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Element 100 · actinide

Fermium (Fm)


Element 100 is a boundary, and it is a hard one. Everything up to fermium can be built in a reactor by feeding neutrons to a target and waiting. Nothing above fermium can. The road ends here, and it ends at a specific isotope with a specific number attached to it.

The wall at element 100

Making heavy elements by neutron capture is a slow climb. A nucleus absorbs a neutron, becomes too neutron-rich to be stable, beta-decays — turning a neutron into a proton and moving one square to the right — and then absorbs another. Repeat for a year in an intense flux and plutonium becomes californium, then einsteinium, then fermium.

The climb reaches fermium-257, which lasts 100.5 days. To go further, fermium-257 would have to capture one more neutron and become fermium-258. It does, and fermium-258 splits in half by spontaneous fission, with 370 microseconds as its half-life. There is no time for it to absorb anything else, and no time for it to beta-decay into element 101. Every atom that reaches that square is destroyed before it can do anything useful.

This is the fermium wall, and it splits the periodic table into two zones with completely different production economics. Below element 100, the heavy elements are made in kilogram-scale reactor campaigns and separated chemically in bulk. Above it, every single element has to be assembled one nucleus at a time in an accelerator, by slamming two smaller nuclei together and hoping they stick. The change is not gradual. It happens at one isotope, over 370 microseconds.

Two fragments of tin

Why fermium-258 fissions so violently is itself worth explaining, because the answer is one of the prettier results in nuclear structure.

Most heavy nuclei fission asymmetrically: they break into a large fragment and a smaller one, and the mass distribution has two humps. Fermium-257 does this. Fermium-258 does not. It splits almost exactly down the middle, into two fragments of mass around 129, with a very high release of energy and an unusually narrow spread.

The reason is that each half is close to tin-132 — a nucleus with 50 protons and 82 neutrons, both of them magic numbers, making it one of the most tightly bound configurations available anywhere in that mass range. Fermium-258 has just enough nucleons to make two of them. The fission is fast and symmetric because the products are exceptionally stable, and the sudden onset of this behaviour across a couple of mass units is what slams the door shut on the neutron-capture route.

An open claim and a classified one

Fermium was found alongside einsteinium in the debris of the Ivy Mike test of November 1952, in the same filter papers and coral, by the same Berkeley, Argonne and Los Alamos effort. The isotope identified was fermium-255. Like its neighbour, the result was classified, because the isotopic spread in the debris disclosed things about the device that nobody intended to publish.

That secrecy created a genuine rival claim. In 1953 and 1954, a Stockholm group at the Nobel Institute of Physics fired oxygen ions at uranium and reported a new alpha-emitting activity with a half-life of around half an hour, which they assigned to a fermium isotope. Their work was independent, unclassified, and published — the first appearance of element 100 in the open literature, produced by a completely different method from the American discovery it did not know about. The Stockholm group did not press a claim to the element, and priority is conventionally given to the Ivy Mike work, but the sequence is a real illustration of what classification does to scientific credit.

Enrico Fermi died in November 1954, before the American results were released and before the name was chosen. He was never aware that element 100 would carry it.

Nobody has ever seen it

Einsteinium exists in amounts you can put on a balance. Fermium never has, and there is no prospect that it ever will.

The largest amounts ever assembled run to something on the order of a billion atoms of fermium-257 — which sounds enormous and is far too little to see, to weigh, or to gather into a solid. Fermium has therefore never been reduced to a metal at all. Its tabulated melting point is a prediction of the actinide series rather than an observation, and no fermium compound has ever been isolated in the solid state either.

What is known about fermium's chemistry comes entirely from tracer work: solutions containing a few thousand atoms, studied by how they move through an ion-exchange column relative to elements whose behaviour is already understood. That work establishes the essentials. Fermium in solution is overwhelmingly trivalent, exactly like the late lanthanides it echoes. It can be pushed down to a +2 state more easily than the actinides below it can, which is one of several signs that the 5f shell is being drawn in tightly as the series ends and is contributing less and less to bonding.

Fermium's own isotopes reinforce the point about the wall. Beyond fermium-257 the half-lives collapse: fermium-259 lasts about a second and a half, fermium-260 a few milliseconds. Element 100 is not merely the last stop on the reactor route. It is the point at which nuclear stability itself starts running out, and everything beyond it exists on borrowed time measured in seconds.

Isotopes of Fermium

No isotope of Fermium has a measurable natural abundance, and only one has a relative atomic mass on record.

Isotopes of Fermium with relative atomic mass and natural abundance
IsotopeRelative atomic massNatural abundance
257Fm257.0951061(69)none

100

Fm

Fermium

actinide

Standard atomic weight
[257]the mass number of the longest-lived isotope; this element has no stable one
Group / period / block
3 · 7 · f
Electron configuration
[Rn] 5f12 7s2
Electrons per shell
2, 8, 18, 32, 30, 8, 2
State at 20 °C
solid
Melting point
1800 K · 1527 °C
Boiling point
not known
Density
not known
Electronegativity
1.3 (Pauling)
First ionisation energy
6.5 eV
Common oxidation states
+3
Discovery
1952 · credited to Lawrence Berkeley National Laboratory

Hazard facts

  • Radioactive Every isotope is unstable, so the element emits ionising radiation as it decays.

These are properties of the element, stated as facts. Nothing on this site describes how to handle or work with any substance.

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