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RSAA News of the Month: December 2003

First Light in the New Year
2004 will see new telescopes in action on Stromlo and Siding Spring

 

During 2004 new telescopes will start operations on both Stromlo and Siding Spring. The telescopes are "guest observatories", renting their sites from the ANU. First to come online will be two Stromlo based telescopes operated by Electro Optic Systems (EOS) of Queanbeyan. They will be followed later in the year by the Faulkes South telescope at Siding Spring.

Since 1998 EOS had operated a 1metre Satellite Laser Ranging (SLR) telescope on Stromlo for Geoscience Australia. The installation was completely destroyed in the firestorm of Jan 18, 2003.

In Dec 2002 work had started on a new 1.8metre telescope installation, the prototype of four being built by EOS for the Keck Observatory in Hawaii. The dome for the 1.8m was completed in October and telescope installation is now complete. The mirror was installed in August, testing of the systems is underway and first light is expected in early 2004. The laser laboratory has been rebuilt and a new SLR telescope installed. Laser ranging will also recommence early in the new year.

Images showing the rapid restoration and growth of the EOS observatory on Stromlo. The first image shows the SLR complex just before the fires. The second shows the almost complete destruction of the site. Following images show the 1.8m dome construction, the rebuilding of the laboratory, a 1.8m telescope in the factory, and the completed observatory with 1.8m and 1m domes and laboratory.

For a brief movie (requires Quicktime) showing the new 1m SLR being installed, click here.
For further details about the telescopes, domes and systems produced by EOS,
click here.

The 1.8m telescope is the prototype of a batch of four destined to become part of the Keck optical interferometer. This combines the image signals from the world's two largest telescopes, the 10m Keck reflectors, and the four 1.8m EOS outrigger telescopes, the so-called "SideKecks". The resulting images will be the deepest and sharpest ever obtained. EOS are using the Stromlo 1.8m to thoroughly test all facets of the telescope and control systems before commencing construction at Keck.

When testing is complete the telescope will be used to identify and track space junk, the debris left in orbit by satellite launches. This debris presents a real danger to spacecraft and the catalogue of orbits will be commercially available. The 1.8m will eventually move to Hawaii. The 1-m will continue the program interrupted by the fire, measuring the exact orbits of satellites that are vital links in the worldwide navigation, surveying and communication networks.

Meanwhile at Siding Spring the Australian element of the world's largest group of educational telescopes is a step nearer completion. During December the enclosure for the Faulkes South Telescope was completed. Unlike the classical domed telescope enclosure, this one opens like a clamshell and leaves the telescope completely exposed during use.

The enclosure for the Faulkes South Telescope at Siding Spring

The Faulkes Telescopes are 2m telescopes sited on Haleakala in Hawaii (Faulkes North) and Siding Spring (Faulkes South). Their purpose is to allow students in schools and colleges in the United Kingdom, Hawaii and Australia to make astronomical observations with research class robotic telescopes, direct from the classroom via the Internet. Faulkes North saw first light in August this year, Faulkes South is due for completion in mid-2004.

Partners in the project are the Dill Faulkes Educational Trust, the University of Hawaii, The Australian National University, the Anglo-Australian Observatory, the Royal Observatory Greenwich, Liverpool John Moores University, the National Space Science Centre/University of Leicester, the Particle Physics and Astronomy Research Council and Swinburne University, Melbourne.

For full information on the Faulkes Telescope Project, including registration details for intending users, click here.


RSAA News of the Month Archive