Since I am on my way to Chile, I thought it might be worthwhile posting about the European Extremely Large Telescope (E-ELT) the planned location for which is Cerro Armazones, a mountain at an altitude of 3060 metres in the central part of Chile's Atacama Desert, one of the driest places on Earth.
The E-ELT is currently in the detailed design phase with construction scheduled to begin in 2011. I discovered that Autodesk software assists with the design of the specifications for the optical system. The telescope could be operational in the next decade.
The telescope's mirror will be 39.3 metres in diameter. The mirror design is based on an innovative five-mirror scheme. The primary mirror consists of almost 1000 segments, each 1.4 metres wide, but only 50 mm thick. The optical design calls for a large secondary mirror 4.2 metres in diameter. The telescope is designed to correct for atmospheric turbulence. Mirrors include actuators that allow the mirrors to be distorted in milliseconds. The range of wavelengths supported by the telescope's instrumnetation ranges from optical to mid-infrared. The mirror is designed to gather 15 times more light than the largest optical telescopes operating today.
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