Water vapour equal to 2,000 times Earth’s oceans detected in `star forming` cloudPublished On: Wed, Oct 10th, 2012 | Astrophysics | By ANI
Researchers at the ESA’s Herschel space observatory have spotted enough water vapour to fill Earth’s oceans more than 2000 times over, in a gas and dust cloud that is on the verge of collapsing into a new Sun-like star.
Stars form within cold, dark clouds of gas and dust — ‘pre-stellar cores’ — that contain all the ingredients to make solar systems like our own.
Water, essential to life on Earth, 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 alien planetary systems.
More than 2000 Earth oceans-worth of water vapor were detected, liberated from icy dust grains by high-energy cosmic rays passing through the cloud.
“To produce that amount of vapor, there must be a lot of water ice in the cloud, more than three million frozen Earth oceans’ worth,” said Paola Caselli from the University of Leeds, UK, lead author of the paper describing the finding.
“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,” Caselli noted.
The observations also revealed that the water molecules are flowing towards the heart of the cloud where a new star will probably 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 center,” said Dr. 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,” she stated.
Some of the water vapor 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,” said ESA’s Herschel project scientist, Goran Pilbratt.
The discovery was reported in Astrophysical Journal Letters.
C. Codella et al. The Herschel and IRAM CHESS Spectral Surveys of the Protostellar Shock L1157-B1: Fossil Deuteration, 2012 Astrophysical Journal Letters, 757 L9