two hydrogen atoms
Helium atoms in a star are formed through the process of nuclear fusion. In the core of a star, hydrogen atoms combine through a series of fusion reactions to form helium atoms. This happens when hydrogen atoms collide and fuse together, releasing energy in the process.
Normal "main sequence" stars fuse hydrogen into helium during most of the star's life. The core of a star gets so hot that the hydrogen atoms begin to fuse together. As hydrogen only has 1 proton when if fuses with another hydrogen atom it has 2 protons so has become helium.
The big bang produced the helium no present in the sun's core. The universe cooled down enough after the big bang to form the formation of helium and hydrogen.
Fusion of smaller atoms to form larger atome is a nuclear change. Ex: 4 hydrogen atoms FUSE to form an atom of helium through a compeles set of nuclear reactions.
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
In nuclear fusion, four hydrogen atoms fuse together to form one helium atom. This process releases a large amount of energy in the form of heat and light.
Hydrogen atoms fuse into helium.
The gas formed when hydrogen atoms fuse is helium. Stars do this.
Helium atoms in a star are formed through the process of nuclear fusion. In the core of a star, hydrogen atoms combine through a series of fusion reactions to form helium atoms. This happens when hydrogen atoms collide and fuse together, releasing energy in the process.
When hydrogen atoms fuse together in the sun's core, they create helium. This process releases energy in the form of light and heat, which provides the sun's power.
Oxygen is produced through repeated hydrogen fusion in stars. One such process would start with the hydrogen atoms fusing to form helium. And then the helium would fuse to form beryllium. That in turn would fuse to create oxygen.
fusion. Hydrogen atoms fuse together deep in the core to form helium atoms and release energy
Normal "main sequence" stars fuse hydrogen into helium during most of the star's life. The core of a star gets so hot that the hydrogen atoms begin to fuse together. As hydrogen only has 1 proton when if fuses with another hydrogen atom it has 2 protons so has become helium.
Hydrogen atoms fuse to become helium atoms during the process of nuclear fusion in stars. This process releases a large amount of energy and is the source of the sun's energy.
Yes. Hydrogen atoms fuse together to form helium - releasing heat as a by-product. The helium atoms migrate from the centre of the sun to its surface - reverting back to hydrogen as they do so. The cycle repeats itself.
When two hydrogen atoms fuse to become one helium atom.
When two hydrogen atoms fuse to become one helium atom.