Dubnium
Dubnium is named after Dubna, Russia, site of the Joint Institute for Nuclear Research (JINR) where it was first clearly synthesised. Only a handful of atoms are made at a time; they decay within seconds.
- Atomic Number105105 protons, 105 electrons
- Atomic Mass268.126 uOver 105× heavier than hydrogen
- State at Room TempSolidpredicted solid
- DensityNot measuredPredicted from periodic trends
- Melting / BoilingNot yet measuredDecays in milliseconds to hours
- Discovered1967First produced 1967s
What is Dubnium?
Db-268 has a half-life of approx. 28 hours. First produced in 1968 at Dubna. Named after Dubna, Russia, to reflect the Soviet role in its discovery. The Berkeley team called it hahnium for several years in a naming dispute.
With 105 protons, Dubnium sits in Group 5 of the periodic table, Period 7, in the superheavy transactinide region. Its properties are predicted largely from theory and from single-atom chemistry experiments, not from bulk measurements.
Where you find Dubnium
On Earth
Dubnium does not exist naturally. It is made only artificially in nuclear physics laboratories by firing beams of one heavy nucleus at another and watching for the rare collisions that fuse them together. The main laboratories capable of producing superheavy elements are JINR in Dubna (Russia), GSI in Darmstadt (Germany), RIKEN in Japan and Lawrence Livermore National Laboratory in California.
How we use Dubnium
Dubnium has no practical uses. Only a handful of atoms have ever been produced, each existing for a fraction of a second to a few minutes. Research focuses on understanding nuclear structure, testing theoretical models of the atom, and searching for the predicted "island of stability", a region of superheavy nuclei that may be significantly longer-lived than those currently known.
How it was discovered
Db-268 has a half-life of approx. 28 hours. First produced in 1968 at Dubna. Named after Dubna, Russia, to reflect the Soviet role in its discovery. The Berkeley team called it hahnium for several years in a naming dispute.
Deeper dive: superheavy elements and the island of stability
Nuclear physicists predict that certain combinations of protons and neutrons, "magic numbers", create particularly stable nuclei. For superheavy elements, a theoretical "island of stability" is predicted around element 114 (flerovium) or beyond, where nuclei with the right magic number of neutrons might have half-lives of years or even longer rather than milliseconds. So far, the search continues. Elements 113-118 were all officially confirmed and named in 2016, completing Period 7 of the periodic table. Whether an eighth period of elements beyond oganesson (118) can ever be made and studied remains one of the great open questions in chemistry and nuclear physics.
Superheavy elements are made by accelerating beams of lighter nuclei (often calcium-48, because of its convenient doubly-magic structure) to high energies and firing them at heavy targets (lead, bismuth, uranium, curium, californium). Very rarely, two nuclei fuse instead of bouncing apart. The fusion product is detected by its characteristic radioactive decay chain, a signature sequence of alpha decays each producing a known element, counted backwards to identify the original product.
Moving to 106 protons on the periodic table brings us to the next superheavy element.