton-proton chain is the name given to one common fusion reaction occurring in stars by which hydrogen is converted to helium, along with the release of energy.
The mass of the star and the related temperature of the stellar core determine the thermonuclear process type of the star. The stars of the solar mass produce energy from Hydrogen in the proton-proton cycle (two and three proton nuclei appear in intermediate stages of the fusion, end product is Helium); stars twice (or more) as heavy run the HNC cycle (Although Helium is here still the end product, Nitrogen and Carbon appear in intermediate fusion stages, too). Once the Hydrogen is used up, gravity collapse makes the temperatures rise until the next , heavier element fusion cycle is activated. As the temperature rises, other numerous fusion cycles can produce all existing elements. The heaviest ones are created in the extraordinary high temperatures of the supernovae-explosions
No, this is the fusion reaction which occurs in the sun and other stars. See the link below.
Nuclear fusion. We call the activity stellar nucleosynthesis. The proton-proton chain results in the fusion of helium from the hydrogen that makes up most of the sun. A link is provided to the Wikipedia articles on the sun (specifically its core) and on the proton-proton chain.
Through an internal thermonuclear fusion reaction, the sun uses four protons in a process called the proton-proton chain which results in the release of two positrons, two neutrinos, two gamma rays, helium, and energy.
Through an internal thermonuclear fusion reaction, the sun uses four protons in a process called the proton-proton chain which results in the release of two positrons, two neutrinos, two gamma rays, helium, and energy. electromagnetic radiation
I can't remember if it is the proton-proton chain or if it's the CNO cycle... i'm pretty sure it's the CNO cycle, but i'm not 100% sure.
The proton-proton chain is the name given to one common fusion reaction occurring in stars by which hydrogen is converted to helium, along with the release of energy.
Hydrogen (essentially a proton-proton reaction)
The mass of the star and the related temperature of the stellar core determine the thermonuclear process type of the star. The stars of the solar mass produce energy from Hydrogen in the proton-proton cycle (two and three proton nuclei appear in intermediate stages of the fusion, end product is Helium); stars twice (or more) as heavy run the HNC cycle (Although Helium is here still the end product, Nitrogen and Carbon appear in intermediate fusion stages, too). Once the Hydrogen is used up, gravity collapse makes the temperatures rise until the next , heavier element fusion cycle is activated. As the temperature rises, other numerous fusion cycles can produce all existing elements. The heaviest ones are created in the extraordinary high temperatures of the supernovae-explosions
The proton-proton chain accounts for more than 98% of the fusion reactions in our Sun. The balance in the carbon-nitrogen-oxygen catalytic chain reaction.
No, this is the fusion reaction which occurs in the sun and other stars. See the link below.
The Sun produces energy by nuclear fusion. It follows the steps of the proton-proton(P-P) chain, which converts hydrogen to helium. The core of the Sun produces about 99% of heat through fusion.
The Sun produces energy by nuclear fusion. It follows the steps of the proton-proton(P-P) chain, which converts hydrogen to helium. The core of the Sun produces about 99% of heat through fusion.
The helium nucleus is formed during the proton-proton reaction by the fusion of four protons. Two of the protons are converted to neutrons by the weak interaction.
Nuclear fusion. We call the activity stellar nucleosynthesis. The proton-proton chain results in the fusion of helium from the hydrogen that makes up most of the sun. A link is provided to the Wikipedia articles on the sun (specifically its core) and on the proton-proton chain.