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.

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