By Emily Lehmann
There’s a new star in the making in the world of astronomy, with our Australian Square Kilometre Array Pathfinder (ASKAP) named as a finalist in The Australian Innovation Challenge’s Manufacturing, Construction and Infrastructure category*.
We recently shared some of the first images produced by the amazing ASKAP telescope. It comprises a cluster of 36 radio dishes that work in conjunction with a powerful supercomputer to form what is, in effect, a single composite radio telescope a massive six kilometres across.
This allows it to survey the night sky very quickly, taking panoramic snapshots over 100 times the size of the full moon (as viewed from Earth, of course!).
The world-leading facility is revolutionising astronomy, and this award nomination is a welcome recognition. You can vote for it here – just scroll down to the bottom of the page.
Now, for all you space cadets, here’s five astronomical facts about why ASKAP is out of this world and a sure-fire winner:
- ASKAP’s 36 radio dishes, each 12 metres in diameter, give it the capacity to scan the whole sky and make it sensitive to whisper-quiet signals from the Milky Way.
- ASKAP is an outstanding telescope in its own right, as well as a technology demonstrator for the Square Kilometre Array (SKA). This pioneering technology will make ASKAP the fastest radio telescope in the world for surveying the sky.
- Once built, the SKA will comprise of a vast army of radio receivers distributed over tens to hundreds of kilometres in remote areas of Western Australia and Africa.
- The SKA will generate five million million bytes of information in its first day. That’s almost as many grains of sand on all of the world’s beaches.
- ASKAP is located in the remote Murchison Shire of Western Australia, which was chosen because there is hardly any human activity and so little background radio noise.
ASKAP is one of four CSIRO projects already in the running for different categories in the Oz’s Innovation Challenge (we’ve also written about swarm sensing and Direct Nickel). You can #voteCSIRO for any and all of them – just follow the links from the Challenge’s home page!
By Nola Wilkinson
Ever wondered what there is between the stars? Dr Naomi McClure-Griffiths not only wonders about it, she’s on a mission to find out.
Naomi is fascinated with the life of stars, the behaviour of interstellar gas, and how gas and stars interact. “As an astronomer, I’d like to understand how the galaxy formed and how it’s living its life,” she says.
“The galaxy is much more frothy and bubbly than we ever thought. It looks like the head on a glass of beer.”
Very large stars, 8-20 times the size of our sun, experience dramatic supernova explosions that push gas out of the galaxy via solar winds travelling at up to 1000 kilometres a second.
It is these solar winds that blow bubbles in the gas between the stars, creating a frothy, foamy appearance.
Watch this video to find out more about Naomi and her amazing work:
By Lisa Harvey-Smith, CSIRO
The first images from Australia’s Square Kilometre Array Pathfinder (ASKAP) telescope have given scientists a sneak peek at the potential images to come from the much larger Square Kilometre Array (SKA) telescope currently being developed.
ASKAP comprises a cluster of 36 large radio dishes that work together with a powerful supercomputer to form (in effect) a single composite radio telescope 6km across.
What makes ASKAP truly special is the wide-angle “radio cameras”, known as phased array feeds, which can take up to 36 images of the sky simultaneously and stitch them together to generate a panoramic image.
Why panoramic vision?
Traditional radio telescope arrays such as the Australia Telescope Compact Array near Narrabri, NSW, are powerful probes of deep-space objects. But their limited field of view (approximately equivalent to the full moon) means that undertaking major research projects such as studying the structure of the Milky Way, or carrying out a census of millions of galaxies, is slow, painstaking work that can take many years to realise.
The special wide-angle radio receivers on ASKAP will increase the telescope’s field of vision 30 times, allowing astronomers to build up an encyclopedic knowledge of the sky.
This technological leap will enable us to study many astrophysical phenomena that are currently out of reach, including the evolution of galaxies and cosmic magnetism over billions of years.
For the past 12 months a team of CSIRO astronomers has been testing these novel radio cameras fitted on a test array of six antennas.
The first task for the team was to test the ability of the cameras to image wide fields-of-view and thus demonstrate ASKAP’s main competitive advantage. The results were impressive!
One of the first test images from the ASKAP test array is seen above. The hundreds of star-like points are actually galaxies, each containing billions of stars, seen in radio waves. Using CSIRO’s new radio cameras, nine overlapping images were taken simultaneously and stitched together.
The resulting image covers an area of sky more than five times greater than is normally visible with a radio telescope. The information contained in such images will help us to rapidly build up a picture of the evolution of galaxies over several billion years.
Where next for ASKAP to look
On the back of this success, the commissioning team turned the telescope to the Sculptor or “silver coin” galaxy to test its ability to study deep-space objects.
Sculptor is a spiral galaxy like our own Milky Way, but appears elongated as it is seen almost edge-on from earth.
This image (above) shows the radio waves emitted by hydrogen gas that is swirling in an almost circular motion around the galaxy as it rotates.
The red side of the galaxy is moving away from us and the blue side is moving towards us. The speed of rotation tells us the galaxy’s mass.
The team has also tested the ability of the telescope to “weigh” the gas in very distant galaxies. The image (below) shows a grouping of overlapping galaxies called a gravitational lens.
Seven billion years ago, radio waves from a distant galaxy were absorbed by a foreground galaxy in this group. That signal was processed by ASKAP to form the spectrum (top right in the above image).
Although not visually pretty, this type of observation has enormous scientific value, allowing astronomers to understand how quickly galaxies use up their star-forming fuel.
The latest demonstration with the ASKAP test array is a movie (below) of layers through a cloud of gas in our Milky Way.
This series of images – similar to an MRI scan imaging slices through the human body – demonstrates the ability of the telescope to measure the intricate motions of the spiral arms of the Milky Way and other galaxies.
Building to the bigger array
These images are just the beginning of a new era in radio astronomy, starting with SKA pathfinders like ASKAP and culminating in the construction of the SKA radio telescope.
Once built, the SKA will comprise a vast army of radio receivers distributed over tens to hundreds of kilometres in remote areas of Western Australia and South Africa.
Just like ASKAP combines signals from several dishes, the SKA will use a supercomputer to build up a composite image of the sky.
Each ensemble of antennas will work together to photograph distant astronomical objects that are so faint, that they can’t be seen at all with current technology.
The SKA will thereby open up vast tracts of unexplored space to scientific study, making it a game-changer in astrophysical and cosmological research.
Where does our Galaxy get the fuel to keep forming stars? The answer may lie in thousands of gas clouds flying around the outskirts of our Galaxy.
Originally posted on Universe @ CSIRO:
“Food pills” were a staple of science fiction for decades. For our Galaxy, they may be real.
The Galaxy has been making stars for the last 8 billion years. What’s kept it going all that time?
When old stars die, some of their gas goes back into the galactic “soup” for star making. But in the long run a lot of it gets locked up in long-lived dwarf stars.
So the Galaxy needs fresh supplies of gas.
Astronomer think that gas rains in from, probably in the form of “clouds”, and that this fuels the star-making.
But there’s a problem.
If a regular gas cloud were to hit the warm outer parts of the Galaxy — the halo — the gas would dissipate, and not reach the Galaxy’s starry disk where the party is going on.
Something must hold the gas clouds together on their way to the…
View original 229 more words
Some exciting news from ‘The Dish’ today.
Originally posted on Universe @ CSIRO:
In the journal Science today, astronomers using our Parkes telescope have revealed signs of cataclysms in the distant Universe.
They’ve found four ‘bursts’ or ‘flashes’ of radio waves, the furthest one coming from about 11 billion light-years away. And, they say, if you had ‘radio eyes’ — eyes that could detect radio waves — you’d see one of these ‘bursts’ going off somewhere in the sky every ten seconds. It would be like a continuous show of distant fireworks.
What is a ‘burst’? It’s a spike in the radio energy the telescope receives. Here, from the Science paper, is what the astronomers found. (‘Flux density’ means signal strength.)
‘FRB’ stands for Fast Radio Burst. Because they really are very fast, lasting for only a couple of milliseconds.
The speed of the bursts, their strength, and other characteristics of the radio signal, all help to show what the bursts…
View original 370 more words
If you thought ISS Commander Chris Hadfield’s micro gravity rendition of Space Oddity was the hit of the week, think again.
The latest album from electro music duo Daft Punk is being launched in Wee Waa this week and we’re ready to get down. It was reported that the French duo chose Wee Waa, in regional NSW, because of its proximity to our Australia Telescope. The global album launch will include a party at the Wee Waa show on Friday night.
The Australia Telescope Compact Array is so ready that it’s been getting down to Daft Punk’s Get Lucky.
Our researchers are getting into the swing of things too, giving a tour of the telescope operating room in signature Daft Punk helmets.
And finally, researchers dancing.
Meet Giovanna Zanardo: a PhD student at the International Centre for Radio Astronomy Research who’s using our telescopes to study the remains of a star that exploded in 1987.
Called Supernova 1987A, the explosion made astronomers super excited, because it was the first naked-eye supernova to occur since optical telescopes were invented four centuries ago.
Giovanna has been using the Australia Telescope Compact Array – a set of six dishes near Narrabri, NSW – to study the aftermath of the exploded star. And this month she’s going to be using our iconic Parkes telescope to look at it again.
While at Parkes, Giovanna and fellow scientists will be looking to see if a pulsar – a compact spinning star packed with neutrons – has been created after the collapse of the star’s core, which drove the stellar explosion.
“My PhD in astronomy has been a fantastic journey. I’ve got a front row seat to watch the evolution of a truly amazing object and the chance to use all of Australia’s radio telescopes.”
Giovanna began her career as a structural engineer in Western Australia, but after hearing plans to build the Square Kilometre Array (SKA), she saw this as an opportunity to get into radio astronomy.
From the moment she had a glimpse at the early radio images of Supernova 1987A, Giovanna was hooked. And she’s never looked back.
“I became an engineer because I love structures – but I’ve always loved physics and astronomy. My work allows me to combine the two by investigating large structures in space and seeing how they impact and interact with the surrounding environment,” says Giovanna.
To learn more about careers with us, head to our LinkedIn page.