Helium - 2He: the essentials
- Name: helium
- Symbol: He
- Atomic number: 2
- Relative atomic mass (Ar): 4.002602 (2) g, r [see notes g r]
- Standard state: gas at 298 K
- Appearance: colourless
- Classification: Non-metallic
- Group in periodic table: 18
- Group name: Noble gas
- Period in periodic table: 1
- Block in periodic table: p
- Shell structure: 2
- CAS Registry: 7440-59-7
Helium atoms have 2 electrons and the shell structure is 2. The ground state electronic configuration of neutral helium is 1s2 and the term symbol of helium is 1S0.
Helium: description
Helium is one of the so-called noble gases. Helium gas is an unreactive, colourless, and odourless monoatomic gas. Helium is available in pressurised tanks.
Helium is the second most abundant element in the universe after hydrogen. α-particles are doubly ionised helium atoms, He2+.
Helium is used in lighter than air balloons and while heavier than hydrogen, is far safer since helium does not burn. Speaking after breathing an atmosphere rich in helium results in a squeaky voice (don't try it!).
Helium is present in the atmosphere at about 0.0005% (1 part in 200000) by volume and is an important component within hydrocarbon gases in the USA. Its origin in these gases is traced to the decay of radioactive elements in rocks.
Emma's first birthday balloon is filled with helium and so rises in air.
Helium: physical properties
- Density of solid: 214 kg m-3
- Molar volume: 21.00 cm3
- Thermal conductivity: 0.1513 W m‑1 K‑1
Helium: heat properties
- Melting point: 0.95 [‑272.2 °C (‑458 °F)] K
- Boiling point: 4.22 [‑268.93 °C (‑452.07 °F)] K
- Enthalpy of fusion: 20.5 kJ mol-1
Helium: atom sizes
- Atomic radius (empirical): (no data) pm
- Molecular single bond covalent radius: 46 (coordination number 1,2) ppm
- van der Waals radius: [ 143 ] ppm
Helium: electronegativities
- Pauling electronegativity: (no data) (Pauling units)
- Allred Rochow electronegativity: 5.50 (Pauling units)
- Mulliken-Jaffe electronegativity: 3.49 (s orbital)
Helium: orbital properties
- First ionisation energy: 2372.32 kJ mol‑1
- Second ionisation energy: 5250.51 kJ mol‑1
- Third ionisation energy: (no data) kJ mol‑1
Helium: abundances
- Universe: 230000000 ppb by weight
- Crustal rocks: 5.5 ppb by weight
- Human: (no data) ppb by weight
Helium: crystal structure
Helium: biological data
- Human abundance by weight: (no data) ppb by weight
Helium has no biological role.
Helium: uses
Helium: reactions
Reactions of helium as the element with air, water, halogens, acids, and bases where known.
Helium: binary compounds
Binary compounds with halogens (known as halides), oxygen (known as oxides), hydrogen (known as hydrides), and other compounds of helium where known.
Helium: compound properties
Bond strengths; lattice energies of helium halides, hydrides, oxides (where known); and reduction potentials where known.
Helium: history
Helium was discovered by Sir William Ramsay and independently by N. A. Langley and P. T. Cleve in 1895 at London, England and Uppsala, Sweden. Origin of name: from the Greek word "helios" meaning "sun".Helium: isotopes
Helium has two isotopes but it consists almost entirely of He-4 with natural He only containing just over 0.0001% of He-3. Thousands of liters of He-3 are used annually in cryogenic applications and He-3 is also used as a neutron counter in nuclear application. He-3 is also applied in magnetic resonance imaging.
Helium: isolation
Isolation: there is very little helium on earth as nearly all present during and immediately after the earth's formation has long since been lost as it is so light. Just about all the helium remaining on the planet is the result of radioactive decay. While there is some helium in the atmosphere, currently its isolation from that source by liquefaction and separation of air is not normally economic. This is bacause it is easier, and cheaper, to isolate the gas from certain natural gases. Concentrations of helium in natural gas in the USA are as high as 7% and other good sources include natural gas from some sources in Poland. It is isolable from these gases by liquefaction and separation of from the natural gas. This would not normally be carried out in the laboratory and helium is available commercially in cylinders under pressure.