Helium
Overview
Helium is the second-lightest element in the universe and the second most abundant, accounting for about one-quarter of all visible matter by mass. The bulk of helium was formed in the moments after the Big Bang, but it has since been produced in the cores of about 90% of stars by fusing hydrogen. In fact, helium is named after the Greek god of the sun—Helios—after it was identified in 1868 via a then-unfamiliar spectral signature in sunlight.
Like other noble gases, helium has a complete outermost shell of electrons around its nucleus, making it largely chemically unreactive. This property makes it an invaluable shield in chemically sensitive processes, such as semiconductor fabrication, fiber optic manufacturing, and arc welding. Because it remains liquid at extremely low temperatures, helium is used as a coolant for superconducting magnets in various scientific equipment, including MRI scanners and particle accelerators. Famously, it also provides buoyancy for weather and party balloons alike and changes one's voice if breathed in.
Beneath Earth's surface, underground deposits of helium produced by radioactive elements can be harvested during natural gas extraction. However, because of its lightness, any that escapes to Earth's atmosphere gets lost to space, contributing to its status as a nonrenewable resource.
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