Element 36 takes its name from the Greek word, kryptos meaning hidden. Like all other members of group 18 (the noble gases), it is colourless, odourless, and occurs in only minute amounts in the Earth's atmosphere (1.14 ppm in dry air). It was Sir William Ramsay who, following the 1894 discovery of argon with Lord Rayleigh, suggested that a new family of elements would now need to be accommodated within the periodic table. In 1898 Ramsay, together with Morris Travers, went on to discover krypton, and two weeks later neon and xenon in residues remaining after evaporating nearly all components of liquid air.

Krypton gas is commercially produced by fractional distillation of liquefied air. Its only other notable source is uranium fission from nuclear reactors. It produces 85Kr (fission yield 0.3%), a radioisotope with a half-life of 10.8 years, which decays into non-radioactive 85Rb, and which has been used to detect clandestine military-based nuclear activities.

For a time (1960–1983), the metre was defined as 1,650,763.73 wavelengths of the red-orange (605 nm) emission line of 86Kr. Element 36 serves in high-performance incandescent light bulbs to retard the evaporation of the tungsten filament, improving efficiency and enhancing the brightness and lifetime of the bulb — although these are now being superseded by LED technology. The krypton–fluoride laser, a type of excimer or exciplex (excited complex) laser, is widely employed in photolithography, which has enabled further miniaturization of semiconductor devices and an increase in their densities on silicon chips. In addition to its lighter noble-gas neighbour argon, krypton may also be found in homes where it serves as a high-efficiency thermal insulator in double- or triple-pane glass windows. Liquid krypton electromagnetic calorimeters employed in particle physics research hold up to 30 tonnes of krypton and are the largest known concentrations of this rare gas.

Synthesis of KrF2 by UV-irradiation of liquid-N2-cooled solid Kr and liquid F2 with a Hg lamp. Credit: MATIC LOZINŠEK

Krypton is the lightest noble gas to form compounds that are isolable in macroscopic amounts. The synthesis and isolation of the first krypton compound, KrF2, was reported in 1963 shortly after the syntheses of the first xenon compounds in 1962 — 65 years after the discovery of these noble gases1,2 — although unfortunately at the time it was erroneously described as KrF4 instead1. Krypton difluoride has so far remained the only isolated binary krypton compound. Unlike xenon compounds, which have been characterized for xenon in the +½, +2, +4, +6, and +8 oxidation states, krypton chemistry is limited to the +2 oxidation state and all known compounds have been derived from KrF2 (ref. 3).

Owing to its thermodynamic instability, KrF2 is a better source of F radicals and a much stronger oxidizer than elemental fluorine, F2. Its synthesis in gram quantities is challenging and only a few low-temperature methods3 based on the generation of F radicals are in use, such as hot wire, electric glow discharge, and UV photolysis (pictured) methods. Derivatives of KrF2 are often prepared by utilizing its fluoride-ion donor abilities, which in reaction with strong Lewis acids such as SbF5 or AsF5, forms salts of the KrF+ and Kr2F3+ cations4. With weak fluoride acceptors, KrF2 forms fluoride-bridged adducts where the KrF2 ligand coordinates through fluorine to either metal or non-metal centres, for example MOF4 (M = Cr, Mo, W) and BrOF2+. The Lewis acidity of the KrF+ cation has been exploited for the synthesis of [HCNKrF]+[AsF6], which features the first example of a krypton–nitrogen bond5. Krypton is, however, rather selective in its choice of bonding partners and will only bond under the right conditions to the most electronegative atoms — fluorine, oxygen, and nitrogen — with only one example of a Kr–O bond known thus far, in Kr(OTeF5)2.

The extreme oxidizing abilities of KrF2 and KrF+ have been exploited for the syntheses of otherwise hard-to-attain high-valent compounds containing Ag(III), Ni(IV), Au(V), and exotic species such as TcVIIOF5, OsVIIIO2F4, ClVIIF6+, and BrVIIF6+. These applications demonstrate that the original krypton compound, KrF2, is not simply a chemical curiosity in the scientific cabinet of wonders but also a part of the chemist's toolbox.

In 1938, the name of this element inspired the naming of Krypton, Superman's birth planet, as well as the powerful material originating from this planet called kryptonite. The analogy between the 'superoxidants' KrF2, KrF+, and Kr2F3+, which rob other strong oxidant species of their electrons, and kryptonite, which robs Superman of his powers, is, of course, pure coincidence.