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.
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.
Hydrogen and oxygen. On the sun two hydrogen atoms and one oxygen atom are fused at the core which keeps the suns light going and giving it more energy. The result of this is water. H2( hydrogen 2 ) O( oxygen ) h2o
The atoms in compounds are held together by chemical bonds
DNA is held together by hydrogen bonds between the nitrogenous bases adenine (A) and thymine (T), as well as cytosine (C) and guanine (G). These base pairs form the rungs of the DNA double helix, providing stability to the overall DNA structure.
A hydrogen molecule is held together by a covalent bond, where the two hydrogen atoms share their electrons in order to achieve a stable electron configuration. This shared pair of electrons creates a bond that keeps the atoms together.
there is infinity + atoms because atoms are mad out of atoms so it keeps going
The charge of the proton is positive while the charge of the electron is negative. This keeps the atom together. Unlike most atoms, the hydrogen atoms have only two particles in them.
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 state of matter that keeps atoms together is solid. Liquids and gases allow atoms to break apart from each other.
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.
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 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.
Becuase the Hydrogen bonds keeps the water atoms from separating until a high temperature is reached.
van der waals forces
very wet water. make sure it is wet. ALSO, it must have two atoms of hydrogen, and one atom of oxygen.
The sun produce energy when it converts hydrogen atoms into helium atoms in the core of the sun. This process will go on for as long as there is enough hydrogen to convert. In some larger stars, the process can also stop if the pressure of the converted atoms become too high. In this case, the sun may explode from the pressure itself into a super nova.