Press release: 1 September 2010
ESA’s (European Space Agency) Herschel infrared space observatory has discovered that ultraviolet starlight is a key ingredient for making water in the atmosphere of some stars. It is the only explanation for why a dying star is surrounded by a gigantic cloud of hot water vapour. These new results were published on 2nd September 2010 in 'Nature' magazine.
Every recipe needs a secret ingredient. When astronomers discovered an unexpected cloud of water vapour around the old star CW Leonis in 2001, they immediately began searching for the source. Water is known to be present around several types of stars, but CW Leonis is a “carbon star” and therefore thought not to produce water. Initially they suspected the star’s heat must be evaporating comets or even dwarf planets to produce the water.
Now, Herschel’s PACS (Photodetector Array Camera and Spectrometer) and SPIRE instruments have revealed that the secret ingredient is ultraviolet light, because the water vapour is too hot to have come from the destruction of icy celestial bodies and is distributed throughout the stellar wind, including deep down near the surface of the star itself. This suggests that the water is being created by a previously unsuspected chemical process where ultraviolet radiation from interstellar space is breaking up the carbon monoxide and releasing oxygen atoms that can then react with hydrogen to form water molecules.
Professor Leen Decin from Katholieke Universiteit Leuven, Belgium, who led this research, explained, "We already knew there was water in the vicinity of the star, but the previous assumption was that it was probably due to evaporating icy comets orbiting around the star.” The new Herschel observations have shown that the water is being formed much closer to the star itself, at temperatures approaching 1000oC. Prof Decin added, “This is really exciting, since it is the first time that we have seen a lot of carbon and water molecules co-existing close to a very luminous, but dying, star. Carbon and water are two of the major the building blocks for life as we know it on Earth. The same mechanisms triggered by ultraviolet light might have played a crucial role in prebiotic processes on the early Earth.”
Ultraviolet starlight would normally be blocked by the material flowing from the star as its outer layers billow out in a stellar wind. It was already known that the stellar wind is “clumpy” but the Herschel results have shown that some regions around the star must have no wind. These empty regions allow the ultraviolet light to reach the deepest layers of the star’s atmosphere and initiate the chemical reactions that produce the water.
Professor Mike Barlow of University College London, co-author of the Nature paper, said "The discovery of water vapour from the outflowing wind of a carbon star has required a complete re-evaluation of our models for the chemical processes in such flows and testifies to the exceptional capabilities of the spectrometers on-board the Herschel Space Observatory."
CW Leonis is a red giant star which is only a few times the mass of the Sun but has expanded to hundreds of times its size. Nuclear fusion reactions deep inside the star are converting helium into carbon, much of which has ended up in the outer layers of the star’s atmosphere. It is this abundance of Carbon in the atmospheres of these types of stars that has previously led scientists to believe that water could not exist; with so much carbon all of the oxygen should be locked up in carbon monoxide (CO).
Professor Matt Griffin of Cardiff University, Principal Investigator for Herschel's SPIRE instrument, said, “This is the kind of result that the people who built SPIRE love to see - a real surprise, and one that makes us re-think our ideas about how stars evolve. The discovery of water where it shouldn't really exist shows the power of Herschel to reveal new aspects of the Universe.
“What this result and others are telling us is that there is water everywhere in the Universe - we are seeing it in comets, planets, all over the place in our galaxy and in other galaxies. With Herschel we are going to be able to understand how it helps shape the development and evolution of stars and planets.”
Dr David Parker, Director of Space Science and Exploration for the UK Space Agency, added, “Once again, the Herschel team have wowed us with an amazing new discovery. Herschel is a key part of the UK Space Agency’s programme to explore the ancient Universe and understand how galaxies, stars and planets form. This unique, European space observatory is really excelling itself and continues to unveil the secrets of previously unseen parts of our Universe.”
Notes to editors
- Dr Chris North
UK Herschel Outreach Officer
Tel: +44 (0)2920 870 537
- Professor Mike Barlow
University College London
Tel: +44 (0)20 7679 7160
- Julia Short
STFC and UK Space Agency
Tel: +44 (0) 1793 442 012
Image and caption
- Image 1: The red giant carbon star CW Leonis as seen by the PACS and SPIRE cameras on board Herschel. The star itself is too bright to be seen well, but it is releasing material in a violent stellar wind, some of which is seen in a “bow shock” to the left of the star in this image. Observations with the PACS and SPIRE spectrometers have shown that water vapour is being formed deep down near the surface of the star; a place where it was previously thought to be impossible. This means that the stellar wind must be much more “clumpy” than previously thought, with some regions having a much weaker wind than others. This allows ultraviolet light from interstellar space to reach the deeper, warmer regions and trigger the creation of water vapour.
Credit: ESA / PACS / SPIRE / MESS Consortia
A copy of the Nature paper ‘Warm water vapour in the sooty outflow from a luminous carbon star’ is available from the UK Space Agency Press Office.
CW Leonis is a red giant star in the constellation of Leo. The star is classified as a “carbon-star”, and at a distance of around 500 light years is the closest such star to Earth.
Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA. Since launch on 14th May 2009, Herschel spent several months undergoing careful tests on the performance of the instruments and calibration. This was followed by the Science Demonstration Phase: the period when the instruments were tested to their full capabilities.
To date, the mission has gone almost perfectly. The performance of the spacecraft has been shown to be well within pre-launch expectations, all three instruments are working extremely reliably, and the data from the Science Demonstration Phase is exceedingly promising. Herschel is now in a routine science phase, and will continue observing until its liquid helium coolant runs out in around two and half years.
The SPIRE instrument contains an imaging photometer (camera) and an imaging spectrometer. The camera operates in three wavelength bands centred on 250, 350 and 500 μm, and so can make images of the sky simultaneously in three sub-millimetre “colours”. The spectrometer covers the range 200–670 μm, allowing the spectral features of atoms and molecules to be measured. SPIRE was designed and built by an international collaboration, led by Professor Matt Griffin of Cardiff University.
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