Noble gas compound

Noble gas compounds are chemical compounds that include an element from group 18 of the periodic table, the noble gases.

History and background

It was initially believed that the noble gases could not form compounds due to their full valence shell of electrons that rendered them very chemically stable and unreactive.

All noble gases have full s and p outer electron shells (except helium, which has no p sublevel), and so do not form chemical compounds easily. Because of their high ionization energy and almost zero electron affinity, they were not expected to be reactive.

In 1933 Linus Pauling predicted that the heavier noble gases would be able to form compounds with fluorine and oxygen. Specifically, he predicted the existence of krypton hexafluoride (KrF₆) and xenon hexafluoride (XeF₆), speculated that XeF₈ might exist as an unstable compound, and suggested that xenic acid would form perxenate salts.^[1][2] These predictions proved quite accurate, although subsequent predictions for XeF₈ indicated that it would be not only thermodynamically unstable, but kinematically unstable.^[3] As of 2013, XeF₈ has not been made, although the octafluoroxenate(VI) anion (XeF2−
8) has been observed.

The heavier noble gases have more electron shells than the lighter ones. Hence, the outermost electrons experience a shielding effect from the inner electrons that makes them more easily ionized, since they are less strongly attracted to the positively-charged nucleus. This results in an ionization energy low enough to form stable compounds with the most electronegative elements, fluorine and oxygen, and even with less electronegative elements such as nitrogen and carbon under certain circumstances.^[4][5]

True noble gas compounds

While a presentation of what is known about these might follow their increasing atomic weights, here, they are presented in terms of the decreasing weights (of the non-radioactive gases), because this best reflects the priority of their discovery, and the breadth of available information for these compounds. (Radon is not chemically inert but its short half-life and the high energy of its radioactivity make difficult investigation of the sole described fluoride, RnF₂ and its reaction products.^[6])

Xenon compounds

The first published report, in June 1962, of a noble gas compound was by Neil Bartlett, who noticed that the highly oxidising compound platinum hexafluoride ionised O₂ to O+
2. As the ionisation energy of O₂ to O+
2 (1165 kJ mol⁻¹) is nearly equal to the ionisation energy of Xe to Xe⁺ (1170 kJ mol⁻¹), he tried the reaction of Xe with PtF₆. This yielded a crystalline product, xenon hexafluoroplatinate, whose formula was proposed to be Xe+
[PtF
6]−
.^[2][7] It was later shown that the compound is actually more complex, containing both XeFPtF₅ and XeFPt₂F₁₁.^[8] This was the first real compound of any noble gas.

In September 1962, Howard Claasen reported the synthesis of a simple (two-element) noble gas compound, xenon tetrafluoride, by subjecting xenon and fluorine to a high temperature.^[9] In November 1962, Rudolf Hoppe of Universität Münster reported that xenon and fluorine can react to form xenon difluoride.^[10]

In recent years, further studies of XeF₄ have appeared, and several additional compounds of noble gases, particularly xenon, have been prepared, among them the xenon fluorides (XeF₂, XeF₆), oxyfluorides (XeOF₂, XeOF₄, XeO₂F₂, XeO₃F₂, XeO₂F₄) and oxides (XeO
2, XeO₃ and XeO₄). Xenon difluoride has been produced by the exposure of Xe and F₂ gases to sunlight, a result which eluded observation for 50 years. Xenon fluorides react with several other fluorides to form fluoroxenates, such as sodium octafluoroxenate (Na+
2XeF2−
8), and fluoroxenonium salts, such as trifluoroxenonium hexafluoroantimoniate (XeF+
3SbF−
6).

In terms of other halide reactivity, short-lived excimers of noble gas halides such as XeCl₂ are prepared in situ, and are used in the function of excimer lasers.

Recently, xenon has been shown to produce a wide variety of compounds of the type XeO_nX₂ where n is 1,2 or 3 and X is any electronegative group, such as CF₃, C(SO₂CF₃)₃, N(SO₂F)₂, N(SO₂CF₃)₂, OTeF₅, O(IO₂F₂), etc.; the range of compounds is impressive, similar to that seen with the neighbouring element iodine, running into the thousands and involving bonds between xenon and oxygen, nitrogen, carbon, boron and even gold, as well as perxenic acid, several halides, and complex ions.

A compound with an Xe-Xe bond has been reported, and is noteworthy: the compound Xe₂Sb₂F₁₁ contains a Xe–Xe bond, and it is the longest element-element bond known (308.71 pm = 3.0871 Å).^[11] Short-lived excimers of Xe₂ are reported to exist as a part of the function of excimer lasers.

Krypton compounds

Following the first successful synthesis of xenon compounds, synthesis of krypton difluoride (KrF
2) was reported in 1963.^[12] Krypton gas reacts with fluorine gas under extreme forcing conditions, forming KrF₂ according to the following equation:

Kr + F₂ → KrF₂

KrF₂ reacts with strong Lewis acids to form salts of the KrF⁺ and Kr
2F+
3 cations.^[12] The preparation of KrF
4 reported by Grosse in 1963, using the Claasen method, was subsequently shown to be a mistaken identification.^[13]

Krypton compounds with other than Kr-F bonds (compounds with atoms other than fluorine) have also been described. KrF
2 reacts with B(OTeF
5)
3 to produces the unstable compound, Kr(OTeF
5)
2, with a krypton-oxygen bond. A krypton-nitrogen bond is found in the cation [HC≡N–Kr–F]+
, produced by the reaction of KrF
2 with [HC≡NH]+
[AsF−
6] below −50 °C.^[14]

Argon compounds

The discovery of HArF was announced in 2000.^[15][16] The compound can exist in low temperature argon matrices for experimental studies, and has also been studied computationally.^[16] Argon hydride ion ArH+
was obtained in 70th of last century.^[17] This molecular ion has also been identified in the Crab nebula, based on the frequency of its light emissions.^[18]

Neon and helium compounds

A neon compound has yet to be described or identified. There is some theoretical evidence for a few metastable helium compounds which may exist at very low temperatures and extreme pressures, though none are confirmed by experiment. The stable cation, HeH⁺, was reported in 1925^[19]).

Reports prior to xenon hexafluoroplatinate and xenon tetrafluoride

Clathrates

Prior to 1962, the only isolated compounds of noble gases were clathrates (including clathrate hydrates); other compounds such as coordination compounds were observed only by spectroscopic means.^[2] Clathrates (also known as cage compounds) are compounds of noble gases in which they are trapped within cavities of crystal lattices of certain organic and inorganic substances. The essential condition for their formation is that the guest (noble gas) atoms should be of appropriate size to fit in the cavities of the host crystal lattice; for instance, Ar, Kr, and Xe can form clathrates with crystalline β-quinol, but He and Ne cannot fit because they are too small. As well, Kr and Xe can appear as guests in crystals of melanophlogite.

Coordination compounds

Coordination compounds such as Ar·BF₃ have been postulated to exist at low temperatures, but have never been confirmed. Also, compounds such as WHe₂ and HgHe₂ were reported to have been formed by electron bombardment, but recent research has shown that these are probably the result of He being adsorbed on the surface of the metal; therefore, these compounds cannot truly be considered chemical compounds.

Hydrates

Hydrates are formed by compressing noble gases in water, where it is believed that the water molecule, a strong dipole, induces a weak dipole in the noble gas atoms, resulting in dipole-dipole interaction. Heavier atoms are more influenced than smaller ones, hence Xe·6H₂O was reported to have been the most stable hydrate. The existence of these compounds have, however, been disputed in recent years.

Fullerene adducts

Noble gases can also form endohedral fullerene compounds where the noble gas atom is trapped inside a fullerene molecule. In 1993, it was discovered that when C₆₀ is exposed to a pressure of around 3 bar of He or Ne, the complexes He@C₆₀ and Ne@C₆₀ are formed.^[20] Under these conditions, only about one out of every 650,000 C₆₀ cages was doped with a helium atom; with higher pressures (3000 bar), it is possible to achieve a yield of up to 0.1%. Endohedral complexes with argon, krypton and xenon have also been obtained, as well as numerous adducts of He@C₆₀.^[21]

Applications

Most applications of noble gas compounds are either as oxidising agents or as a means to store noble gases in a dense form. Xenic acid is a valuable oxidising agent because it has no potential for introducing impurities—xenon is simply liberated as a gas—and so is rivalled only by ozone in this regard.^[2] The perxenates are even more powerful oxidizing agents. Xenon-based oxidants have also been used for synthesizing carbocations stable at room temperature, in SO
2ClF solution.^[22]

Stable salts of xenon containing very high proportions of fluorine by weight (such as tetrafluoroammonium heptafluoroxenate, NF₄XeF₇, and the related tetrafluoroammonium octafluoroxenate (NF₄)₂XeF₈), have been developed as highly energetic oxidisers for use as propellants in rocketry.^{[23] [24]}

The xenon fluorides are good fluorinating agents.

Clathrates have been used for separation of He and Ne from Ar, Kr, and Xe, and also for the transportation of Ar, Kr, and Xe. (For instance, radioactive isotopes of krypton and xenon are difficult to store and dispose, and compounds of these elements may be more easily handled than the gaseous forms.^[2]) In addition, clathrates of radioisotopes may provide suitable formulations for experiments requiring sources of particular types of radiation; hence. ⁸⁵Kr clathrate provides a safe source of beta particles, while ¹³³Xe clathrate provides a useful source of gamma rays.

References

Resources

• Khriachtchev, Leonid; Räsänen, Markku; Gerber, R. Benny (2009). "Noble-Gas Hydrides: New Chemistry at Low Temperatures". Accounts of Chemical Research 42 (1): 183–91. doi:10.1021/ar800110q. PMID 18720951. 

Noble gas compounds Helium compounds HeH+ LiHe He2 Neon compounds No neon compounds have yet been identified. Argon compounds HArF ArCF22+ Krypton compounds KrF2 HKrCN HKrC2H Kr(OTeF5)2 HCNKrF2 Xenon compounds Xe(0) AuXe4(Sb2F11)2 Xe(I) XePtF6 XeRhF6 Xe(II) XeF2 XeFPtF5 XeFPt2F11 Xe2F3PtF6 XeCl2 Organoxenon(II) compounds Xe(IV) XeO2 XeF4 XeOF2 N(CH3)4XeF5 Organoxenon(IV) compounds Xe(VI) XeO3 XeF6 XeOF4 H2XeO4 (NO)2XeF8 Xe(VIII) XeO4 H4XeO6 Radon compounds Rn(II) RnF2 RnFSb2F11 Rn(VI) RnO3