
Neutral atoms can still interact with each other. When close enough, some pairs of atoms link up to form molecules joined together by a bond. By sharing electrons, the atoms are able to complete their outermost shells and become more stable.
The only atoms that have filled outer electron orbitals are those of Group 8, the noble atoms. All other neutral atoms are called 'radicals' and have some unfilled outer orbital. This allows for the possibility that an external electron moves into that orbital. When two atoms come close to each other, their outer
The presence of other atoms may alter the other orbitals' energy, possibly enough to shift an electron from one orbital to another and affecting the valence. For example,
When two atoms' orbitals overlap, they split into two orbitals, one has a lower energy, thus an attracting
The simplest bonds are those between similar atoms. Below are the most common types of such bonds and anti-bonds, either axial, termed σ (sigma), or 'planar', termed π (pi). As two atoms approach each other, their orbitals modify as follows:
Each full bond decreases the molecules' energy by about
Dissimilar atoms with different energy levels of orbitals vary in the way they combine their orbitals;
Partially filled bonds are unstable, allowing interactions with further electrons.
Each bond vibrates longitudinally with a natural frequency that depends on the bond energy and the atoms' masses, about
A
The average bond energies between atoms are as follows:
Note that the average bond energy in general is larger for smaller atoms and for single bonds of different sizes, but is weaker for double/triple bonds between atoms of different sizes. Actual bond energies vary depending on the molecule.
Different atoms attract the electrons in a covalent bond with different amounts. Like most other properties of atoms, this varies 'diagonally' from
Between atoms of different electronegativity, the orbitals are weighted towards one of the atoms, skewing the bond to one atom. The resulting skewed bond is called a polar bond.
Also when an
Molecules with polar bonds are effectively electric dipoles with a large moment. An electric field turns them in about
A symmetric bond, on the other hand, acts not like a dipole but like a quadrupole or weaker, and is not affected by microwaves.
When the electro-negativity difference between the two atoms is large, one or more electrons from the electropositive atom transfer to the electronegative one, forming two nearby
Molecules can lose or gain electrons to become ions, just like atoms, independently of its bond polarity.
The configuration of the molecular bonds around an atom depends on the number of bonds with other atoms (red) and the filled outer orbitals (pink).
Bonds and filled orbitals are negatively charged, so they repel each other as far as possible.

















The neutral noble atoms (group 8), such as

Most atoms (except


(One can imagine that to name all the different possible organic molecules is a problem.)

Some molecules can repeat themselves to form very large molecules called polymers. There is no limit to how big such molecules can get.

Molecules change their shape continually as the single bonds rotate. But double and triple bonds are rigid.
(Click on molecule.)
Very large molecules are mostly entangled and so have restricted bond rotations; but they vibrate and thus may change their overall shape. At higher temperatures, they untangle.
The traditional notation used to denote a molecule is simply to list down the constituent atoms as in
Molecules with the same constituent atoms but placed differently are effectively different molecules — they are called


— same atoms but in different functional groups



e.g., helical molecules


Geometric

— when there is a choice in orientation, the same choice is made throughout the polymer;

— orientation choices alternate or keep a pattern;

— orientation choices are random.

A large molecule may "fold" up in (very) many different ways, producing effectively different variants of the same molecule.
Conversely, two large molecules, that are quite different from each other, may fold up so that they have the same outward appearance (electrically).
At high temperatures, energy (from photons or collisions) cause bonds in molecules to break; as the temperature is lowered, this happens temporarily. Below a temperature of about
Electrons in molecules can absorb energy by jumping to a higher-energy molecular orbital. An excited molecule normally falls back to its low-energy orbital by emitting a photon in
Click on molecule
Large molecules may have different charges on different parts of the molecule; in this case it is effectively ionic or polar even if it may be overall neutral in charge.
The charge attractions between large molecules may cause them to "stick" together even though there are no actual covalent bonds between them. This can occur on larger scales as well.
Molecules vary in how stable they are. Some may be insufficiently stable and reform into new molecules by recombining their atoms. There are two basic processes for such reactions to occur:
A bond may be inherently weak and breaks up spontaneously or when hit hard.
The molecule breaks up into two radicals (with partially filled orbitals) or two ions (+ and -). Higher temperatures increase the vibrational energy of the bonds, making it more likely that they break.
Coversely, two molecules may meet and form a bond. This occurs mostly between two free radicals that collide by chance, or two ions (+ and -) or polar molecules that attract each other, especially energetic 'free' electrons and protons.
Atoms have different energies ("affinities") for their outer electrons. Electropositive atoms, or ions, have high-energy outer electrons that can be donated to electronegative atoms/ions, that have low-energy unfilled orbitals.
An acid molecule is one that can lose a
When a charged ion or a polar molecule approaches a neutral molecule it may induce it to become more polar and transfer electrons while breaking and reforming bonds.
A bond rearrangement may occur, possibly even within a molecule:
Molecules that are semi-stable require activation energy to react; this can be in the form of an energetic collision (high temperature) or the absorption of a photon, or excessive bond strain.
The rate at which a reaction occurs (per molecule) depends on how often collisions occur (concentration of the reacting molecule \(n\)), and their energy (temperature \(T\)), how difficult it is to react (the activation energy barrier \(E\)) and the entropy benefits of the reaction \(\Delta S\) (e.g., more/less molecules, of mixed elements) :-
\[ne^{\Delta S - E/T}\]A high pressure favors the formation of fewer larger molecules, and increases the rate of collisions; low pressure favors more smaller molecules.
Reactions between molecules in the gas or liquid phase are faster than in the solid phase; reactions between immiscible fluids or solids is constrained to occur at their surface; the concentration of particles at the surface boundary may be higher/lower than inside the fluid.
Given a number of molecules, a network of reactions may occur.
The network on the left has a multitude of reactions:
CH3 + O2 → CH2O + OH
CH2O + OH → CHO + H2O
CHO → CO + H
O2 + H → OH + O
CO + O → CO2
O2 + OH → HO2 + O
CO + HO2 → CO2 + OH
....
Most reactions quoted by scientists are the starting and end-results of the molecules, and ignore the intermediate steps.
The slowest step/s in the fastest path will dominate the whole process. The end-result of reactions is the elimination, addition or substitution of parts of a molecule, the transfer of electrons, or the rearrangement of a molecule into an isomer.
The product molecules are more stable (have less energy) at the given thermodynamic conditions, because they have stronger unstrained bonds.