Scientists from the University of Leeds have discovered enough water vapour to fill Earth’s oceans more than 2000 times over in a gas and dust cloud which is about to collapse into a Sun-like star.
The research, led by Professor Paola Caselli, is the first detection of water vapour in a pre-stellar core, the cold, dark clouds of gas and dust from which stars form.
To produce that amount of vapour, there must be a lot of water ice in the cloud, more than three million frozen Earth oceans worth, says Professor Caselli, the lead author of the paper published in Astrophysical Journal Letters.
The discovery was made using the European Space Agencys Herschel Space Observatory, in a pre-stellar core known as Lynds 1544, in the constellation of Taurus.
Water has previously been detected outside of our Solar System as gas and ice coated onto tiny dust grains near sites of active star formation, and in proto-planetary discs capable of forming planetary systems.
More than 2000 Earth oceans-worth of water vapour were detected, liberated from icy dust grains by high-energy cosmic rays passing through the cloud.
Before our observations, the understanding was that all the water was frozen onto dust grains because it was too cold to be in the gas phase and so we could not measure it.
Now we will need to review our understanding of the chemical processes in this dense region and, in particular, the importance of cosmic rays to maintain some amount of water vapour.
The research also revealed that water molecules are flowing towards the heart of the cloud where a new star is likely to form, indicating that gravitational collapse has just started.
There is absolutely no sign of stars in this dark cloud today, but by looking at the water molecules, we can see evidence of motion inside the region that can be understood as collapse of the whole cloud towards the centre, says Professor Caselli.
There is enough material to form a star at least as massive as our Sun, which means it could also be forming a planetary system, possibly one like ours.
Some of the water vapour detected in L1544 will go into forming the star, but the rest will be incorporated into the surrounding disc, providing a rich water reservoir to feed potential new planets.
Thanks to Herschel, we can now follow the water trail from a molecular cloud in the interstellar medium, through the star formation process, to a planet like Earth where water is a crucial ingredient for life, says ESAs Herschel project scientist, Göran Pilbratt.
Notes for Editors
First detection of water vapour in a pre-stellar core, by P. Caselli et al. has been accepted for publication in Astrophysical Journal Letters. The pre-print version is available here: http://arxiv.org/abs/1208.5998
Herschel studied the dark cloud L1544 as part of the Water in Star-forming regions with Herschel (WISH) key programme using the Heterodyne Instrument for the Far-Infrared spectrometer (HIFI) on Herschel. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA. HIFI was designed and built by a nationally funded consortium led by SRON Netherlands Institute for Space Research. The consortium includes institutes from France, Germany, USA, Canada, Ireland, Italy, Poland, Russia, Spain, Sweden, Switzerland and Taiwan.
For further information
Professor Paola Caselli is available for interview.
Please contact Richard Mellor, Media Relations Assistant, University of Leeds
Tel: +44 (0)113 3434031
For information on the Herschel Space Observatory, contact Markus Bauer, ESA Science and Robotic Exploration Communication Officer
Tel: +31 71 565 6799
Mob: +31 61 594 3 954
ESA Herschel Project Scientist
Tel: +31 71 565 3621
Image: Taurus molecular cloud
Herschels infrared view of part of the Taurus Molecular Cloud, within which the bright, cold pre-stellar cloud L1544 can be seen at the lower left. It is surrounded by many other clouds of gas and dust of varying density.
The Taurus Molecular Cloud is about 450 light years from Earth and is the nearest large region of star formation.
Download here: https://docs.google.com/open?id=0B691WmQZab8LWjRhMmgxSVpsWDQ