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The following is a news release from the
University of Arizona.
TUCSON, AZ (UNIVERSITY OF ARIZONA)
- The next generation of adaptive optics has arrived at the Large
Binocular Telescope on Mt. Graham, northeast of Tucson.
This new
technology provides astronomers with a new level of image sharpness
never before seen.
Developed in a collaboration between Italy's
Arcetri Observatory of the Istituto Nazionale di Astrofisica, or INAF,
and the University of Arizona's Steward
Observatory, this technology represents a remarkable step
forward for astronomy.
"This is an incredibly exciting time as
this new adaptive optics system allows us to achieve our potential as
the world's most powerful optical telescope," said Richard Green,
director of the LBT. "The successful results show that the next
generation of astronomy has arrived, while providing a glimpse of the
awesome potential the LBT will be capable of for years to come."
Until
relatively recently, ground-based telescopes had to live with
wavefront distortion caused by the Earth's atmosphere that significantly
blurred the images of distant objects (this is why stars appear to
twinkle to the human eye).
While there have been advancements in
adaptive optics technology to correct atmospheric blurring, the LBT's
innovative system takes this concept to a new level.
This success
was achieved through the combination of several innovative
technologies.
The first is the secondary mirror, which was
designed from the start to be a main component of the LBT rather than an
additional element as on other telescopes.
The concave
secondary mirror is .91 meters in diameter (3 feet) and only 1.6
millimeters thick.
The mirror is so thin and pliable that it can
easily be manipulated by actuators pushing on 672 tiny magnets glued to
the back of the mirror, which offers far greater flexibility and
accuracy than previous systems on other telescopes.
An
innovative "pyramid" sensor detects atmospheric distortions and
manipulates the mirror in real time to cancel out the blurring,
allowing the telescope to literally see as clear as if there were no
atmosphere.
Incredibly, the mirror is capable of making
adjustments every one thousandth of a second, with accuracy to better
than 10 nanometers (a nanometer is one millionth the size of a
millimeter).
In closed-dome tests beginning May 12 and sky tests
every night since May 25, astronomer Simone Esposito and his INAF team
tested the new device, achieving exceptional results.
The LBT's
adaptive optics system, called the First Light Adaptive Optics system,
or FLAO, immediately outperformed all other comparable systems,
delivering an image quality greater than three times sharper than the
Hubble Space Telescope using just one of the LBT's two 8.4 meter
mirrors.
When the adaptive optics are in place for both mirrors
and their light is combined appropriately, it is expected that the LBT
will achieve image sharpness 10 times that of the Hubble.
Setting
a New Standard for Optical Astronomy
The index of the
perfection of image quality is known as the Strehl Ratio, with a ratio
of 100 percent equivalent to an absolutely perfect image.
Without
adaptive optics, the ratio for ground-based telescopes is less than 1
percent.
The adaptive optics systems on other major telescopes
today improve image quality up to about 30 percent to 50 percent in the
near-infrared wavelengths where the testing was conducted.
In
the initial testing phase, the LBT's adaptive optics system has been
able to achieve unprecedented Strehl Ratio of 60 to 80 percent, a
nearly two-thirds improvement in image sharpness over other existing
systems.
The results exceeded all expectations and were so
precise the testing team had difficulty believing its findings.
However,
testing has continued since the system was first put on the sky on May
25, and the LBT's adaptive optics have functioned flawlessly and
achieved peak Strehl Ratios of 82 to 84 percent.
"The results on
the first night were so extraordinary that we thought it might be a
fluke, but every night since the adaptive optics have continued to
exceed all expectations. These results were achieved using only one of
LBT's mirrors. Imagine the potential when we have adaptive optics on
both of LBT's giant eyes," Esposito said.
More images from the
adaptive optics system are available at the LBT
Observatory website.
A Decade of Effort Delivers
Technological Triumph
Development of the LBT's adaptive
optics system took longer than a decade through an international
collaboration.
INAF, in particular the Arcetri Observatory,
conceived the instrument design and developed the electro-mechanical
system, while the University of Arizona Mirror Lab created the optical
elements, and the Italian companies Microgate and ADS International
engineered several components.
A prototype system was previously
installed on the Multiple Mirror Telescope, or MMT, at Mt. Hopkins,
Ariz.
The MMT system uses roughly half the number of actuators
as the LBT's final version, but it demonstrated the viability of the
design.
The LBT's infrared test camera, which produced the
accompanying images, was a joint development of INAF in Bologna and the
MPIA in Heidelberg.
"This has been a tremendous success for
INAF and all of the partners in the LBT," said Piero Salinari, research
director at the Arcetri Observatory, INAF. "After more than a decade
and with so much care and effort having gone into this project, it is
really rewarding to see it succeed so astoundingly."
More on
LBT
The $120 million LBT on Mount Graham utilizes two giant
8.4 meter mirrors and with the new adaptive optics the telescope will
have the resolution of a 22.8-meter, or approximately 75-foot
telescope.
The new adaptive optics will enable versatile
instruments such as the near-infrared camera spectrometer, which allows
astronomers to penetrate interstellar dust clouds and reveal the
secrets of the youngest and most distant galaxies, to achieve their
full potential on the LBT.
The LBT is an international
collaboration among institutions in the U.S., Italy and Germany. The
LBT Corporation partners are:
- The University of Arizona on
behalf of the Arizona university system
- Istituto
Nazionale di Astrofisica, Italy
- LBT
Beteiligungsgesellschaft, Germany, representing the Max Planck Society,
the Astrophysical Institute Potsdam, and Heidelberg University
- The Ohio State University
- The Research
Corporation, on behalf of The University of Notre Dame, University of
Minnesota and University of Virginia
(Copyright 2010 by
the University of Arizona. All Rights Reserved.)