Valence electrons are the fundamental negatively charged particles in the outermost area of atoms that contribute to the formation of chemical bonds. Regardless of the type of chemical interaction (ionic, covalent, or metallic) between atoms, changes in the atomic structure are limited to the outermost, or valence, electrons. Because they are less strongly attracted to the positive atomic nucleus than the inner electrons, they can be exchanged or transferred with surrounding atoms during the bonding process. Valence electrons are also important in the conduction of electric current in metals and semiconductors.
Valence Electron
The valence of an atom is the amount of electrons it needs to lose or gain to reach the octet or maintain stability. The electrons in the outer shells that are not filled are known as valence electrons.
The majority of chemical activities utilise valence electrons, which have a higher energy than electrons in inner orbits. They let us figure out an element’s chemical properties, such as its valency and how it forms bonds with other elements. It also tells us how easy it is for atoms to form bonds, how many unpaired electrons are there, and how many atoms are involved.
Characteristics of Valence Electrons
Electrons are thought to inhabit orbitals within an atom and play a role in chemical bonding. When an atom has completed its octet, which can be done through electron transfer or sharing, it is the most stable. Some of the most important characteristics of a valence electron are:
- The valence electron is found only in the main group elements’ outermost electron shell.
- An atom with a closed valence electron shell is usually chemically inert.
- The valence electrons of an element also determine its electrical conductivity. Depending on the nature of the components, it can be a metal, a non-metal, or a metalloid.
Determination of Valence Electrons
In neutral atoms, the number of valence electrons is equal to the atom’s main group number.
Number of valence electrons Equals to Number of main groups (neutral atoms).
An element’s main group number can be found in its periodic table column. For example, carbon is in group 4 and has four valence electrons. The valence electron count of oxygen is 6. It belongs to group 6 and has a valence electron count of 6.
Valence Bond Theory
According to the valence bond theory, all bonds are established between two atoms by the donation of an electron from each atom. Because many atoms connect with delocalized electrons, this is a false assumption. The VB hypothesis predicts that there are no unpaired electrons in molecular oxygen. The VB theory performs a decent job of explaining the morphologies of covalent compounds qualitatively. While the Molecular Orbital (MO) theory is useful for learning about bonds in general. It is more difficult to understand, but it better predicts actual molecular properties than VB theory. Because of discrepancies in the energy levels of orbitals in the molecule, the MO theory predicts electron transitions. MO theory has been proven to be more accurate on multiple occasions, and as a result, it is chosen.
Valence Bond theory encompasses both the formation of covalent bonds and the electronic structure of molecules. Inside a molecule, electrons occupy specific atoms’ atomic orbitals, and electrons from one atom are attracted to the nucleus of another atom, according to the hypothesis. The attraction between the atoms increases greater as they get closer until they reach a point where the electron density causes repulsion. At the shortest distance between the two atoms, the lowest potential energy is obtained, and this electron density is assumed to be what holds the two atoms together in a chemical bond.
Valence
In chemistry, valence (sometimes spelled valency) is the property of an element that determines the number of other atoms with which it can combine. The phrase was coined in 1868 to indicate both the overall capacity of combination of an element and the numerical value of that power of combination.
For 19th-century chemists, explaining and systematising valence was a major challenge. Because no good theory of its causation existed, most of the effort was focused on developing empirical methods for calculating the valences of the components. The amount of hydrogen atoms with which an atom of the element can mix or replace in a compound was used to calculate the element’s characteristic valence. However, it became clear that the valences of numerous elements differed in different compounds. The discovery by American scientist G.N. Lewis (1916) of the chemical bond of organic compounds as a pair of electrons held together by two atoms and serving to hold them together was the first major step in the development of a good explanation of valence and chemical combination. In the same year, W. Kossel, a German physicist, explained the nature of the chemical bond between electrically charged atoms (ions). After a detailed electronic theory of the periodic system of the elements was established, the theory of valence was reconstructed in terms of electronic structures and interatomic forces. As a result of this circumstance, several new concepts were developed to represent various kinds of atom interaction: ionic valence, covalence, oxidation number, coordination number, and metallic valence.
Examples
A neutral carbon atom has 6 electrons in a 1s22s22p2 electron shell configuration. Because four electrons can be accepted to fill the 2p orbital, carbon has a valence of four.
Conclusion
In 1425, the Latin word valentia, which indicates strength or capacity, was used to explain the word “valence.” The concept of valence was developed in the second half of the nineteenth century to explain chemical bonding and molecular structure. In a paper published in 1852, Edward Frankland proposed the theory of chemical valences.
The number of electrons required to fill an atom’s outermost shell is known as valence. Because there are exceptions, the more general definition of valence is the number of electrons that a certain atom bonds with or the number of bonds that an atom creates.
The maximum number of univalent atoms that can combine with an atom, according to the IUPAC formal definition. The maximum number of hydrogen or chlorine atoms is usually used as the basis for the definition. It’s worth noting that the IUPAC only defines a single valence value (the maximum), despite the fact that atoms are known to have many valences. Copper, for example, usually has a valence of 1 or 2.