Hydrogen isotope biogeochemistry

Hydrogen isotope biogeochemistry (HIBGC) is the scientific study of biological, geological, and chemical processes in the environment using the distribution and relative abundance of hydrogen isotopes. Hydrogen has two stable isotopes, protium 1H and deuterium 2H, which vary in relative abundance on the order of hundreds of permil. The ratio between these two species can be called the hydrogen isotopic signature of a substance. Understanding isotopic fingerprints and the sources of fractionation that lead to variation between them can be applied to address a diverse array of questions ranging from ecology and hydrology to geochemistry and paleoclimate reconstructions. Since specialized techniques are required to measure natural hydrogen isotopic composition (HIC), HIBGC provides uniquely specialized tools to more traditional fields like ecology and geochemistry.

History of hydrogen isotopes

Earliest work The study of hydrogen stable isotopes began with the discovery of deuterium by chemist Harold Urey. Even though the neutron was not realized until 1932, Urey began searching for "heavy hydrogen" in 1931. Urey and his colleague George Murphy calculated the redshift of heavy hydrogen from the Balmer series and observed very faint lines on a spectrographic study. To intensify the spectroscopic lines for publishable data, Murphy and Urey paired with Ferdinand Brickwedde and distilled a more concentrated pool of heavy hydrogen, now called deuterium. This work on hydrogen isotopes won Urey the 1934 Nobel Prize in Chemistry.

Also in 1934, scientists Ernest Rutherford, Mark Oliphant, and Paul Harteck, produced the radioisotope tritium (hydrogen-3, 3H) by hitting deuterium with high-energy nuclei. The deuterium used in the experiment was a generous gift of heavy water from UC Berkeley physicist Gilbert N. Lewis. Bombarding deuterium produced two previously undetected isotopes, helium-3 (3He) and 3H. Rutherford and his colleagues successfully created 3H, but incorrectly assumed that 3He was the radioactive component. The work of Luis Walter Alvarez and Robert Cornog first isolated 3H and reversed Rutherford's incorrect notion. Alvarez reasoned that tritium was radioactive, but did not measure the half-life, though calculations at the time suggested >10 years. At the end of World War II, physical chemist Willard Libby detected the residual radioactivity of a tritium sample with a Geiger counter, providing a more accurate understanding of the half-life, now accepted as 12.3 years.

Impact on physical chemistry The discovery of hydrogen isotopes also impacted physics in the 1940s, as nuclear magnetic resonance spectroscopy was first invented. Organic chemists now use nuclear magnetic resonance (NMR) to map protein interactions or identify small compounds, but NMR was first a passion project of physicists. All three isotopes of hydrogen were found to have magnetic properties suitable for NMR spectroscopy. The first chemist to fully express an application of NMR was George Pake, who measured gypsum ( CaSO 4 ⋅ 2 H 2 O {\displaystyle {\ce {CaSO4.2H2O}}} ) as a crystal and powder. The signal observed, called the Pake doublet, was from the magnetically active hydrogens in water. Pake then calculated the proton-proton bond length. NMR measurements were further revolutionized when commercial machines became available in the 1960s. Before this, NMR experiments involved constructing massive projects, locating large magnets, and hand wiring miles of copper coil. Proton NMR remained the most popular technique throughout advancements in following decades, but 2H and 3H were used in other flavors of NMR spectroscopy. 2H has a different magnetic moment and spin than 1H, but generally a much smaller signal. Historically, deuterium NMR is a poor alternative to proton NMR, but has been used to study the behavior of lipids on cell membranes. A variant of 2H NMR called 2H-SNIF has shown potential for understating position-specific isotope compositions and comprehending biosynthetic pathways. Tritium is also used in NMR, as it is the only nucleus more sensitive than 1H, generating very large signals. However, tritium's radioactivity discouraged many studies of 3H-NMR. While tritium's radioactivity discourages use in spectroscopy, tritium is essential for nuclear weapons. Scientists began understanding nuclear energy as early as the 1800s, but large advancements were made in studies of the atomic bomb in the early 1940s. Wartime research, especially the Manhattan Project, greatly advanced the understanding of radioactivity. 3H is a byproduct in reactors, a result of hitting lithium-6 with neutrons, producing almost 5 MeV of energy.

6 L i + n ⟶

4 H e +

3 H + 5 M e V {\displaystyle {}^{6}\mathrm {Li} +n\longrightarrow {}^{4}\mathrm {He} +{}^{3}\mathrm {H} +5\ \mathrm {MeV} }

In boosted fission weapons a mix of 2H and 3H is heated until there is thermonuclear fusion to produce helium and free neutrons. These fast neutrons then cause further fission, creating "boosting". In 1951, in Operation Greenhouse, a prototype named George, validated the proof of concept for such a weapon. However, the first true boosted fission bomb, Greenhouse Item, was successfully tested in 1952, giving a 45.5-kiloton yield, nearly double that of an unboosted bomb. The United States stopped producing tritium in nuclear reactors in 1988, but nuclear tests in the 1950s added large spikes of radionuclides to the air, especially carbon-14 and 3H. This complicated measurements for geologists using carbon dating. However, some oceanographers benefited from the 3H increase, using the signal in the water to trace physical mixing of water masses.

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