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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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