London:  A chance discovery by a team of researchers including physicists from the Tata Institute of Fundamental Research in Mumbai has provided experimental evidence that stars may generate sound.

The study of fluids in motion — now known as hydrodynamics — goes back to the Egyptians, so it is not often that new discoveries are made. However when examining the interaction of an ultra-intense laser with a plasma target, the team observed something unexpected.

John Pasley from University of York realised that in the trillionth of a second after the laser strikes, plasma flowed rapidly from areas of high density to more stagnant regions of low density, in such a way that it created something like a traffic jam.

Plasma piled up at the interface between the high and low density regions, generating a series of pressure pulses: a sound wave. However, the sound generated was at such a high frequency that it would have left even bats and dolphins struggling!

With a frequency of nearly a trillion hertz, the sound generated was not only unexpected, but was also at close to the highest frequency possible in such a material — six million times higher than that which can be heard by any mammal!

“One of the few locations in nature where we believe this effect would occur is at the surface of stars. When they are accumulating new material, stars could generate sound in a very similar manner to that which we observed in the laboratory,” explained Pasley.

So the stars might be singing — but, since sound cannot propagate through the vacuum of space, no one can hear them.

The technique used to observe the sound waves in the lab works very much like a police speed camera.

It allows the scientists to accurately measure how fluid is moving at the point that is struck by the laser on timescales of less than a trillionth of a second.

“It was initially hard to determine the origin of the acoustic signals, but our model produced results that compared favourably with the wavelength shifts observed in the experiment,” concluded Alex Robinson from the Plasma Physics Group at York.