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  2. Superheavy element - Wikipedia

    en.wikipedia.org/wiki/Superheavy_element

    Superheavy elements, also known as transactinide elements, transactinides, or super-heavy elements, or superheavies for short, are the chemical elements with atomic number greater than 104. [1] The superheavy elements are those beyond the actinides in the periodic table; the last actinide is lawrencium (atomic number 103).

  3. Island of stability - Wikipedia

    en.wikipedia.org/wiki/Island_of_stability

    Despite these unsuccessful attempts to observe long-lived superheavy nuclei, [34] new superheavy elements were synthesized every few years in laboratories through light-ion bombardment and cold fusion [k] reactions; rutherfordium, the first transactinide, was discovered in 1969, and copernicium, eight protons closer to the island of stability ...

  4. Unbihexium - Wikipedia

    en.wikipedia.org/wiki/Unbihexium

    Unbihexium has attracted attention among nuclear physicists, especially in early predictions targeting properties of superheavy elements, for 126 may be a magic number of protons near the center of an island of stability, leading to longer half-lives, especially for 310 Ubh or 354 Ubh which may also have magic numbers of neutrons.

  5. Darmstadtium - Wikipedia

    en.wikipedia.org/wiki/Darmstadtium

    In 1996, the Russian team proposed the name becquerelium after Henri Becquerel. [59] The American team in 1997 proposed the name hahnium [60] after Otto Hahn (previously this name had been used for element 105). The name darmstadtium (Ds) was suggested by the GSI team in honor of the city of Darmstadt, where the element was discovered.

  6. Nihonium - Wikipedia

    en.wikipedia.org/wiki/Nihonium

    The name comes from the common Japanese name for Japan (日本, nihon). Very little is known about nihonium, as it has been made only in very small amounts that decay within seconds. The anomalously long lives of some superheavy nuclides, including some nihonium isotopes, are explained by the island of stability theory.

  7. Unbinilium - Wikipedia

    en.wikipedia.org/wiki/Unbinilium

    The SO interaction is especially strong for the superheavy elements because their electrons move faster—at velocities comparable to the speed of light—than those in lighter atoms. [4] In unbinilium atoms, it lowers the 7p and 8s electron energy levels, stabilizing the corresponding electrons, but two of the 7p electron energy levels are ...

  8. Copernicium - Wikipedia

    en.wikipedia.org/wiki/Copernicium

    In the periodic table of the elements, copernicium is a d-block transactinide element and a group 12 element. During reactions with gold , it has been shown [ 8 ] to be an extremely volatile element, so much so that it is possibly a gas or a volatile liquid at standard temperature and pressure .

  9. Extinct isotopes of superheavy elements - Wikipedia

    en.wikipedia.org/wiki/Extinct_isotopes_of...

    Extinct isotopes of superheavy elements are isotopes of superheavy elements whose half-lives were too short to have lasted through the formation of the Solar System, [1] and because they are not replenished by natural processes, can nowadays only be found as their decay products (from alpha decay, cluster decay or spontaneous fission) trapped within sediment and meteorite samples dating ...

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