Fermium (Fm)
actinideSolid
Peso atomico standard
[257]Configurazione elettronica
[Rn] 5f12 7s2Punto di fusione
1526,85 °CPunto di ebollizione
N/DDensità
9700 kg/m³Stati di ossidazione
+2, +3Elettronegatività (Pauling)
1,3Energia di ionizzazione (1ª)
6,5 eVAnno della scoperta
1952Raggio atomico
N/DDettagli
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.
The bulk appearance of fermium metal is unknown because the element has not been isolated in visible, weighable quantities. Any metallic form and many ordinary physical properties are therefore inferred from actinide trends rather than directly observed.
Fermium has no commercial or practical technological use. Its uses are confined to basic research in nuclear chemistry, actinide separations, and studies of very heavy-element production. Some fermium isotopes, especially ²⁵⁷Fm because of its comparatively long half-life among fermium nuclides, have been used in tracer-scale experiments to characterize chemical behavior and nuclear decay. Availability is too limited for routine applications.
Due to the small amounts produced and its short half-life, there are currently no uses for fermium outside of basic scientific research.
Owing to the minute amounts of fermium produced and all of its isotopes having relatively short half-lives, there are currently no uses for it outside of basic scientific research that expands knowledge of the rest of the periodic table.
Fermium chemistry is known from tracer-scale aqueous work. The stable oxidation state in solution is Fm³⁺, and separations commonly exploit its similarity to trivalent lanthanides and neighboring actinides. Specific solid compounds have not been prepared in bulk. Simple halides such as fermium(III) chloride, FmCl₃, and oxides such as fermium(III) oxide, Fm₂O₃, are expected by analogy, but their bulk properties are not experimentally established. Fm²⁺ has been reported under strongly reducing conditions in solution.
See more information at the Fermium compound page.
All fermium isotopes are radioactive, and their hazards depend strongly on isotope, activity, decay mode, and chemical form. Handling is limited to specialized radiochemical facilities using remote methods and containment. The principal risks are external and internal radiation exposure from trace samples; ingestion, inhalation, or contamination of skin and equipment must be prevented. Ordinary chemical toxicity is poorly characterized and is secondary to radiological hazard.
Fermium has no meaningful natural environmental cycle. It is not a primordial element, and any natural production would be at atom-scale levels and short-lived. Environmental presence is mainly a theoretical or historical consequence of nuclear explosions or specialized laboratory work, where quantities are extremely small. Because no bulk releases or stable reservoirs exist, its ecological behavior is inferred from actinide chemistry rather than field observation.
Fermium has no commodity market, industrial demand, or recycling economy. It is made only in microscopic quantities by intense neutron irradiation of lighter actinides in high-flux reactors or by nuclear explosion debris in historical discoveries. Isolation requires elaborate radiochemical separation from many actinide and fission-product contaminants, and decay limits storage and distribution. Access is therefore governed by national research facilities, target availability, and scientific need rather than price-based supply.
Produced by bombarding lighter transuranium elements with still lighter particles or by neutron capture.
Fermium is not expected to have a persistent cosmic abundance. Its isotopes are too short-lived to survive from stellar nucleosynthesis or the formation of the Solar System. Very neutron-rich environments may transiently form nuclei in this mass region, but fermium would decay long before incorporation into stable planetary materials. Confirmed fermium is a human-made product on Earth.
- Fermium was first identified in debris from the Ivy Mike thermonuclear test.
- ²⁵⁷Fm is the most useful fermium isotope for chemistry because it lives long enough for tracer experiments.
- The element is named after Enrico Fermi.
- Fermium marks the point where neutron capture synthesis of heavier actinides becomes strongly limited by short half-l by
- Only atom-scale or tracer-scale chemical studies have been possible.
Immagini
Proprietà
Fisiche
- Raggio di van der Waals
- 245 pm Confronta Raggio di van der Waals di tutti gli elementi →
- Densità
- 9700 kg/m³ Confronta Densità di tutti gli elementi →
- Fase in condizioni STP
- Solido Confronta Fase in condizioni STP di tutti gli elementi →
- Punto di fusione
- 1526,85 °C Confronta Punto di fusione di tutti gli elementi →
Chimiche
- Elettronegatività (Pauling)
- 1,3 Confronta Elettronegatività (Pauling) di tutti gli elementi →
- Affinità elettronica
- 0,339 eV
- Energia di ionizzazione (1ª)
- 6,5 eV Confronta Energia di ionizzazione (1ª) di tutti gli elementi →
- Energia di ionizzazione (2ª)
- 12,400043 eV Confronta Energia di ionizzazione (2ª) di tutti gli elementi →
- Energia di ionizzazione (3ª)
- 23,20008 eV Confronta Energia di ionizzazione (3ª) di tutti gli elementi →
- Energia di ionizzazione (4ª)
- 39,300135 eV Confronta Energia di ionizzazione (4ª) di tutti gli elementi →
- Energia di ionizzazione (5ª)
- 55,000189 eV Confronta Energia di ionizzazione (5ª) di tutti gli elementi →
- Stati di ossidazione
- +2, +3 Confronta Stati di ossidazione di tutti gli elementi →
- Elettroni di valenza
- 3 Confronta Elettroni di valenza di tutti gli elementi →
- Configurazione elettronica
- [Rn] 5f12 7s2
Termodinamiche
- Calore di sublimazione
- 4,145722 eV
- Calore di atomizzazione
- 4,145722 eV
Nucleari
- Protoni
- 100 Confronta Protoni di tutti gli elementi →
- Neutroni
- 157 Confronta Neutroni di tutti gli elementi →
- Isotopi noti
- 20 Confronta Isotopi noti di tutti gli elementi →
- Isotopi stabili
- 0 Confronta Isotopi stabili di tutti gli elementi →
- Numero di massa (isotopo più stabile)
- 257
- Isotopo più stabile
- Fm-257
- Anno della scoperta
- 1952
Abbondanza
N/D
Struttura cristallina
N/D
Struttura elettronica
- Elettroni per guscio
- 2, 8, 18, 32, 30, 8, 2 Confronta Elettroni per guscio di tutti gli elementi →
Identificativi
- Numero CAS
- 7440-72-4 Confronta Numero CAS di tutti gli elementi →
- Simbolo di termine
- 3H6
- InChI
- InChI=1S/Fm
- Chiave InChI
- MIORUQGGZCBUGO-UHFFFAOYSA-N
Configurazione elettronica Misurato
Fm: 5f¹² 7s²[Rn] 5f¹² 7s²1s² 2s² 2p⁶ 3s² 3p⁶ 3d¹⁰ 4s² 4p⁶ 4d¹⁰ 5s² 5p⁶ 4f¹⁴ 5d¹⁰ 6s² 6p⁶ 5f¹² 7s²Modello atomico
Gli isotopi modificano il numero di neutroni, la massa e la stabilità — non la configurazione elettronica di un atomo neutro.
Modello atomico schematico, non in scala.
Impronta atomica
Spettro di emissione / assorbimento
Distribuzione isotopica
Nessun isotopo stabile.
| Numero di massa | Massa atomica (u) | Abbondanza naturale | Emivita |
|---|---|---|---|
| 242 Radioattivo | 242,07343 ± 0,00043 | N/D | 800 us |
| 241 Radioattivo | 241,07421 ± 0,00032 | N/D | 730 us |
| 258 Radioattivo | 258,09708 ± 0,00022 | N/D | 370 us |
| 243 Radioattivo | 243,07446 ± 0,00023 | N/D | 231 ms |
| 256 Radioattivo | 256,0917745 ± 0,0000078 | N/D | 157.1 minuti |
Fase / Stato
Motivo: 1501,8 °C sotto il punto di sublimazione (1526,85 °C)
Schema non in scala
Punti di transizione di fase
Energie di transizione
Energia necessaria per sublimare 1 mol al punto di sublimazione
Densità
In condizioni standard
In condizioni standard
Spettri atomici
Sono visualizzati 10 di 100. Ordinamento per carica ionica crescente.
Livelli disponibili ?
| Ione | Carica | Livelli |
|---|---|---|
| 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 |
Dati sulla struttura cristallina non disponibili
Raggi ionici
| Carica | Coordinazione | Spin | Raggio |
|---|---|---|---|
| +3 | 9 | N/D | 110.5 pm |
Composti
Isotopi (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.
| Numero di massa | Massa atomica (u) | Abbondanza naturale | Emivita | Modalità di decadimento | |
|---|---|---|---|---|---|
| 242 Radioattivo | 242,07343 ± 0,00043 | N/D | 800 us | SF ≈100%α ? | |
| 241 Radioattivo | 241,07421 ± 0,00032 | N/D | 730 us | SF =?α<14% β+<12% | |
| 258 Radioattivo | 258,09708 ± 0,00022 | N/D | 370 us | SF ≈100%α ? | |
| 243 Radioattivo | 243,07446 ± 0,00023 | N/D | 231 ms | α =91±0.3%SF =9±0.3%β+ ? | |
| 256 Radioattivo | 256,0917745 ± 0,0000078 | N/D | 157.1 minuti | SF =91.9±0.3%α =8.1±0.3% |
Proprietà estese
Raggi covalenti (dati estesi)
- Raggio covalente (Pyykkö)
- 167 pm
Raggi di van der Waals
- UFF
- 328,6 pm
Scale di numerazione
- Mendeleev
- 36
- Pettifor
- 37
- Glawe
- 44
Scale di elettronegatività
- Ghosh
- 0
Polarizzabilità e dispersione
- Polarizzabilità dipolare
- 113 a.u.
- Polarizzabilità dipolare (inc.)
- 20 a.u.
Transizioni di fase e allotropi
| Punto di fusione | 1800,15 K |
Categorie degli stati di ossidazione
Dati di riferimento avanzati
Dettaglio dei raggi cristallini (1)
| Carica | CN | Spin | rcrystal (pm) | Origine |
|---|---|---|---|---|
| 3 | IX | — | 124,5 |
Modalità di decadimento degli isotopi (46)
| Isotopo | Modalità | Intensità |
|---|---|---|
| 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% |
Dati aggiuntivi
Estimated Crustal Abundance
The estimated element abundance in the earth's crust.
Not Applicable
Riferimenti (1)
Estimated Oceanic Abundance
The estimated element abundance in the earth's oceans.
Not Applicable
Riferimenti (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).
Riferimenti (1)
- [6] Fermium https://periodic.lanl.gov/100.shtml
Riferimenti
(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.
