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  2. Helium - Wikipedia

    en.wikipedia.org/wiki/Helium

    Helium (from Greek: ἥλιος, romanized: helios, lit. 'sun') is a chemical element; it has symbol He and atomic number 2. It is a colorless, odorless, non-toxic, inert, monatomic gas and the first in the noble gas group in the periodic table.

  3. Helium-3 - Wikipedia

    en.wikipedia.org/wiki/Helium-3

    [18] [19] Samples of the lithium ore spodumene from Edison Mine, South Dakota were found to contain 12 parts of helium-3 to a million parts of helium-4. Samples from other mines showed 2 parts per million. [18] Helium is also present as up to 7% of some natural gas sources, [20] and large sources have over 0.5% (above 0.2% makes it viable to ...

  4. Noble gas - Wikipedia

    en.wikipedia.org/wiki/Noble_gas

    Pierre Janssen and Joseph Norman Lockyer had discovered a new element on 18 August 1868 while looking at the chromosphere of the Sun, and named it helium after the Greek word for the Sun, ἥλιος (hḗlios). [9] No chemical analysis was possible at the time, but helium was later found to be a noble gas.

  5. Nuclear fusion - Wikipedia

    en.wikipedia.org/wiki/Nuclear_fusion

    The Sun is a main-sequence star, and, as such, generates its energy by nuclear fusion of hydrogen nuclei into helium. In its core, the Sun fuses 620 million metric tons of hydrogen and makes 616 million metric tons of helium each second. The fusion of lighter elements in stars releases energy and the mass that always accompanies it.

  6. The fate of America's largest supply of helium is up in the air

    www.aol.com/fate-america-largest-supply-helium...

    The Federal Helium Reserve was supposed to be sold off in 2021. Scientists hope it will remain in government hands. The fate of America's largest supply of helium is up in the air

  7. Standard solar model - Wikipedia

    en.wikipedia.org/wiki/Standard_solar_model

    For example, since the Sun formed, some of the helium and heavy elements have settled out of the photosphere by diffusion. As a result, the Solar photosphere now contains about 87% as much helium and heavy elements as the protostellar photosphere had; the protostellar Solar photosphere was 71.1% hydrogen, 27.4% helium, and 1.5% metals. [2]

  8. Solar System - Wikipedia

    en.wikipedia.org/wiki/Solar_System

    The Sun is a typical star that maintains a balanced equilibrium by the fusion of hydrogen into helium at its core, releasing this energy from its outer photosphere. Astronomers classify it as a G-type main-sequence star. The largest objects that orbit the Sun are the eight planets.

  9. Scientists obtain image of a star on the precipice of disaster

    www.aol.com/news/scientists-obtain-image-star...

    For instance, the sun is already more than 4.5 billion years old and has billions more to go. WOH G64's diameter is immense as it puffs up before its expected explosion in the relatively near future.