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Orbital hybridisation |
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Orbital hybridisationIn chemistry, hybridisation is the mixing of atomic orbitals to form new orbitals suitable for bonding. Hybridisation is an integral part of the valence shell electron-pair repulsion (VSEPR) theory as well as a quantum mechanical model for orbital electrons to decribe groups 2,3,4 of the periodic families of elements whose electron orbital clouds fuse into one hybrid orbital. Groups 1,5,6 and 7 in the period table do not hybridise. The hybridisation theory was theorised by chemist Linus Pauling in order to explain the existence of molecules such as methane (CH4). The problem with the existence of methane is this: It is made up of a carbon atom bonded to four hydrogen atoms. Carbon's ground-state configuration is 1s² 2s² 2px¹ 2py¹ or perhaps more easily read:
(Note: The 1s orbital is lower in energy than the 2s orbital, and the 2s orbital is lower in energy than the 2p orbitals) The valence bond theory would predict, based on the existence of two half filled p-type orbitals (the designations px py or pz are meaningless at this point, as they do not fill in any particular order), that C forms two covalent bonds. CH2, however, is known as a methylene group and cannot exist outside of a molecular system. Therefore, this theory alone cannot explain the existence of CH4. Furthermore, ground state orbitals cannot be used for bonding in CH4. While exciting a 2s electron into a 2p orbital would theoretically allow for four bonds, according to the valence bond theory which has been proved experimentally correct for systems like O2 this would imply that the various bonds of CH4 would have differing energies due to differing levels of orbital overlap. Once again, this has been experimentally disproved: any hydrogen can be removed from a carbon with equal ease. To summarise, to explain the existence of CH4 and many other molecules a method by which as many as 12 bonds (for transition metals) of equal strength (and therefore equal length) can be created is required. The answer is the theory of hybridisation. At this time it is important to note that orbitals are, and always will be, a model. They are not real. They are derived from specialised solutions of the Schrödinger equation and therefore to hybridise, to mix an orbital, is simply to change the mathematical function governing where that electron should be. It is not altering the structure of the atom in any way. The first step in hybridisation is the excitation of one (or more) electrons. From this point of the explanation on, it can be assumed that the subject of study is carbon in the context of methane, for simplicity. The proton that forms the nucleus of a hydrogen atom attracts one of the valence electrons on carbon. This causes an excitation, moving a 2s electron into a 2p orbital. This, however, increases the influence of the carbon nucleus on the valence electrons by increasing the effective core potential (the amount of charge the nucleus exerts on a given electron = Charge of Core - Charge of all electrons closer to the nucleus). The combination of these forces creates new mathematical functions known as hybridised orbitals. In the case of carbon attempting to bond with four hydrogens, four orbitals are required. Therefore, the 2s orbital (core orbitals are almost never involved in bonding) mixes with the three 2p orbitals to form four sp3 hybrids (read as s p three). See graphical summary below. becomes
translates into Similarly, other C-compounds and other molecules may be explained, for example ethene (C2H4). Carbon will never form any less than four bonds unless it is given no other choice, which only seldom occurs. Therefore, ethene has two double bonds between the carbons. The Lewis structure looks like this:
Carbon will sp2 hybridise, because hybrid orbitals will form only sigma bonds and one pi bond is required for the double bond between the carbons. The hydrogen-carbon bonds are all of equal strength and length, which agrees with experimental data. Molecule shapeHybridisation helps to explain molecule shape.
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