Theoretically, yes, it could be split into 2 of the Deuterium isotype (1 proton, 1 neutron). However this would generate colossal energy, as the process is similar to that of an atomic bomb, only on a smaller scale (uranium has a lot more protons and neutrons to split).
They are fused into helium and create energy. But it takes 4 hydrogen atoms to make 1 atom of helium. The Hydrogen is first converted to Deuterium (heavy hydrogen), and the two deuterium atoms fuse to make the Helium atom. This process releases a lot of energy, not the least because of the neutrons released. Lol
boob
Helium
The bond holding the diatomic molecule of hydrogen (which exists in hydrogen gas) is a single covalent bond. This is the sharing of one electron in their 1s orbital, forming an stable electron that of helium: 1s2
Acetyl is a chemical made up of nitrogen and two hydrogen atoms
two hydrogen atoms
The sun produces energy by fusing hydrogen atoms into helium atoms. This is a nuclear fusion that occurs at the sun's core.
hydrogen and helium
When two hydrogen atoms fuse to become one helium atom.
When two hydrogen atoms fuse to become one helium atom.
The hydrogen nucleus has a single proton. The helium nucleus has two protons and one or two neutrons.
This is the fusing of hydrogen atoms to form helium atoms, and in some cases heavier elements as well. The dominant reaction in our Sun is the combining of hydrogen isotope atoms to form helium atoms. Deuterium atoms, which are hydrogen atoms which have a neutron, are forced together to form a helium atom, which is two protons and two neutrons, and some energy is produced. The Sun is slowing using up its supply of hydrogen, but there is enough to last for at least another two or three billion years.
yes
The fusion of two hydrogen atoms yielding a helium atom expels a large amount energy.
Water is chemically H2O and there is no helium (He) in water. Water has two hydrogen atoms and one oxygen atom.
It's called the proton-proton cycle. It's the source of the sun's energy. Also called nuclear fusion.
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.