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Dusty experiments are solving interstellar water mystery

Last Updated on Tuesday, 13 April 2010 19:28
Published on Tuesday, 13 April 2010 19:26
molecular_cloud_spitzer_smaall.jpgDust may be a nuisance around the house but it plays a vital role in the formation of the key ingredient for life on Earth – water – according to researchers at Heriot-Watt University.  The results from pioneering experiments to solve one of the mysteries of the interstellar space, where did all the water come from, will be presented by Victoria Frankland at the RAS National Astronomy Meeting in Glasgow on Wednesday 14th April.

“We think that the Earth’s water was delivered by comets during the early stages of Earth’s history and that comets were formed from interstellar material left over after the birth of the Sun, but the next step back has been unclear,” said Ms Frankland.  

Water is relatively abundant in the interstellar medium and hydrogen atoms are extremely common, but there is a problem with the other vital ingredient for H2O. Gas phase reactions that can take place in the interstellar medium are limited by the low temperatures and pressures. Experiments show that it is possible for hydrogen atoms to combine with molecules of oxygen (O2) or ozone (O3) under the conditions of the interstellar medium.  However, observations by recent satellite missions have detected very little gaseous molecular oxygen (O2) and ozone (O3) has never been detected at all in these regions of space. On the other hand, atomic oxygen (O) is quite plentiful, but gas phase reactions between hydrogen and atomic oxygen can’t account for the amount of water observed. Even the observed quantities of atomic oxygen suggest that some is ‘missing’ in star-forming regions compared to the rest of interstellar space.

Ms Frankland and her colleagues at Heriot-Watt believe the dust grains, which make up about 1% of the interstellar medium, hold the key by providing a surface that helps reactions take place. In addition, some molecules remain stuck to the surface, building up an icy coating over time. This coating, which is mainly water ice, can then play a role in reactions.

The team at Heriot-Watt has pioneered surface science techniques to evaluate experimentally exactly how such reactions might occur. However, the temperatures in interstellar space can reach just a few degrees above absolute zero, so recreating the conditions in the laboratory has been a challenge.

“Our experiments rely on being able to reproduce in the laboratory the very low pressures and low temperatures of these star-forming regions. We set up our experiments in a vacuum chamber and cool it down to –268 degrees Celsius, then use surface sensitive techniques to explore the physical and chemical behaviour of oxygen atoms and molecules on the surfaces of dust and ice grains.” said Ms Frankland.

Initially, the experiments have been looking at how the surfaces of dust particles affect the reactions of oxygen in its various forms in order to eliminate other water formation reactions. However, the ultimate aim of this research will be to combine atomic beams of oxygen and hydrogen study in situ water formation on a grain surface.

“These initial experiments are having some interesting results in that they are allowing us to look at how the ice coating develops on the dust particles. It appears that oxygen atoms may become trapped inside the icy mantles.  We need to do more work, but it may be that our experiments might help solve the mystery of the missing atomic oxygen as well as where the water has come from,” said Ms Frankland.

CONTACTS

Victoria Frankland
Department of Chemistry
School of Engineering and Physical Sciences,
William Perkin Building,
Heriot-Watt University,
Edinburgh, EH14 4AS
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NAM 2010 Press Office (12th – 16th April only)
Room G358
Gilmorehill Building
University of Glasgow.
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Anita Heward
Press Officer
Royal Astronomical Society
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Dr Robert Massey
Press and Policy Officer
Royal Astronomical Society
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IMAGES
Molecular cloud. Credit: NASA/JPL-Caltech/L. Allen (Harvard-Smithsonian CfA)
http://ipac.jpl.nasa.gov/media_images/ssc2005-23a1.jpg

FURTHER INFORMATION
THE RAS NATIONAL ASTRONOMY MEETING 2010
The RAS National Astronomy Meeting 2010 will take place from 12-16th April at the University of Glasgow. The conference is held in conjunction with the UK Solar Physics (UKSP) and Magnetosphere Ionosphere and Solar-Terrestrial Physics (MIST) meetings. NAM2010 (www.astro.gla.ac.uk/nam2010/) is principally sponsored by the Royal Astronomical Society (RAS) and the University of Glasgow.

THE ROYAL ASTRONOMICAL SOCIETY
The Royal Astronomical Society (RAS: www.ras.org.uk), founded in 1820, encourages and promotes the study of astronomy, solar-system science, geophysics and closely related branches of science. The RAS organises scientific meetings, publishes international research and review journals, recognises outstanding achievements by the award of medals and prizes, maintains an extensive library, supports education through grants and outreach activities and represents UK astronomy nationally and internationally. Its more than 3000 members (Fellows), a third based overseas, include scientific researchers in universities, observatories and laboratories as well as historians of astronomy and others.

THE UNIVERSITY OF GLASGOW
The University of Glasgow (founded 1451) is one of the world’s top 100 research universities with more than 70 per cent of its research rated as world-leading or internationally excellent. The Physics and Astronomy Department is one of the top four in the UK’s major research-intensive universities, the Russell Group.
The conference comes to Glasgow during the 250th anniversary year of the founding of the Regius Chair of Astronomy at the University of Glasgow, first held by astronomer and meteorologist Alexander Wilson in 1760. The present incumbent is Prof. John Brown, 10th Astronomer Royal for Scotland.