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  2. Neon - Wikipedia

    en.wikipedia.org/wiki/Neon

    Neon is a colorless, odorless, inert monatomic gas under standard conditions, with approximately two-thirds the density of air. Neon was discovered in 1898 alongside krypton and xenon, identified as one of the three remaining rare inert elements in dry air after the removal of nitrogen, oxygen, argon, and carbon dioxide.

  3. Oxygen - Wikipedia

    en.wikipedia.org/wiki/Oxygen

    Oxygen: Fluorine: Neon: Sodium: ... has shown that the Sun has a higher proportion of oxygen-16 than does the ... inhales 1.8 to 2.4 grams of oxygen per ...

  4. Lifting gas - Wikipedia

    en.wikipedia.org/wiki/Lifting_gas

    Only certain lighter than air gases are suitable as lifting gases. Dry air has a density of about 1.29 g/L (gram per liter) at standard conditions for temperature and pressure (STP) and an average molecular mass of 28.97 g/mol, [1] and so lighter-than-air gases have a density lower than this.

  5. Prices of chemical elements - Wikipedia

    en.wikipedia.org/wiki/Prices_of_chemical_elements

    Hydrogen, nitrogen, oxygen and chlorine are cheapest by volume at atmospheric pressure. When there is no public data on the element in its pure form, price of a compound is used, per mass of element contained. This implicitly puts the value of compounds' other constituents, and the cost of extraction of the element, at zero.

  6. Noble gas - Wikipedia

    en.wikipedia.org/wiki/Noble_gas

    For instance, argon, krypton, and xenon form clathrates with hydroquinone, but helium and neon do not because they are too small or insufficiently polarizable to be retained. [61] Neon, argon, krypton, and xenon also form clathrate hydrates, where the noble gas is trapped in ice. [62] An endohedral fullerene compound containing a noble gas atom

  7. Standard atomic weight - Wikipedia

    en.wikipedia.org/wiki/Standard_atomic_weight

    In 2015, the atomic weight of ytterbium was updated. [17] Per 2017, 14 atomic weights were changed, including argon changing from single number to interval value. [18] [19] The value published can have an uncertainty, like for neon: 20.1797(6), or can be an interval, like for boron: [10.806, 10.821].

  8. Oxygen-burning process - Wikipedia

    en.wikipedia.org/wiki/Oxygen-burning_process

    As a result, neon burning occurs at lower temperatures than 16 O + 16 O. [9] During neon burning, oxygen and magnesium accumulate in the core of the star. At the onset of oxygen burning, oxygen in the stellar core is plentiful due to the helium-burning process (4 He(2α,γ) 12 C(α,γ) 16 O), carbon-burning process (12 C(12 C,α) 20 Ne, 12 C(α ...

  9. Atomic mass - Wikipedia

    en.wikipedia.org/wiki/Atomic_mass

    However, because oxygen-17 and oxygen-18 are also present in natural oxygen this led to two different tables of atomic mass. The unified scale based on carbon-12, 12 C, met the physicists' need to base the scale on a pure isotope, while being numerically close to the chemists' scale.