It is the nulei which fuse.
Nuclei are positively charged and thus repel each other. The kinetic energy of the nuclei must be very large for nuclei to be able to fuse, such as at the surface of the sun, where hydrogen nuclei fuse to form helium nuclei.
The strong nuclear force is the force that keeps the nucleus of an atom together. This force is stronger than the electromagnetic force, which tends to repel positive protons from each other in the nucleus.
The main reaction in the sun that produces energy is nuclear fusion. This process involves hydrogen atoms fusing together to form helium, releasing a large amount of energy in the form of light and heat.
Atoms do not collapse because of the balance between the electromagnetic force, which repels the positively charged protons in the nucleus, and the strong nuclear force, which holds the nucleus together. This balance keeps the atom stable and prevents it from collapsing.
Geothermal energy, generated from Earth's internal heat, does not depend on the sun. Nuclear energy, derived from splitting atoms or fusing them together, is another energy resource independent of solar radiation.
Welding is the process of joining two pieces of metal together by heating them to a high temperature and then fusing them together.
Hydrogen atoms are fusing into helium atoms in the Sun's core through the process of nuclear fusion. This fusion reaction releases a tremendous amount of energy that powers the Sun and produces light and heat.
Yes it does. It produces helium by fusing hydrogen
The state of matter that keeps atoms together is solid. Liquids and gases allow atoms to break apart from each other.
Our Sun, as with all main-sequence stars, is heated by the energy of fusing hydrogen atom to make helium atoms. The gigantic gravity of a main-sequence star causes hydrogen atoms to be smashed together, or 'fused'. The huge heat that results keeps the Sun puffed up to its huge size. In another 4.5 billion years, more or less, the hydrogen will be largely used up, and the Sun will shrink to a point that helium atoms are smashed together, creating lithium atoms. When all the lithium atoms have been largely smashed together and used up, the Sun will shrink again, and beryllium atoms will result.
The type of bond that keeps atoms close together but is considered very weak is the van der Waals force. It is an attractive force between uncharged particles.
technically speaking, stars are first made of Hydrogen. The moment the star comes to life, it starts fusing together Hydrogen atoms, forming helium. when a star is nearing the end of its life, it starts fusing together helium and keeps on fusing until there is nothing more to fuse. then, the star dies.
Fusing means to join two pieces of garments together. When garments are fused together, they become more supported and stabilized.
The fusing of hydrogen atoms into helium.
Helium atoms
in atomic science, fission is the splitting of atoms, fusion is the fusing of atoms
The force that keeps atoms together when they share electrons is called a covalent bond. In a covalent bond, atoms share electron pairs in order to achieve a more stable electron configuration. This sharing of electrons creates a strong attraction between the atoms, keeping them joined together in a molecule.
The sun's energy (and that of all other stars) comes from nuclear fusion. The nuclei of hydrogen atoms (ie protons) fuse together to produce helium and release energy.