The deuterium fingerprint

Subscribe options

Select your newsletters:

Please enter your email address:

@

Your email address will only be used for the purpose of sending you the ITER Organization publication(s) that you have requested. ITER Organization will not transfer your email address or other personal data to any other party or use it for commercial purposes.

If you change your mind, you can easily unsubscribe by clicking the unsubscribe option at the bottom of an email you've received from ITER Organization.

For more information, see our Privacy policy.

News & Media

Latest ITER Newsline

  • Augmented reality | Assessing the future work environment

    As part of their collaboration within the Site Support Agreement*, ITER and its neighbour CEA are developing a novel approach to explore, analyze and assess the [...]

    Read more

  • Diagnostics and instrumentation | First welding on the vacuum vessel

    Beginning in 2035, ITER will open a window into "burning plasmas"—a state of matter that exists in the core of stars only. Observing, assessing and mo [...]

    Read more

  • Assembly | Machining workshop opens on site

    Construction of an on-site machining workshop began in December 2019 and was completed on schedule in September 2020.The new workshop will be operated by the D [...]

    Read more

  • Neutral Beam Test Facility | Power is ready for the prototype injector

    The European Domestic Agency has carried out successful site acceptance tests at the ITER Neutral Beam Test Facility on power supply equipment installed ov [...]

    Read more

  • In-vessel coils | First components arrive on site

    ITER has received the first shipments of mineral-insulated conductor for ITER's in-vessel coils. The first lengths are destined for winding and bending trials a [...]

    Read more

Of Interest

See archived entries

The deuterium fingerprint

Robert Arnoux

This image of Comet Hartley 2 was captured by NASA's EPOXI mission between 3 and 4 November, 2010, during the spacecraft's flyby of this 2.25-kilometre-long, 300-million-tonne, peanut-shaped chunk of ice. The deuterium fingerprint in the comet's ice perfectly matches that of terrestrial waters. (Click to view larger version...)
This image of Comet Hartley 2 was captured by NASA's EPOXI mission between 3 and 4 November, 2010, during the spacecraft's flyby of this 2.25-kilometre-long, 300-million-tonne, peanut-shaped chunk of ice. The deuterium fingerprint in the comet's ice perfectly matches that of terrestrial waters.
The water molecule, as every primary school student learns, is made of one atom of oxygen and two atoms of hydrogen. But water as we know it, whether in a glass, in a lake or in the ocean, is not exclusively composed of H2O molecules. It also includes a tiny fraction of D2O, a molecule in which hydrogen is replaced by its heavy isotope, deuterium—the very deuterium that will be used as a fusion fuel in ITER.

The D2O fraction in water is invariable. It is the same in the Durance River as in the Amazon, in the Indian Ocean or in the Mediterranean.

Now, this rule applies only to terrestrial waters. Elsewhere in the Universe, the proportion of D2O molecules in a given volume of water can be quite different: astronomical observations and measurements have determined that in comets, for instance, the proportion of D2O is twice what it is on Earth.

Comets, often dubbed "dirty snowballs," are a mixture of ice and dust. They are the lonely wanderers of our solar system whose orbits sometimes cause collisions with larger bodies. Such a spectacular event occurred in July 1994 when Comet Shoemaker—Levy 9 collided with Jupiter.

Billions of years ago, such cosmic crashes were much more frequent. It has long been an accepted theory that comets, whacking into the infant Earth, played a significant role in creating our planet's oceans.

However, because of the difference in the deuterium ratio of comets' ice and oceans' water, comets alone could not be credited with delivering the total amount of water that presently covers 70 percent of the Earth's surface. Hence, current theories considered that less than 10 percent of Earth's water originated from comet—the remaining 90 percent still somewhat of a mystery.

That is, until the European Space Agency's (ESA) infrared space telescope Herschel focused on Comet Hartley 2, a 2.25-kilometre-long, 300-million-tonne peanut-shaped chunk of ice.

"Comet Hartley's deuterium-to-hydrogen ratio is almost exactly the same as the water in Earth's oceans," says Paul Hartogh, of the Max-Planck-Institut für Sonnensystemforschung in Katlenburg-Lindau, Germany, who led the international team of astronomers in this work.

Hartley's deuterium fingerprint perfectly matches that of terrestrial waters. If the comet has siblings, then, one of the most discussed issues in Earth's early history could be close to being solved.

Click here to see the news story on the ESA website.
 


return to the latest published articles