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Fermium @ Periodic Table of Chemical Elements

12345678 910111213141516 1718
IIIIIIbIVb VbVIbVIIbVIIIbIb IIbIIIIVVVI VIIVIII
1H
1.0079
2He
4.0026
3Li
6.9412
4Be
9.0121
5B
10.811
6C
12.010
7N
14.006
8O
15.999
9F
18.998
10Ne
20.179
11Na
22.989
12Mg
24.305
13Al
26.981
14Si
28.085
15P
30.973
16S
32.065
17Cl
35.453
18Ar
39.948
19K
39.098
20Ca
40.078
21Sc
44.955
22Ti
47.867
23V
50.941
24Cr
51.996
25Mn
54.938
26Fe
55.845
27Co
58.933
28Ni
58.693
29Cu
63.546
30Zn
65.409
31Ga
69.723
32Ge
72.641
33As
74.921
34Se
78.963
35Br
79.904
36Kr
83.798
37Rb
85.467
38Sr
87.621
39Y
88.905
40Zr
91.224
41Nb
92.906
42Mo
95.942
43Tc
98.906
44Ru
101.07
45Rh
102.90
46Pd
106.42
47Ag
107.86
48Cd
112.41
49In
114.81
50Sn
118.71
51Sb
121.76
52Te
127.60
53I
126.90
54Xe
131.29
55Cs
132.90
56Ba
137.32
57La
138.90
72Hf
178.49
73Ta
180.94
74W
183.84
75Re
186.20
76Os
190.23
77Ir
192.21
78Pt
195.08
79Au
196.96
80Hg
200.59
81Tl
204.38
82Pb
207.21
83Bi
208.98
84Po
208.98
85At
209.98
86Rn
222.01
87Fr
223.01
88Ra
226.02
89Ac
227.02
104Rf
261.10
105Db
262.11
106Sg
266.12
107Bh
264.12
108Hs
269
109Mt
278
110Ds
281
111Rg
282
112Cn
285
113Nh
286
114Fl
289
115Mc
290
116Lv
293
117Ts
294
118Og
294
Lanthanoids58Ce
140.11
59Pr
140.90
60Nd
144.24
61Pm
146.91
62Sm
150.36
63Eu
151.96
64Gd
157.25
65Tb
158.92
66Dy
162.50
67Ho
164.93
68Er
167.25
69Tm
168.93
70Yb
173.04
71Lu
174.96
Actinoids90Th
232.03
91Pa
231.03
92U
238.02
93Np
237.04
94Pu
244.06
95Am
243.06
96Cm
247.07
97Bk
247.07
98Cf
251.07
99Es
252.08
100Fm
257.09
101Md
258.09
102No
259.10
103Lr
260.10
Alkali metals Alkali earth metals Transition metals Other metals Metaloids Non-metals Halogens Noble gases
Element

100

Fm

Fermium

257.0951

2
8
18
32
30
8
2
Fermium photo
Basic properties
Atomic number100
Atomic weight257.0951 amu
Element familyActinoids
Period7
Group2
Blocks-block
Discovery year1952
Isotope distribution
None
Physical properties
Density 9.7 g/cm3 (STP)
Atomic hydrogen (H) 8.988E-5
Meitnerium (Mt) 28
Melting1527 °C
Helium (He) -272.2
Carbon (C) 3675
Chemical properties
Oxidation states
(less common)
+3
(+2)
First ionization potential 6.498 eV
Cesium (Cs) 3.894
Helium (He) 24.587
Electron affinity 0.350 eV
Nobelium (No) -2.33
Atomic chlorine (Cl) 3.612725
Electronegativity1.3
Cesium (Cs) 0.79
Atomic fluorine (F) 3.98
Atomic radius
Electronic properties
Electrons per shell2, 8, 18, 32, 30, 8, 2
Electronic configuration[Rn] 5f127s2
Bohr atom model
Bohr atom model
Orbital box diagram
Orbital box diagram
Valence electrons14
Lewis dot structure Fermium Lewis dot structure
Orbital Visualization
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Electrons-

Fermium (Fm): Periodic Table Element

Scientific Review Article | Chemistry Reference Series

Abstract

Fermium (Fm, atomic number 100) represents a synthetic actinide element that occupies a unique position as the heaviest element synthesizable by neutron bombardment of lighter elements. Discovered in 1952 in the debris of the first hydrogen bomb explosion, fermium exhibits characteristic actinide chemistry with predominant +3 oxidation states and limited nuclear stability. The element's most stable isotope, 257Fm, possesses a half-life of 100.5 days, while other isotopes demonstrate significantly shorter decay periods. Fermium's chemical behavior manifests through enhanced complex formation relative to preceding actinides, attributed to increased effective nuclear charge. Current applications remain restricted to fundamental nuclear research due to production limitations and radioactive decay constraints.

Introduction

Fermium occupies atomic number 100 in the periodic table, representing the terminal element accessible through neutron capture synthesis methods. This synthetic actinide demonstrates fundamental importance in understanding superheavy element chemistry and nuclear physics principles. The element's electronic configuration [Rn]5f127s2 places it within the actinide series, exhibiting characteristic f-block properties with enhanced nuclear instability typical of transuranium elements. Named after Enrico Fermi, the pioneer of controlled nuclear reactions, fermium's discovery marked a significant milestone in superheavy element research. The element's position beyond the natural occurrence boundary necessitates artificial synthesis, limiting availability to specialized research facilities equipped with high-flux neutron sources or particle accelerators.

Physical Properties and Atomic Structure

Fundamental Atomic Parameters

Fermium possesses atomic number 100 with electronic configuration [Rn]5f127s2, placing twelve electrons in the 5f subshell. The atomic radius has been estimated at approximately 1.70 Å based on theoretical calculations and comparison with neighboring actinides. Ionic radius for Fm3+ measures approximately 0.85 Å, reflecting the lanthanide contraction effect within the actinide series. The effective nuclear charge experienced by valence electrons increases significantly compared to lighter actinides, contributing to enhanced bonding characteristics and complex stability. Spectroscopic studies reveal energy level structures consistent with 5f12 configuration, though comprehensive atomic spectroscopy remains limited by sample availability and short half-lives.

Macroscopic Physical Characteristics

Fermium metal has not been isolated in bulk quantities, preventing direct measurement of macroscopic physical properties. Theoretical predictions suggest a face-centered cubic crystal structure typical of heavy actinides, with estimated density of approximately 9.7 g/cm³. The melting point is projected to be around 1800 K based on trends within the actinide series. Sublimation enthalpy measurements using fermium-ytterbium alloys yielded values of 142 ± 42 kJ/mol at 298 K. Magnetic susceptibility studies indicate paramagnetic behavior consistent with unpaired 5f electrons. The element exhibits metallic character in theoretical models, though experimental verification remains challenging due to sample limitations and radioactive decay.

Chemical Properties and Reactivity

Electronic Structure and Bonding Behavior

Fermium's chemical behavior demonstrates characteristic actinide properties with predominant +3 oxidation state stability. The 5f12 electronic configuration provides twelve unpaired electrons in aqueous solution, contributing to paramagnetic properties and specific spectroscopic signatures. The +2 oxidation state proves accessible under reducing conditions, with electrode potential Fm3+/Fm2+ estimated at -1.15 V versus standard hydrogen electrode. This reduction potential compares favorably with ytterbium(III)/(II), indicating moderate stability of the divalent state. Bonding in fermium complexes exhibits predominantly ionic character, with increased covalency compared to lighter actinides due to enhanced effective nuclear charge and contracted ionic radius.

Electrochemical and Thermodynamic Properties

Electrochemical studies reveal Fm3+/Fm0 standard reduction potential of -2.37 V, establishing fermium as highly electropositive. The Fm3+ ion exhibits hydration number of 16.9 in aqueous solution, with acid dissociation constant of 1.6 × 10-4 (pKa = 3.8). These values reflect enhanced charge density compared to preceding actinides, resulting in stronger metal-ligand interactions. Successive ionization energies follow predicted trends for actinides, with first ionization energy estimated at 627 kJ/mol. The enhanced effective nuclear charge contributes to contracted orbital radii and increased binding energies throughout the electron configuration.

Chemical Compounds and Complex Formation

Binary and Ternary Compounds

Fermium compounds remain limited to solution chemistry due to microscopic sample sizes and radioactive constraints. Fermium(II) chloride (FmCl2) has been identified through coprecipitation studies with samarium(II) chloride, representing the only characterized solid binary compound. Oxide formation likely follows actinide trends, suggesting stable Fm2O3 stoichiometry under oxidizing conditions. Halide complexes demonstrate enhanced stability relative to einsteinium and californium analogs, attributed to increased effective nuclear charge effects. Hydrolysis products include hydroxide species at elevated pH, with precipitation occurring above pH 3.8 based on acid dissociation measurements.

Coordination Chemistry and Complex Formation

Fermium(III) forms stable complexes with hard donor ligands containing oxygen and nitrogen atoms. Complexation with α-hydroxyisobutyrate demonstrates enhanced stability compared to lighter actinides, facilitating chromatographic separation protocols. Chloride and nitrate anionic complexes exhibit increased formation constants relative to californium and einsteinium analogs. The coordination number typically ranges from 8 to 9 in aqueous solution, consistent with large ionic radius requirements. Organic chelating agents such as EDTA and DTPA form exceptionally stable complexes, exploiting the high charge density of Fm3+. These coordination properties prove essential for separation and purification procedures in radiochemical processing.

Natural Occurrence and Isotopic Analysis

Geochemical Distribution and Abundance

Fermium does not occur naturally in Earth's crust due to the absence of stable isotopes and extremely short half-lives of all known nuclides. Primordial fermium, if present during Earth's formation, has completely decayed over geological timescales. The element briefly existed in the natural nuclear reactor at Oklo, Gabon, approximately 2 billion years ago through neutron capture processes, but no longer persists. Terrestrial fermium production occurs exclusively through artificial synthesis in nuclear reactors, particle accelerators, or nuclear weapons testing. Atmospheric detection following nuclear tests provides the only environmental occurrence, typically at femtogram to picogram levels dispersed in fallout debris.

Nuclear Properties and Isotopic Composition

Twenty fermium isotopes are characterized with mass numbers ranging from 241 to 260. The most stable isotope, 257Fm, exhibits a half-life of 100.5 days through α-decay to 253Cf. Other significant isotopes include 255Fm (t½ = 20.07 hours), 254Fm (t½ = 3.2 hours), and 253Fm (t½ = 3.0 days). Isotopes heavier than 257Fm undergo spontaneous fission with microsecond to millisecond half-lives, creating the "fermium gap" that limits superheavy element synthesis via neutron capture. Nuclear properties follow predicted trends for actinides, with α-decay predominating for lighter isotopes and spontaneous fission becoming significant for heavier masses. Cross-sections for neutron capture reactions decrease dramatically with increasing mass number, contributing to synthesis limitations.

Industrial Production and Technological Applications

Extraction and Purification Methodologies

Fermium production relies primarily on neutron bombardment of lighter actinides in high-flux research reactors. The High Flux Isotope Reactor (HFIR) at Oak Ridge National Laboratory serves as the primary source, producing picogram quantities through months-long irradiation campaigns. Target materials consist of curium or berkelium isotopes, with successive neutron captures leading to fermium formation. Production yields decrease exponentially with atomic number, limiting 257Fm availability to subnanogram quantities annually. Nuclear weapons testing historically provided larger amounts, with the 1969 Hutch test yielding 4.0 pg of 257Fm from 10 kg of debris, though recovery efficiency remained extremely low at 10-7 of total production.

Technological Applications and Future Prospects

Current fermium applications focus exclusively on fundamental nuclear physics and chemistry research. Studies of superheavy element properties utilize fermium as a benchmark for theoretical model validation and spectroscopic technique development. Nuclear structure investigations employ fermium isotopes to explore shell effects and decay mechanisms near the proposed "island of stability." Potential future applications include neutron source development for specialized research and medical isotope production, though practical implementation requires significant advances in production efficiency. Enhanced synthesis methods through improved reactor designs or novel nuclear reactions may expand availability for applied research programs.

Historical Development and Discovery

The discovery of fermium emerged from the Manhattan Project's hydrogen bomb development program in the early 1950s. Initial detection occurred in debris analysis from the "Ivy Mike" thermonuclear test on November 1, 1952, at Enewetak Atoll. Albert Ghiorso and colleagues at the University of California Berkeley identified isotope 255Fm through its characteristic 7.1 MeV α-particle emissions and 20-hour half-life. The discovery remained classified until 1955 due to Cold War security concerns, despite independent synthesis by Swedish researchers in 1954 using ion bombardment techniques. Element naming honored Enrico Fermi, recognizing his contributions to nuclear physics and reactor development. Systematic studies began following declassification, establishing fermium's position as the heaviest neutron-capture synthesizable element and launching superheavy element research programs.

Conclusion

Fermium occupies a pivotal position in the periodic table as the terminal element accessible through neutron bombardment synthesis, marking the practical limit of bulk element production. Its unique nuclear properties and chemical behavior provide fundamental insights into actinide chemistry and superheavy element physics. The element's enhanced complex stability and distinctive electrochemical properties reflect increased effective nuclear charge effects characteristic of the heaviest actinides. While current applications remain confined to basic research due to synthesis limitations and radioactive instability, fermium continues to serve as a crucial benchmark for theoretical model development and experimental technique advancement in nuclear science.

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