Overview

Helium is the second-lightest element in the universe and the second most abundant, comprising 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.

1440 Findings

Hours of research by our editors, distilled into minutes of clarity.

  • An overview of helium, the nonrenewable resource that's lighter than air

    The second element in the periodic table naturally forms deep underground over the course of billions of years through the decay of radioactive elements, but it is used and lost to space at rates faster than it is generated. Because of this and its extensive applications in scientific technologies, scientists continue to seek avenues for its exploration, storage, and recycling.

  • How scientists discovered helium from sunlight over a decade before seeing it on Earth

    In 1868, using tools that dispersed light into its constituent colors like a prism, astronomers Pierre Janssen and Joseph Norman Lockyer independently identified a bright yellow line in the solar spectrum that didn't match any known element. Fourteen years later, amid continued skepticism over the existence of a new element, the same spectral signature was observed in lava on Earth.

  • Why Earth's atmosphere constantly loses the universe's lightest elements to space

    The masses of hydrogen and helium are too small for these gases to be held by Earth's gravitational force, particularly when these atoms are given energy from collisions with high-speed particles from the sun. Although the planet loses a meter-wide balloon's worth of hydrogen every second, it will still take billions of years to exhaust the planet of this element.

  • Why stories about helium 'running out' indicate market volatility rather than scarcity

    Only a few locations on Earth contain natural gas reserves with sufficiently high helium concentrations to make their extraction commercially viable, and geopolitical conflicts in these areas significantly affect helium production. This makes cost a major impediment to helium availability, particularly for scientific research, amid growing demand and ongoing depletion of reserves that took billions of years to form.

  • Why helium helped preserve the US's founding documents, but was later replaced

    In 1951, the Charters of Freedom were stored in glass and metal cases filled with helium, which would not chemically react with the documents. After microscopic cracks were identified in the glass through which helium could leak out of and, experts feared, pollutants could infiltrate, new encasements made of aluminum, titanium, and argon replaced the old system in 2003.

  • How helium enables MRI machines to look inside organisms

    By cooling the machine's magnets with liquid helium to extremely low temperatures, they can generate and maintain powerful magnetic fields that align the hydrogen atoms in living things to point toward a patient's head or feet. A radio pulse nudges these atoms, which realign and induce a measurable signal in nearby electrical coils. These signals are captured in slices and then stacked into a 3D reconstruction.

  • Why trying to freeze helium creates a fluid that can travel through solids and climb walls

    Once cooled to temperatures just above 2 Kelvin, helium-4 atoms begin to exhibit superfluidity, a quantum property in which all atoms collectively inhabit the same low-energy state and behave in perfect unison. This coordination removes the internal friction that causes liquids to cling to surfaces, allowing them to slide through microscopic pores and scale container walls.

  • Why breathing helium, sulfur hexafluoride, and other gases changes your voice

    The speed of sound varies depending on the properties of the material it travels through, including its density. Because helium is less dense than air, sound travels faster, altering the timbre of one's voice to be squeakier by enhancing its higher frequencies. In molecules that are heavier than air, low-frequency sounds are enhanced, producing a deeper voice.

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