Moscovium
Moscovium is named after the Moscow Oblast, the Russian region where the JINR laboratory in Dubna is located. It was first synthesised in 2003 in a collaboration between Dubna and Lawrence Livermore.
- Atomic Number115115 protons, 115 electrons
- Atomic Mass290.196 uOver 115× heavier than hydrogen
- State at Room TempExpected to be a Solidpredicted solid
- DensityNot measuredPredicted from periodic trends
- Melting / BoilingNot yet measuredDecays in milliseconds to hours
- Discovered2003First produced 1997s
What is Moscovium?
Mc-290 has a half-life of approx. 650 milliseconds. Officially recognised in 2016. Sits below bismuth in Group 15. Named moscovium (Mc) to honour the Moscow region of Russia.
With 115 protons, Moscovium sits in Group 15 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 Moscovium
On Earth
Moscovium 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 Moscovium
Moscovium 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
Mc-290 has a half-life of approx. 650 milliseconds. Officially recognised in 2016. Sits below bismuth in Group 15. Named moscovium (Mc) to honour the Moscow region of Russia.
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 116 protons on the periodic table brings us to the next superheavy element.