Dubnium (Db)
transition-metalSolid
Standard Atomic Weight
[268]Electron configuration
[Rn] 7s2 5f14 6d3Melting point
N/ABoiling point
N/ADensity
2.930000e+4 kg/m³Oxidation states
+3, +4, +5Electronegativity (Pauling)
N/AIonization energy (1st)
Discovery year
1967Atomic radius
139 pmDetails
Dubnium is a synthetic transactinide element in group 5, below tantalum. It is known only from accelerator-produced atoms of radioactive isotopes, so its chemistry is studied by rapid, highly sensitive methods rather than by weighing or handling bulk material. Its observed behavior is broadly consistent with a heavy group 5 element, though relativistic effects and nuclear instability make its chemistry experimentally difficult.
Dubnium does not occur naturally in the Earth’s crust. Credit for the first synthesis of this element is given jointly to Albert Ghiorso and his team at the University of California in Berkeley and Georgi Flerov and his team at the Joint Institute for Nuclear Research (JINR) in Dubna, Russia (Fig. IUPAC.105.1). The element is named for the location of the Joint Institute for Nuclear Research (JINR) laboratory in Dubna, Russia [646], [647]. Dubnium has no isotopic applications outside of scientific research.
Dubnium is named after the site of the Joint Institute for Nuclear Research in Dubna, Russia.
Scientists working at the Joint Institute for Nuclear Research in Dubna, Russia, first reported the production of dubnium in 1967. They bombarded atoms of americium-243 with ions of neon-22, forming atoms of dubnium-260 and five free neutrons and atoms of dubnium-261 and four free neutrons. In 1970, a group of scientists working at the Lawrence Radiation Laboratory, now known as the Lawrence Berkeley Laboratory, in Berkeley, California, bombarded atoms of californium-249 with ions of nitrogen-15, forming atoms of dubnium-260 and 4 free neutrons. Credit for the discovery of dubnium is still under debate. Dubnium's most stable isotope, dubnium-268, has a half-life of about 32 hours and decays through spontaneous fission.
In 1967 G.N. Flerov reported that a Soviet team working at the Joint Institute for Nuclear Research at Dubna may have produced a few atoms of 260105 and 261105 by bombarding 243Am with 22Ne. The evidence was based on time-coincidence measurements of alpha energies.
In 1970 Dubna scientists synthesized Element 105 and, by the end of April 1970, "had investigated all the types of decay of the new element and had determined its chemical properties," according to a report in 1970. The Soviet group had not proposed a name for 105. In late April 1970, it was announced that Ghiorso, Nurmia, Haris, K.A.Y. Eskola, and P.L. Eskola, working at the University of California at Berkeley, had positively identified element 105. The discovery was made by bombarding a target of 249Cf with a beam of 84 MeV nitrogen nuclei in the Heavy Ion Linear Accelerator (HILAC). When a15N nuclear is absorbed by a 249Cf nucleus, four neutrons are emitted and a new atom of 260105 with a half-life of 1.6 s is formed. While the first atoms of Element 105 are said to have been detected conclusively on March 5, 1970, there is evidence that Element 105 had been formed in Berkeley experiments a year earlier by the method described.
Ghiorso and his associates have attempted to confirm Soviet findings by more sophisticated methods without success. The Berkeley Group proposed the name hahnium after the late German scientist Otto Hahn (1879-1968) and symbol Ha. However, the International Union of Pure and Applied Chemistry panel members in 1977 recommended that element 105 be named to Dubnium (symbol Db) after the site of the Joint Institute for Nuclear Research in Russia. Unfortunately, the name hahnium will not be used again according to the rules for naming new elements. Some scientists still use the earlier name of hahnium because it had been used for about 25 years.
Images
Properties
Physical
Chemical
Thermodynamic
N/A
Nuclear
Abundance
N/A
Reactivity
N/A
Crystal Structure
N/A
Electronic Structure
Identifiers
Electron Configuration Predicted
Db: 5f¹⁴ 6d³ 7s²[Rn] 5f¹⁴ 6d³ 7s²1s² 2s² 2p⁶ 3s² 3p⁶ 3d¹⁰ 4s² 4p⁶ 4d¹⁰ 5s² 5p⁶ 4f¹⁴ 5d¹⁰ 6s² 6p⁶ 5f¹⁴ 6d³ 7s²Atomic model
Isotopes change neutron count, mass, and stability — not the electron configuration of a neutral atom.
Schematic atomic model, not to scale.
Atomic Fingerprint
Emission / Absorption Spectrum
Isotope Distribution
No stable isotopes.
| Mass number | Atomic mass (u) | Natural abundance | Half-life |
|---|---|---|---|
| 259 Radioactive | 259.109492 ± 0.000057 | N/A | 510 ms |
| 266 Radioactive | 266.12103 ± 0.0003 | N/A | 80 minutes |
| 255 Radioactive | 255.10707 ± 0.00045 | N/A | 54 ms |
| 262 Radioactive | 262.11407 ± 0.00015 | N/A | 34 seconds |
| 263 Radioactive | 263.11499 ± 0.00018 | N/A | 29 seconds |
Phase / State
Phase/state data not available
Atomic Spectra
Showing 10 of 94 Atomic Spectra. Sorted by ion charge (ascending).
Levels Holdings ?
| Ion | Charge | Levels |
|---|---|---|
| Db I | 0 | 2 |
| Db II | +1 | 2 |
| Db III | +2 | 2 |
| Db IV | +3 | 2 |
| Db V | +4 | 2 |
| Db VI | +5 | 2 |
| Db VII | +6 | 2 |
| Db VIII | +7 | 2 |
| Db IX | +8 | 2 |
| Db X | +9 | 2 |
Phase/state data not available
Compounds
Isotopes (5)
In October 1971, it was announced that two new isotopes of element 105 were synthesized with the heavy ion linear accelerator by A. Ghiorso and co-workers a Berkeley. Element 261105 was produced both by bombarding 250Cf with 15N and by bombarding 249Bk with 16O. The isotope emits 8.93-MeV alpha particles and decays to 257Lr with a half-life of about 1.8 s. Element 262105 was produced by bombarding 249Bk with 18O. It emits 8.45 MeV alpha particles and decays to 258Lr with a half-life of about 40 s. Seven isotopes of element 105 (unnilpentium) are now recognized.
| Mass number | Atomic mass (u) | Natural abundance | Half-life | Decay mode | |
|---|---|---|---|---|---|
| 259 Radioactive | 259.109492 ± 0.000057 | N/A | 510 ms | α =100% | |
| 266 Radioactive | 266.12103 ± 0.0003 | N/A | 80 minutes | α ?SF =?β+ ? | |
| 255 Radioactive | 255.10707 ± 0.00045 | N/A | 54 ms | SF ≈67%α ? | |
| 262 Radioactive | 262.11407 ± 0.00015 | N/A | 34 seconds | SF =52±0.4%α =48±0.4%β+ ? | |
| 263 Radioactive | 263.11499 ± 0.00018 | N/A | 29 seconds | SF =56±1.4%α =37±1.4%β+ =6.9±1.6% |
Extended Properties
Covalent Radii (Extended)
Numbering Scales
Polarizability & Dispersion
Oxidation State Categories
Advanced Reference Data
Isotope Decay Modes (35)
| Isotope | Mode | Intensity |
|---|---|---|
| 255 | SF | 67% |
| 255 | A | — |
| 256 | A | 70% |
| 256 | B+ | 30% |
| 256 | SF | — |
| 257 | A | 94% |
| 257 | SF | 6% |
| 257 | B+ | — |
| 258 | A | 64% |
| 258 | B+ | 36% |
Additional Data
Estimated Crustal Abundance
The estimated element abundance in the earth's crust.
Not Applicable
References (1)
Estimated Oceanic Abundance
The estimated element abundance in the earth's oceans.
Not Applicable
References (1)
References
(8)
Data deposited in or computed by PubChem
The half-life and atomic mass data was provided by the Atomic Mass Data Center at the International Atomic Energy Agency.
Element data are cited from the Atomic weights of the elements (an IUPAC Technical Report). The IUPAC periodic table of elements can be found at https://iupac.org/what-we-do/periodic-table-of-elements/. Additional information can be found within IUPAC publication doi:10.1515/pac-2015-0703 Copyright © 2020 International Union of Pure and Applied Chemistry.
The information are cited from Pure Appl. Chem. 2018; 90(12): 1833-2092, https://doi.org/10.1515/pac-2015-0703.
Thomas Jefferson National Accelerator Facility (Jefferson Lab) is one of 17 national laboratories funded by the U.S. Department of Energy. The lab's primary mission is to conduct basic research of the atom's nucleus using the lab's unique particle accelerator, known as the Continuous Electron Beam Accelerator Facility (CEBAF). For more information visit https://www.jlab.org/
The periodic table at the LANL (Los Alamos National Laboratory) contains basic element information together with the history, source, properties, use, handling and more. The provenance data may be found from the link under the source name.
The periodic table contains NIST's critically-evaluated data on atomic properties of the elements. The provenance data that include data for atomic spectroscopy, X-ray and gamma ray, radiation dosimetry, nuclear physics, and condensed matter physics may be found from the link under the source name. Ref: https://www.nist.gov/pml/atomic-spectra-database
This section provides all form of data related to element Dubnium.
