![[IOP]](http://images.iop.org/cws/icons/themes/phw/colophon-small.png){kind=icon}
The VLT uses active optics to reduce the
effect of atmospheric turbulence on observations.
In this technique the
optical quality of a star is continually monitored against a reference star and
the
surface of the
mirror adjusted to ensure that the
image remains focused at all times.
Similar adjustments are made to counteract the
effects of gravity on the
mirror.
These techniques will allow each individual telescope to see objects 15 million times dimmer than the
faintest stars visible to the
naked eye.
Tests carried out by the ESO astronomers last week on the first of the telescopes to be completed - called UT1 - indicate that the 0.38 arc second resolution is better than expected For example,
the test image of the Clover Leaf quasar is one of the best ground-based images of this object ever obtained. Testing on the telescope will continue until April 1999,
when the telescope will be opened to the astronomy community.
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First light for Europe's new telescope
May 28, 1998
The Very Large Telescope (VLT) in Chile has released its first images. According to the European Southern Observatory, which operates the $500m telescope, the images reveal that the VLT is capable of better angular resolution than any other ground-based telescope. When completed in 2003, the VLT will consist of four interconnected 8.2-metre diameter telescopes. The VLT will use interferometric techniques to combine light from the four telescopes to provide the collecting power of a 16 metre telescope, making it the largest optical telescope in the world. The new images come from the first of these 8.2m dishes.
