Hydrogen [1] (hydrogenium, υδωρ = the water, γ εννειν = to give birth) is the first element in the periodic table of the elements having the atomic number 1 and the electron configuration 1s 1 . Hydrogen was prepared many years before it was recognized as a distinct substance by Cavendish in 1766 and it was named by Lavoisier. Hydrogen is the most abundant of all elements in the universe and it is thought that the heavier elements were, and still are, built from hydrogen and helium. It has been estimated that hydrogen makes up more than 90 % of all the atoms or 75 % of the mass of the universe. It is found in the sun and most stars, and plays an important part in the proton-proton reaction and calin rbon-nitrogen cycle, which accounts for the energy of the sun and stars. It is thought that hydrogen is a major component of the planet Jupiter and that at some depth in the planet's interior the pressure is so great that solid molecular hydrogen is converted into solid metallic hydrogen.The ordinary isotope of hydrogen, H is known as Protium and has an atomic weight of 1.0078 (1 proton and 1 electron). In 1932, Urey [2] announced the preparation of a stable isotope, Deuterium (D) with an atomic weight of 2.0140 (1 proton, 1 neutron and 1 electron). Two years later an unstable isotope, Tritium (T), with an atomic weight of 3.0161 (1 proton, 2 neutrons and 1 electron) was discovered [3]. Tritium has a half-life of 12.5 years [4]. Deuterium is found in 0.017 % of all hydrogen isotopes [5]. Tritium atoms are also present in ≈10 −18 % of all hydrogen isotopes as a result of natural processes in the atmosphere, as well as from fallout from past atmospheric nuclear weapons tests and the operation of nuclear reactors and fuel reprocessing plants (Table 4.1 and Figure 4.1).