11:35 24 February 2006 
NewScientist.com news service 
Maggie McKee 
  http://www.newscientistspace.com/article.ns?id=dn8770

A powerful new laser that shoots 90 kilometres into the atmosphere to produce 
an "artificial star" has been tested for the first time by the Very Large 
Telescope in Chile. 

Astronomers will use the observations of the laser to correct the blurring in 
telescope images caused by turbulence in the Earth's atmosphere. This will 
allow them to image celestial objects with the VLT at a resolution 10 times 
finer than currently possible.

Atmospheric turbulence is the one of the key factors limiting the resolution 
and light-collecting ability of Earth-based telescopes. So astronomers have 
been developing adaptive optics systems that measure the turbulence using 
lasers, then correct for it by adjusting the shape of a telescope's various 
mirrors about 100 times per second. 

"Laser guide star systems" vastly improve the sensitivity and resolution of 
observations at infrared wavelengths. But, improvements at the shorter optical 
wavelengths would require deforming a mirror 1000 times per second. 

The laser systems are already installed on four large telescopes in the 
northern hemisphere, including the Keck Observatory in Hawaii. Now, astronomers 
have tested the first such system in the southern hemisphere. It is installed 
on Yepun, one of the four 8.2-metre telescopes that make up the VLT in Cerro 
Paranal, Chile.

Meteorite residue
The laser is beamed into the sky, where it causes a layer of sodium atoms at an 
altitude of about 90 kilometres to glow. The sodium layer originates from 
meteorite impacts. The glow produces an artificial star whose change in 
appearance allows astronomers to measure atmospheric turbulence.

The VLT system comprises a powerful orange laser that sits inside a special 
clean-room next to the telescope and an optical fibre that sends the laser 
light to a small "launch" telescope at the top of Yepun. The launch telescope 
sends a 50 centimetre-wide beam of light into the sky to produce the artificial 
star.

Work on the laser began in 2005, but was not easy, says Richard Davies, project 
manager for the laser's development at the Max Planck Institute for 
Extraterrestrial Physics in Munich, Germany. The orange light it uses is at a 
wavelength not used commercially and the laser also requires 1000 times more 
power than typical instruments - it could not be bought off-the-shelf.

Small earthquake
The laser was tested by itself for the first time on 28 January, then used 
again with two adaptive optics instruments on 9 and 10 February. These tests 
showed the artificial star was about twice as large on the sky as it was 
designed to be, Davies told New Scientist: "It's not so big we can't use it, 
but it's not as small as would be optimal."

The problem is probably due to a small earthquake that shook the site and bent 
the launch telescope's mirror. Telescope managers plan to build a new mount for 
the telescope that will straighten out the mirror. The laser guide star system 
is expected to begin science operations later in 2006.

Such systems will lay the groundwork for more advanced adaptive optics systems 
planned for future telescopes, which may boast mirrors as wide as 60 metres. 
"To really make use of these big mirrors, they will have to have laser guide 
stars as standards," Davies says.



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