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The International Union of Pure and Applied Chemistry's (IUPAC) definition of a chemical reaction is “a process that results in the interconversion of chemical species.” A chemical species is “an ensemble of the chemical elements which is identifiable as a separately distinguishable entity.” The transformation of reacting species into a new chemical product can be likened conceptually to events that occur in everyday life—it involves the interaction of objects (molecules, atoms, ions) with each other, and the outcome of the process is governed by their relative sizes, positions, and energies. A key has to be inserted correctly into a lock for it to be opened, and an egg's shell can be broken only by the application of sufficient force. The relation of these ideas will become clearer as the fundamental processes governing a chemical reaction are examined.

A discussion of chemical reactions in the context of time is highly appropriate: They have occurred since the dawn of time, they are both controlled by time, and, given the huge range of timescales on which reactions can take place, for example, the rusting of an iron nail compared to dynamite exploding, they exert an influence over the course of time. The history of chemical reactions in time is discussed in a manner complementary to the discovery of the chemical elements, although the two are very closely linked. This entry gives detailed consideration to the timescale on which chemical reactions occur: the very fast; those that are easier for human beings to contemplate; and the very slow. This highlights the technical ingenuity of scientists who have developed many sophisticated techniques to study ultrafast reactions.

History of Chemical Reactions

The world as we know it, indeed the entire universe, is composed of the chemical elements. The 94 known chemical elements (there are more in the periodic table, but they do not occur naturally) were formed shortly after the start of time as we know it—the big bang—and have been combining with each other ever since. Shortly after the big bang, extreme temperatures are believed to have favored the fusion of the separate neutrons and protons present, forming helium and deuterium nuclei, in a process termed big bang nucleosynthesis. These positively charged nuclei subsequently combined with the negatively charged primordial particles present, electrons, to produce the first atoms, of which most were hydrogen. The extreme conditions generated by the production of the first stars are believed to have created heavier elements through the processes of stellar and supernova nucleosynthesis, and cosmic ray spoliation. The first chemical reactions would have now occurred, with simple chemical entities based on light atoms such as carbon, nitrogen, and oxygen produced in abundance.

The formation of the earth (c. 4.6 billion years ago) was followed by the Hadean eon, where the earth began to take shape. Changes in the chemical composition of the atmosphere, afforded by volcanic eruptions, the cooling of the earth's surface, and asteroid bombardment, have been proposed to have been instrumental in the development of life. The generation of small organic molecules, known to be monomeric constituents of living organisms from the most basic chemical species, is propounded as one of the most widely accepted theories of the origin of life. The combination of a-amino acid molecules to form polypeptide chains; the similar production of nucleotides, phosphates, and sugars could, theoretically, react together in such a way as to give the double-helix of life, DNA. The classic Miller-Urey experiment exposed a mixture of simple gases and water vapor to an electrical discharge (to mimic lightning), and the ensuing chemical reactions were indeed found to produce simple biomolecules that are essential to life. An early earth atmosphere rich in ammonia, methane, water, carbon dioxide, and nitrogen could have been transformed chemically to give a so-called primordial soup.

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