Noble Gas
The noble gases constitute Group 18 of the periodic table—helium, neon, argon, krypton, xenon, radon, and oganesson—characterized by closed valence electron shells, high ionization energies, and specialized hypervalent reactivity in heavy congeners.
The noble gases (historically termed inert gases or aerogens) constitute Group 18 (formerly Group VIII or Group 0) at the far right column of the periodic table, comprising six naturally occurring monatomic gases—helium (He, Z = 2), neon (Ne, Z = 10), argon (Ar, Z = 18), krypton (Kr, Z = 36), xenon (Xe, Z = 54), and radioactive radon (Rn, Z = 86)—together with the synthetic superheavy Period 7 element oganesson (Og, Z = 118). Isolated primarily between 1894 and 1898 by Lord Rayleigh (John William Strutt) and Sir William Ramsay through fractional distillation of liquid air (awarded the 1904 Nobel Prizes in Physics and Chemistry), the noble gases possess completely filled s and p valence shells (1*s*2 for helium; ns2np6 valence octets for Ne through Rn).
Because a closed-shell electronic configuration yields a zero net spin and zero orbital angular momentum (ground spectroscopic term 1S0), a large HOMO–LUMO energy gap, the highest first ionization energy (IE1) in each period, and a negative electron affinity (EA < 0), the lighter noble gases resist ordinary covalent or ionic bond formation. However, in 1962 Neil Bartlett overthrew the dogma of absolute noble-gas inertness by oxidizing xenon with platinum hexafluoride (PtF6), opening a rich chemistry of hypervalent xenon, krypton, and radon fluorides and oxides governed by VSEPR theory and three-center four-electron bonds.
🧪 Interactive Simulation: Inspect the 3D geometries and equatorial/axial lone pairs of noble-gas fluorides (XeF2 and XeF4) in VSEPR Lab.
Electronic Configuration, Ionization Trends, and London Dispersion Forces
Closed-Shell Stability and Periodic Physical Properties
In any horizontal period of the periodic table, the Group 18 noble gas marks the completion of the principal valence np subshell (or the 1*s* shell in helium). Adding one more electron to a neutral noble gas atom requires populating the next higher principal quantum shell ((n + 1)s), which is strongly shielded by the inner ns2np6 core; consequently, all natural noble gases have endothermic (negative) electron affinities and cannot form stable gas-phase anions (X−). Conversely, removing an electron from the compact, unshielded ns2np6 shell requires surmounting the highest first ionization energy (IE1) of any element in that row—ranging from 24.59 eV (2,372 kJ mol−1) in helium down to 12.13 eV (1,170 kJ mol−1) in xenon and 10.75 eV (1,037 kJ mol−1) in radon.
Because two ground-state noble gas atoms have filled bonding (1*σ*g2) and antibonding (1*σ*u*2) molecular orbitals (net Molecular Orbital bond order = 0), they exist as monatomic gases (Cp,m / CV,m = γ = 5/3 ≈ 1.667) with zero permanent electric dipole moment (μ = 0 D). In the liquid and solid states, noble gas atoms attract one another exclusively via weak quantum-mechanical London dispersion forces (Vdisp ∝ −*α*2 IE1 / r6). As atomic number Z increases down Group 18 from He to Rn, the outer valence shell expands radially and becomes increasingly polarizable (static dipole polarizability α increases 20-fold from 0.205 Å3 in He to 4.04 Å3 in Xe), strengthening London dispersion attractions and raising both normal boiling points and enthalpies of vaporization monotonically down the column:
| Element (Z, Symbol) | Valence Configuration | First Ionization Energy (IE1) | Polarizability (α, Å3) | Van der Waals Radius (rvdW) | Normal Boiling Point (1 atm) | Atmospheric Volume Fraction (Dry Air) |
|---|---|---|---|---|---|---|
| Helium (2, He) | 1*s*2 | 2,372 kJ mol−1 (24.59 eV) | 0.205 Å3 | 140 pm | 4.22 K (−268.93 °C) | 5.24 ppmv (0.000524%) |
| Neon (10, Ne) | 2*s*2 2*p*6 | 2,081 kJ mol−1 (21.56 eV) | 0.396 Å3 | 154 pm | 27.07 K (−246.08 °C) | 18.18 ppmv (0.001818%) |
| Argon (18, Ar) | 3*s*2 3*p*6 | 1,521 kJ mol−1 (15.76 eV) | 1.641 Å3 | 188 pm | 87.30 K (−185.85 °C) | 9,340 ppmv (0.934%) |
| Krypton (36, Kr) | 4*s*2 4*p*6 | 1,351 kJ mol−1 (14.00 eV) | 2.484 Å3 | 202 pm | 119.93 K (−153.22 °C) | 1.14 ppmv (0.000114%) |
| Xenon (54, Xe) | 5*s*2 5*p*6 | 1,170 kJ mol−1 (12.13 eV) | 4.044 Å3 | 216 pm | 165.03 K (−108.12 °C) | 0.087 ppmv (87 ppbv) |
| Radon (86, Rn) | 6*s*2 6*p*6 | 1,037 kJ mol−1 (10.75 eV) | 5.3 Å3 | 220 pm | 211.3 K (−61.7 °C) | Trace (~10−19, from 226Ra decay) |
| Oganesson (118, Og) | 7*s*2 7*p*1/22 7*p*3/24 | ~860 kJ mol−1 (~8.9 eV, calc.) | ~5.8 Å3 (calc.) | — | ~320–380 K (predicted semiconducting solid/liquid) | Synthetic (t1/2 ≈ 0.7 ms for 294Og) |
Chemical Reactivity: Neil Bartlett's 1962 Discovery and Hypervalent Xenon Compounds
Oxidation of Xenon by PtF6 and the Fluorine-Oxygen Requirement
For over six decades after William Ramsay's discovery of the Group 18 elements, chemists assumed that closed-shell octets could not form stable chemical bonds. In March 1962 at the University of British Columbia, Neil Bartlett reacted dark-red platinum hexafluoride vapor (PtF6, a powerful one-electron oxidizer) with molecular oxygen (O2) to isolate the ionic dioxygenyl salt [O2]+[PtF6]−. Noticing that the first ionization energy of molecular dioxygen (IE1(O2 → O2+) = 1,175 kJ mol−1 / 12.2 eV) is virtually identical to the first ionization energy of atomic xenon (IE1(Xe → Xe+) = 1,170 kJ mol−1 / 12.13 eV), Bartlett mixed orange-yellow xenon gas with red PtF6 vapor at room temperature and immediately precipitated a mustard-yellow solid (formulated as [XeF]+[PtF6]− / Xe[PtF6]x). Within months, Howard Claassen, Henry Selig, and John Malm at Argonne National Laboratory synthesized binary xenon tetrafluoride (XeF4) directly from the elements (Xe + 2 F2 at 400 °C and 6 atm), followed rapidly by XeF2 and XeF6.
Why do stable covalent compounds of xenon and krypton form almost exclusively with fluorine (χP = 3.98) and oxygen (χP = 3.44)? In a hypervalent three-center four-electron bond (F–Xe–F), the non-bonding HOMO (ψ2) places negative charge on the two terminal ligands while the central xenon atom carries a positive partial charge, requiring:
- A heavy noble gas (Xe, Rn, or Kr) with a low enough ionization energy (IE1 ≤ 14.0 eV) and radially accessible valence np orbitals.
- Small, strongly electronegative ligands (F or O) with low homonuclear bond dissociation energy (*D*°(F–F) = 159 kJ mol−1) and high electronegativity so that the exothermic formation of polar Xe–F bonds (*D*° ≈ 131 kJ mol−1 per bond) outweighs the promotion cost.
VSEPR Geometries of Xenon Fluorides, Oxides, and Oxyfluorides
Xenon spans even oxidation states from +2 to +8, serving as the textbook showcase of VSEPR theory across steric numbers 4, 5, 6, and 7:
- Xenon(+2) — XeF2 (AX2E3, SN = 5, Linear D∞h): Prepared by UV photolysis of a 1:1 Xe/F2 mixture; three equatorial lone pairs at 120° leave the two fluorine atoms colinear at 180° (r(Xe–F) = 1.977 Å).
- Xenon(+4) — XeF4 (AX4E2, SN = 6, Square Planar D4h): Two trans (180°) axial lone pairs leave four fluorine atoms in a square plane at 90° angles (r(Xe–F) = 1.953 Å, μ = 0 D).
- Xenon(+6) — XeF6 (AX6E1, SN = 7, Fluxional C3v Distorted Octahedron), XeOF4 (AX5E1, Square Pyramidal C4v), and XeO3 (AX3E1, Trigonal Pyramidal C3v): Hydrolysis of XeF4 or XeF6 by water yields xenon trioxide (XeO3), a shock-sensitive white crystalline solid (Δ*H*f° = +402 kJ mol−1) that decomposes back to Xe(g) + 3/2 O2(g), whereas controlled 1:1 hydrolysis of XeF6 yields volatile XeOF4 (where the double-bonded oxo ligand =O sits opposite the axial lone pair at 180°, with Feq–Xe=O angle 91.8°).
- Xenon(+8) — XeO4 (AX4E0, Tetrahedral Td) and Perxenate XeO64− (AX6E0, Octahedral Oh): Utilizing all eight 5*s*25*p*6 valence electrons leaves zero lone pairs on xenon.
Lighter krypton (IE1 = 14.00 eV) forms endothermic krypton difluoride (KrF2, Δ*H*f° = +60.2 kJ mol−1, linear D∞h, r(Kr–F) = 1.89 Å) under low-temperature electric discharge at 77 K, and argon forms the matrix-isolated argon fluorohydride (HArF) at 8–27 K (discovered by Markku Räsänen in 2000, bonded as an ionic-covalent [HAr]+F− 3c–4e triad). Neither helium nor neon forms any neutral stable covalent compound at ambient pressures, though high-pressure diamond-anvil experiments (>113 GPa) have synthesized the electride crystal Na2He.
Cosmochemical and Radiogenic Origins, Applications, and General Anesthesia
Primordial Big Bang Helium versus Radiogenic Crustal Argon-40 and Helium-4
The isotopic abundances of the noble gases in Earth's atmosphere record two distinct nuclear processes:
- Big Bang and Stellar Nucleosynthesis vs. Gravitational Escape: Although helium is the second most abundant element in the universe (~24% by mass, synthesized as 4He during the first three minutes of the Big Bang and via proton-proton fusion in stars), Earth's atmosphere contains only 5.24 ppmv of helium because thermal Maxwell–Boltzmann velocities of light He atoms (M = 4.00 g mol−1) in the upper exosphere exceed Earth's gravitational escape velocity (vesc = 11.2 km s−1, Jeans escape). Virtually all terrestrial commercial helium is radiogenic 4He (alpha particles, 4He2+) produced by the subterranean α-decay of crustal uranium (238U, 235U) and thorium (232Th) and trapped alongside natural gas deposits.
- Why Argon (0.934%) Is 500 Times More Abundant in Air Than Neon (18.2 ppmv): Even though neon is a major product of carbon/alpha stellar nucleosynthesis in the cosmos, 99.60% of terrestrial atmospheric argon consists of a single radiogenic isotope—40Ar (rather than cosmic 36Ar)—produced continuously over 4.54 billion years by the electron-capture / positron radioactive decay of crustal potassium-40 (40K, t1/2 = 1.248 × 109 years), forming the foundation of K–Ar and 40Ar/39Ar radiometric dating.
Frequently Asked Questions
How can chemically unreactive xenon gas act as a general anesthetic and neuroprotectant in the human brain?
Although atomic xenon forms zero covalent bonds under physiological conditions (37 °C, 1 atm), inhaling a gas mixture containing 50%–70% Xe produces rapid surgical general anesthesia (MAC ≈ 63%–71% atm) without the hemodynamic depression or greenhouse-gas persistence of halogenated ethers. Because xenon's large 5*s*25*p*6 electron cloud is highly polarizable (α = 4.04 Å3), xenon dissolves into hydrophobic protein cavities and binds reversibly via London dispersion and charge-induced dipole forces directly inside the aromatic glycine-binding pocket of neuronal N-methyl-D-aspartate (NMDA) glutamate receptors (as well as two-pore-domain K+ channels, TREK-1). By competitively blocking glycine co-agonist binding to NMDA receptors on postsynaptic neurons, xenon inhibits excitatory glutamatergic neurotransmission and prevents Ca2+-mediated excitotoxicity.
Why is liquid helium the only substance that never solidifies at 1 atm pressure even as temperature approaches absolute zero (0 K)?
For every element except helium, cooling at standard atmospheric pressure (1 atm / 101.3 kPa) reduces thermal kinetic energy until attractive intermolecular forces lock the atoms into a crystalline solid lattice. In helium-4 (4He) and helium-3 (3He), however, two factors combine: (1) helium has the weakest London dispersion attraction of any atom (α = 0.205 Å3, Lennard-Jones well depth ε/kB ≈ 10.2 K), and (2) because the helium nucleus has a very small mass (m = 4 u), confining a helium atom within an interatomic lattice spacing Δ*x* imposes a large Heisenberg zero-point quantum kinetic energy (EZPE ≈ ℏ2 / 2*m*(Δ*x*)2 ≈ 25 K per atom) that exceeds the shallow potential well depth. Consequently, at 1 atm helium remains a quantum liquid all the way down to 0 K, transitioning below Tλ = 2.172 K into a zero-viscosity Bose–Einstein condensate superfluid (Helium II), and solidifying into a crystal only under external pressures exceeding 25 atm (2.5 MPa).
Why is superheavy Element 118 (Oganesson, Og) predicted to behave as a reactive semiconducting solid rather than a noble gas?
In the Period 7 Group 18 element oganesson (Og, Z = 118), valence electrons near the massive Z = 118 nucleus move at relativistic speeds approaching the speed of light (v/c ≈ Zαfs ≈ 0.86). Special-relativistic Dirac–Fock calculations show that spin-orbit coupling splits the 7*p* subshell into a strongly stabilized inner 7*p*1/22 pair and a strongly destabilized, radially expanded outer 7*p*3/24 subshell by roughly 10 eV, while blurring the distinct shell structure of the Electron Localization Function into a uniform Fermi-gas distribution. As a result, oganesson is predicted to have a high polarizability (~5.8 Å3), a positive electron affinity (~0.06–0.08 eV), a narrow band gap (~1.5 eV), and a melting/boiling point above room temperature (~320–380 K)—making Element 118 neither "noble" nor a "gas" at 298 K.
References
- Bartlett, N. (1962). "Xenon hexafluoroplatinate(V) Xe+[PtF6]−." Proceedings of the Chemical Society, 1962(June), 218. https://doi.org/10.1039/PS9620000197
- Claassen, H. H., Selig, H., & Malm, J. G. (1962). "Xenon tetrafluoride." Journal of the American Chemical Society, 84(18), 3593–3593. https://doi.org/10.1021/ja00877a042
- Franks, N. P., Dickinson, R., de Sousa, S. L. M., Hall, A. C., & Lieb, W. R. (1998). "How does xenon produce anaesthesia?" Nature, 396(6709), 324. https://doi.org/10.1038/24525
- Jerabek, P., Schuetrumpf, B., Schwerdtfeger, P., & Nazarewicz, W. (2018). "Electron and nucleon localization functions of oganesson: Approaching the Thomas-Fermi limit." Physical Review Letters, 120(5), 053001. https://doi.org/10.1103/PhysRevLett.120.053001