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ESO Council Gives Green Light to Detailed Study of the European Extremely Large Telescope

		"The decision by the ESO Council to go ahead with the design study for an European Extremely Large Telescope is a very exciting one for European astronomy," said Richard Wade, President of the ESO Council. "Today is a great day because the ESO Council has authorised us to go forward with the final design of the next flagship telescope of ESO,"says Catherine Cesarsky, ESO's Director General. Since the end of last year, ESO has been working together with its user community of European astronomers and astrophysicists to define the new giant telescope needed by the middle of the next decade. More than one hundred astronomers from all European countries have been involved throughout 2006, helping the ESO Project Offices to produce a novel concept, in which performance, cost, schedule and risk were carefully evaluated.
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This fast pace has also been possible thanks to early conceptual studies in Europe (such as the ESO OWL and the EURO-50 studies) and research and development done in collaboration with a large number of European institutes and high-tech industries to develop critical enabling technologies within the framework of the EU FP6 programme and with significant contributions from all partners. Provisionally dubbed E-ELT for the European Extremely Large Telescope, ESO's innovative concept was presented in detail two weeks ago to more than 250 European astronomers at a conference in Marseille. Their enthusiastic welcome paved the way for the decision by the ESO Council to move to the crucial next phase, detailed design of the full facility.
"At the end of the three year Final Design Study, we will know exactly how everything is going to be built including a detailed costing," said Cesarsky. "We then hope to start construction and have it ready by 2017, when we can install instruments and use it!" The present concept, estimated to cost around 800 million euro, features as a baseline a telescope with a 42 m diameter mirror, and is revolutionary. "A telescope of this size could not be built without a complete rethinking of the way we make telescopes," said Catherine Cesarsky. The primary 42 m diameter mirror is composed of 906 hexagonal segments, each 1.45 m in size, while the secondary mirror is as large as 6 m in diameter. In order to overcome the fuzziness of stellar images due to atmospheric turbulence the telescope needs to incorporate adaptive mirrors		The European Extremely Large Telescope (Artist's Impression) Image:   © ESO		Celestron SkyScout Personal Planetarium  Lab Equipment on eBay  Buy bargain-priced lab equipment on eBay.    U.S. site – eBay.com  Card-Based Test (VME/PCI/VXI/PXI)  Digital Multimeters  Optical Test Equipment  Oscilloscopes  Oscilloscope Test Probes  Power Supplies  Signal/Function Generators  Spectrum Analyzers  Technical Cameras  Telescopes
into its optics. A tertiary mirror, 4.2 m in diameter, relays the light to the adaptive optics system, composed of two mirrors: a 2.5 m mirror supported by 5000 or more actuators able to distort its own shape a thousand times per second, and one 2.7 m in diameter that performs the final image corrections. This five mirror approach results in an exceptional image quality, with no significant aberrations in the field of view. A notable feature of the E-ELT is that a very high-order adaptive optics system is an integral part of the telescope's optical design. Post-focal Adaptive Optics (AO), i.e. built into the instruments and not in the telescope design itself, is now a mature technology with seven AO systems and a laser guide star in operation at Paranal. Embedding AO into the telescope as a baseline option is the natural evolutionary step in telescope design. The site of the E-ELT is not yet fixed as studies are still undergoing with a plan to make a decision by 2008. Extremely Large Telescopes are considered worldwide as one of the highest priorities in ground-based astronomy. They will vastly advance astrophysical knowledge, allowing detailed studies of subjects including planets around other stars, the first objects in the Universe, super-massive black holes, and the nature and distribution of the dark matter and dark energy which dominate the Universe. With a diameter of 42 m and its adaptive optics concept, the E-ELT will be more than one hundred times more sensitive than the present-day largest optical telescopes, such as the 10-m Keck telescopes or the 8.2-m VLT telescopes. "This is really the beginning of a new era for optical and infrared astronomy," said Catherine Cesarsky.
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