It's been billed as an astronomical equivalent of the Large Hadron Collider, offering new insights into the formation of the universe and so powerful that it might even detect alien life.
"It will have a deep impact on the way we perceive our place in the universe and how we understand its history and its future," says Michiel van Haarlem, interim director general of the SKA project.
The Square Kilometer
Array (SKA) is an international effort to build the world's largest
radio telescope, one which will probe the dark heart of space shedding
new light on dark matter, black holes, stars and galaxies.
"It will have a deep impact on the way we perceive our place in the universe and how we understand its history and its future," says Michiel van Haarlem, interim director general of the SKA project.
"We know we are going to discover things that we haven't already. It's going to be very exciting," van Haarlem said.
Taking its name from the total size of its collecting area, the SKA telescope will consist of 3,000 dish antennas, each one around 15 meters wide. Construction is slated to begin in 2016.
Collectively the surface
area of all the dishes will amount to one square kilometer -- hence the
name -- all combining to detect radio waves that penetrate the Earth's
atmosphere, emitted by stars, galaxies and quasars.
Two other types of radio
receptors -- aperture antennas and array antennas -- will combine with
the dishes to provide continuous frequency coverage from 70 MHz to 10
GHz.
"It's not like an optical telescope where you see an image of the sky
directly. What you do is measure signals from the antennas and process
them," van Haarlem says.
Around half the antennas will sit in a "central core region" made up of three separate five-kilometer clusters.
The remainder will extend out in five carefully aligned "spiral arms"
stretching out ever more sparsely over an area in excess of 3,000
kilometers (1,864 miles) or more.
The configuration, say scientists, will create the most sensitive radio telescope ever built.
Currently, that honor is held by the Very Large Array (VLA) in New Mexico, says Alastair Edge, from Durham University -- a leading UK center for astronomical research.
"(VLA has) just
undergone a very large refit. Telescopes themselves haven't changed but
the computing at the back end has changed dramatically," Edge said.
At the moment, we simply don't have the computing power for the SKA telescope to perform at full tilt, Edge says.
Van Haarlem concurs.
"We're talking about huge computing hardware that still needs to be developed. There's a big challenge there," he said.
Supercomputers capable of performing billions and billions of operations per second will be required, but the results will be spectacular, van Haarlem says.
"We will have
high-resolution images where we will actually peer into the center of
what is going on in galaxies," van Haarlem said.
"We will also have the
big picture where we can make surveys of vast areas of the sky to map
out the large-scale structure of the universe."
The project is entering a crucial stage with an announcement on where the array will be based expected imminently.
Two locations, one in South Africa's Northern Cape, the other in western Australia, are in the running.
Brian Boyle, project director of the Australia/New Zealand bid,
extols the virtues of Western Australia's "intrinsic radio quietness"
and the "excellent geophysics" of the proposed Australian site.
From CNN Tech News
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