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  2. Helium dimer - Wikipedia

    en.wikipedia.org/wiki/Helium_dimer

    However, the van der Waals force exists between helium atoms as shown by the existence of liquid helium, and at a certain range of distances between atoms the attraction exceeds the repulsion. So a molecule composed of two helium atoms bound by the van der Waals force can exist. [4] The existence of this molecule was proposed as early as 1937. [5]

  3. Isotopes of helium - Wikipedia

    en.wikipedia.org/wiki/Isotopes_of_helium

    In Earth's atmosphere, the ratio of 3 He to 4 He is 1.343(13) × 10 −6. [5] However, the isotopic abundance of helium varies greatly depending on its origin. In the Local Interstellar Cloud , the proportion of 3 He to 4 He is 1.62(29) × 10 −4 , [ 6 ] which is ~121 times higher than in Earth's atmosphere.

  4. Lambda point - Wikipedia

    en.wikipedia.org/wiki/Lambda_point

    At pressure of 1 atmosphere, the transition occurs at approximately 2.17 K. The lowest pressure at which He-I and He-II can coexist is the vapor−He-I−He-II triple point at 2.1768 K (−270.9732 °C) and 5.0418 kPa (0.049759 atm), which is the "saturated vapor pressure " at that temperature (pure helium gas in thermal equilibrium over the ...

  5. Helium - Wikipedia

    en.wikipedia.org/wiki/Helium

    [132] [133] The concentration is low and fairly constant despite the continuous production of new helium because most helium in the Earth's atmosphere escapes into space by several processes. [134] [135] [136] In the Earth's heterosphere, a part of the upper atmosphere, helium and hydrogen are the most abundant elements.

  6. Liquid helium - Wikipedia

    en.wikipedia.org/wiki/Liquid_helium

    Liquid helium is a physical state of helium at very low temperatures at standard atmospheric pressures.Liquid helium may show superfluidity.. At standard pressure, the chemical element helium exists in a liquid form only at the extremely low temperature of −269 °C (−452.20 °F; 4.15 K).

  7. Helium-3 - Wikipedia

    en.wikipedia.org/wiki/Helium-3

    The partial pressure of helium in the Earth's atmosphere is about 0.52 pascals (7.5 × 10 −5 psi), and thus helium accounts for 5.2 parts per million of the total pressure (101325 Pa) in the Earth's atmosphere, and 3 He thus accounts for 7.2 parts per trillion of the atmosphere.

  8. Helium compounds - Wikipedia

    en.wikipedia.org/wiki/Helium_compounds

    Noble gas cluster ions exist for different noble gases. Singly charged cluster ions containing xenon exist with the formula He n Xe + m, where n and m ≥ 1. [74] Many different He n Kr + exist with n between 1 and 17, with higher values possible. He n Kr + 2 and He n Kr + 3 also exist for many values of n. He 12 Kr + 2 and He 12 Kr +

  9. Atmosphere of Earth - Wikipedia

    en.wikipedia.org/wiki/Atmosphere_of_Earth

    The atmosphere serves as a protective buffer between the Earth's surface and outer space, shields the surface from most meteoroids and ultraviolet solar radiation, keeps it warm and reduces diurnal temperature variation (temperature extremes between day and night) through heat retention (greenhouse effect), redistributes heat and moisture among ...