Max Planck Institute for Astronomy - Annual Report 2005
Max Planck Institute for Astronomy - Annual Report 2005
Max Planck Institute for Astronomy - Annual Report 2005
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V People and Events<br />
V.1 First Light <strong>for</strong> the Large Binocular Telescope<br />
On October 12 th , <strong>2005</strong>, the first astronomical pictures<br />
were taken with the Large Binocular Telescope (LBT).<br />
This »First Light« was an important milestone in the<br />
commissioning of the world’s largest single telescope.<br />
Under the coordination of the MPIA, five German institutes<br />
are LBT partners contributing to the development of<br />
this unique telescope. The LBT will open up completely<br />
new opportunities <strong>for</strong> extrasolar planet research and the<br />
investigation of the distant Universe.<br />
Located on the 3190 m high Mount Graham, Arizona,<br />
the LBT is one of the outstanding scientific-technical<br />
projects of modern astronomical research. The telescope<br />
is equipped with two primary mirrors of 8.4 m diameter<br />
each that are fixed on one common mount and thus can<br />
be pointed simultaneously to distant celestial objects.<br />
By combining the light paths of both mirrors, the LBT<br />
gathers as much light as a telescope of 11.8 m aperture,<br />
thus surpassing the Hubble Space Telescope's light gathering<br />
power by a factor of 24.<br />
Even more important, however, is the fact that the<br />
LBT should be able to achieve the resolving power<br />
equivalent to a single 22.8 m telescope. This ambitious<br />
goal can only be accomplished by using an adaptive op-<br />
tics system combined with Fizeau interferometry. Some<br />
components of the LBT necessary <strong>for</strong> this technique are<br />
still under development. These include the extremely<br />
thin adaptive secondary mirrors and the linc-nirvana<br />
instrument which will provide the interferometric combination<br />
of the two light beams. MPIA is the PI <strong>Institute</strong><br />
<strong>for</strong> the building and development of this central LBT<br />
component (see Chapter IV.4).<br />
The go-ahead <strong>for</strong> first light was given when the first<br />
primary mirror was mounted into the telescope structure.<br />
On October 12 th , <strong>2005</strong>, the telescope was pointed towards<br />
the spiral galaxy NGC 891, which lies at a distance of<br />
24 million light years in the constellation of Andromeda.<br />
The first high-quality images were taken with the Large<br />
Binocular Camera (LBC) in the telescope's primary<br />
focus through a blue filter (a camera version <strong>for</strong> the red<br />
spectral range is under construction). The LBC, with its<br />
core of four CCD detectors of 2046 3 4608 pixels each,<br />
has been provided by the Italian partners of the project.<br />
Several exposures with a total of five minutes exposure<br />
time were combined into a single image with<br />
Fig. V.1.1: Still one-eyed: The LBT on Mount Graham.<br />
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