Fm 100

Fermium (Fm)

actinide
Period: 7 Block: s

Solid

Standard Atomic Weight

[257]

Electron configuration

[Rn] 5f12 7s2

Melting point

1526.85 °C (1800 K)

Boiling point

N/A

Density

9700 kg/m³

Oxidation states

+2, +3

Electronegativity (Pauling)

1.3

Ionization energy (1st)

Discovery year

1952

Atomic radius

N/A

Details

Name origin Named in honor of the scientist Enrico Fermi.
Discovery country United States
Discoverers Argonne, Los Alamos, U of Calif

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

Van der Waals radius 245 pm
Density
Phase at STP solid
Melting point 1526.85 °C

Chemical

Electronegativity (Pauling) 1.3
Electron affinity
Ionization energy (1st)
Ionization energy (2nd)
Ionization energy (3rd)
Ionization energy (4th)
Ionization energy (5th)
Oxidation states +2, +3
Valence electrons 3
Electron configuration
Electron configuration (semantic)

Thermodynamic

Heat of sublimation 4.145722 eV
Heat of atomization 4.145722 eV

Nuclear

Stable isotopes 0
Mass number (most stable) 257
Discovery year 1952

Abundance

N/A

Reactivity

N/A

Crystal Structure

N/A

Electronic Structure

Electrons per shell 2, 8, 18, 32, 30, 8, 2

Identifiers

CAS number 7440-72-4
Term symbol
InChI InChI=1S/Fm
InChI Key MIORUQGGZCBUGO-UHFFFAOYSA-N

Electron Configuration Measured

Ion charge
Protons 100
Electrons 100
Charge Neutral
Configuration Fm: 5f¹² 7s²
Electron configuration
Measured
[Rn] 5f¹² 7s²
1s² 2s² 2p⁶ 3s² 3p⁶ 3d¹⁰ 4s² 4p⁶ 4d¹⁰ 5s² 5p⁶ 4f¹⁴ 5d¹⁰ 6s² 6p⁶ 5f¹² 7s²
Orbital diagram
1s
2/2
2s
2/2
2p
6/6
3s
2/2
3p
6/6
4s
2/2
3d
10/10
4p
6/6
5s
2/2
4d
10/10
5p
6/6
6s
2/2
4f
14/14
5d
10/10
6p
6/6
7s
2/2
5f
12/14 2↑
Total electrons: 100 Unpaired: 2 ?

Atomic model

Protons 100
Neutrons 143
Electrons 100
Mass number 243
Stability Radioactive

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

0 / 0 (0 with intensity)
Measured
Emission Visible: 380–750 nm

Isotope Distribution

No stable isotopes.

Mass numberAtomic mass (u)Natural abundanceHalf-life
242 Radioactive242.07343 ± 0.00043N/A800 us
241 Radioactive241.07421 ± 0.00032N/A730 us
258 Radioactive258.09708 ± 0.00022N/A370 us
243 Radioactive243.07446 ± 0.00023N/A231 ms
256 Radioactive256.0917745 ± 0.0000078N/A157.1 minutes
Measured

Phase / State

1 atm / 101.325 kPa
Solid 25 °C (298.15 K)

Reason: 1501.8 °C below sublimation point (1526.85 °C)

Sublimation point 1526.85 °C
0 K Current temperature: 25 °C 6000 K
Phase timeline

Schematic, not to scale

Solid
Gas
Sublimation
25°C
Solid
Liquid
Gas
Current

Phase transition points

Sublimation point Literature
1526.85 °C
Current phase Calculated
Solid

Transition energies

Heat of sublimation Literature
4.145722 eV

Energy required to sublime 1 mol at sublimation point

Density

Reference density Literature
9700 kg/m³

At standard conditions

Current density Calculated
9700 kg/m³

At standard conditions

Atomic Spectra

Showing 10 of 100 Atomic Spectra. Sorted by ion charge (ascending).

Levels Holdings ?

IonChargeLevels
Fm I 02
Fm II +12
Fm III +22
Fm IV +32
Fm V +42
Fm VI +52
Fm VII +62
Fm VIII +72
Fm IX +82
Fm X +92
NIST Levels Holdings →
100 Fm 257

Fermium — Atomic Orbital Visualizer

[Rn] 5f12 7s2
Energy levels 2 8 18 32 30 8 2
Oxidation states +2, +3
HOMO 5f n=5 · l=3 · m=-3
Fermium — Atomic Orbital Visualizer Preview
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100 Fm 257

Fermium — Crystal Structure Visualizer

Crystal structure data not available

Ionic Radii

ChargeCoordinationSpinRadius
+39N/A110.5 pm

Compounds

Fm
257.095 u
Fm
255.090 u
Fm
254.087 u
Fm
257.095 u
Fm
252.082 u
Fm
253.085 u

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 numberAtomic mass (u)Natural abundanceHalf-lifeDecay mode
242 Radioactive242.07343 ± 0.00043N/A800 us
SF ≈100%α ?
241 Radioactive241.07421 ± 0.00032N/A730 us
SF =?α<14% β+<12%
258 Radioactive258.09708 ± 0.00022N/A370 us
SF ≈100%α ?
243 Radioactive243.07446 ± 0.00023N/A231 ms
α =91±0.3%SF =9±0.3%β+ ?
256 Radioactive256.0917745 ± 0.0000078N/A157.1 minutes
SF =91.9±0.3%α =8.1±0.3%
242 Radioactive
Atomic mass (u) 242.07343 ± 0.00043
Natural abundance N/A
Half-life 800 us
Decay mode
SF ≈100%α ?
241 Radioactive
Atomic mass (u) 241.07421 ± 0.00032
Natural abundance N/A
Half-life 730 us
Decay mode
SF =?α<14% +1
258 Radioactive
Atomic mass (u) 258.09708 ± 0.00022
Natural abundance N/A
Half-life 370 us
Decay mode
SF ≈100%α ?
243 Radioactive
Atomic mass (u) 243.07446 ± 0.00023
Natural abundance N/A
Half-life 231 ms
Decay mode
α =91±0.3%SF =9±0.3% +1
256 Radioactive
Atomic mass (u) 256.0917745 ± 0.0000078
Natural abundance N/A
Half-life 157.1 minutes
Decay mode
SF =91.9±0.3%α =8.1±0.3%

Extended Properties

Covalent Radii (Extended)

Covalent radius (Pyykkö)  

Van der Waals Radii

UFF  

Numbering Scales

Mendeleev
Pettifor
Glawe

Electronegativity Scales

Ghosh

Polarizability & Dispersion

Dipole polarizability  
Dipole polarizability (unc.)  

Phase Transitions & Allotropes

Melting point1800.15 K

Oxidation State Categories

+2 extended
+3 main

Advanced Reference Data

Crystal Radii Detail (1)
ChargeCNSpinrcrystal (pm)Origin
3IX124.5
Isotope Decay Modes (46)
IsotopeModeIntensity
241SF
241A14%
241B+12%
242SF100%
242A
243A91%
243SF9%
243B+
244SF97%
244B+2%

Additional Data

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)

References

(9)
2 Atomic Mass Data Center (AMDC), International Atomic Energy Agency (IAEA)
Fm

The half-life and atomic mass data was provided by the Atomic Mass Data Center at the International Atomic Energy Agency.

3 IUPAC Commission on Isotopic Abundances and Atomic Weights (CIAAW)
Fermium

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.

4 IUPAC Periodic Table of the Elements and Isotopes (IPTEI)

The information are cited from Pure Appl. Chem. 2018; 90(12): 1833-2092, https://doi.org/10.1515/pac-2015-0703.

License note: Copyright (c) 2020 International Union of Pure and Applied Chemistry. The International Union of Pure and Applied Chemistry (IUPAC) contribution within Pubchem is provided under a CC-BY-NC-ND 4.0 license, unless otherwise stated.
5 Jefferson Lab, U.S. Department of Energy
Fermium

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/

License note: Please see citation and linking information: https://education.jlab.org/faq/index.html
6 Los Alamos National Laboratory, U.S. Department of Energy
Fermium

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.

7 NIST Physical Measurement Laboratory
Fermium

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

8 PubChem Elements
Fermium

This section provides all form of data related to element Fermium.

9 PubChem Elements
Fermium

The element property data was retrieved from publications.

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