Tritium trinkets
in your element
Tritium trinkets
Scientists take nomenclature seriously, but tritium was named in a casual aside. Brett F. Thornton and
Shawn C. Burdette discuss the heavy, radioactive hydrogen isotope that is available for purchase online.
W
hy is 3H called tritium and
not simply hydrogen-3? More
specifically, why have 2H and
3
H been named as if they are elements,
when thousands of other isotopes are
not deemed worthy? In the early 1900s,
a number of radioactive isotopes held
individual names, but these fell out of use
long ago. IUPAC formally disallowed isotope
names, except those of hydrogen, in 1957.
Only a few unsanctioned exceptions — such
as radiocarbon for 14C, thoron for 220Rn
and ionium for 230Th — persist in
specialized fields.
When the concept of isotopy was
realized, many isotopes that had previously
been seen as unique elements were grouped
together as single elements on the periodic
table due to their apparently identical
chemistry. Although slight chemical
differences had been observed for some
isotopes, the discovery of hydrogen isotopes
was a significant inflection point. 2H and
3
H clearly did not behave exactly like
‘ordinary’ 1H in chemical reactions, which
provided a clear rationale for naming them
separately. Soon after the discoveries of 2H
and 3H, chemistry teachers were told1 to
exercise “caution in stating that the chemical
properties of the isotopes of an element
are identical” — a caution that even today
is not always heeded.
American scientists Harold Urey, George
Murphy and Ferdinand Brickwedde,
who had discovered deuterium in 1932,
proposed the name tritium for the notyet-discovered 3H in their 1933 report2 in
which the name deuterium was suggested
for 2H. This pre-emptive proposal for 3H
added further controversy to what soon
became an acrimonious public debate over
the appropriateness of the name deuterium3.
Across the Atlantic, Ernest Rutherford
endorsed diplogen for 2H and diplon for its
nucleus. His fame provided visibility to these
alternatives. Soon thereafter, in early 1934 at
Cambridge University, Mark Oliphant, Paul
Harteck and Ernest Rutherford reported4
producing 3H by ‘diplon’ bombardment of
H
686
D
T
He
Li
‘diplogen’. The article conspicuously did not
mention, or suggest, a name for the new
isotope.
The initial Cambridge report incorrectly
claimed 3H was stable, because the other
reaction product, 3He, was believed to be
the source of radioactivity3. By the time the
opposite was shown to be true5, the name
tritium was already in common use. Shortly
before his death in 1937, Rutherford
penned a retrospective on 3H advocating
for the name triterium (ref. 6). Despite his
efforts, triterium did not displace Urey’s
tritium, and triplogen, the counterpart to
diplogen, gained even less support.
Tritium occurs naturally on Earth,
although in vanishingly low concentrations.
It is produced in the stratosphere, where
cosmic ray spallation releases neutrons that
impact 14N to yield 12C and T. The natural
amount of tritium in the entire atmosphere
may be less than 2 kg, but testing of fusion
weapons produced about 200 kg more by
the early 1960s. Its decay (12.3 year halflife) has proven useful for many geophysical
tracer studies, especially in surface and
groundwater systems, as well as the oceans.
Tritium is an extremely weak β-emitter,
not harmful unless inhaled or ingested
in unlikely large quantities. Furthermore,
its decay product is the stable 3He. These
characteristics make tritium one of the most
widely available radioactive substances. A
wide selection of keychains, necklaces and
watches can be easily purchased online
that incorporate a minuscule amout of
tritium, whose decay excites a phosphor,
such as copper-doped ZnS, providing selfluminescence for years without batteries or
external power.
Tritium remains special amongst the
isotopes — and not just on account of
its name. The T +D reaction is the most
promising one for fusion energy in the
future. As the isotopes of an element
differ only by their number of neutrons,
the relative mass difference between an
element’s isotopes is greater for lighter
elements, and greatest by far for hydrogen.
Vast fields of research now depend on slight
Be
B
C
N
O
F
Ne
Credit: Emma Sofia Karlsson, Stockholm, Sweden
variances in isotope chemistry, often driven
by the differing masses. But although 208Pb
is about 0.5% heavier than 207Pb, and 13C is
about 8.5% heavier than 12C, T is about 200%
heavier than 1H. With this huge relative mass
difference, T versus 1H is an extreme outlier
compared to isotope pairs of other elements.
A pity, perhaps, that the relatively short halflife and rarity make its bulk chemistry more
difficult to study, as tritium is truly in a class
of its own for isotope effects.
❐
Brett F. Thornton1* and Shawn C. Burdette2*
The Department of Geological Sciences and Bolin
Centre for Climate Research, Stockholm University,
Stockholm, Sweden. 2The Department of Chemistry
and Biochemistry, Worcester Polytechnic Institute,
Worcester, MA, USA. Twitter: @geochembrett;
@WPIBurdette
*e-mail: ;
1
Published online: 21 May 2018
https://doi.org/10.1038/s41557-018-0070-3
References
1. Wildman, E. A. J. Chem. Ed. 11, 11–16 (1935).
2. Urey, H. C., Murphy, G. M. & Brickwedde, F. G. J. Chem. Phys. 1,
512–513 (1933).
3. Stuewer, R. H. Am. J. Phys. 54, 206 (1986).
4. Oliphant, M. L. E., Harteck, P. & Rutherford, E. Proc. R. Soc. A
144, 692–703 (1934).
5. Alvarez, L. W. & Cornog, R. Phys. Rev. 56, 613 (1939).
6. Rutherford, E. Nature 140, 303–305 (1937).
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Nature Chemistry | VOL 10 | JUNE 2018 | 686 | www.nature.com/naturechemistry
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