The discovery of isotopesBy the end of the 18th century many facts were known about the way that chemical elements combine. For example, it was known that if 1 gram of element A reacts with 10 grams of element B, then 2 grams of A will react with 20 grams of B. This was explained, in 1803, by the chemist John Dalton, who suggested that all matter is composed of tiny particles, called atoms. In Dalton's theory, all the atoms of the same element had the same weight, and elements differed from each other because they were composed of atoms of different weights.
From measurements of the amounts of different substances which took part in chemical reactions, it was possible to measure the atomic weight (also known as the relative atomic mass) of these elements. The atomic weight of an element is the weight of an atom of the element compared with that of a hydrogen atom.
In 1815, William Prout noticed that most atomic weights were almost exactly whole numbers, so that the weight of each atom was almost exactly a multiple of that of a single hydrogen atom. For example, the nitrogen atom is 14 times, and the oxygen atom 16 times, as heavy as the hydrogen atom. This led him to suggest that all atoms were composed of hydrogen atoms. However, when more accurate measurements of atomic weights were made, it was found that they were not exactly whole numbers. Chlorine, for example, was found to have an atomic weight of 35.5. This brought about the downfall of Prout's hypothesis, and it was not until the atomic scientists of the 20th century made their discoveries about the structures of individual atoms that a proper explanation of the values of atomic weights could be found.
In 1897, J. J. Thomson discovered the electron, and in 1911 Ernest Rutherford discovered that the atom consists of a small positively charged core, called the nucleus, surrounded by a number of negatively charged electrons. The positive charge on the nucleus is exactly equal to the total of negative charges carried by the electrons.
It is the number and arrangement of electrons in the atom which determines its chemical behavior. The atomic weights merely determine the amounts of each element which take part in a chemical reaction.
It is therefore possible to have two atoms of the same element of different atomic weight, but which have identical chemical properties because the atomic numbers (and therefore the numbers of electrons in the atoms) are the same. Such atoms are called isotopes. Francis W. Aston, in 1919, using a mass spectrograph, was able to separate isotopes of different elements. In the mass spectrograph it is possible to separate atoms of different atomic weights, and to determine how much of each isotope is present.
The atomic weights of the isotopes of the elements are very nearly whole numbers, and the reason for this became apparent when James Chadwick, in 1932, discovered the neutron. The neutron is an uncharged particle of mass one. It became clear that the atomic nucleus was composed of protons (particles of mass one carrying a single positive charge) and neutrons. For example, the nucleus of helium, which has an atomic weight of 4 and an atomic number of 2, consist of 2 neutrons and 2 protons. The nucleus of the chlorine isotope atomic weight 35 consists of 17 protons and 18 neutrons, whilst the chlorine isotope atomic weight 37 consists of 17 protons and 20 neutrons. The atomic number of both isotopes is 17.
Separation of isotopesWhilst the chemical properties of an element, as determined by the number and arrangement in shells of the electrons, are the same, the physical properties differ. It is this difference in physical properties which enables separation of the isotope to be carried out. For example, the most obvious difference between isotopes of an element is that of mass. This leads to differences in the rates of diffusion of the different gaseous isotopes of an element through a porous membrane, and to different rates of evaporation in liquid elements. Both of these properties have been used to separate isotopes.
In ordinary water there are 660 ordinary H2O molecules to every heavy water molecule. When water containing sodium hydroxide is electrolyzed, oxygen is evolved at the anode (positive electrode). Both hydrogen and deuterium are evolved at the cathode (negative electrode). Because the deuterium molecules are twice as heavy as the hydrogen molecules, they are evolved at a lower rate than the hydrogen molecules, and tend to be left behind, in solution. Enrichment of the solution with the heavy isotope therefore results, but it is only a slight enrichment, because the proportion of heavy atoms present in the solution is small, and some of these atoms are evolved with the light ones. The process has therefore to be repeated many times with successive additions of water, followed by electrolysis, until the required concentration is obtained. To obtain 1 gram of 99% pure heavy water, 100,000 grams of ordinary water has to electrolyzed.
Similar difficulties are encountered in the other methods of separating isotopes. For example, in the diffusion method of separation, passage through a plate containing tiny holes will separate gaseous compounds of isotopes of the element uranium. In practice, to obtain 99% purity of the U235, 5,000 such plates, through which the gas diffuses in succession, would be required.
So while there are many ways of separating isotopes – others include distillation (formerly used to produce heavy water), centrifuging, and laser methods – none is easy in practice, and it is not surprising that the discovery of isotopes had to wait for the work of 20th century physicists and chemists.
Artificial isotopes and radioisotopesAll the isotopes which have been mentioned so far occur in nature. Isotopes can be created by putting elements into a nuclear reactor. Inside the reactor the element is bombarded with neutrons and occasionally a neutron will enter a nucleus to form an artificial isotope. Many of these isotopes break up spontaneously, emitting charged particles. These radioactive isotopes, or radioisotopes, find many uses in the diagnosis and treatment of disease.
Isotopes and lifeOf astrobiological interest is the fact that isotopic ratios of particular elements are affected by the presence of life. For example, nitrogen gas is enriched in 14N when produced by denitrification, and hydrogen sulfide is enriched in 32S when it results from sulfate reduction. Such patterns of fractionation provide clues for the remote sensing of life on other worlds. For more on this, see extraterrestrial life, detection.
Related categories• ATOMIC AND NUCLEAR PHYSICS
• PHYSICAL CHEMISTRY
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