Under the joint hosting arrangements, Australia will host the SKA’s survey telescope and its low frequency aperture array antennas. 

In 2012 the SKA Organisation made the announcement that the telescope would be co hosted between South Africa and Australia, with Australia hosting two critical components not only to the final SKA, but also the cutting edge research which would lead up to it.

The ASKAP Survey telescope

The Australian Square Kilometre Array Pathfinder, or ASKAP, is  CSIRO’s (Commonwealth Scientific and Industrial Research Organisation) radio telescope currently being commissioned at the Murchison Radio-astronomy Observatory (MRO) in Western Australia. Another important precursor for the SKA located in that region is the MWA (Murchison Widefield Array)

As part of SKA Phase one, Australia’s existing 36 dish ASKAP survey telescope will be expanded out to 96 dishes. Equipped with phased array feed (PAF) technology, this element of the SKA will be able to survey large areas of the sky in great detail.  ASKAP itself will work as a separate instrument in its own right for some years before being integrated in to the SKA Phase 1

The phased array feed (PAF) for ASKAP provides the antenna with a wide field-of-view (FoV) by creating 30 separate (simultaneous) beams to give a FoV of 30 square degrees (The width of your little finger at arms length is around 1 degree), speeding up survey time quite considerably.

In addition to being a world-leading telescope in its own right, ASKAP is an important technology demonstrator for the SKA. ASKAP’s home, the Murchison Radio-astronomy Observatory site will be the central site for major components of SKA telescope infrastructure in Australia

Low frequency aperture arrays

In Phase one, Australia will host several hundred thousand smaller ‘dipole’ antenna (each about a metre in height) which will intercept low frequency radio waves. This array will be expanded to several million antenna in Phase two. The MWA telescope is providing important input in to the design and science goals which the low frequency aperture arrays will be undertaking.

Low frequency aperture arrays

Low frequency aperture array, to be located in Australia. Credit: SKA Organisation

Videos showing the SKA including animations of how the array will look in Australia can be found in our Multimedia Section

Note: Although Australia and New Zealand submitted a joint bid to host the SKA, no SKA infrastructure is likely to be sited in New Zealand under the current dual site solution.

Nevertheless, New Zealand remains a member of the SKA Organisation, and will maintain its close collaboration with Australia. Science and industry groups in New Zealand are currently preparing their contribution to the pre-construction phase.


View the ASKAP and the Australian SKA site on Google maps.


More about ASKAP

The Australian SKA Pathfinder (ASKAP) is a new radio telescope that is providing an important testbed for SKA technology and will itself be incorporated into Phase one of the SKA.

The telescope has been designed and built by Australia’s CSIRO in collaboration with leading overseas astronomers and engineers.

The Australian Government has committed funding of AUD $111 million to the Australian SKA Pathfinder.

To help meet the scientific, technical and budgetary goals of the international SKA, the ASKAP telescope will develop and trial highly innovative new technologies on timescales consistent with the overall international SKA plan. ASKAP comprises 36 twelve metre dish antennas, each of which will be equipped with a multi-element receiver, or phased array feed, to enable unprecedented surveys of the sky.

ASKAP Telescopes

Elevated View of several ASKAP Telescopes: Image: CSIRO

The ASKAP project is currently in an intense phase of technology development. All areas are at the cutting-edge of technology and scientists and engineers from the CSIRO are achieving significant breakthroughs in the design and construction of revolutionary new radio feed technologies which will be vital to the SKA





More about the MWA

The MWA Telescope

The MWA Antenna – Image (C) David Herne (ICRAR)


The Murchison Widefi eld Array (MWA) seen in the image above, is a low-frequency radio telescope operating between 80 and 300 MHz. Already delivering first class science,  it is located at the Murchison Radio-astronomy Observatory (MRO) in Western Australia and is one of three telescopes designated as a Precursor for the SKA. The MWA has been developed by an international collaboration, including partners from Australia, India, New Zealand, and the United States. It is became fully operational beginning in 2013. Whilst a precursor to the SKA it won’t be integrated in to the final SKA telescope, and will continue to work as an independent resource in its own right.

The MWA will perform large surveys of the entire Southern Hemisphere sky and acquire deep observations on targeted regions. It will enable astronomers to pursue four key science objectives. The primary endeavour is the hunt for intergalactic hydrogen gas that surrounded early galaxies during the cosmological epoch of reionization. The MWA will also provide new insights into our Milky Way galaxy and its magnetic field, pulsing and exploding stellar objects, and the science of space weather that connects our Sun to the environment here on Earth.

The Murchison region where the ASKAP and SKA telescopes will eventually be located, are traditional lands of the Wajarri Yamatji People, who signed an indigenous land use agreement, which protects the Aboriginal people’s cultural heritage. The agreement also brought significant benefits in terms of education and infrastructure to the local peoples in what is one of the most sparsely populated regions on Earth.


ASKAP dedication

The ASKAP dedication ceremony (Image courtesy of Sky and Telescope)













Australia – New Zealand SKA Website (External Link)

Murchison Widefield Array Website (External Link)

ASKAP Website (External Link)

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