A pit of writhing snakes, or a galactic mosh pit – that's what the first picture of turbulent gas in our Milky Way looks like. A recent collaboration between WUN partners, the University of Sydney and the University of Wisconsin-Madison used a radio telescope in eastern Australia to make the groundbreaking image, published in Nature earlier this month.
The space between the stars in our galaxy is not empty, but is filled with thin gas that continually swirls and churns.
“This is the first time anyone has been able to make a picture of this interstellar turbulence,” said Professor Bryan Gaensler of the University of Sydney's Institute for Astronomy. “People have been trying to do this for 30 years.”
Turbulence makes the universe magnetic, helps stars form, and spreads the heat from supernova explosions through the galaxy.
“We now plan to study turbulence throughout the Milky Way. Ultimately this will help us understand why some parts of the galaxy are hotter than others, and why stars form at particular times in particular places,” Professor Gaensler said.
Gaensler and his team studied a region of our galaxy about 10,000 light-years away in the constellation Norma. They used CSIRO's Australia Telescope Compact Array because “it is one of the world's best telescopes for this kind of work,” as Dr Robert Braun, Chief Scientist at CSIRO Astronomy and Space Science explained.
The radio telescope was tuned to receive radio waves that come from the Milky Way. As these waves travel through the swirling interstellar gas, one of their properties—polarisation—is very slightly altered, and the radio telescope can detect this. Polarisation is the direction the waves 'vibrate'. Light can be polarised: some sunglasses filter out light polarised in one direction while letting through other light.
The researchers measured the polarisation changes over an area of sky and used them to make a spectacular image of overlapping entangled tendrils, resembling writhing snakes. The 'snakes' are regions of gas where the density and magnetic field are changing rapidly as a result of turbulence.
The 'snakes' also show how fast the gas is churning—an important number for describing the turbulence. Team member Blakesley Burkhart, a PhD student from the University of Wisconsin, made several computer simulations of turbulent gas moving at different speeds.
Understanding the dynamics of this interstellar medium is important according to University of Wisconsin-Madison astronomy professor Alexander Lazarian. It is responsible for the one essential process of all galaxies: star formation. “While the result may seem esoteric it will help rewrite astrophysics textbooks” says Lazarian, “because the work reveals the key role of turbulence in the various phases of the interstellar medium. This is a very different picture from that still in most text books on astrophysics where the interstellar medium in galaxies can be treated mostly like a static one”.
WUN is a global network of leading research universities, many of whom are the leading centers of astronomy research in the world.
For more information: please contact Karen McLaren, International Development Officer (Networks), The University of Sydney at karen.mclaren@sydney.edu.au
This article was written using material sourced from University of Sydney News and University of Wisconsin News.
