Fermium (Fm)
actinideSolid
Standard Atomic Weight
[257]Electron configuration
[Rn] 5f12 7s2Melting point
1526.85 °C (1800 K)Boiling point
N/ADensity
9700 kg/m³Oxidation states
+2, +3Electronegativity (Pauling)
1.3Ionization energy (1st)
Discovery year
1952Atomic radius
N/ADetails
Fermium is a synthetic actinide and the element with atomic number 100. It is produced only in minute amounts in high-neutron-flux reactions and is studied mainly by radiochemical and nuclear methods. Its chemistry is dominated by the +3 oxidation state, broadly resembling that of other late actinides and lanthanides. No macroscopic metallic sample has been prepared, and most measured properties are isotope- or solution-specific.
Fermium does not occur naturally in the Earth’s crust. It was first identified in December 1952 by American scientists from the Argonne National Laboratory near Chicago, Illinois, the Los Alamos National Laboratory in Los Alamos, New Mexico, and The University of California Laboratory in Berkeley, California in the debris of thermonuclear weapons (Fig. IUPAC.100.1). The element was named for Enrico Fermi, who built the first man-made nuclear reactor. 255Fm (with a half-life of 20 h) was the first fermium isotope identified. Fermium is the heaviest element that can be formed by neutron bombardment of lighter elements and is thus the heaviest element that can be synthesized in macroscopic quantities [632], [633].
Fermium is of interest in particle physics research, but it has no commercial applications. 253Fm was one of the decay products used to confirm synthesis of copernicium in a particle accelerator experiment [634].
Fermium is the heaviest synthetic element that can be formed by neutron bombardment of lighter elements, and hence the heaviest element that can be prepared in macroscopic quantities. The chemical properties of fermium have been studied solely using tracer amounts and innovative experimental techniques are required. Fermium metal has not been prepared, however measurements have been made on fermium alloys with rare earth metals and a number of predictions have been made. It was deduced that fermium metal prefers a divalent state but with modest compression can form a trivalent state. Other measurements on mixed fermium alloys and compounds include the magnetic moment, inner-shell binding energies, x-ray energies, sublimation enthalpy, etc.
The chemistry of fermium is typical of the late actinides, with a dominance of the +3 oxidation state but also a tendency toward an accessible +2 oxidation state. In the solid state no pure fermium compounds have been prepared, however Fm(III) has been studied by co-crystallization techniques as a trace component in a rare earth matrix with the same charge. Fermium co-precipitates with rare earth fluorides and hydroxides. In aqueous solution, fermium exists in solution as the Fm3+ ion, which has a hydration number of 16.9 and an acid dissociation constant of 1.6 × 10-4 (pKa = 3.8). Fm3+ forms complexes with a wide variety of organic ligands with hard donor atoms such as oxygen, and these complexes are usually more stable than those of the lighter actinides. It also forms complexes with ligands such as chloride or nitrate and, again, these complexes appear to be more stable than those formed by einsteinium or californium. Bonding in the heavier actinides is mostly ionic in character and the ionic radius of the Fm3+ ion is smaller than the preceding An3+ ions because of the actinide contraction. This is the result of a higher effective nuclear charge of fermium, and thus fermium forms shorter and stronger metal–ligand bonds. In the heavier actinides there is an increasing tendency to form a divalent ion that emerges at einsteinium. Fm3+ can be readily reduced to stable Fm2+ using moderately strong reducing agents such as samarium(II) chloride. In aqueous media, the Fm(III)/Fm(III) redox couple has been investigated via radio-electrochemistry and other techniques. The electrode potentials have been estimated to be similar to that of the ytterbium redox couple. The redox potentials for the various fermium couples have been measured and/or estimated by various workers: Fm3+ → Fm2+ (- 1.15 V); Fm2+ → Fm0 (-2.37 V), all versus the Normal Hydrogen Electrode.
Fermium was discovered by a team of scientists led by Albert Ghiorso in 1952 while studying the radioactive debris produced by the detonation of the first hydrogen bomb. The isotope they discovered, fermium-255, has a half-life of about 20 hours and was produced by combining 17 neutrons with uranium-238, which then underwent eight beta decays. Today, fermium is produced though a lengthy chain of nuclear reactions that involves bombarding each isotope in the chain with neutrons and then allowing the resulting isotope to undergo beta decay. Fermium's most stable isotope, fermium-257, has a half-life of about 100.5 days. It decays into californium-253 through alpha decay or decays through spontaneous fission.
Fermium, element 100, is the eighth transuranium element of the actinide series and is named after the Italian physicist and Nobel Laureate Enrico Fermi. Element 100 was first discovered in 1952 in the fallout from the 10-megaton "Ivy Mike" nuclear test in the south Pacific the first successful test of a hydrogen fusion bomb. Researchers identified a new Pu-244 isotope found on filter papers on drone aircraft flown through the fallout. They determined that it could only have formed by the unexpected absorption of six neutrons by uranium-238 followed by successive beta-decays. At the time, the absorption of neutrons by a heavy nucleus was thought to be a rare process, but the identification of Pu-244 raised the possibility that still more neutrons could have been absorbed by the uranium nuclei leading to additional new elements.
Element 99, einsteinium was discovered almost immediately on other filter papers by Albert Ghiorso and co-workers at the Lawrence Berkeley Laboratory in collaboration with Argonne and Los Alamos National Laboratories, demonstrating that 15 neutrons were captured by U-238! The subsequent discovery of fermium required more material, as the yield of element 100 was expected to be at least an order of magnitude lower than that of einsteinium. So, contaminated coral from ground zero on Eniwetok atoll was shipped to Berkeley for processing and analysis. About two months after the Ivy-Mike test, a new activity was isolated emitting high-energy α-particles (7.1 MeV) with a half-life of about 1 day. It was the β- decay daughter of an isotope of einsteinium, and it had to be an isotope of element 100. : It was identified as 255Fm (half-life 20.07 hours). The discovery of the new elements, and the new data on neutron capture, was kept secret on the orders of the U.S. Military until 1955 due to Cold War tensions. Later the Berkeley team was able to prepare elements 99 and 100 in the lab by neutron bombardment of Pu-239 in a cyclotron. They published this work in 1954, with the disclaimer that these were not the first studies that had been carried out on the element. The 'Ivy Mike' studies were later declassified and published in 1955. Meanwhile, a group at the Nobel Institute for Physics in Stockholm independently claimed discovery of element 100 by producing an isotope with a 30-minute half-life and published their work in May 1954. Nevertheless, the historical precedence of the Berkeley team was generally recognized, and with it the prerogative to name the new element in honor of the recently deceased Enrico Fermi, the developer of the first artificial self-sustained nuclear reactor.
Images
Properties
Physical
Chemical
Thermodynamic
Nuclear
Abundance
N/A
Reactivity
N/A
Crystal Structure
N/A
Electronic Structure
Identifiers
Electron Configuration Measured
Fm: 5f¹² 7s²[Rn] 5f¹² 7s²1s² 2s² 2p⁶ 3s² 3p⁶ 3d¹⁰ 4s² 4p⁶ 4d¹⁰ 5s² 5p⁶ 4f¹⁴ 5d¹⁰ 6s² 6p⁶ 5f¹² 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 |
|---|---|---|---|
| 242 Radioactive | 242.07343 ± 0.00043 | N/A | 800 us |
| 241 Radioactive | 241.07421 ± 0.00032 | N/A | 730 us |
| 258 Radioactive | 258.09708 ± 0.00022 | N/A | 370 us |
| 243 Radioactive | 243.07446 ± 0.00023 | N/A | 231 ms |
| 256 Radioactive | 256.0917745 ± 0.0000078 | N/A | 157.1 minutes |
Phase / State
Reason: 1501.8 °C below sublimation point (1526.85 °C)
Schematic, not to scale
Phase transition points
Transition energies
Energy required to sublime 1 mol at sublimation point
Density
At standard conditions
At standard conditions
Atomic Spectra
Showing 10 of 100 Atomic Spectra. Sorted by ion charge (ascending).
Levels Holdings ?
| Ion | Charge | Levels |
|---|---|---|
| Fm I | 0 | 2 |
| Fm II | +1 | 2 |
| Fm III | +2 | 2 |
| Fm IV | +3 | 2 |
| Fm V | +4 | 2 |
| Fm VI | +5 | 2 |
| Fm VII | +6 | 2 |
| Fm VIII | +7 | 2 |
| Fm IX | +8 | 2 |
| Fm X | +9 | 2 |
Crystal structure data not available
Ionic Radii
| Charge | Coordination | Spin | Radius |
|---|---|---|---|
| +3 | 9 | N/A | 110.5 pm |
Compounds
Isotopes (5)
A total of 21 known isotopes of fermium exist with atomic weights from 242 to 260, including 2 that are metastable. Fermium-257 is the longest-lived with a half-life of 100.5 days. Other relatively long-lived isotopes include Fm-253 (3 days), Fm-252 (25.4 hours) and Fm-255 (~20 hours). Fm-250, with a half-life of 30 minutes, was shown to be a decay product of nobelium, element 102 and the chemical identification of the isotope 250Fm confirmed the production and discovery of element 102. All the remaining isotopes of fermium have half-lives ranging from 30 minutes to less than a millisecond. The neutron-capture product of fermium-257, 258Fm, undergoes spontaneous fission with a half-life of just 370 microseconds; 259Fm and 260Fm are also unstable with respect to spontaneous fission (t½ = 1.5 s and 4 ms respectively). This means that the neutron capture production chain essentially terminates at mass number 257 because of the very short spontaneous fission half-lives of the heavier isotopes.
| Mass number | Atomic mass (u) | Natural abundance | Half-life | Decay mode | |
|---|---|---|---|---|---|
| 242 Radioactive | 242.07343 ± 0.00043 | N/A | 800 us | SF ≈100%α ? | |
| 241 Radioactive | 241.07421 ± 0.00032 | N/A | 730 us | SF =?α<14% β+<12% | |
| 258 Radioactive | 258.09708 ± 0.00022 | N/A | 370 us | SF ≈100%α ? | |
| 243 Radioactive | 243.07446 ± 0.00023 | N/A | 231 ms | α =91±0.3%SF =9±0.3%β+ ? | |
| 256 Radioactive | 256.0917745 ± 0.0000078 | N/A | 157.1 minutes | SF =91.9±0.3%α =8.1±0.3% |
Extended Properties
Covalent Radii (Extended)
Van der Waals Radii
Numbering Scales
Electronegativity Scales
Polarizability & Dispersion
Phase Transitions & Allotropes
| Melting point | 1800.15 K |
Oxidation State Categories
Advanced Reference Data
Crystal Radii Detail (1)
| Charge | CN | Spin | rcrystal (pm) | Origin |
|---|---|---|---|---|
| 3 | IX | — | 124.5 |
Isotope Decay Modes (46)
| Isotope | Mode | Intensity |
|---|---|---|
| 241 | SF | — |
| 241 | A | 14% |
| 241 | B+ | 12% |
| 242 | SF | 100% |
| 242 | A | — |
| 243 | A | 91% |
| 243 | SF | 9% |
| 243 | B+ | — |
| 244 | SF | 97% |
| 244 | B+ | 2% |
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)
Production
Production of this element (from raw materials or other compounds containing the element).
Because of the short half-life of all fermium isotopes, all that may have been present on the Earth during its formation has long since decayed away. Einsteinium and fermium did occur in the natural nuclear fission reactor at Oklo, but no longer exist. Fermium is produced as the result of multiple neutron captures in lighter elements, such as uranium and curium, followed by successive beta decays. The probability of such events increases with increased neutron flux, and nuclear explosions are the most powerful neutron sources on Earth. Fermium is also produced by the bombardment of lighter actinides with neutrons in nuclear reactors or accelerators. Fermium-257 is the heaviest isotope that is obtained via neutron capture, and can only be produced in nanogram quantities. The major source is the 85 MW High Flux Isotope Reactor (HFIR) at the Oak Ridge National Laboratory in Tennessee, USA. In a HFIR "campaign", tens of grams of curium are irradiated to produce heavier actinides and picogram quantities of fermium. The quantities of fermium produced in 20–200 kiloton thermonuclear explosions are believed to be of the order of milligrams, although it is mixed in with a huge quantity of debris. Forty picograms of 257Fm were recovered from 10 kilograms of debris from the 'Hutch' nuclear test in 1969. After production, fermium must be separated from debris and a host of other actinides and lanthanide fission products by solvent extraction, ion exchange, etc.). The annual reactor production of fermium-257 is in the picogram range. However, pure 255Fm (half-life 20 hours) can be easily isolated by "milking" the beta-decay daughter of pure 255Es (half-life 39.8 days).
References (1)
- [6] Fermium https://periodic.lanl.gov/100.shtml
References
(9)
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 Fermium.
The element property data was retrieved from publications.
