Island of stability
The island of stability is a term from nuclear physics, which describes the possibility of elements which have particularly stable "magic numbers" of protons and neutrons. This would allow certain isotopes of some transuranic elements to be far more stable than others, and thus decay much more slowly.
The idea of the island of stability was first proposed by Glenn T. Seaborg. The hypothesis is that the atomic nucleus is built up in "shells" in a manner similar to the electron shells in atoms. In both cases shells are just groups of quantum energy levels that are relatively close to each other. Energy levels from quantum states in two different shells will be separated by a relatively large energy gap. So when the numbers of neutrons and protons completely fill the energy levels of a given shell in the nucleus, then the binding energy per nucleon will reach a local minimum and thus that particular configuration will have a longer lifetime than nearby isotopes that do not have filled shells.
A filled shell would have "magic numbers" of neutrons and protons. One possible magic number of neutrons is 184, and some possible matching proton numbers are 114, 120 and 126 — which would mean that the most stable possible isotopes would be ununquadium-298, unbinilium-304 and unbihexium-310. Of particular note is Ubh-310, which would be "doubly magic" (both its proton number of 126 and neutron number of 184 are thought to be magic) and thus the most likely to have a very long half-life. The next lighter doubly-magic nucleus is Lead-208, the heaviest stable nucleus and most stable heavy metal. None of these isotopes has yet been produced. Isotopes of elements 110 through 114 have been produced and these isotopes are significantly slower to decay than isotopes of nearby nuclei on the periodic table.
The following table shows information about predicted (and observed) isotopes of elements 110 through 120. Keep in mind that half-lifes do not match decay time for individual atoms.
Number | Name | # isotopes (known) | # isotopes observed | Predicted longest half-life | Observed longest half-life | Link |
---|---|---|---|---|---|---|
110 | darmstadtium | 15 | 10 | 11 s | 210 ms | Isotopes of darmstadtium |
111 | roentgenium | 12 | 4 | 10 min | 3.6 s | Isotopes of roentgenium |
112 | ununbium | 9 | 1 | 10 s | 1.1 ms | Isotopes of ununbium |
113 | ununtrium | 6 | 2 | 20 min | 480 ms | Isotopes of ununtrium |
114 | ununquadium | 5 | 4 | 2.6 s | 2.6 s | Isotopes of ununquadium |
115 | ununpentium | 5 | 2 | 1 min | 87 ms | Isotopes of ununpentium |
116 | ununhexium | 5 | 4 | 61 ms | 61 ms | Isotopes of ununhexium |
117 | ununseptium | 2 | 0 | N/A | N/A | Isotopes of ununseptium |
118 | ununoctium | 1 | 0 | N/A | N/A | Isotopes of ununoctium |
119 | ununennium | 0 | 0 | N/A | N/A | Isotopes of ununennium |
120 | unbinilium | 0 | 0 | N/A | N/A | Isotopes of unbinilium |
The half lives of elements in the island are uncertain. Many physicists think they are relatively short, on the order of minutes, hours, or perhaps days. However, some theoretical calculations indicate that their half lives may be long (some calculations put it on the order of 109 years)[citation needed]. Many chemists and science fiction writers have claimed that these elements could have unusual properties, and, if long lived enough, various applications (such as targets in nuclear physics and neutron sources). However after the isolation of several of these elements, the island of stability still hasn't been reached.
Island of relative stability
232Th (thorium), 235U and 238U (uranium) are the only naturally occurring isotopes beyond bismuth that are relatively stable over the current lifespan of the universe. Bismuth was found to be unstable in 2003, with an α-emission half-life of 1.9 × 1019 years for Bi-209. All other isotopes beyond bismuth are relatively or very unstable. So the main periodic table ends at bismuth, with an island at thorium and uranium. Between bismuth and thorium there is an island of severe instability, which renders such elements as astatine, radon, and francium extremely short-lived relative to all but the heaviest elements found so far.
Another island
The relatively unstable elements reach up to 257Fm (fermium), after which they get very unstable due to spontaneous fission until somewhat more stable, spherical nuclei are obtained at the island of stability, set in the ocean of instability.
External links
- The synthesis of spherical superheavy nuclei in 48Ca induced reactions
- Uut and Uup Add Their Atomic Mass to Periodic Table
- New elements discovered and the island of stability sighted
- First postcard from the island of nuclear stability
- Second postcard from the island of stability
- Superheavy Elements "Island of Stability"
- Superheavy elements
- Can superheavy elements (such as Z=116 or 118) be formed in a supernova? Can we observe them?
- In search of the island of stability - New observations (as of August 2006) may help extend the periodic table.
See also
- Island of stability : Ununquadium – Unbinilium – Unbihexium
- Isotope table and Isotope table (divided) - the best visualization of the island of stability
- Periodic table and Periodic table (extended)