In fusion engines we call stars, protons, which are hydrogen nuclei, are forced together and fused to create helium. This happens in early stellar life with the small- to medium-sized stars. When the protons are forced together, the first step involves fusing a pair of protons together with the weak interaction or weak nuclear force mediating the change of a proton into a neutron. Deuterium, or heavy hydrogen, is created. When deuterium reacts with a proton and the pair of particles are fused, a helium-3 nucleus is formed. From there, the reaction possibilities increase and we view what could occur along branches. This is the proton-proton chain reaction that is the basic process in stellar nucleosynthesis. The key to understanding these reactions is the knowledge of the ability of a proton to transform into a neutron through mediation by the weak nuclear force.
Hydrogen fusion occurs in stars to create helium. This process, known as nuclear fusion, involves the fusion of hydrogen nuclei to form helium nuclei, releasing large amounts of energy in the process.
Two hydrogen atoms can be combined through a nuclear fusion process to form a helium atom. This fusion process involves the two hydrogen atoms combining their nuclei to form a helium nucleus, releasing a large amount of energy in the process. This reaction is the core process that powers the sun and other stars.
nuclear fusion of hydrogen to form helium
It's called the proton-proton cycle. It's the source of the sun's energy. Also called nuclear fusion.
helium and some neutrons
hydrogen fusion
Hydrogen fusion occurs in stars to create helium. This process, known as nuclear fusion, involves the fusion of hydrogen nuclei to form helium nuclei, releasing large amounts of energy in the process.
Two hydrogen atoms can be combined through a nuclear fusion process to form a helium atom. This fusion process involves the two hydrogen atoms combining their nuclei to form a helium nucleus, releasing a large amount of energy in the process. This reaction is the core process that powers the sun and other stars.
nuclear fusion of hydrogen to form helium
It's called the proton-proton cycle. It's the source of the sun's energy. Also called nuclear fusion.
The most likely form of fusion to be successful on earth will be to produce helium from hydrogen isotopes. Helium has two protons and two neutrons in its nucleus.
Nuclear fusion converts hydrogen atoms into helium atoms. In the fusion process, hydrogen nuclei combine to form helium nuclei, releasing a large amount of energy in the form of heat and light.
Nuclear fusion, in which hydrogen-1 is fused into helium-4.
nuclear fusion
Helium is produced.
nuclear fusion!!
helium and some neutrons