The Murchison Widefield Array is a telescope with no moving parts. Credit: David Herne, ICRAR
Far outback in Western Australia, 32 tiles—flat, stationary sensors—each carrying 16 dipole antennas have begun collecting scientific data.
These first tiles will ultimately form part of a much bigger array of 512 tiles, the Murchison Widefield Array (MWA)—Australia’s second Square Kilometre Array (SKA) demonstrator project. Like CSIRO’s Australian SKA Pathfinder (ASKAP), the MWA is being built at the remote, radio-quiet Murchison Radio-astronomy Observatory (MRO). Continue reading Telescope of tiles→
The world’s largest telescope, the Square Kilometre Array (SKA), is expected to generate more data in a single day than the world does in a year at present. And even its prototype, CSIRO’s ASKAP, is expected to accumulate more information within six hours of being switched on than all previous radio telescopes combined.
Such gargantuan streams of data require serious management, and that will be one of the jobs of the $80 million iVEC Pawsey Centre in Perth, which is due to be completed in 2013.
The planned Pawsey High-Performance Computing Centre for SKA Science in Perth (photo credit: Woodhead/CSIRO)
The energy of ultra-high energy (UHE) cosmic rays that strike the Earth’s atmosphere make the energy produced from particle collisions by the Large Hadron Collider look puny. A team based in South Australia is now developing the techniques and technology to find out where such energetic particles could possibly originate. They ultimately hope to use the proposed SKA telescope to conduct their search.
“We think some cosmic rays are produced in the remnants of supernovae—exploding stars—but where the most energetic ones come from, that’s a mystery,” says Justin Bray, a PhD student hunting for their source as part of the LUNASKA (Lunar Ultra-high-energy Neutrino Astrophysics using SKA) project led by Ray Protheroe at the University of Adelaide and Ron Ekers at CSIRO. Continue reading Tracing cosmic rays from radio pulses→
THE FIRST ASKAP DISH BEING ERECTED IN FEBRUARY 2010. CREDIT: DAVE DEBOER, CSIRO
It’s not due to begin operating until 2013, but astronomers from around the world are already lining up to use CSIRO’s Australian Square Kilometre Array Pathfinder (ASKAP). In fact, the first five years of ASKAP’s operation are already booked out, with ten major international Survey Science projects looking for pulsars, measuring cosmic magnetic fields, studying millions of galaxies, and more. Continue reading Australia’s SKA demonstrator already booked out→
CSIRO’s Parkes telescope records pulsar signals to try to detect gravitational waves. Credit: David McClenaghan / CSIRO
Einstein’s general theory of relativity predicts them, and they could be scattered throughout the Universe. But so far, gravitational waves— ‘ripples’ in the fabric of space and time—have never been detected. Several Australian teams of astronomers are trying to catch the first signs of one.
MATTHEW BAILES IN THE SWINBURNE VIRTUAL REALITY THEATRE IN FRONT OF AN IMAGE OF THE DOUBLE PULSAR DISCOVERED WITH CSIRO’S PARKES RADIO TELESCOPE. CREDIT: SWINBURNE UNIVERSITY OF TECHNOLOGY.
The technology used in your PC or PlayStation is also helping drive a revolution in radio astronomy—the replacement of custom-built hardware with flexible software and data solutions.
“Hardware solutions for radio astronomy have been evolving, but computer power has been evolving much faster,” says Matthew Bailes, from the Swinburne Centre for Astrophysics and Supercomputing. The Centre has developed software systems that are now used in Australia and overseas. Continue reading PlayStation graphics chips drive astronomy supercomputer→
A DEPICTION OF THE DISTRIBUTION OF MATTER IN AN OBJECT NEARLY TEN MILLION LIGHT YEARS ACROSS AND A THOUSAND TIMES THE MASS OF THE MILKY WAY. THOUSANDS OF THESE EXIST IN THE OBSERVABLE UNIVERSE. CREDIT: GREG POOLE, SWINBURNE UNIVERSITY OF TECHNOLOGY.
Over aeons of time cosmic gas comes together, stars begin to form, supernovae explode, galaxies collide. And computational astronomers can watch it all unfold inside a supercomputer. That’s the kind of work post-doctoral fellows Rob Crain and Greg Poole are doing at the Swinburne Centre for Astrophysics and Supercomputing. Continue reading Supercomputers bring theory to life→
THE MASSIVE DENSE CLOUD OF HYDROGEN (SHOWN BY THE RED CONTOURS), CALLED BYF73, APPEARS TO BE COLLAPSING IN ON ITSELF DUE TO GRAVITY, FORMING HUGE PROTOSTARS (SEEN AS RED)
Enormous collapsing clouds of cosmic gas and dust may yield clues on how massive stars form, which is an enduring mystery of astronomy.
One such cloud, called BYF73, has been studied by a research team using CSIRO’s Mopra radio telescope. Peter Barnes, an Australian researcher working at the University of Florida in the US, leads the team. The massive hydrogen cloud is collapsing in on itself and will probably form a huge cluster of young stars. Continue reading Mega star nursery gives birth to new knowledge→
PARTICLES EMITTING RADIO WAVES STREAM MILLIONS OF LIGHT-YEARS INTO SPACE FROM THE HEART OF THE GALAXY CENTAURUS A. CREDIT: ILANA FEAIN, TIM CORNWELL & RON EKERS (CSIRO). ATCA NORTHERN MIDDLE LOBE POINTING COURTESY R. MORGANTI (ASTRON), PARKES DATA COURTESY N. JUNKES (MPIFR).
At the centre of a nearby galaxy lurks an object of huge interest, a super-massive black hole. CSIRO scientists have used their radio telescopes to take a picture of the galaxy surrounding it, a task some thought could not be done, because of the sheer size and radio brightness of the scene. The image of Centaurus A took about 1,200 hours of observations and a further 10,000 hours of computer processing to put together, but the work is already beginning to bear fruit.
“We didn’t generate this image just to make a pretty picture,” says lead scientist Ilana Feain of CSIRO Astronomy and Space Science. “We want to understand in detail how the energy from super-massive black holes influences the formation and evolution of their host galaxies.” Continue reading Recording the impact of a super-massive black hole→
A BALLOON LAUNCH AT ALICE SPRINGS. CREDIT: R. SOOD.
Scientists are using the unique advantages of Australia’s Red Centre to conduct high-altitude balloon flights for astronomical research. The clear air and low population of central Australia make it the ideal location for balloon-based research.
For most types of astronomy, observatories are typically built high on the tops of mountains, far out in space or high in the sky, dangling from 150-metre-tall helium balloons. Continue reading Alice Springs—gateway to the stars→
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