Astronomers at the Paranal observatory in Chile have created the world’s largest virtual optical telescope linking four telescopes, so that they operate as a single device.
The telescopes of the Very Large Telescope (VLT) form a virtual mirror of 130 metres in diameter.
A previous attempt to link the telescopes last March failed.
Thursday’s link-up was the system’s scientific verification – the final step before scientific work starts.
Linking all four units of the VLT will give scientists a much more detailed look at the universe than previous experiments using just two or three telescopes to create a virtual mirror.
The process that links separate telescopes together is known as interferometry.
In this mode, the VLT becomes the biggest ground-based optical telescope on earth.
Besides creating a gigantic virtual mirror, interferometry also greatly improves the telescope’s spatial resolution and zooming capabilities.
The VLT is one of several telescopes in the Atacama Desert, set up by the European Southern Observatory (ESO).
ESO is an international research organization headquartered in Munich, Germany, and sponsored by 15 member countries.
Even prior to the start of the operation, as the domes of the four VLT units opened on a desert mountaintop in Chile, excitement filled the Paranal observatory’s tiny control room.
It was going to be a special night, said one of the astronomers.
The head of instrumentation at Paranal, Frederic Gonte, called the event a “milestone in our quest for uncovering secrets of the universe”.
“It’s an extremely important step because now we know that we’re ready to do real science,” Frederic Gonte said.
“From now on we’ll be able to observe things we were not able to observe before.”
To link the VLT units, the team of international astronomers and engineers used an instrument called Pionier, which replaces a multitude of mirrors with a single optical microchip.
Although the first attempt to combine the four telescopes happened in March 2011, it did not really work, said Jean-Philippe Berger, a French astronomer involved in the project.
But this time, it was already pretty clear that all the instruments were working correctly, Jean-Philippe Berger added.
“Last time, the atmospheric conditions and vibrations in the system were so bad that the data was just worthless, we stopped after half an hour knowing that it wouldn’t improve,” he said.
“So this attempt is a real first one to carry out observations for several hours straight to test the system in different conditions.”
From now on, the system will be offered to the astronomical community, he added – any astronomer working at Paranal or visiting it will be able to use it.
VLTI, or the VLT Interferometer, has been used since 2002 to link together up to three VLT telescopes, as well as four small auxiliary telescopes that reside beside the big ones on the same platform at Cerra Paranal mountain, at 2,635m altitude.
The main component of an optical telescope is a mirror, and the light coming from a particular object being observed with separate telescopes – such as a star, a nebula or a galaxy – first gets reflected off individual mirrors.
And this is where the interferometer comes into play.
It directs the light underground into tunnels, where specific instruments compensate for the delay that inevitably exists when more than one telescope is used.
Once there is no delay, the light is combined into one single beam – and the image astronomers get is what would have been produced by a single telescope with a gigantic mirror and a much better zoom.
In the case of the VLT, the zooming capability becomes almost 20 times better, said Jean-Philippe Berger.
Jean-Philippe Berger explained that although the biggest “virtual” mirror of 130 m in diameter has already been achieved by linking two farthest from each other telescopes, using all four units gives astronomers several advantages.
“The more telescopes the better – you want to generate a plane to fill that virtual mirror, to increase the efficiency to reconstruct an image, in order to observe more complex objects in the sky,” he said.
“With two telescopes, you typically observe round stars, for which you’re only interested in the diameter, or binary stars, where you can measure the separation between the two stars.
“With four telescopes, you can start thinking about triple stars or young stars surrounded by a protoplanetary disk – a disk of dust and gas that forms planets.”
“Now, the zoo of objects accessible to us will be much bigger.”
