Within the atomic nucleus, two hydrogen nucleii (single protons in only this case) fuse to form a single helium nucleus.
On The Larger Scale this occurs always in Stars.
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.
The primary atomic reaction that occurs on the sun is nuclear fusion, specifically the fusion of hydrogen atoms to form helium. This process releases a large amount of energy in the form of light and heat.
The nuclear fusion order for a star like our Sun involves the conversion of hydrogen into helium. This fusion process occurs in multiple stages, beginning with the fusion of hydrogen isotopes (protons) into deuterium, and then further reactions combine deuterium to form helium-3 and, ultimately, helium-4.
In a star's nuclear reactions, hydrogen is converted into helium. This process, known as nuclear fusion, occurs in the core of a star, where high temperatures and pressures cause hydrogen atoms to combine to form helium.
The process is called nuclear fusion. It occurs in the core of stars, including our sun, where hydrogen atoms combine to form helium, releasing energy in the form of light and heat.
Nuclear fusion in the sun occurs when hydrogen atoms combine to form helium atoms. This process releases large amounts of energy in the form of photons. The intense pressure and temperature in the sun's core create the conditions necessary for nuclear fusion to occur.
Hydrogen undergoes nuclear fusion to form helium in a process that releases a large amount of energy. This process is the main source of energy for stars, including our Sun. The newly formed helium atom is more stable than the original hydrogen atoms.
In the sun, nuclear fusion reactions convert hydrogen into helium, releasing large amounts of energy in the form of heat and light. This process is the transformation of nuclear energy into thermal and electromagnetic energy.
Nuclear Fusion
nuclear fusion
The source of the sun's energy is nuclear fusion, which occurs in its core. This process involves the fusion of hydrogen atoms to form helium, releasing a tremendous amount of energy in the form of light and heat.
Its called as nuclear fusion. The nucleus of hydrogen atoms fuse together and form helium nucleus. There is some difference of the two masses resulting it to become energy by Einstein's formulae e=mc^2