helium-4
Quick Summary
Helium-4 (4He) is a stable isotope of helium, the second lightest element. It is the most abundant stable isotope of helium, outnumbering helium-3 by a significant margin. The nucleus of helium-4 contains two protons and two neutrons, giving it a mass number of four.1
Helium-4 is produced naturally through radioactive decay, specifically as alpha particles ejected from the nuclei of heavier radioactive elements. While helium is abundant in the universe, particularly in stars where it's formed by nuclear fusion, its presence in Earth's atmosphere is minimal due to its low density, which allows it to escape into space.1
Liquid helium-4 exhibits unique properties, including superfluidity below 2.18 K, a state where it flows with virtually no viscosity. This characteristic makes it invaluable in cryogenics for achieving extremely low temperatures. Helium-4 is also used in welding, rocket propulsion, and as a lifting gas for balloons.1
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heliumAbundance and isotopes…or 3He) and four (helium-4, or 4He) are stable; all the others are radioactive, decaying very rapidly into other substances. The helium that is present on Earth is not a primordial component but has been generated by radioactive decay. Alpha particles, ejected from the nuclei of heavier radioactive substances,…
Read More…or 3He) and four (helium-4, or 4He) are stable; all the others are radioactive, decaying very rapidly into other substances. The helium that is present on Earth is not a primordial component but has been generated by radioactive decay. Alpha particles, ejected from the nuclei of heavier radioactive substances,…
Read More- superfluidityDiscovery
…protons and one neutron, and helium-4 (or 4He), with two protons and two neutrons. 4He forms the bulk of naturally occurring helium, but the lighter isotope 3He has been formed, since about 1950, in experimentally useful quantities by the decay of tritium produced in nuclear reactors.
Read More…protons and one neutron, and helium-4 (or 4He), with two protons and two neutrons. 4He forms the bulk of naturally occurring helium, but the lighter isotope 3He has been formed, since about 1950, in experimentally useful quantities by the decay of tritium produced in nuclear reactors.
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