By Xinhua science writers Yu Zheng, Wang Aihua
BEIJING, June 4 (Xinhua) -- China built the finest
optical telescope to scan 10 million celestial spectra in the coming five-to-six
years, one of the world's most ambitious astronomical endeavors to record key
data betraying how the universe was formed.
The Chinese government, which awarded the 235 million-yuan (34 million U.S. dollars) contract to a consortium of elite astronomers and engineers, officially unveiled Thursday the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST), the biggest telescope of its kind in the world.
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The undated file photo shows the exterior of the Large Sky Area Multi-Object Fiber Spectroscopy Telescope (LAMOST) in Xinglong, Hebei Province, north China. The LAMOST of the Xinlong Station of National Astronomical Observatories under Chinese Academy of Sciences passed the national examination on June 4. The telescope with a reflecting Schmidt corrector MA and a spherical primary mirror MB is the largest of its kinds in the world. The size of MB is 6.67m x 6.05m, while that of MA is 5.72m x 4.40m, and the effective aperture in diameter is 3.6m-4.9m. The LAMOST will be able to observe 4,000 astronomical spectrum during a period of 1.5 hours in a single night. (Xinhua/Wang Yongji) Photo Gallery>>> |
The research team, led by Cui Xiangqun, a
world-renowned active optics expert who heads the Nanjing Institute of
Astronomical Optics and Technology under the Chinese Academy of Sciences (CAS),
made a breakthrough in synchronized movements of 24 hexagonal mirrors of a
Schmidt reflecting corrector, which is used to track celestial bodies for
scientific analyses.
Cui and her team even made each mirror piece, 1.1
meters in diametrical length, capable of deformation for more precise targeting
and error correction in observations. Light from celestial bodies are reflected
to a bigger spherical mirror, made up of 37 same-sized hexagonal mirrors in a
similar way.
With the 3.6-meter-aperture reflector and the
4.9-meter-aperture spherical mirror, together with a focal plane mounted with
4,000 optical fibers, all cutting-edge technologies, scientists, could ascertain
spectra of 2.5 million fixed stars, 2.5 million galaxies, 1.5 million brighter
cluster galaxies and one million quasi-stellar objects, mostly in the north
celestial sphere.
All the 10 million spectra are expected to be completed within five-to-six years, Cui said, adding that the data would be subsequently accessible to global scientists.
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Visitors look at a part of the Large Sky Area Multi-Object Fiber Spectroscopy Telescope (LAMOST) in Xinglong, Hebei Province, north China, June 4, 2009.(Xinhua/Wang Yongji) Photo Gallery>>> |
Spectra are key for astronomers to read celestial
bodies' chemical composition, density, atmosphere and magnetism. So far, the
science community have found the existence of billions of celestial bodies, but
have only managed to collect spectra of about one in every 10,000 of them.
The ambitious goal of collecting so much data
encouraged Cui and her team to overcome the obstacles making a super large
telescope that has both a big aperture and wide field of view.
Inspired by her mentor Su Dingqiang, a leading
Chinese astronomer who is also a prestigious CAS member, the 58-year-old Cui
combined a 15-story-high scope, missile silo-like observatory tower on top of a
960-meter hill 170 kilometers northeast of Beijing.
During observation nights, the upper parts of the lower dome are removed and starlight is reflected from the mirror up through the 40-meter tube to the primary mirror.
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Staff members introduce the Large Sky Area Multi-Object Fiber Spectroscopy Telescope (LAMOST) in Xinglong, Hebei Province, north China, June 4, 2009. (Xinhua/Wang Yongji) Photo Gallery>>> |
The light of space is fed into the front ends of
optical fibers positioned on a focal plane, before real-time data are recorded
into spectrographs fixed in a room underneath.
The idea was developed from the spherical and
aspherical mirror combination, invented by German opticist B. V. Schmidt in
1931. It also uses advanced active optics technologies.
Dr. R. N. Wilson, inventor of the active optics
theory, wrote in an e-mail to Cui, his former colleague at the European Southern
Observatory, that LAMOST "embodies every aspect of the most advanced and modern
telescope technology."
Continuing mankind's dream of understanding the
universe, triggered by the invention of astronomical telescope by Italy's
Galileo Galilei, Chinese scientists are hoping to capitalize on the "costly big
toy" to unravel dark matter, dark energy, as well as celestial formation and
evolution.
Before LAMOST, the American Sloan Digital Sky Survey
(SDSS) had been the most powerful spectra-collecting optical telescope.
Installed in a New Mexican astronomical station, SDSS has an aperture of 2.5
meters.
In recent months, Cui's huge telescope managed to
capture more than 3,600 spectra in each of the four trials on clear Spring
nights.
"We're quite comfortable with the scans," Cui said.
"Most of the time, we shot the targets exactly, if not hitting the bull's eyes."
University of Chicago Prof. Donald York, founding
director of SDSS, said in an e-mail interview with Xinhua that the data for
well-positioned fibers of LAMOST looked "very good."
York, however, said that precise calibrated data in
wavelength and absolute flux of the celestial bodies cannot be done until the
telescope's fiber positioning becomes "perfect" after debugging.
California Institute of Technology astronomer Richard
Ellis said, "A large telescope is one of the best examples of what a
civilization does well, and I think here we look at the LAMOST now and we see
what China has done."
Cui said Chinese scientists might consider building a
similar big telescope on Antarctica, to gain wider and clearer cosmic
view.