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  2. Atmospheric escape - Wikipedia

    en.wikipedia.org/wiki/Atmospheric_escape

    Heavier molecules are less likely to escape because they move slower than lighter molecules at the same temperature. This is why hydrogen escapes from an atmosphere more easily than carbon dioxide. Second, a planet with a larger mass tends to have more gravity, so the escape velocity tends to be greater, and fewer particles will gain the energy ...

  3. Interstellar medium - Wikipedia

    en.wikipedia.org/wiki/Interstellar_medium

    This is much faster than the random motions of atoms in the ISM, but since the orbital motion of the gas is coherent, the average motion does not directly affect structure in the ISM. The vertical scale height of the ISM is set in roughly the same way as the Earth's atmosphere, as a balance between the local gravitation field (dominated by the ...

  4. Atomic diffusion - Wikipedia

    en.wikipedia.org/wiki/Atomic_diffusion

    For example, along the grain boundaries and certain crystalline defects such as dislocations there is more open space, thereby allowing for a lower activation energy for diffusion. Atomic diffusion in polycrystalline materials is therefore often modeled using an effective diffusion coefficient , which is a combination of lattice, and grain ...

  5. Nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Nucleosynthesis

    The amounts of total mass in elements heavier than hydrogen and helium (called 'metals' by astrophysicists) remains small (few percent), so that the universe still has approximately the same composition. Stars fuse light elements to heavier ones in their cores, giving off energy in the process known as stellar nucleosynthesis.

  6. Ionization - Wikipedia

    en.wikipedia.org/wiki/Ionization

    The trend in the ionization energy of atoms is often used to demonstrate the periodic behavior of atoms with respect to the atomic number, as summarized by ordering atoms in Mendeleev's table. This is a valuable tool for establishing and understanding the ordering of electrons in atomic orbitals without going into the details of wave functions ...

  7. The Vacuum of Space Won't Last Forever. In Fact, It ... - AOL

    www.aol.com/vacuum-space-wont-last-forever...

    The decay of the vacuum of space will occur if the Higgs field tunnels, like skipping the line, to a higher overall energy setting. Our universe has an overall equilibrium that will shred apart if ...

  8. Reionization - Wikipedia

    en.wikipedia.org/wiki/Reionization

    The neutral hydrogen had been ions at an earlier stage in the history of the universe, thus the conversion back into ions is termed a reionization. The reionization was driven by energetic photons emitted by the first stars and galaxies. [1] In the timeline of the universe, neutral hydrogen gas was originally formed when primordial hydrogen ...

  9. Molecules in stars - Wikipedia

    en.wikipedia.org/wiki/Molecules_in_stars

    Matter is made up by atoms (formed by protons and other subatomic particles). When the environment is right, atoms can join together and form molecules, which give rise to most materials studied in materials science. But certain environments, such as high temperatures, don't allow atoms to form molecules, as the environmental energy exceeds ...