Guide star helps Keck see the light
Lab scientists in collaboration with the W.M. Keck Observatory have created
a "virtual" guide star over Hawaii. The virtual guide star will
be used with adaptive optics on the Keck II telescope to greatly increase
the resolution of fine details of astronomical objects.
Installed in 1999, the Keck adaptive optics system has enabled astronomers
to minimize the blurring effects of the Earth’s atmosphere, producing
images with unprecedented detail and resolution. The adaptive optics system
uses light from a relatively bright star to measure the atmospheric distortions
and to correct for them, but only about 1 percent of the sky contains
stars sufficiently bright to be of use. The new virtual guide star will
enable Keck astronomers to study nearly the entire sky with the high resolution
of adaptive optics.
The virtual guide star, which achieved "first light" on Dec.
23, was created using a 20-watt dye laser to illuminate a diffuse layer
of sodium atoms that exists 60 miles (95 km) above the Earth’s surface.
When activated by the laser, the sodium atoms produced a very small source
of light, less than a meter (39 inches) in diameter, which allowed the
adaptive optics system to measure the distortions of the atmosphere. Two
more commissionings are scheduled for later this month.
The resulting virtual star was measured at 9.5 magnitude, about 25 times
fainter than anything that can be seen by the unaided eye, but bright
enough to operate the adaptive optics system. The star appeared orange,
the same color of common low-pressure sodium vapor streetlights. The virtual
guide star system was developed in collaboration with the W.M. Keck Observatory,
with additional support provided by the National Aeronautics and Space
Administration (NASA) and the National Science Foundation’s Center
for Adaptive Optics (CfAO) at UC Santa Cruz.
Scientists and engineers from the Laser Science & Technology Division
of the National Ignition Facility Directorate at LLNL played a key role
in preparing the laser that creates the guide star. For two and a half
years, Deanna Pennington, Curtis Brown, Pam Danforth and Holger Jones
worked in Hawaii redesigning, demonstrating and commissioning the laser
system on the telescope so that the virtual guide star could achieve "first
light."
The team hopes to integrate the system with adaptive optics in June when
they will be able to see a real star.
Adaptive optics refers to the ability to compensate or adapt to turbulence
in the Earth’s atmosphere, removing the blurring of starlight. Adaptive
optics systems measure the distortions of the light from a star and then
remove the distortions by bouncing the light off a deformable mirror that
corrects the image several hundred times per second.
With Keck adaptive optics, for which LLNL scientists developed the fast
real-time control system, astronomers are obtaining infrared images with
four times better resolution than the Hubble Space Telescope, which orbits
high above the Earth’s atmosphere. Many significant discoveries have
already been attributed to Keck adaptive optics, and the Keck virtual
guide star is expected to lead to many more.
"We have seen lasers develop into powerful tools in fields ranging
from medicine to compact disc players," said Claire Max of LLNL and
UC Santa Cruz, principal investigator for the Keck laser project. "Our
new virtual guide star marks the start of a new era, when we’ll see
lasers contributing to astronomy as well."
The Keck virtual guide star system consists of a dye laser that is used
to produce light with the wavelength of the atomic sodium resonance line
at 589 nm. The 20-watt output of the dye laser is projected out of a 20-inch
(50 cm) lens attached to the side of the 10-meter Keck II telescope. It
is based on a concept originally implemented by LLNL scientists at the
UC Lick Observatory at Mount Hamilton.
"We asked for an early present this year, and just before Christmas
we were given a virtual star that will dramatically increase the research
capabilities of the world’s largest telescope," said Frederic
Chaffee, director of the W.M. Keck Observatory. "This effort could
not have been possible without the talent and dedication of our adaptive
optics and laser guide star team. We couldn’t be happier with these
results, and we look forward to fully integrating the laser with our adaptive
optics system by the middle of 2002."
The main components of the Keck adaptive optics system are a wavefront
sensor camera, a fast control computer and a deformable mirror. The wavefront
sensor camera measures distortions due to atmospheric turbulence using
light from the guide star. A control computer computes the wavefront distortion
up to 670 times a second and sends commands to the deformable mirror.
The deformable mirror, about six inches (15 cm) in diameter, is made out
of a thin sheet of reflective glass controlled by 349 actuators that can
adjust the shape of the mirror by several microns, a distance large enough
to correct for atmospheric distortions.
The Keck virtual guide star system is the world’s most powerful laser
currently in use at an astronomical telescope. The laser was developed
by LLNL staff who also played a key role in the deployment of the laser
at the telescope.
For images of the virtual guide star, see
http://www.llnl.gov/llnl/06news/NewsMedia/keck_images.html
For further images, go to
http://www2.keck.hawaii.edu:3636/realpublic/gen_info/kiosk/news/laser.html